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Sample records for des lacs magpie

  1. magpie

    Energy Science and Technology Software Center (OSTI)

    2013-09-05

    Magpie is a set of scripts to allow users to run Hadoop jobs on generic clusters rather than require users to build Hadoop specific clusters.

  2. E CO LAC | Open Energy Information

    Open Energy Info (EERE)

    LAC Jump to: navigation, search Name: E&CO LAC Place: Bloomfield, New York Zip: NJ 07003 Sector: Services Product: E&Co is an independent non-profit organization which provids...

  3. Monochromatic radiography of high energy density physics experiments on the MAGPIE generator

    SciTech Connect (OSTI)

    Hall, G. N. Burdiak, G. C.; Suttle, L.; Stuart, N. H.; Swadling, G. F.; Lebedev, S. V.; Smith, R. A.; Patankar, S.; Suzuki-Vidal, F.; Grouchy, P. de; Harvey-Thompson, A. J.; Bennett, M.; Bland, S. N.; Pickworth, L.; Skidmore, J.

    2014-11-15

    A monochromatic X-ray backlighter based on Bragg reflection from a spherically bent quartz crystal has been developed for the MAGPIE pulsed power generator at Imperial College (1.4 MA, 240ns) [I. H. Mitchell et al., Rev. Sci. Instrum. 67, 1533 (2005)]. This instrument has been used to diagnose high energy density physics experiments with 1.865 keV radiation (Silicon He-?) from a laser plasma source driven by a ?7 J, 1 ns pulse from the Cerberus laser. The design of the diagnostic, its characterisation and performance, and initial results in which the instrument was used to radiograph a shock physics experiment on MAGPIE are discussed.

  4. Lac Courte Oreilles Band - Energy Analysis

    Office of Environmental Management (EM)

    Location of Lac Courte Oreilles * The Lac Courte Oreilles (LCO) Reservation is in Northern Wisconsin, 90 miles from Duluth, Minnesota and 11 miles from Hayward. About Lac Courte Oreilles * The reservation is presently 76,465 acres and is 15 miles wide. * We have a seven member Tribal Governing Board with four year terms. * LCO's membership is about 6,700 with nearly half of its members residing on or near the reservation * There are 25 distinctly different communities within the reservation for

  5. Mille Lacs Energy Cooperative | Open Energy Information

    Open Energy Info (EERE)

    Cooperative Place: Minnesota Phone Number: 1-800-450-2191 Website: www.mlecmn.net Facebook: https:www.facebook.compagesMille-Lacs-Energy-Cooperative299198793447582 Outage...

  6. Dominican Republic-Regional Programme for LAC: Support for the...

    Open Energy Info (EERE)

    Programme for LAC: Support for the Preparation of the National Climate Change Policy (Redirected from UNDP-Dominican Republic Regional Programme for LAC - Support for the...

  7. File:(131112) Presentacion LAC LEDs.pdf | Open Energy Information

    Open Energy Info (EERE)

    (131112) Presentacion LAC LEDs.pdf Jump to: navigation, search File File history File usage File:(131112) Presentacion LAC LEDs.pdf Size of this preview: 800 600 pixels. Go to...

  8. LAC Regional Platform Workshop Agenda | Open Energy Information

    Open Energy Info (EERE)

    world Home About Resources & Tools Expert Assistance News & Events Publications Join Contact LAC Workshop Announcement Agenda Participant Package Accommodations Location &...

  9. LAC Regional Platform Workshop Report | Open Energy Information

    Open Energy Info (EERE)

    world Home About Resources & Tools Expert Assistance News & Events Publications Join Contact LAC Workshop Announcement Agenda Participant Package Accommodations Location &...

  10. Comments of Mille Lacs Energy Cooperative | Department of Energy

    Office of Environmental Management (EM)

    Mille Lacs Energy Cooperative Comments of Mille Lacs Energy Cooperative Comments of Mille Lacs Energy Cooperative on Implementing the National Broadband Plan by Studying the Communications Requirements of Electric Utilities to Inform Federal Smart Grid Policy PDF icon Comments of Mille Lacs Energy Cooperative More Documents & Publications Comments of Utilities Telecom Council Communications Requirements of Smart Grid Technologies NBP RFI: Communications Requirements - Reply Comments of

  11. Lac Courte Oreilles Band of Lake Superior Ojibwe

    Office of Environmental Management (EM)

    Oreilles Band of Lake Superior Ojibwe Leslie Isham, Director/Assistant Director Lac Courte Oreilles Energy Project Lac Courte Oreilles Public works Department First Steps towards Tribal Weatherization Assessing the Feasibility of the Hydro Dam About Lac Courte Oreilles (LCO) * Located in Upper Northwest Wisconsin * 76,000 acres and 15 miles wide * 90 miles from Duluth 100 miles from Eau Claire 10 miles from Hayward * Close to 6,000 members, 50% live on or near the reservation * 68% unemployment

  12. Lac Courte Oreilles Lake Superior Band of Ojibwe Energy Projects

    Office of Environmental Management (EM)

    OdaawaaZaga'iganing or Lac Courte Oreilles Lake Superior Band Of Ojibwe LCO Energy Department Staff: Director: Leslie Isham Coordinator: Denise Johnson Energy Projects: Assessing Hydro Dam First Steps Toward Tribal Weatherization Lac Courte Oreilles's Mission We, the Anishinaabeg, the people of OdaawaaZaaga'iganing, the Lac Courte Oreilles Tribe, will sustain our heritage by preserving our past, strengthening our present and embracing our future. We will defend our inherent sovereign rights and

  13. Lac qui Parle County, Minnesota: Energy Resources | Open Energy...

    Open Energy Info (EERE)

    A. Places in Lac qui Parle County, Minnesota Bellingham, Minnesota Boyd, Minnesota Dawson, Minnesota Louisburg, Minnesota Madison, Minnesota Marietta, Minnesota Nassau,...

  14. Fond du Lac Band Leads Climate Resilience Efforts on Lake Superior...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Fond du Lac Band Leads Climate Resilience Efforts on Lake Superior Chippewa Indian Reservation Fond du Lac Band Leads Climate Resilience Efforts on Lake Superior Chippewa Indian ...

  15. Assessing the Hydro Dam at Lac Courte Oreilles

    Office of Environmental Management (EM)

    "Assessing the Hydro Dam at Lac Courte Oreilles" Lac Courte Oreilles Band of Lake Superior Ojibwe Leslie Isham, Director, LCO Energy Project Assistant Director, LCO Public Works 9796N Cty. Hwy K Hayward, WI 54843 About Lac Courte Oreilles (LCO) * Located in upper Northwest Wisconsin * Land base is about 76,000 acres * 7,275 members * Adopted Kyoto Protocol in 2005 * Land Use Comprehensive Plan adopted in 2006 * 2008 DOE First Steps Grant Awarded LCO Tribal Mission We, the Anishinaabeg,

  16. Diffuse γ-ray emission from unresolved BL Lac objects

    SciTech Connect (OSTI)

    Di Mauro, M.; Donato, F.; Lamanna, G.; Sanchez, D. A.

    2014-05-10

    Blazars, active galactic nuclei with a jet pointing toward the Earth, represent the most abundant class of high-energy extragalactic γ-ray sources. The subset of blazars known as BL Lac objects is on average closer to Earth (i.e., younger) and characterized by harder spectra at high energy than the whole sample. The fraction of BL Lacs that is too dim to be detected and resolved by current γ-ray telescopes is therefore expected to contribute to the high-energy isotropic diffuse γ-ray background (IGRB). The IGRB has been recently measured over a wide energy range by the Large Area Telescope (LAT) on board the Gamma-ray Space Telescope (Fermi). We present a new prediction of the diffuse γ-ray flux due to the unresolved BL Lac blazar population. The model is built upon the spectral energy distribution and the luminosity function derived from the fraction of BL Lacs detected (and spectrally characterized) in the γ-ray energy range. We focus our attention on the O(100) GeV energy range, predicting the emission up to the TeV scale and taking into account the absorption on the extragalactic background light. In order to better shape the BL Lac spectral energy distribution, we combine the Fermi-LAT data with Imaging Atmospheric Cerenkov Telescope measurements of the most energetic sources. Our analysis is carried on separately for low- and intermediate-synchrotron-peaked BL Lacs on the one hand and high-synchrotron-peaked BL Lacs on the other hand: we find in fact statistically different features for the two. The diffuse emission from the sum of both BL Lac classes increases from about 10% of the measured IGRB at 100 MeV to ∼100% of the data level at 100 GeV. At energies greater than 100 GeV, our predictions naturally explain the IGRB data, accommodating their softening with increasing energy. Uncertainties are estimated to be within of a factor of two of the best-fit flux up to 500 GeV.

  17. In vivo expression of the lacY gene in two segments leads to functional lac permease

    SciTech Connect (OSTI)

    Bibi, E.; Kaback, H.R. )

    1990-06-01

    The lacY gene of Escherichia coli was cut into two approximately equal-size fragments with Afl II and subcloned individually or together under separate lac operator/promoters in plasmid pT7-5. Under these conditions, lac permease is expressed in two portions: (i) the N-terminal portion (the N terminus, the first six putative transmembrane helices, and most of putative loop 7) and (ii) the C-terminal portion (the last six putative transmembrane helices and the C terminus). Cells harboring pT7-5 encoding both fragments transport lactose at about 30% the rate of cells expressing intact permease to a comparable steady-state level of accumulation. In contrast, cells expressing either half of the permease independently do not transport lactose. As judged by ({sup 35}S)methionine labeling and immunoblotting, intact permease in completely absent from the membrane of cells expressing lacY fragments either individually or together. Thus, transport activity must result from an association between independently synthesized pieces of lac permease. When the gene fragments are expressed individually, the N-terminal portion of the permease is observed inconsistently, and the C-terminal portion is not observed. When the gene fragments are expressed together, polypeptides identified as the N- and C-terminal moieties of the permease are found in the membrane. It is concluded that the N- or C-terminal halves of lac permease are proteolyzed when synthesized independently and that association between the two complementing polypeptides leads to a more stable, catalytically active complex.

  18. Wind Resource Assessment Report: Mille Lacs Indian Reservation, Minnesota

    SciTech Connect (OSTI)

    Jimenez, A. C.

    2013-12-01

    The U.S. Environmental Protection Agency (EPA) launched the RE-Powering America's Land initiative to encourage development of renewable energy on potentially contaminated land and mine sites. EPA collaborated with the U.S. Department of Energy's (DOE's) National Renewable Energy Laboratory (NREL) and the Mille Lacs Band of Chippewa Indians to evaluate the wind resource and examine the feasibility of a wind project at a contaminated site located on the Mille Lacs Indian Reservation in Minnesota. The wind monitoring effort involved the installation of a 60-m met tower and the collection of 18 months of wind data at multiple heights above the ground. This report focuses on the wind resource assessment, the estimated energy production of wind turbines, and an assessment of the economic feasibility of a potential wind project sited this site.

  19. CLUSTERING OF ?-RAY-SELECTED 2LAC FERMI BLAZARS

    SciTech Connect (OSTI)

    Allevato, V.; Finoguenov, A.; Cappelluti, N.

    2014-12-20

    We present the first measurement of the projected correlation function of 485 ?-ray-selected blazars, divided into 175 BL Lacertae (BL Lacs) and 310 flat-spectrum radio quasars (FSRQs) detected in the 2 year all-sky survey by the Fermi-Large Area Telescope. We find that Fermi BL Lacs and FSRQs reside in massive dark matter halos (DMHs) with log M{sub h} = 13.35{sub ?0.14}{sup +0.20} and log M{sub h} = 13.40{sub ?0.19}{sup +0.15} h {sup 1} M {sub ?}, respectively, at low (z ? 0.4) and high (z ? 1.2) redshift. In terms of clustering properties, these results suggest that BL Lacs and FSRQs are similar objects residing in the same dense environment typical of galaxy groups, despite their different spectral energy distributions, power, and accretion rates. We find no difference in the typical bias and hosting halo mass between Fermi blazars and radio-loud active galactic nuclei (AGNs), supporting the unification scheme simply equating radio-loud objects with misaligned blazar counterparts. This similarity in terms of the typical environment they preferentially live in, suggests that blazars tend to occupy the center of DMHs, as already pointed out for radio-loud AGNs. This implies, in light of several projects looking for the ?-ray emission from DM annihilation in galaxy clusters, a strong contamination from blazars to the expected signal from DM annihilation.

  20. Fond du Lac Band Leads Climate Resilience Efforts on Lake Superior Chippewa

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Indian Reservation | Department of Energy Fond du Lac Band Leads Climate Resilience Efforts on Lake Superior Chippewa Indian Reservation Fond du Lac Band Leads Climate Resilience Efforts on Lake Superior Chippewa Indian Reservation September 23, 2014 - 11:24am Addthis From the White House Council on Environmental Quality blog: Last Friday I had the pleasure of visiting the Fond du Lac Band of Lake Superior Chippewa Indian Reservation. I was joined by Raina Thiele, Associate Director of White

  1. Lac du Flambeau Band of Lake Superior Chippewa Indians - Conservation and Renewable Energy Planning

    Office of Environmental Management (EM)

    du Flambeau Tribal Energy Program Lac du Flambeau Tribal Energy Program Renewable Energy and Conservation Renewable Energy and Conservation Planning Planning Larry Wawronowicz Larry Wawronowicz Deputy Administrator of Natural Resources Deputy Administrator of Natural Resources November 8, 2007 November 8, 2007 Lac du Flambeau Band of Lake Superior Lac du Flambeau Band of Lake Superior Chippewa Indians Chippewa Indians DE DE - - PS36 PS36 - - 06GO96038 06GO96038 Brief Summary of Tribe Brief

  2. LEDSGP/about/Latin America and Caribbean Regional Platform/LAC...

    Open Energy Info (EERE)

    aboutLatin America and Caribbean Regional PlatformLAC Regional Platform Workshop < LEDSGP | about | Latin America and Caribbean Regional Platform Jump to: navigation,...

  3. Ward Co. Dunn Co. McLean Co. McHenry Co. Mountrail Co. McKenzie Co.

    Gasoline and Diesel Fuel Update (EIA)

    WHISKEY JOE WHITE ASH SPRING COULEE DES LACS MAGPIE HARTLAND BEICEGEL CREEK RANCH COULEE WINNER CRAZY MAN CREEK GROS VENTRE BANK W BULLSNAKE UPLAND COULEE REFUGE LARSON GARNET ALKALI CREEK PLUMER RATTLESNAKE POINT ELLSWORTH CHURCH BORDER HANSON GROVER HULSE COULEE SAKAKAWEA AURELIA ROUND TOP BUTTE GORHAM BUTTE W MARMON MANITOU SHEALEY CLAYTON SERGIS N SADDLE BUTTE HAYLAND CEDAR COULEE BOWLINE LITTLE BUTTE LONG CREEK RHOADES HEDBERG FILLMORE EIDSVOLD FAIRFIELD WOLF BAY TOBACCO GARDEN N SPRING

  4. Sustaining the natural and economical resources of the Lac Courte Oreilles, Leslie Isham; Jason Weaver

    SciTech Connect (OSTI)

    Isham, Leslie; Weaver, Jason

    2013-09-30

    The Lac Courte Oreilles Band of Lake Superior Chippewa Indians, located in northwest Wisconsin has developed a project, entitled Sustaining the Natural and Economic Resources of the LCO Ojibwe. This technical report is a summary of the project.

  5. Magpie | Open Energy Information

    Open Energy Info (EERE)

    Place: Denver, CO Zip: 80234 Region: Rockies Area Sector: Services Product: Customer Software Development Services for Independent Software Vendors, System Integrators and their...

  6. Winter Hydroelectric Dam Feasibility Assessment: The Lac Courte Oreilles Band of Lake Superior Ojibwe

    Energy Savers [EERE]

    WINTER HYDROELECTRIC DAM FEASIBILITY ASSESSMENT THE LAC COURTE OREILLES BAND OF LAKE SUPERIOR OJIBWE PRESENTED BY JASON WEAVER LAC COURTE OREILLES HISTORY * WE ARE LOCATED IN SAWYER COUNTY IN THE NORTHWESTERN REGION OF WISCONSIN. * WE HAVE 7,310 ENROLLED TRIBAL MEMBERS * THE RESERVATION CONSIST OF 76,465 ACRES, ABOUT 10,500 ACRES ARE WATER * WE HAVE ENTERED 4 SOVEREIGN TREATIES WITH THE U.S. GOVERNMENT. 1825, 1837, 1842 AND THE LA POINTE TREATY OF 1854 WHICH ESTABLISHED THE CURRENT RESERVATIONS

  7. Lac Courte Oreilles Band of Lake Superior Chippewa Indians - Energy Analysis

    Office of Environmental Management (EM)

    Oreilles Band of Lake Superior Ojibwe Location of Lac Courte Oreilles About Lac Courte Oreilles (LCO) * The reservation is presently 76,465 acres and is 15 miles wide. * We have a seven member Tribal Governing Board with four year terms. * LCO's membership is about 7,000 with nearly half of its members residing on or near the reservation * There are 25 distinctly different communities within the reservation for a total of 1,019 households (2000 Census). * LCO operates two casinos; recently

  8. Lac Courte Oreilles Band of Lake Superior Chippewa Indians- 2007 Project

    Broader source: Energy.gov [DOE]

    The Lac Courte Oreilles Band of Lake Superior Chippewa will gather and compile information on the tribe's energy use, conduct energy audits of reservation facilities, identify where conservation efforts would be worthwhile, and evaluate policy changes needed to implement conservation measures.

  9. Project Reports for Lac Courte Oreilles Band of Lake Superior Chippewa Indians- 2007 Project

    Broader source: Energy.gov [DOE]

    The Lac Courte Oreilles Band of Lake Superior Chippewa will gather and compile information on the tribe's energy use, conduct energy audits of reservation facilities, identify where conservation efforts would be worthwhile, and evaluate policy changes needed to implement conservation measures.

  10. STRUCTURED JETS IN BL LAC OBJECTS: EFFICIENT PeV NEUTRINO FACTORIES?

    SciTech Connect (OSTI)

    Tavecchio, Fabrizio; Ghisellini, Gabriele; Guetta, Dafne

    2014-09-20

    The origin of high-energy neutrinos (0.11 PeV range) detected by IceCube remains a mystery. In this work, we explore the possibility that efficient neutrino production can occur in structured jets of BL Lac objects, characterized by a fast inner spine surrounded by a slower layer. This scenario has been widely discussed in the framework of the high-energy emission models for BL Lac objects and radio galaxies. One of the relevant consequences of a velocity structure is the enhancement of the inverse Compton emission caused by the radiative coupling of the two zones. We show that a similar boosting could occur for the neutrino output of the spine through the photo-meson reaction of high-energy protons scattering off the amplified soft target photon field of the layer. Assuming the local density and the cosmological evolution of ?-ray BL Lac object derived from Fermi Large Area Telescope data, we calculate the expected diffuse neutrino intensity, which can match the IceCube data for a reasonable choice of parameters.

  11. Utilisation des défibrillateurs

    ScienceCinema (OSTI)

    None

    2011-10-06

    Information faite par le service medical et le service des pompiers sur l'utilisation des defibrillateurs.

  12. Lac du Flambeau Band of Lake Superior Chippewa Indians Strategic Energy Plan

    SciTech Connect (OSTI)

    Bryan Hoover

    2009-11-16

    This plan discusses the current energy use on the Lac du Flambeau Reservation, the current status of the Tribe's energy program, as well as the issues and concerns with energy on the reservation. This plan also identifies and outlines energy opportunities, goals, and objectives for the Tribe to accomplish. The overall goal of this plan is to address the energy situation of the reservation in a holistic manner for the maximum benefit to the Tribe. This plan is an evolving document that will be re-evaluated as the Tribe's energy situation changes.

  13. Lac du Flambeau Band of Lake Superior Chippewa Indians - Conservation and Renewable Energy Planning

    Office of Environmental Management (EM)

    Bryan Hoover Lac du Flambeau Band of Lake Superior Chippewa Indians November 20, 2008 * Located in North Central Wisconsin. * The reservation is 144 square miles or 86,000 acres. * Population 3,400 Tribal Members. * Checkerboard Reservation * Area- 86,630 acres or 144 square miles * Land Ownership- 66.8%-Tribal land 33.2%-Fee land * 260 Lakes * 71 Miles of Streams * 24,000 Acres of Wetlands * 41,733 Acres of Forests * Develop and evaluate baseline data on energy consumption, costs, trends and

  14. THE 2001-2003 LOW STATE OF NOVA LACERTAE 1950 (DK LAC)

    SciTech Connect (OSTI)

    Honeycutt, R. K.; Jacobson, H.; Hoffman, D.; Maxwell, T.; Croxall, K.; Kafka, S.; Henden, A. A.; Robertson, J. W. E-mail: jacob189@msu.edu E-mail: tmaxwell@astro.indiana.edu E-mail: skafka@dtm.ciw.edu E-mail: Jeff.Robertson@atu.edu

    2011-04-15

    We report on extensive photometry of DK Lac obtained during the interval 1990-2009, which includes a 2 mag low state during 2001-2003. Much of the photometry consists of exposures obtained with a typical spacing of several days, but also includes 26 sequences of continuous photometry each lasting 2-7 hr. We find no evidence for periodicities in our data. We do find that the random variations in the low state are approximately twice those in the high state, when expressed in magnitudes. The lack of orbital-timescale variations is attributed to the nearly face-on presentation of the disk. There is a 0.2 mag decline in the high-state brightness of the system over 19 years, which is consistent with the behavior of other old novae in the decades following outburst. High-state spectra are also presented and discussed. We find that the equivalent width of H{alpha} falls by about double from 1991 to 2008. The photometric properties are discussed in the context of the hibernation scenario for the behavior of novae between outbursts, in which we conclude that low states in old novae are probably unrelated to their possible entrance into hibernation.

  15. Financiere des Energies | Open Energy Information

    Open Energy Info (EERE)

    Jump to: navigation, search Name: Financiere des Energies Place: Saint Contest, France Zip: 14280 Product: Prospects for new production sites and looks for the best...

  16. Multi-wavelength study of flaring activity in BL Lac object S5 0716+714 during the 2015 outburst

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Chandra, Sunil; Zhang, Haocheng; Kushwaha, Pankaj; Singh, K. P.; Bottcher, M.; Kaur, Navpreet; Baliyan, K. S.

    2015-08-17

    We present a detailed investigation of the flaring activity observed from a BL Lac object, S5 0716+714 , during its brightest ever optical state in the second half of 2015 January. Observed almost simultaneously in the optical, X-rays, and γ-rays, a significant change in the degree of optical polarization (PD) and a swing in the position angle (PA) of polarization were recorded. A TeV (VHE) detection was also reported by the MAGIC consortium during this flaring episode. Two prominent sub-flares, peaking about five days apart, were seen in almost all of the energy bands. The multi-wavelength light curves, spectral energymore » distribution, and polarization are modeled using the time-dependent code developed by Zhang et al. This model assumes a straight jet threaded by large-scale helical magnetic fields taking into account the light travel time effects, incorporating synchrotron flux and polarization in 3D geometry. Furthermore, the rapid variation in PD and rotation in PA are most likely due to reconnections happening in the emission region in the jet, as suggested by the change in the ratio of toroidal to poloidal components of the magnetic field during the quiescent and flaring states.« less

  17. HUBBLE/COS OBSERVATIONS OF THE Ly{alpha} FOREST TOWARD THE BL Lac OBJECT 1ES 1553+113

    SciTech Connect (OSTI)

    Danforth, Charles W.; Keeney, Brian A.; Stocke, John T.; Shull, J. Michael; Yao Yangsen, E-mail: danforth@casa.colorado.ed [CASA, Department of Astrophysical and Planetary Sciences, University of Colorado, 389-UCB, Boulder, CO 80309 (United States)

    2010-09-01

    We present new moderate-resolution, far-ultraviolet spectra from the Hubble Space Telescope/Cosmic Origins Spectrograph (HST/COS) of the BL Lac object 1ES 1553+113 covering the wavelength range 1135 A < {lambda} < 1795 A. The data show a smooth continuum with a wealth of narrow (b < 100 km s{sup -1}) absorption features arising in the interstellar medium and intergalactic medium. These features include 41 Ly{alpha} absorbers at 0 < z{sub abs} < 0.43, 14 of which are detected in multiple Lyman lines and 6 of which show absorption in one or more metal lines. We analyze a metal-rich triplet ({Delta}cz {approx} 1000 km s{sup -1}) of Ly{alpha} absorbers at z{sub abs} {approx} 0.188 in which O VI, N V, and C III absorption is detected. Silicon ions (Si III, Si IV) are not detected to fairly strong upper limits and we use the measured Si III/C III upper limit to derive an abundance limit (C/Si) {>=} 4(C/Si){sub sun} for the strongest component of the absorber complex. Galaxy redshift surveys show a number of massive galaxies at approximately the same redshift as this absorption complex, suggesting that it arises in a large-scale galaxy filament. As one of the brightest extragalactic X-ray and {gamma}-ray sources, 1ES 1553+113 is of great interest to the high-energy astrophysics community. With no intrinsic emission or absorption features, 1ES 1553+113 has no direct redshift determination. We use intervening Ly{alpha} absorbers to place a direct limit on the redshift: z{sub em}>0.395 based on a confirmed Ly{alpha}+O VI absorber and z{sub em}>0.433 based on a single-line detection of Ly{alpha}. The current COS data are only sensitive to Ly{alpha} absorbers at z < 0.47, but we present statistical arguments that z{sub em} {approx}< 0.58 (at a 1{sigma} confidence limit) based on the non-detection of any Ly{beta} absorbers at z>0.4.

  18. Community Environmental Response Facilitation Act (CERFA) report. Fort Des Moines, Des Moines, Iowa. Final report

    SciTech Connect (OSTI)

    Young, B.; Rausch, K.; Kang, J.

    1994-04-01

    This report presents the results of the Community Environmental Response Facilitation Act (CERFA) investigation conducted by The Earth Technology Corporation (TETC) at the Fort Des Moines, a U.S. Government property selected for closure by the Base Realignment and Closure (BRAC) Commission. Under CERFA Federal agencies are required to identify real property that can be immediately reused and redeveloped. Satisfying this objective requires the identification of real property where no hazardous substances or petroleum products, regulated by the Comprehensive Environmental Response, Compensation, and Liability Act (CERCLA), were stored for one year or more, known to have been released, or disposed. Fort Des Moines is a 53.28-acre site located in Polk County, Iowa, within the city limits of Des Moines. The installation's primary mission is to provide support and shelter for the U.S. Army Reserve. Activities associated with the property that have environmental significance are photographic processing, vehicle maintenance, printing, and fuel storage. TETC reviewed existing investigation documents; U.S. Environmental Protection Agency (USEPA), State, and county regulatory records; environmental data bases; and title documents pertaining to Fort Des Moines during this investigation. In addition, TETC conducted interviews and visual inspections of Fort Des Moines as well as visual inspections and data base searches for the surrounding properties. Information in this CERFA Report was current as of April 1994.

  19. Des Plaines, Illinois: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    10th congressional district.12 Registered Energy Companies in Des Plaines, Illinois Gas Technology Institute (Partnership for Advanced Residential Retrofit) NARI National...

  20. Laboratoire de Physique des Interfaces et Couches Minces LPICM...

    Open Energy Info (EERE)

    Laboratoire de Physique des Interfaces et Couches Minces (LPICM) Place: Palaiseau, France Zip: 91128 Sector: Carbon Product: Research department of the Ecole Polytechnique in...

  1. Sécurité au-delà des mythes et des croyances

    ScienceCinema (OSTI)

    None

    2011-10-06

    Présentation orale en français, support visuel en français et en anglais. La pire des failles de sécurité est l'impression de sécurité. Le décalage entre la compréhension que l?on a des technologies utilisées, et leurs potentiels réels, ainsi que l'impact potentiellement négatif qu'elles peuvent avoir sur nos vies, n'est pas toujours compris, ou pris en compte par la plupart d'entre-nous. On se contente de nos perceptions pour ne pas avoir à se confronter à la réalité... Alors qu'en est-il vraiment ? En matière de sécurité qui de l'humain ou des technologies a le contrôle ?

  2. Des Moines, Washington: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    This article is a stub. You can help OpenEI by expanding it. Des Moines is a city in King County, Washington. It falls under Washington's 9th congressional district.12...

  3. A Touch of Green for Des Moines’ Sherman Hill

    Broader source: Energy.gov [DOE]

    Des Moines' Green & Main intends to intends to renovate an abandoned 1930s grocery store into a mixed-use facility with LEED Platinum certification – a prestigious badge of energy efficiency and sustainable building practices.

  4. West Des Moines, Iowa: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Hide Map This article is a stub. You can help OpenEI by expanding it. West Des Moines is a city in Dallas County and Polk County and Warren County, Iowa. It falls...

  5. APUI Incubateur de l Ecole des Mines de Douai | Open Energy Informatio...

    Open Energy Info (EERE)

    APUI Incubateur de l Ecole des Mines de Douai Jump to: navigation, search Name: APUI Incubateur de l'Ecole des Mines de Douai Place: France Sector: Services Product: General...

  6. After 105 Years, Historic City Hall in West Des Moines, Iowa Goes Green |

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Department of Energy After 105 Years, Historic City Hall in West Des Moines, Iowa Goes Green After 105 Years, Historic City Hall in West Des Moines, Iowa Goes Green May 9, 2011 - 5:22pm Addthis The restored Historic City Hall building in West Des Moines' Valley Junction neighborhood. | Photo credit: Vicky Saylor The restored Historic City Hall building in West Des Moines' Valley Junction neighborhood. | Photo credit: Vicky Saylor April Saylor April Saylor Former Digital Outreach Strategist,

  7. Des Moines Area Community College | OSTI, US Dept of Energy, Office of

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Scientific and Technical Information Des Moines Area Community College Spotlights Home DOE Applauds DMACC Science and Technical Programs Des Moines Area Community College Des Moines Area Community College Des Moines, Iowa Agri/Natural Resources Biology Biomass Operations Biotechnology Environmental Science Information Technology Manufacturing Technology Microcomputers Civil Engineering Pre-Medical Telecommunications Wind Turbines Ames Laboratory Ames Laboratory is one of DOE's 10 Office of

  8. Simulations of the OzDES AGN reverberation mapping project

    SciTech Connect (OSTI)

    King, Anthea L.; Martini, Paul; Davis, Tamara M.; Denney, K. D.; Kochanek, C. S.; Peterson, Bradley M.; Skielboe, Andreas; Vestergaard, Marianne; Huff, Eric; Watson, Darach; Banerji, Manda; McMahon, Richard; Sharp, Rob; Lidman, C.

    2015-08-26

    As part of the Australian spectroscopic dark energy survey (OzDES) we are carrying out a large-scale reverberation mapping study of ~500 quasars over five years in the 30 deg2 area of the Dark Energy Survey (DES) supernova fields. These quasars have redshifts ranging up to 4 and have apparent AB magnitudes between 16.8 mag < r < 22.5 mag. The aim of the survey is to measure time lags between fluctuations in the quasar continuum and broad emission-line fluxes of individual objects in order to measure black hole masses for a broad range of active galactic nuclei (AGN) and constrain the radiusluminosity (RL) relationship. Here we investigate the expected efficiency of the OzDES reverberation mapping campaign and its possible extensions. We expect to recover lags for ~3545 % of the quasars. AGN with shorter lags and greater variability are more likely to yield a lag measurement, and objects with lags ?6 months or ~1 yr are expected to be recovered the most accurately. The baseline OzDES reverberation mapping campaign is predicted to produce an unbiased measurement of the RL relationship parameters for H?, MgII?2798, and C IV?1549. As a result, extending the baseline survey by either increasing the spectroscopic cadence, extending the survey season, or improving the emission-line flux measurement accuracy will significantly improve the RL parameter constraints for all broad emission lines.

  9. The DES Science Verification Weak Lensing Shear Catalogs

    SciTech Connect (OSTI)

    Jarvis, M.

    2015-07-20

    We present weak lensing shear catalogs for 139 square degrees of data taken during the Science Verification (SV) time for the new Dark Energy Camera (DECam) being used for the Dark Energy Survey (DES). We describe our object selection, point spread function estimation and shear measurement procedures using two independent shear pipelines, IM3SHAPE and NGMIX, which produce catalogs of 2.12 million and 3.44 million galaxies respectively. We also detail a set of null tests for the shear measurements and find that they pass the requirements for systematic errors at the level necessary for weak lensing science applications using the SV data. Furthermore, we discuss some of the planned algorithmic improvements that will be necessary to produce sufficiently accurate shear catalogs for the full 5-year DES, which is expected to cover 5000 square degrees.

  10. Partager : des technologies de pointe au service de la société

    ScienceCinema (OSTI)

    None

    2011-10-06

    Médecine, climatologie, métrologie et informatique, les techniques utilisées par le LHC trouvent déjà des répercussions dans d?autres domaines scientifiques. Utilisant des techniques inédites, la physique des particules en fait bénéficier la société toute entière.

  11. Simulations of the OzDES AGN reverberation mapping project

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    King, Anthea L.; Martini, Paul; Davis, Tamara M.; Denney, K. D.; Kochanek, C. S.; Peterson, Bradley M.; Skielboe, Andreas; Vestergaard, Marianne; Huff, Eric; Watson, Darach; et al

    2015-08-26

    As part of the Australian spectroscopic dark energy survey (OzDES) we are carrying out a large-scale reverberation mapping study of ~500 quasars over five years in the 30 deg2 area of the Dark Energy Survey (DES) supernova fields. These quasars have redshifts ranging up to 4 and have apparent AB magnitudes between 16.8 mag < r < 22.5 mag. The aim of the survey is to measure time lags between fluctuations in the quasar continuum and broad emission-line fluxes of individual objects in order to measure black hole masses for a broad range of active galactic nuclei (AGN) and constrainmore » the radius–luminosity (R–L) relationship. Here we investigate the expected efficiency of the OzDES reverberation mapping campaign and its possible extensions. We expect to recover lags for ~35–45 % of the quasars. AGN with shorter lags and greater variability are more likely to yield a lag measurement, and objects with lags ≲6 months or ~1 yr are expected to be recovered the most accurately. The baseline OzDES reverberation mapping campaign is predicted to produce an unbiased measurement of the R–L relationship parameters for Hβ, MgIIλ2798, and C IVλ1549. As a result, extending the baseline survey by either increasing the spectroscopic cadence, extending the survey season, or improving the emission-line flux measurement accuracy will significantly improve the R–L parameter constraints for all broad emission lines.« less

  12. Cosmology from Cosmic Shear with DES Science Verification Data

    SciTech Connect (OSTI)

    Abbott, T.

    2015-07-20

    We present the first constraints on cosmology from the Dark Energy Survey (DES), using weak lensing measurements from the preliminary Science Verification (SV) data. We use 139 square degrees of SV data, which is less than 3% of the full DES survey area. Using cosmic shear 2-point measurements over three redshift bins we find ?8(m=0.3)0.5 = 0:81 0:06 (68% confidence), after marginalising over 7 systematics parameters and 3 other cosmological parameters. Furthermore, we examine the robustness of our results to the choice of data vector and systematics assumed, and find them to be stable. About 20% of our error bar comes from marginalising over shear and photometric redshift calibration uncertainties. The current state-of-the-art cosmic shear measurements from CFHTLenS are mildly discrepant with the cosmological constraints from Planck CMB data. Our results are consistent with both datasets. Our uncertainties are ~30% larger than those from CFHTLenS when we carry out a comparable analysis of the two datasets, which we attribute largely to the lower number density of our shear catalogue. We investigate constraints on dark energy and find that, with this small fraction of the full survey, the DES SV constraints make negligible impact on the Planck constraints. The moderate disagreement between the CFHTLenS and Planck values of ?8(?m=0.3)0.5 is present regardless of the value of w.

  13. Superfund Record of Decision (EPA Region 7): Des Moines TCE Site, Operable Unit 3, Des Moines, IA. (Second remedial action), September 1992. Final report

    SciTech Connect (OSTI)

    Not Available

    1992-09-18

    The Des Moines TCE site is located southwest of downtown Des Moines, Polk County, Iowa. Land use in the area is predominantly industrial and commercial, and part of the site lies within the floodplain of the Raccoon River. Water from the Des Moines Water Works north infiltration gallery was found to be contaminated with trichloroethylene (TCE), dichloroethylene (DCE), and vinyl chloride at levels above accepted drinking water standards. The ROD addresses OU3, which encompasses potential sources of ground water contamination in an area north of the Raccoon River. The selected remedial action for OU3 includes no action with periodic groundwater monitoring.

  14. Explorer : des clés pour mieux comprendre la matière

    ScienceCinema (OSTI)

    None

    2011-10-06

    Le LHC va-t-il bouleverser les théories de l'infiniment petit ? Les physiciens aimeraient que l'accélérateur fasse trembler le modèle standard. Cette théorie des particules élémentaires et des forces laisse de nombreuses zones d'ombre. Le LHC et ses expériences ont été conçus pour les éclairer.

  15. Lac Courte Oreilles Hydro Dam Assessment

    SciTech Connect (OSTI)

    Weaver, Jason; Meyers, Amy

    2014-12-31

    The main objective of this project was to investigate upgrading the existing hydro power generating system at the Winter Dam. The tribe would like to produce more energy and receive a fair market power purchase agreement so the dam is no longer a drain on our budget but a contributor to our economy. We contracted Kiser Hydro, LLC Engineering for this project and received an engineering report that includes options for producing more energy with cost effective upgrades to the existing turbines. Included in this project was a negotiation of energy price sales negotiations.

  16. Cosmic Shear Measurements with DES Science Verification Data

    SciTech Connect (OSTI)

    Becker, M. R.

    2015-07-20

    We present measurements of weak gravitational lensing cosmic shear two-point statistics using Dark Energy Survey Science Verification data. We demonstrate that our results are robust to the choice of shear measurement pipeline, either ngmix or im3shape, and robust to the choice of two-point statistic, including both real and Fourier-space statistics. Our results pass a suite of null tests including tests for B-mode contamination and direct tests for any dependence of the two-point functions on a set of 16 observing conditions and galaxy properties, such as seeing, airmass, galaxy color, galaxy magnitude, etc. We use a large suite of simulations to compute the covariance matrix of the cosmic shear measurements and assign statistical significance to our null tests. We find that our covariance matrix is consistent with the halo model prediction, indicating that it has the appropriate level of halo sample variance. We also compare the same jackknife procedure applied to the data and the simulations in order to search for additional sources of noise not captured by the simulations. We find no statistically significant extra sources of noise in the data. The overall detection significance with tomography for our highest source density catalog is 9.7σ. Cosmological constraints from the measurements in this work are presented in a companion paper (DES et al. 2015).

  17. EECBG Success Story: After 105 Years, Historic City Hall in West Des Moines, Iowa Goes Green

    Broader source: Energy.gov [DOE]

    The city of West Des Moines, Iowa is used funding to renovate the Historic City Hall building located in Valley Junction, including the installation of four geothermal heating wells, a rooftop covered with vegetation, solar panels and permeable pavers to allow stormwater through to the soil below. Learn more.

  18. DES13S2cmm: The first superluminous supernova from the Dark Energy Survey

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Papadopoulos, A.; Plazas, A. A.; D"Andrea, C. B.; Sullivan, M.; Nichol, R. C.; Barbary, K.; Biswas, R.; Brown, P. J.; Covarrubias, R. A.; Finley, D. A.; et al

    2015-03-23

    We present DES13S2cmm, the first spectroscopically-confirmed superluminous supernova (SLSN) from the Dark Energy Survey (DES). We briefly discuss the data and search algorithm used to find this event in the first year of DES operations, and outline the spectroscopic data obtained from the European Southern Observatory (ESO) Very Large Telescope to confirm its redshift (z = 0.663 ± 0.001 based on the host-galaxy emission lines) and likely spectral type (type I). Using this redshift, we find MpeakU = –21.05+0.10–0.09 for the peak, rest-frame U-band absolute magnitude, and find DES13S2cmm to be located in a faint, low-metallicity (sub-solar), low stellar-mass hostmore » galaxy (log(M/M⊙) = 9.3 ± 0.3), consistent with what is seen for other SLSNe-I. We compare the bolometric light curve of DES13S2cmm to fourteen similarly well-observed SLSNe-I in the literature and find it possesses one of the slowest declining tails (beyond +30 days rest frame past peak), and is the faintest at peak. Moreover, we find the bolometric light curves of all SLSNe-I studied herein possess a dispersion of only 0.2–0.3 magnitudes between +25 and +30 days after peak (rest frame) depending on redshift range studied; this could be important for ‘standardising’ such supernovae, as is done with the more common type Ia. We fit the bolometric light curve of DES13S2cmm with two competing models for SLSNe-I – the radioactive decay of ⁵⁶Ni, and a magnetar – and find that while the magnetar is formally a better fit, neither model provides a compelling match to the data. Although we are unable to conclusively differentiate between these two physical models for this particular SLSN-I, further DES observations of more SLSNe-I should break this degeneracy, especially if the light curves of SLSNe-I can be observed beyond 100 days in the rest frame of the supernova.« less

  19. DES13S2cmm: The first superluminous supernova from the Dark Energy Survey

    SciTech Connect (OSTI)

    Papadopoulos, A.; Plazas, A. A.; D"Andrea, C. B.; Sullivan, M.; Nichol, R. C.; Barbary, K.; Biswas, R.; Brown, P. J.; Covarrubias, R. A.; Finley, D. A.; Fischer, J. A.; Foley, R. J.; Goldstein, D.; Gupta, R. R.; Kessler, R.; Kovacs, E.; Kuhlmann, S. E.; Lidman, C.; March, M.; Nugent, P. E.; Sako, M.; Smith, R. C.; Spinka, H.; Wester, W.; Abbott, T. M. C.; Abdalla, F.; Allam, S. S.; Banerji, M.; Bernstein, J. P.; Bernstein, R. A.; Carnero, A.; da Costa, L. N.; DePoy, D. L.; Desai, S.; Diehl, H. T.; Eifler, T.; Evrard, A. E.; Flaugher, B.; Frieman, J. A.; Gerdes, D.; Gruen, D.; Honscheid, K.; James, D.; Kuehn, K.; Kuropatkin, N.; Lahav, O.; Maia, M. A. G.; Makler, M.; Marshall, J. L.; Merritt, K. W.; Miller, C. J.; Miquel, R.; Ogando, R.; Roe, N. A.; Romer, A. K.; Rykoff, E.; Sanchez, E.; Santiago, B. X.; Scarpine, V.; Schubnell, M.; Sevilla, I.; Soares-Santos, M.; Suchyta, E.; Swanson, M.; Tarle, G.; Thaler, J.; Tucker, L. D.; Wechsler, R. H.; Zuntz, J.

    2015-03-23

    We present DES13S2cmm, the first spectroscopically-confirmed superluminous supernova (SLSN) from the Dark Energy Survey (DES). We briefly discuss the data and search algorithm used to find this event in the first year of DES operations, and outline the spectroscopic data obtained from the European Southern Observatory (ESO) Very Large Telescope to confirm its redshift (z = 0.663 0.001 based on the host-galaxy emission lines) and likely spectral type (type I). Using this redshift, we find MpeakU = 21.05+0.100.09 for the peak, rest-frame U-band absolute magnitude, and find DES13S2cmm to be located in a faint, low-metallicity (sub-solar), low stellar-mass host galaxy (log(M/M?) = 9.3 0.3), consistent with what is seen for other SLSNe-I. We compare the bolometric light curve of DES13S2cmm to fourteen similarly well-observed SLSNe-I in the literature and find it possesses one of the slowest declining tails (beyond +30 days rest frame past peak), and is the faintest at peak. Moreover, we find the bolometric light curves of all SLSNe-I studied herein possess a dispersion of only 0.20.3 magnitudes between +25 and +30 days after peak (rest frame) depending on redshift range studied; this could be important for standardising such supernovae, as is done with the more common type Ia. We fit the bolometric light curve of DES13S2cmm with two competing models for SLSNe-I the radioactive decay of ??Ni, and a magnetar and find that while the magnetar is formally a better fit, neither model provides a compelling match to the data. Although we are unable to conclusively differentiate between these two physical models for this particular SLSN-I, further DES observations of more SLSNe-I should break this degeneracy, especially if the light curves of SLSNe-I can be observed beyond 100 days in the rest frame of the supernova.

  20. DES13S2cmm: The first superluminous supernova from the dark energy survey

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Papadopoulos, A.; D'Andrea, C. B.; Sullivan, M.; Nichol, R. C.; Barbary, K.; Biswas, R.; Brown, P. J.; Covarrubias, R. A.; Finley, D. A.; Fischer, J. A.; et al

    2015-03-23

    We present DES13S2cmm, the first spectroscopically-confirmed superluminous supernova (SLSN) from the Dark Energy Survey (DES). We briefly discuss the data and search algorithm used to find this event in the first year of DES operations, and outline the spectroscopic data obtained from the European Southern Observatory (ESO) Very Large Telescope to confirm its redshift (z = 0.663 0.001 based on the host-galaxy emission lines) and likely spectral type (type I). Using this redshift, we find MUpeak = -21.05????-0.09 for the peak, rest-frame U-band absolute magnitude, and find DES13S2cmm to be located in a faint, low metallicity (sub-solar), low stellar-massmorehost galaxy (log(M/M_sun) = 9.3 0.3); consistent with what is seen for other SLSNe-I. We compare the bolometric light curve of DES13S2cmm to fourteen similarly well-observed SLSNe-I in the literature and find it possesses one of the slowest declining tails (beyond +30 days rest frame past peak), and is the faintest at peak. Moreover, we find the bolometric light curves of all SLSNe-I studied herein possess a dispersion of only 0.2-0.3 magnitudes between +25 and +30 days after peak (rest frame) depending on redshift range studied; this could be important for 'standardising' such supernovae, as is done with the more common type Ia. We fit the bolometric light curve of DES13S2cmm with two competing models for SLSNe-I - the radioactive decay of ??Ni, and a magnetar - and find that while the magnetar is formally a better fit, neither model provides a compelling match to the data. Although we are unable to conclusively differentiate between these two physical models for this particular SLSN-I, further DES observations of more SLSNe-I should break this degeneracy, especially if the light curves of SLSNe-I can be observed beyond 100 days in the rest frame of the supernova.less

  1. Redshift Distributions of Galaxies in the DES Science Verification Shear Catalogue and Implications for Weak Lensing

    SciTech Connect (OSTI)

    Bonnett, C.

    2015-07-21

    We present photometric redshift estimates for galaxies used in the weak lensing analysis of the Dark Energy Survey Science Verification (DES SV) data. Four model- or machine learning-based photometric redshift methods { annz2, bpz calibrated against BCC-U fig simulations, skynet, and tpz { are analysed. For training, calibration, and testing of these methods, we also construct a catalogue of spectroscopically confirmed galaxies matched against DES SV data. The performance of the methods is evalu-ated against the matched spectroscopic catalogue, focusing on metrics relevant for weak lensing analyses, with additional validation against COSMOS photo-zs. From the galaxies in the DES SV shear catalogue, which have mean redshift 0.72 0.01 over the range 0:3 < z < 1:3, we construct three tomographic bins with means of z = {0.45; 0.67,1.00g}. These bins each have systematic uncertainties ?z ? 0.05 in the mean of the fiducial skynet photo-z n(z). We propagate the errors in the redshift distributions through to their impact on cosmological parameters estimated with cosmic shear, and find that they cause shifts in the value of ?8 of approx. 3%. This shift is within the one sigma statistical errors on ?8 for the DES SV shear catalog. We also found that further study of the potential impact of systematic differences on the critical surface density, ?crit, contained levels of bias safely less than the statistical power of DES SV data. We recommend a final Gaussian prior for the photo-z bias in the mean of n(z) of width 0:05 for each of the three tomographic bins, and show that this is a sufficient bias model for the corresponding cosmology analysis.

  2. Mapping and Simulating Systematics Due to Spatially-Varying Observing Conditions in DES Science Verification Data

    SciTech Connect (OSTI)

    Leistedt, B.

    2015-07-20

    Spatially-varying depth and characteristics of observing conditions, such as seeing, airmass, or sky background, are major sources of systematic uncertainties in modern galaxy survey analyses, in particular in deep multi-epoch surveys. We present a framework to extract and project these sources of systematics onto the sky, and apply it to the Dark Energy Survey (DES) to map the observing conditions of the Science Verification (SV) data. The resulting distributions and maps of sources of systematics are used in several analyses of DES SV to perform detailed null tests with the data, and also to incorporate systematics in survey simulations. We illustrate the complementarity of these two approaches by comparing the SV data with the BCC-UFig, a synthetic sky catalogue generated by forward-modelling of the DES SV images. We then analyse the BCC-UFig simulation to construct galaxy samples mimicking those used in SV galaxy clustering studies. We show that the spatially-varying survey depth imprinted in the observed galaxy densities and the redshift distributions of the SV data are successfully reproduced by the simulation and well-captured by the maps of observing conditions. The combined use of the maps, the SV data and the BCC-UFig simulation allows us to quantify the impact of spatial systematics on N(z), the redshift distributions inferred using photometric redshifts. We conclude that spatial systematics in the SV data are mainly due to seeing fluctuations and are under control in current clustering and weak lensing analyses. However, they will need to be carefully characterised in upcoming phases of DES in order to avoid biasing the inferred cosmological results. The framework presented is relevant to all multi-epoch surveys, and will be essential for exploiting future surveys such as the Large Synoptic Survey Telescope, which will require detailed null-tests and realistic end-to-end image simulations to correctly interpret the deep, high-cadence observations of the sky.

  3. OzDES multifibre spectroscopy for the Dark Energy Survey: First-year operation and results

    SciTech Connect (OSTI)

    Yuan, Fang

    2015-07-29

    The Australian Dark Energy Survey (OzDES) is a five-year, 100-night, spectroscopic survey on the Anglo-Australian Telescope, whose primary aim is to measure redshifts of approximately 2500 Type Ia supernovae host galaxies over the redshift range 0.1 < z < 1.2, and derive reverberation-mapped black hole masses for approximately 500 active galactic nuclei and quasars over 0.3 < z < 4.5. This treasure trove of data forms a major part of the spectroscopic follow-up for the Dark Energy Survey for which we are also targeting cluster galaxies, radio galaxies, strong lenses, and unidentified transients, as well as measuring luminous red galaxies and emission line galaxies to help calibrate photometric redshifts. Here, we present an overview of the OzDES programme and our first-year results. Between 2012 December and 2013 December, we observed over 10 000 objects and measured more than 6 000 redshifts. Our strategy of retargeting faint objects across many observing runs has allowed us to measure redshifts for galaxies as faint as mr = 25 mag. We outline our target selection and observing strategy, quantify the redshift success rate for different types of targets, and discuss the implications for our main science goals. In conclusion, we highlight a few interesting objects as examples of the fortuitous yet not totally unexpected discoveries that can come from such a large spectroscopic survey.

  4. Joint Analysis of Galaxy-Galaxy Lensing and Galaxy Clustering: Methodology and Forecasts for DES

    SciTech Connect (OSTI)

    Park, Y.

    2015-07-19

    The joint analysis of galaxy-galaxy lensing and galaxy clustering is a promising method for inferring the growth function of large scale structure. Our analysis will be carried out on data from the Dark Energy Survey (DES), with its measurements of both the distribution of galaxies and the tangential shears of background galaxies induced by these foreground lenses. We develop a practical approach to modeling the assumptions and systematic effects affecting small scale lensing, which provides halo masses, and large scale galaxy clustering. Introducing parameters that characterize the halo occupation distribution (HOD), photometric redshift uncertainties, and shear measurement errors, we study how external priors on different subsets of these parameters affect our growth constraints. Degeneracies within the HOD model, as well as between the HOD and the growth function, are identified as the dominant source of complication, with other systematic effects sub-dominant. The impact of HOD parameters and their degeneracies necessitate the detailed joint modeling of the galaxy sample that we employ. Finally, we conclude that DES data will provide powerful constraints on the evolution of structure growth in the universe, conservatively/optimistically constraining the growth function to 7.9%/4.8% with its first-year data that covered over 1000 square degrees, and to 3.9%/2.3% with its full five-year data that will survey 5000 square degrees, including both statistical and systematic uncertainties.

  5. OzDES multifibre spectroscopy for the Dark Energy Survey: First-year operation and results

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Yuan, Fang

    2015-07-29

    The Australian Dark Energy Survey (OzDES) is a five-year, 100-night, spectroscopic survey on the Anglo-Australian Telescope, whose primary aim is to measure redshifts of approximately 2500 Type Ia supernovae host galaxies over the redshift range 0.1 < z < 1.2, and derive reverberation-mapped black hole masses for approximately 500 active galactic nuclei and quasars over 0.3 < z < 4.5. This treasure trove of data forms a major part of the spectroscopic follow-up for the Dark Energy Survey for which we are also targeting cluster galaxies, radio galaxies, strong lenses, and unidentified transients, as well as measuring luminous red galaxiesmore » and emission line galaxies to help calibrate photometric redshifts. Here, we present an overview of the OzDES programme and our first-year results. Between 2012 December and 2013 December, we observed over 10 000 objects and measured more than 6 000 redshifts. Our strategy of retargeting faint objects across many observing runs has allowed us to measure redshifts for galaxies as faint as mr = 25 mag. We outline our target selection and observing strategy, quantify the redshift success rate for different types of targets, and discuss the implications for our main science goals. In conclusion, we highlight a few interesting objects as examples of the fortuitous yet not totally unexpected discoveries that can come from such a large spectroscopic survey.« less

  6. OzDES multifibre spectroscopy for the Dark Energy Survey: First-year operation and results

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Yuan, Fang; Plazas, A. A.; Lidman, C.; Davis, T. M.; Childress, M.; Abdalla, F. B.

    2015-07-29

    OzDES is a five-year, 100-night, spectroscopic survey on the Anglo-Australian Telescope, whose primary aim is to measure redshifts of approximately 2,500 Type Ia supernovae host galaxies over the redshift range 0.1 morehelp calibrate photometric redshifts. Here we present an overview of the OzDES program and our first-year results. Between Dec 2012 and Dec 2013, we observed over 10,000 objects and measured more than 6,000 redshifts. Our strategy of retargeting faint objects across many observing runs has allowed us to measure redshifts for galaxies as faint as mr = 25 mag. We outline our target selection and observing strategy, quantify the redshift success rate for different types of targets, and discuss the implications for our main science goals. Finally, we highlight a few interesting objects as examples of the fortuitous yet not totally unexpected discoveries that can come from such a large spectroscopic survey.less

  7. Wide-Field Lensing Mass Maps from DES Science Verification Data

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Chang, C.; Vikram, V.; Jain, B.

    2015-07-29

    We present a mass map reconstructed from weak gravitational lensing shear measurements over 139 deg2 from the Dark Energy Survey (DES) Science Verification data. The mass map probes both luminous and dark matter, thus providing a tool for studying cosmology. We find good agreement between the mass map and the distribution of massive galaxy clusters identified using a red-sequence cluster finder. Potential candidates for super-clusters and voids are identified using these maps. We measure the cross-correlation between the mass map and a magnitude-limited foreground galaxy sample and find a detection at the 6.8? level with 20 arcminute smoothing. These measurementsmoreare consistent with simulated galaxy catalogs based on ?CDM Nbody simulations, suggesting low systematics uncertainties in the map. We summarize our key findings in this letter; the detailed methodology and tests for systematics are presented in a companion paper.less

  8. Costa Rica-Regional Programme for LAC: Preparation of Sectoral...

    Open Energy Info (EERE)

    of regional and global partners." Program Focus The program will focus on reducing poverty and inequality, strengthening democratic governance, increasing disaster preparedness...

  9. LAC Regional Platform Workshop General Information | Open Energy...

    Open Energy Info (EERE)

    Visas Participants Presentations Outcomes Report Links Contact Us General Information (English) General information LEDS GP INCAE English-rev FINAL.pdf Informacion General LEDS GP...

  10. Dominican Republic-Regional Programme for LAC: Support for the...

    Open Energy Info (EERE)

    of regional and global partners." Program Focus The program will focus on reducing poverty and inequality, strengthening democratic governance, increasing disaster preparedness...

  11. LAC Regional Platform Workshop Participant Package | Open Energy...

    Open Energy Info (EERE)

    Announcement Agenda Participant Package Accommodations Location & Transportation Insurance & Visas Participants Presentations Outcomes Report Links Contact Us General...

  12. LAC Regional Platform Workshop Links | Open Energy Information

    Open Energy Info (EERE)

    Announcement Agenda Participant Package Accommodations Location & Transportation Insurance & Visas Participants Presentations Outcomes Report Links Contact Us One Page Event...

  13. Fond du Lac County, Wisconsin: Energy Resources | Open Energy...

    Open Energy Info (EERE)

    Oakfield, Wisconsin Ripon, Wisconsin Rosendale, Wisconsin Springvale, Wisconsin St. Cloud, Wisconsin Taycheedah, Wisconsin Waupun, Wisconsin Retrieved from "http:...

  14. DES J0454–4448: Discovery of the first luminous z ≥ 6 quasar from the Dark Energy Survey

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Reed, S. L.

    2015-10-28

    We present the first results of a survey for high-redshift, z ≥ 6, quasars using izY multicolour photometric observations from the Dark Energy Survey (DES). Here we report the discovery and spectroscopic confirmation of the zAB, YAB = 20.2, 20.2 (M1450 = –26.5) quasar DES J0454–4448 with a redshift of z = 6.09±0.02 based on the onset of the Ly α forest and an H i near zone size of 4.1+1.1–1.2 proper Mpc. The quasar was selected as an i-band drop out with i–z = 2.46 and zAB < 21.5 from an area of ~300 deg2. It is the brightestmore » of our 43 candidates and was identified for spectroscopic follow-up solely based on the DES i–z and z–Y colours. The quasar is detected by WISE and has W1AB = 19.68. The discovery of one spectroscopically confirmed quasar with 5.7 < z < 6.5 and zAB ≤ 20.2 is consistent with recent determinations of the luminosity function at z ~ 6. DES when completed will have imaged ~5000 deg2 to YAB = 23.0 (5σ point source) and we expect to discover 50–100 new quasars with z > 6 including 3–10 with z > 7 dramatically increasing the numbers of quasars currently known that are suitable for detailed studies.« less

  15. redMaGiC. Selecting Luminous Red Galaxies from the DES Science Verification Data

    SciTech Connect (OSTI)

    Rozo, E.

    2015-07-20

    We introduce redMaGiC, an automated algorithm for selecting Luminous Red Galaxies (LRGs). The algorithm was developed to minimize photometric redshift uncertainties in photometric large-scale structure studies. redMaGiC achieves this by self-training the color-cuts necessary to produce a luminosity-thresholded LRG sam- ple of constant comoving density. Additionally, we demonstrate that redMaGiC photo-zs are very nearly as accurate as the best machine-learning based methods, yet they require minimal spectroscopic training, do not suffer from extrapolation biases, and are very nearly Gaussian. We apply our algorithm to Dark Energy Survey (DES) Science Verification (SV) data to produce a redMaGiC catalog sampling the redshift range z ? [0.2,0.8]. Our fiducial sample has a comoving space density of 10-3 (h-1Mpc)-3, and a median photo-z bias (zspec zphoto) and scatter (?z=(1 + z)) of 0.005 and 0.017 respectively.The corresponding 5? outlier fraction is 1.4%. We also test our algorithm with Sloan Digital Sky Survey (SDSS) Data Release 8 (DR8) and Stripe 82 data, and discuss how spectroscopic training can be used to control photo-z biases at the 0.1% level.

  16. Galaxy Clustering, Photometric Redshifts and Diagnosis of Systematics in the DES Science Verification Data

    SciTech Connect (OSTI)

    Crocce, M.

    2015-12-09

    We study the clustering of galaxies detected at i < 22.5 in the Science Verification observations of the Dark Energy Survey (DES). Two-point correlation functions are measured using 2.3 106 galaxies over a contiguous 116 deg2 region in five bins of photometric redshift width ?z = 0.2 in the range 0.2 < z < 1.2. The impact of photometric redshift errors is assessed by comparing results using a template-based photo-zalgorithm (BPZ) to a machine-learning algorithm (TPZ). A companion paper presents maps of several observational variables (e.g. seeing, sky brightness) which could modulate the galaxy density. Here we characterize and mitigate systematic errors on the measured clustering which arise from these observational variables, in addition to others such as Galactic dust and stellar contamination. After correcting for systematic effects, we then measure galaxy bias over a broad range of linear scales relative to mass clustering predicted from the Planck ? cold dark matter model, finding agreement with the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS) measurements with ?2 of 4.0 (8.7) with 5 degrees of freedom for the TPZ (BPZ) redshifts. Furthermore, we test a linear bias model, in which the galaxy clustering is a fixed multiple of the predicted non-linear dark matter clustering. The precision of the data allows us to determine that the linear bias model describes the observed galaxy clustering to 2.5 percent accuracy down to scales at least 410 times smaller than those on which linear theory is expected to be sufficient.

  17. Galaxy Clustering, Photometric Redshifts and Diagnosis of Systematics in the DES Science Verification Data

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Crocce, M.

    2015-12-09

    We study the clustering of galaxies detected at i < 22.5 in the Science Verification observations of the Dark Energy Survey (DES). Two-point correlation functions are measured using 2.3 × 106 galaxies over a contiguous 116 deg2 region in five bins of photometric redshift width Δz = 0.2 in the range 0.2 < z < 1.2. The impact of photometric redshift errors is assessed by comparing results using a template-based photo-zalgorithm (BPZ) to a machine-learning algorithm (TPZ). A companion paper presents maps of several observational variables (e.g. seeing, sky brightness) which could modulate the galaxy density. Here we characterize andmore » mitigate systematic errors on the measured clustering which arise from these observational variables, in addition to others such as Galactic dust and stellar contamination. After correcting for systematic effects, we then measure galaxy bias over a broad range of linear scales relative to mass clustering predicted from the Planck Λ cold dark matter model, finding agreement with the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS) measurements with χ2 of 4.0 (8.7) with 5 degrees of freedom for the TPZ (BPZ) redshifts. Furthermore, we test a ‘linear bias’ model, in which the galaxy clustering is a fixed multiple of the predicted non-linear dark matter clustering. The precision of the data allows us to determine that the linear bias model describes the observed galaxy clustering to 2.5 percent accuracy down to scales at least 4–10 times smaller than those on which linear theory is expected to be sufficient.« less

  18. Product equation of state for polysulfone

    SciTech Connect (OSTI)

    Ticknor, Christopher

    2015-09-30

    Here we review the new polysulfone product equation of state (EOS) made with magpie, a chemical equilibrium code.

  19. Estimation of the extragalactic background light using TeV observations of BL Lac objects

    SciTech Connect (OSTI)

    Sinha, Atreyee; Acharya, B. S.; Sahayanathan, S.; Godambe, S.; Misra, R. E-mail: acharya@tifr.res.in E-mail: gsagar@barc.ernet.in

    2014-11-01

    The very high-energy (VHE) gamma-ray spectral index of high-energy peaked blazars correlates strongly with its corresponding redshift, whereas no such correlation is observed in the X-ray or GeV bands. We attribute this correlation to photon-photon absorption of TeV photons with the extragalactic background light (EBL), and utilizing this we compute the allowed flux range for the EBL, which is independent of previous estimates. The observed VHE spectrum of the sources in our sample can be well approximated by a power law, and if the de-absorbed spectrum is also assumed to be a power law, then we show that the spectral shape of EBL will be ?n(?) ? klog (?/? {sub p}). We estimate the range of values for the parameters defining the EBL spectrum, k and ? {sub p}, such that the correlation of the intrinsic VHE spectrum with redshift is nullified. The estimated EBL depends only on the observed correlation and the assumption of a power-law source spectrum. Specifically, it does not depend on the spectral modeling or radiative mechanism of the sources or on any theoretical shape of the EBL spectrum obtained through cosmological calculations. The estimated EBL spectrum is consistent with the upper and lower limits imposed by different observations. Moreover, it also agrees closely with the theoretical estimates obtained through cosmological evolution models.

  20. Lac Courte Oreilles Band of Lake Superior Chippewa Indians- 2010 Hydropower Project

    Broader source: Energy.gov [DOE]

    The feasibility study of hydropower will answer three questions: 1) How can hydropower be developed to create a sustainable economic stream that contributes to the financial viability of the tribe? 2) How can this venture meet the energy needs of the community? 3) How can hydropower be developed without jeopardizing Mother Earth or the cultural beliefs of the tribe?

  1. Lac Courte Oreilles Band of Lake Superior Chippewa Indians- 2010 Energy Efficiency Project

    Broader source: Energy.gov [DOE]

    This weatherization training will result in a reduction of the use and cost of energy by increasing the number of homes that are weatherized.

  2. Project Reports for Lac Courte Oreilles Band of Lake Superior Chippewa Indians- 2010 Project

    Broader source: Energy.gov [DOE]

    The feasibility study of hydropower will answer three questions: 1) How can hydropower be developed to create a sustainable economic stream that contributes to the financial viability of the tribe? 2) How can this venture meet the energy needs of the community? 3) How can hydropower be developed without jeopardizing Mother Earth or the cultural beliefs of the tribe?

  3. Project Reports for Lac Courte Oreilles Band of Lake Superior Chippewa Indians- 2010 Project

    Broader source: Energy.gov [DOE]

    This weatherization training will result in a reduction of the use and cost of energy by increasing the number of homes that are weatherized.

  4. LEDSGP/about/Latin America and Caribbean Regional Platform/LAC...

    Open Energy Info (EERE)

    and Caribbean Regional Platform Workshop 12-14 November 2012 Alajuela, Costa Rica, INCAE Business School The workshop is an initiative of the LEDS Global Partnership (http:...

  5. Lac du Flambeau Band of Lake Superior Chippewa Indians- 2007 Project

    Broader source: Energy.gov [DOE]

    The elements of the proposed project are to establish a baseline, then assess, evaluate, and plan for optimal utilization of conservation and renewable energy resources and technologies on tribal lands.

  6. Project Reports for Lac du Flambeau Band of Lake Superior Chippewa Indians- 2007 Project

    Broader source: Energy.gov [DOE]

    The elements of the proposed project are to establish a baseline, then assess, evaluate, and plan for optimal utilization of conservation and renewable energy resources and technologies on tribal lands.

  7. Lac Courte Oreilles Band of Lake Superior Chippewa Indians- 2010 Project

    Broader source: Energy.gov [DOE]

    The feasibility study of hydropower will answer three questions: 1) How can hydropower be developed to create a sustainable economic stream that contributes to the financial viability of the tribe? 2) How can this venture meet the energy needs of the community? 3) How can hydropower be developed without jeopardizing Mother Earth or the cultural beliefs of the tribe?

  8. Materials Data on La(C2N3)3 (SG:63) by Materials Project

    DOE Data Explorer [Office of Scientific and Technical Information (OSTI)]

    Kristin Persson

    2014-11-02

    Computed materials data using density functional theory calculations. These calculations determine the electronic structure of bulk materials by solving approximations to the Schrodinger equation. For more information, see https://materialsproject.org/docs/calculations

  9. Comparison of effectiveness of sub-slab ventilation systems for indoor radon mitigation: A numerical study; Comparaison a l`aide d`un outil numerique de l`efficacite des systemes de ventilation active du sol limitant la penetration du radon dans l`habitat

    SciTech Connect (OSTI)

    Bonnefous, Y.C. |; Gadgil, A.J.; Allard, F.

    1992-04-01

    The functioning of an active sub-slab ventilation system (SVS) has been studied successfully with the help of a previously evaluated numerical model. The parameters explored are the permeability of the sub-slab and the gravel placed beneath it, the amplitude of applied pressure at the installation point of the system and the functioning method: depressurization or pressurization. The mechanisms contributing to the success of the two systems are identified. This numerical study shows that the presence of a layer of gravel beneath the sub-slab considerably improves the performance of the SVS. Considered separately from the extremely permeable sub-slabs, the depressurization systems perform better than the pressurization systems. 17 refs. [Francais] Le fonctionnement des Systemes de Ventilation active du Sol (SVS) a ete etudie a l`aide d`un outil numerique precedemment evalue avec succes. Les parametres explores sont les permeabilites du sol et du gravier place sous plancher bas, l`amplitude de la pression appliquee au point d`installation du systeme, et le mode de fonctionnement: Depressurisation ou Pressurisation. Les mecanismes contribuant au succes des deux systemes sont identifies. Cette etude numerique montre que la presence d`une couche de gravier sous plancher bas ameliore de facon considerable les performances des SVS. Mis a part le cas des sols extremement permeables, les systemes de Depressurisation ont de meilleures performances que les systemes de Pressurisation. 17 refs.

  10. Pulsed Power Technology at Sandia National Laboratories

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    are some specific sites on Pulsed Power MAGPIE Pulsed Power Facility, Imperial College NIF Naval Research Laboratory, Plasma Physics Division Reviews of U.S. Fusion Policy UKAEA...

  11. Carter Co. Harding Co. Perkins Co. Dunn Co. Dawson Co. Fallon...

    U.S. Energy Information Administration (EIA) Indexed Site

    PETES CREEK CASH OLLIE BOXCAR S CORRAL CREEK GOLD WIBAUX HALLIDAY RHAME RICHARDTON ... CHAMA MURPHY CREEK DEER CREEK N RPD13 RPD12 GOLD S BLUE MOUNTAIN GOSSETT MAGPIE BEICEGEL ...

  12. Carter Co. Harding Co. Perkins Co. Dunn Co. Dawson Co. Fallon...

    U.S. Energy Information Administration (EIA) Indexed Site

    CASH HALLIDAY WIBAUX CORRAL CREEK BOXCAR S GOLD RHAME RICHARDTON DELHI RPDBUTTECO3 ... ZENITH-NEWTON VERSIPPI MURPHY CREEK DEER CREEK N GOLD S RPD13 RPD12 BLUE MOUNTAIN MAGPIE ...

  13. Ground-water geochemistry and radionuclide activity in the Cambrian-Ordovician aquifer of Dodge and Fond du Lac counties, Wisconsin. Technical report

    SciTech Connect (OSTI)

    Weaver, T.R.; Bahr, J.M.; Anderson, M.P.

    1990-01-01

    Analyses of groundwater from wells in the Cambrian-Ordovician aquifer of eastern Wisconsin indicate that regions of the aquifer contain elevated concentrations of dissolved solids, chloride and sulfate. Groundwater from several wells in the area also approach or exceed the current drinking water standard for combined radium activity. Significant changes in groundwater chemistry occur where the aquifer becomes confined by the Maquoketa shale. Concentrations of Cl(-), SO4(2-) and Na(+) increase in the confined region, and the highest combined radium activities are typically observed in the area. Geochemical modeling implies that the observed changes in major ion groundwater chemistry occur in response to the presence of the confining unit which may act as a source of SO4(2-), through gypsum dissolution, and Na(+), through cation exchange. A finite difference groundwater flow model was linked to a particle tracking routine to determine groundwater flow paths and residence times in the aquifer near the boundary between unconfined and confined conditions. Results suggest that the presence of the confining unit produces a vertically stratified flow regime in the confined region.

  14. Centrales au gaz et Energies renouvelables: comparer des pommes avec des pommes

    SciTech Connect (OSTI)

    Bolinger, Mark; Wiser, Ryan; Golove, William

    2003-10-20

    The fundamental conclusion that we draw from this analysis is that one should not to base itself blindly on forecasts prices of natural gas when one compare contracts at price fixes with producers of renewable energy with contracts at variable prices with promoters power stations with gas. Indeed, forecasts of the prices of gas do not succeed not to enter the associated costs with the covering of the risk, that they are connected to the negative pressure against the cover, with the CAPM, with costs of transaction or with unspecified combination of three. Thus, insofar as price stability to length term is developed, better way of comparing the two choices would be to have recourse to the data on the prices in the long term natural gas, and not with forecasts of the prices. During three last years at least, the use of these prices in the long term would have besides license to correct a methodological error who, obviously, seem to have supported unduly, and of relatively important way, power stations with natural gas compared to their competitors of renewable energies.

  15. Lightning Arrestor Connectors Production Readiness

    SciTech Connect (OSTI)

    Marten, Steve; Linder, Kim; Emmons, Jim; Gomez, Antonio; Hasam, Dawud; Maurer, Michelle

    2008-10-20

    The Lightning Arrestor Connector (LAC), part M, presented opportunities to improve the processes used to fabricate LACs. The A## LACs were the first production LACs produced at the KCP, after the product was transferred from Pinnellas. The new LAC relied on the lessons learned from the A## LACs; however, additional improvements were needed to meet the required budget, yield, and schedule requirements. Improvement projects completed since 2001 include Hermetic Connector Sealing Improvement, Contact Assembly molding Improvement, development of a second vendor for LAC shells, general process improvement, tooling improvement, reduction of the LAC production cycle time, and documention of the LAC granule fabrication process. This report summarizes the accomplishments achieved in improving the LAC Production Readiness.

  16. Weak Lensing by Galaxy Troughs in DES Science Verification Data

    SciTech Connect (OSTI)

    Gruen, D.

    2015-09-29

    We measure the weak lensing shear around galaxy troughs, i.e. the radial alignment of background galaxies relative to underdensities in projections of the foreground galaxy field over a wide range of redshift in Science Verification data from the Dark Energy Survey. Our detection of the shear signal is highly significant (10?15? for the smallest angular scales) for troughs with the redshift range z ? [0.2, 0.5] of the projected galaxy field and angular diameters of 10 arcmin1. These measurements probe the connection between the galaxy, matter density, and convergence fields. By assuming galaxies are biased tracers of the matter density with Poissonian noise, we find agreement of our measurements with predictions in a fiducial ? cold dark matter model. Furthermore, the prediction for the lensing signal on large trough scales is virtually independent of the details of the underlying model for the connection of galaxies and matter. Our comparison of the shear around troughs with that around cylinders with large galaxy counts is consistent with a symmetry between galaxy and matter over- and underdensities. In addition, we measure the two-point angular correlation of troughs with galaxies which, in contrast to the lensing signal, is sensitive to galaxy bias on all scales. Finally, the lensing signal of troughs and their clustering with galaxies is therefore a promising probe of the statistical properties of matter underdensities and their connection to the galaxy field.

  17. Des Plaines Landfill Biomass Facility | Open Energy Information

    Open Energy Info (EERE)

    mW 0.0038 GW Commercial Online Date 2004 Heat Rate (BTUkWh) 12916.67 References EPA Web Site1 Loading map... "minzoom":false,"mappingservice":"googlemaps3","type":"TERRAIN...

  18. Weak lensing by galaxy troughs in DES Science Verification data

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Gruen, D.; Friedrich, O.; Amara, A.; Bacon, D.; Bonnett, C.; Hartley, W.; Jain, B.; M. Jarvis; Kavprzak, T.; Krause, E.; et al

    2015-11-29

    In this study, we measure the weak lensing shear around galaxy troughs, i.e. the radial alignment of background galaxies relative to underdensities in projections of the foreground galaxy field over a wide range of redshift in Science Verification data from the Dark Energy Survey. Our detection of the shear signal is highly significant (10σ–15σ for the smallest angular scales) for troughs with the redshift range z ϵ [0.2, 0.5] of the projected galaxy field and angular diameters of 10 arcmin…1°. These measurements probe the connection between the galaxy, matter density, and convergence fields. By assuming galaxies are biased tracers ofmore » the matter density with Poissonian noise, we find agreement of our measurements with predictions in a fiducial Λ cold dark matter model. The prediction for the lensing signal on large trough scales is virtually independent of the details of the underlying model for the connection of galaxies and matter. Our comparison of the shear around troughs with that around cylinders with large galaxy counts is consistent with a symmetry between galaxy and matter over- and underdensities. In addition, we measure the two-point angular correlation of troughs with galaxies which, in contrast to the lensing signal, is sensitive to galaxy bias on all scales. The lensing signal of troughs and their clustering with galaxies is therefore a promising probe of the statistical properties of matter underdensities and their connection to the galaxy field.« less

  19. Forum des Jeuns du Gabon | Open Energy Information

    Open Energy Info (EERE)

    drought and land degradation, Environmentally sound technologies, Gender, Human rights and Sustainable development plans References "UNEP Major Groups Directory"...

  20. Microsoft Word - FY12 Fee Des.doc

    National Nuclear Security Administration (NNSA)

    NR0000031 copies of the amendment; (b) By acknowledging receipt of this amendment on each copy of the offer submitted; or (c) By separate letter or telegram which includes a reference to the solicitation and amendment numbers. FAILURE OF YOUR ACKNOWLEDGEMENT TO BE RECEIVED AT THE PLACE DESIGNATED FOR THE RECEIPT OF OFFERS PRIOR TO THE HOUR AND DATE SPECIFIED MAY RESULT IN REJECTION OF YOUR OFFER. If by virtue of this amendment you desire to change an offer already submitted, such change may be

  1. CX-003491: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Fond du Lac Hydroelectric ProjectCX(s) Applied: B5.1Date: 08/17/2010Location(s): Fond du Lac, MinnesotaOffice(s): Energy Efficiency and Renewable Energy, Golden Field Office

  2. Browse Societies by Language -- E-print Network Societies by...

    Office of Scientific and Technical Information (OSTI)

    des Sciences, des Lettres et des Arts Tunisian Academy of the Sciences, ... de Psilogie Quebec Society of Psychology -- Socit Qubcoise pour l'tude ...

  3. LEDSGP/events/2013workshop | Open Energy Information

    Open Energy Info (EERE)

    Society, Asia LEDS Partnership and the LAC LEDS regional platform. The workshop will be open to participation by officials and experts from government agencies, international...

  4. Eco Alternative | Open Energy Information

    Open Energy Info (EERE)

    Alternative Jump to: navigation, search Name: Eco'Alternative Place: Le Bourget-du-Lac, France Zip: 73370 Product: Complete PV system installer with modules supplied by companies...

  5. Sculpting bespoke mountains: Determining free energies with basis...

    Office of Scientific and Technical Information (OSTI)

    ; McGovern, Michael 2 ; de Pablo, Juan J. 3 + Show Author Affiliations Department of Chemical and Biomolecular Engineering, University of Notre Dame du Lac, Notre Dame,...

  6. Argentina-Support for the Preparation of National Climate Change...

    Open Energy Info (EERE)

    Argentina-Support for the Preparation of National Climate Change Strategy Jump to: navigation, search Name UNDP-Argentina Regional Programme for LAC - Support for the preparation...

  7. SEP Success Story: A Touch of Green for Des Moines’ Sherman Hill

    Broader source: Energy.gov [DOE]

    When the Green & Main Initiative completes the renovation of a 1930s grocery store, the previously abandoned building will be LEED Platinum certified, with a green roof and 54 original windows retrofitted to achieve high energy efficiency standards. Learn more.

  8. The LMC geometry and outer stellar populations from early DES data

    SciTech Connect (OSTI)

    Balbinot, Eduardo; Plazas, A.; Santiago, B. X.; Girardi, L.; Pieres, A.; da Costa, L. N.; Maia, M. A. G.; Gruendl, R. A.; Walker, A. R.; Yanny, B.; Drlica-Wagner, A.; Benoit-Levy, A.; Abbott, T. M. C.; Allam, S. S.; Annis, J.; Bernstein, J. P.; Bernstein, R. A.; Bertin, E.; Brooks, D.; Buckley-Geer, E.; Rosell, A. Carnero; Cunha, C. E.; Depoy, D. L.; Desai, S.; Diehl, H. T.; Doel, P.; Estrada, J.; Evrard, A. E.; Fausti Neto, A.; Finley, D. A.; Flaugher, B.; Frieman, J. A.; Gruen, D.; Honscheid, K.; James, D.; Kuehn, K.; Kuropatkin, N.; Lahav, O.; March, M.; Marshall, J. L.; Miller, C.; Miquel, R.; Ogando, R.; Peoples, J.; Scarpine, V.; Schubnell, M.; Sevilla-Noarbe, I.; Smith, R. C.; Soares-Santos, M.; Suchyta, E.; Swanson, M. E. C.; Tarle, G.; Tucker, D. L.; Wechsler, R.; Zuntz, J.

    2015-03-20

    The Dark Energy Camera has captured a large set of images as part of Science Verification (SV) for the Dark Energy Survey. The SV footprint covers a large portion of the outer Large Magellanic Cloud (LMC), providing photometry 1.5 magnitudes fainter than the main sequence turn-off of the oldest LMC stellar population. We derive geometrical and structural parameters for various stellar populations in the LMC disc. For the distribution of all LMC stars, we find an inclination of i = 38.140.08 (near side in the North) and a position angle for the line of nodes of ?? = 129.510.17. We find that stars younger than ~4 Gyr are more centrally concentrated than older stars. Fitting a projected exponential disc shows that the scale radius of the old populations is R>4Gyr = 1.41 0.01 kpc, while the younger population has R<4Gyr = 0.72 0.01 kpc. However, the spatial distribution of the younger population deviates significantly from the projected exponential disc model. The distribution of old stars suggests a large truncation radius of Rt = 13.5 0.8 kpc. If this truncation is dominated by the tidal field of the Galaxy, we find that the LMC is ?24+96 times less massive than the encircled Galactic mass. By measuring the Red Clump peak magnitude and comparing with the best-fit LMC disc model, we find that the LMC disc is warped and thicker in the outer regions north of the LMC centre. As a result, our findings may either be interpreted as a warped and flared disc in the LMC outskirts, or as evidence of a spheroidal halo component.

  9. Targeted Energy Efficiency Expert Evaluation Report: Neal Smith Federal Building, Des Moines, IA

    SciTech Connect (OSTI)

    Fernandez, Nicholas; Goddard, James K.; Underhill, Ronald M.; Gowri, Krishnan

    2013-03-01

    This report summarizes the energy efficiency measures identified and implemented, and an analysis of the energy savings realized using low-cost/no-cost control system measures identified.

  10. A Radiometric All-Sky Infrared Camera (RASICAM) for DES/CTIO

    SciTech Connect (OSTI)

    Lewis, Peter M.; Rogers, Howard; Schindler, Rafe H.; /SLAC

    2010-08-25

    A novel radiometric all-sky infrared camera [RASICAM] has been constructed to allow automated real-time quantitative assessment of night sky conditions for the Dark Energy Camera [DECam] located on the Blanco Telescope at the Cerro Tololo Inter-American Observatory in Chile. The camera is optimized to detect the position, motion and optical depth of thin, high (8-10km) cirrus clouds and contrails by measuring their apparent temperature above the night sky background. The camera system utilizes a novel wide-field equiresolution catadioptic mirror system that provides sky coverage of 2{pi} azimuth and 14-90{sup o} from zenith. Several new technological and design innovations allow the RASICAM system to provide unprecedented cloud detection and IR-based photometricity quantification. The design of the RASICAM system is presented.

  11. The LMC geometry and outer stellar populations from early DES data

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Balbinot, Eduardo; Plazas, A.; Santiago, B. X.; Girardi, L.; Pieres, A.; da Costa, L. N.; Maia, M. A. G.; Gruendl, R. A.; Walker, A. R.; Yanny, B.; et al

    2015-03-20

    The Dark Energy Camera has captured a large set of images as part of Science Verification (SV) for the Dark Energy Survey. The SV footprint covers a large portion of the outer Large Magellanic Cloud (LMC), providing photometry 1.5 magnitudes fainter than the main sequence turn-off of the oldest LMC stellar population. We derive geometrical and structural parameters for various stellar populations in the LMC disc. For the distribution of all LMC stars, we find an inclination of i = –38.14°±0.08° (near side in the North) and a position angle for the line of nodes of θ₀ = 129.51°±0.17°. Wemore » find that stars younger than ~4 Gyr are more centrally concentrated than older stars. Fitting a projected exponential disc shows that the scale radius of the old populations is R>4Gyr = 1.41 ± 0.01 kpc, while the younger population has R<4Gyr = 0.72 ± 0.01 kpc. However, the spatial distribution of the younger population deviates significantly from the projected exponential disc model. The distribution of old stars suggests a large truncation radius of Rt = 13.5 ± 0.8 kpc. If this truncation is dominated by the tidal field of the Galaxy, we find that the LMC is ≃24+9–6 times less massive than the encircled Galactic mass. By measuring the Red Clump peak magnitude and comparing with the best-fit LMC disc model, we find that the LMC disc is warped and thicker in the outer regions north of the LMC centre. As a result, our findings may either be interpreted as a warped and flared disc in the LMC outskirts, or as evidence of a spheroidal halo component.« less

  12. Status report on an engineering design study of hermetic liquid argon calorimetry for the SSC (Superconducting Super Collider)

    SciTech Connect (OSTI)

    Adams, T.; Davis, M.; DiGiacomo, N.J.; Easom, B.; Gordon, H.; Hupp, J.; Killian, K.; Kroon, P.; Lajczok, M.; Marx, M. . Astronautics Group; Brookhaven National Lab., Upton, NY; Martin Marietta Aerospace, Denver, CO . Astronautics Group; Brookhaven National Lab., Upton, NY; Martin Marietta Aerospace, Denver, CO . Astronautics Group; State Un

    1989-01-01

    There is general recognition that engineering issues are critical to the viability of liquid argon calorimetry (LAC) at the Superconducting Super Collider (SSC). We have undertaken to quantitatively address these issues and, if possible, perform a preliminary design of a proof of principle'' LAC for SSC. To establish LAC as viable at SSC, we must demonstrate that the physics performance of the device is acceptable, despite the presence of dead material due to vessels and support structure. Our approach involves the construction, by a team of physicists and engineers, of one three dimensional model of the LAC system, built as a hierarchy of components and structures, from which we directly perform interferences checks, mechanical, thermal and magnetic analyses, particle tracking, hermeticity evaluation, physics simulation and assembly. This study, begun in February 1989 as part of the SSC generic detector R and D program, was immediately preceded by a workshop at which engineering details of existing and planned LAC systems were thoroughly examined. We describe below the status of our work, beginning with short descriptions of the tools used, the study requirements and LAC configuration baseline. We then detail the LAC design as it presently stands, including assembly considerations, and conclude with a quantitative assessment of the LAC hermeticity. 19 refs., 12 figs.

  13. CX-001634: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Meteorological Tower Installation Mille Lacs Band of Ojibwa Indian ReservationCX(s) Applied: B3.1, A9Date: 04/08/2010Location(s): County of Mille Lacs, MinnesotaOffice(s): Energy Efficiency and Renewable Energy, Golden Field Office

  14. Use of spherically bent crystals to diagnose wire array z pinches

    SciTech Connect (OSTI)

    Shelkovenko, T.A.; Pikuz, S.A.; Hammer, D.A.; Ampleford, D.J.; Bland, S.N.; Bott, S.C.; Chittenden, J.P.; Lebedev, S.V.

    2004-10-01

    Spherically bent mica and quartz crystals have provided time-integrated spectra and monochromatic images in self-radiation of wire array z-pinch implosions on the MAGPIE generator (1 MA, 240 ns) at Imperial College. Diagnostics based on spherically bent crystals offer higher efficiencies than those based on flat or convex dispersion elements, allowing positioning far from the pinch with good debris shielding. A mica crystal spectrometer produced an image of the pinch in each emission line with about 100 {mu}m axial resolution. Combining the results of monochromatic imaging and spectra confirmed the presence of bright spots, probably generated by energetic electrons inside the pinch.

  15. Structure of Stagnated Plasma in Aluminium Wire Array Z-pinches

    SciTech Connect (OSTI)

    Hall, G.N.; Bland, S.N.; Lebedev, S.V.; Ampleford, D.J.; Palmer, J.B.A.; Bott, S.C.; Rapley, J.; Chittenden, J.P.; Pikuz, S.A.; Shelkovenko, T.A.

    2006-01-05

    Experiments with aluminium wire array Z-pinches have been carried out on the MAGPIE generator (1MA, 240ns) at Imperial College London. It has been shown that in these arrays there are two intense sources of radiation during stagnation: line emission from a precursor-sized object and continuum radiation from bright-spots of significantly higher temperature randomly distributed around this object such as to produce a hollow emission profile. Spatially resolved spectra produced by spherically-bent crystals were recorded, both time-integrated and time-resolved, and were used to show that these two sources of radiation peak at the same time.

  16. Danger radiations

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le conférencier Mons.Hofert parle des dangers et risques des radiations, le contrôle des zones et les précautions à prendre ( p.ex. film badge), comment mesurer les radiations etc.

  17. Ablation dynamics in coiled wire-array Z-pinches

    SciTech Connect (OSTI)

    Hall, G. N.; Lebedev, S. V.; Suzuki-Vidal, F.; Swadling, G.; Chittenden, J. P.; Bland, S. N.; Harvey-Thompson, A.; Knapp, P. F.; Blesener, I. C.; McBride, R. D.; Chalenski, D. A.; Blesener, K. S.; Greenly, J. B.; Pikuz, S. A.; Shelkovenko, T. A.; Hammer, D. A.; Kusse, B. R.

    2013-02-15

    Experiments to study the ablation dynamics of coiled wire arrays were performed on the MAGPIE generator (1 MA, 240 ns) at Imperial College, and on the COBRA generator at Cornell University's Laboratory of Plasma Studies (1 MA, 100 ns). The MAGPIE generator was used to drive coiled wires in an inverse array configuration to study the distribution of ablated plasma. Using interferometry to study the plasma distribution during the ablation phase, absolute quantitative measurements of electron line density demonstrated very high density contrasts between coiled ablation streams and inter-stream regions many millimetres from the wire. The measured density contrasts for a coiled array were many times greater than that observed for a conventional array with straight wires, indicating that a much greater axial modulation of the ablated plasma may be responsible for the unique implosion dynamics of coiled arrays. Experiments on the COBRA generator were used to study the complex redirection of plasma around a coiled wire that gives rise to the ablation structure exhibited by coiled arrays. Observations of this complex 3D plasma structure were used to validate the current model of coiled array ablation dynamics [Hall et al., Phys. Rev. Lett. 100, 065003 (2008)], demonstrating irrefutably that plasma flow from the wires behaves as predicted. Coiled wires were observed to ablate and implode in the same manner on both machines, indicating that current rise time should not be an issue for the scaling of coiled arrays to larger machines with fast current rise times.

  18. White House Climate Task Force Tribal Leaders Listening Session

    Broader source: Energy.gov [DOE]

    On Wednesday, February 12, Karen Diver, Chairwoman of the Fond du Lac Band of Lake Superior Chippewa, and Reggie Joule, Mayor of Alaska’s Northwest Arctic Borough, both of whom are members of...

  19. ESO VERY LARGE TELESCOPE OPTICAL SPECTROSCOPY OF BL LACERTAE OBJECTS. IV. NEW SPECTRA AND PROPERTIES OF THE FULL SAMPLE

    SciTech Connect (OSTI)

    Landoni, M.; Treves, A.; Barattini, M.; Falomo, R.; Sbarufatti, B.; Decarli, R.; Kotilainen, J.

    2013-04-15

    We present the last chapter of a spectroscopy program aimed at deriving the redshift or a lower limit to the redshift of BL Lac objects using medium-resolution spectroscopy. Here we report new spectra for 33 BL Lac object candidates obtained in 2008-2009, confirming the BL Lac nature of 25 sources and obtaining new redshifts for 5 objects. These new observations are combined with our previous data in order to construct a homogeneous sample of {approx}70 BL Lac objects with high-quality spectroscopy. All these spectra can be accessed at the Web site http://www.oapd.inaf.it/zbllac/. The average spectrum, beaming properties of the full sample, discussion of intervening systems, and future perspectives are addressed.

  20. CX-006083: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Ground Source Heat Pump Installation - Lac Qui Parle County Courthouse, MinnesotaCX(s) Applied: B5.1Date: 06/27/2011Location(s): Madison, MinnesotaOffice(s): Energy Efficiency and Renewable Energy, Golden Field Office

  1. Slide 1

    Office of Environmental Management (EM)

    event (typical), 78 samples collected annually 12 Water Supply Wells at LAC, CSF Buckman Well Field, and Pueblo de San Ildefonso, and Springs in White Rock Canyon City of...

  2. High density growth of T7 expression strains with auto-induction option

    DOE Patents [OSTI]

    Studier, F. William (Stony Brook, NY)

    2010-07-20

    A bacterial growth medium for promoting auto-induction of transcription of cloned DNA in cultures of bacterial cells grown batchwise is disclosed. The transcription is under the control of a lac repressor. Also disclosed is a bacterial growth medium for improving the production of a selenomethionine-containing protein or polypeptide in a bacterial cell, the protein or polypeptide being produced by recombinant DNA techniques from a lac or T7lac promoter, the bacterial cell encoding a vitamin B12-dependent homocysteine methylase. Finally, disclosed is a bacterial growth medium for suppressing auto-induction of expression in cultures of bacterial cells grown batchwise, said transcription being under the control of lac repressor.

  3. Siting Wind Energy | Open Energy Information

    Open Energy Info (EERE)

    Siting Wind Energy Jump to: navigation, search Wind turbines at the Forward Wind Energy Center in Fond du Lac and Dodge Counties, Wisconsin. Photo from Ruth BaranowskiNREL, NREL...

  4. Leading the Charge: Native Leaders Give Tribes a Voice on White House

    Office of Environmental Management (EM)

    Climate Task Force | Department of Energy Native Leaders Give Tribes a Voice on White House Climate Task Force Leading the Charge: Native Leaders Give Tribes a Voice on White House Climate Task Force March 13, 2014 - 10:56am Addthis Chairwoman Karen Diver, Fond du Lac Band of Lake Superior Chippewa (MN) Chairwoman Karen Diver, Fond du Lac Band of Lake Superior Chippewa (MN) Mayor Reggie Joule, Northwest Arctic Borough (AK) Mayor Reggie Joule, Northwest Arctic Borough (AK) Chairwoman Karen

  5. Structure of stagnated plasma in aluminum wire array Z pinches

    SciTech Connect (OSTI)

    Hall, G. N.; Pikuz, S. A.; Shelkovenko, T. A.; Bland, S. N.; Lebedev, S. V.; Ampleford, D. J.; Palmer, J. B. A.; Bott, S. C.; Rapley, J.; Chittenden, J. P.; Apruzese, J. P.

    2006-08-15

    Experiments with aluminum wire array Z pinches have been carried out on the mega-ampere generator for plasma implosion experiments (MAGPIE) at Imperial College London [I. H. Mitchell et al., Rev. Sci. Instrum. 67, 1533 (1996)]. It has been shown that in these arrays, there are two intense sources of radiation during stagnation; Al XII line emission from a precursor-sized object, and both continuum and Al XIII radiation from bright spots of either significantly higher temperature or density randomly distributed around this object so as to produce a hollow emission profile. Spatially resolved spectra produced by spherically bent crystals were recorded, both time-integrated and time-resolved, and were used to show that these two sources of radiation peak at the same time.

  6. Relativistic jet properties of GeV-TeV blazars and possible implications for the jet formation, composition, and cavity kinematics

    SciTech Connect (OSTI)

    Zhang, Jin; Lu, Ye; Zhang, Shuang-Nan; Sun, Xiao-Na; Liang, En-Wei; Lu, Rui-Jing E-mail: lew@gxu.edu.cn

    2014-06-20

    We fit the spectral energy distributions of a GeV-TeV flat spectrum radio quasar (FSRQ) sample with the leptonic model. Their ?{sub min} of the relativistic electron distributions, which significantly affect the estimate of the jet properties, are constrained, with a typical value of ?48. Their jet power, magnetized parameter, radiation efficiency, and jet production and radiation rates per central black hole (BH) mass are derived and compared with those of BL Lacertae (BL Lac) objects. We show that the FSRQ jets may be dominated by the Poynting flux and have a high radiation efficiency, whereas the BL Lac object jets are likely dominated by particles and have a lower radiation efficiency than FSRQs. Being different from BL Lac objects, the jet powers of FSRQs are proportional to their central BH masses. The jet production and radiation rates of the FSRQs distribute in narrow ranges and are correlated with each other, whereas no similar feature is found for the BL Lac objects. We also show that the jet power is correlated with the cavity kinetic power: the magnetic field energy in the jets may provide the cavity kinetic energy of FSRQs, and the kinetic energy of cold protons in the jets may be crucial for the cavity kinetic energy of BL Lac objects. We suggest that the dominating formation mechanism of FSRQ jets may be the Blandford-Znajek process, but BL Lac object jets may be produced via the Blandford-Payne and/or Blandford-Znajek processes, depending on the structures and accretion rates of accretion disks.

  7. Field Testing of LIDAR-Assisted Feedforward Control Algorithms for Improved Speed Control and Fatigue Load Reduction on a 600-kW Wind Turbine: Preprint

    SciTech Connect (OSTI)

    Kumar, Avishek A.; Bossanyi, Ervin A.; Scholbrock, Andrew K.; Fleming, Paul; Boquet, Mathieu; Krishnamurthy, Raghu

    2015-12-14

    A severe challenge in controlling wind turbines is ensuring controller performance in the presence of a stochastic and unknown wind field, relying on the response of the turbine to generate control actions. Recent technologies such as LIDAR, allow sensing of the wind field before it reaches the rotor. In this work a field-testing campaign to test LIDAR Assisted Control (LAC) has been undertaken on a 600-kW turbine using a fixed, five-beam LIDAR system. The campaign compared the performance of a baseline controller to four LACs with progressively lower levels of feedback using 35 hours of collected data.

  8. Research- Knowledge

    ScienceCinema (OSTI)

    None

    2011-04-25

    S.Mansholt, connu sur le marché commun de la communité européenne, est agriculteur et agronome de profession et un des pionnier et animateur des affaires d'unification européene

  9. Energy Citations Database (ECD) - Availability

    Office of Scientific and Technical Information (OSTI)

    vente des publications des Communautes Europeenes 37, rue Glesener-Luxembourg. FD U.S. Fish and Wildlife Service, 18th and C Streets, N.W., Mail Stop 1111, Arlington Square Bldg.,...

  10. Celebration of PS

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le DG John Adams parle des premières années du PS avec présentation des dias ainsi il honore Pierre Germain qui après 24 ans de travail quitte sa fonction.

  11. Sciences and society

    SciTech Connect (OSTI)

    2008-01-10

    J.Luns des Pays-Bas, ancien sctaire gnral de NATO (OTAN=Organisation du trait de l'Atlantique Nord) parle du pass, prsent et future de la dfense europenne et des relations est et ouest

  12. EECBG Success Story: After 105 Years, Historic City Hall in West...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    After 105 Years, Historic City Hall in West Des Moines, Iowa Goes Green EECBG Success Story: After 105 Years, Historic City Hall in West Des Moines, Iowa Goes Green May 9, 2011 -...

  13. CX-006500: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Magellan Des Moines Biodiesel Terminal ProjectCX(s) Applied: B5.1Date: 09/06/2011Location(s): Des Moines, IowaOffice(s): Energy Efficiency and Renewable Energy, Golden Field Office

  14. Fermilab | Newsroom | Press Releases | March 10, 2015: Scientists...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    3 March 10, 2015 FOR IMMEDIATE RELEASE Scientists find rare dwarf satellite galaxy candidates in Dark Energy Survey data DES-Dwarf-Galaxies DES-Dwarf-Galaxies Previous Next...

  15. Departure Roger Anthoine

    SciTech Connect (OSTI)

    2007-11-28

    Remerciements et discours du D.G. H.Schopper l'occasion du dpart de Roger Anthoine (attach de presse), qui travaillait dans la communication et quitte le Cern aprs 27 ans de service. Il gardait des relations avec des mdias internationaux et la presse locale; remise des cadeaux: album photo avec images des muss de Genve et un radio aviation; R.A. fait un rsum de ses activits et souvenirs et remercie ses collaborateurs

  16. PET

    ScienceCinema (OSTI)

    None

    2011-04-25

    le DG fait l'introduction et laisse la parole à plusieurs intervenants au sujet de la physique des particules

  17. Gas Technology Institute (Partnership for Advanced Residential...

    Open Energy Info (EERE)

    Technology Institute (Partnership for Advanced Residential Retrofit) Jump to: navigation, search Name: Gas Technology Institute Place: Des Plaines, IL Website:...

  18. Utilization Technology Institute | Open Energy Information

    Open Energy Info (EERE)

    Utilization Technology Institute Jump to: navigation, search Name: Utilization Technology Institute Place: Des Plaines, IL References: Utilization Technology Institute1...

  19. Visit CD

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le DG H.Schopper souhaite la bienvenue aux ambassadeurs des pays membres et aux représentants des pays avec lesquels le Cern entretient des relations proches et fait un exposé sur les activités au Cern

  20. CX-004608: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Chippewa Tribe of Minnesota on behalf of the Mille Lacs Band Renewable Energy Technologies on Government BuildingsCX(s) Applied: B3.6, B5.1Date: 01/08/2010Location(s): Tower, MinnesotaOffice(s): Energy Efficiency and Renewable Energy

  1. CX-004607: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Chippewa Tribe of Minnesota on behalf of the Mille Lacs Band Residential and Commercial Building Energy AuditsCX(s) Applied: A9, B5.1Date: 01/08/2010Location(s): Tower, MinnesotaOffice(s): Energy Efficiency and Renewable Energy

  2. Atomic spectrum of plutonium

    SciTech Connect (OSTI)

    Blaise, J.; Fred, M.; Gutmacher, R.G.

    1984-08-01

    This report contains plutonium wavelengths, energy level classifications, and other spectroscopic data accumulated over the past twenty years at Laboratoire Aime Cotton (LAC) Argonne National Laboratory (ANL), and Lawrence Livermore National Laboratory (LLNL). The primary purpose was term analysis: deriving the energy levels in terms of quantum numbers and electron configurations, and evaluating the Slater-Condon and other parameters from the levels.

  3. L-Area Reactor - 1993 annual - groundwater monitoring report

    SciTech Connect (OSTI)

    Chase, J.A.

    1994-09-01

    Groundwater was sampled and analyzed during 1993 from wells monitoring the water table at the following locations in L Area: the L-Area Acid/Caustic Basin (four LAC wells), L-Area Research Wells in the southern portion of the area (outside the fence; three LAW wells), the L-Area Oil and Chemical Basin (four LCO wells), the L-Area Disassembly Basin (two LDB wells), the L-Area Burning/Rubble Pit (four LRP wells), and the L-Area Seepage Basin (four LSB wells). During 1993, tetrachloroethylene was detected above its drinking water standard (DWS) in the LAC, LAW, LCO, and LDB well series. Lead exceeded its 50 {mu}g/L standard in the LAW, LDB, and LRP series, and tritium was above its DWS in the LAW, LCO, and LSB series. Apparently anomalous elevated levels of the common laboratory contaminant bis(2-ethylhexyl)phthalate were reported during first quarter in one well each in the LAC series and LCO series, and during third quarter in a different LCO well. Extensive radionuclide analyses were performed during 1993 in the LAC, LAW, and LCO well series. No radionuclides other than tritium were reported above DWS or Flag 2 criteria.

  4. The endocrine disruptor diethylstilbestrol induces adipocyte differentiation and promotes obesity in mice

    SciTech Connect (OSTI)

    Hao, Chan-Juan; Cheng, Xue-Jia; Xia, Hong-Fei, E-mail: hongfeixia@yahoo.com.cn; Ma, Xu

    2012-08-15

    Epidemiology studies indicate that exposure to endocrine disruptors during developmental window contributes to adipogenesis and the development of obesity. Implication of endocrine disruptor such as diethylstilbestrol (DES) on adipose tissue development has been poorly investigated. Here we evaluated the effects of DES on adipocyte differentiation in vitro and in vivo, and explored potential mechanism involved in its action. DES induced 3T3-L1 preadipocyte differentiation in a dose-dependent manner, and activated the expression of estrogen receptor (ER) and peroxisome proliferator-acivated receptor (PPAR) ? as well as its target genes required for adipogenesis in vitro. ER mediated the enhancement of DES-induced PPAR? activity. Moreover, DES perturbed key regulators of adipogenesis and lipogenic pathway in vivo. In utero exposure to low dose of DES significantly increased body weight, liver weight and fat mass in female offspring at postnatal day (PND) 60. In addition, serum triglyceride and glucose levels were also significantly elevated. These results suggest that perinatal exposure to DES may be expected to increase the incidence of obesity in a sex-dependent manner and can act as a potential chemical stressor for obesity and obesity-related disorders. -- Highlights: ? DES induced adipocyte differentiation in a dose-dependent manner in 3T3-L1 cells. ? DES activated adipogenic critical regulators and markers in vitro and in vivo. ? Perinatal exposure to DES led to the obese phenotype in female offspring. ? DES might be a potential chemical stressor for obesity and obesity-related disorders.

  5. An HST/COS observation of broad Ly? emission and associated absorption lines of the BL Lacertae object H 2356-309

    SciTech Connect (OSTI)

    Fang, Taotao [Department of Astronomy and Institute of Theoretical Physics and Astrophysics, Xiamen University, Xiamen, Fujian 361005 (China); Danforth, Charles W.; Stocke, John T.; Shull, J. Michael [CASA, Department of Astrophysical and Planetary Sciences, University of Colorado, 389-UCB, Boulder, CO 80309 (United States); Buote, David A. [Department of Physics and Astronomy, 4129 Frederick Reines Hall, University of California, Irvine, CA 92697 (United States); Canizares, Claude R. [Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139 (United States); Gastaldello, Fabio, E-mail: fangt@xmu.edu.cn [IASF-Milano, INAF, via Bassini 15, Milan I-20133 (Italy)

    2014-11-01

    Weak spectral features in BL Lacertae objects (BL Lacs) often provide a unique opportunity to probe the inner region of this rare type of active galactic nucleus. We present a Hubble Space Telescope/Cosmic Origins Spectrograph observation of the BL Lac H 2356-309. A weak Ly? emission line was detected. This is the fourth detection of a weak Ly? emission feature in the ultraviolet (UV) band in the so-called high-energy peaked BL Lacs, after Stocke et al. Assuming the line-emitting gas is located in the broad line region (BLR) and the ionizing source is the off-axis jet emission, we constrain the Lorentz factor (?) of the relativistic jet to be ?8.1 with a maximum viewing angle of 3.6. The derived ? is somewhat larger than previous measurements of ? ? 3-5, implying a covering factor of ?3% of the line-emitting gas. Alternatively, the BLR clouds could be optically thin, in which case we constrain the BLR warm gas to be ?10{sup 5} M {sub ?}. We also detected two H I and one O VI absorption lines that are within |?v| < 150 km s{sup 1} of the BL Lac object. The O VI and one of the H I absorbers likely coexist due to their nearly identical velocities. We discuss several ionization models and find a photoionization model where the ionizing photon source is the BL Lac object that can fit the observed ion column densities with reasonable physical parameters. This absorber can either be located in the interstellar medium of the host galaxy or in the BLR.

  6. RADIATION MECHANISM AND JET COMPOSITION OF GAMMA-RAY BURSTS AND GeV-TeV-SELECTED RADIO-LOUD ACTIVE GALACTIC NUCLEI

    SciTech Connect (OSTI)

    Zhang Jin; Lu Ye; Zhang Shuangnan; Liang Enwei; Sun Xiaona; Zhang Bing

    2013-09-01

    Gamma-ray bursts (GRBs) and GeV-TeV-selected radio-loud active galactic nuclei (AGNs) are compared based on our systematic modeling of the observed spectral energy distributions of a sample of AGNs with a single-zone leptonic model. We show that the correlation between the jet power (P{sub jet}) and the prompt gamma-ray luminosity (L{sub jet}) of GRBs is consistent, within the uncertainties, with the correlation between jet power and the synchrotron peak luminosity (L{sub s,jet}) of flat spectrum radio quasars (FSRQs). Their radiation efficiencies ({epsilon}) are also comparable (>10% for most sources), which increase with the bolometric jet luminosity (L{sub bol,jet}) for FSRQs and with the L{sub jet} for GRBs with similar power-law indices. BL Lac objects (BL Lacs) do not follow the P{sub jet}-L{sub s,jet} relation of FSRQs. They have lower {epsilon} and L{sub bol,jet} values than FSRQs, and a tentative L{sub bol,jet}-{epsilon} relation is also found, with a power-law index different from that of the FSRQs. The magnetization parameters ({sigma}) of FSRQs are on average larger than that of BL Lacs. They are anti-correlated with {epsilon} for the FSRQs, but positively correlated with {epsilon} for the BL Lacs. GeV narrow-line Seyfert 1 galaxies potentially share similar properties with FSRQs. Based on the analogy between GRBs and FSRQs, we suggest that the prompt gamma-ray emission of GRBs is likely produced by the synchrotron process in a magnetized jet with high radiation efficiency, similar to FSRQs. The jets of BL Lacs, on the other hand, are less efficient and are likely more matter-dominated.

  7. Summary Statistics for Homemade ?Play Dough? -- Data Acquired at LLNL

    SciTech Connect (OSTI)

    Kallman, J S; Morales, K E; Whipple, R E; Huber, R D; Martz, A; Brown, W D; Smith, J A; Schneberk, D J; Martz, Jr., H E; White, III, W T

    2010-03-11

    Using x-ray computerized tomography (CT), we have characterized the x-ray linear attenuation coefficients (LAC) of a homemade Play Dough{trademark}-like material, designated as PDA. Table 1 gives the first-order statistics for each of four CT measurements, estimated with a Gaussian kernel density estimator (KDE) analysis. The mean values of the LAC range from a high of about 2700 LMHU{sub D} 100kVp to a low of about 1200 LMHUD at 300kVp. The standard deviation of each measurement is around 10% to 15% of the mean. The entropy covers the range from 6.0 to 7.4. Ordinarily, we would model the LAC of the material and compare the modeled values to the measured values. In this case, however, we did not have the detailed chemical composition of the material and therefore did not model the LAC. Using a method recently proposed by Lawrence Livermore National Laboratory (LLNL), we estimate the value of the effective atomic number, Z{sub eff}, to be near 10. LLNL prepared about 50mL of the homemade 'Play Dough' in a polypropylene vial and firmly compressed it immediately prior to the x-ray measurements. We used the computer program IMGREC to reconstruct the CT images. The values of the key parameters used in the data capture and image reconstruction are given in this report. Additional details may be found in the experimental SOP and a separate document. To characterize the statistical distribution of LAC values in each CT image, we first isolated an 80% central-core segment of volume elements ('voxels') lying completely within the specimen, away from the walls of the polypropylene vial. All of the voxels within this central core, including those comprised of voids and inclusions, are included in the statistics. We then calculated the mean value, standard deviation and entropy for (a) the four image segments and for (b) their digital gradient images. (A digital gradient image of a given image was obtained by taking the absolute value of the difference between the initial image and that same image offset by one voxel horizontally, parallel to the rows of the x-ray detector array.) The statistics of the initial image of LAC values are called 'first order statistics;' those of the gradient image, 'second order statistics.'

  8. Summary Statistics for Fun Dough Data Acquired at LLNL

    SciTech Connect (OSTI)

    Kallman, J S; Morales, K E; Whipple, R E; Huber, R D; Brown, W D; Smith, J A; Schneberk, D J; Martz, Jr., H E; White, III, W T

    2010-03-11

    Using x-ray computerized tomography (CT), we have characterized the x-ray linear attenuation coefficients (LAC) of a Play Dough{trademark}-like product, Fun Dough{trademark}, designated as PD. Table 1 gives the first-order statistics for each of four CT measurements, estimated with a Gaussian kernel density estimator (KDE) analysis. The mean values of the LAC range from a high of about 2100 LMHU{sub D} at 100kVp to a low of about 1100 LMHU{sub D} at 300kVp. The standard deviation of each measurement is around 1% of the mean. The entropy covers the range from 3.9 to 4.6. Ordinarily, we would model the LAC of the material and compare the modeled values to the measured values. In this case, however, we did not have the composition of the material and therefore did not model the LAC. Using a method recently proposed by Lawrence Livermore National Laboratory (LLNL), we estimate the value of the effective atomic number, Z{sub eff}, to be near 8.5. LLNL prepared about 50mL of the Fun Dough{trademark} in a polypropylene vial and firmly compressed it immediately prior to the x-ray measurements. Still, layers can plainly be seen in the reconstructed images, indicating that the bulk density of the material in the container is affected by voids and bubbles. We used the computer program IMGREC to reconstruct the CT images. The values of the key parameters used in the data capture and image reconstruction are given in this report. Additional details may be found in the experimental SOP and a separate document. To characterize the statistical distribution of LAC values in each CT image, we first isolated an 80% central-core segment of volume elements ('voxels') lying completely within the specimen, away from the walls of the polypropylene vial. All of the voxels within this central core, including those comprised of voids and inclusions, are included in the statistics. We then calculated the mean value, standard deviation and entropy for (a) the four image segments and for (b) their digital gradient images. (A digital gradient image of a given image was obtained by taking the absolute value of the difference between the initial image and that same image offset by one voxel horizontally, parallel to the rows of the x-ray detector array.) The statistics of the initial image of LAC values are called 'first order statistics;' those of the gradient image, 'second order statistics.'

  9. National Association of the Remodeling Industry (NARI) | Open...

    Open Energy Info (EERE)

    Association of the Remodeling Industry (NARI) Jump to: navigation, search Name: National Association of the Remodeling Industry (NARI) Place: Des Plaines, IL Website: www.nari.org...

  10. AgraGate Carbon Credits Corporation | Open Energy Information

    Open Energy Info (EERE)

    AgraGate Carbon Credits Corporation Jump to: navigation, search Name: AgraGate Carbon Credits Corporation Place: Des Moines, Iowa Zip: 50266 Product: Offset aggregators that work...

  11. The english at Cern

    ScienceCinema (OSTI)

    None

    2011-04-25

    Assemblée du personnel anglais traitant des sujets tels affaires sociales, salaires, caisse de pension etc....avec plusieurs conférenciers (date inconnue)

  12. Iowa Department of Economic Development | Open Energy Information

    Open Energy Info (EERE)

    Department of Economic Development Jump to: navigation, search Name: Iowa Department of Economic Development Place: Des Moines, Iowa Zip: 50309 Product: Iowa economic development...

  13. 65th Birthday of Dr.Owen Lock

    ScienceCinema (OSTI)

    None

    2011-04-25

    Remerciements au Dr.Owen Lock, un des pionniers du Cern, à l'occasion de son 65me anniversaire et sa retraite (avec plusieurs intervenants)

  14. General Staff Meeting

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le DG H.Schopper informe le personnel des derniers événements au Cern, comme: 1.) Décision du LEP 2.) Budget 3.) Pension

  15. Jawaharlal Nehru

    ScienceCinema (OSTI)

    None

    2011-04-25

    L'orateur S.E. Giusti del Giardino a connu Nehru (ennemi des castes) les dernières années de sa vie

  16. Roeder Farms | Open Energy Information

    Open Energy Info (EERE)

    Developer 5045 Wind Partners Energy Purchaser Alliant Energy Location Des Moines IA Coordinates 43.29729211, -93.28315258 Show Map Loading map... "minzoom":false,"mapp...

  17. Iowa Office of Energy Independence | Open Energy Information

    Open Energy Info (EERE)

    navigation, search Name: Iowa Office of Energy Independence Place: Des Moines, Iowa Zip: IA 50319 Product: In 2007, Governor Culver and the Iowa State Legislature created the...

  18. Energy Savings with Acceptable Indoor Air Quality Through Improved Air Flow Control in Residential Retrofit

    Broader source: Energy.gov [DOE]

    Lead Performer: Gas Technology Institute—Des Plaines, IL Partners: -- University of Illinois, Urbana IL -- Midwest Energy Efficiency Alliance, Chicago IL

  19. June 16 & 17, 2014 Meeting of the Electricity Advisory Committee...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Doug Larson, WIEB Steve Beuning, Xcel Carrie Cullen Hitt, SEIA Tuesday, June 17, 2014 Panel - Distributed Energy Storage (DES) - Wanda Reder, S&C, moderator Willem Fadrhonc, STEM ...

  20. International Association of Public Transport | Open Energy Informatio...

    Open Energy Info (EERE)

    search Name: International Association of Public Transport Address: Rue Sainte-Marie 6 (Quai des Charbonnages) Place: Brussels, Belgium Zip: B-1080 Sector: Vehicles Year...

  1. Apollo Solar Energy Inc | Open Energy Information

    Open Energy Info (EERE)

    Inc Jump to: navigation, search Name: Apollo Solar Energy Inc Place: Bethel, Connecticut Zip: 68010 Sector: Solar Product: String representation "The company des ... e &...

  2. Solaire Durance | Open Energy Information

    Open Energy Info (EERE)

    Jump to: navigation, search Name: Solaire Durance Place: France Sector: Solar Product: Joint venture between French state bank la Caisse des Dpots and French solar power...

  3. "Title","Creator/Author","Publication Date","OSTI Identifier...

    Office of Scientific and Technical Information (OSTI)

    Royale Pour L'Avancement Des Sciences","USDOE","36 MATERIALS SCIENCE Clean Coal Technology Coal - Environmental Processes",,"The feasibility of using carbon dioxide as...

  4. 2016 High School Science Bowl Participating Teams | The Ames...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    (Bettendorf) Prince of Peace (Clinton) Regina (Iowa City) Roland-Story Shenandoah St. Albert (Council Bluffs) Union (La Porte City) Valley (West Des Moines) West Central Valley...

  5. Transcendental Meditation

    ScienceCinema (OSTI)

    None

    2011-04-25

    K.Wallace, qui vient des Etats Unis, parle des effects physiologiques de la méditation transcendantale. Il a fait son bachelor en physique à l'Université de Los Angeles et son doctorat en physiologie aussi à Los Angeles, mais à l'Institut de Recherche sur le cerveau. Il travaille maintenat à Harvard Medical School ou il continue des recherches biochimiques et physiologiques sur l'application médicale de la méditation transcendantale. Il s'occupe principalement des maladies cardiaques et de hypertension artérielle.

  6. FY 2014 Projects for Improving the Design, Construction, and...

    Energy Savers [EERE]

    Institute (Des Plaines, Ill.) - Simultaneous Waste Heat and Water Recovery from Power Plant Flue Gases for Advanced Energy Systems. The project team will further develop an...

  7. St. Charles County, Missouri: Energy Resources | Open Energy...

    Open Energy Info (EERE)

    Missouri O'Fallon, Missouri Portage Des Sioux, Missouri St. Charles, Missouri St. Paul, Missouri St. Peters, Missouri Weldon Spring Heights, Missouri Weldon Spring, Missouri...

  8. Browse by Discipline -- E-print Network Subject Pathways: Plasma...

    Office of Scientific and Technical Information (OSTI)

    Ecole des Mines de Nantes Kasher, Roni (Roni Kasher) - Zuckerberg Institute for Water Research, Zuckerberg Institute for Water Research, Jacob Blaustein Institutes for Desert ...

  9. Departure Roger Anthoine

    ScienceCinema (OSTI)

    None

    2011-04-25

    Remerciements et discours du D.G. H.Schopper à l'occasion du départ de Roger Anthoine (attaché de presse), qui travaillait dans la communication et quitte le Cern après 27 ans de service. Il gardait des relations avec des médias internationaux et la presse locale; remise des cadeaux: album photo avec images des musés de Genève et un radio aviation; R.A. fait un résumé de ses activités et souvenirs et remercie ses collaborateurs

  10. Cloning and expression of autogenes encoding RNA poly,erases of T7-like bacteriophages

    DOE Patents [OSTI]

    Studier, F. William (Stony Brook, NY); Dubendorff, John W. (Sound Beach, NY)

    1998-01-01

    This invention relates to the cloning and expression of autogenes encoding RNA polymerases of T7 and T7-like bacteriophages, in which the RNA polymerase gene is transcribed from a promoter which is recognized by the encoded RNA polymerase. Cloning of T7 autogenes was achieved by reducing the activity of the RNA polymerase sufficiently to permit host cell growth. T7 RNA polymerase activity was controlled by combining two independent methods: lac-repression of the recombinant lac operator-T7 promoter in the autogene and inhibition of the polymerase by T7 lysozyme. Expression systems for producing the RNA polymerases of T7 and other T7-like bacteriophages, and expression systems for producing selected gene products are described, as well as other related materials and methods.

  11. Cloning and expression of autogenes encoding RNA polymerases of T7-like bacteriophages

    DOE Patents [OSTI]

    Studier, F. William (Stony Brook, NY); Dubendorff, John W. (Sound Beach, NY)

    1998-01-01

    This invention relates to the cloning and expression of autogenes encoding RNA polymerases of T7 and T7-like bacteriophages, in which the RNA polymerase gene is transcribed from a promoter which is recognized by the encoded RNA polymerase. Cloning of T7 autogenes was achieved by reducing the activity of the RNA polymerase sufficiently to permit host cell growth. T7 RNA polymerase activity was controlled by combining two independent methods: lac-repression of the recombinant lac operator-T7 promoter in the autogene and inhibition of the polymerase by T7 lysozyme. Expression systems for producing the RNA polymerases of T7 and other T7-like bacteriophages, and expression systems for producing selected gene products are described, as well as other related materials and methods.

  12. Cloning and expression of autogenes encoding RNA polymerases of T7-like bacteriophages

    DOE Patents [OSTI]

    Studier, F.W.; Dubendorff, J.W.

    1998-10-20

    This invention relates to the cloning and expression of autogenes encoding RNA polymerases of T7 and T7-like bacteriophages, in which the RNA polymerase gene is transcribed from a promoter which is recognized by the encoded RNA polymerase. Cloning of T7 autogenes was achieved by reducing the activity of the RNA polymerase sufficiently to permit host cell growth. T7 RNA polymerase activity was controlled by combining two independent methods: lac-repression of the recombinant lac operator-T7 promoter in the autogene and inhibition of the polymerase by T7 lysozyme. Expression systems for producing the RNA polymerases of T7 and other T7-like bacteriophages, and expression systems for producing selected gene products are described, as well as other related materials and methods. 12 figs.

  13. Cloning and expression of autogenes encoding RNA polymerases of T7-like bacteriophages

    DOE Patents [OSTI]

    Studier, F.W.; Dubendorff, J.W.

    1998-11-03

    This invention relates to the cloning and expression of autogenes encoding RNA polymerases of T7 and T7-like bacteriophages, in which the RNA polymerase gene is transcribed from a promoter which is recognized by the encoded RNA polymerase. Cloning of T7 autogenes was achieved by reducing the activity of the RNA polymerase sufficiently to permit host cell growth. T7 RNA polymerase activity was controlled by combining two independent methods: lac-repression of the recombinant lac operator-T7 promoter in the autogene and inhibition of the polymerase by T7 lysozyme. Expression systems for producing the RNA polymerases of T7 and other T7-like bacteriophages, and expression systems for producing selected gene products are described, as well as other related materials and methods. 12 figs.

  14. Repressor-mediated tissue-specific gene expression in plants

    DOE Patents [OSTI]

    Meagher, Richard B. (Athens, GA); Balish, Rebecca S. (Oxford, OH); Tehryung, Kim (Athens, GA); McKinney, Elizabeth C. (Athens, GA)

    2009-02-17

    Plant tissue specific gene expression by way of repressor-operator complexes, has enabled outcomes including, without limitation, male sterility and engineered plants having root-specific gene expression of relevant proteins to clean environmental pollutants from soil and water. A mercury hyperaccumulation strategy requires that mercuric ion reductase coding sequence is strongly expressed. The actin promoter vector, A2pot, engineered to contain bacterial lac operator sequences, directed strong expression in all plant vegetative organs and tissues. In contrast, the expression from the A2pot construct was restricted primarily to root tissues when a modified bacterial repressor (LacIn) was coexpressed from the light-regulated rubisco small subunit promoter in above-ground tissues. Also provided are analogous repressor operator complexes for selective expression in other plant tissues, for example, to produce male sterile plants.

  15. LA-UR-14-22379 Trails Management at LANL

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    4-22379 Trails Management at LANL New informational kiosk and gates installed at the Potrillo Canyon Loop trailhead in TA-71 near Pajarito Acres. Background Recreational trails use at Los Alamos National Laboratory (LANL) has been considered one of the benefits of working and living in Los Alamos County (LAC). However, there was never an explicit Department of Energy (DOE)/National Nuclear Security Administration (NNSA) or Los Alamos National Security, LLC policy or mechanism to balance trails

  16. Tribal Leaders Provide White House with Input on Bolstering Climate

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Resilience | Department of Energy Leaders Provide White House with Input on Bolstering Climate Resilience Tribal Leaders Provide White House with Input on Bolstering Climate Resilience January 7, 2015 - 10:29am Addthis As members of the President's State, Local, and Tribal Leaders Task Force on Climate Preparedness, Mayor Reggie Joule, Northwest Arctic Borough (AK) and Chairwoman Karen Diver, Fond du Lac Band of Lake Superior Chippewa (MN), were tasked by the President with providing

  17. THE MICRO-ARCSECOND SCINTILLATION-INDUCED VARIABILITY (MASIV) SURVEY. III. OPTICAL IDENTIFICATIONS AND NEW REDSHIFTS

    SciTech Connect (OSTI)

    Pursimo, Tapio; Ojha, Roopesh; Rickett, Barney J.; Dutka, Michael S.; Koay, Jun Yi; Bignall, Hayley E.; Macquart, Jean-Pierre; Lovell, James E. J.; Kedziora-Chudczer, Lucyna

    2013-04-10

    Intraday variability (IDV) of the radio emission from active galactic nuclei is now known to be predominantly due to interstellar scintillation (ISS). The MASIV (The Micro-Arcsecond Scintillation-Induced Variability) survey of 443 flat spectrum sources revealed that the IDV is related to the radio flux density and redshift. A study of the physical properties of these sources has been severely handicapped by the absence of reliable redshift measurements for many of these objects. This paper presents 79 new redshifts and a critical evaluation of 233 redshifts obtained from the literature. We classify spectroscopic identifications based on emission line properties, finding that 78% of the sources have broad emission lines and are mainly FSRQs. About 16% are weak lined objects, chiefly BL Lacs, and the remaining 6% are narrow line objects. The gross properties (redshift, spectroscopic class) of the MASIV sample are similar to those of other blazar surveys. However, the extreme compactness implied by ISS favors FSRQs and BL Lacs in the MASIV sample as these are the most compact object classes. We confirm that the level of IDV depends on the 5 GHz flux density for all optical spectral types. We find that BL Lac objects tend to be more variable than broad line quasars. The level of ISS decreases substantially above a redshift of about two. The decrease is found to be generally consistent with ISS expected for beamed emission from a jet that is limited to a fixed maximum brightness temperature in the source rest frame.

  18. DISCOVERY OF AN EXTENDED X-RAY JET IN AP LIBRAE

    SciTech Connect (OSTI)

    Kaufmann, S.; Wagner, S. J.; Tibolla, O.

    2013-10-20

    Chandra observations of the low-energy-peaked BL Lac object (LBL) AP Librae (AP Lib) revealed the clear discovery of a non-thermal X-ray jet. AP Lib is the first LBL with an extended non-thermal X-ray jet that shows emission into the very high energy range. The X-ray jet has an extension of ?15''(? 14 kpc). The X-ray jet morphology is similar to the radio jet observed with Very Large Array at 1.36 GHz emerging in the southeast direction and bends by 50 at a distance of 12'' toward the northeast. The intensity profiles of the X-ray emission studied are consistent with those found in the radio range. The spectral analysis reveals that the X-ray spectra of the core and jet region are both inverse-Compton-(IC)-dominated. This adds to a still small sample of BL Lac objects whose X-ray jets are IC-dominated and thus more similar to the high-luminosity Fanaroff-Riley II sources than to the low-luminosity Fanaroff-Riley I objects, which are usually considered to be the parent population of BL Lac objects.

  19. Science and Society

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le conférencier (qui? L'introduction manque) est économiste et directeur d'un institut de recherche. Il parlera des conséquences économiques désastreuses des dépenses militaires.

  20. Iowa Water and Wastewater Operators Seek SEP Certification in New Pilot Program

    Broader source: Energy.gov [DOE]

    The Des Moines Metropolitan Wastewater Reclamation Authority (WRA) and Des Moines Water Works have committed to participate in the Superior Energy Performance (SEP) program as the first members of a new program pilot. SEP recognizes facilities that meet the ISO 50001 global energy management standard and demonstrate improved energy performance.

  1. Memorial Lew Kowarski

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le DG J.Adams et d'autres intervenants rendent hommage à L.Kowarski (1907-1979), un des pionniers du Cern en 1952, né à St.Petersbourg et physicien, chimiste et ingénieur. Depuis sa retraite en 1972, il se consacra à l'enseignement et est conseiller des Nations Unies.

  2. CX-001027: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Development of an Autogas Network (Des Plains)CX(s) Applied: A9, B2.5, B3.6, B5.1Date: 03/02/2010Location(s): Des Plaines, IllinoisOffice(s): Energy Efficiency and Renewable Energy, National Energy Technology Laboratory

  3. Sciences and society

    ScienceCinema (OSTI)

    None

    2011-04-25

    J.Luns des Pays-Bas, ancien sécétaire général de NATO (OTAN=Organisation du traité de l'Atlantique Nord) parle du passé, présent et future de la défense européenne et des relations est et ouest

  4. CX-006016: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Energy Efficiency and Conservation Block Grant Program - Iowa-City-West Des MoinesCX(s) Applied: A1, A9, B2.5, B5.1Date: 05/27/2011Location(s): Des Moines, IowaOffice(s): Energy Efficiency and Renewable Energy

  5. CX-005264: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Illinois-City-Des PlainesCX(s) Applied: A9, B2.5, B3.6, B5.1Date: 02/15/2011Location(s): Des Plaines, IllinoisOffice(s): Energy Efficiency and Renewable Energy

  6. CX-003913: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Iowa-City-Des MoinesCX(s) Applied: A1, A9, A11, B1.32, B5.1Date: 09/17/2010Location(s): Des Moines, IowaOffice(s): Energy Efficiency and Renewable Energy

  7. The new role of scientists

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le D.G. Jentschke fait l'introduction et présente le Prof.Kowarsky, spécialiste en microbiologie, physique nucléaire et une des fondateurs du Cern. Il parle entre autre de l'énergie nucléaire (pacifique)et de remise en questions des valeurs scientifiques et techniques

  8. Meeting Jentschke

    ScienceCinema (OSTI)

    None

    2011-04-25

    Après une introduction des dernières recherches et nouvelles au Cern, le DG W.Jentschke parle du futur management du Cern avec deux nouv directeurs générales, responsables pour les 5 ans prochains: le Dr.J.B.Adams qui s'occupera de l'administration du Cern et aussi de la construction des bâtiments et équipements et Le Dr.L.van Hove qui sera responsable pour les activités de la recherche. Le DG parle des changes et structures prévus, des services communs, des différentes divisions et leurs chefs etc...

  9. Two-dimensional electron gas in monolayer InN quantum wells

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Pan, Wei; Dimakis, Emmanouil; Wang, George T.; Moustakas, Theodore D.; Tsui, Daniel C.

    2014-11-24

    We report in this letter experimental results that confirm the two-dimensional nature of the electron systems in monolayer InN quantum wells embedded in GaN barriers. The electron density and mobility of the two-dimensional electron system (2DES) in these InN quantum wells are 5×1015 cm-2 and 420 cm2 /Vs, respectively. Moreover, the diagonal resistance of the 2DES shows virtually no temperature dependence in a wide temperature range, indicating the topological nature of the 2DES.

  10. Mutual Insurance Company of West

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Step : On the right side of the homepage under "Identity The Protection," click on "Create Member Account." Once you log in, create an additional username and password to For more information call - - or visit ARAGLegalCenter.com. Limitations and exclusions apply. Insurance products are underwritten by ARAG Insurance Company of Des Moines, Iowa, GuideOne ® Mutual Insurance Company of West Des Moines, Iowa or GuideOne Specialty Mutual Insurance Company of West Des Moines,

  11. LACERTA I AND CASSIOPEIA III. TWO LUMINOUS AND DISTANT ANDROMEDA SATELLITE DWARF GALAXIES FOUND IN THE 3{pi} PAN-STARRS1 SURVEY

    SciTech Connect (OSTI)

    Martin, Nicolas F.; Laevens, Benjamin P. M.; Slater, Colin T.; Bell, Eric F.; Schlafly, Edward F.; Morganson, Eric; Rix, Hans-Walter; Bernard, Edouard J.; Ferguson, Annette M. N.; Finkbeiner, Douglas P.; Burgett, William S.; Chambers, Kenneth C.; Hodapp, Klaus W.; Kaiser, Nicholas; Kudritzki, Rolf-Peter; Magnier, Eugene A.; Morgan, Jeffrey S.; Tonry, John L.; Wainscoat, Richard J.; Price, Paul A.

    2013-07-20

    We report the discovery of two new dwarf galaxies, Lacerta I/Andromeda XXXI (Lac I/And XXXI) and Cassiopeia III/Andromeda XXXII (Cas III/And XXXII), in stacked Pan-STARRS1 r{sub P1}- and i{sub P1}-band imaging data. Both are luminous systems (M{sub V} {approx} -12) located at projected distances of 20. Degree-Sign 3 and 10. Degree-Sign 5 from M31. Lac I and Cas III are likely satellites of the Andromeda galaxy with heliocentric distances of 756{sup +44}{sub -28} kpc and 772{sup +61}{sub -56} kpc, respectively, and corresponding M31-centric distances of 275 {+-} 7 kpc and 144{sup +6}{sub -4} kpc. The brightest of recent Local Group member discoveries, these two new dwarf galaxies owe their late discovery to their large sizes (r{sub h} = 4.2{sup +0.4}{sub -0.5} arcmin or 912{sup +124}{sub -93} pc for Lac I; r{sub h} = 6.5{sup +1.2}{sub -1.0} arcmin or 1456 {+-} 267 pc for Cas III) and consequently low surface brightness ({mu}{sub 0} {approx} 26.0 mag arcsec{sup -2}), as well as to the lack of a systematic survey of regions at large radii from M31, close to the Galactic plane. This latter limitation is now alleviated by the 3{pi} Pan-STARRS1 survey, which could lead to the discovery of other distant Andromeda satellite dwarf galaxies.

  12. The Evolution of Swift/BAT blazars and the origin of the MeV background

    SciTech Connect (OSTI)

    Ajello, M.; Costamante, L.; Sambruna, R.M.; Gehrels, N.; Chiang, J.; Rau, A.; Escala, A.; Greiner, J.; Tueller, J.; Wall, J.V.; Mushotzky, R.F.; /NASA, Goddard

    2009-10-17

    We use 3 years of data from the Swift/BAT survey to select a complete sample of X-ray blazars above 15 keV. This sample comprises 26 Flat-Spectrum Radio Quasars (FSRQs) and 12 BL Lac objects detected over a redshift range of 0.03 < z < 4.0. We use this sample to determine, for the first time in the 15-55 keV band, the evolution of blazars. We find that, contrary to the Seyfert-like AGNs detected by BAT, the population of blazars shows strong positive evolution. This evolution is comparable to the evolution of luminous optical QSOs and luminous X-ray selected AGNs. We also find evidence for an epoch-dependence of the evolution as determined previously for radio-quiet AGNs. We interpret both these findings as a strong link between accretion and jet activity. In our sample, the FSRQs evolve strongly, while our best-fit shows that BL Lacs might not evolve at all. The blazar population accounts for 10-20% (depending on the evolution of the BL Lacs) of the Cosmic X-ray background (CXB) in the 15-55 keV band. We find that FSRQs can explain the entire CXB emission for energies above 500 keV solving the mystery of the generation of the MeV background. The evolution of luminous FSRQs shows a peak in redshift (z{sub c} = 4.3 {+-} 0.5) which is larger than the one observed in QSOs and X-ray selected AGNs. We argue that FSRQs can be used as tracers of massive elliptical galaxies in the early Universe.

  13. BROAD Ly{alpha} EMISSION FROM THREE NEARBY BL LACERTAE OBJECTS

    SciTech Connect (OSTI)

    Stocke, John T.; Danforth, Charles W. [CASA, Department of Astrophysical and Planetary Sciences, University of Colorado, 389-UCB, Boulder, CO 80309 (United States); Perlman, Eric S., E-mail: danforth@casa.colorado.edu, E-mail: stocke@casa.colorado.edu, E-mail: eperlman@fit.edu [Florida Institute of Technology, Physics and Space Sciences Department, 150 West University Boulevard, Melbourne, FL 32901 (United States)

    2011-05-10

    We present far-UV HST/COS spectra of four nearby BL Lac objects. BL Lac spectra are dominated by a smooth, power-law continuum which arises in a relativistic jet. However, the spectra are not necessarily featureless; weak, broad- and/or narrow-line emission is sometimes seen in high-quality optical spectra. We present detections of Ly{alpha} emission in HST/COS spectra of Mrk 421 (z = 0.030) and PKS 2005-489 (z = 0.071) as well as an archival HST/GHRS observation of Mrk 501 (z = 0.0337). Archival HST/STIS observations of PKS 2155-304 (z = 0.116) show no Ly{alpha} emission to a very low upper limit. Using the assumption that the broad-line region (BLR) clouds are symmetrically placed around the active galactic nucleus (AGN), we use these measured Ly{alpha} emission features to constrain either the relativistic {Gamma} values for the ionizing continuum produced by the jet (in the ionization-bounded case) or the mass of warm gas (in the density-bounded case). While realistic {Gamma} values can be obtained for all four cases, the values for Mrk 421 and PKS 2155-304 are high enough to suggest that covering factors of BLR clouds of {approx}1%-2% might be required to provide consistency with earlier values of Doppler boosting and viewing angles suggested for this class of BL Lacs. This discrepancy also exists in the case of M 87, where the amount of Doppler boosting in our direction is expected to be minimal, again suggestive of a small covering factor of BLR clouds. If, as these small covering factors might suggest, the assumptions of a density-bounded model could be more correct, then the observed Ly{alpha} luminosities require that BL Lac/FR 1 nuclei possess very little warm gas (10{sup -4} to 10{sup -5} M{sub sun}) as suggested by Guilbert et al. If these clouds are in pressure balance with a hotter ({approx}10{sup 6} K) gas, the BLR contains too little mass to power the AGN by accretion alone.

  14. mlw8264.tmp

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    ,,...... sLAc-PuB--5l93 DE90 OO81OO THE E(2S4 CODE SYSTEM: SOLUTION OF GAMMA-RAY AND ELECTRON TRANSPORT PROBLEMS* W. R. NELSON AND YOSHIHITO NAMITO~ Stanford Linear Accelerator Center Stanford University, Stanford, California 94305 Abstract In this paperwe present an overview of the EGS4 Code System-a general purpose package forthe Monte (larlosimulatio no fthetransport of electrons and photons. During the last 10-15 years EGS has been widely used todesignaccelera- tors and detectors for

  15. Multinational societies and syndicates

    ScienceCinema (OSTI)

    None

    2011-04-25

    Monsieur Charles Levinson, par la longue expérience qu'il a acquise au contact des sociétés multinationales et syndicats, nous en parle ce soir

  16. Iowa Community College Campuses Reduce Energy Use

    Broader source: Energy.gov [DOE]

    Des Moines Area Community College (DMACC) serves more than 65,000 Iowans on six campuses, making it the largest two-year college in the state of Iowa.

  17. DG's Meeting

    ScienceCinema (OSTI)

    None

    2011-04-25

    Exposés du DG H.Schopper, Blackburne et du président du comité des finances concernant le budget, salaires, pensions etc...avec discussion et questions

  18. Meditation and Reality

    ScienceCinema (OSTI)

    None

    2011-04-25

    A.Sujata demande dans son exposé entre autre à ceux/celles des auditeurs/trices qui sont heureux/ses, de lever la main.....qu'est le bonheur?

  19. Churches and Apartheid

    ScienceCinema (OSTI)

    None

    2011-04-25

    Lucas Vischer fait parti du concile mondial des églises et nous parle d'eglises et d'apartheid en Afrique du Sud et se pose la question d'un changement sans violence.....

  20. Science and Society-Consequences of engineering

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le conférencier Mons.Rorsch parle des possibles conséquences économiques et culturelles de la technologie en générale, aussi pour l'environnement

  1. Eyes Witness Report on South Vietnam

    ScienceCinema (OSTI)

    None

    2011-04-25

    Mons. Nielson, conseiller des Etats Unis auprès de L'ONU, apporte son témoignage et exprime son opinion quand à la guerre du Vietnam (Sud)

  2. Category:SmallHotel | Open Energy Information

    Open Energy Info (EERE)

    Cleveland OH Ohio Power Co.png SVSmallHotel Cleveland... 68 KB SVSmallHotel Concord NH Public Service Co of NH.png SVSmallHotel Concord N... 71 KB SVSmallHotel Des Moines IA...

  3. Renewable Energy Research | Open Energy Information

    Open Energy Info (EERE)

    Research Jump to: navigation, search Name: Renewable Energy Research Address: 2113 C Boulevard St Regis Place: Dollard des Ormeaux Zip: H9B 2M9 Region: Canada Sector: Marine and...

  4. Senior Staff Meeting

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le DG C.Rubbia informe sur les négociations avec le personnel, les discussions avec le conseil d'administration et le budget, suivi des questions

  5. Electricity Advisory Committee Meeting Presentations June 2014...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Tuesday, June 17, 2014 Panel - Distributed Energy Storage (DES) - Wanda Reder, S&C, moderator Willem Fadrhonc, STEM Tom Weaver, AEP Melicia Charles, CPUC Tom Bialek, SDG&E Panel - ...

  6. Obama Administration Announces More Than $16 Million for Energy...

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    16 Million for Energy Projects in Iowa Obama Administration Announces More Than 16 Million for Energy Projects in Iowa June 22, 2009 - 12:00am Addthis Des Moines, IA - U.S. ...

  7. CX-003877: Categorical Exclusion Determination

    Office of Energy Efficiency and Renewable Energy (EERE)

    Hybrid Membrane/Absorption Process for Post-Combustion Carbon Dioxide CaptureCX(s) Applied: B3.6Date: 09/10/2010Location(s): Des Plaines, IllinoisOffice(s): Fossil Energy, National Energy Technology Laboratory

  8. Inauguration SC

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le DG W.Jentschke ouvre l'inauguration du Syncro Cyclotron (8') et remercie Mons. Michaelis qui prend la parole (30') avant Mons. Wilkinson (53') qui parle du futur de la machine avec présentation des dias.

  9. CX-004386: Categorical Exclusion Determination

    Office of Energy Efficiency and Renewable Energy (EERE)

    Chicago Area Alternative Fuels Deployment ProjectCX(s) Applied: B5.1Date: 11/04/2010Location(s): Des Plaines, IllinoisOffice(s): Energy Efficiency and Renewable Energy, National Energy Technology Laboratory

  10. HyRadix Inc | Open Energy Information

    Open Energy Info (EERE)

    search Name: HyRadix Inc Place: Des Plaines,, Illinois Zip: IL 60018-1 Sector: Hydro, Hydrogen Product: The company aims to develop and supply small-scale hydrogen generation...

  11. Information Meeting- Education

    ScienceCinema (OSTI)

    None

    2011-04-25

    Suite à un circulaire, Messieurs Goldschmidt et Ullmann donnent plus d'information et attendent des questions/réponses concernant les problèmes d'éducation d'enfants

  12. Mutual Insurance Company of West

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    call 800-247-4184 or visit ARAGLegalCenter.com. Limitations and exclusions apply. Insurance products are underwritten by ARAG Insurance Company of Des Moines, Iowa, GuideOne ...

  13. Colloquy Niels Bohr

    ScienceCinema (OSTI)

    None

    2011-04-25

    Célébration du 100me anniversaire de Niels Bohr (1885 - 1962), un des fondateurs de la physique moderne. Plusieurs orateurs parlent de cet homme et le développement de la physique

  14. CX-000339: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Chicago Area Alternative Fuel Deployment ProjectCX(s) Applied: A1, A9Date: 12/10/2009Location(s): Des Plaines, IllinoisOffice(s): Energy Efficiency and Renewable Energy, National Energy Technology Laboratory

  15. CX-004285: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Indigo Dawn Green and Main Street ProjectCX(s) Applied: A9, B5.1Date: 10/20/2010Location(s): Des Moines, IowaOffice(s): Energy Efficiency and Renewable Energy, Golden Field Office

  16. West Burlington, Iowa: Energy Resources | Open Energy Information

    Open Energy Info (EERE)

    Hide Map This article is a stub. You can help OpenEI by expanding it. West Burlington is a city in Des Moines County, Iowa. It falls under Iowa's 2nd...

  17. Fermilab Today

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    with the Dark Energy Survey The constraints we deduce from DES SV lensing data (in purple) on the amount of matter in the universe, m, and the amplitude of fluctuations in...

  18. Fragment Screen against HIV Protease: Discovery of Two Allosteric...

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Screen against HIV Protease. Chem. Biol. Drug Des. 75: 257-268. References Brenner, B., Routy, J-P., Quan, Y., Moisi, D., Oliveira, M., Turner, D., Wainberg, M. A. &...

  19. Expo NL inauguration

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le DG H.Schopper souhaite la bienvenue à toutes les personnes présentes. Plusieurs discours à l'occasion de l'inauguration officielle de l'expo des Pays-Bas.

  20. Fermilab Today

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Russia. Read more Frontier Science Result: DES The Dark Energy Survey looks at massive galaxy clusters - and finds filaments With data from the new DECam imager, the Dark Energy...

  1. Churches and Apartheid

    SciTech Connect (OSTI)

    2006-01-16

    Lucas Vischer fait parti du concile mondial des glises et nous parle d'eglises et d'apartheid en Afrique du Sud et se pose la question d'un changement sans violence.....

  2. Gestational exposure to diethylstilbestrol alters cardiac structure/function, protein expression and DNA methylation in adult male mice progeny

    SciTech Connect (OSTI)

    Haddad, Rami, E-mail: rami.haddad@mail.mcgill.ca [Lady Davis Institute for Medical Research, Jewish General Hospital, 3755 chemin Cote Ste Catherine, Montral, Qubec, Canada H3T 1E2 (Canada) [Lady Davis Institute for Medical Research, Jewish General Hospital, 3755 chemin Cote Ste Catherine, Montral, Qubec, Canada H3T 1E2 (Canada); Division of Experimental Medicine, Department of Medicine, McGill University, 850 Sherbrooke Street, Montral, Qubec, Canada H3A 1A2 (Canada); Kasneci, Amanda, E-mail: amanda.kasneci@mail.mcgill.ca [Lady Davis Institute for Medical Research, Jewish General Hospital, 3755 chemin Cote Ste Catherine, Montral, Qubec, Canada H3T 1E2 (Canada)] [Lady Davis Institute for Medical Research, Jewish General Hospital, 3755 chemin Cote Ste Catherine, Montral, Qubec, Canada H3T 1E2 (Canada); Mepham, Kathryn, E-mail: katherine.mepham@mail.mcgill.ca [Lady Davis Institute for Medical Research, Jewish General Hospital, 3755 chemin Cote Ste Catherine, Montral, Qubec, Canada H3T 1E2 (Canada) [Lady Davis Institute for Medical Research, Jewish General Hospital, 3755 chemin Cote Ste Catherine, Montral, Qubec, Canada H3T 1E2 (Canada); Division of Experimental Medicine, Department of Medicine, McGill University, 850 Sherbrooke Street, Montral, Qubec, Canada H3A 1A2 (Canada); Sebag, Igal A., E-mail: igal.sebag@mcgill.ca [Division of Cardiology, Jewish General Hospital, 3755 chemin Cote Ste Catherine, Montral, Qubec, Canada H3T 1E2 (Canada); and others

    2013-01-01

    Pregnant women, and thus their fetuses, are exposed to many endocrine disruptor compounds (EDCs). Fetal cardiomyocytes express sex hormone receptors making them potentially susceptible to re-programming by estrogenizing EDCs. Diethylstilbestrol (DES) is a proto-typical, non-steroidal estrogen. We hypothesized that changes in adult cardiac structure/function after gestational exposure to the test compound DES would be a proof in principle for the possibility of estrogenizing environmental EDCs to also alter the fetal heart. Vehicle (peanut oil) or DES (0.1, 1.0 and 10.0 ?g/kg/da.) was orally delivered to pregnant C57bl/6n dams on gestation days 11.514.5. At 3 months, male progeny were left sedentary or were swim trained for 4 weeks. Echocardiography of isoflurane anesthetized mice revealed similar cardiac structure/function in all sedentary mice, but evidence of systolic dysfunction and increased diastolic relaxation after swim training at higher DES doses. The calcium homeostasis proteins, SERCA2a, phospholamban, phospho-serine 16 phospholamban and calsequestrin 2, are important for cardiac contraction and relaxation. Immunoblot analyses of ventricle homogenates showed increased expression of SERCA2a and calsequestrin 2 in DES mice and greater molecular remodeling of these proteins and phospho-serine 16 phospholamban in swim trained DES mice. DES increased cardiac DNA methyltransferase 3a expression and DNA methylation in the CpG island within the calsequestrin 2 promoter in heart. Thus, gestational DES epigenetically altered ventricular DNA, altered cardiac function and expression, and reduced the ability of adult progeny to cardiac remodel when physically challenged. We conclude that gestational exposure to estrogenizing EDCs may impact cardiac structure/function in adult males. -- Highlights: ? Gestational DES changes cardiac SERCA2a and CASQ2 expression. ? Echocardiography identified systolic dysfunction and increased diastolic relaxation. ? DES increased DNMT3a expression and increased CpG DNA methylation. ? DES impacts fetal heart reducing cardiac reserve on challenge in adulthood. ? Fetal heart can be re-programmed by a non-steroidal estrogen.

  3. Senior Staff Meeting

    ScienceCinema (OSTI)

    None

    2011-04-25

    Herbert Lengler fait l'introduction et remercie le DG, les directeurs et le vice président de l'association du personnel pour leur présence. Il parlera des activités depuis la dernière réunion et fera des commentaires sur l'"Abragam Commitee Final Report". Une discussion suivra sur plusieurs points importants.

  4. Discovery of two gravitationally lensed quasars in the Dark Energy Survey

    SciTech Connect (OSTI)

    Agnello, A.

    2015-10-01

    In this study, we present spectroscopic confirmation of two new lensed quasars via data obtained at the 6.5m Magellan/Baade Telescope. The lens candidates have been selected from the Dark Energy Survey (DES) and WISE based on their multi-band photometry and extended morphology in DES images. Images of DES J0115-5244 show two blue point sources at either side of a red galaxy. Our long-slit data confirm that both point sources are images of the same quasar at zs = 1.64. The Einstein Radius estimated from the DES images is 0.51''. DES J2146-0047 is in the area of overlap between DES and the Sloan Digital Sky Survey (SDSS). Two blue components are visible in the DES and SDSS images. The SDSS fiber spectrum shows a quasar component at zs = 2.38 and absorption compatible with Mg II and Fe II at zl = 0.799, which we tentatively associate with the foreground lens galaxy. The long-slit Magellan spectra show that the blue components are resolved images of the same quasar. Furthermore, the Einstein Radius is 0.68'' corresponding to an enclosed mass of 1.6 1011 M?. Three other candidates were observed and rejected, two being low-redshift pairs of starburst galaxies, and one being a quasar behind a blue star. These first confirmation results provide an important empirical validation of the data-mining and model-based selection that is being applied to the entire DES dataset.

  5. Discovery of two gravitationally lensed quasars in the Dark Energy Survey

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Agnello, A.

    2015-10-01

    In this study, we present spectroscopic confirmation of two new lensed quasars via data obtained at the 6.5m Magellan/Baade Telescope. The lens candidates have been selected from the Dark Energy Survey (DES) and WISE based on their multi-band photometry and extended morphology in DES images. Images of DES J0115-5244 show two blue point sources at either side of a red galaxy. Our long-slit data confirm that both point sources are images of the same quasar at zs = 1.64. The Einstein Radius estimated from the DES images is 0.51''. DES J2146-0047 is in the area of overlap between DES andmore » the Sloan Digital Sky Survey (SDSS). Two blue components are visible in the DES and SDSS images. The SDSS fiber spectrum shows a quasar component at zs = 2.38 and absorption compatible with Mg II and Fe II at zl = 0.799, which we tentatively associate with the foreground lens galaxy. The long-slit Magellan spectra show that the blue components are resolved images of the same quasar. Furthermore, the Einstein Radius is 0.68'' corresponding to an enclosed mass of 1.6 × 1011 M⊙. Three other candidates were observed and rejected, two being low-redshift pairs of starburst galaxies, and one being a quasar behind a blue star. These first confirmation results provide an important empirical validation of the data-mining and model-based selection that is being applied to the entire DES dataset.« less

  6. Personnel

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le président du conseil M.Doran explique la décision que le conseil du Cern vient de prendre sur la 4.étape du régime complémentaire des pensions. Le président du comité des finances le Dr.Andersen ainsi que le Prof.Connor(?) prennent aussi la parole

  7. Investigation of excess thyroid cancer incidence in Los Alamos County

    SciTech Connect (OSTI)

    Athas, W.F.

    1996-04-01

    Los Alamos County (LAC) is home to the Los Alamos National Laboratory, a U.S. Department of Energy (DOE) nuclear research and design facility. In 1991, the DOE funded the New Mexico Department of Health to conduct a review of cancer incidence rates in LAC in response to citizen concerns over what was perceived as a large excess of brain tumors and a possible relationship to radiological contaminants from the Laboratory. The study found no unusual or alarming pattern in the incidence of brain cancer, however, a fourfold excess of thyroid cancer was observed during the late-1980`s. A rapid review of the medical records for cases diagnosed between 1986 and 1990 failed to demonstrate that the thyroid cancer excess had resulted from enhanced detection. Surveillance activities subsequently undertaken to monitor the trend revealed that the excess persisted into 1993. A feasibility assessment of further studies was made, and ultimately, an investigation was conducted to document the epidemiologic characteristics of the excess in detail and to explore possible causes through a case-series records review. Findings from the investigation are the subject of this report.

  8. Structure and Biochemestry of Laccases from the Lignin-Degrading Basidiomycete, Ganoderma lucidum

    SciTech Connect (OSTI)

    C.A.Reddy, PI

    2005-06-30

    G. lucidum is one of the most important and widely distributed ligninolytic white rot fungi from habitats such as forest soils, agricultural soils, and tropical mangrove ecosystems and produce laccases as an important family of lignin modifying enzymes. Biochemically, laccases are blue multi copper oxidases that couple four electron reduction of molecular oxygen to water. There is a growing interest in the use of laccases for a variety of industrial applications such as bio-pulping and biobleaching as well as in their ability to detoxify a wide variety of toxic environmental pollutants. These key oxidative enzymes are found in all the three domains of life: Eukaryota. Prokarya, and Archaea. Ganoderma lucidum (strain no.103561) produces laccase with some of the highest activity (17,000 micro katals per mg of protein) reported for any laccases to date. Our results showed that this organism produces at least 11 different isoforms of laccase based on variation in mol. weight and/or PI. Our Studies showed that the presence of copper in the medium yields 15- to 20-fold greater levels of enzyme by G. lucidum. Dialysation of extra cellular fluid of G. lucidum against 10mM sodium tartrate (pH5.5) gave an additional 15 to 17 fold stimulation of activity with an observed specific activity of 17,000 {micro}katals/mg protein. Dialysis against acetate buffer gave five fold increase in activity while dialysis against glycine showed inhibition of activity. Purification by FPLC and preparative gel electrophoresis gave purified fractions that resolved into eleven isoforms as separated by isoelectric focusing, and the PI,s were 4.7, 4.6, 4.5, 4.3, 4.2, 4.1, 3.8, 3.7, 3.5, 3.4 and 3.3. Genomic clones of laccase were isolated using G. lucidum DNA as a template and using inverse PCR and forward/reverse primers corresponding to the sequences of the conserved copper binding region in the N-terminal domain of one of the laccases of this organism. Inverse PCR amplication of HindIII digested and ligated G.lucidum DNA was done using ABI Geneamp XL PCR kit in Ribocycler. The 5 conserved copper binding region of laccase was used for designing forward primer (5TCGACAATTCTTTCCTGTACG3) and reverse primer (5 TGGAGATGGG ACACT GGCTTATC 3). The PCR profile was 95 C for 3min, 94 C for 1min, 57 C for 30 sec and 68 C for 5min. for 30 cycles, and the final extension was at 72 C for 10min. The resulting {approx}2.7 Kb inverse PCR fragment was cloned into ZERO TOPOII blunt ligation vector (INVITROGEN) and screened on Kanamycin plates. Selected putative clones containing inserts were digested with a battery of restriction enzymes and analyzed on 1% agarose gels. Restriction digestion of these clones with BamHI, PstI, SalI, PvuII, EcoRI, and XhoI revealed 8 distinct patterns suggesting gene diversity. Two clones were sequenced using overlapping primers on ABI system. The sequences were aligned using Bioedit program. The aa sequences of the clones were deduced by Genewise2 program using Aspergillus as the reference organism. Eukaryotic gene regulatory sequences were identified using GeneWise2 Program. Laccase sequence alignments and similarity indexes were calculated using ClustalW and BioEdit programs. Blast analysis of two distinct BamHI clones, lac1 and lac4, showed that the proteins encoded by these clones are fungal laccase sequences. The coding sequence of lac1gene is interrupted by 6 introns ranging in size from 37-55 nt and encodes a mature protein consisting of 456 aa (Mr: 50,160), preceded by a putative 37-aa signal sequence. This predicted Mr is in agreement with the range of Mrs previously reported by us for the laccases of G. lucidum. The deduced aa sequence of LAC1 showed relatively high degree of homology with laccases of other basidiomycetes. It showed 96% homology to full-length LAC4 protein and 47-53% similarity to unpublished partial laccase sequences of other G. lucidum strains. Among the other basidiomycete laccases, LAC1 showed the highest similarity of 53-55% to Trametes versicolorLAC3 and LAC4. The consensus copper-binding domains found in ot

  9. Simultaneous Observations of PKS 2155--304 with H.E.S.S., Fermi, RXTE and ATOM: Spectral Energy Distributions and Variability in a Low State

    SciTech Connect (OSTI)

    Aharonian, F.; Akhperjanian, A.G.; Anton, G.; Barres de Almeida, U.; Bazer-Bachi, A.R.; Becherini, Y.; Behera, B.; Bernlohr, K.; Boisson, C.; Bochow, A.; Borrel, V.; Brion, E.; Brucker, J.; Brun, P.; Buhler, R.; Bulik, T.; Busching, I.; Boutelier, T.; Chadwick, P.M.; Charbonnier, A.; Chaves, R.C.G.; /more authors..

    2009-05-07

    We report on the first simultaneous observations that cover the optical, X-ray, and high-energy gamma-ray bands of the BL Lac object PKS 2155-304. The gamma-ray bands were observed for 11 days, between 2008 August 25 and 2008 September 6 (MJD 54704-54715), jointly with the Fermi Gamma-ray Space Telescope and the HESS atmospheric Cherenkov array, providing the first simultaneous MeV-TeV spectral energy distribution (SED) with the new generation of {gamma}-ray telescopes. The ATOM telescope and the RXTE and Swift observatories provided optical and X-ray coverage of the low-energy component over the same time period. The object was close to the lowest archival X-ray and very high energy (VHE; >100 GeV) state, whereas the optical flux was much higher. The light curves show relatively little ({approx}30%) variability overall when compared to past flaring episodes, but we find a clear optical/VHE correlation and evidence for a correlation of the X-rays with the high-energy spectral index. Contrary to previous observations in the flaring state, we do not find any correlation between the X-ray and VHE components. Although synchrotron self-Compton models are often invoked to explain the SEDs of BL Lac objects, the most common versions of these models are at odds with the correlated variability we find in the various bands for PKS 2155-304.

  10. Long term observations of B2 1215+30 with veritas

    SciTech Connect (OSTI)

    Aliu, E.; Errando, M.; Archambault, S.; Arlen, T.; Aune, T.; Beilicke, M.; Buckley, J. H.; Bugaev, V.; Benbow, W.; Bird, R.; Bouvier, A.; Cesarini, A.; Connolly, M. P.; Ciupik, L.; Cui, W.; Feng, Q.; Finley, J. P.; Dumm, J.; Falcone, A.; Federici, S.; Collaboration: VERITAS collaboration; and others

    2013-12-20

    We report on VERITAS observations of the BL Lac object B2 1215+30 between 2008 and 2012. During this period, the source was detected at very high energies (VHEs; E > 100 GeV) by VERITAS with a significance of 8.9? and showed clear variability on timescales larger than months. In 2011, the source was found to be in a relatively bright state and a power-law fit to the differential photon spectrum yields a spectral index of 3.6 0.4{sub stat} 0.3{sub syst} with an integral flux above 200 GeV of (8.0 0.9{sub stat} 3.2{sub syst}) 10{sup 12} cm{sup 2} s{sup 1}. No short term variability could be detected during the bright state in 2011. Multi-wavelength data were obtained contemporaneously with the VERITAS observations in 2011 and cover optical (Super-LOTIS, MDM, Swift/UVOT), X-ray (Swift/XRT), and gamma-ray (Fermi-LAT) frequencies. These were used to construct the spectral energy distribution (SED) of B2 1215+30. A one-zone leptonic model is used to model the blazar emission and the results are compared to those of MAGIC from early 2011 and other VERITAS-detected blazars. The SED can be reproduced well with model parameters typical for VHE-detected BL Lac objects.

  11. JET PROPERTIES OF GeV-SELECTED RADIO-LOUD NARROW-LINE SEYFERT 1 GALAXIES AND POSSIBLE CONNECTION TO THEIR DISK AND CORONA

    SciTech Connect (OSTI)

    Sun, Xiao-Na; Lin, Da-Bin; Liang, En-Wei; Zhang, Jin; Xue, Zi-Wei; Zhang, Shuang-Nan

    2015-01-01

    The observed spectral energy distributions of five GeV-selected narrow-line Seyfert 1 (NLS1) galaxies are fitted with a model including the radiation ingredients from the relativistic jet, the accretion disk, and the corona. We compare the properties of these GeV NLS1 galaxies with flat spectrum radio quasars (FSRQs), BL Lacertae objects (BL Lacs), and radio-quiet (RQ) Seyfert galaxies, and explore possible hints for jet-disk/corona connection. Our results show that the radiation physics and the jet properties of the GeV NLS1 galaxies resemble that of FSRQs. The luminosity variations of PMN J0948+0022 and 1H 0323+342 at the GeV band is tightly correlated with the beaming factor (?), similar to that observed in FSRQ 3C 279. The accretion disk luminosities and the jet powers of the GeV NLS1 galaxies cover both the ranges of FSRQs and BL Lacs. With the detection of bright corona emission in 1H 0323+342, we show that the ratio of the corona luminosity (L {sub corona}) to the accretion disk luminosity (L {sub d}) is marginally within the high end of this ratio distribution for an RQ Seyfert galaxy sample, and the variation of jet luminosity may connect with L {sub corona}. However, it is still unclear whether a system with a high L {sub corona}/L {sub d} ratio prefers to power a jet.

  12. LAr calorimeter for SCC with a common vacuum bulkhead---a concept to improve hermeticity

    SciTech Connect (OSTI)

    Pope, W.L. ); Watt, R.D. )

    1989-11-01

    A new concept for a Barrel/Endcap LAr Calorimeter (LAC) is described in which the Barrel and Endcaps are in separate vacuum enclosures but share a common vacuum bulkhead (CVB). We explore 2 possible bulkhead construction types; welded plate sandwich panels, and brazed sandwich panels in which the core is an isotropic cellular solid--foamed aluminum. Gas lines and electric cables from he innermost Drift Chamber pass through radial holes in the core of the sandwich bulkhead. The CVB concept offers the potential to obtain a more hermetic calorimeter with significantly reduced dead material and/or space in the interface region common to conventional design LAr detectors for the SSC with Endcap features. To utilize a common additional steps to remove the Drift Chamber, a large increase in Endcap standby heat leak, and perhaps, new cryogenic safety issues. We find that significant amount of dead mass can be removed from critical regions of the vacuum shells when compared to a promising SSC LAC reference design. It is also shown that the increased standby heat leak of this concept can be easily removed by existing cooling capacity in another large LAr calorimeter. It is further shown that shut-downs need not be appreciably longer. Finally, it is argued that cryogen spill hazards can be avoided if the Endcap's LAr is removed during Drift chamber maintenance shutdowns, and that cryogenic safety is not compromised.

  13. Structural and functional characterization of human and murine C5a anaphylatoxins

    SciTech Connect (OSTI)

    Schatz-Jakobsen, Janus Asbjrn; Yatime, Laure Larsen, Casper; Petersen, Steen Vang; Klos, Andreas; Andersen, Gregers Rom

    2014-06-01

    The structure of the human C5aR antagonist, C5a-A8, reveals a three-helix bundle conformation similar to that observed for human C5a-desArg, whereas murine C5a and C5a-desArg both form the canonical four-helix bundle. These conformational differences are discussed in light of the differential C5aR activation properties observed for the human and murine complement anaphylatoxins across species. Complement is an ancient part of the innate immune system that plays a pivotal role in protection against invading pathogens and helps to clear apoptotic and necrotic cells. Upon complement activation, a cascade of proteolytic events generates the complement effectors, including the anaphylatoxins C3a and C5a. Signalling through their cognate G-protein coupled receptors, C3aR and C5aR, leads to a wide range of biological events promoting inflammation at the site of complement activation. The function of anaphylatoxins is regulated by circulating carboxypeptidases that remove their C-terminal arginine residue, yielding C3a-desArg and C5a-desArg. Whereas human C3a and C3a-desArg adopt a canonical four-helix bundle fold, the conformation of human C5a-desArg has recently been described as a three-helix bundle. Here, the crystal structures of an antagonist version of human C5a, A8{sup ?7173}, and of murine C5a and C5a-desArg are reported. Whereas A8{sup ?7173} adopts a three-helix bundle conformation similar to human C5a-desArg, the two murine proteins form a four-helix bundle. A cell-based functional assay reveals that murine C5a-desArg, in contrast to its human counterpart, exerts the same level of activition as murine C5a on its cognate receptor. The role of the different C5a conformations is discussed in relation to the differential activation of C5a receptors across species.

  14. DESAlert: Enabling real-time transient follow-up with Dark Energy Survey data

    SciTech Connect (OSTI)

    Poci, A.

    2015-04-12

    The Dark Energy Survey (DES) is currently undertaking an observational program imaging 1/4 of the southern hemisphere sky with unprecedented photometric accuracy. In the process of observing millions of faint stars and galaxies to constrain the parameters of the dark energy equation of state, the DES will obtain pre-discovery images of the regions surrounding an estimated 100 gamma-ray bursts (GRBs) over five years. Once GRBs are detected by, e.g., the Swift satellite, the DES data will be extremely useful for follow-up observations by the transient astronomy community. We describe a recently-commissioned suite of software that listens continuously for automated notices of GRB activity, collates useful information from archival DES data, and promulgates relevant data products back to the community in near-real-time. Of particular importance are the opportunities that DES data provide for relative photometry of GRBs or their afterglows, as well as for identifying key characteristics (e.g., photometric redshifts) of potential GRB host galaxies. We provide the functional details of the DESAlert software as it presently operates, as well as the data products that it produces, and we show sample results from the application of DESAlert to several previously-detected GRBs.

  15. Conference B.Bettelheim

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le Dr.Bruno Bettelheim, psychologue américain, d'origine viennoise, a passé son doctorat en psychologie à l'université de Vienne. Il émigra aux Etats-Unis et enseigna la psychologie au Rockford College en Illinois et la psychologie de l'éducation à L'université de Chicago, où il dirigea également l'institut orthogénique Sonia-Shankman pour le traitement des enfants psychotiques. Cet homme a bouleversé la compréhension des relations parents et enfants en y introduisant la psychanalyse. Basé sur ses expériences aux Etats-Unis,il nous parle des changements dans la structure de la famille et ses conséquences pour la relation entre enfants et parents.

  16. Voyage dans le noir. Trous noirs, matière noire, énergie noire et antimatière

    ScienceCinema (OSTI)

    None

    2011-10-06

    Et si nous faisions avec les physiciens un voyage dans le noir ? De l'astrophysique à la physique des particules les trois noirs, la matière noire, l'énergie noire ou l?antimatière intriguent et fascinent. Que sont ces objets qui bousculent nos idées et qui véhiculent parfois des craintes irraisonnées? Luis Alvarez-Gaume, Michael Doser et Christophe Grojean, physiciens du CERN vous invitent à mettre en lumière (!) les constituants de base de la matière et à explorer les mystères de la physique contemporaine. Une soirée lumineuse pour éclairer des concepts et ne plus avoir peur du noir.

  17. Air-gap gating of MgZnO/ZnO heterostructures

    SciTech Connect (OSTI)

    Tambo, T.; Falson, J. Kozuka, Y.; Maryenko, D.; Tsukazaki, A.; Kawasaki, M.

    2014-08-28

    The adaptation of air-gap dielectric based field-effect transistor technology to controlling the MgZnO/ZnO heterointerface confined two-dimensional electron system (2DES) is reported. We find it possible to tune the charge density of the 2DES via a gate electrode spatially separated from the heterostructure surface by a distance of 5??m. Under static gating, the observation of the quantum Hall effect suggests that the charge carrier density remains homogeneous, with the 2DES in the 3?mm square sample the sole conductor. The availability of this technology enables the exploration of the charge carrier density degree of freedom in the pristine sample limit.

  18. Eight ultra-faint galaxy candidates discovered in year two of the Dark Energy Survey

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Drlica-Wagner, A.

    2015-11-04

    We report the discovery of eight new ultra-faint dwarf galaxy candidates in the second year of optical imaging data from the Dark Energy Survey (DES). Six of these candidates are detected at high confidence, while two lower-confidence candidates are identified in regions of non-uniform survey coverage. The new stellar systems are found by three independent automated search techniques and are identified as overdensities of stars, consistent with the isochrone and luminosity function of an old and metal-poor simple stellar population. The new systems are faint (MV > -4.7 ) and span a range of physical sizes (17 pc < r1/2more » < 181pc) and heliocentric distances (25 kpc < D⊙ < 214 kpc). All of the new systems have central surface brightnesses consistent with known ultra-faint dwarf galaxies (μ 27.5 mag arcsec -2). Roughly half of the DES candidates are more distant, less luminous, and/or have lower surface brightnesses than previously known Milky Way satellite galaxies. Most of the candidates are found in the southern part of the DES footprint close to the Magellanic Clouds. We find that the DES data alone exclude (p < 10-3) a spatially isotropic distribution of Milky Way satellites and that the observed distribution can be well, though not uniquely, described by an association between several of the DES satellites and the Magellanic system. Furthermore, our model predicts that the full sky may hold ~100 ultra-faint galaxies with physical properties comparable to the DES satellites and that 20%–30% of these would be spatially associated with the Magellanic Clouds.« less

  19. Eight ultra-faint galaxy candidates discovered in year two of the Dark Energy Survey

    SciTech Connect (OSTI)

    Drlica-Wagner, A.

    2015-11-04

    We report the discovery of eight new ultra-faint dwarf galaxy candidates in the second year of optical imaging data from the Dark Energy Survey (DES). Six of these candidates are detected at high confidence, while two lower-confidence candidates are identified in regions of non-uniform survey coverage. The new stellar systems are found by three independent automated search techniques and are identified as overdensities of stars, consistent with the isochrone and luminosity function of an old and metal-poor simple stellar population. The new systems are faint (MV > -4.7 ) and span a range of physical sizes (17 pc < r1/2 < 181pc) and heliocentric distances (25 kpc < D? < 214 kpc). All of the new systems have central surface brightnesses consistent with known ultra-faint dwarf galaxies (? 27.5 mag arcsec -2). Roughly half of the DES candidates are more distant, less luminous, and/or have lower surface brightnesses than previously known Milky Way satellite galaxies. Most of the candidates are found in the southern part of the DES footprint close to the Magellanic Clouds. We find that the DES data alone exclude (p < 10-3) a spatially isotropic distribution of Milky Way satellites and that the observed distribution can be well, though not uniquely, described by an association between several of the DES satellites and the Magellanic system. Furthermore, our model predicts that the full sky may hold ~100 ultra-faint galaxies with physical properties comparable to the DES satellites and that 20%30% of these would be spatially associated with the Magellanic Clouds.

  20. EVIDENCE FOR THE DISKY ORIGIN OF LUMINOUS VIRGO DWARF ELLIPTICALS FROM THE KINEMATICS OF THEIR GLOBULAR CLUSTER SYSTEMS

    SciTech Connect (OSTI)

    Beasley, Michael A.; Cenarro, A. Javier; Brodie, Jean P. E-mail: cenarro@iac.es E-mail: brodie@ucolick.org

    2009-06-15

    We report evidence for dynamically significant rotation in the globular cluster systems of two luminous Virgo dwarf ellipticals, VCC1261 and VCC1528. Including previous results for VCC1087, the globular cluster systems of all three Virgo dwarf ellipticals studied in detail to date exhibit v {sub rot}/{sigma}{sub los}>1. Taking the rotation seen in the globular clusters as a maximal disk rotation, and accounting for the possible fading of any hypothetical progenitor galaxy, we find all three dwarf elliptical galaxies (dEs) lie on the r-band Tully-Fisher relation. We argue that these data support the hypothesis that luminous dEs are the remnants of transformed disk galaxies. We also obtained deep, longslit data for the stars in VCC1261 and VCC1528. Both these galaxies show rapid rotation in their inner regions, with spatial scales of {approx}0.5 kpc. These rotation velocities are surprisingly similar to those seen in the globular cluster systems. At larger radii, we see little rotation in the dEs themselves. Since our longslit data for Virgo dEs extend out to 1-2 effective radii (typical of deep observations), whereas the globular clusters extend out to 4-7 effective radii, we conclude that nondetections of rotation in many luminous dEs may simply be due to a lack of radial coverage in the stellar data, and that globular clusters represent singularly sensitive probes of the dynamics of dEs. Based on these data, we suggest that gas disks are significant sites of globular cluster formation in the early universe.

  1. THE DARK ENERGY SURVEY: PROSPECTS FOR RESOLVED STELLAR POPULATIONS

    SciTech Connect (OSTI)

    Rossetto, Bruno M.; Santiago, Baslio X.; Girardi, Lo; Camargo, Julio I. B.; Balbinot, Eduardo; da Costa, Luiz N.; Yanny, Brian; Maia, Marcio A. G.; Makler, Martin; Ogando, Ricardo L. C.; Pellegrini, Paulo S.; Ramos, Beatriz; de Simoni, Fernando; Armstrong, R.; Bertin, E.; Desai, S.; Kuropatkin, N.; Lin, H.; Mohr, J. J.; Tucker, D. L.

    2011-06-01

    Wide angle and deep surveys, regardless of their primary purpose, always sample a large number of stars in the Galaxy and in its satellite system. We here make a forecast of the expected stellar sample resulting from the Dark Energy Survey and the perspectives that it will open for studies of Galactic structure and resolved stellar populations in general. An estimated 1.2 x 108 stars will be sampled in DES grizY filters in the southern equatorial hemisphere. This roughly corresponds to 20% of all DES sources. Most of these stars belong to the stellar thick disk and halo of the Galaxy.

  2. THE DARK ENERGY SURVEY: PROSPECTS FOR RESOLVED STELLAR POPULATIONS

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Rossetto, Bruno M.; Santiago, Baslio X.; Girardi, Lo; Camargo, Julio I. B.; Balbinot, Eduardo; da Costa, Luiz N.; Yanny, Brian; Maia, Marcio A. G.; Makler, Martin; Ogando, Ricardo L. C.; et al

    2011-06-01

    Wide angle and deep surveys, regardless of their primary purpose, always sample a large number of stars in the Galaxy and in its satellite system. We here make a forecast of the expected stellar sample resulting from the Dark Energy Survey and the perspectives that it will open for studies of Galactic structure and resolved stellar populations in general. An estimated 1.2 x 108 stars will be sampled in DES grizY filters in the southern equatorial hemisphere. This roughly corresponds to 20% of all DES sources. Most of these stars belong to the stellar thick disk and halo of themoreGalaxy.less

  3. Human Rights

    ScienceCinema (OSTI)

    None

    2011-04-25

    Daniel Meyer, Président de la ligue française de défense de droits de l'homme et du citoyen fait un exposé sur son engagement (politique). Dans la deuxième partie, une avocate brésilienne (en exil)donne un témoignage de la violation des droits de l'homme sous la dictature militaire de son pays; elle a défendu pendant 6 ans des prisonniers politiques.

  4. Eia.gov BETA - Data - U.S. Energy Information Administration (EIA)

    Gasoline and Diesel Fuel Update (EIA)

    Tableau croisé des definitions English FranÇais Español A B C D E É F G H I J K L M N O P Q R S T U V W X Y Z Parcourir les termes liés aux catégories suivantes: pétrole brut et équivalents liquides de gaz naturel additifs et composés oxygénés Produits pétroliers gaz naturel biocarburant électricité Consultez l'index des termes

  5. Fermilab Cultural Events in Chicago's Far West Side

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Art of Darkness Images from the Dark Energy Survey On Display: February 19, 2016 -April 29, 2016 Reception - Friday, March 18 5-7pm Fermilab Art Gallery, Wilson Hall The universe has been expanding since the Big Bang almost 14 billion years ago. Now, the expansion of the universe is accelerating, driven by a new fundamental form of energy called dark energy. The Dark Energy Survey (DES) is a collaboration of more than 400 scientists from over 30 institutions across 7 countries. DES aims to find

  6. Iran Thomas Auditorium, 8600

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    January 29, 2010 11:00 am Iran Thomas Auditorium, 8600 (Bio)Functional Polymer Surfaces generated via Surface-Initiated, Controlled Radical Polymerization Harm-Anton Klok Laboratoire des Polymères, Institut des Matériaux, Ecole Polytechnique Fédérale de Lausanne (EPFL) CH-1015 Lausanne, Switzerland CNMS D D I I S S C C O O V V E E R R Y Y SEMINAR SERIES Abstract: This contribution will discuss the use of polymer brushes prepared via surface-initiated atom transfer radical polymerization

  7. Needs assessment for fire department services and resources for the Los Alamos National Laboratory, Los Alamos, New Mexico. Final report

    SciTech Connect (OSTI)

    1995-11-15

    This report has been developed in response to a request from the Los Alamos National Laboratory (LANL) to evaluate the need for fire department services so as to enable the Laboratory to plan effective fire protection and thereby: meet LANL`s regulatory and contractual obligations; interface with the Department of Energy (DOE) and other agencies on matters relating to fire and emergency services; and ensure appropriate protection of the community and environment. This study is an outgrowth of the 1993 Fire Department Needs Assessment (prepared for DOE) but is developed from the LANL perspective. Input has been received from cognizant and responsible representatives at LANL, DOE, Los Alamos County (LAC) and the Los Alamos Fire Department (LAFD).

  8. Identification Of Natural Dyes On Archaeological Textile Objects Using Laser Induced Fluorescent Technique

    SciTech Connect (OSTI)

    Abdel-Kareem, O.; Eltokhy, A.; Harith, M. A.

    2011-09-22

    This study aims to evaluate the use of Laser Fluorescent as a non-destructive technique for identification of natural dyes on archaeological textile objects. In this study wool textile samples were dyed with 10 natural dyes such as cochineal, cutch, henna, indigo, Lac, madder, safflower, saffron, sumac and turmeric. These dyes common present on archaeological textile objects to be used as standard dyed textile samples. These selected natural dyes will be used as known references that can be used a guide to identify unknown archaeological dyes. The dyed textile samples were investigated with laser radiation in different wavelengths to detect the best wavelengths for identification each dye. This study confirms that Laser Florescent is very useful and a rapid technique can be used as a non-destructive technique for identification of natural dyes on archaeological textile objects. The results obtained with this study can be a guide for all conservators in identification of natural organic dyes on archaeological textile objects.

  9. Developing a Biosensor for Estrogens in Water Samples: Study ofthe Real-time Response of Live Cells of the Estrogen-sensitive YeastStrain RMY/ER-ERE using Fluorescence Microscopy

    SciTech Connect (OSTI)

    Wozei, E.; Hermanowicz, S.W.; Holman, H-Y.N.

    2006-01-01

    Using a fluorescein di-{beta}-d-galactopyranoside (FDG) substrate we show that in live cells of an estrogen-sensitive yeast strain RMY/ER-ERE with human estrogen receptor (ER{alpha}) gene and the lacZ gene which encodes {beta}-galactosidase, the uptake of 17{beta}-estradiol (E2) and the subsequent production of {beta}-galactosidase enzyme occur quite rapidly, with maximal enzyme-catalyzed product formation evident after about 30 min of exposure to E2. This finding which agrees with the well-known rates of enzyme-catalyzed reactions could have implications for shortening the duration of environmental sample screening and monitoring regimes using yeast-based estrogen assays, and the development of biosensors for environmental estrogens to complement quantification methods.

  10. Developing a Biosensor for Estrogens in Water Samples: Study ofthe Real-time Response of Live Cells of the Estrogen-sensitive YeastStrain RMY/ER-ERE using Fluorescence Microscopy

    SciTech Connect (OSTI)

    Wozei, E.; Hermanowicz, S.W.; Holman, H-Y.N.

    2005-07-13

    Using a fluorescein di-{beta}-D-galactopyranoside (FDG) substrate we show that in live cells of an estrogen-sensitive yeast strain RMY/ER-ERE with human estrogen receptor (ER{alpha}) gene and the lacZ gene which encodes {beta}-galactosidase, the uptake of 17 {beta}-estradiol (E2) and the subsequent production of {beta}-galactosidase enzyme occur quite rapidly, with maximal enzyme-catalyzed product formation evident after about 30 minutes of exposure to E2. This finding which agrees with the well-known rates of enzyme-catalyzed reactions could have implications for shortening the duration of environmental sample screening and monitoring regimes using yeast-based estrogen assays, and the development of biosensors for environmental estrogens to complement quantification methods.

  11. MOJAVE. X. PARSEC-SCALE JET ORIENTATION VARIATIONS AND SUPERLUMINAL MOTION IN ACTIVE GALACTIC NUCLEI

    SciTech Connect (OSTI)

    Lister, M. L.; Richards, J. L.; Aller, M. F.; Aller, H. D.; Homan, D. C.; Kellermann, K. I.; Kovalev, Y. Y.

    2013-11-01

    We describe the parsec-scale kinematics of 200 active galactic nucleus (AGN) jets based on 15 GHz Very Long Baseline Array (VLBA) data obtained between 1994 August 31 and 2011 May 1. We present new VLBA 15 GHz images of these and 59 additional AGNs from the MOJAVE and 2 cm Survey programs. Nearly all of the 60 most heavily observed jets show significant changes in their innermost position angle over a 12-16 yr interval, ranging from 10 to 150 on the sky, corresponding to intrinsic variations of ?0.5 to ?2. The BL Lac jets show smaller variations than quasars. Roughly half of the heavily observed jets show systematic position angle trends with time, and 20 show indications of oscillatory behavior. The time spans of the data sets are too short compared to the fitted periods (5-12 yr), however, to reliably establish periodicity. The rapid changes and large jumps in position angle seen in many cases suggest that the superluminal AGN jet features occupy only a portion of the entire jet cross section and may be energized portions of thin instability structures within the jet. We have derived vector proper motions for 887 moving features in 200 jets having at least five VLBA epochs. For 557 well-sampled features, there are sufficient data to additionally study possible accelerations. We find that the moving features are generally non-ballistic, with 70% of the well-sampled features showing either significant accelerations or non-radial motions. Inward motions are rare (2% of all features), are slow (<0.1 mas yr{sup 1}), are more prevalent in BL Lac jets, and are typically found within 1 mas of the unresolved core feature. There is a general trend of increasing apparent speed with distance down the jet for both radio galaxies and BL Lac objects. In most jets, the speeds of the features cluster around a characteristic value, yet there is a considerable dispersion in the distribution. Orientation variations within the jet cannot fully account for the dispersion, implying that the features have a range of Lorentz factor and/or pattern speed. Very slow pattern speed features are rare, comprising only 4% of the sample, and are more prevalent in radio galaxy and BL Lac jets. We confirm a previously reported upper envelope to the distribution of speed versus beamed luminosity for moving jet features. Below 10{sup 26} W Hz{sup 1} there is a fall-off in maximum speed with decreasing 15 GHz radio luminosity. The general shape of the envelope implies that the most intrinsically powerful AGN jets have a wide range of Lorentz factors up to ?40, while intrinsically weak jets are only mildly relativistic.

  12. Lightning arrestor connector lead magnesium niobate qualification pellet test procedures.

    SciTech Connect (OSTI)

    Tuohig, W.; Mahoney, Patrick A.; Tuttle, Bruce Andrew; Wheeler, Jill Susanne

    2009-02-01

    Enhanced knowledge preservation for DOE DP technical component activities has recently received much attention. As part of this recent knowledge preservation effort, improved documentation of the sample preparation and electrical testing procedures for lead magnesium niobate--lead titanate (PMN/PT) qualification pellets was completed. The qualification pellets are fabricated from the same parent powders used to produce PMN/PT lightning arrestor connector (LAC) granules at HWF&T. In our report, the procedures for fired pellet surface preparation, electrode deposition, electrical testing and data recording are described. The dielectric measurements described in our report are an information only test. Technical reasons for selecting the electrode material, electrode size and geometry are presented. The electrical testing is based on measuring the dielectric constant and dissipation factor of the pellet during cooling from 280 C to 220 C. The most important data are the temperature for which the peak dielectric constant occurs (Curie Point temperature) and the peak dielectric constant magnitude. We determined that the peak dielectric constant for our procedure would be that measured at 1 kHz at the Curie Point. Both the peak dielectric constant and the Curie point parameters provide semi-quantitative information concerning the chemical and microstructural homogeneity of the parent material used for the production of PMN/PT granules for LACs. Finally, we have proposed flag limits for the dielectric data for the pellets. Specifically, if the temperature of the peak dielectric constant falls outside the range of 250 C {+-} 30 C we propose that a flag limit be imposed that will initiate communication between production agency and design agency personnel. If the peak dielectric constant measured falls outside the range 25,000 {+-} 10,000 we also propose that a flag limit be imposed.

  13. Studies of the jet in BL Lacertae. I. Recollimation shock and moving emission features

    SciTech Connect (OSTI)

    Cohen, M. H.; Hovatta, T.; Meier, D. L.; Arshakian, T. G.; Homan, D. C.; Kovalev, Y. Y.; Pushkarev, A. B.; Savolainen, T.

    2014-06-01

    Parsec-scale VLBA images of BL Lac at 15 GHz show that the jet contains a permanent quasi-stationary emission feature 0.26 mas (0.34 pc projected) from the core, along with numerous moving features. In projection, the tracks of the moving features cluster around an axis at a position angle of 166.6 that connects the core with the standing feature. The moving features appear to emanate from the standing feature in a manner strikingly similar to the results of numerical two-dimensional relativistic magneto-hydrodynamic (RMHD) simulations in which moving shocks are generated at a recollimation shock (RCS). Because of this, and the close analogy to the jet feature HST-1 in M87, we identify the standing feature in BL Lac as an RCS. We assume that the magnetic field dominates the dynamics in the jet, and that the field is predominantly toroidal. From this we suggest that the moving features are compressions established by slow and fast mode magneto-acoustic MHD waves. We illustrate the situation with a simple model in which the slowest moving feature is a slow-mode wave, and the fastest feature is a fast-mode wave. In the model, the beam has Lorentz factor ?{sub beam}{sup gal}?3.5 in the frame of the host galaxy and the fast mode wave has Lorentz factor ?{sub Fwave}{sup beam}?1.6 in the frame of the beam. This gives a maximum apparent speed for the moving features, ?{sub app} = v{sub app}/c = 10. In this model the Lorentz factor of the pattern in the galaxy frame is approximately three times larger than that of the beam itself.

  14. C.F.von Weizsäcker-High Energy Physics

    ScienceCinema (OSTI)

    None

    2011-04-25

    C.F.von Weizsäcker (1912-2007),physicien,philosophe et "chercheur de paix", prit la décision de faire des études de physique sous l'influence de W.Heisenberg qu'il rencontra en 1927.

  15. Impressions on Chinas Popular Republic

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le D.G. Jentschke présente le Prof.Yang, née en 1922 en Chine où il a aussi fait ses études; il parle de ses impressions en Chine (p.e. mariage etc....) avec présentation des dias

  16. Combining Galaxy-Galaxy Lensing and Galaxy Clustering

    SciTech Connect (OSTI)

    Park, Youngsoo; Krause, Elisabeth; Dodelson, Scott; Jain, Bhuvnesh; Amara, Adam; Becker, Matt; Bridle, Sarah; Clampitt, Joseph; Crocce, Martin; Honscheid, Klaus; Gaztanaga, Enrique; Sanchez, Carles; Wechsler, Risa

    2015-01-01

    Combining galaxy-galaxy lensing and galaxy clustering is a promising method for inferring the growth rate of large scale structure, a quantity that will shed light on the mechanism driving the acceleration of the Universe. The Dark Energy Survey (DES) is a prime candidate for such an analysis, with its measurements of both the distribution of galaxies on the sky and the tangential shears of background galaxies induced by these foreground lenses. By constructing an end-to-end analysis that combines large-scale galaxy clustering and small-scale galaxy-galaxy lensing, we also forecast the potential of a combined probes analysis on DES datasets. In particular, we develop a practical approach to a DES combined probes analysis by jointly modeling the assumptions and systematics affecting the different components of the data vector, employing a shared halo model, HOD parametrization, photometric redshift errors, and shear measurement errors. Furthermore, we study the effect of external priors on different subsets of these parameters. We conclude that DES data will provide powerful constraints on the evolution of structure growth in the universe, conservatively/ optimistically constraining the growth function to 8%/4.9% with its first-year data covering 1000 square degrees, and to 4%/2.3% with its full five-year data covering 5000 square degrees.

  17. 10th Anniversary P.S.

    ScienceCinema (OSTI)

    None

    2011-04-25

    John Adams parle de la préhistoire du P.S. avec présentation des dias. Le DG B.Gregory prend la parole. Les organisateurs présentent sous la direction du "Prof.Ocktette"(?) un sketch très humoristique (p.e.existence de Quark etc.....)

  18. KINEMATIC PROPERTIES AS PROBES OF THE EVOLUTION OF DWARF GALAXIES IN THE VIRGO CLUSTER

    SciTech Connect (OSTI)

    Toloba, E.; Gorgas, J.; De Paz, A. Gil; Boselli, A.; Peletier, R. F.; Yildiz, U.; Cenarro, A. J.; Gadotti, D. A.; Pedraz, S.

    2009-12-10

    We present new observational results on the kinematical, morphological, and stellar population properties of a sample of 21 dEs located both in the Virgo Cluster and in the field, which show that 52% of the dEs (1) are rotationally supported, (2) exhibit structural signs of typical rotating systems such as disks, bars, or spiral arms, (3) are younger (approx3 Gyr) than non-rotating dEs, and (4) are preferentially located either in the outskirts of Virgo or in the field. This evidence is consistent with the idea that rotationally supported dwarfs are late-type spirals or irregulars that recently entered the cluster and lost their gas through a ram pressure stripping event, quenching their star formation and becoming dEs through passive evolution. We also find that all, but one, galaxies without photometric hints for hosting disks are pressure supported and are all situated in the inner regions of the cluster. This suggests a different evolution from the rotationally supported systems. Three different scenarios for these non-rotating galaxies are discussed (in situ formation, harassment, and ram pressure stripping).

  19. E-mail et Web : pour une navigation sans risque

    ScienceCinema (OSTI)

    None

    2011-10-06

    Présentation orale en français, support visuel en anglais. À travers des exemples concrets, vous consoliderez vos connaissances et pourrez ainsi réajuster vos habitudes concernant l?utilisation sécurisée de votre boîte e-mail et de votre navigateur Web.

  20. Science anc Society

    ScienceCinema (OSTI)

    None

    2011-04-25

    S.P.Worden, membre technique de l'U.S.délégation à Genève pour les négociations sur les armes nucléaires, est physicien, astronome, scientifique et officier de l'armée de l'air. Il parlera des technologies de défense stratégique

  1. Meeting LEP

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le DG J.Adams fait l'introduction et présente les deux autres orateurs. Pierre Darriulat qui fait un doscours sur la physique à l'occasion du LEP, Wolfgang Schnell, qui parle du projet de la machine LEP et le DG lui-même contribue avec quelques réflexions. Présentation des dias

  2. Problem of Questioning

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le Prof.Leprince-Ringuet, chercheur sur le plan scientifique, artistique et humain, parle de la remise en question des hommes et la remise en question scientifique fondamentale ou exemplaire- plusieurs personnes prennent la parole p.ex Jeanmairet, Adam, Gregory. Le Prof.Gregory clot la soirée en remerciant le Prof.Leprince-Ringuet

  3. Science and Society

    ScienceCinema (OSTI)

    None

    2011-04-25

    Dans une période d'un mois, 2me conférence sur le contrôle d'armes. Le conférencier Drell, américain, parle comme son collègue Worden (AUDIO-1985-005) des problèmes de défense stratégique.

  4. Andrei Sakharov

    ScienceCinema (OSTI)

    None

    2011-04-25

    Ce discours donné par Mons.Jonauch qui est né en Tchécoslovaquie et a fait ses études à Leningrad, Moscou et Prague, est organisé par le comité Youri Orlov. Le conférencier parle de Andrei Sakharov, ce physicien et homme soviétique qui fit ses études à Moscou, effectua des recherches sur les armes thermonucléaires et entra à l'Académie des Sciences d'URSS en 1953. Il participa à la mise au point de la bombe à hydrogène, mais s'opposa quelques années plus tard à la poursuite des expériences nucléaires. Il créa en 1970 le comité pour la défense des droits de l'homme ce que lui valut le prix Nobel de la paix en 1975.

  5. Western Dilemma

    ScienceCinema (OSTI)

    None

    2011-04-25

    L'association du personnel présente Anthony Sampson, écrivain connu dans le monde entier par ses nombreux ouvrages et publications (International Harold Tribune, Observer, News Week). Il nous parle du commerce des armes et du Moyen Orient.

  6. Press conference

    ScienceCinema (OSTI)

    None

    2011-04-25

    Exposés de plusieurs intervenants de la direction et du conseil, comme le Prof.Ramsey, président du conseil sur l'adhésion récente de la Finlande et le "boom" scientifique des pays de l'est.

  7. CX-003043: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Development of a Training Program for Commercial Building TechniciansCX(s) Applied: A1, A9, A11Date: 07/19/2010Location(s): Des Plaines, IllinoisOffice(s): Energy Efficiency and Renewable Energy, National Energy Technology Laboratory

  8. STELLAR KINEMATICS AND STRUCTURAL PROPERTIES OF VIRGO CLUSTER DWARF EARLY-TYPE GALAXIES FROM THE SMAKCED PROJECT. III. ANGULAR MOMENTUM AND CONSTRAINTS ON FORMATION SCENARIOS

    SciTech Connect (OSTI)

    Toloba, E.; Guhathakurta, P.; Peletier, R. F.; Emsellem, E.; Lisker, T.; Van de Ven, G.; Simon, J. D.; Adams, J. J.; Benson, A. J.; Falcn-Barroso, J.; Ry?, A.; Gorgas, J.; Hensler, G.; Janz, J.; Laurikainen, E.; Salo, H.; Paudel, S.

    2015-02-01

    We analyze the stellar kinematics of 39 dwarf early-type galaxies (dEs) in the Virgo Cluster. Based on the specific stellar angular momentum ?{sub Re} and the ellipticity, we find 11 slow rotators and 28 fast rotators. The fast rotators in the outer parts of the Virgo Cluster rotate significantly faster than fast rotators in the inner parts of the cluster. Moreover, 10 out of the 11 slow rotators are located in the inner 3 (D < 1 Mpc) of the cluster. The fast rotators contain subtle disk-like structures that are visible in high-pass filtered optical images, while the slow rotators do not exhibit these structures. In addition, two of the dEs have kinematically decoupled cores and four more have emission partially filling in the Balmer absorption lines. These properties suggest that Virgo Cluster dEs may have originated from late-type star-forming galaxies that were transformed by the environment after their infall into the cluster. The correlation between ?{sub Re} and the clustercentric distance can be explained by a scenario where low luminosity star-forming galaxies fall into the cluster, their gas is rapidly removed by ram-pressure stripping, although some of it can be retained in their core, their star formation is quenched but their stellar kinematics are preserved. After a long time in the cluster and several passes through its center, the galaxies are heated up and transformed into slow rotating dEs.

  9. CX-002724: Categorical Exclusion Determination

    Broader source: Energy.gov [DOE]

    Area of Interest 3 Deployment of Flex Combined Heat and Power System (Funding Opportunity Announcement 0000016)CX(s) Applied: B3.6Date: 06/21/2010Location(s): Des Plains, IllinoisOffice(s): Energy Efficiency and Renewable Energy, National Energy Technology Laboratory

  10. Meeting DG's

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le DG J.Adams commente les 3 thèmes de la réunion: 1.) le prochain DG du Cern (qui sera H.Schopper) 2.) le LEP 3.) les conclusions du comité des finances concernant salaires, allocations etc. Discussion entre le DG J.Adams, Mons.Ullmann, chef du personel et l'auditoire

  11. Science and Society

    ScienceCinema (OSTI)

    None

    2011-04-25

    "Can nuclear war be controled?"- la guerre nucléaire peut-elle être contrôlée? Tel est le thème de cette conférence avec présentation des dias.

  12. The Dark Energy Survey Data Management System

    SciTech Connect (OSTI)

    Mohr, Joseph J.; Barkhouse, Wayne; Beldica, Cristina; Bertin, Emmanuel; Dora Cai, Y.; Nicolaci da Costa, Luiz A.; Darnell, J.Anthony; Daues, Gregory E.; Jarvis, Michael; Gower, Michelle; Lin, Huan; /Fermilab /Rio de Janeiro Observ.

    2008-07-01

    The Dark Energy Survey (DES) collaboration will study cosmic acceleration with a 5000 deg2 griZY survey in the southern sky over 525 nights from 2011-2016. The DES data management (DESDM) system will be used to process and archive these data and the resulting science ready data products. The DESDM system consists of an integrated archive, a processing framework, an ensemble of astronomy codes and a data access framework. We are developing the DESDM system for operation in the high performance computing (HPC) environments at the National Center for Supercomputing Applications (NCSA) and Fermilab. Operating the DESDM system in an HPC environment offers both speed and flexibility. We will employ it for our regular nightly processing needs, and for more compute-intensive tasks such as large scale image coaddition campaigns, extraction of weak lensing shear from the full survey dataset, and massive seasonal reprocessing of the DES data. Data products will be available to the Collaboration and later to the public through a virtual-observatory compatible web portal. Our approach leverages investments in publicly available HPC systems, greatly reducing hardware and maintenance costs to the project, which must deploy and maintain only the storage, database platforms and orchestration and web portal nodes that are specific to DESDM. In Fall 2007, we tested the current DESDM system on both simulated and real survey data. We used TeraGrid to process 10 simulated DES nights (3TB of raw data), ingesting and calibrating approximately 250 million objects into the DES Archive database. We also used DESDM to process and calibrate over 50 nights of survey data acquired with the Mosaic2 camera. Comparison to truth tables in the case of the simulated data and internal crosschecks in the case of the real data indicate that astrometric and photometric data quality is excellent.

  13. Le LHC, un tunnel cosmique

    ScienceCinema (OSTI)

    None

    2011-10-06

    Et si la lumière au bout du tunnel du LHC était cosmique ? En d?autres termes, qu?est-ce que le LHC peut nous apporter dans la connaissance de l?Univers ? Car la montée en énergie des accélérateurs de particules nous permet de mieux appréhender l?univers primordial, chaud et dense. Mais dans quel sens dit-on que le LHC reproduit des conditions proches du Big bang ? Quelles informations nous apporte-t-il sur le contenu de l?Univers ? La matière noire est-elle détectable au LHC ? L?énergie noire ? Pourquoi l?antimatière accumulée au CERN est-elle si rare dans l?Univers ? Et si le CERN a bâti sa réputation sur l?exploration des forces faibles et fortes qui opèrent au sein des atomes et de leurs noyaux, est-ce que le LHC peut nous apporter des informations sur la force gravitationnelle qui gouverne l?évolution cosmique ? Depuis une trentaine d?années, notre compréhension de l?univers dans ses plus grandes dimensions et l?appréhension de son comportement aux plus petites distances sont intimement liées : en quoi le LHC va-t-il tester expérimentalement cette vision unifiée ? Tout public, entrée libre / Réservations au +41 (0)22 767 76 76

  14. Distributions of gamma-ray bursts and blazars in the L {sub p}-E {sub p}-plane and possible implications for their radiation physics

    SciTech Connect (OSTI)

    Lyu, Fen; Liang, En-Wei; Liang, Yun-Feng; Sun, Xiao-Na; Lu, Rui-Jing; Zhang, Bing [Department of Physics and GXU-NAOC Center for Astrophysics and Space Sciences, Guangxi University, Nanning 530004 (China); Wu, Xue-Feng [Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008 (China); Zhang, Jin, E-mail: lew@gxu.edu.cn, E-mail: xfwu@pmo.ac.cn, E-mail: zhang@physics.unlv.edu [National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012 (China)

    2014-09-20

    We present a spectral analysis for a sample of redshift-known gamma-ray bursts (GRBs) observed with Fermi/GBM. Together with the results derived from our systematical spectral energy distribution modeling with the leptonic models for a Fermi/LAT blazar sample, we compare the distributions of the GRBs and the blazars by plotting the synchrotron peak luminosity (L {sub s}) and the corresponding peak photon energy E {sub s} of blazars in the L {sub p}-E {sub p}-plane of GRBs, where L {sub p} and E {sub p} are the peak luminosity and peak photon energy of the GRB time-integrated ?f {sub ?} spectrum, respectively. The GRBs are in the high-L {sub p}, high-E {sub p} corner of the plane and a tight L {sub p}-E {sub p} relation is found, i.e., L{sub p}?E{sub p}{sup 2.13{sub ?}{sub 0}{sub .}{sub 4}{sub 6}{sup +{sup 0{sup .{sup 5{sup 4}}}}}}. Both flat spectrum radio quasars (FSRQs) and low-synchrotron peaking BL Lac objects (LBLs) are clustered in the low-E {sub p}, low-L {sub p} corner. Intermediate- and high-synchrotron peaking BL Lac objects (IBLs and HBLs) have E {sub s} ? 2 10{sup 3}-10{sup 2} keV and L {sub s} ? 10{sup 44}-10{sup 47} erg s{sup 1}, but no dependence of L {sub s} on E {sub s} is found. We show that the tight L{sub p} -E{sub p} relation of GRBs is potentially explained with the synchrotron radiation of fast-cooling electrons in a highly magnetized ejecta, and the weak anti-correlation of L {sub s}-E {sub s} for FSRQs and LBLs may be attributed to synchrotron radiation of slow-cooling electrons in a moderately magnetized ejecta. The distributions of IBLs and HBLs in the L {sub p}-E {sub p}-plane may be interpreted with synchrotron radiation of fast-cooling electrons in a matter-dominated ejecta. These results may present a unified picture for the radiation physics of relativistic jets in GRBs and blazars within the framework of the leptonic synchrotron radiation models.

  15. MOJAVE: Monitoring of jets in active galactic nuclei with VLBA experiments. XI. Spectral distributions

    SciTech Connect (OSTI)

    Hovatta, Talvikki; Aller, Margo F.; Aller, Hugh D.; Clausen-Brown, Eric; Kovalev, Yuri Y.; Pushkarev, Alexander B.; Savolainen, Tuomas; Homan, Daniel C.; Lister, Matthew L.

    2014-06-01

    We have obtained milliarcsecond-scale spectral index distributions for a sample of 190 extragalactic radio jets through the Monitoring of Jets in Active Galactic Nuclei with the VLBA Experiments (MOJAVE) project. The sources were observed in 2006 at 8.1, 8.4, 12.1, and 15.4 GHz, and we have determined spectral index maps between 8.1 and 15.4 GHz to study the four-frequency spectrum in individual jet features. We have performed detailed simulations to study the effects of image alignment and (u, v)-plane coverage on the spectral index maps to verify our results. We use the spectral index maps to study the spectral index evolution along the jet and determine the spectral distributions in different locations of the jets. The core spectral indices are on average flat with a mean value of +0.22 0.03 for the sample, while the jet spectrum is in general steep with a mean index of 1.04 0.03. A simple power-law fit is often inadequate for the core regions, as expected if the cores are partially self-absorbed. The overall jet spectrum steepens at a rate of about 0.001 to 0.004 per deprojected parsec when moving further out from the core with flat spectrum radio quasars having significantly steeper spectra (mean 1.09 0.04) than the BL Lac objects (mean 0.80 0.05). However, the spectrum in both types of objects flattens on average by ?0.2 at the locations of the jet components indicating particle acceleration or density enhancements along the jet. The mean spectral index at the component locations of 0.81 0.02 corresponds to a power-law index of ?2.6 for the electron energy distribution. We find a significant trend that jet components with linear polarization parallel to the jet (magnetic field perpendicular to the jet) have flatter spectra, as expected for transverse shocks. Compared to quasars, BL Lacs have more jet components with perpendicular magnetic field alignment, which may explain their generally flatter spectra. The overall steepening of the spectra with distance can be explained with radiative losses if the jets are collimating or with the evolution of the high-energy cutoff in the electron spectrum if the jets are conical. This interpretation is supported by a significant correlation with the age of the component and the spectral index, with older components having steeper spectra.

  16. Italian Exposition

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le DG parle dans son allocution à l'occasion de l'exposition (suivi d'une visite)de la contribution du Cern à la création d'une espace de la technologie européenne. Il parle de la manière comment organiser des formes fructueuses de coopération et coordination internationales dans ce domaine. "Afin de renforcer encore notre relation avec l'industrie et intensifier le transfert de la technologie nous proposerons au ministre de recherche de poursuivre dans le cadre du programme EUREKA ensemble avec les industries des programmes concrètes." Le ministre italien prend ensuite la parole.

  17. 25th Birthday Cern- Restaurant

    ScienceCinema (OSTI)

    None

    2011-04-25

    Cérémonie du 25ème anniversaire du Cern avec plusieurs orateurs et la présence de nombreux autorités cantonales et communales genevoises et personnalités, directeurs généraux, ministres, chercheurs.... Le conseiller féderal et chef du département des affaires étrangères de la confédération Monsieur Pierre Aubert prend la parole pour célébrer à la fois les résultats très remarquables de la coopération internationale en matière scientifique, mais aussi la volonté politique des états européens de mettre en commun leurs ressources pour faire oeuvre d'avenir. Un grand hommage est aussi donné aux deux directeurs disparus, les prof.Bakker et Gregory.

  18. Conference Salam/Musset

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le DG L.Van Hove introduit le Prof. A.Salam né en 1926 dans l'ouest du Pakistan, un des gagnants du prix nobel de physique de cette année. Célébration de ses contributions théoriques mondialement connues. Après chaque discours, un petit historique est présenté par Paul Musset. Mention honorable aussi pour l'expérience Gargamelle et ses collaborateurs.

  19. Inauguration LEP

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le DG H.Schopper salue le président de la république française, F.Mitterand, le président de la confédaration suisse P.Aubert, ainsi que les ministres et représentants du gouvernement des 12 états membres pour la célébration et inauguration du LEP.

  20. ITP Glass: Industrial Glass Bandwidth Analysis Final Report, August 2007

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Industrial Glass Bandwidth Analysis Prepared by: David M. Rue James Servaites Dr. Warren Wolf Gas Technology Institute Energy Utilization Center August 2007 Industrial Glass Bandwidth Analysis FINAL REPORT Prepared by: David M. Rue James Servaites Dr. Warren Wolf (independent consultant) Gas Technology Institute 1700 S. Mount Prospect Rd Des Plaines, IL 60018 Prepared for: U.S. Department of Energy Contract No. DE-FC36-03GO13092 August 2007 Table of Contents Table of Figures

  1. History of Cern

    ScienceCinema (OSTI)

    None

    2011-04-25

    Cérémonie à l'occasion de l'apparition du premier volume du livre sur l'histoire du Cern, avec plusieurs personnes présentes qui jouaient un rôle important dans cette organisation européenne couronnée de succès grâce à l'esprit des membres fondateurs qui est et restera essentiel

  2. Photometric Redshifts for the Dark Energy Survey and VISTA and Implications

    Office of Scientific and Technical Information (OSTI)

    for Large Scale Structure (Journal Article) | SciTech Connect SciTech Connect Search Results Journal Article: Photometric Redshifts for the Dark Energy Survey and VISTA and Implications for Large Scale Structure Citation Details In-Document Search Title: Photometric Redshifts for the Dark Energy Survey and VISTA and Implications for Large Scale Structure We conduct a detailed analysis of the photometric redshift requirements for the proposed Dark Energy Survey (DES) using two sets of mock

  3. Hig Resolution Seismometer Insensitive to Extremely Strong Magnetic Fields

    SciTech Connect (OSTI)

    Abramovich, Igor A

    2009-07-14

    A highly sensitive broadband seismic sensor has been developed successfully to be used in beam focusing systems of particale accelerators. The sensor is completely insensitive to extremely strong magnetic fields and to hard radiation conditions that exist at the place of their installation. A unique remote sensor calibration method has been invented and implemented. Several such sensors were sold to LAPP (LAPP-IN2P3/CNRS-Universit de Savoie; Laboratoire d'Annecy-le-Vieux de Physique des Particules)

  4. CMI Education and Outreach in 2013 | Critical Materials Institute

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    3 CMI education and outreach in 2013: Hardin Valley Academy in Knoxville, Tennessee, December: CMI Director Alex King talked to sophomores Materials Research Society, Dec. 2: Karl Gschneidner, chief scientist for the Critical Materials Institute, talked with critical materials with materials science and engineering students at the MRS Fall conference TEDxDes Moines, Sept. 8: CMI Director Alex King presented "The Dawn of the Age of Critical Materials"

  5. NREL: Photovoltaics Research - Stephan Lany, Ph.D.

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Stephan Lany, Ph.D. Scientist V Photo of Stephan Lany 303-384-6652 Stephan.Lany@nrel.gov Stephan Lany is a computational materials scientist with a background in electronic structure calculations for semiconducting materials. He received his doctorate in physics in 2002 from the Universität des Saarlandes, Germany, and joined NREL in 2003 as a postdoctoral researcher. As a staff scientist, he is currently leading computational research activities in support of the Energy Frontier Research

  6. Lab hosts Science Bound students for My Brother's Keeper event | The Ames

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Laboratory Lab hosts Science Bound students for My Brother's Keeper event Ames Laboratory hosted approximately 100 eighth-grade students on Feb. 13 who are participating in the Science Bound program through Iowa State University. The students were from the Marshalltown, Denison and Des Moines school districts. After a welcome from Ames Laboratory Director Adam Schwartz, and a viewing of the Ames Laboratory "I Love Science" video, the students rotated between five stations for

  7. Roberta Poloni | Center for Gas SeparationsRelevant to Clean Energy

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Technologies | Blandine Jerome Roberta Poloni Previous Next List Poloni Roberta Poloni Formerly: Postdoctoral Researcher, Department of Chemical & Biomolecular Engineering University of California, Berkeley Presently: Postoctoral Researcher, Laboratoire de Science et Ingéniérie des Matériaux et Procédés, Institut Polytechnique de Grenoble, France Ph.D. in Physics, University of Lyon-1, France BS in Physics, Camerino, Italy EFRC research: Detailed studies on the CO2 locations in

  8. Torleif Ericson 60th Birthday

    ScienceCinema (OSTI)

    None

    2011-04-25

    Plusieurs discours à l'occasion du 60me anniversaire de Torleif Ericson, physicien né à Lund (Suède), et remerciements pour son travail et son effort de relier la physique des particules à la physique nucléaire. A la fin de la cérémonie un document scientifique de 400 pages "die Festschrift" lui est remis comme cadeau d'anniversaire avec un grand nombre de contributions d'amis etc...

  9. Microsoft Word - grosdidier.doc

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Stratification and Radiative Transfer Y. Grosdidier,S. Lovejoy McGill University Montreal, Canada B. P. Watson St. Lawrence University Canton, New York D. Schertzer École Nationale des Ponts et Chaussées Toulouse, France Introduction: Differential stratification and convection of the atmosphere over wide ranges of scales Theories of atmospheric dynamics, turbulence, cloud structure and atmospheric radiative transfer are nearly all based on the idea that at small enough scales, structures are

  10. Application for presidential permit OE Docket No. PP-371 Northern Pass

    Energy Savers [EERE]

    Transmission LLC: Addendum to Application | Department of Energy Addendum to Application Application for presidential permit OE Docket No. PP-371 Northern Pass Transmission LLC: Addendum to Application On October 14, 2010, Northern Pass Transmission, LLC submitted an application for a Presidential Permit to construct a 1,200 MW high voltage direct current ("HVDC") transmission line (the "Application") from the Des Cantons substation in Quebec, to Franklin, New Hampshire

  11. Low-Cost Gas Heat Pump For Building Space Heating | Department of Energy

    Energy Savers [EERE]

    Gas Heat Pump For Building Space Heating Low-Cost Gas Heat Pump For Building Space Heating Credit: Stone Mountain Technologies Credit: Stone Mountain Technologies Lead Performer: Stone Mountain Technologies - Erwin, TN Partners: -- A.O. Smith - Milwaukee, WI -- Gas Technology Institute - Des Plaines, IL DOE Funding: $903,000 Cost Share: $232,294 Project Term: 3/1/2013 - 2/28/2015 Funding Opportunity: Energy Savings Through Improved Mechanical Systems and Building Envelope Technologies 2012

  12. Everest

    ScienceCinema (OSTI)

    None

    2011-04-25

    Chris Bonington, est né à Hampstead et a fait des études à University Collège School à Londres et au Royal Military Academy à Sundhorst. Il est un alpiniste mondialement connu qui a fait un grand nombre de premiers ascensions, comme celle de la face sud-ouest de l'Everest avec une équipe de 70 hommes en septembre 1975

  13. Electricity Advisory Committee Meeting Presentations June 2014 - Tuesday,

    Office of Environmental Management (EM)

    June 17, 2014 | Department of Energy Tuesday, June 17, 2014 Electricity Advisory Committee Meeting Presentations June 2014 - Tuesday, June 17, 2014 The Department of Energy's Electricity Advisory Committee held a meeting on Monday, June 16 and Tuesday, June 17 at the National Rural Electric Cooperative Association, 4301 Wilson Blvd., Arlington, VA. Tuesday, June 17, 2014 Panel - Distributed Energy Storage (DES) - Wanda Reder, S&C, moderator Willem Fadrhonc, STEM Tom Weaver, AEP Melicia

  14. Modeling the transfer function for the Dark Energy Survey

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Chang, C.; Busha, M. T.; Wechsler, R. H.; Refregier, A.; Amara, A.; Rykoff, E.; Becker, M. R.; Bruderer, C.; Gamper, L.; Leistedt, B.; et al

    2015-03-04

    We present a forward-modelling simulation framework designed to model the data products from the Dark Energy Survey (DES). This forward-model process can be thought of as a transfer function a mapping from cosmological and astronomical signals to the final data products used by the scientists. Using output from the cosmological simulations (the Blind Cosmology Challenge), we generate simulated images (the Ultra Fast Image Simulator, Berge et al. 2013) and catalogs representative of the DES data. In this work we simulate the 244 deg2 coadd images and catalogs in 5 bands for the DES Science Verification (SV) data. The simulationmoreoutput is compared with the corresponding data to show that major characteristics of the images and catalogs can be captured. We also point out several directions of future improvements. Two practical examples, star/galaxy classification and proximity effects on object detection, are then used to demonstrate how one can use the simulations to address systematics issues in data analysis. With clear understanding of the simplifications in our model, we show that one can use the simulations side-by-side with data products to interpret the measurements. This forward modelling approach is generally applicable for other upcoming and future surveys. As a result, it provides a powerful tool for systematics studies which is sufficiently realistic and highly controllable.less

  15. Modeling the Transfer Function for the Dark Energy Survey

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Chang, C.

    2015-03-04

    We present a forward-modeling simulation framework designed to model the data products from the Dark Energy Survey (DES). This forward-model process can be thought of as a transfer function—a mapping from cosmological/astronomical signals to the final data products used by the scientists. Using output from the cosmological simulations (the Blind Cosmology Challenge), we generate simulated images (the Ultra Fast Image Simulator) and catalogs representative of the DES data. In this work we demonstrate the framework by simulating the 244 deg2 coadd images and catalogs in five bands for the DES Science Verification data. The simulation output is compared with themore » corresponding data to show that major characteristics of the images and catalogs can be captured. We also point out several directions of future improvements. Two practical examples—star-galaxy classification and proximity effects on object detection—are then used to illustrate how one can use the simulations to address systematics issues in data analysis. With clear understanding of the simplifications in our model, we show that one can use the simulations side-by-side with data products to interpret the measurements. This forward modeling approach is generally applicable for other upcoming and future surveys. It provides a powerful tool for systematics studies that is sufficiently realistic and highly controllable.« less

  16. Modeling the transfer function for the Dark Energy Survey

    SciTech Connect (OSTI)

    Chang, C.; Busha, M. T.; Wechsler, R. H.; Refregier, A.; Amara, A.; Rykoff, E.; Becker, M. R.; Bruderer, C.; Gamper, L.; Leistedt, B.; Peiris, H.; Abbott, T.; Abdalla, F. B.; Balbinot, E.; Banerji, M.; Bernstein, R. A.; Bertin, E.; Brooks, D.; Carnero, A.; Desai, S.; da Costa, L. N.; Cunha, C. E.; Eifler, T.; Evrard, A. E.; Fausti Neto, A.; Gerdes, D.; Gruen, D.; James, D.; Kuehn, K.; Maia, M. A. G.; Makler, M.; Ogando, R.; Plazas, A.; Sanchez, E.; Santiago, B.; Schubnell, M.; Sevilla-Noarbe, I.; Smith, C.; Soares-Santos, M.; Suchyta, E.; Swanson, M. E. C.; Tarle, G.; Zuntz, J.

    2015-03-04

    We present a forward-modelling simulation framework designed to model the data products from the Dark Energy Survey (DES). This forward-model process can be thought of as a transfer function a mapping from cosmological and astronomical signals to the final data products used by the scientists. Using output from the cosmological simulations (the Blind Cosmology Challenge), we generate simulated images (the Ultra Fast Image Simulator, Berge et al. 2013) and catalogs representative of the DES data. In this work we simulate the 244 deg2 coadd images and catalogs in 5 bands for the DES Science Verification (SV) data. The simulation output is compared with the corresponding data to show that major characteristics of the images and catalogs can be captured. We also point out several directions of future improvements. Two practical examples, star/galaxy classification and proximity effects on object detection, are then used to demonstrate how one can use the simulations to address systematics issues in data analysis. With clear understanding of the simplifications in our model, we show that one can use the simulations side-by-side with data products to interpret the measurements. This forward modelling approach is generally applicable for other upcoming and future surveys. As a result, it provides a powerful tool for systematics studies which is sufficiently realistic and highly controllable.

  17. Ultra-broadband 2D electronic spectroscopy of carotenoid-bacteriochlorophyll interactions in the LH1 complex of a purple bacterium

    SciTech Connect (OSTI)

    Maiuri, Margherita; Rhault, Julien; Polli, Dario; Cerullo, Giulio; Carey, Anne-Marie; Hacking, Kirsty; Cogdell, Richard J.; Garavelli, Marco; Ler, Larry

    2015-06-07

    We investigate the excitation energy transfer (EET) pathways in the photosynthetic light harvesting 1 (LH1) complex of purple bacterium Rhodospirillum rubrum with ultra-broadband two-dimensional electronic spectroscopy (2DES). We employ a 2DES apparatus in the partially collinear geometry, using a passive birefringent interferometer to generate the phase-locked pump pulse pair. This scheme easily lends itself to two-color operation, by coupling a sub-10 fs visible pulse with a sub-15-fs near-infrared pulse. This unique pulse combination allows us to simultaneously track with extremely high temporal resolution both the dynamics of the photoexcited carotenoid spirilloxanthin (Spx) in the visible range and the EET between the Spx and the B890 bacterio-chlorophyll (BChl), whose Q{sub x} and Q{sub y} transitions peak at 585 and 881 nm, respectively, in the near-infrared. Global analysis of the one-color and two-color 2DES maps unravels different relaxation mechanisms in the LH1 complex: (i) the initial events of the internal conversion process within the Spx, (ii) the parallel EET from the first bright state S{sub 2} of the Spx towards the Q{sub x} state of the B890, and (iii) the internal conversion from Q{sub x} to Q{sub y} within the B890.

  18. The geometric factor of electrostatic plasma analyzers: A case study from the Fast Plasma Investigation for the Magnetospheric Multiscale mission

    SciTech Connect (OSTI)

    Collinson, Glyn A.; Dorelli, John C.; Moore, Thomas E.; Pollock, Craig; Mariano, Al; Shappirio, Mark D.; Adrian, Mark L.; Avanov, Levon A.; Lewis, Gethyn R.; Kataria, Dhiren O.; Bedington, Robert; Owen, Christopher J.; Walsh, Andrew P.; Arridge, Chris S.; Gliese, Ulrik; Barrie, Alexander C.; Tucker, Corey

    2012-03-15

    We report our findings comparing the geometric factor (GF) as determined from simulations and laboratory measurements of the new Dual Electron Spectrometer (DES) being developed at NASA Goddard Space Flight Center as part of the Fast Plasma Investigation on NASA's Magnetospheric Multiscale mission. Particle simulations are increasingly playing an essential role in the design and calibration of electrostatic analyzers, facilitating the identification and mitigation of the many sources of systematic error present in laboratory calibration. While equations for laboratory measurement of the GF have been described in the literature, these are not directly applicable to simulation since the two are carried out under substantially different assumptions and conditions, making direct comparison very challenging. Starting from first principles, we derive generalized expressions for the determination of the GF in simulation and laboratory, and discuss how we have estimated errors in both cases. Finally, we apply these equations to the new DES instrument and show that the results agree within errors. Thus we show that the techniques presented here will produce consistent results between laboratory and simulation, and present the first description of the performance of the new DES instrument in the literature.

  19. LHC, le Big Bang en éprouvette

    ScienceCinema (OSTI)

    None

    2011-10-06

    Notre compréhension de l?Univers est en train de changer? Bar des Sciences - Tout public Débat modéré par Marie-Odile Montchicourt, journaliste de France Info. Evenement en vidéoconférence entre le Globe de la science et de l?innovation, le bar le Baloard de Montpellier et la Maison des Métallos à Paris. Intervenants au CERN : Philippe Charpentier et Daniel Froideveaux, physiciens au CERN. Intervenants à Paris : Vincent Bontemps, philosophe et chercheur au CEA ; Jacques Arnould, philosophe, historien des sciences et théologien, Jean-Jacques Beineix, réalisateur, producteur, scénariste de cinéma. Intervenants à Montpellier (LPTA) : André Neveu, physicien théoricien et directeur de recherche au CNRS ; Gilbert Moultaka, physicien théoricien et chargé de recherche au CNRS. Partenariat : CERN, CEA, IN2P3, Université MPL2 (LPTA) Dans le cadre de la Fête de la science 2008

  20. SOURCE IDENTIFICATION IN THE IGR J17448-3232 FIELD: DISCOVERY OF THE SCORPIUS GALAXY CLUSTER

    SciTech Connect (OSTI)

    Barrire, Nicolas M.; Tomsick, John A.; Wik, Daniel R.; Chaty, Sylvain; Rodriguez, Jrome

    2015-01-20

    We use a 43 ks XMM-Newton observation to investigate the nature of sources first distinguished by a follow-up Chandra observation of the field surrounding INTEGRAL source IGR J17448-3232, which includes extended emission and a bright point source previously classified as a blazar. We establish that the extended emission is a heretofore unknown massive galaxy cluster hidden behind the Galactic bulge. The emission-weighted temperature of the cluster within the field of view is 8.8 keV, with parts of the cluster reaching temperatures of up to 12 keV; no cool core is evident. At a redshift of 0.055, the cluster is somewhat under-luminous relative to the X-ray luminosity-temperature relation, which may be attributable to its dynamical state. We present a preliminary analysis of its properties in this paper. We also confirm that the bright point source is a blazar, and we propose that it is either a flat spectrum radio quasar or a low-frequency peaked BL Lac object. We find four other fainter sources in the field, which we study and tentatively identify. Only one, which we propose is a foreground Galactic X-ray binary, is hard enough to contribute to IGR J17448-3232, but it is too faint to be significant. We thus determine that IGR J17448-3232 is in fact the galaxy cluster up to ?45 keV and the blazar beyond.

  1. Detection of phenols using engineered bacteria

    DOE Patents [OSTI]

    Wise, Arlene A. (Philadelphia, PA); Kuske, Cheryl R. (Los Alamos, NM); Terwilliger, Thomas C. (Santa Fe, NM)

    2007-12-04

    Detection of phenols using engineered bacteria. A biosensor can be created by placing a reporter gene under control of an inducible promoter. The reporter gene produces a signal when a cognate transcriptional activator senses the inducing chemical. Creation of bacterial biosensors is currently restricted by limited knowledge of the genetic systems of bacteria that catabolize xenobiotics. By using mutagenic PCR to change the chemical specificity of the Pseudomonas species CF600 DmpR protein, the potential for engineering novel biosensors for detection of phenols has been demonstrated. DmpR, a well-characterized transcriptional activator of the P. CF600's dmp operon mediates growth on simple phenols. Transcription from Po, the promoter heading the dmp operon, is activated when the sensor domain of DmpR interacts with phenol and mono-substituted phenols. By altering the sensor domain of the DmpR, a group of DmpR derivatives that activate transcription of a Po-lacZ fusion in response to eight of the EPA's eleven priority pollutant phenols has been created. The assays and the sensor domain mutations that alter the chemical specificity of DmpR is described.

  2. Ligand specificity of MobR, a transcriptional regulator for the 3-hydroxybenzoate hydroxylase gene of Comamonas testosteroni KH122-3s

    SciTech Connect (OSTI)

    Yoshida, Mariko; Hiromoto, Takeshi; Hosokawa, Keiichi; Yamaguchi, Hiroshi; Fujiwara, Shinsuke

    2007-10-19

    MobR from Comamonas testosteroni KH122-3s is a member of the MarR family of transcriptional regulators and functions as a repressor for the mobA gene that encodes a 3-hydroxybenzoate 4-hydroxylase. 3-Hydroxybenzoate binds to MobR as a ligand, resulting in an efficient induction of mobA. Various 3-hydroxybenzoate analogues were examined for their inducibilities using the mobA::lacZ transcriptional fusion system. {beta}-Galactosidase was induced by the addition of 2,3-dihydroxybenzoate or 3,5-dihydroxybenzoate besides 3-hydroxybenzoate, suggesting that the hydroxyl group at position 3 is critical in addition to the carboxyl group on the aromatic ring. A gel mobility-shift assay also showed that MobR was released from the target DNA in the presence of these compounds. Circular dichroism studies demonstrated that MobR adopted two conformational states corresponding to the 3-hydroxybenzoate-bound and unbound forms. Other ligands also induced the structural change as well; however, the tertiary structures of converted forms were different from those by 3-hydroxybenzoate.

  3. Environmental research brief: Pollution prevention assessment for a manufacturer of automotive lighting equipment and accessories

    SciTech Connect (OSTI)

    Fleischman, M.; Couch, B.; Handmaker, A.; Looby, G.P.

    1995-08-01

    The US Environmental Protection Agency (EPA) has funded a Pilot project to assist small and medium-size manufacture who want to minimize their generation of waste but who lac the expertise to do so. In an effort to assist these manufacturers Waste Minimization Assessment Centers (WMACs) we established at selected universities and procedures were adapted from the EPA Waste Minimization Opportunity Assessment Manual. The WMAC team at the University of Tennessee performed an assessment at a plant that manufactures outboard motors for water craft. Three basic subunits received from other manufacturing plants undergo primarily painting and assembly operations in order to produce the final product. The team`s report, detailing findings and recommendations, indicated that paint overspray waste and spent clean-up solvent are generated in large quantities and that significant cost savings could be achieved by installing robotic paint application equipment. This Research Brief was developed by the principal investigators and EPA`s National Risk Management Research Laboratory, Cincinnati, OH, to announce key findings of an ongoing research project that is fully documented in a separate report of the same title available from University City Science Center.

  4. POLARIZATION STRUCTURE IN THE CORE OF 1803+784: A SIGNATURE OF RECOLLIMATION SHOCKS?

    SciTech Connect (OSTI)

    Cawthorne, T. V.; Jorstad, S. G.; Marscher, A. P.

    2013-07-20

    The extragalactic radio source 1803+784 is a BL Lac object that shows rapid variability and strong linear polarization. Very long baseline interferometry observations reveal that the core possesses a distinctive structure in polarized intensity with two maxima on axis and two minima symmetrically placed on either side. The approximately radial pattern of electric field polarization rods is reminiscent of the results obtained earlier by Cawthorne for conical shocks, but, individually, these do not reproduce the main features of the polarized intensity images. In numerical simulations and experiments, these shocks occur in pairs and help to stabilize jets as they adjust to changes in environment. Here, the polarization resulting from such structures is investigated using an approximate, analytical approach, by making some simple assumptions about the nature of the flow between two such shock waves. For fairly small viewing angles, it is found that a reasonable representation of the core polarization of 1803+784 can be obtained. The similarity between the observed and model polarizations supports the view that the core structure in 1803+784 represents a recollimation shock, and that such shock waves may be responsible for the first disturbance and hence brightening of the quiescent flow in astrophysical jets.

  5. Discovery of Very High Energy Gamma Rays from PKS 1424+240 and Multiwavelength Constraints on its Redshift

    SciTech Connect (OSTI)

    Acciari, V.A.; Aliu, E.; Arlen, T.; Aune, T.; Bautista, M.; Beilicke, M. Benbow, W.; Bottcher, M.; Boltuch, D.; Bradbury, S.M.; Buckley, J.H.; Bugaev, V.; Byrum, K.; Cannon, A.; Cesarini, A.; Chow, Y.C.; Ciupik, L.; Cogan, P.; Cui, W.; Duke, C.; Falcone, A.; /more authors..

    2012-04-05

    We report the first detection of very-high-energy (VHE) gamma-ray emission above 140GeV from PKS 1424+240, a BL Lac object with an unknown redshift. The photon spectrum above 140GeV measured by VERITAS is well described by a power law with a photon index of 3.8 {+-}0.5{sub stat} {+-} 0.3{sub syst} and a flux normalization at 200 GeV of (5.1 {+-} 0.9{sub stat} {+-} 0.5{sub syst}) x 10{sup -11} TeV{sup -1} cm{sup -2} s{sup -1}, where stat and syst denote the statistical and systematical uncertainty, respectively. The VHE flux is steady over the observation period between MJD 54881 and 55003 (2009 February 19 to June 21). Flux variability is also not observed in contemporaneous high energy observations with the Fermi Large Area Telescope (LAT). Contemporaneous X-ray and optical data were also obtained from the Swift XRT and MDM observatory, respectively. The broadband spectral energy distribution (SED) is well described by a one-zone synchrotron self-Compton (SSC) model favoring a redshift of less than 0.1. Using the photon index measured with Fermi in combination with recent extragalactic background light (EBL) absorption models it can be concluded from the VERITAS data that the redshift of PKS 1424+240 is less than 0.66.

  6. THE WISE BLAZAR-LIKE RADIO-LOUD SOURCES: AN ALL-SKY CATALOG OF CANDIDATE γ-RAY BLAZARS

    SciTech Connect (OSTI)

    D'Abrusco, R.; Paggi, A.; Smith, H. A.; Massaro, F.; Masetti, N.

    2014-11-01

    We present a catalog of radio-loud candidate γ-ray emitting blazars with WISE mid-infrared colors similar to the colors of confirmed γ-ray blazars. The catalog is assembled from WISE sources detected in all four WISE filters, with colors compatible with the three-dimensional locus of the WISE γ-ray emitting blazars, and which can be spatially cross-matched with radio sources from one of the three radio surveys: NVSS, FIRST, and/or SUMSS. Our initial WISE selection uses a slightly modified version of previously successful algorithms. We then select only the radio-loud sources using a measure of the radio-to-IR flux, the q {sub 22} parameter, which is analogous to the q {sub 24} parameter known in the literature but which instead uses the WISE band-four flux at 22 μm. Our final catalog contains 7855 sources classified as BL Lacs, FSRQs, or mixed candidate blazars; 1295 of these sources can be spatially re-associated as confirmed blazars. We describe the properties of the final catalog of WISE blazar-like radio-loud sources and consider possible contaminants. Finally, we discuss why this large catalog of candidate γ-ray emitting blazars represents a new and useful resource to address the problem of finding low-energy counterparts to currently unidentified high-energy sources.

  7. The 1991-2012 light curve of the old nova HR Lyrae

    SciTech Connect (OSTI)

    Honeycutt, R. K.; Shears, J.; Kafka, S.; Robertson, J. W.; Henden, A. A. E-mail: bunburyobservatory@hotmail.com E-mail: Jeff.Robertson@atu.edu

    2014-05-01

    The 22 yr light curve of HR Lyr, acquired with a typical cadence of 2-6 days, is examined for periodic and quasi-periodic variations. No persistent periodicities are revealed. Rather, the light curve variations often take the form of nearly linear rises and falls having typical e-folding times of about 100 days. Occasional ?0.6 mag outbursts are also seen, with properties similar to those of small outbursts found in some nova-like cataclysmic variables. When the photometry is formed into yearly averages, a decline of 0.012 0.005 mag yr{sup 1} is apparent, consistent with the fading of irradiation-induced M-dot following the nova. The equivalent width of H? is tabulated at three epochs over the interval 1986-2008 in order to compare with a recent result for DK Lac in which H? was found to be fading 50 yr after the nova. However, our results for such a fading in HR Lyr are inconclusive.

  8. ON THE REDSHIFT OF THE VERY HIGH ENERGY BLAZAR 3C 66A

    SciTech Connect (OSTI)

    Furniss, A.; Williams, D. A. [Santa Cruz Institute of Particle Physics and Department of Physics, University of California Santa Cruz, 1156 High Street, Santa Cruz, CA 95064 (United States)] [Santa Cruz Institute of Particle Physics and Department of Physics, University of California Santa Cruz, 1156 High Street, Santa Cruz, CA 95064 (United States); Fumagalli, M. [Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101 (United States)] [Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Danforth, C. [CASA, Department of Astrophysical and Planetary Sciences, University of Colorado, 389-UCB, Boulder, CO 80309 (United States)] [CASA, Department of Astrophysical and Planetary Sciences, University of Colorado, 389-UCB, Boulder, CO 80309 (United States); Prochaska, J. X. [Department of Astronomy and Astrophysics, UCO/Lick Observatory, University of California, 1156 High Street, Santa Cruz, CA 95064 (United States)] [Department of Astronomy and Astrophysics, UCO/Lick Observatory, University of California, 1156 High Street, Santa Cruz, CA 95064 (United States)

    2013-03-20

    As a bright gamma-ray source, 3C 66A is of great interest to the high-energy astrophysics community, having a potential for placing cosmological constraints on models for the extragalactic background light (EBL) and the processes which contribute to this photon field. No firm spectroscopic redshift measurement has been possible for this blazar due to a lack of intrinsic emission and absorption features in optical spectra. We present new far-ultraviolet spectra from the Hubble Space Telescope/Cosmic Origins Spectrograph (HST/COS) of the BL Lac object 3C 66A covering the wavelength range 1132-1800 A. The data show a smooth continuum with intergalactic medium absorption features which can be used to place a firm lower limit on the blazar redshift of z {>=} 0.3347. An upper limit is set by statistically treating the non-detection of additional absorbers beyond z = 0.3347, indicating a redshift of less than 0.41 at 99% confidence and ruling out z {>=} 0.444 at 99.9% confidence. We conclude by showing how the redshift limits derived from the COS spectra remove the potential for this gamma-ray emitting blazar to place an upper limit on the flux of the EBL using high energy data from a flare in 2009 October.

  9. Detection of phenols using engineered bacteria

    DOE Patents [OSTI]

    Wise, Arlene A.; Kuske, Cheryl R.; Terwilliger, Thomas C.

    2004-08-10

    Detection of phenols using engineered bacteria. A biosensor can be created by placing a reporter gene under control of an inducible promoter. The reporter gene produces a signal when a cognate transcriptional activator senses the inducing chemical. Creation of bacterial biosensors is currently restricted by limited knowledge of the genetic systems of bacteria that catabolize xenobiotics. By using mutagenic PCR to change the chemical specificity of the Pseudomonas species CF600 DmpR protein, the potential for engineering novel biosensors for detection of phenols has been demonstrated. DmpR, a well-characterized transcriptional activator of the P. CF600's dmp operon mediates growth on simple phenols. Transcription from Po, the promoter heading the dmp operon, is activated when the sensor domain of DmpR interacts with phenol and mono-substituted phenols. By altering the sensor domain of the DmpR, a group of DmpR derivatives that activate transcription of a Po-lacZ fusion in response to eight of the EPA's eleven priority pollutant phenols has been created. The assays and the sensor domain mutations that alter the chemical specificity of DmpR is described.

  10. Environmental research brief: Pollution prevention assessment for a manufacturer of components for outboard motors

    SciTech Connect (OSTI)

    Jendrucko, R.J.; Coleman, T.N.; Looby, G.P.

    1995-08-01

    The US Environmental Protection Agency (EPA) has funded a Pilot project to assist small and medium-size manufacture who want to minimize their generation of waste but who lac the expertise to do so. In an effort to assist these manufacturers Waste Minimization Assessment Centers (WMACs) we established at selected universities and procedures were adapted from the EPA Waste Minimization Opportunity Assessment Manual. The WMAC team at the University of Tennessee performed an assessment at a plant that manufactures outboard motors for water craft. Three basic subunits received from other manufacturing plants undergo primarily painting and assembly operations in order to produce the final product. The team`s report, detailing findings and recommendations, indicated that paint overspray waste and spent clean-up solvent are generated in large quantities and that significant cost savings could be achieved by installing robotic paint application equipment. This Research Brief was developed by the principal investigators and EPA`s National Risk Management Research Laboratory, Cincinnati, OH, to announce key findings of an ongoing research project that is fully documented in a separate report of the same title available from University City Science Center.

  11. Plasmids encoding therapeutic agents

    DOE Patents [OSTI]

    Keener, William K.

    2007-08-07

    Plasmids encoding anti-HIV and anti-anthrax therapeutic agents are disclosed. Plasmid pWKK-500 encodes a fusion protein containing DP178 as a targeting moiety, the ricin A chain, an HIV protease cleavable linker, and a truncated ricin B chain. N-terminal extensions of the fusion protein include the maltose binding protein and a Factor Xa protease site. C-terminal extensions include a hydrophobic linker, an L domain motif peptide, a KDEL ER retention signal, another Factor Xa protease site, an out-of-frame buforin II coding sequence, the lacZ.alpha. peptide, and a polyhistidine tag. More than twenty derivatives of plasmid pWKK-500 are described. Plasmids pWKK-700 and pWKK-800 are similar to pWKK-500 wherein the DP178-encoding sequence is substituted by RANTES- and SDF-1-encoding sequences, respectively. Plasmid pWKK-900 is similar to pWKK-500 wherein the HIV protease cleavable linker is substituted by a lethal factor (LF) peptide-cleavable linker.

  12. La supraconductivité a 100 ans !

    ScienceCinema (OSTI)

    None

    2011-10-06

    Il y a 100 ans, le 8 avril 1911, une découverte majeure était réalisée : celle de la supraconductivité. La supraconductivité est la caractéristique qu?ont certains métaux et alliages de perdre toute résistance électrique en dessous d?une température donnée. Cette renversante découverte, réalisée de manière presque fortuite par Kammerlingh Onnes de l?Université de Leyde (Pays-Bas) et son étudiant Gilles Holst, a ouvert un nouveau champ de recherche en physique et de fabuleuses perspectives d?applications technologiques. Du point de vue scientifique, la supraconductivité est en effet l?une des rares manifestations de la physique quantique à l?échelle macroscopique.  Du point de vue des retombées techniques, elle est porteuse d?applications majeures dans le domaine de la santé, des communications et de l?énergie. 100 ans après, les physiciens n?ont toujours pas fini d?explorer ce phénomène et ses applications. Le CERN abrite des applications de la supraconductivité à des échelles inédites. L?accélérateur de particules LHC, avec ses milliers d?aimants supraconducteurs répartis sur 27 kilomètres de circonférence, est en effet la plus grande application mondiale de la supraconductivité. Il ne pourrait exister sans elle.  Le CERN fête donc la découverte de la supraconductivité avec une conférence exceptionnelle donnée par Philippe Lebrun. Au cours de cette conférence, l?expérience historique de Kammerlingh Onnes sera reproduite. Philippe Lebrun racontera l?histoire de cette étonnante découverte, en la replaçant dans le contexte scientifique de l?époque. Il racontera les développements scientifiques et les applications du premier siècle de la supraconductivité. Conférence en français Merci de bien vouloir vous inscrire au : +41 22 767 76 76 ou cern.reception@cern.ch

  13. No Galaxy Left Behind: Accurate Measurements with the Faintest Objects in the Dark Energy Survey

    SciTech Connect (OSTI)

    Suchyta, E.

    2015-07-29

    Accurate statistical measurement with large imaging surveys has traditionally required throwing away a sizable fraction of the data. This is because most measurements have have relied on selecting nearly complete samples, where variations in the composition of the galaxy population with seeing, depth, or other survey characteristics are small. We introduce a new measurement method that aims to minimize this wastage, allowing precision measurement for any class of stars or galaxies detectable in an imaging survey. We have implemented our proposal in Balrog, a software package which embeds fake objects in real imaging in order to accurately characterize measurement biases. We also demonstrate this technique with an angular clustering measurement using Dark Energy Survey (DES) data. We first show that recovery of our injected galaxies depends on a wide variety of survey characteristics in the same way as the real data. We then construct a flux-limited sample of the faintest galaxies in DES, chosen specifically for their sensitivity to depth and seeing variations. Using the synthetic galaxies as randoms in the standard LandySzalay correlation function estimator suppresses the effects of variable survey selection by at least two orders of magnitude. Now our measured angular clustering is found to be in excellent agreement with that of a matched sample drawn from much deeper, higherresolution space-based COSMOS imaging; over angular scales of 0.004 < ? < 0.2 , we find a best-fit scaling amplitude between the DES and COSMOS measurements of 1.00 0.09. We expect this methodology to be broadly useful for extending the statistical reach of measurements in a wide variety of coming imaging surveys.

  14. Atmospheric Dispersion Effects in Weak Lensing Measurements

    SciTech Connect (OSTI)

    Plazas, Andrs Alejandro; Bernstein, Gary

    2012-10-01

    The wavelength dependence of atmospheric refraction causes elongation of finite-bandwidth images along the elevation vector, which produces spurious signals in weak gravitational lensing shear measurements unless this atmospheric dispersion is calibrated and removed to high precision. Because astrometric solutions and PSF characteristics are typically calibrated from stellar images, differences between the reference stars' spectra and the galaxies' spectra will leave residual errors in both the astrometric positions (dr) and in the second moment (width) of the wavelength-averaged PSF (dv) for galaxies.We estimate the level of dv that will induce spurious weak lensing signals in PSF-corrected galaxy shapes that exceed the statistical errors of the DES and the LSST cosmic-shear experiments. We also estimate the dr signals that will produce unacceptable spurious distortions after stacking of exposures taken at different airmasses and hour angles. We also calculate the errors in the griz bands, and find that dispersion systematics, uncorrected, are up to 6 and 2 times larger in g and r bands,respectively, than the requirements for the DES error budget, but can be safely ignored in i and z bands. For the LSST requirements, the factors are about 30, 10, and 3 in g, r, and i bands,respectively. We find that a simple correction linear in galaxy color is accurate enough to reduce dispersion shear systematics to insignificant levels in the r band for DES and i band for LSST,but still as much as 5 times than the requirements for LSST r-band observations. More complex corrections will likely be able to reduce the systematic cosmic-shear errors below statistical errors for LSST r band. But g-band effects remain large enough that it seems likely that induced systematics will dominate the statistical errors of both surveys, and cosmic-shear measurements should rely on the redder bands.

  15. Atmospheric Dispersion Effects in Weak Lensing Measurements

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Plazas, Andrés Alejandro; Bernstein, Gary

    2012-10-01

    The wavelength dependence of atmospheric refraction causes elongation of finite-bandwidth images along the elevation vector, which produces spurious signals in weak gravitational lensing shear measurements unless this atmospheric dispersion is calibrated and removed to high precision. Because astrometric solutions and PSF characteristics are typically calibrated from stellar images, differences between the reference stars' spectra and the galaxies' spectra will leave residual errors in both the astrometric positions (dr) and in the second moment (width) of the wavelength-averaged PSF (dv) for galaxies.We estimate the level of dv that will induce spurious weak lensing signals in PSF-corrected galaxy shapes that exceed themore »statistical errors of the DES and the LSST cosmic-shear experiments. We also estimate the dr signals that will produce unacceptable spurious distortions after stacking of exposures taken at different airmasses and hour angles. We also calculate the errors in the griz bands, and find that dispersion systematics, uncorrected, are up to 6 and 2 times larger in g and r bands,respectively, than the requirements for the DES error budget, but can be safely ignored in i and z bands. For the LSST requirements, the factors are about 30, 10, and 3 in g, r, and i bands,respectively. We find that a simple correction linear in galaxy color is accurate enough to reduce dispersion shear systematics to insignificant levels in the r band for DES and i band for LSST,but still as much as 5 times than the requirements for LSST r-band observations. More complex corrections will likely be able to reduce the systematic cosmic-shear errors below statistical errors for LSST r band. But g-band effects remain large enough that it seems likely that induced systematics will dominate the statistical errors of both surveys, and cosmic-shear measurements should rely on the redder bands.« less

  16. F.S.V.B. Volleyball

    ScienceCinema (OSTI)

    None

    2011-04-25

    22me assemblée des délégués de la Fédération Suisse de Volley Ball (F.S.V.B.), en présence entre autres de Claude Delay, représentant de la société fédérale de gymnastique et Hans Gauer, représentant de l'association suisse de gymnastique féminine. Annonce d'une démonstration d'un mini match de volley ball à Meyrin dans l'après-midi.

  17. Isolated spinach ribulose-1,5-bisphosphate carboxylase/oxgenase large subunit .epsilon. n-methyltransferase and method of inactivating ribulose-1,5-bishosphatase .epsilon. n-methyltransferase activity

    DOE Patents [OSTI]

    Houtz, Robert L. (Lexington, KY)

    2001-01-01

    The gene sequence for ribulose-1,5-bisphosphate carboxylase/oxygenase (Rubisco) large subunit (LS) .sup..epsilon. N-methyltansferase (protein methylase III or Rubisco LSMT) from a plant which has a des(methyl) lysyl residue in the LS is disclosed. In addition, the full-length cDNA clones for Rubisco LSMT are disclosed. Transgenic plants and methods of producing same which have the Rubisco LSMT gene inserted into the DNA are also provided. Further, methods of inactivating the enzymatic activity of Rubisco LSMT are also disclosed.

  18. Isolated spinach ribulose-1,5-bisphosphate carboxylase/oxygenase large subunit .sup..epsilon. N-methyltransferase and method of inactivating ribulose-1,5-bisphosphatase carboxylase/oxygenase large subunit .sup..epsilon. N-methyltransferase activity

    DOE Patents [OSTI]

    Houtz, Robert L. (Lexington, KY)

    1999-01-01

    The gene sequence for ribulose-1,5-bisphosphate carboxylase/oxygenase (Rubisco) large subunit (LS) .sup..epsilon. N-methyltransferase (protein methylase III or Rubisco LSMT) from a plant which has a des(methyl) lysyl residue in the LS is disclosed. In addition, the full-length cDNA clones for Rubisco LSMT are disclosed. Transgenic plants and methods of producing same which have the Rubisco LSMT gene inserted into the DNA are also provided. Further, methods of inactivating the enzymatic activity of Rubisco LSMT are also disclosed.

  19. Memorial V.J.Glaser

    ScienceCinema (OSTI)

    None

    2011-04-25

    Plusieurs orateurs rendent hommage au grand physicien et scientifique Vladimir Jurko Glaser (1924 - 1984) qui travaillait au Ruder Boscovic Institut à Zagreb avant de venir au Cern en 1957 où il trouvait un poste permanent au département de physique théorique. Walter Tearing, Harry Lehmann,Henry Epstein, Jacques Bros et André Martin font des résumés biographiques de leurs collègue et ami en honorant ses grands qualités d'homme et ses remarquables conquêtes de la science et leurs accomplissement.

  20. American Socient of Safety Engineers offers Ergonomic Tips for Businesses, Home

    Broader source: Energy.gov [DOE]

    DES PLAINES, IL (March 28, 2002) - With workplace musculoskeletal disorders (MSDs) being the single largest occupational safety and health problem in the U.S. according to the National Institute of Occupational Safety and Health, the American Society of Safety Engineers (ASSE) urges employers to develop and implement now an effective ergonomic system to reduce those injuries. An initial investment in ergonomic programs removes barriers to quality, productivity and human performance by fitting products, tasks, and environments to people and in the long run will save millions later.

  1. 2015HSSB Resultsbracket

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    13 21 3 4 14 5 6 15 22 7 8 16 27 9 10 11 12 L 15 23 L 16 18 L 13 19 L 14 20 24 17 L 21 25 L 22 26 28 L 27 29 30 CHAMPIONSHIP Champion ______________________ Runner-up _______________________ Third Place ____________________________ Fourth Place ___________________________ Challenger Bracket Undefeated Bracket Science Bowl 2016 Double Elimination Competition Central Lee #2 Prince of Peace (withdrew) Valley 94 Ames 50 Grinnell 52 Shenandoah 26 Des Moines Central 78 Lynnville-Sully 8 Boyer Valley

  2. Comparative study of microwave radiation-induced magnetoresistive oscillations induced by circularly- and linearly- polarized photo-excitation

    SciTech Connect (OSTI)

    Ye, Tianyu; Liu, Han -Chun; Wang, Zhuo; Wegscheider, W.; Mani, Ramesh G.

    2015-10-09

    A comparative study of the radiation-induced magnetoresistance oscillations in the high mobility GaAs/AlGaAs heterostructure two dimensional electron system (2DES) under linearly- and circularly- polarized microwave excitation indicates a profound difference in the response observed upon rotating the microwave launcher for the two cases, although circularly polarized microwave radiation induced magnetoresistance oscillations observed at low magnetic fields are similar to the oscillations observed with linearly polarized radiation. For the linearly polarized radiation, the magnetoresistive response is a strong sinusoidal function of the launcher rotation (or linear polarization) angle, θ. As a result, for circularly polarized radiation, the oscillatory magnetoresistive response is hardly sensitive to θ.

  3. ESMC

    ScienceCinema (OSTI)

    None

    2011-04-25

    Workshops de 2 jours au Cern: 1.partie: communication scientifique: plusieurs discours suivis de questions et intenses discussions: 1.François de Closet "le progrès scientifique" 2.Gerhard Moosleiter(?) exposé avec dias et questions 3.H.Meyers "comment créer de meilleures conditions en communication scientifique 2.partie: science et communication :présentation des dias et questions. Une Russe de Moscou parle entre autre de la situation actuelle de la presse scientifique en Russie 3.partie: conclusions et rapports de la veille de differents groupes de travail 4.partie:questions avec C.Rubbia et N.Calder et remerciements

  4. Browse by Discipline -- E-print Network Subject Pathways: Energy Storage,

    Office of Scientific and Technical Information (OSTI)

    Conversion and Utilization -- Energy, science, and technology for the research community -- hosted by the Office of Scientific and Technical Information, U.S. Department of Energy D E F G H I J K L M N O P Q R S T U V W X Y Z Cacciani, Patrice (Patrice Cacciani) - Laboratoire de Physique des Lasers Atomes et Molécules & Centre de Recherches Lasers et Applications, Cahill, Kevin (Kevin Cahill) - Department of Physics and Astronomy, University of New Mexico Caldarelli, Guido (Guido

  5. How to Find Ames Laboratory | The Ames Laboratory

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    How to Find Ames Laboratory Finding the Ames Laboratory The Ames Laboratory has it's main administrative offices in the Technical and Administrative Services Facility (TASF) building on the Iowa State University Campus. For directions, please use the GPS coordinates 42.0305° N, 93.6482° W. For directions from the Des Moines Airport please use the link with the following directions: https://goo.gl/maps/c6SOK Finding the Ames Laboratory on the ISU Campus Image Click on the map to download a

  6. L'Aventure du LHC

    ScienceCinema (OSTI)

    None

    2011-10-06

    Cette présentation s?adressera principalement aux personnes qui ont construit le LHC. La construction du LHC fut longue et difficile. De nombreux problèmes sont apparus en cours de route. Tous ont été résolus grâce au dévouement et à l?engagement du personnel et des collaborateurs. Je reviendrai sur les coups durs et les réussites qui ont marqués ces 15 dernières années et je vous montrerai combien cette machine, le fruit de vos efforts, est extraordinaire.

  7. Browse by Discipline -- E-print Network Subject Pathways: Materials Science

    Office of Scientific and Technical Information (OSTI)

    -- Energy, science, and technology for the research community -- hosted by the Office of Scientific and Technical Information, U.S. Department of Energy L M N O P Q R S T U V W X Y Z Kaâniche, Mohamed (Mohamed Kaâniche) - Laboratoire d'Analyse et d'Architecture des Systèmes du CNRS Kaasbøll, Jens (Jens Kaasbøll) - Institutt for Informatikk, Universitetet i Oslo Kabal, Peter (Peter Kabal) - Department of Electrical and Computer Engineering, McGill University Kaban, Ata (Ata Kaban) -

  8. Browse by Discipline -- E-print Network Subject Pathways: Physics --

    Office of Scientific and Technical Information (OSTI)

    Energy, science, and technology for the research community -- hosted by the Office of Scientific and Technical Information, U.S. Department of Energy L M N O P Q R S T U V W X Y Z Kaajakari, Ville (Ville Kaajakari) - VTT Information Technology Kaâniche, Mohamed (Mohamed Kaâniche) - Laboratoire d'Analyse et d'Architecture des Systèmes du CNRS Kaber, David B. (David B. Kaber) - Department of Industrial and Systems Engineering, North Carolina State University Kachroo, Pushkin (Pushkin

  9. Production of Renewable Fuels from Biomass by FCC

    Office of Energy Efficiency and Renewable Energy (EERE) Indexed Site

    Production of Renewable Fuels from Biomass by FCC Co-processing Biomass 2014 July 30, 2014 Washington, DC © 2014 UOP LLC. All rights reserved. UOP 5354-01 Raymond G. Wissinger UOP LLC Des Plaines, IL Presentation Outline  Background on UOP  Overview of FCC Co-processing  Implementation and Future Plans  Q&A Who is UOP? Honeywell UOP creates knowledge via invention and innovation and applies it to the energy industry Petroleum Petrochemicals Natural Gas  1,570 scientists and

  10. Eia.gov BETA - Analysis & Projections - U.S. Energy Information

    U.S. Energy Information Administration (EIA) Indexed Site

    Administration (EIA) Définitions reliés aux cartes English FranÇais Español A B C D E É F G H I J K L M N O P Q R S T U V W X Y Z Parcourir les termes liés aux catégories suivantes: électricité franchissant une frontière gaz franchissant une frontière liquide franchissant une frontière terminaux méthaniers usines de traitement du gaz naturel centrales électriques raffineries Consultez l'index des termes

  11. Los Alamos National Laboratory * Est. 1943 The Pulse-Newsletter of the Los Alamos Neutron Science Center and Accelerator Operations and Technology Division

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    1 Los Alamos National Laboratory * Est. 1943 The Pulse-Newsletter of the Los Alamos Neutron Science Center and Accelerator Operations and Technology Division I N S I D E 2 From Alex's Desk 3 lujAn Center reseArCh FeAtureD on Cover oF Langmuir 4 FunCtionAl oxiDes unDer extreme ConDi- tions-quest For new mAteriAls 6 heADs uP! By Diana Del Mauro ADEPS Communications Inside the Lujan Neutron Scattering Center, Victor Fanelli is busy preparing a superconducting magnet. In a series of delicate steps,

  12. Tuning the Formations of Metal-Organic Frameworks by Modification of

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Ratio of Reactant, Acidity of Reaction System, and Use of a Secondary Ligand | Center for Gas SeparationsRelevant to Clean Energy Technologies | Blandine Jerome Tuning the Formations of Metal-Organic Frameworks by Modification of Ratio of Reactant, Acidity of Reaction System, and Use of a Secondary Ligand Previous Next List Qian Gao, Ya-Bo Xie, Jian-Rong Li, Da-Qiang Yuan, Audrey A. Yakovenko, Ji-Hong Sun, and Hong-Cai Zhou, Cryst. Growth Des., 2012, 12 (1), pp 281-288 DOI: 10.1021/cg201059d

  13. Open University

    ScienceCinema (OSTI)

    None

    2011-04-25

    Michel Pentz est née en Afrique du Sud et venu au Cern en 1957 comme physicien et président de l'associaion du personnel. Il est également fondateur du mouvement Antiapartheid de Genève et a participé à la fondation de l'Open University en Grande-Bretagne. Il nous parle des contextes pédagogiques, culturels et nationaux dans lesquels la méthode peut s'appliquer.

  14. Ceremony 25th birthday Cern

    ScienceCinema (OSTI)

    None

    2011-04-25

    Célébration du 25ème anniversaire du Cern (jour par jour) avec discours de L.Van Hove et J.B.Adams, des interludes musicals offerts par Mme Mey et ses collègues (au debut 1.mouvement du quatuor avec piano no 3 de L.van Beethoven) Les directeurs généraux procéderont à la remise du souvenir aux membres de personnel ayant 25 années de service dans l'organisation. Un témoignage de reconnaissance est auss fait à l'interprète Mme Zwerner

  15. Quality Control Inspector: Different Programs, Different Responosibilities

    Energy Savers [EERE]

    Quality Control Inspector: Different Programs, Different ResponsibiliDes. A Guide to the JTA So& Skills. Inspects implementaDon of the program. þ þ Documents areas needing improvement in report. þ þ May assure homeowners/clients of follow---up work. ý þ Independent 3 rd party inspectors may be hired by an enDty not in a role to promise follow---up to clients or residents. Agency staff can and should assure clients of proper follow---up when appropriate. May address

  16. HA' R$,kAW CH EM I CAL CO,M i=ANY A

    Office of Legacy Management (LM)

    TH Ii ' HA' R$,kAW CH EM I CAL CO,M i=ANY A December 30, 1955 U. S. Atomic Energy Commission Oak Ridge OperationwOfflce Post Office Box "E" Oak Ridge, Tennessee Attention: Mr. T. Carberry Dear Mr. Carberry: ' ..> In the process of removing 'classified documents from the safes at the Main Office for des$ruction we discovered two sample cylinders of hexafluorlde. If memory serves us right these sample6 were prepared at the request of the Commission and shipped to the Unl- versity of

  17. Microsoft Word - SDS SRP 4 14 2014.docx

    Office of Environmental Management (EM)

    Str rengthe Fede S ening L eral Mo Stand Safet Line Ma onitorin dard ty Des Apr i anagem g of Nu Revi sign S ril 2014 ment O uclear ew P Strate Oversig Facilitie Plan egy ht and es CD-0 OFF C FICE OF E S S C CD-1 ENVIRON Standard afety De ritical Decisi CD-2 A ii NMENTA d Review esign St ion (CD) App CD April 2014 AL MANA w Plan trategy plicability D-3 AGEMENT CD-4 T Post Operation iii FOREWORD The Chief of Nuclear Safety (CNS) is developing of series of Standard Review Plans (SRPs) to provide

  18. First NuSTAR Observations of Mrk 501 within a Radio to TeV Multi-Instrument Campaign

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Furniss, Amy

    2015-10-08

    We report on simultaneous broadband observations of the TeV-emitting blazar Markarian 501 between 2013 April 1 and August 10, including the first detailed characterization of the synchrotron peak with Swift and NuSTAR. During the campaign, the nearby BL Lac object was observed in both a quiescent and an elevated state. The broadband campaign includes observations with NuSTAR, MAGIC, VERITAS, the Fermi Large Area Telescope, Swift X-ray Telescope and UV Optical Telescope, various ground-based optical instruments, including the GASP-WEBT program, as well as radio observations by OVRO, Metshovi, and the F-Gamma consortium. Some of the MAGIC observations were affected by amoresand layer from the Saharan desert, and had to be corrected using event-by-event corrections derived with a Light Detection and Ranging (LIDAR) facility. This is the first time that LIDAR information is used to produce a physics result with Cherenkov Telescope data taken during adverse atmospheric conditions, and hence sets a precedent for the current and future ground-based gamma-ray instruments. The NuSTAR instrument provides unprecedented sensitivity in hard X-rays, showing the source to display a spectral energy distribution (SED) between 3 and 79 keV consistent with a log-parabolic spectrum and hard X-ray variability on hour timescales. None (of the four extended NuSTAR observations) show evidence of the onset of inverse-Compton emission at hard X-ray energies. We apply a single-zone equilibrium synchrotron self-Compton (SSC) model to five simultaneous broadband SEDs. We find that the SSC model can reproduce the observed broadband states through a decrease in the magnetic field strength coinciding with an increase in the luminosity and hardness of the relativistic leptons responsible for the high-energy emission.less

  19. TEMPORAL CORRELATIONS BETWEEN OPTICAL AND GAMMA-RAY ACTIVITY IN BLAZARS

    SciTech Connect (OSTI)

    Cohen, Daniel P.; Filippenko, Alexei V.; Zheng, WeiKang; Li, Weidong; Romani, Roger W.; Cenko, S. Bradley

    2014-12-20

    We have been using the 0.76m Katzman Automatic Imaging Telescope (KAIT) at Lick Observatory to optically monitor a sample of 157 blazars that are bright in gamma-rays being detected with high significance (?10?) in one year by the Large Area Telescope (LAT) on the Fermi Gamma-ray Space Telescope. We attempt to observe each source on a three-day cadence with KAIT, subject to weather and seasonal visibility. The gamma-ray coverage is essentially continuous. KAIT observations extend over much of the five-year Fermi mission for several objects, and most have >100 optical measurements spanning the last three years. These blazars (flat-spectrum radio quasars and BL Lac objects) exhibit a wide range of flaring behavior. Using the discrete correlation function (DCF), here we search for temporal relationships between optical and gamma-ray light curves in the 40 brightest sources in hopes of placing constraints on blazar acceleration and emission zones. We find strong optical-gamma-ray correlation in many of these sources at time delays of ?1 to ?10days, ranging between 40 and +30days. A stacked average DCF of the 40 sources verifies this correlation trend, with a peak above 99% significance indicating a characteristic time delay consistent with 0days. These findings strongly support the widely accepted leptonic models of blazar emission. However, we also find examples of apparently uncorrelated flares (optical flares with no gamma-ray counterpart and gamma-ray flares with no optical counterpart) that challenge simple, one-zone models of blazar emission. Moreover, we find that flat-spectrum radio quasars tend to have gamma-rays leading the optical, while intermediate- and high-synchrotron peak blazars with the most significant peaks have smaller lags/leads. It is clear that long-term monitoring at high cadence is necessary to reveal the underlying physical correlation.

  20. The naphthalene catabolic (nag) genes of Polaromonas naphthalenivorans CJ2: Evolutionary implications for two gene clusters and novel regulatory control

    SciTech Connect (OSTI)

    Jeon, C.O.; Park, M.; Ro, H.S.; Park, W.; Madsen, E.L.

    2006-02-15

    Polaromonas naphthalenivorans CJ2, found to be responsible for the degradation of naphthalene in situ at a coal tar waste-contaminated site, is able to grow on mineral salts agar media with naphthalene as the sole carbon source. Beginning from a 484-bp nagAc-like region, we used a genome walking strategy to sequence genes encoding the entire naphthalene degradation pathway and additional flanking regions. We found that the naphthalene catabolic genes in P. naphthalenivorans CJ2 were divided into one large and one small gene cluster, separated by an unknown distance. The large gene cluster is bounded by a LysR-type regulator (nagR). The small cluster is bounded by a MarR-type regulator (nagR2). The catabolic genes of P. naphthalenivorans CJ2 were homologous to many of those of Ralstonia U2, which uses the gentisate pathway to convert naphthalene to central metabolites. However, three open reading frames (nagY, nagM, and nagN), present in Ralstonia U2, were absent. Also, P. naphthalenivorans carries two copies of gentisate dioxygenase (nagI) with 77.4% DNA sequence identity to one another and 82% amino acid identity to their homologue in Ralstonia sp. strain U2. Investigation of the operons using reverse transcription PCR showed that each cluster was controlled independently by its respective promoter. Insertional inactivation and lacZ reporter assays showed that nagR2 is a negative regulator and that expression of the small cluster is not induced by naphthalene, salicylate, or gentisate. Association of two putative Azoarcus-related transposases with the large cluster and one Azoarcus-related putative salicylate 5-hydroxylase gene (ORF2) in the small cluster suggests that mobile genetic elements were likely involved in creating the novel arrangement of catabolic and regulatory genes in P. naphthalenivorans.

  1. First-epoch VLBA imaging of 20 new TeV blazars

    SciTech Connect (OSTI)

    Piner, B. Glenn; Edwards, Philip G.

    2014-12-10

    We present Very Long Baseline Array (VLBA) images of 20 TeV blazars not previously well studied on the parsec scale. All 20 of these sources are high-frequency peaked BL Lac objects (HBLs). Observations were made between August and December of 2013 at a frequency of 8.4 GHz. These observations represent the first epoch of a VLBA monitoring campaign on these blazars, and they significantly increase the fraction of TeV HBLs studied with high-resolution imaging. The peak very long baseline interferometry (VLBI) flux densities of these sources range from ?10 to ?100 mJy bm{sup 1}, and parsec-scale jet structure is detected in all sources. About half of the VLBI cores are resolved, with brightness temperature upper limits of a few times 10{sup 10} K, and we find that a brightness temperature of ?2 10{sup 10} K is consistent with the VLBI data for all but one of the sources. Such brightness temperatures do not require any relativistic beaming to reduce the observed value below commonly invoked intrinsic limits; however, the lack of detection of counterjets does place a modest limit on the bulk Lorentz factor of ? ? 2. These data are thus consistent with a picture where weak-jet sources like the TeV HBLs develop significant velocity structures on parsec scales. We also extend consideration to the full sample of TeV HBLs by combining the new VLBI data with VLBI and gamma-ray data from the literature. By comparing measured VLBI and TeV fluxes to samples with intrinsically uncorrelated luminosities generated by Monte Carlo simulations, we find a marginally significant correlation between the VLBI and TeV fluxes for the full TeV HBL sample.

  2. Enhancing Complex System Performance Using Discrete-Event Simulation

    SciTech Connect (OSTI)

    Allgood, Glenn O; Olama, Mohammed M; Lake, Joe E

    2010-01-01

    In this paper, we utilize discrete-event simulation (DES) merged with human factors analysis to provide the venue within which the separation and deconfliction of the system/human operating principles can occur. A concrete example is presented to illustrate the performance enhancement gains for an aviation cargo flow and security inspection system achieved through the development and use of a process DES. The overall performance of the system is computed, analyzed, and optimized for the different system dynamics. Various performance measures are considered such as system capacity, residual capacity, and total number of pallets waiting for inspection in the queue. These metrics are performance indicators of the system's ability to service current needs and respond to additional requests. We studied and analyzed different scenarios by changing various model parameters such as the number of pieces per pallet ratio, number of inspectors and cargo handling personnel, number of forklifts, number and types of detection systems, inspection modality distribution, alarm rate, and cargo closeout time. The increased physical understanding resulting from execution of the queuing model utilizing these vetted performance measures identified effective ways to meet inspection requirements while maintaining or reducing overall operational cost and eliminating any shipping delays associated with any proposed changes in inspection requirements. With this understanding effective operational strategies can be developed to optimally use personnel while still maintaining plant efficiency, reducing process interruptions, and holding or reducing costs.

  3. Wide-field lensing mass maps from Dark Energy Survey science verification data: Methodology and detailed analysis

    SciTech Connect (OSTI)

    Vikram, V.

    2015-07-29

    Weak gravitational lensing allows one to reconstruct the spatial distribution of the projected mass density across the sky. These mass maps provide a powerful tool for studying cosmology as they probe both luminous and dark matter. In this paper, we present a weak lensing mass map reconstructed from shear measurements in a 139 deg2 area from the Dark Energy Survey (DES) science verification data. We compare the distribution of mass with that of the foreground distribution of galaxies and clusters. The overdensities in the reconstructed map correlate well with the distribution of optically detected clusters. We demonstrate that candidate superclusters and voids along the line of sight can be identified, exploiting the tight scatter of the cluster photometric redshifts. We cross-correlate the mass map with a foreground magnitude-limited galaxy sample from the same data. Our measurement gives results consistent with mock catalogs from N-body simulations that include the primary sources of statistical uncertainties in the galaxy, lensing, and photo-z catalogs. The statistical significance of the cross-correlation is at the 6.8? level with 20 arcminute smoothing. We find that the contribution of systematics to the lensing mass maps is generally within measurement uncertainties. In this study, we analyze less than 3% of the final area that will be mapped by the DES; the tools and analysis techniques developed in this paper can be applied to forthcoming larger data sets from the survey.

  4. Cooling the dark energy camera instrument

    SciTech Connect (OSTI)

    Schmitt, R.L.; Cease, H.; DePoy, D.; Diehl, H.T.; Estrada, J.; Flaugher, B.; Kuhlmann, S.; Onal, Birce; Stefanik, A.; /Fermilab

    2008-06-01

    DECam, camera for the Dark Energy Survey (DES), is undergoing general design and component testing. For an overview see DePoy, et al in these proceedings. For a description of the imager, see Cease, et al in these proceedings. The CCD instrument will be mounted at the prime focus of the CTIO Blanco 4m telescope. The instrument temperature will be 173K with a heat load of 113W. In similar applications, cooling CCD instruments at the prime focus has been accomplished by three general methods. Liquid nitrogen reservoirs have been constructed to operate in any orientation, pulse tube cryocoolers have been used when tilt angles are limited and Joule-Thompson or Stirling cryocoolers have been used with smaller heat loads. Gifford-MacMahon cooling has been used at the Cassegrain but not at the prime focus. For DES, the combined requirements of high heat load, temperature stability, low vibration, operation in any orientation, liquid nitrogen cost and limited space available led to the design of a pumped, closed loop, circulating nitrogen system. At zenith the instrument will be twelve meters above the pump/cryocooler station. This cooling system expected to have a 10,000 hour maintenance interval. This paper will describe the engineering basis including the thermal model, unbalanced forces, cooldown time, the single and two-phase flow model.

  5. The Dark Energy Survey Camera (DECam)

    SciTech Connect (OSTI)

    Diehl, H.Thomas; /Fermilab

    2011-09-09

    The Dark Energy Survey (DES) is a next generation optical survey aimed at understanding the expansion rate of the Universe using four complementary methods: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. To perform the survey, the DES Collaboration is building the Dark Energy Camera (DECam), a 3 square degree, 570 Megapixel CCD camera that will be mounted at the prime focus of the Blanco 4-meter telescope at the Cerro Tololo Inter-American Observatory. CCD production has finished, yielding roughly twice the required 62 2k x 4k detectors. The construction of DECam is nearly finished. Integration and commissioning on a 'telescope simulator' of the major hardware and software components, except for the optics, recently concluded at Fermilab. Final assembly of the optical corrector has started at University College, London. Some components have already been received at CTIO. 'First-light' will be sometime in 2012. This oral presentation concentrates on the technical challenges involved in building DECam (and how we overcame them), and the present status of the instrument.

  6. TIDAL INTERACTION AS THE ORIGIN OF EARLY-TYPE DWARF GALAXIES IN GROUP ENVIRONMENTS

    SciTech Connect (OSTI)

    Paudel, Sanjaya; Ree, Chang H.

    2014-11-20

    We present a sample of dwarf galaxies that suffer ongoing disruption by the tidal forces of nearby massive galaxies. By analyzing structural and stellar population properties using the archival imaging and spectroscopic data from the Sloan Digital Sky Survey (SDSS), we find that they are likely a ''smoking gun'' example of the formation through tidal stirring of early-type dwarf galaxies (dEs) in the galaxy group environment. The inner cores of these galaxies are fairly intact and the observed light profiles are well fit by the Srsic functions while the tidally stretched stellar halos are prominent in the outer parts. They are all located within a sky-projected distance of 50 kpc from the centers of the host galaxies and no dwarf galaxies have relative line-of-sight velocities larger than 205 km s{sup 1} to their hosts. We derive the Composite Stellar Population properties of these galaxies by fitting the SDSS optical spectra to a multiple-burst composite stellar population model. We find that these galaxies accumulate a significant fraction of stellar mass within the last 1 Gyr and contain a majority stellar population with an intermediate age of 2 to 4 Gyr. Based on this evidence, we argue that tidal stirring, particularly through the galaxy-galaxy interaction, might have an important role in the formation and evolution of dEs in the group environment where the influence of other gas stripping mechanism might be limited.

  7. Automated transient identification in the Dark Energy Survey

    SciTech Connect (OSTI)

    Goldstein, D. A.; D'Andrea, C. B.; Fischer, J. A.; Foley, R. J.; Gupta, R. R.; Kessler, R.; Kim, A. G.; Nichol, R. C.; Nungent, P.; Papadopoulos, A.; Sako, M.; Smith, M.; Sullivan, M.; Thomas, R. C.; Wester, W.; Wolf, R. C.; Abdalla, F. B.; Banjeri, M.; Benoit-Levy, A.; Bertin, E.; Brooks, D.; Rosell, A. Carnero; Castander, F. J.; da Costa, L. N.; Covarrubias, R.; DePoy, D. L.; Desai, S.; Diehl, H. T.; Doel, P.; Eifler, T. F.; Neto, A. Fausti; Finley, D. A.; Flaugher, B.; Fosalba, P.; Frieman, J.; Gerdes, D.; Gruen, D.; Gruendl, R. A.; James, D.; Kuehn, K.; Kuropatkin, N.; Lahav, O.; Li, T. S.; Maia, M. A. G.; Makler, M.; March, M.; Marshall, J. L.; Martini, P.; Merritt, K. W.; Miquel, R.; Nord, B.; Ogando, R.; Plazas, A. A.; Romer, A. K.; Roodman, A.; Sanchez, E.; Scarpine, V.; Schubnell, M.; Sevilla-Noarbe, I.; Smith, R. C.; Soares-Santos, M.; Sobreira, F.; Suchyta, E.; Swanson, M. E. C.; Tarle, G.; Thaler, J.; Walker, A. R.

    2015-09-01

    We describe an algorithm for identifying point-source transients and moving objects on reference-subtracted optical images containing artifacts of processing and instrumentation. The algorithm makes use of the supervised machine learning technique known as Random Forest. We present results from its use in the Dark Energy Survey Supernova program (DES-SN), where it was trained using a sample of 898,963 signal and background events generated by the transient detection pipeline. After reprocessing the data collected during the first DES-SN observing season (2013 September through 2014 February) using the algorithm, the number of transient candidates eligible for human scanning decreased by a factor of 13.4, while only 1.0% of the artificial Type Ia supernovae (SNe) injected into search images to monitor survey efficiency were lost, most of which were very faint events. Furthermore, we characterize the algorithm's performance in detail, and we discuss how it can inform pipeline design decisions for future time-domain imaging surveys, such as the Large Synoptic Survey Telescope and the Zwicky Transient Facility.

  8. Automated transient identification in the Dark Energy Survey

    SciTech Connect (OSTI)

    Goldstein, D. A.

    2015-08-20

    We describe an algorithm for identifying point-source transients and moving objects on reference-subtracted optical images containing artifacts of processing and instrumentation. The algorithm makes use of the supervised machine learning technique known as Random Forest. We present results from its use in the Dark Energy Survey Supernova program (DES-SN), where it was trained using a sample of 898,963 signal and background events generated by the transient detection pipeline. After reprocessing the data collected during the first DES-SN observing season (2013 September through 2014 February) using the algorithm, the number of transient candidates eligible for human scanning decreased by a factor of 13.4, while only 1.0 percent of the artificial Type Ia supernovae (SNe) injected into search images to monitor survey efficiency were lost, most of which were very faint events. Here we characterize the algorithm's performance in detail, and we discuss how it can inform pipeline design decisions for future time-domain imaging surveys, such as the Large Synoptic Survey Telescope and the Zwicky Transient Facility.

  9. Automated transient identification in the Dark Energy Survey

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Goldstein, D. A.; D'Andrea, C. B.; Fischer, J. A.; Foley, R. J.; Gupta, R. R.; Kessler, R.; Kim, A. G.; Nichol, R. C.; Nungent, P.; Papadopoulos, A.; et al

    2015-09-01

    We describe an algorithm for identifying point-source transients and moving objects on reference-subtracted optical images containing artifacts of processing and instrumentation. The algorithm makes use of the supervised machine learning technique known as Random Forest. We present results from its use in the Dark Energy Survey Supernova program (DES-SN), where it was trained using a sample of 898,963 signal and background events generated by the transient detection pipeline. After reprocessing the data collected during the first DES-SN observing season (2013 September through 2014 February) using the algorithm, the number of transient candidates eligible for human scanning decreased by a factormore » of 13.4, while only 1.0% of the artificial Type Ia supernovae (SNe) injected into search images to monitor survey efficiency were lost, most of which were very faint events. Furthermore, we characterize the algorithm's performance in detail, and we discuss how it can inform pipeline design decisions for future time-domain imaging surveys, such as the Large Synoptic Survey Telescope and the Zwicky Transient Facility.« less

  10. Influence of the support of CoMo sulfide catalysts and of the addition of potassium and platinum on the catalytic performances for the hydrodeoxygenation of carbonyl, carboxyl, and guaiacol-type molecules

    SciTech Connect (OSTI)

    Centeno, A.; Laurent, E.; Delmon, B. [Universite Catholique de Louvain, Louvain-la-Neuve (Belgium)] [Universite Catholique de Louvain, Louvain-la-Neuve (Belgium)

    1995-07-01

    The present work corresponds to part of a program aimed at upgrading oil obtained by pyrolysis of biomass by hydrotreatment (hydrodeoxygenation HDO). CoMo sulfide catalysts, nonsupported, supported on different supports (alumina, carbon, silica), or modified by K or Pt, were used. The authors used a model reacting mixture containing compounds representative of the molecules that must react to permit a primary stabilisation of the pyrolytic oil: 4-methy lacetophenone (4-MA), diethylsebacate (DES), and guaiacol (GUA). In the reaction of the carbonyl group of the 4-MA it is shown that no important role is played by any acid-base mechanism; dispersion determines the activity. Acidity of the support influences the formation of active sites for decarboxylation and hydrogenation of the carboxyl group of DES. It was confirmed that guaiacol-type molecules lead to coking reactions. The role of acidity in the mechanism of these reactions is confirmed, but the modifications made in the catalysts in this work are still not sufficient to control coke deposition. The catalysts supported on carbon lead to the direct elimination of the methoxyl group of the guaiacol. Carbon, on the whole, seems to be a promising support. This work suggests that appropriate modifications of the hydrotreating catalysts can lead to a more effective process for stabilisation of the bio-oils by reaction with hydrogen. 55 refs., 3 figs., 5 tabs.

  11. Discovery of a Stellar Overdensity in Eridanus-Phoenix in the Dark Energy Survey

    SciTech Connect (OSTI)

    Li, T.S.; et al.

    2015-09-14

    We report the discovery of an excess of main sequence turn-off stars in the direction of the constellations of Eridanus and Phoenix from the first year data of the Dark Energy Survey (DES). The Eridanus-Phoenix (EriPhe) overdensity is centered around l~285 deg and b~-60 deg and spans at least 30 deg in longitude and 10 deg in latitude. The Poisson significance of the detection is at least 9 sigma. The stellar population in the overdense region is similar in brightness and color to that of the nearby globular cluster NGC 1261, indicating that the heliocentric distance of EriPhe is about d~16 kpc. The extent of EriPhe in projection is therefore at least ~4 kpc by ~3 kpc. On the sky, this overdensity is located between NGC 1261 and a new stellar stream discovered by DES at a similar heliocentric distance, the so-called Phoenix Stream. Given their similar distance and proximity to each other, it is possible that these three structures may be kinematically associated. Alternatively, the EriPhe overdensity is morphologically similar to the Virgo overdensity and the Hercules-Aquila cloud, which also lie at a similar Galactocentric distance. These three overdensities lie along a polar plane separated by ~120 deg and may share a common origin. Spectroscopic follow-up observations of the stars in EriPhe are required to fully understand the nature of this overdensity.

  12. Eight new Milky Way companions discovered in first-year Dark Energy Survey data

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Bechtol, K.

    2015-06-30

    We report the discovery of eight new Milky Way companions inmore » $$\\sim 1800\\;{\\mathrm{deg}}^{2}$$ of optical imaging data collected during the first year of the Dark Energy Survey (DES). Each system is identified as a statistically significant over-density of individual stars consistent with the expected isochrone and luminosity function of an old and metal-poor stellar population. The objects span a wide range of absolute magnitudes (MV from $-2.2$ to $$-7.4\\;\\mathrm{mag}$$), physical sizes ($$10-170\\;\\mathrm{pc}$$), and heliocentric distances ($$30-330\\;\\mathrm{kpc}$$). Based on the low surface brightnesses, large physical sizes, and/or large Galactocentric distances of these objects, several are likely to be new ultra-faint satellite galaxies of the Milky Way and/or Magellanic Clouds. We introduce a likelihood-based algorithm to search for and characterize stellar over-densities, as well as identify stars with high satellite membership probabilities. As a result, we also present completeness estimates for detecting ultra-faint galaxies of varying luminosities, sizes, and heliocentric distances in the first-year DES data.« less

  13. Wide-field lensing mass maps from Dark Energy Survey science verification data: Methodology and detailed analysis

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Vikram, V.

    2015-07-29

    Weak gravitational lensing allows one to reconstruct the spatial distribution of the projected mass density across the sky. These “mass maps” provide a powerful tool for studying cosmology as they probe both luminous and dark matter. In this paper, we present a weak lensing mass map reconstructed from shear measurements in a 139 deg2 area from the Dark Energy Survey (DES) science verification data. We compare the distribution of mass with that of the foreground distribution of galaxies and clusters. The overdensities in the reconstructed map correlate well with the distribution of optically detected clusters. We demonstrate that candidate superclustersmore » and voids along the line of sight can be identified, exploiting the tight scatter of the cluster photometric redshifts. We cross-correlate the mass map with a foreground magnitude-limited galaxy sample from the same data. Our measurement gives results consistent with mock catalogs from N-body simulations that include the primary sources of statistical uncertainties in the galaxy, lensing, and photo-z catalogs. The statistical significance of the cross-correlation is at the 6.8σ level with 20 arcminute smoothing. We find that the contribution of systematics to the lensing mass maps is generally within measurement uncertainties. In this study, we analyze less than 3% of the final area that will be mapped by the DES; the tools and analysis techniques developed in this paper can be applied to forthcoming larger data sets from the survey.« less

  14. Discovery of a stellar overdensity in Eridanus-Phoenix in the dark energy survey

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Li, T. S.; Balbinot, E.; Mondrik, N.; Marshall, J. L.; Yanny, B.; Bechtol, K.; Drlica-Wagner, A.; Oscar, D.; Santiago, B.; Simon, J. D.; et al

    2016-01-27

    We report the discovery of an excess of main sequence turn-off stars in the direction of the constellations of Eridanus and Phoenix from the first year data of the Dark Energy Survey (DES). The Eridanus-Phoenix (EriPhe) overdensity is centered around l~285 deg and b~-60 deg and spans at least 30 deg in longitude and 10 deg in latitude. The Poisson significance of the detection is at least 9 sigma. The stellar population in the overdense region is similar in brightness and color to that of the nearby globular cluster NGC 1261, indicating that the heliocentric distance of EriPhe is aboutmore » d~16 kpc. The extent of EriPhe in projection is therefore at least ~4 kpc by ~3 kpc. On the sky, this overdensity is located between NGC 1261 and a new stellar stream discovered by DES at a similar heliocentric distance, the so-called Phoenix Stream. Given their similar distance and proximity to each other, it is possible that these three structures may be kinematically associated. Alternatively, the EriPhe overdensity is morphologically similar to the Virgo overdensity and the Hercules-Aquila cloud, which also lie at a similar Galactocentric distance. These three overdensities lie along a polar plane separated by ~120 deg and may share a common origin. Spectroscopic follow-up observations of the stars in EriPhe are required to fully understand the nature of this overdensity.« less

  15. Eight new Milky Way companions discovered in first-year Dark Energy Survey data

    SciTech Connect (OSTI)

    Bechtol, K.; et al.

    2015-06-30

    We report the discovery of eight new Milky Way companions in $\\sim 1800\\;{\\mathrm{deg}}^{2}$ of optical imaging data collected during the first year of the Dark Energy Survey (DES). Each system is identified as a statistically significant over-density of individual stars consistent with the expected isochrone and luminosity function of an old and metal-poor stellar population. The objects span a wide range of absolute magnitudes (MV from $-2.2$ to $-7.4\\;\\mathrm{mag}$), physical sizes ($10-170\\;\\mathrm{pc}$), and heliocentric distances ($30-330\\;\\mathrm{kpc}$). Based on the low surface brightnesses, large physical sizes, and/or large Galactocentric distances of these objects, several are likely to be new ultra-faint satellite galaxies of the Milky Way and/or Magellanic Clouds. We introduce a likelihood-based algorithm to search for and characterize stellar over-densities, as well as identify stars with high satellite membership probabilities. As a result, we also present completeness estimates for detecting ultra-faint galaxies of varying luminosities, sizes, and heliocentric distances in the first-year DES data.

  16. The Difference Imaging Pipeline for the Transient Search in the Dark Energy Survey

    SciTech Connect (OSTI)

    Kessler, R.

    2015-09-09

    We describe the operation and performance of the difference imaging pipeline (DiffImg) used to detect transients in deep images from the Dark Energy Survey Supernova program (DES-SN) in its first observing season from 2013 August through 2014 February. DES-SN is a search for transients in which ten 3 deg2 fields are repeatedly observed in the g, r, i, zpassbands with a cadence of about 1 week. Our observing strategy has been optimized to measure high-quality light curves and redshifts for thousands of Type Ia supernovae (SNe Ia) with the goal of measuring dark energy parameters. The essential DiffImg functions are to align each search image to a deep reference image, do a pixel-by-pixel subtraction, and then examine the subtracted image for significant positive detections of point-source objects. The vast majority of detections are subtraction artifacts, but after selection requirements and image filtering with an automated scanning program, there are ~130 detections per deg2 per observation in each band, of which only ~25% are artifacts. Of the ~7500 transients discovered by DES-SN in its first observing season, each requiring a detection on at least two separate nights, Monte Carlo (MC) simulations predict that 27% are expected to be SNe Ia or core-collapse SNe. Another ~30% of the transients are artifacts in which a small number of observations satisfy the selection criteria for a single-epoch detection. Spectroscopic analysis shows that most of the remaining transients are AGNs and variable stars. Fake SNe Ia are overlaid onto the images to rigorously evaluate detection efficiencies and to understand the DiffImg performance. Furthermore, the DiffImg efficiency measured with fake SNe agrees well with expectations from a MC simulation that uses analytical calculations of the fluxes and their uncertainties. In our 8 "shallow" fields with single-epoch 50% completeness depth ~23.5, the SN Ia efficiency falls to 1/2 at redshift z ≈ 0.7; in our 2 "deep" fields with mag-depth ~24.5, the efficiency falls to 1/2 at z ≈ 1.1. A remaining performance issue is that the measured fluxes have additional scatter (beyond Poisson fluctuations) that increases with the host galaxy surface brightness at the transient location. This bright-galaxy issue has minimal impact on the SNe Ia program, but it may lower the efficiency for finding fainter transients on bright galaxies.

  17. Réunion publique HR

    ScienceCinema (OSTI)

    None

    2011-10-06

    Chers Collègues,Je me permets de vous rappeler qu'une réunion publique organisée par le Département HR se tiendra aujourd'hui:Vendredi 30 avril 2010 à 9h30 dans l'Amphithéâtre principal (café offert dès 9h00).Durant cette réunion, des informations générales seront données sur:le CERN Admin e-guide, qui est un nouveau guide des procédures administratives du CERN ayant pour but de faciliter la recherche d'informations pratiques et d'offrir un format de lecture convivial;le régime d'Assurance Maladie de l'Organisation (présentation effectuée par Philippe Charpentier, Président du CHIS Board) et;la Caisse de Pensions (présentation effectuée par Théodore Economou, Administrateur de la Caisse de Pensions du CERN).Une transmission simultanée de cette réunion sera assurée dans l'Amphithéâtre BE de Prévessin et également disponible à l'adresse suivante: http://webcast.cern.chJe me réjouis de votre participation!Meilleures salutations,Anne-Sylvie CatherinChef du Département des Ressources humaines__________________________________________________________________________________Dear Colleagues,I should like to remind you that a plublic meeting organised by HR Department will be held today:Friday 30 April 2010 at 9:30 am in the Main Auditorium (coffee from 9:00 am).During this meeting, general information will be given about:the CERN Admin e-guide which is a new guide to the Organization's administrative procedures, drawn up to facilitate the retrieval of practical information and to offer a user-friendly format;the CERN Health Insurance System (presentation by Philippe Charpentier, President of the CHIS Board) and;the Pension Fund (presentation by Theodore Economou, Administrator of the CERN Pension Fund).A simultaneous transmission of this meeting will be broadcast in the BE Auditorium at Prévessin and will also be available at the following address. http://webcast.cern.chI look forward to your participation!Best regards,Anne-Sylvie CatherinHead, Human Resources Department

  18. The Difference Imaging Pipeline for the Transient Search in the Dark Energy Survey

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Kessler, R.

    2015-09-09

    We describe the operation and performance of the difference imaging pipeline (DiffImg) used to detect transients in deep images from the Dark Energy Survey Supernova program (DES-SN) in its first observing season from 2013 August through 2014 February. DES-SN is a search for transients in which ten 3 deg2 fields are repeatedly observed in the g, r, i, zpassbands with a cadence of about 1 week. Our observing strategy has been optimized to measure high-quality light curves and redshifts for thousands of Type Ia supernovae (SNe Ia) with the goal of measuring dark energy parameters. The essential DiffImg functions aremore » to align each search image to a deep reference image, do a pixel-by-pixel subtraction, and then examine the subtracted image for significant positive detections of point-source objects. The vast majority of detections are subtraction artifacts, but after selection requirements and image filtering with an automated scanning program, there are ~130 detections per deg2 per observation in each band, of which only ~25% are artifacts. Of the ~7500 transients discovered by DES-SN in its first observing season, each requiring a detection on at least two separate nights, Monte Carlo (MC) simulations predict that 27% are expected to be SNe Ia or core-collapse SNe. Another ~30% of the transients are artifacts in which a small number of observations satisfy the selection criteria for a single-epoch detection. Spectroscopic analysis shows that most of the remaining transients are AGNs and variable stars. Fake SNe Ia are overlaid onto the images to rigorously evaluate detection efficiencies and to understand the DiffImg performance. Furthermore, the DiffImg efficiency measured with fake SNe agrees well with expectations from a MC simulation that uses analytical calculations of the fluxes and their uncertainties. In our 8 "shallow" fields with single-epoch 50% completeness depth ~23.5, the SN Ia efficiency falls to 1/2 at redshift z ≈ 0.7; in our 2 "deep" fields with mag-depth ~24.5, the efficiency falls to 1/2 at z ≈ 1.1. A remaining performance issue is that the measured fluxes have additional scatter (beyond Poisson fluctuations) that increases with the host galaxy surface brightness at the transient location. This bright-galaxy issue has minimal impact on the SNe Ia program, but it may lower the efficiency for finding fainter transients on bright galaxies.« less

  19. Coherent Anti-Stokes Raman Scattering Spectroscopy of Single Molecules in Solution

    SciTech Connect (OSTI)

    Sunney Xie, Wei Min, Chris Freudiger, Sijia Lu

    2012-01-18

    During this funding period, we have developed two breakthrough techniques. The first is stimulated Raman scattering microscopy, providing label-free chemical contrast for chemical and biomedical imaging based on vibrational spectroscopy. Spontaneous Raman microscopy provides specific vibrational signatures of chemical bonds, but is often hindered by low sensitivity. We developed a three-dimensional multiphoton vibrational imaging technique based on stimulated Raman scattering (SRS). The sensitivity of SRS imaging is significantly greater than that of spontaneous Raman microscopy, which is achieved by implementing high-frequency (megahertz) phase-sensitive detection. SRS microscopy has a major advantage over previous coherent Raman techniques in that it offers background-free and readily interpretable chemical contrast. We demonstrated a variety of biomedical applications, such as differentiating distributions of omega-3 fatty acids and saturated lipids in living cells, imaging of brain and skin tissues based on intrinsic lipid contrast, and monitoring drug delivery through the epidermis. This technology offers exciting prospect for medical imaging. The second technology we developed is stimulated emission microscopy. Many chromophores, such as haemoglobin and cytochromes, absorb but have undetectable fluorescence because the spontaneous emission is dominated by their fast non-radiative decay. Yet the detection of their absorption is difficult under a microscope. We use stimulated emission, which competes effectively with the nonradiative decay, to make the chromophores detectable, as a new contrast mechanism for optical microscopy. We demonstrate a variety of applications of stimulated emission microscopy, such as visualizing chromoproteins, non-fluorescent variants of the green fluorescent protein, monitoring lacZ gene expression with a chromogenic reporter, mapping transdermal drug distribu- tions without histological sectioning, and label-free microvascular imaging based on endogenous contrast of haemoglobin. For all these applications, sensitivity is orders of magnitude higher than for spontaneous emission or absorption contrast, permitting nonfluorescent reporters for molecular imaging. Although we did not accomplish the original goal of detecting single-molecule by CARS, our quest for high sensitivity of nonlinear optical microscopy paid off in providing the two brand new enabling technologies. Both techniques were greatly benefited from the use of high frequency modulation for microscopy, which led to orders of magnitude increase in sensitivity. Extensive efforts have been made on optics and electronics to accomplish these breakthroughs.

  20. Supporting Advanced Scientific Computing Research * Basic Energy Sciences * Biological

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Energy S ciences N etwork Enabling Virtual Science June 9, 2009 Steve C o/er steve@es.net Dept. H ead, E nergy S ciences N etwork Lawrence B erkeley N aDonal L ab The E nergy S ciences N etwork The D epartment o f E nergy's O ffice o f S cience i s o ne o f t he l argest s upporters o f basic r esearch i n t he p hysical s ciences i n t he U .S. * Directly s upports t he r esearch o f s ome 1 5,000 s cienDsts, p ostdocs a nd g raduate s tudents at D OE l aboratories, u niversiDes, o ther F

  1. Club of Rome

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le Club de Rome s'est fait connaître du grand public par la publication du premier ouvrage "Halte à la croissance" qui a fait l'object d'un débat, il y a 2 ans. Le Prof. Tinbergen a commencé par s'adonner à la physique, il est docteur en physique et très tôt il s'est tourné vers les problèmes sociaux économiques. Il est expert auprès des nombreux gouvernements et organisations internationales et il a vu ses travaux couronnés par le prix Nobel en 1969.

  2. The Fifth Omega Laser Facility Users Group Workshop

    SciTech Connect (OSTI)

    Petrasso, R. D.

    2015-10-01

    A capacity gathering of over 100 researchers from 25 universities and laboratories met at the Laboratory for Laser Energetics (LLE) for the Fifth Omega Laser Facility Users Group (OLUG) workshop. The purpose of the 2.5-day workshop was to facilitate communications and exchanges among individual Omega users and between users and the LLE management; to present ongoing and proposed research; to encourage research opportunities and collaborations that could be undertaken at the Omega Laser Facility and in a complementary fashion at other facilities [such as the National Ignition Facility (NIF) or the Laboratoire pour lUtilisation des Lasers Intenses (LULI)]; to provide an opportunity for students, postdoctoral fellows, and young researchers to present their research in an informal setting; and to provide feedback to LLE management from the users about ways to improve the facility and future experimental campaigns.

  3. Cultural Alimentation in Latin America

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le Prof. Paolo Freire(nom?) a dirigé en Brésil un plan national d'alphabétisatation d'adultes. La base de sa méthode est d'essayer de ne pas rester sur la mécanique du mot, mais de le relier avec la réalité sociale et donner un réveillement critique de la conscience populaire en face de la réalité historique du pays. Il était professeur d'histoire et de philosophie de Récife, puis exilé et depuis il était prof. à Harvard, a travaillé à l'Unesco et est maintenant conseiller spécial à l'Office d'Education du centre oecuménique des églises

  4. Final report for the virtual channel encryptor laboratory directed research and development project

    SciTech Connect (OSTI)

    Gibson, D.J.; Sarfaty, R.A.

    1997-08-01

    A workstation with a single physical connection to a data communications network may have a requirement for simultaneous `virtual` communication channels to more than one destination. This report describes the development of techniques based on the Data Encryption Standard (DES) which encrypt these virtual channels to secure the data being transmitted against unauthorized access. A software module has been developed for the UNIX operating system using these techniques for encryption, and some development has also been done on a hardware device to be included between the workstation and network which can also provide these functions. The material presented in this report will be useful to those with a need to protect information in data communications systems from unauthorized access.

  5. Les vies de Galilée

    ScienceCinema (OSTI)

    None

    2011-10-06

    Qu'est-ce que l'astronomie? A quoi sert-elle ? Qui était Galilée ? Une soirée avec Fiami, auteur et dessinateur autour des vies de Galilée, titre de son nouvel ouvrage. Galilée y joue le protagoniste ou le complice de grandes découvertes à différentes époques et sous divers profils : Galilée à Babylone (-568) | Galilée à Alexandrie (-197) | Galilée en Inde (499) | Galilée à Venise (1609) | Galilée et Halley (1705) | Galilée revient (2009) Dans le cadre de l'année mondiale de l'astronomie. » Tout public » Entrée libre » Réservation groupes au +41 (0)22 767 76 76

  6. Heteropolymer freezing and design: Towards physical models of protein folding

    SciTech Connect (OSTI)

    Pande, Vijay S. [Chemistry Department, Stanford University, Stanford, California 94305-5080 (United States)] [Chemistry Department, Stanford University, Stanford, California 94305-5080 (United States); Grosberg, Alexander Yu. [Department of Physics, University of Minnesota, Minneapolis, Minnesota 55455 (United States)] [Department of Physics, University of Minnesota, Minneapolis, Minnesota 55455 (United States); Tanaka, Toyoichi [Department of Physics and Center for Materials Science and Engineering, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139 (United States)] [Department of Physics and Center for Materials Science and Engineering, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139 (United States)

    2000-01-01

    Protein folding has become one of the most actively studied problems in modern molecular biophysics. Approaches to the problem combine ideas from the physics of disordered systems, polymer physics, and molecular biology. Much can be learned from the statistical properties of model heteropolymers, the chain molecules having different monomers in irregular sequences. Even in highly evolved proteins, there is a strong random element in the sequences, which gives rise to a statistical ensemble of sequences for a given folded shape. Simple analytic models give rise to phase transitions between random, glassy, and folded states, depending on the temperature T and the design temperature T{sup des} of the ensemble of sequences. Besides considering the analytic results obtainable in a random-energy model and in the Flory mean-field model of polymers, the article reports on confirming numerical simulations. (c) 2000 The American Physical Society.

  7. Electron heating due to microwave photoexcitation in the high mobility GaAs/AlGaAs two dimensional electron system

    SciTech Connect (OSTI)

    Ramanayaka, A. N.; Mani, R. G.; Wegscheider, W.

    2013-12-04

    We extract the electron temperature in the microwave photo-excited high mobility GaAs/AlGaAs two dimensional electron system (2DES) by studying the influence of microwave radiation on the amplitude of Shubnikov-de Haas oscillations (SdHOs) in a regime where the cyclotron frequency, ?{sub c}, and the microwave angular frequency, ?, satisfy 2? ? ?{sub c} ? 3.5? The results indicate that increasing the incident microwave power has a weak effect on the amplitude of the SdHOs and therefore the electron temperature, in comparison to the influence of modest temperature changes on the dark-specimen SdH effect. The results indicate negligible electron heating under modest microwave photo-excitation, in good agreement with theoretical predictions.

  8. Local Voltage Support from Distributed Energy Resources to Prevent Air Conditioner Motor Stalling

    SciTech Connect (OSTI)

    Baone, Chaitanya A; Xu, Yan; Kueck, John D

    2010-01-01

    Microgrid voltage collapse often happens when there is a high percentage of low inertia air-conditioning (AC) motors in the power systems. The stalling of the AC motors results in Fault Induced Delayed Voltage Recovery (FIDVR). A hybrid load model including typical building loads, AC motor loads, and other induction motor loads is built to simulate the motoring stalling phenomena. Furthermore, distributed energy resources (DE) with local voltage support capability are utilized to boost the local bus voltage during a fault, and prevent the motor stalling. The simulation results are presented. The analysis of the simulation results show that local voltage support from multiple DEs can effectively and economically solve the microgrid voltage collapse problem.

  9. Comparative study of microwave radiation-induced magnetoresistive oscillations induced by circularly- and linearly- polarized photo-excitation

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Ye, Tianyu; Liu, Han -Chun; Wang, Zhuo; Wegscheider, W.; Mani, Ramesh G.

    2015-10-09

    A comparative study of the radiation-induced magnetoresistance oscillations in the high mobility GaAs/AlGaAs heterostructure two dimensional electron system (2DES) under linearly- and circularly- polarized microwave excitation indicates a profound difference in the response observed upon rotating the microwave launcher for the two cases, although circularly polarized microwave radiation induced magnetoresistance oscillations observed at low magnetic fields are similar to the oscillations observed with linearly polarized radiation. For the linearly polarized radiation, the magnetoresistive response is a strong sinusoidal function of the launcher rotation (or linear polarization) angle, θ. As a result, for circularly polarized radiation, the oscillatory magnetoresistive response ismore » hardly sensitive to θ.« less

  10. Offshore Wind Guidance Document: Oceanography and Sediment Stability (Version 1) Development of a Conceptual Site Model.

    SciTech Connect (OSTI)

    Roberts, Jesse D.; Jason Magalen; Craig Jones

    2014-06-01

    This guidance document provide s the reader with an overview of the key environmental considerations for a typical offshore wind coastal location and the tools to help guide the reader through a thoro ugh planning process. It will enable readers to identify the key coastal processes relevant to their offshore wind site and perform pertinent analysis to guide siting and layout design, with the goal of minimizing costs associated with planning, permitting , and long - ter m maintenance. The document highlight s site characterization and assessment techniques for evaluating spatial patterns of sediment dynamics in the vicinity of a wind farm under typical, extreme, and storm conditions. Finally, the document des cribe s the assimilation of all of this information into the conceptual site model (CSM) to aid the decision - making processes.

  11. Tomography and weak lensing statistics

    SciTech Connect (OSTI)

    Munshi, Dipak; Coles, Peter; Kilbinger, Martin E-mail: peter.coles@astro.cf.ac.uk

    2014-04-01

    We provide generic predictions for the lower order cumulants of weak lensing maps, and their correlators for tomographic bins as well as in three dimensions (3D). Using small-angle approximation, we derive the corresponding one- and two-point probability distribution function for the tomographic maps from different bins and for 3D convergence maps. The modelling of weak lensing statistics is obtained by adopting a detailed prescription for the underlying density contrast that involves hierarchal ansatz and lognormal distribution. We study the dependence of our results on cosmological parameters and source distributions corresponding to the realistic surveys such as LSST and DES. We briefly outline how photometric redshift information can be incorporated in our results. We also show how topological properties of convergence maps can be quantified using our results.

  12. LANL: AOT & LANSCE The Pulse March 2010

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    Los Alamos National Laboratory * Est. 1943 The Pulse-Newsletter of the Los Alamos Neutron Science Center and Accelerator Operations and Technology Division I N S I D E 2 Tajima receives DOe early career awarD 2 NeuTrON reflec- TOmeTry prOviDes firsT sub-NaNOmeTer visualizaTiON Of live cell aDhesiON 3 creaTiNg a high- efficieNcy cOmpacT iON acceleraTOr, aN alTerNaTive TO larger, mOre cOsTly sTruc- Tures 4 heaDs up! LANSCE beam reliability achieves "world class" ranking AOT has issued

  13. LANL: AOT & LANSCE The Pulse October 2011

    Broader source: All U.S. Department of Energy (DOE) Office Webpages (Extended Search)

    1 Los Alamos National Laboratory * Est. 1943 The Pulse-Newsletter of the Los Alamos Neutron Science Center and Accelerator Operations and Technology Division I N S I D E 3 From Alex's Desk 3 NeutroN scAtteriNg proviDes iNsight iNto eNzymAtic DegrADAtioN oF cellulose 4 NeutroN totAl scAtteriNg moNitors shiFts iN vAleNce stAtes 5 NeutroN reFlec- tometry exAmiNes the perFormANce oF rADiAtioN-resistANt mAteriAls 6 meAsuriNg the FissioN NeutroN spectrum At lANsce 7 heADs up! Daniel Shoemaker receives

  14. Large linear magnetoresistance in a GaAs/AlGaAs heterostructure

    SciTech Connect (OSTI)

    Aamir, Mohammed Ali, E-mail: aamir@physics.iisc.ernet.in; Goswami, Srijit, E-mail: aamir@physics.iisc.ernet.in; Ghosh, Arindam [Department of Physics, Indian Institute of Science, Bangalore 560 012 (India); Baenninger, Matthias; Farrer, Ian; Ritchie, David A. [Cavendish Laboratory, University of Cambridge, J.J. Thomson Avenue, Cambridge CB3 0HE (United Kingdom); Tripathi, Vikram [Department of Theoretical Physics, Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005 (India); Pepper, Michael [Department of Electrical and Electronic Engineering, University College, London WC1E 7JE (United Kingdom)

    2013-12-04

    We report non-saturating linear magnetoresistance (MR) in a two-dimensional electron system (2DES) at a GaAs/AlGaAs heterointerface in the strongly insulating regime. We achieve this by driving the gate voltage below the pinch-off point of the device and operating it in the non-equilibrium regime with high source-drain bias. Remarkably, the magnitude of MR is as large as 500% per Tesla with respect to resistance at zero magnetic field, thus dwarfing most non-magnetic materials which exhibit this linearity. Its primary advantage over most other materials is that both linearity and the enormous magnitude are retained over a broad temperature range (0.3 K to 10 K), thus making it an attractive candidate for cryogenic sensor applications.

  15. High Energy Physics at the University of Illinois

    SciTech Connect (OSTI)

    Liss, Tony M.; Thaler, Jon J.

    2013-07-26

    This is the final report for DOE award DE-FG02-91ER40677 (“High Energy Physics at the University of Illinois”), covering the award period November 1, 2009 through April 30, 2013. During this period, our research involved particle physics at Fermilab and CERN, particle physics related cosmology at Fermilab and SLAC, and theoretical particle physics. Here is a list of the activities described in the final report: * The CDF Collaboration at the Fermilab Tevatron * Search For Lepton Flavor Violation in the Mu2e Experiment At Fermilab * The ATLAS Collaboration at the CERN Large Hadron Collider * the Study of Dark Matter and Dark Energy: DES and LSST * Lattice QCD * String Theory and Field Theory * Collider Phenomenology

  16. The Sixth Omega Laser Facility Users Group Workshop

    SciTech Connect (OSTI)

    Petrasso, R. D.

    2014-10-01

    A capacity gathering of over 100 researchers from 25 universities and laboratories met at the Laboratory for Laser Energetics (LLE) for the Sixth Omega Laser Facility Users Group (OLUG) workshop. The purpose of the 2.5-day workshop was to facilitate communications and exchanges among individual OMEGA users, and between users and the LLE management; to present ongoing and proposed research; to encourage research opportunities and collaborations that could be undertaken at the Omega Laser Facility and in a complementary fashion at other facilities [such as the National Ignition Facility (NIF) or the Laboratoire pour lUtilisation des Lasers Intenses (LULI)]; to provide an opportunity for students, postdoctoral fellows, and young researchers to present their research in an informal setting; and to provide feedback from the users to LLE management about ways to improve and keep the facility and future experimental campaigns at the cutting edge.

  17. Memorial W.Gentner

    ScienceCinema (OSTI)

    None

    2011-04-25

    Le DG H.Schopper fait une introduction pour la commémoration et cérémonie de la vie et du travail du Prof.Wolfgang Gentner. W. Gentner, physicien allemand, né en 1906 à Francfort et mort en septembre 1980 à Heidelberg, était directeur au Cern de 1955 à 1960, président du "scientific policy commitee" de 1968 à 1971 et président du Conseil du Cern de 1972 à 1974. Il était un des fondateurs du Cern et 4 personnes qui l'ont bien connu lui rendent hommage, entre autres un de ses élèves, ainsi que Mme ?, J.B.Adams et O.Sheffard(?)

  18. Material report in support to RCC-MRX code 2010 stainless steel parts and products

    SciTech Connect (OSTI)

    Ancelet, Olivier; Lebarbe, Thierry; Dubiez-Le Goff, Sophie; Bonne, Dominique; Gelineau, Odile

    2012-07-01

    This paper presents the Material Report dedicated to stainless steels parts and products issued by AFCEN (Association Francaise pour les regles de Conception et de Construction des Materiels des Chaudieres Electro-Nucleaires) in support to RCC-MRx 2010 Code. The RCC-MRx Code is the result of the merger of the RCC-MX 2008, developed in the context of the research reactor Jules Horowitz Reactor project, in the RCC-MR 2007, which set up rules applicable to the design of components operating at high temperature and to the Vacuum Vessel of ITER (a presentation of RCC-MRx 2010 Code is the subject of another paper proposed in this Congress; it explains in particular the status of this Code). This Material Report is part of a set of Criteria of RCC-MRx (this set of Criteria is under construction). The Criteria aim at explaining the design and construction rules of the Code. They cover analyses rules as well as part procurement, welding, methods of tests and examination and fabrication rules. The Material Report particularly provides justifications and explanations on requirements and features dealing with parts and products proposed in the Code. The Material Report contains the following information: Introduction of the grade(s): codes and standards and Reference Procurement Specifications covering parts and products, applications and experience gained, - Physical properties, - Mechanical properties used for design calculations (base metal and welds): basic mechanical properties, creep mechanical properties, irradiated mechanical properties, - Fabrication: experience gained, metallurgy, - Welding: weldability, experience gained during welding and repair procedure qualifications, - Non-destructive examination, - In-service behaviour. In the article, examples of data supplied in the Material Report dedicated to stainless steels will be exposed. (authors)

  19. Clean Energy Application Center

    SciTech Connect (OSTI)

    Freihaut, Jim

    2013-09-30

    The Mid Atlantic Clean Energy Application Center (MACEAC), managed by The Penn State College of Engineering, serves the six states in the Mid-Atlantic region (Pennsylvania, New Jersey, Delaware, Maryland, Virginia and West Virginia) plus the District of Columbia. The goals of the Mid-Atlantic CEAC are to promote the adoption of Combined Heat and Power (CHP), Waste Heat Recovery (WHR) and District Energy Systems (DES) in the Mid Atlantic area through education and technical support to more than 1,200 regional industry and government representatives in the region. The successful promotion of these technologies by the MACEAC was accomplished through the following efforts; (1)The MACEAC developed a series of technology transfer networks with State energy and environmental offices, Association of Energy Engineers local chapters, local community development organizations, utilities and, Penn State Department of Architectural Engineering alumni and their firms to effectively educate local practitioners about the energy utilization, environmental and economic advantages of CHP, WHR and DES; (2) Completed assessments of the regional technical and market potential for CHP, WHR and DE technologies application in the context of state specific energy prices, state energy and efficiency portfolio development. The studies were completed for Pennsylvania, New Jersey and Maryland and included a set of incentive adoption probability models used as a to guide during implementation discussions with State energy policy makers; (3) Using the technical and market assessments and adoption incentive models, the Mid Atlantic CEAC developed regional strategic action plans for the promotion of CHP Application technology for Pennsylvania, New Jersey and Maryland; (4) The CHP market assessment and incentive adoption model information was discussed, on a continuing basis, with relevant state agencies, policy makers and Public Utility Commission organizations resulting in CHP favorable incentive programs in New Jersey, Pennsylvania, Maryland and Delaware; (5) Developed and maintained a MACEAC website to provide technical information and regional CHP, WHR and DE case studies and site profiles for use by interested stakeholders in information transfer and policy discussions; (6) Provided Technical Assistance through feasibility studies and on site evaluations. The MACEAC completed 28 technical evaluations and 9 Level 1 CHP analyses ; and (7) the MACEAC provided Technical Education to the region through a series of 29 workshops and webinars, 37 technical presentations, 14 seminars and participation in 13 CHP conferences.

  20. Nicotine impairs cyclooxygenase-2-dependent kinin-receptor-mediated murine airway relaxations

    SciTech Connect (OSTI)

    Xu, Yuan Cardell, Lars-Olaf

    2014-02-15

    Introduction: Cigarette smoke induces local inflammation and airway hyperreactivity. In asthmatics, it worsens the symptoms and increases the risk for exacerbation. The present study investigates the effects of nicotine on airway relaxations in isolated murine tracheal segments. Methods: Segments were cultured for 24 h in the presence of vehicle, nicotine (10 ?M) and/or dexamethasone (1 ?M). Airway relaxations were assessed in myographs after pre-contraction with carbachol (1 ?M). Kinin receptors, cyclooxygenase (COX) and inflammatory mediator expressions were assessed by real-time PCR and confocal-microscopy-based immunohistochemistry. Results: The organ culture procedure markedly increased bradykinin- (selective B{sub 2} receptor agonist) and des-Arg{sup 9}-bradykinin- (selective B{sub 1} receptor agonist) induced relaxations, and slightly increased relaxation induced by isoprenaline, but not that induced by PGE{sub 2}. The kinin receptor mediated relaxations were epithelium-, COX-2- and EP2-receptor-dependent and accompanied by drastically enhanced mRNA levels of kinin receptors, as well as inflammatory mediators MCP-1 and iNOS. Increase in COX-2 and mPGES-1 was verified both at mRNA and protein levels. Nicotine selectively suppressed the organ-culture-enhanced relaxations induced by des-Arg{sup 9}-bradykinin and bradykinin, at the same time reducing mPGES-1 mRNA and protein expressions. ?7-nicotinic acetylcholine receptor inhibitors ?-bungarotoxin and MG624 both blocked the nicotine effects on kinin B{sub 2} receptors, but not those on B{sub 1}. Dexamethasone completely abolished kinin-induced relaxations. Conclusion: It is tempting to conclude that a local inflammatory process per se could have a bronchoprotective component by increasing COX-2 mediated airway relaxations and that nicotine could impede this safety mechanism. Dexamethasone further reduced airway inflammation together with relaxations. This might contribute to the steroid resistance seen in some patients with asthma. - Highlights: Nicotine from smoking impaired epithelial COX-2-mediated airway relaxation. Nicotine's effects were at least partially mediated by ?7-nicotinic receptors. Kinin-receptor-mediated airway relaxations are mediated by EP2 receptors in mice. Nicotine reduced mPGES-1 mRNA and protein expressions in airway smooth muscle. Dexamethasone could not restore nicotine-impaired airway relaxations.

  1. Northeast Clean Energy Application Center

    SciTech Connect (OSTI)

    Bourgeois, Tom

    2013-09-30

    From October 1, 2009 through September 30, 2013 (contract period), the Northeast Clean Energy Application Center (NE-CEAC) worked in New York and New England (Connecticut, Rhode Island, Vermont, Massachusetts, New Hampshire, and Maine) to create a more robust market for the deployment of clean energy technologies (CETs) including combined heat and power (CHP), district energy systems (DES), and waste heat recovery (WHR) systems through the provision of technical assistance, education and outreach, and strategic market analysis and support for decision-makers. CHP, DES, and WHR can help reduce greenhouse gas emissions, reduce electrical and thermal energy costs, and provide more reliable energy for users throughout the United States. The NE-CEACs efforts in the provision of technical assistance, education and outreach, and strategic market analysis and support for decision-makers helped advance the market for CETs in the Northeast thereby helping the region move towards the following outcomes: Reduction of greenhouse gas emissions and criteria pollutants Improvements in energy efficiency resulting in lower costs of doing business Productivity gains in industry and efficiency gains in buildings Lower regional energy costs Strengthened energy security Enhanced consumer choice Reduced price risks for end-users Economic development effects keeping more jobs and more income in our regional economy Over the contract period, NE-CEAC provided technical assistance to approximately 56 different potential end-users that were interested in CHP and other CETs for their facility or facilities. Of these 56 potential end-users, five new CHP projects totaling over 60 MW of install capacity became operational during the contract period. The NE-CEAC helped host numerous target market workshops, trainings, and webinars; and NE-CEAC staff delivered presentations at many other workshops and conferences. In total, over 60 different workshops, conferences, webinars, and presentation were hosted or delivered during the contract period. The NE-CEAC also produced publically available educational materials such as CHP project profiles. Finally, the NE-CEAC worked closely with the relevant state agencies involved with CHP development. In New York, the NE-CEAC played an important role in securing and maintaining funding for CHP incentive programs administered by the New York State Energy Research Development Authority. NE-CEAC was also involved in the NYC Mayor's Office DG Collaborative. The NECEAC was also named a strategic resource for the Connecticut Department of Energy and Environmental Protections innovative Microgrid Pilot Program.

  2. Water Supply at Los Alamos 1998-2001

    SciTech Connect (OSTI)

    Richard J. Koch; David B. Rogers

    2003-03-01

    For the period 1998 through 2001, the total water used at Los Alamos from all sources ranged from 1325 million gallons (Mg) in 1999 to 1515 Mg in 2000. Groundwater production ranged from 1323 Mg in 1999 to 1506 Mg in 2000 from the Guaje, Pajarito, and Otowi fields. Nonpotable surface water used from Los Alamos reservoir ranged from zero gallons in 2001 to 9.3 Mg in 2000. For years 1998 through 2001, over 99% of all water used at Los Alamos was groundwater. Water use by Los Alamos National Laboratory (LANL) between 1998 and 2001 ranged from 379 Mg in 2000 to 461 Mg in 1998. The LANL water use in 2001 was 393 Mg or 27% of the total water use at Los Alamos. Water use by Los Alamos County ranged from 872 Mg in 1999 to 1137 Mg in 2000, and averaged 1006 Mg/yr. Four new replacement wells in the Guaje field (G-2A, G-3A, G-4A, and G-5A) were drilled in 1998 and began production in 1999; with existing well G-1A, the Guaje field currently has five producing wells. Five of the old Guaje wells (G-1, G-2, G-4, G-5, and G-6) were plugged and abandoned in 1999, and one well (G-3) was abandoned but remains as an observation well for the Guaje field. The long-term water level observations in production and observation (test) wells at Los Alamos are consistent with the formation of a cone of depression in response to water production. The water level decline is gradual and at most has been about 0.7 to 2 ft per year for production wells and from 0.4 to 0.9 ft/yr for observation (test) wells. The largest water level declines have been in the Guaje field where nonpumping water levels were about 91 ft lower in 2001 than in 1951. The initial water levels of the Guaje replacement wells were 32 to 57 ft lower than the initial water levels of adjacent original Guaje wells. When production wells are taken off-line for pump replacement or repair, water levels have returned to within about 25 ft of initial static levels within 6 to 12 months. Thus, the water-level trends suggest no adverse impacts by production on long-term water supply sustainability at Los Alamos. This report summarizes production data and aquifer conditions for water production and monitor wells in the Los Alamos, New Mexico, and Los Alamos National Laboratory (LANL) area (Figure 1). Water production wells are grouped within the Guaje, Pajarito, and Otowi fields, the locations of which are shown on Figure 1. Wells from these fields supply all the potable water used for municipal and most industrial purposes in Los Alamos County (LAC), at LANL, and at Bandelier National Monument. This report has three primary objectives: (1) Provide a continuing historical record of metered well production and overall water usage; (2) Provide data to the Department of Energy (DOE) and LANL management, and Los Alamos County planners for operation of the water supply system and for long-range water resource planning; and (3) Provide water-level data from regional aquifer production wells, test wells, and monitoring wells.

  3. DESI and other Dark Energy experiments in the era of neutrino mass measurements

    SciTech Connect (OSTI)

    Font-Ribera, Andreu; McDonald, Patrick; Mostek, Nick; Reid, Beth A.; Seo, Hee-Jong; Slosar, Ane E-mail: PVMcDonald@lbl.gov E-mail: BAReid@lbl.gov E-mail: anze@bnl.gov

    2014-05-01

    We present Fisher matrix projections for future cosmological parameter measurements, including neutrino masses, Dark Energy, curvature, modified gravity, the inflationary perturbation spectrum, non-Gaussianity, and dark radiation. We focus on DESI and generally redshift surveys (BOSS, HETDEX, eBOSS, Euclid, and WFIRST), but also include CMB (Planck) and weak gravitational lensing (DES and LSST) constraints. The goal is to present a consistent set of projections, for concrete experiments, which are otherwise scattered throughout many papers and proposals. We include neutrino mass as a free parameter in most projections, as it will inevitably be relevant DESI and other experiments can measure the sum of neutrino masses to ? 0.02 eV or better, while the minimum possible sum is ? 0.06 eV. We note that constraints on Dark Energy are significantly degraded by the presence of neutrino mass uncertainty, especially when using galaxy clustering only as a probe of the BAO distance scale (because this introduces additional uncertainty in the background evolution after the CMB epoch). Using broadband galaxy power becomes relatively more powerful, and bigger gains are achieved by combining lensing survey constraints with redshift survey constraints. We do not try to be especially innovative, e.g., with complex treatments of potential systematic errors these projections are intended as a straightforward baseline for comparison to more detailed analyses.

  4. Direct production of hydrogen and aromatics from methane or natural gas: Review of recent U.S. patents

    SciTech Connect (OSTI)

    Lucia M. Petkovic; Daniel M. Ginosar

    2012-03-01

    Since the year 2000, the United States Patent and Trademark Office (USPTO) has granted a dozen patents for inventions related to methane dehydroaromatization processes. One of them was granted to UOP LLC (Des Plaines). It relates to a catalyst composition and preparation method. Two patents were granted to Conoco Phillips Company (Houston, TX). One was aimed at securing a process and operating conditions for methane aromatization. The other was aimed at securing a process that may be integrated with separation of wellhead fluids and blending of the aromatics produced from the gas with the crude. Nine patents were granted to ExxonMobil Chemical Patents Inc. (Houston, TX). Most of these were aimed at securing a dehydroaromatization process where methane-containing feedstock moves counter currently to a particulate catalyst. The coked catalyst is heated or regenerated either in the reactor, by cyclic operation, or in annex equipment, and returned to the reactor. The reactor effluent stream may be separated in its main components and used or recycled as needed. A brief summary of those inventions is presented in this review.

  5. Improving the Field Performance of Natural Gas Furnaces, Chicago, Illinois (Fact Sheet)

    SciTech Connect (OSTI)

    Rothgeb, S.; Brand, L.

    2013-11-01

    The objective of this project is to examine the impact that common installation practices and age-induced equipment degradation may have on the installed performance of natural gas furnaces, as measured by steady-state efficiency and AFUE. PARR identified twelve furnaces of various ages and efficiencies that were operating in residential homes in the Des Moines Iowa metropolitan area and worked with a local HVAC contractor to retrieve them and test them for steady-state efficiency and AFUE in the lab. Prior to removal, system airflow, static pressure, equipment temperature rise, and flue loss measurements were recorded for each furnace. After removal from the field the furnaces were transported to the Gas Technology Institute (GTI) laboratory, where PARR conducted steady-state efficiency and AFUE testing. The test results show that steady-state efficiency in the field was 6.4% lower than that measured for the same furnaces under standard conditions in the lab, which included tuning the furnace input and air flow rate. Comparing AFUE measured under ASHRAE standard conditions with the label value shows no reduction in efficiency for the furnaces in this study over their 15 to 24 years of operation when tuned to standard conditions. Further analysis of the data showed no significant correlation between efficiency change and the age or the rated efficiency of the furnace.

  6. Star/galaxy separation at faint magnitudes: Application to a simulated Dark Energy Survey

    SciTech Connect (OSTI)

    Soumagnac, M.T.; et al.

    2013-06-21

    We address the problem of separating stars from galaxies in future large photometric surveys. We focus our analysis on simulations of the Dark Energy Survey (DES). In the first part of the paper, we derive the science requirements on star/galaxy separation, for measurement of the cosmological parameters with the Gravitational Weak Lensing and Large Scale Structure probes. These requirements are dictated by the need to control both the statistical and systematic errors on the cosmological parameters, and by Point Spread Function calibration. We formulate the requirements in terms of the completeness and purity provided by a given star/galaxy classifier. In order to achieve these requirements at faint magnitudes, we propose a new method for star/galaxy separation in the second part of the paper. We first use Principal Component Analysis to outline the correlations between the objects parameters and extract from it the most relevant information. We then use the reduced set of parameters as input to an Artificial Neural Network. This multi-parameter approach improves upon purely morphometric classifiers (such as the classifier implemented in SExtractor), especially at faint magnitudes: it increases the purity by up to 20% for stars and by up to 12% for galaxies, at i-magnitude fainter than 23.

  7. Railroad accident report: Head-on collision between Iowa Interstate Railroad Extra 470 West and Extra 406 East with release of hazardous materials near Altoona, Iowa, on July 30, 1988. Irregular report

    SciTech Connect (OSTI)

    Not Available

    1989-07-06

    About 11:40 a.m. central daylight saving time on July 30, 1988, Iowa Interstate Railroad Ltd. (IAIS) freight trains Extra 470 West and Extra 406 East collided head on within the yard limits of Altoona, Iowa, about 10 miles east of Des Moines, Iowa. All 5 locomotive units from both trains; 11 cars of Extra 406 East; and 3 cars, including two tank cars containing denatured alcohol, of Extra 470 West derailed. The denatured alcohol, which was released through the pressure relief valves and the manway domes of the two derailed tank cars, was ignited by the fire resulting from the collision of the locomotives. Both crew members of Extra 470 West were fatally injured; the two crew members of Extra 406 East were only slightly injured. The estimated damage (including lading) as a result of this accident exceeded $1 million. The major safety issues in the accident include operational methods employed by the IAIS, training and selection of train and engine personnel, supervisory oversight by the IAIS, design of closure fittings on hazardous materials rail tanks, and oversight of regional railroads by the Federal Railroad Administration.

  8. DEMONSTRATION OF POTENTIAL FOR SELECTIVE CATALYTIC REDUCTION AND DIESEL PARTICULATE FILTERS

    SciTech Connect (OSTI)

    McGILL,R; KHAIR, M; SHARP, C

    2003-08-24

    This project addresses the potential for Selective Catalytic Reduction (SCR) devices (using urea as reductant) together with Diesel Particulate Filters (DPF) and low-pressure loop exhaust gas recirculation (EGR) to achieve future stringent emissions standards for heavy-duty engines powering Class 8 vehicles. Two emission control systems consisting of the three technologies (EGR, SCR, and DPF) were calibrated on a Caterpillar C-12 heavy-duty diesel engine. Results of these calibrations showed good promise in meeting the 2010 heavy-duty emission standards as set forth by the Environmental Protection Agency (EPA). These two emission control systems were developed to evaluate a series of fuels that have similar formulations except for their sulfur content. Additionally, one fuel, code-named BP15, was also evaluated. This fuel was prepared by processing straight-run distillate stocks through a commercial, single stage hydrotreater employing high activity catalyst at maximum severity. An additional goal of this program is to provide data for an on-going EPA technology review that evaluates progress toward meeting 2007/2010 emission standards. These emissions levels were to be achieved not only on the transient test cycles but in other modes of operation such as the steady-state Euro-III style emission test known as the OICA (Organisation Internationale des Compagnies d'Automobiles) or the ESC (European Stationary Cycle). Additionally, hydrocarbon and carbon monoxide emissions standards are to be met.

  9. Conceptual design of a gas turbine for PFBC applications

    SciTech Connect (OSTI)

    Bannister, R.L.; McGuigan, A.W.; Risley, T.P.; Smith, O.J.

    1992-01-01

    First generation pressurized fluidized bed (PFBC) technology has potential advantages which include: lower capital cost, Unproved environmental performance, shorter lead times, higher efficiency and enhanced fuel flexibility. Coal firing with combustion turbines experiments have been conducted for over forty years. These efforts have evolved to the point where commercial demonstrations are now feasible. The PFBC is one of these technologies. It will be demonstrated as part of the Clean Coal III initiative. PFBC technology is applicable for new installations, replacement of existing equipment as well as repower and retrofit. Included with these options is the opportunity to reduce dependency on fuel oil and well as enhancing environmental performance and increasing efficiency. The turbo-machinery will require design changes to meet the requirements for PFBC application. The major change to the combustion turbine take place in the center section. This section will include provisions to supply compressed air to the PFBC as well as receive vitiated air from the PFBC. These efforts also have the objective of reducing the degree of change from a standard unit. Under a clean coal program a first generation PFBC demonstration win take place at the Des Moines Energy Center. For this demonstration it will be necessary to remove two stages from the 251B12 compressor. This will make the air supplied by the compressor suitable for the PFBC system. The results from this program will be applicable to the DMEC-1 program.

  10. Conceptual design of a gas turbine for PFBC applications

    SciTech Connect (OSTI)

    Bannister, R.L.; McGuigan, A.W.; Risley, T.P.; Smith, O.J.

    1992-12-31

    First generation pressurized fluidized bed (PFBC) technology has potential advantages which include: lower capital cost, Unproved environmental performance, shorter lead times, higher efficiency and enhanced fuel flexibility. Coal firing with combustion turbines experiments have been conducted for over forty years. These efforts have evolved to the point where commercial demonstrations are now feasible. The PFBC is one of these technologies. It will be demonstrated as part of the Clean Coal III initiative. PFBC technology is applicable for new installations, replacement of existing equipment as well as repower and retrofit. Included with these options is the opportunity to reduce dependency on fuel oil and well as enhancing environmental performance and increasing efficiency. The turbo-machinery will require design changes to meet the requirements for PFBC application. The major change to the combustion turbine take place in the center section. This section will include provisions to supply compressed air to the PFBC as well as receive vitiated air from the PFBC. These efforts also have the objective of reducing the degree of change from a standard unit. Under a clean coal program a first generation PFBC demonstration win take place at the Des Moines Energy Center. For this demonstration it will be necessary to remove two stages from the 251B12 compressor. This will make the air supplied by the compressor suitable for the PFBC system. The results from this program will be applicable to the DMEC-1 program.

  11. Fluidized-bed copper oxide process. Phase IV. Conceptual design and economic evaluation, Volume I. Final report

    SciTech Connect (OSTI)

    1994-11-30

    Universal Oil Products, Inc. (UOP) of Des Plaines, Illinois has contracted A.E. Roberts & Associates, Inc. (AERA) of Atlanta, Georgia to prepare a sensitivity analysis for the development of the Fluidized-bed Copper Oxide (FBCO) process. As proposed by AERA in September 1991, development of the FBCO process design for a 500 mega-watt (MW) unit was divided into three tasks: (1) Establishment of a Conceptual Design, (2) Conceptual Design, (3) Cost Analysis Task 1 determined the basis for a conceptual design for the 500 megawatt (MW) FBCO process. It was completed by AERA in September of 1992, and a report was submitted at that time {open_quotes}Establishment of the Design Basis for Application to a 500 MW Coal-fired Facility.{close_quotes} Task 2 gathered all pertinent data available to date and reviewed its applicability to the 500 MW FBCO process. Work on this task was carried out on a joint basis by the AERA team members: Roberts & Schaefers worked on the dense phase transport aspect of the design; Cornell and Carnegie Mellon Universities worked on the design kinetics and modeling; and AERA contributed commercial power and combustion experience. Task 3 provides budgetary cost estimates for the FBCO process and competing alternative technologies for sulfur dioxide and nitrogen oxide removal.

  12. Improving Gas Furnace Performance: A Field and Laboratory Study at End of Life

    SciTech Connect (OSTI)

    Brand, L.; Yee, S.; Baker, J.

    2015-02-01

    In 2010, natural gas provided 54% of total residential space heating energy the U.S. on a source basis, or 3.5 Quadrillion Btu. Natural gas burned in furnaces accounted for 92% of that total, and boilers and other equipment made up the remainder. A better understanding of installed furnace performance is a key to energy savings for this significant energy usage. In this project, the U.S. Department of Energy Building America team Partnership for Advanced Residential Retrofit examined the impact that common installation practices and age-induced equipment degradation may have on the installed performance of natural gas furnaces over the life of the product, as measured by steady-state efficiency and annual efficiency. The team identified 12 furnaces of various ages and efficiencies that were operating in residential homes in the Des Moines, Iowa, metropolitan area and worked with a local heating, ventilation, and air conditioning contractor to retrieve furnaces and test them at the Gas Technology Institute laboratory for steady-state efficiency and annual efficiency. Prior to removal, system airflow, static pressure, equipment temperature rise, and flue loss measurements were recorded for each furnace as installed in the house.

  13. Fibre optique à la maison en Pays de Gex et de Bellegarde

    ScienceCinema (OSTI)

    None

    2011-10-06

    Le Syndicat Intercommunal d’Electricité de l’Ain(SIEA) déploie un réseau FTTH (Fiber To The Home) de fibres optiques dans le département de l’Ain vers l’ensemble des habitations. Le déploiement sur la zone pilote du Pays de Gex et du Bassin Bellegardien arrive dans la phase terminale vers les habitations. Le SIEA présentera ses activités, l’état du développement du réseau, les implications d’une connexion fibre optique et les procédures d’abonnement. La présentation sera donnée en Français. -------------------------------------------------------------------------------------------------------------------------------Public conference "Optical fiber To The Home in Pays de Gex et de Bellegarde" Michel Chanel et Jean Paul Goy (SIEA) Wednesday, 19th May at 11.30 hrs., Council Chamber, CERN The ‘’ Syndicat Intercommunal d’Electricité de l’Ain’’(SIEA) is deploying an optical fiber network FTTH (Fiber To The Home) in the Ain department towards the ensemble of houses. The installation on the pilot areas of Pays de Gex and Bassin Bellegardien is arriving in the phase of connecting houses. The SIEA will show its activities, the state of the network development, the implications of an optical fiber connection and the contract procedures. The presentation will be given in French

  14. Wide-field lensing mass maps from Dark Energy Survey science verification data: Methodology and detailed analysis

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Vikram, V.; Sheldon, E.; Chang, C.; Jain, B.; Bacon, D.; Amara, A.; Becker, M. R.; Bernstein, G.; Bonnett, C.; Bridle, S.; et al

    2015-07-29

    Weak gravitational lensing allows one to reconstruct the spatial distribution of the projected mass density across the sky. These mass maps provide a powerful tool for studying cosmology as they probe both luminous and dark matter. In this paper, we present a weak lensing mass map reconstructed from shear measurements in a 139 deg2 area from the Dark Energy Survey science verification data. We compare the distribution of mass with that of the foreground distribution of galaxies and clusters. The overdensities in the reconstructed map correlate well with the distribution of optically detected clusters. We demonstrate that candidate superclusters andmorevoids along the line of sight can be identified, exploiting the tight scatter of the cluster photometric redshifts. We cross-correlate the mass map with a foreground magnitude-limited galaxy sample from the same data. Our measurement gives results consistent with mock catalogs from N-body simulations that include the primary sources of statistical uncertainties in the galaxy, lensing, and photo-z catalogs. The statistical significance of the cross-correlation is at the 6.8? level with 20 arcminute smoothing. We find that the contribution of systematics to the lensing mass maps is generally within measurement uncertainties. We analyze less than 3% of the final area that will be mapped by the DES; the tools and analysis techniques developed in this paper can be applied to forthcoming larger data sets from the survey.less

  15. Technology Solutions Case Study: Improving the Field Performance of Natural Gas Furnaces

    SciTech Connect (OSTI)

    2013-11-01

    The objective of this project is to examine the impact that common installation practices and age-induced equipment degradation may have on the installed performance of natural gas furnaces, as measured by steady-state efficiency and AFUE. PARR identified twelve furnaces of various ages and efficiencies that were operating in residential homes in the Des Moines Iowa metropolitan area and worked with a local HVAC contractor to retrieve them and test them for steady-state efficiency and AFUE in the lab. Prior to removal, system airflow, static pressure, equipment temperature rise, and flue loss measurements were recorded for each furnace. After removal from the field the furnaces were transported to the Gas Technology Institute (GTI) laboratory, where PARR conducted steady-state efficiency and AFUE testing. The test results show that steady-state efficiency in the field was 6.4% lower than that measured for the same furnaces under standard conditions in the lab, which included tuning the furnace input and air flow rate. Comparing AFUE measured under ASHRAE standard conditions with the label value shows no reduction in efficiency for the furnaces in this study over their 15 to 24 years of operation when tuned to standard conditions. Further analysis of the data showed no significant correlation between efficiency change and the age or the rated efficiency of the furnace.

  16. Lessons from Iowa : development of a 270 megawatt compressed air energy storage project in midwest Independent System Operator : a study for the DOE Energy Storage Systems Program.

    SciTech Connect (OSTI)

    Holst, Kent; Huff, Georgianne; Schulte, Robert H.; Critelli, Nicholas

    2012-01-01

    The Iowa Stored Energy Park was an innovative, 270 Megawatt, $400 million compressed air energy storage (CAES) project proposed for in-service near Des Moines, Iowa, in 2015. After eight years in development the project was terminated because of site geological limitations. However, much was learned in the development process regarding what it takes to do a utility-scale, bulk energy storage facility and coordinate it with regional renewable wind energy resources in an Independent System Operator (ISO) marketplace. Lessons include the costs and long-term economics of a CAES facility compared to conventional natural gas-fired generation alternatives; market, legislative, and contract issues related to enabling energy storage in an ISO market; the importance of due diligence in project management; and community relations and marketing for siting of large energy projects. Although many of the lessons relate to CAES applications in particular, most of the lessons learned are independent of site location or geology, or even the particular energy storage technology involved.

  17. The Open Science Grid status and architecture

    SciTech Connect (OSTI)

    Pordes, Ruth; Petravick, Don; Kramer, Bill; Olsen, James D.; Livny, Miron; Roy, Gordon A.; Avery, Paul Ralph; Blackburn, Kent; Wenaus, Torre J.; Wuerthwein, Frank K.; Foster, Ian; /Chicago U. /Indiana U.

    2007-09-01

    The Open Science Grid (OSG) provides a distributed facility where the Consortium members provide guaranteed and opportunistic access to shared computing and storage resources. The OSG project[1] is funded by the National Science Foundation and the Department of Energy Scientific Discovery through Advanced Computing program. The OSG project provides specific activities for the operation and evolution of the common infrastructure. The US ATLAS and US CMS collaborations contribute to and depend on OSG as the US infrastructure contributing to the World Wide LHC Computing Grid on which the LHC experiments distribute and analyze their data. Other stakeholders include the STAR RHIC experiment, the Laser Interferometer Gravitational-Wave Observatory (LIGO), the Dark Energy Survey (DES) and several Fermilab Tevatron experiments- CDF, D0, MiniBoone etc. The OSG implementation architecture brings a pragmatic approach to enabling vertically integrated community specific distributed systems over a common horizontal set of shared resources and services. More information can be found at the OSG web site: www.opensciencegrid.org.

  18. Wide-field lensing mass maps from Dark Energy Survey science verification data: Methodology and detailed analysis

    SciTech Connect (OSTI)

    Vikram, V.; Sheldon, E.; Chang, C.; Jain, B.; Bacon, D.; Amara, A.; Becker, M. R.; Bernstein, G.; Bonnett, C.; Bridle, S.; Brout, D.; Busha, M.; Frieman, J.; Gaztanaga, E.; Hartley, W.; Jarvis, M.; Kacprzak, T.; Kovacs, A.; Lahav, O.; Leistedt, B.; Lin, H.; Melchior, P.; Peiris, H.; Rozo, E.; Rykoff, E.; Sanchez, C.; Sheldon, E.; Troxel, M. A.; Wechsler, R.; Zuntz, J.; Abbott, T.; Abdalla, F. B.; Armstrong, R.; Banerji, M.; Bauer, A. H.; Benoit-Levy, A.; Bertin, E.; Brooks, D.; Buckley-Geer, E.; Burke, D. L.; Capozzi, D.; Carnero Rosell, A.; Kind, M. Carrasco; Castander, F. J.; Crocce, M.; Cunha, C. E.

    2015-07-29

    Weak gravitational lensing allows one to reconstruct the spatial distribution of the projected mass density across the sky. These mass maps provide a powerful tool for studying cosmology as they probe both luminous and dark matter. In this paper, we present a weak lensing mass map reconstructed from shear measurements in a 139 deg2 area from the Dark Energy Survey science verification data. We compare the distribution of mass with that of the foreground distribution of galaxies and clusters. The overdensities in the reconstructed map correlate well with the distribution of optically detected clusters. We demonstrate that candidate superclusters and voids along the line of sight can be identified, exploiting the tight scatter of the cluster photometric redshifts. We cross-correlate the mass map with a foreground magnitude-limited galaxy sample from the same data. Our measurement gives results consistent with mock catalogs from N-body simulations that include the primary sources of statistical uncertainties in the galaxy, lensing, and photo-z catalogs. The statistical significance of the cross-correlation is at the 6.8? level with 20 arcminute smoothing. We find that the contribution of systematics to the lensing mass maps is generally within measurement uncertainties. We analyze less than 3% of the final area that will be mapped by the DES; the tools and analysis techniques developed in this paper can be applied to forthcoming larger data sets from the survey.

  19. Third international workshop on ice storage for cooling applications

    SciTech Connect (OSTI)

    Gorski, A.J.

    1986-04-01

    The third international workshop on ice storage for cooling applications which was informal and interactive in nature, was open to persons interested in all ice-growing technologies and in ice storage, both seasonal and diurnal. Presentations were made on some 20 topics, ranging from freezers in Alaska to ice cooling of commercial jet aircraft. Workshop tours included visits to ice-storage systems at Commonwealth Edison's facilities in Bolingbrook and Des Plaines Valley, the A.C. Neilsen builing in Northbrook, and the new State of Illinois Center in Chicago. The first workshop in the present series considered the future of ice storage and predicted applications in the agricultural sector, desalinization, and commercial ice production. Progress has been rapid in the intervening two years, and an important topic at the third workshop was the possible use of ''warm ices'' (clathrate hydrates) for energy storage. This report consists primarily of abstracts of presentations made at the workshop. Persons wishing to obtain further information about particular papers should contact the speakers directly; speakers' addresses and telephone numbers are listed in this report.

  20. Impact of operating parameters changing on energy, environment and economic efficiencies of a lean burn gas engine used in a cogeneration plant

    SciTech Connect (OSTI)

    Lemoult, B.; Tazerout, M.; Rousseau, S.

    1998-07-01

    The facts that national electrical company Electricite de France (EDF) has a monopoly on electrical power production in France and an extensive installed base of nuclear power plants, explain the difficulty encountered in developing cogeneration technology in France. Cogeneration only really first appeared in this country in the early 1990's, with the liberalization of energy markets and the government's encouragement. Since then, the number of cogeneration plants has continuously increased and electrical generating capacity is now approximately 1,200 MWe. Turbine and reciprocating engines (most of which are natural gas fired) account respectively for about 55% and 45% of the installed power. Unlike other countries, such as Germany--which has about two thousand 500 kWe and smaller units--the future of low-power cogeneration in France is far from assured, and there are currently less than 10 such plants. To help develop this efficient technology for producing electrical power and hot water, the Ecole des Mines de Nantes purchased a 210 kWe cogeneration generator set in 1996. This facility provides all or part of the school's electrical and heat requirements during five months between November and March. This cogeneration facility is also used during the rest of the year to perform research experiments in the field of lean-burn natural gas combustion. Lastly, it is also used to provide training for industry in cogeneration technology. Within this context, work was undertaken to study the set's energy and emissions performance, in relation to such parameters as spark advance and air factor, and at various loads.

  1. LNG demand, shipping will expand through 2010

    SciTech Connect (OSTI)

    True, W.R.

    1998-02-09

    The 1990s, especially the middle years, have witnessed a dramatic turnaround in the growth of liquefied-natural-gas demand which has tracked equally strong natural-gas demand growth. This trend was underscored late last year by several annual studies of world LNG demand and shipping. As 1998 began, however, economic turmoil in Asian financial markets has clouded near-term prospects for LNG in particular and all energy in general. But the extent of damage to energy markets is so far unclear. A study by US-based Institute of Gas Technology, Des Plaines, IL, reveals that LNG imports worldwide have climbed nearly 8%/year since 1980 and account for 25% of all natural gas traded internationally. In the mid-1970s, the share was only 5%. In 1996, the most recent year for which complete data are available, world LNG trade rose 7.7% to a record 92 billion cu m, outpacing the overall consumption for natural gas which increased 4.7% in 1996. By 2015, says the IGT study, natural-gas use would surpass coal as the world`s second most widely used fuel, after petroleum. Much of this growth will occur in the developing countries of Asia where gas use, before the current economic crisis began, was projected to grow 8%/year through 2015. Similar trends are reflected in another study of LNG trade released at year end 1997, this from Ocean Shipping Consultants Ltd., Surrey, U.K. The study was done too early, however, to consider the effects of the financial problems roiling Asia.

  2. Mass and galaxy distributions of four massive galaxy clusters from Dark Energy Survey Science Verification data

    SciTech Connect (OSTI)

    Melchior, P.; Suchyta, E.; Huff, E.; Hirsch, M.; Kacprzak, T.; Rykoff, E.; Gruen, D.; Armstrong, R.; Bacon, D.; Bechtol, K.; Bernstein, G. M.; Bridle, S.; Clampitt, J.; Honscheid, K.; Jain, B.; Jouvel, S.; Krause, E.; Lin, H.; MacCrann, N.; Patton, K.; Plazas, A.; Rowe, B.; Vikram, V.; Wilcox, H.; Young, J.; Zuntz, J.; Abbott, T.; Abdalla, F. B.; Allam, S. S.; Banerji, M.; Bernstein, J. P.; Bernstein, R. A.; Bertin, E.; Buckley-Geer, E.; Burke, D. L.; Castander, F. J.; da Costa, L. N.; Cunha, C. E.; Depoy, D. L.; Desai, S.; Diehl, H. T.; Doel, P.; Estrada, J.; Evrard, A. E.; Neto, A. F.; Fernandez, E.; Finley, D. A.; Flaugher, B.; Frieman, J. A.; Gaztanaga, E.; Gerdes, D.; Gruendl, R. A.; Gutierrez, G. R.; Jarvis, M.; Karliner, I.; Kent, S.; Kuehn, K.; Kuropatkin, N.; Lahav, O.; Maia, M. A. G.; Makler, M.; Marriner, J.; Marshall, J. L.; Merritt, K. W.; Miller, C. J.; Miquel, R.; Mohr, J.; Neilsen, E.; Nichol, R. C.; Nord, B. D.; Reil, K.; Roe, N. A.; Roodman, A.; Sako, M.; Sanchez, E.; Santiago, B. X.; Schindler, R.; Schubnell, M.; Sevilla-Noarbe, I.; Sheldon, E.; Smith, C.; Soares-Santos, M.; Swanson, M. E. C.; Sypniewski, A. J.; Tarle, G.; Thaler, J.; Thomas, D.; Tucker, D. L.; Walker, A.; Wechsler, R.; Weller, J.; Wester, W.

    2015-03-31

    We measure the weak-lensing masses and galaxy distributions of four massive galaxy clusters observed during the Science Verification phase of the Dark Energy Survey. This pathfinder study is meant to 1) validate the DECam imager for the task of measuring weak-lensing shapes, and 2) utilize DECam's large field of view to map out the clusters and their environments over 90 arcmin. We conduct a series of rigorous tests on astrometry, photometry, image quality, PSF modelling, and shear measurement accuracy to single out flaws in the data and also to identify the optimal data processing steps and parameters. We find Science Verification data from DECam to be suitable for the lensing analysis described in this paper. The PSF is generally well-behaved, but the modelling is rendered difficult by a flux-dependent PSF width and ellipticity. We employ photometric redshifts to distinguish between foreground and background galaxies, and a red-sequence cluster finder to provide cluster richness estimates and cluster-galaxy distributions. By fitting NFW profiles to the clusters in this study, we determine weak-lensing masses that are in agreement with previous work. For Abell 3261, we provide the first estimates of redshift, weak-lensing mass, and richness. Additionally, the cluster-galaxy distributions indicate the presence of filamentary structures attached to 1E 0657-56 and RXC J2248.7-4431, stretching out as far as 1degree (approximately 20 Mpc), showcasing the potential of DECam and DES for detailed studies of degree-scale features on the sky.

  3. Unusual Application Of Ion Beam Analysis For The Study Of Surface Layers On Materials Relevant To Cultural Heritage

    SciTech Connect (OSTI)

    Mathis, F.; Salomon, J.; Aucouturier, M.; Trocellier, P.

    2006-12-01

    Recently a new thematic of research -- intentional patinas on antic copper-base objects -- lead the AGLAE (Accelerateur Grand Louvre pour l'Analyse Elementaire) team of the C2RMF (Centre de Recherche et de Restauration des Musees de France) to improve its methods of analyzing thin surface layers both in their elemental composition and in-depth elemental distribution. A new beam extraction set-up containing a particle detector has been developed in order to use a 6 MeV alpha beam both in PIXE and RBS mode and to monitor precisely the ion dose received by the sample. Both RBS and ionization cross sections were assessed in order to make sure that the analysis can be quantitative. This set up allows great progresses in the understanding of both nature and structure of this very particular oxide layer obtained in the antiquity by chemical treatment on copper alloys, containing gold and/or silver and presenting very interesting properties of color and stability.Besides the non destructive properties of the IBA in external beam mode, this method of analyzing allows the study of samples in interaction with its environment. This was used to study the high temperature oxidation of Cu-Sn alloys using a furnace developed in order to heat a sample and analyze it in RBS mode at the same time. This new way of studying the growth of oxide layers permits to understand the oxidation mechanism of this system and to propose an experimental model for the identification of oxide layers due to an exposition to a high temperature, model needed for a long time by curators in charge of the study and the conservation of archaeological bronzes.

  4. Mass and galaxy distributions of four massive galaxy clusters from Dark Energy Survey Science Verification data

    DOE Public Access Gateway for Energy & Science Beta (PAGES Beta)

    Melchior, P.; Suchyta, E.; Huff, E.; Hirsch, M.; Kacprzak, T.; Rykoff, E.; Gruen, D.; Armstrong, R.; Bacon, D.; Bechtol, K.; et al

    2015-03-31

    We measure the weak-lensing masses and galaxy distributions of four massive galaxy clusters observed during the Science Verification phase of the Dark Energy Survey. This pathfinder study is meant to 1) validate the DECam imager for the task of measuring weak-lensing shapes, and 2) utilize DECam's large field of view to map out the clusters and their environments over 90 arcmin. We conduct a series of rigorous tests on astrometry, photometry, image quality, PSF modelling, and shear measurement accuracy to single out flaws in the data and also to identify the optimal data processing steps and parameters. We find Sciencemore » Verification data from DECam to be suitable for the lensing analysis described in this paper. The PSF is generally well-behaved, but the modelling is rendered difficult by a flux-dependent PSF width and ellipticity. We employ photometric redshifts to distinguish between foreground and background galaxies, and a red-sequence cluster finder to provide cluster richness estimates and cluster-galaxy distributions. By fitting NFW profiles to the clusters in this study, we determine weak-lensing masses that are in agreement with previous work. For Abell 3261, we provide the first estimates of redshift, weak-lensing mass, and richness. Additionally, the cluster-galaxy distributions indicate the presence of filamentary structures attached to 1E 0657-56 and RXC J2248.7-4431, stretching out as far as 1degree (approximately 20 Mpc), showcasing the potential of DECam and DES for detailed studies of degree-scale features on the sky.« less

  5. Turbulent Flow Effects on the Biological Performance of Hydro-Turbines

    SciTech Connect (OSTI)

    Richmond, Marshall C.; Romero Gomez, Pedro DJ

    2014-08-25

    The hydro-turbine industry uses Computational Fluid Dynamics (CFD) tools to predict the flow conditions as part of the design process for new and rehabilitated turbine units. Typically the hydraulic design process uses steady-state simulations based on Reynolds-Averaged Navier-Stokes (RANS) formulations for turbulence modeling because these methods are computationally efficient and work well to predict averaged hydraulic performance, e.g. power output, efficiency, etc. However, in view of the increasing emphasis on environmental concerns, such as fish passage, the consideration of the biological performance of hydro-turbines is also required in addition to hydraulic performance. This leads to the need to assess whether more realistic simulations of the turbine hydraulic environment ?those that resolve unsteady turbulent eddies not captured in steady-state RANS computations? are needed to better predict the occurrence and extent of extreme flow conditions that could be important in the evaluation of fish injury and mortality risks. In the present work, we conduct unsteady, eddy-resolving CFD simulations on a Kaplan hydro-turbine at a normal operational discharge. The goal is to quantify the impact of turbulence conditions on both the hydraulic and biological performance of the unit. In order to achieve a high resolution of the incoming turbulent flow, Detached Eddy Simulation (DES) turbulence model is used. These transient simulations are compared to RANS simulations to evaluate whether extreme hydraulic conditions are better captured with advanced eddy-resolving turbulence modeling techniques. The transient simulations of key quantities such as pressure and hydraulic shear flow that arise near the various components (e.g. wicket gates, stay vanes, runner blades) are then further analyzed to evaluate their impact on the statistics for the lowest absolute pressure (nadir pressures) and for the frequency of collisions that are known to cause mortal injury in fish passing through hydro-turbines.

  6. HR Public meeting

    ScienceCinema (OSTI)

    None

    2011-10-06

    Cher(e)s collgues, En collaboration avec le Dpartement HR, le Directeur gnral a le plaisir de vous convier une runion publique qui se tiendra le vendredi 25 juin 2010 9h30 dans l?Amphithtre principal (Btiment 500)*. Un caf d?accueil y sera servi partir de 9h. Cette runion abordera les thmes suivants : ? Valeurs de l?Organisation (Directeur gnral) ? Code de Conduite (Directeur gnral / Anne-Sylvie Catherin) ? Cration du nouveau rle d?Ombudsperson (Vincent Vuillemin) Ces prsentations seront suivies d?une sance de questions-rponses. Nous esprons vous retrouver nombreux le 25 juin ! Meilleures salutations, Anne-Sylvie Catherin Chef du Dpartement des Ressources humaines *Cette runion sera retransmise simultanment dans l?Amphithtre BE de Prvessin (Btiment 864) et galement disponible l?adresse suivante : http://webcast.cern.ch -------------------------------------------------------- Dear colleagues, In collaboration with HR Department, the Director-General would like to invite you to an information meeting which will be held on Friday 25 June 2010 at 9:30 am in the Main Auditorium (Building 500)*. A welcome coffee will be available from 9:00 am. During this meeting, information will be given about: ? Organization?s values (Director-General) ? Code of Conduct (Director-General / Anne-Sylvie Catherin) ? New Ombudsperson role (Vincent Vuillemin) These presentations will be followed by a questions & answers session. We look forward to seeing you all on 25 June! Best regards, Anne-Sylvie Catherin Head, Human Resources Department *This meeting will be simultaneously retransmitted in BE Auditorium (Building 864) and available at the following address: http://webcast.cern.ch.

  7. EMAPS: An Efficient Multiscale Approach to Plasma Systems with Non-MHD Scale Effects

    SciTech Connect (OSTI)

    Omelchenko, Yuri A; Karimabadi, Homa

    2014-10-14

    Using Discrete-Event Simulation (DES) as a novel paradigm for time integration of large-scale physics-driven systems, we have achieved significant breakthroughs in simulations of multi-dimensional magnetized plasmas where ion kinetic and finite Larmor radius (FLR) and Hall effects play a crucial role. For these purposes we apply a unique asynchronous simulation tool: a parallel, electromagnetic Particle-in-Cell (PIC) code, HYPERS (Hybrid Particle Event-Resolved Simulator), which treats plasma electrons as a charge neutralizing fluid and solves a self-consistent set of non-radiative Maxwell, electron fluid equations and ion particle equations on a structured computational grid. HYPERS enables adaptive local time steps for particles, fluid elements and electromagnetic fields. This ensures robustness (stability) and efficiency (speed) of highly dynamic and nonlinear simulations of compact plasma systems such spheromaks, FRCs, ion beams and edge plasmas. HYPERS is a unique asynchronous code that has been designed to serve as a test bed for developing multi-physics applications not only for laboratory plasma devices but generally across a number of plasma physics fields, including astrophysics, space physics and electronic devices. We have made significant improvements to the HYPERS core: (1) implemented a new asynchronous magnetic field integration scheme that preserves local divB=0 to within round-off errors; (2) Improved staggered-grid discretizations of electric and magnetic fields. These modifications have significantly enhanced the accuracy and robustness of 3D simulations. We have conducted first-ever end-to-end 3D simulations of merging spheromak plasmas. The preliminary results show: (1) tilt-driven relaxation of a freely expanding spheromak to an m=1 Taylor helix configuration and (2) possibility of formation of a tilt-stable field-reversed configuration via merging and magnetic reconnection of two double-sided spheromaks with opposite helicities.

  8. Opacity of iron, nickel, and copper plasmas in the x-ray wavelength range: Theoretical interpretation of 2p-3d absorption spectra

    SciTech Connect (OSTI)

    Blenski, T.; Loisel, G.; Poirier, M.; Thais, F.; Arnault, P.; Caillaud, T.; Fariaut, J.; Gilleron, F.; Pain, J.-C.; Porcherot, Q.; Reverdin, C.; Silvert, V.; Villette, B.; Bastiani-Ceccotti, S.; Turck-Chieze, S.; Foelsner, W.; Gaufridy de Dortan, F. de

    2011-09-15

    This paper deals with theoretical studies on the 2p-3d absorption in iron, nickel, and copper plasmas related to LULI2000 (Laboratoire pour l'Utilisation des Lasers Intenses, 2000J facility) measurements in which target temperatures were of the order of 20 eV and plasma densities were in the range 0.004-0.01 g/cm{sup 3}. The radiatively heated targets were close to local thermodynamic equilibrium (LTE). The structure of 2p-3d transitions has been studied with the help of the statistical superconfiguration opacity code sco and with the fine-structure atomic physics codes hullac and fac. A new mixed version of the sco code allowing one to treat part of the configurations by detailed calculation based on the Cowan's code rcg has been also used in these comparisons. Special attention was paid to comparisons between theory and experiment concerning the term features which cannot be reproduced by sco. The differences in the spin-orbit splitting and the statistical (thermal) broadening of the 2p-3d transitions have been investigated as a function of the atomic number Z. It appears that at the conditions of the experiment the role of the term and configuration broadening was different in the three analyzed elements, this broadening being sensitive to the atomic number. Some effects of the temperature gradients and possible non-LTE effects have been studied with the help of the radiative-collisional code scric. The sensitivity of the 2p-3d structures with respect to temperature and density in medium-Z plasmas may be helpful for diagnostics of LTE plasmas especially in future experiments on the {Delta}n=0 absorption in medium-Z plasmas for astrophysical applications.

  9. Deployment of FlexCHP System

    SciTech Connect (OSTI)

    Cygan, David

    2015-11-01

    The Gas Technology Institute (GTI), along with its partner Integrated CHP Systems Corporation, has developed and demonstrated an Ultra-Low-Nitrogen Oxide (ULN) Flexible Combined Heat and Power (FlexCHP) system that packages a state-of-the-art Capstone C65 gas microturbine and Johnston PFXX100 boiler with an innovative natural gas-fired supplemental burner. Supplemental burners add heat as needed in response to facility demand, which increases energy efficiency, but typically raises exhaust NOx levels, degrading local air quality unless a costly and complicated catalytic treatment system is added. The FlexCHP system increases energy efficiency and achieves the 2007 California Air Resource Board (CARB) distributed generation emissions standards for Nitrogen oxides (NOx), Carbon Monoxide (CO), and Total Hydrocarbons (THC) without catalytic exhaust gas treatment. The key to this breakthrough performance is a simple and reliable burner design which utilizes staged combustion with engineered internal recirculation. This ULN burner system successfully uses turbine exhaust as an oxidizer, while achieving high efficiencies and low emissions. In tests at its laboratory facilities in Des Plaines, Illinois, GTI validated the ability of the system to achieve emissions of NOx, CO, and THC below the CARB criteria of 0.07, 0.10, and 0.02 lb/MW-h respectively. The FlexCHP system was installed at the field demonstration site, Inland Empire Foods, in Riverside, California to verify performance of the technology in an applied environment. The resulting Combined Heat and Power (CHP) package promises to make CHP implementation more attractive, mitigate greenhouse gas emissions, and improve the reliability of electricity supply.

  10. Cupola Furnace Computer Process Model

    SciTech Connect (OSTI)

    Seymour Katz

    2004-12-31

    The cupola furnace generates more than 50% of the liquid iron used to produce the 9+ million tons of castings annually. The cupola converts iron and steel into cast iron. The main advantages of the cupola furnace are lower energy costs than those of competing furnaces (electric) and the ability to melt less expensive metallic scrap than the competing furnaces. However the chemical and physical processes that take place in the cupola furnace are highly complex making it difficult to operate the furnace in optimal fashion. The results are low energy efficiency and poor recovery of important and expensive alloy elements due to oxidation. Between 1990 and 2004 under the auspices of the Department of Energy, the American Foundry Society and General Motors Corp. a computer simulation of the cupola furnace was developed that accurately describes the complex behavior of the furnace. When provided with the furnace input conditions the model provides accurate values of the output conditions in a matter of seconds. It also provides key diagnostics. Using clues from the diagnostics a trained specialist can infer changes in the operation that will move the system toward higher efficiency. Repeating the process in an iterative fashion leads to near optimum operating conditions with just a few iterations. More advanced uses of the program have been examined. The program is currently being combined with an ''Expert System'' to permit optimization in real time. The program has been combined with ''neural network'' programs to affect very easy scanning of a wide range of furnace operation. Rudimentary efforts were successfully made to operate the furnace using a computer. References to these more advanced systems will be found in the ''Cupola Handbook''. Chapter 27, American Foundry Society, Des Plaines, IL (1999).

  11. High Fidelity Simulations of Large-Scale Wireless Networks

    SciTech Connect (OSTI)

    Onunkwo, Uzoma; Benz, Zachary

    2015-11-01

    The worldwide proliferation of wireless connected devices continues to accelerate. There are 10s of billions of wireless links across the planet with an additional explosion of new wireless usage anticipated as the Internet of Things develops. Wireless technologies do not only provide convenience for mobile applications, but are also extremely cost-effective to deploy. Thus, this trend towards wireless connectivity will only continue and Sandia must develop the necessary simulation technology to proactively analyze the associated emerging vulnerabilities. Wireless networks are marked by mobility and proximity-based connectivity. The de facto standard for exploratory studies of wireless networks is discrete event simulations (DES). However, the simulation of large-scale wireless networks is extremely difficult due to prohibitively large turnaround time. A path forward is to expedite simulations with parallel discrete event simulation (PDES) techniques. The mobility and distance-based connectivity associated with wireless simulations, however, typically doom PDES and fail to scale (e.g., OPNET and ns-3 simulators). We propose a PDES-based tool aimed at reducing the communication overhead between processors. The proposed solution will use light-weight processes to dynamically distribute computation workload while mitigating communication overhead associated with synchronizations. This work is vital to the analytics and validation capabilities of simulation and emulation at Sandia. We have years of experience in Sandias simulation and emulation projects (e.g., MINIMEGA and FIREWHEEL). Sandias current highly-regarded capabilities in large-scale emulations have focused on wired networks, where two assumptions prevent scalable wireless studies: (a) the connections between objects are mostly static and (b) the nodes have fixed locations.

  12. SNF AGING SYSTEM DESCRIPTION DOCUMENT

    SciTech Connect (OSTI)

    L.L. Swanson

    2005-04-06

    The purpose of this system description document (SDD) is to establish requirements that drive the design of the spent nuclear fuel (SNF) aging system and associated bases, which will allow the design effort to proceed. This SDD will be revised at strategic points as the design matures. This SDD identifies the requirements and describes the system design, as it currently exists, with emphasis on attributes of the design provided to meet the requirements. This SDD is an engineering tool for design control; accordingly, the primary audience and users are design engineers. This SDD is part of an iterative design process. It leads the design process with regard to the flow down of upper tier requirements onto the system. Knowledge of these requirements is essential in performing the design process. The SDD follows the design with regard to the description of the system. The description provided in the SDD reflects the current results of the design process. Throughout this SDD, the term aging cask applies to vertical site-specific casks and to horizontal aging modules. The term overpack is a vertical site-specific cask that contains a dual-purpose canister (DPC) or a disposable canister. Functional and operational requirements applicable to this system were obtained from ''Project Functional and Operational Requirements'' (F&OR) (Curry 2004 [DIRS 170557]). Other requirements that support the design process were taken from documents such as ''Project Design Criteria Document'' (PDC) (BSC 2004 [DES 171599]), ''Site Fire Hazards Analyses'' (BSC 2005 [DIRS 172174]), and ''Nuclear Safety Design Bases for License Application'' (BSC 2005 [DIRS 171512]). The documents address requirements in the ''Project Requirements Document'' (PRD) (Canori and Leitner 2003 [DIRS 166275]). This SDD includes several appendices. Appendix A is a Glossary; Appendix B is a list of key system charts, diagrams, drawings, lists and additional supporting information; and Appendix C is a list of procedures that will be used to operate the system.

  13. TEXAS LPG FUEL CELL DEVELOPMENT AND DEMONSTRATION PROJECT Full-Text - Submission contains both citation data and full-text of the journal article. Full-text can be either a pre-print or post-print, but not the copyrighted article.

    SciTech Connect (OSTI)

    SOUTHWEST RESEARCH LABORATORY SUBMITTED BY SUBCONTRACTOR, RAILROAD COMMISSION OF TEXAS

    2004-07-26

    The State Energy Conservation Office has executed its first Fuel Cell Project which was awarded under a Department of Energy competitive grant process. The Texas LPG Fuel Processor Development and Fuel Cell Demonstration Program is a broad-based public/private partnership led by the Texas State Energy Conservation Office (SECO). Partners include the Alternative Fuels Research and Education Division (AFRED) of the Railroad Commission of Texas; Plug Power, Inc., Latham, NY, UOP/HyRadix, Des Plaines, IL; Southwest Research Institute (SwRI), San Antonio, TX; the Texas Natural Resource Conservation Commission (TNRCC), and the Texas Department of Transportation (TxDOT). The team proposes to mount a development and demonstration program to field-test and evaluate markets for HyRadix?s LPG fuel processor system integrated into Plug Power?s residential-scale GenSys? 5C (5 kW) PEM fuel cell system in a variety of building types and conditions of service. The program?s primary goal is to develop, test, and install a prototype propane-fueled residential fuel cell power system supplied by Plug Power and HyRadix in Texas. The propane industry is currently funding development of an optimized propane fuel processor by project partner UOP/HyRadix through its national checkoff program, the Propane Education and Research Council (PERC). Following integration and independent verification of performance by Southwest Research Institute, Plug Power and HyRadix will produce a production-ready prototype unit for use in a field demonstration. The demonstration unit produced during this task will be delivered and installed at the Texas Department of Transportation?s TransGuide headquarters in San Antonio, Texas. Simultaneously, the team will undertake a market study aimed at identifying and quantifying early-entry customers, technical and regulatory requirements, and other challenges and opportunities that need to be addressed in planning commercialization of the units. For further information please contact Mary-Jo Rowan at mary-jo.rowan@cpa.state.tx.us

  14. RECONSTRUCTING REDSHIFT DISTRIBUTIONS WITH CROSS-CORRELATIONS: TESTS AND AN OPTIMIZED RECIPE

    SciTech Connect (OSTI)

    Matthews, Daniel J.; Newman, Jeffrey A., E-mail: djm70@pitt.ed, E-mail: janewman@pitt.ed [Department of Physics and Astronomy, University of Pittsburgh, 3941 O'Hara Street, Pittsburgh, PA 15260 (United States)

    2010-09-20

    Many of the cosmological tests to be performed by planned dark energy experiments will require extremely well-characterized photometric redshift measurements. Current estimates for cosmic shear are that the true mean redshift of the objects in each photo-z bin must be known to better than 0.002(1 + z), and the width of the bin must be known to {approx}0.003(1 + z) if errors in cosmological measurements are not to be degraded significantly. A conventional approach is to calibrate these photometric redshifts with large sets of spectroscopic redshifts. However, at the depths probed by Stage III surveys (such as DES), let alone Stage IV (LSST, JDEM, and Euclid), existing large redshift samples have all been highly (25%-60%) incomplete, with a strong dependence of success rate on both redshift and galaxy properties. A powerful alternative approach is to exploit the clustering of galaxies to perform photometric redshift calibrations. Measuring the two-point angular cross-correlation between objects in some photometric redshift bin and objects with known spectroscopic redshift, as a function of the spectroscopic z, allows the true redshift distribution of a photometric sample to be reconstructed in detail, even if it includes objects too faint for spectroscopy or if spectroscopic samples are highly incomplete. We test this technique using mock DEEP2 Galaxy Redshift survey light cones constructed from the Millennium Simulation semi-analytic galaxy catalogs. From this realistic test, which incorporates the effects of galaxy bias evolution and cosmic variance, we find that the true redshift distribution of a photometric sample can, in fact, be determined accurately with cross-correlation techniques. We also compare the empirical error in the reconstruction of redshift distributions to previous analytic predictions, finding that additional components must be included in error budgets to match the simulation results. This extra error contribution is small for surveys that sample large areas of sky (>{approx}10{sup 0}-100{sup 0}), but dominant for {approx}1 deg{sup 2} fields. We conclude by presenting a step-by-step, optimized recipe for reconstructing redshift distributions from cross-correlation information using standard correlation measurements.

  15. DISCRETE ELEMENT MODELING OF BLADE–STRIKE FREQUENCY AND SURVIVAL OF FISH PASSING THROUGH HYDROKINETIC TURBINES

    SciTech Connect (OSTI)

    Romero Gomez, Pedro DJ; Richmond, Marshall C.

    2014-04-17

    Evaluating the consequences from blade-strike of fish on marine hydrokinetic (MHK) turbine blades is essential for incorporating environmental objectives into the integral optimization of machine performance. For instance, experience with conventional hydroelectric turbines has shown that innovative shaping of the blade and other machine components can lead to improved designs that generate more power without increased impacts to fish and other aquatic life. In this work, we used unsteady computational fluid dynamics (CFD) simulations of turbine flow and discrete element modeling (DEM) of particle motion to estimate the frequency and severity of collisions between a horizontal axis MHK tidal energy device and drifting aquatic organisms or debris. Two metrics are determined with the method: the strike frequency and survival rate estimate. To illustrate the procedure step-by-step, an exemplary case of a simple runner model was run and compared against a probabilistic model widely used for strike frequency evaluation. The results for the exemplary case showed a strong correlation between the two approaches. In the application case of the MHK turbine flow, turbulent flow was modeled using detached eddy simulation (DES) in conjunction with a full moving rotor at full scale. The CFD simulated power and thrust were satisfactorily comparable to experimental results conducted in a water tunnel on a reduced scaled (1:8.7) version of the turbine design. A cloud of DEM particles was injected into the domain to simulate fish or debris that were entrained into the turbine flow. The strike frequency was the ratio of the count of colliding particles to the crossing sample size. The fish length and approaching velocity were test conditions in the simulations of the MHK turbine. Comparisons showed that DEM-based frequencies tend to be greater than previous results from Lagrangian particles and probabilistic models, mostly because the DEM scheme accounts for both the geometric aspects of the passage event ---which the probabilistic method does--- as well as the fluid-particle interactions ---which the Lagrangian particle method does. The DEM-based survival rates were comparable to laboratory results for small fish but not for mid-size fish because of the considerably different turbine diameters. The modeling framework can be used for applications that aim at evaluating the biological performance of MHK turbine units during the design phase and to provide information to regulatory agencies needed for the environmental permitting process.

  16. Final Report for Research in High Energy Physics at the University of Pennsylvania for the period ending April 30, 2012

    SciTech Connect (OSTI)

    Williams, Hugh H.; Balasubramanian, V.; Bernstein, G.; Beier, E. W.; Cvetiˇc, M.; Gladney, L.; Jain, B.; Klein, J.; Kroll, J.; Lipeles, E.; Ovrut, B.; Thomson, E.

    2015-07-23

    The University of Pennsylvania elementary particle physics/particle cosmology group, funded by the Department of Energy Office of Science, participates in research in high energy physics and particle cosmology that addresses some of the most important unanswered questions in science. The research is divided into five areas. Energy Frontier - We participate in the study of proton-proton collisions at the Large Hadron Collider in Geneva, Switzerland using the ATLAS detector. The University of Pennsylvania group was responsible for the design, installation, and commissioning of the front-end electronics for the Transition Radiation Tracker (TRT) and plays the primary role in its maintenance and operation. We play an important role in the triggering of ATLAS, and we have made large contributions to the TRT performance and to the study and identification of electrons, photons, and taus. We have been actively involved in searches for the Higgs boson and for SUSY and other exotic particles. We have made significant contributions to measurement of Standard Model processes such as inclusive photon production and WW pair production. We also have participated significantly in R&D for upgrades to the ATLAS detector. Cosmic Frontier - The Dark Energy Survey (DES) telescope will be used to elucidate the nature of dark energy and the distribution of dark matter. Penn has played a leading role both in the use of weak gravitational lensing of distant galaxies and the discovery of large numbers of distant supernovae. The techniques and forecasts developed at Penn are also guiding the development of the proposed Large Synoptic Survey Telescope (LSST).We are also developing a new detector, MiniClean, to search for direct detection of dark matter particles. Intensity Frontier - We are participating in the design and R&D of detectors for the Long Baseline Neutrino Experiment (now DUNE), a new experiment to study the properties of neutrinos. Advanced Techology R&D - We have an extensive involvement in electronics required for sophisticated new detectors at the LHC and are developing electronics for the LSST camera. Theoretical Physics - We are carrying out a broad program studying the fundamental forces of nature and early universe cosmology and mathematical physics. Our activities span the range from model building, formal field theory, and string theory to new paradigms for cosmology and the interface of string theory with mathematics. Our effort combines extensive development of the formal aspects of string theory with a focus on real phenomena in particle physics, cosmology and gravity.

  17. HR Public meeting

    ScienceCinema (OSTI)

    None

    2011-10-06

    Cher(e)s collègues, En collaboration avec le Département HR, le Directeur général a le plaisir de vous convier à une réunion publique qui se tiendra le vendredi 25 juin 2010 à 9h30 dans l?Amphithéâtre principal (Bâtiment 500)*. Un café d?accueil y sera servi à partir de 9h. Cette réunion abordera les thèmes suivants : ? Valeurs de l?Organisation (Directeur général) ? Code de Conduite (Directeur général / Anne-Sylvie Catherin) ? Création du nouveau rôle d?Ombudsperson (Vincent Vuillemin) Ces présentations seront suivies d?une séance de questions-réponses. Nous espérons vous retrouver nombreux le 25 juin ! Meilleures salutations, Anne-Sylvie Catherin Chef du Département des Ressources humaines *Cette réunion sera retransmise simultanément dans l?Amphithéâtre BE de Prévessin (Bâtiment 864) et également disponible à l?adresse suivante : http://webcast.cern.ch -------------------------------------------------------- Dear colleagues, In collaboration with HR Department, the Director-General would like to invite you to an information meeting which will be held on Friday 25 June 2010 at 9:30 am in the Main Auditorium (Building 500)*. A welcome coffee will be available from 9:00 am. During this meeting, information will be given about: ? Organization?s values (Director-General) ? Code of Conduct (Director-General / Anne-Sylvie Catherin) ? New Ombudsperson role (Vincent Vuillemin) These presentations will be followed by a questions & answers session. We look forward to seeing you all on 25 June! Best regards, Anne-Sylvie Catherin Head, Human Resources Department *This meeting will be simultaneously retransmitted in BE Auditorium (Building 864) and available at the following address: http://webcast.cern.ch.

  18. Magnified Weak Lensing Cross Correlation Tomography

    SciTech Connect (OSTI)

    Ulmer, Melville P., Clowe, Douglas I.

    2010-11-30

    This project carried out a weak lensing tomography (WLT) measurement around rich clusters of galaxies. This project used ground based photometric redshift data combined with HST archived cluster images that provide the WLT and cluster mass modeling. The technique has already produced interesting results (Guennou et al, 2010,Astronomy & Astrophysics Vol 523, page 21, and Clowe et al, 2011 to be submitted). Guennou et al have validated that the necessary accuracy can be achieved with photometric redshifts for our purposes. Clowe et al titled "The DAFT/FADA survey. II. Tomographic weak lensing signal from 10 high redshift clusters," have shown that for the **first time** via this purely geometrical technique, which does not assume a standard rod or candle, that a cosmological constant is **required** for flat cosmologies. The intent of this project is not to produce the best constraint on the value of the dark energy equation of state, w. Rather, this project is to carry out a sustained effort of weak lensing tomography that will naturally feed into the near term Dark Energy Survey (DES) and to provide invaluable mass calibration for that project. These results will greatly advance a key cosmological method which will be applied to the top-rated ground-based project in the Astro2020 decadal survey, LSST. Weak lensing tomography is one of the key science drivers behind LSST. CO-I Clowe is on the weak lensing LSST committee, and senior scientist on this project, at FNAL James Annis, plays a leading role in the DES. This project has built on successful proposals to obtain ground-based imaging for the cluster sample. By 1 Jan, it is anticipated the project will have accumulated complete 5-color photometry on 30 (or about 1/3) of the targeted cluster sample (public webpage for the survey is available at http://cencos.oamp.fr/DAFT/ and has a current summary of the observational status of various clusters). In all, the project has now been awarded the equivalent of over 60 nights on 4-m class telescopes, which gives concrete evidence of strong community support for this project. The WLT technique is based on the dependence of the gravitational shear signal on the angular diameter distances between the observer, the lens, and the lensed galaxy to measure cosmological parameters. By taking the ratio of measured shears of galaxies with different redshifts around the same lens, one obtains a measurement of the ratios of the angular diameter distances involved. Making these observations over a large range of lenses and background galaxy redshifts will measure the history of the expansion rate of the universe. Because this is a purely geometric measurement, it is insensitive to any form of evolution of objects or the necessity to understand the physics in the early universe. Thus, WLT was identified by the Dark Energy Task Force as perhaps the best method to measure the evolution of DE. To date, however, the conjecture of the DETF has not been experimentally verified, but will be by the proposed project. The primary reason for the lack of tomography measurements is that one must have an exceptional data-set to attempt the measurement. One needs both extremely good seeing (or space observations) in order to minimize the point spread function smearing corrections on weak lensing shear measurements and deep, multi-color data, from B to z, to measure reliable photometric redshifts of the background galaxies being lensed (which are typically too faint to obtain spectroscopic redshifts). Because the entire process from multi-drizzling the HST images, and then creating shear maps, to gathering the necessary ground based observations, to generating photo-zs and then carrying out the tomography is a complicated task, until the creation of our team, nobody has taken the time to connect all the levels of expertise necessary to carry out this project based on HST archival data. Our data are being used in 2 Ph.D. theses. Kellen Murphy, at Ohio University, is using the tomography data along with simulations in a thesis expected to be completed in Jun

  19. Enhanced vector borne disease surveillance of California Culex mosquito populations reveals spatial and species-specific barriers of infection.

    SciTech Connect (OSTI)

    VanderNoot, Victoria A.; Curtis, Deanna Joy; Koh, Chung-Yan; Brodsky, Benjamin H; Lane, Todd

    2014-08-01

    Monitor i ng in f ectio n s in v ect o rs su c h as m osquit o es, s a nd fl i es, tsetse fl i es, a nd ticks to i denti f y hu m a n path o gens m a y s e r v e as a n ear l y w arn i ng det e ction system t o dir e ct loc a l g o v er n ment dise a se pr e v en t i v e m easu r e s . One major hurdle i n de t ection is the abi l i t y to scre e n l arge n u mbers of v e c t ors for h uman patho g ens w i thout t h e u s e of ge n o t y pe - s p ecific m o lecu l ar tec h nique s . N e x t genera t ion s equ e nc i ng (NG S ) pr o v i des a n unbi a sed p latfo r m capab l e of identi f y i ng k n o w n a n d unk n o w n p ath o ge n s circula t ing w i thin a v e ctor p opul a tion, but utili z ing t h is te c h nolo g y i s tim e - con s u ming a n d cos t l y for v ecto r -b o rne disease su r v e illan c e pr o gra m s. T o addr e s s this w e d e v e lop e d cos t -eff e ct i v e Ilumina(r) R NA- S eq l i bra r y p r epara t ion m e thodol o gies i n con j u n ction w i t h an automa t ed c ompu t at i onal a n a l y sis pipel i n e to ch a racter i ze t h e microbial popula t ions c ircula t i n g in Cu l e x m o squit o e s (Cul e x qui n quef a s c iatu s , C ul e x quinq u efasc i atus / pip i ens co m pl e x h y bri d s, and C u l e x ta r salis ) t hroug h out Californ i a. W e assembled 2 0 n o vel a n d w e l l -do c ume n ted a r b o v i ruses repres e nting mem b e rs of B u n y a v ir i da e , F l a v i virid a e, If a virida e , Meson i v i rida e , Nid o v iri d ae, O rtho m y x o virid a e, Pa r v o v iri d ae, Re o virid a e, R h a b d o v i rid a e, T y m o v iri d ae, a s w ell as s e v e r al u n assi g n e d v irus e s . In addit i o n, w e m app e d mRNA s pecies to d i vergent s peci e s of t r y panos o ma a nd pl a s modium eu k a r yotic parasit e s and cha r a c terized t he p r oka r yot i c microb i al c o mposit i on to i d enti f y bacteri a l tran s c r ipts der i v ed from wolba c hia, clo s tridi u m, m y c oplas m a, fusoba c terium and c am p y l o bacter bac t er i al spec i e s . W e utilized the s e mic r obial transcri p tomes pre s e nt in g e ogra p hical l y defined Cul e x po p ul a tions to defi n e spatial and m osqui t o specie s -spec i fic ba r r iers of i n fecti o n. T he v i r ome and microbi o me c o mpos i tion id e ntified in e ach mosqui t o p o ol pr o v i ded suf f icient resolut i on to dete r m i ne both the mosq u ito species and the g e o graphic regi o n in Californ i a w h e re t h e mosqui t o po o l orig i n ated. T his d a ta pr o v i des ins i ght in t o the compl e x i t y of microb i al spec i es cir c ulati n g in med i cal l y i mport a nt Culex mosqui t oes a nd t h eir potent i al im p act o n t he tran s missi o n of v ector-b o rne human / veter i na r y p a t hogens in C a liforn i a.

  20. Advancement of High Temperature Black Liquor Gasification Technology

    SciTech Connect (OSTI)

    Craig Brown; Ingvar Landalv; Ragnar Stare; Jerry Yuan; Nikolai DeMartini; Nasser Ashgriz

    2008-03-31

    Weyerhaeuser operates the world's only commercial high-temperature black liquor gasifier at its pulp mill in New Bern, NC. The unit was started-up in December 1996 and currently processes about 15% of the mill's black liquor. Weyerhaeuser, Chemrec AB (the gasifier technology developer), and the U.S. Department of Energy recognized that the long-term, continuous operation of the New Bern gasifier offered a unique opportunity to advance the state of high temperature black liquor gasification toward the commercial-scale pressurized O2-blown gasification technology needed as a foundation for the Forest Products Bio-Refinery of the future. Weyerhaeuser along with its subcontracting partners submitted a proposal in response to the 2004 joint USDOE and USDA solicitation - 'Biomass Research and Development Initiative'. The Weyerhaeuser project 'Advancement of High Temperature Black Liquor Gasification' was awarded USDOE Cooperative Agreement DE-FC26-04NT42259 in November 2004. The overall goal of the DOE sponsored project was to utilize the Chemrec{trademark} black liquor gasification facility at New Bern as a test bed for advancing the development status of molten phase black liquor gasification. In particular, project tasks were directed at improvements to process performance and reliability. The effort featured the development and validation of advanced CFD modeling tools and the application of these tools to direct burner technology modifications. The project also focused on gaining a fundamental understanding and developing practical solutions to address condensate and green liquor scaling issues, and process integration issues related to gasifier dregs and product gas scrubbing. The Project was conducted in two phases with a review point between the phases. Weyerhaeuser pulled together a team of collaborators to undertake these tasks. Chemrec AB, the technology supplier, was intimately involved in most tasks, and focused primarily on the design, specification and procurement of facility upgrades. Chemrec AB is also operating a pressurized, O2-blown gasifier pilot facility in Piteaa, Sweden. There was an exchange of knowledge with the pressurized projects including utilization of the experimental results from facilities in Piteaa, Sweden. Resources at the Georgia Tech Research Corporation (GTRC, a.k.a., the Institute of Paper Science and Technology) were employed primarily to conduct the fundamental investigations on scaling and plugging mechanisms and characterization of green liquor dregs. The project also tapped GTRC expertise in the development of the critical underlying black liquor gasification rate subroutines employed in the CFD code. The actual CFD code development and application was undertaken by Process Simulation, Ltd (PSL) and Simulent, Ltd. PSL focused on the overall integrated gasifier CFD code, while Simulent focused on modeling the black liquor nozzle and description of the black liquor spray. For nozzle development and testing Chemrec collaborated with ETC (Energy Technology Centre) in Piteae utilizing their test facility for nozzle spray investigation. GTI (Gas Technology Institute), Des Plains, IL supported the team with advanced gas analysis equipment during the gasifier test period in June 2005.

  1. Corrective Action Investigation Plan for Corrective Action Unit 309: Area 12 Muckpiles, Nevada Test Site, Nevada, Rev. No. 0

    SciTech Connect (OSTI)

    Robert F. Boehlecke

    2004-12-01

    This Corrective Action Investigation Plan (CAIP) for Corrective Action Unit (CAU) 309, Area 12 Muckpiles, Nevada Test Site (NTS), Nevada, has been developed in accordance with the ''Federal Facility Agreement and Consent Order'' (FFACO) that was agreed to by the State of Nevada, the U.S. Department of Energy, and the U.S. Department of Defense. The general purpose of the investigation is to ensure that adequate data are collected to provide sufficient and reliable information to identify, evaluate, and select technically viable corrective actions. Corrective Action Unit 309 is comprised of the following three corrective action sites (CASs) in Area 12 of the NTS: (1) CAS 12-06-09, Muckpile; (2) CAS 12-08-02, Contaminated Waste Dump (CWD); and (3) CAS 12-28-01, I-, J-, and K-Tunnel Debris. Corrective Action Site 12-06-09 consists of a muckpile and debris located on the hillside in front of the I-, J-, and K-Tunnels on the eastern slopes of Rainier Mesa in Area 12. The muckpile includes mining debris (muck) and debris generated during the excavation and construction of the I-, J-, and K-Tunnels. Corrective Action Site 12-08-02, CWD, consists of a muckpile and debris and is located on the hillside in front of the re-entry tunnel for K-Tunnel. For the purpose of this investigation CAS 12-28-01 is defined as debris ejected by containment failures during the Des Moines and Platte Tests and the associated contamination that is not covered in the two muckpile CASs. This site consists of debris scattered south of the I-, J-, and K-Tunnel muckpiles and extends down the hillside, across the valley, and onto the adjacent hillside to the south. In addition, the site will cover the potential contamination associated with ''ventings'' along the fault, fractures, and various boreholes on the mesa top and face. One conceptual site model was developed for all three CASs to address possible contamination migration pathways associated with CAU 309. The data quality objective (DQO) process was used to identify and define the type, quantity, and quality of data needed to complete the investigation phase of the corrective action process. The DQO process addresses the primary problem that sufficient information is not available to determine the appropriate corrective action for the CAU. Due to the practical constraints posed by steep slopes on and around the CAU 309 muckpiles, a conservative, simplifying strategy was developed to resolve the presence and nature of contaminants. This strategy includes the use of historical data from similar sites (i.e., previously investigated NTS muckpiles) and the collection of samples from accessible areas of the muckpiles. Based on site history, process knowledge, and previous investigations of similar sites, contaminants of potential concern for CAU 309 collectively include radionuclides, total petroleum hydrocarbons (diesel range only), polychlorinated biphenyls, ''Resource Conservation and Recovery Act'' metals, volatile organic compounds, and semivolatile organic compounds.

  2. SRNL SHELF LIFE STUDIES - SCC STUDIES AT ROOM TEMPERTURE [stress corrosion cracking

    SciTech Connect (OSTI)

    Mickalonis, J.; Duffey, J.

    2014-11-12

    Phase II, Series 2 corrosion testing performed by the Savannah River National Laboratory (SRNL) for the Department of Energy 3013 container has been completed. The corrosion tests are part of an integrated plan conducted jointly by Los Alamos National Laboratory and the Savannah River Site. SRNL was responsible for conducting corrosion studies in small-scale vessels to address the influence of salt composition, water loading, and type of oxide/salt contact on the relative humidity inside a 3013 container and on the resulting corrosion of Type 304L and 316L stainless steel (304L and 316L). This testing was conducted in two phases: Phase I evaluated a broad spectrum of salt compositions and initial water loadings on the salt mixtures exposed to 304L and 316L and the resulting corrosion; Phase II evaluated the corrosion of 304L at specific water loadings and a single salt composition. During Phase I testing at high initial moisture levels (0.35 to 1.24 wt%)a, the roomtemperature corrosion of 304L exposed to a series of plutonium oxide/chloride salt mixtures ranged from superficial staining to pitting and stress corrosion cracking (SCC). 304L teardrop coupons that exhibited SCC were directly exposed to a mixture composed of 98 wt % PuO2, 0.9 wt % NaCl, 0.9 wt % KCl, and 0.2 wt % CaCl2. Cracking was not observed in a 316L teardrop coupon. Pitting was also observed in this environment for both 304L and 316L with depths ranging from 20 to 100 ?m. Neither pitting nor SCC was observed in mixtures with a greater chloride salt concentration (5 and 28 wt%). These results demonstrated that for a corrosive solution to form a balance existed between the water loading and the salt chloride concentration. This chloride solution results from the interaction of loaded water with the hydrating CaCl2 salt. In Phase II, Series 1 tests, the SCC results were shown to be reproducible with cracking occurring in as little as 85 days. The approximate 0.5 wt% moisture level was found to result in an initial relative humidity of ~55% within the small-scale vessels. Pits were found to be associated with cracks and appeared to act as initiators for the cracking. In a vapor-space only exposure, the weld oxide, which results from the TIG closure weld used to fabricate the teardrop coupon, was also shown to be more susceptible to pitting corrosion than a surface free from weld oxide. This result has important implications for the closure weld of the 3013 inner can since the weld oxide on the can internal surface cannot be removed. The results from the Phase II, Series 2 tests further demonstrated the significance of forming a solution with a critical chloride concentration for corrosion to proceed. 304L teardrop coupons were found to corrode only by pitting with a similar oxide/salt mixture as used in Series 1 testing but with a lower water loading of 0.2 wt%, which resulted in an initial relative humidity of 35-38%. These tests ran twice as long as those for Series 1 testing. The exposure condition was also found to impact the corrosion with salt-exposed surfaces showing lower corrosion resistance. Additional analyses of the Series 2 coupons are recommended especially for determining if cracks emanate from the bottom of pits. Data generated under the 2009 3013 corrosion test plan, as was presented here, increased the understanding of the corrosion process within a sealed 3013 container. Along with the corrosion data from destructive evaluations of 3013 containers, the inner can closure weld region (ICCWR) has been identified as the most vulnerable area of the inner can where corrosion may lead to corrosive species leaking to the interior surface of the outer container, thereby jeopardizing the integrity of the 3013 container. A new corrosion plan has been designed that will characterize the corrosion at the ICCWR of 3013 DEs as well as parameters affecting this corrosion.

  3. Spectroscopic Needs for Imaging Dark Energy Experiments

    SciTech Connect (OSTI)

    Newman, Jeffrey A.; Slosar, Anze; Abate, Alexandra; Abdalla, Filipe B.; Allam, Sahar; Allen, Steven W.; Ansari, Reza; Bailey, Stephen; Barkhouse, Wayne A.; Beers, Timothy C.; Blanton, Michael R.; Brodwin, Mark; Brownstein, Joel R.; Brunner, Robert J.; Carrasco-Kind, Matias; Cervantes-Cota, Jorge; Chisari, Nora Elisa; Colless, Matthew; Comparat, Johan; Coupon, Jean; Cheu, Elliott; Cunha, Carlos E.; de la Macorra, Alex; DellAntonio, Ian P.; Frye, Brenda L.; Gawiser, Eric J.; Gehrels, Neil; Grady, Kevin; Hagen, Alex; Hall, Patrick B.; Hearin, Andrew P.; Hildebrandt, Hendrik; Hirata, Christopher M.; Ho, Shirley; Honscheid, Klaus; Huterer, Dragan; Ivezic, Zeljko; Kneib, Jean -Paul; Kruk, Jeffrey W.; Lahav, Ofer; Mandelbaum, Rachel; Marshall, Jennifer L.; Matthews, Daniel J.; Menard, Brice; Miquel, Ramon; Moniez, Marc; Moos, H. W.; Moustakas, John; Papovich, Casey; Peacock, John A.; Park, Changbom; Rhodes, Jason; Sadeh, Iftach; Schmidt, Samuel J.; Stern, Daniel K.; Tyson, J. Anthony; von der Linden, Anja; Wechsler, Risa H.; Wood-Vasey, W. M.; Zentner, A.

    2015-03-15

    Ongoing and near-future imaging-based dark energy experiments are critically dependent upon photometric redshifts (a.k.a. photo-zs): i.e., estimates of the redshifts of objects based only on flux information obtained through broad filters. Higher-quality, lower-scatter photo-zs will result in smaller random errors on cosmological parameters; while systematic errors in photometric redshift estimates, if not constrained, may dominate all other uncertainties from these experiments. The desired optimization and calibration is dependent upon spectroscopic measurements for secure redshift information; this is the key application of galaxy spectroscopy for imaging-based dark energy experiments. Hence, to achieve their full potential, imaging-based experiments will require large sets of objects with spectroscopically-determined redshifts, for two purposes: Training: Objects with known redshift are needed to map out the relationship between object color and z (or, equivalently, to determine empirically-calibrated templates describing the rest-frame spectra of the full range of galaxies, which may be used to predict the color-z relation). The ultimate goal of training is to minimize each moment of the distribution of differences between photometric redshift estimates and the true redshifts of objects, making the relationship between them as tight as possible. The larger and more complete our training set of spectroscopic redshifts is, the smaller the RMS photo-z errors should be, increasing the constraining power of imaging experiments; Requirements: Spectroscopic redshift measurements for ~30,000 objects over >~15 widely-separated regions, each at least ~20 arcmin in diameter, and reaching the faintest objects used in a given experiment, will likely be necessary if photometric redshifts are to be trained and calibrated with conventional techniques. Larger, more complete samples (i.e., with longer exposure times) can improve photo-z algorithms and reduce scatter further, enhancing the science return from planned experiments greatly (increasing the Dark Energy Task Force figure of merit by up to ~50%); Options: This spectroscopy will most efficiently be done by covering as much of the optical and near-infrared spectrum as possible at modestly high spectral resolution (?/?? > ~3000), while maximizing the telescope collecting area, field of view on the sky, and multiplexing of simultaneous spectra. The most efficient instrument for this would likely be either the proposed GMACS/MANIFEST spectrograph for the Giant Magellan Telescope or the OPTIMOS spectrograph for the European Extremely Large Telescope, depending on actual properties when built. The PFS spectrograph at Subaru would be next best and available considerably earlier, c. 2018; the proposed ngCFHT and SSST telescopes would have similar capabilities but start later. Other key options, in order of increasing total time required, are the WFOS spectrograph at TMT, MOONS at the VLT, and DESI at the Mayall 4 m telescope (or the similar 4MOST and WEAVE projects); of these, only DESI, MOONS, and PFS are expected to be available before 2020. Table 2-3 of this white paper summarizes the observation time required at each facility for strawman training samples. To attain secure redshift measurements for a high fraction of targeted objects and cover the full redshift span of future experiments, additional near-infrared spectroscopy will also be required; this is best done from space, particularly with WFIRST-2.4 and JWST; Calibration: The first several moments of redshift distributions (the mean, RMS redshift dispersion, etc.), must be known to high accuracy for cosmological constraints not to be systematics-dominated (equivalently, the moments of the distribution of differences between photometric and true redshifts could be determined instead). The ultimate goal of calibration is to characterize these moments for every subsample used in analyses - i.e., to minimize the uncertainty in their mean redshift, RMS dispersion, etc. rather than to make the moments themselves small. Calibration may be done with the same spectroscopic dataset used for training if that dataset is extremely high in redshift completeness (i.e., no populations of galaxies to be used in analyses are systematically missed). Accurate photo-z calibration is necessary for all imaging experiments; Requirements: If extremely low levels of systematic incompleteness (<~0.1%) are attained in training samples, the same datasets described above should be sufficient for calibration. However, existing deep spectroscopic surveys have failed to yield secure redshifts for 3060% of targets, so that would require very large improvements over past experience. This incompleteness would be a limiting factor for training, but catastrophic for calibration. If <~0.1% incompleteness is not attainable, the best known option for calibration of photometric redshifts is to utilize cross-correlation statistics in some form. The most direct method for this uses cross-correlations between positions on the sky of bright objects of known spectroscopic redshift with the sample of objects that we wish to calibrate the redshift distribution for, measured as a function of spectroscopic z. For such a calibration, redshifts of ~100,000 objects over at least several hundred square degrees, spanning the full redshift range of the samples used for dark energy, would be necessary; and Options: The proposed BAO experiment eBOSS would provide sufficient spectroscopy for basic calibrations, particularly for ongoing and near-future imaging experiments. The planned DESI experiment would provide excellent calibration with redundant cross-checks, but will start after the conclusion of some imaging projects. An extension of DESI to the Southern hemisphere would provide the best possible calibration from cross-correlation methods for DES and LSST. We thus anticipate that our two primary needs for spectroscopy training and calibration of photometric redshifts will require two separate solutions. For ongoing and future projects to reach their full potential, new spectroscopic samples of faint objects will be needed for training; those new samples may be suitable for calibration, but the latter possibility is uncertain. In contrast, wide-area samples of bright objects are poorly suited for training, but can provide high-precision calibrations via cross-correlation techniques. Additional training/calibration redshifts and/or host galaxy spectroscopy would enhance the use of supernovae and galaxy clusters for cosmology. We also summarize additional work on photometric redshift techniques that will be needed to prepare for data from ongoing and future dark energy experiments.

  4. 11,23,1,1,,19,10,"BANGOR HYDRO ELECTRIC CO","ELLSWORTH",0,,1179,"0A",1294,,,95,2941,0,0,3518,0,0,4870,0,0,1732,0,0,3252,0,0,2193,0,0,134,0,0,447,0,0,465,0,0,538,0,0,4295,0,0,3601,0,0,1469,6,50159,"WAT","HY"

    U.S. Energy Information Administration (EIA) Indexed Site

    NAD_UTIL","FILLER","EFFDATE","STATUS","MULTIST","YEAR","GEN01","CON01","STK01","GEN02","CON02","STK02","GEN03","CON03","STK03","GEN04","CON04","STK04","GEN05","CON05","STK05","GEN06","CON06","STK06","GEN07","CON07","STK07","GEN08","CON08","STK08","GEN09","CON09","STK09","GEN10","CON10","STK10","GEN11","CON11","STK11","GEN12","CON12","STK12","PCODE","NERC","UTILCODE","FUELDESC","PMDESC" 11,23,1,1,,19,10,"BANGOR HYDRO ELECTRIC CO","ELLSWORTH",0,,1179,"0A",1294,,,95,2941,0,0,3518,0,0,4870,0,0,1732,0,0,3252,0,0,2193,0,0,134,0,0,447,0,0,465,0,0,538,0,0,4295,0,0,3601,0,0,1469,6,50159,"WAT","HY" 11,23,1,1,,19,15,"BANGOR HYDRO ELECTRIC CO","HOWLAND",0,,1179,"0A",1294,,,95,772,0,0,858,0,0,1012,0,0,727,0,0,1061,0,0,917,0,0,385,0,0,118,0,0,0,0,0,657,0,0,905,0,0,820,0,0,1472,6,50159,"WAT","HY" 11,23,1,1,,19,30,"BANGOR HYDRO ELECTRIC CO","MEDWAY",0,,1179,"0A",1294,,,95,2116,0,0,1715,0,0,1459,0,0,1821,0,0,1946,0,0,2134,0,0,2157,0,0,1797,0,0,1745,0,0,1829,0,0,2224,0,0,2386,0,0,1474,6,50159,"WAT","HY" 11,23,1,3,2,19,30,"BANGOR HYDRO ELECTRIC CO","MEDWAY",0,"LIGHT OIL",1179,"0A",1294,,,95,0,0,553,181,307,419,0,0,593,31,55,538,66,120,418,219,399,383,324,598,481,313,579,614,97,178,575,1,2,573,0,0,608,98,171,611,1474,6,50159,"FO2","IC" 11,23,1,1,,19,35,"BANGOR HYDRO ELECTRIC CO","MILFORD",0,,1179,"0A",1294,,,95,3843,0,0,3348,0,0,4177,0,0,3759,0,0,4855,0,0,4740,0,0,2971,0,0,2432,0,0,1786,0,0,1561,0,0,3510,0,0,4606,0,0,1475,6,50159,"WAT","HY" 11,23,1,1,,19,45,"BANGOR HYDRO ELECTRIC CO","ORONO",0,,1179,"0A",1294,,,95,895,0,0,836,0,0,966,0,0,576,0,0,624,0,0,736,0,0,684,0,0,464,0,0,408,0,0,616,0,0,849,0,0,896,0,0,1476,6,50159,"WAT","HY" 11,23,1,1,,19,55,"BANGOR HYDRO ELECTRIC CO","STILLWATER",0,,1179,"0A",1294,,,95,1191,0,0,844,0,0,939,0,0,1021,0,0,1114,0,0,1181,0,0,1170,0,0,878,0,0,818,0,0,880,0,0,923,0,0,950,0,0,1478,6,50159,"WAT","HY" 11,23,1,1,,19,60,"BANGOR HYDRO ELECTRIC CO","VEAZIE A",0,,1179,"0A",1294,,,95,4314,0,0,3855,0,0,5043,0,0,5153,0,0,6053,0,0,5342,0,0,3542,0,0,2651,0,0,2281,0,0,3932,0,0,5128,0,0,3842,0,0,1479,6,50159,"WAT","HY" 11,23,1,1,,19,62,"BANGOR HYDRO ELECTRIC CO","VEAZIE B",0,,1179,"0A",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,7199,6,50159,"WAT","HY" 11,23,1,3,2,19,68,"BANGOR HYDRO ELECTRIC CO","BAR HARBOR",0,"LIGHT OIL",1179,"0A",1294,,,95,42,73,538,379,659,574,0,0,574,73,128,446,69,125,512,225,420,440,312,579,556,449,813,455,32,60,586,49,89,497,6,10,487,152,264,571,1466,6,50159,"FO2","IC" 11,23,1,3,2,19,75,"BANGOR HYDRO ELECTRIC CO","EASTPORT",0,"LIGHT OIL",1179,"0A",1294,,,95,39,70,576,80,139,412,0,0,586,10,18,557,32,58,494,111,204,464,172,317,495,182,334,509,19,36,472,0,0,470,15,29,429,67,117,460,1468,6,50159,"FO2","IC" 11,23,1,1,,37,5,"CENTRAL MAINE POWER CO","ANDROSCOG 3",0,,3266,"0M",1294,,,95,2536,0,0,2573,0,0,2732,0,0,2703,0,0,2639,0,0,2235,0,0,2379,0,0,2201,0,0,1657,0,0,2352,0,0,2282,0,0,2805,0,0,1480,6,50491,"WAT","HY" 11,23,1,1,,37,10,"CENTRAL MAINE POWER CO","BAR MILLS",0,,3266,"0M",1294,,,95,2420,0,0,1389,0,0,2414,0,0,2364,0,0,2584,0,0,1195,0,0,623,0,0,586,0,0,293,0,0,1310,0,0,2401,0,0,2056,0,0,1481,6,50491,"WAT","HY" 11,23,1,1,,37,20,"CENTRAL MAINE POWER CO","BONNY EAGLE",0,,3266,"0M",1294,,,95,6041,0,0,3654,0,0,5858,0,0,5255,0,0,4575,0,0,2217,0,0,1233,0,0,1084,0,0,592,0,0,3323,0,0,7098,0,0,4100,0,0,1482,6,50491,"WAT","HY" 11,23,1,1,,37,40,"CENTRAL MAINE POWER CO","CATARACT",0,,3266,"0M",1294,,,95,5330,0,0,4194,0,0,4953,0,0,4656,0,0,4888,0,0,5331,0,0,818,0,0,662,0,0,102,0,0,2232,0,0,5064,0,0,4090,0,0,1486,6,50491,"WAT","HY" 11,23,1,1,,37,42,"CENTRAL MAINE POWER CO","CONTINENTAL",0,,3266,"0M",1294,,,95,-14,0,0,-15,0,0,322,0,0,72,0,0,147,0,0,12,0,0,3,0,0,13,0,0,15,0,0,109,0,0,555,0,0,-18,0,0,1487,6,50491,"WAT","HY" 11,23,1,1,,37,50,"CENTRAL MAINE POWER CO","DEER RIP 1",0,,3266,"0M",1294,,,95,2694,0,0,2434,0,0,4080,0,0,3776,0,0,4034,0,0,2023,0,0,686,0,0,215,0,0,83,0,0,1916,0,0,3984,0,0,3453,0,0,1488,6,50491,"WAT","HY" 11,23,1,1,,37,60,"CENTRAL MAINE POWER CO","FT HALIFAX",0,,3266,"0M",1294,,,95,959,0,0,424,0,0,1026,0,0,961,0,0,925,0,0,526,0,0,51,0,0,5,0,0,155,0,0,380,0,0,977,0,0,659,0,0,1490,6,50491,"WAT","HY" 11,23,1,1,,37,75,"CENTRAL MAINE POWER CO","GULF ISLAND",0,,3266,"0M",1294,,,95,10764,0,0,9131,0,0,13512,0,0,13282,0,0,13485,0,0,8299,0,0,5537,0,0,4070,0,0,2892,0,0,9130,0,0,15549,0,0,11464,0,0,1491,6,50491,"WAT","HY" 11,23,1,1,,37,80,"CENTRAL MAINE POWER CO","HARRIS",0,,3266,"0M",1294,,,95,14325,0,0,24479,0,0,22937,0,0,6538,0,0,5448,0,0,21283,0,0,13285,0,0,11928,0,0,12813,0,0,10770,0,0,19708,0,0,26783,0,0,1492,6,50491,"WAT","HY" 11,23,1,1,,37,85,"CENTRAL MAINE POWER CO","HIRAM",0,,3266,"0M",1294,,,95,5791,0,0,3447,0,0,5873,0,0,6762,0,0,6516,0,0,2778,0,0,1397,0,0,1182,0,0,155,0,0,2992,0,0,7160,0,0,4285,0,0,1493,6,50491,"WAT","HY" 11,23,1,1,,37,90,"CENTRAL MAINE POWER CO","MESALONSK 2",0,,3266,"0M",1294,,,95,1280,0,0,585,0,0,1625,0,0,606,0,0,869,0,0,350,0,0,2,0,0,-1,0,0,9,0,0,710,0,0,1668,0,0,745,0,0,1497,6,50491,"WAT","HY" 11,23,1,1,,37,95,"CENTRAL MAINE POWER CO","MESALONSK 3",0,,3266,"0M",1294,,,95,753,0,0,330,0,0,977,0,0,349,0,0,507,0,0,180,0,0,0,0,0,-6,0,0,0,0,0,414,0,0,1038,0,0,416,0,0,1498,6,50491,"WAT","HY" 11,23,1,1,,37,100,"CENTRAL MAINE POWER CO","MESALONSK 4",0,,3266,"0M",1294,,,95,405,0,0,183,0,0,451,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1499,6,50491,"WAT","HY" 11,23,1,1,,37,105,"CENTRAL MAINE POWER CO","MESALONSK 5",0,,3266,"0M",1294,,,95,699,0,0,292,0,0,0,0,0,378,0,0,0,0,0,203,0,0,13,0,0,9,0,0,4,0,0,408,0,0,923,0,0,390,0,0,1500,6,50491,"WAT","HY" 11,23,1,1,,37,110,"CENTRAL MAINE POWER CO","NO GORHAM",0,,3266,"0M",1294,,,95,1215,0,0,963,0,0,842,0,0,520,0,0,455,0,0,503,0,0,595,0,0,604,0,0,413,0,0,340,0,0,740,0,0,1180,0,0,1501,6,50491,"WAT","HY" 11,23,1,1,,37,125,"CENTRAL MAINE POWER CO","SHAWMUT",0,,3266,"0M",1294,,,95,5226,0,0,5495,0,0,6547,0,0,5776,0,0,5295,0,0,4910,0,0,3475,0,0,2346,0,0,2571,0,0,3529,0,0,4803,0,0,6066,0,0,1504,6,50491,"WAT","HY" 11,23,1,1,,37,130,"CENTRAL MAINE POWER CO","SKELTON",0,,3266,"0M",1294,,,95,13276,0,0,8614,0,0,12134,0,0,11304,0,0,11550,0,0,5199,0,0,2833,0,0,2610,0,0,687,0,0,6731,0,0,13037,0,0,9456,0,0,1505,6,50491,"WAT","HY" 11,23,1,1,,37,145,"CENTRAL MAINE POWER CO","WEST BUXTON",0,,3266,"0M",1294,,,95,4424,0,0,2556,0,0,4381,0,0,3723,0,0,3292,0,0,1602,0,0,798,0,0,745,0,0,418,0,0,1944,0,0,4334,0,0,3045,0,0,1508,6,50491,"WAT","HY" 11,23,1,1,,37,150,"CENTRAL MAINE POWER CO","WESTON",0,,3266,"0M",1294,,,95,8095,0,0,8443,0,0,9513,0,0,8520,0,0,7843,0,0,7850,0,0,5819,0,0,4618,0,0,4257,0,0,5361,0,0,7925,0,0,9347,0,0,1509,6,50491,"WAT","HY" 11,23,1,1,,37,155,"CENTRAL MAINE POWER CO","WILLIAMS",0,,3266,"0M",1294,,,95,9171,0,0,9162,0,0,10255,0,0,6585,0,0,7543,0,0,8658,0,0,6098,0,0,5593,0,0,5308,0,0,5891,0,0,8857,0,0,10646,0,0,1510,6,50491,"WAT","HY" 11,23,1,1,,37,160,"CENTRAL MAINE POWER CO","WYMAN HYDRO",0,,3266,"0M",1294,,,95,30298,0,0,37016,0,0,38382,0,0,18735,0,0,24745,0,0,31774,0,0,20433,0,0,17564,0,0,16353,0,0,19735,0,0,40234,0,0,38504,0,0,1511,6,50491,"WAT","HY" 11,23,1,4,2,37,175,"CENTRAL MAINE POWER CO","CAPE",0,"LIGHT OIL",3266,"0M",1294,,,95,40,282,7937,40,336,7601,-57,44,7557,-40,24,7533,5,162,7371,38,208,7316,611,1872,6581,497,1571,5887,-24,32,5855,-32,27,5828,-45,25,5803,-25,145,5552,1484,6,50491,"FO2","GT" 11,23,1,2,2,37,200,"CENTRAL MAINE POWER CO","WYMAN STEAM",0,"LIGHT OIL",3266,"0M",1294,,,95,707,1587,1149,810,1542,1579,117,264,1534,980,1825,1680,366,883,1468,854,1640,1807,783,1460,2327,653,1307,1677,115,266,1410,20,76,1335,486,1282,2039,604,1177,2212,1507,6,50491,"FO2","ST" 11,23,1,2,3,37,200,"CENTRAL MAINE POWER CO","WYMAN STEAM",0,"HEAVY OIL",3266,"0M",1294,,,95,47051,97029,319010,122493,214459,275338,22777,47240,228098,127804,222606,207728,22560,50003,278752,79660,140051,253816,153893,263859,173676,74046,134076,202289,16596,35140,288543,3258,10955,197963,18538,44437,353526,107031,192190,308382,1507,6,50491,"FO6","ST" 11,23,1,3,2,37,204,"CENTRAL MAINE POWER CO","ISLESBORO",0,"LIGHT OIL",3266,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1494,6,50491,"FO2","IC" 11,23,1,3,2,37,206,"CENTRAL MAINE POWER CO","PEAK IS",0,"LIGHT OIL",3266,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1502,6,50491,"FO2","IC" 11,23,1,1,,37,210,"CENTRAL MAINE POWER CO","BRUNSWICK",0,,3266,"0M",1294,,,95,7964,0,0,6898,0,0,11266,0,0,10237,0,0,10095,0,0,6009,0,0,3698,0,0,2974,0,0,2429,0,0,6541,0,0,12216,0,0,8541,0,0,1483,6,50491,"WAT","HY" 11,23,1,1,,37,215,"CENTRAL MAINE POWER CO","W CHANNEL",0,,3266,"0M",1294,,,95,0,0,0,-33,0,0,-20,0,0,-22,0,0,-1,0,0,-1,0,0,-1,0,0,-21,0,0,-1,0,0,19,0,0,-11,0,0,-22,0,0,695,6,50491,"WAT","HY" 11,23,1,1,,37,220,"CENTRAL MAINE POWER CO","BATES UPPER",0,,3266,"0M",1294,,,95,-41,0,0,-34,0,0,610,0,0,144,0,0,273,0,0,15,0,0,1,0,0,15,0,0,18,0,0,217,0,0,4223,0,0,-30,0,0,7044,6,50491,"WAT","HY" 11,23,1,1,,37,225,"CENTRAL MAINE POWER CO","BATES LOWER",0,,3266,"0M",1294,"S",,95,-17,0,0,-16,0,0,-8,0,0,-2,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,-1,0,0,-3,0,0,-17,0,0,7045,6,50491,"WAT","HY" 11,23,1,1,,37,235,"CENTRAL MAINE POWER CO","ANDRO LOWER",0,,3266,"0M",1294,,,95,23,0,0,-11,0,0,21,0,0,-2,0,0,12,0,0,0,0,0,-1,0,0,0,0,0,0,0,0,5,0,0,38,0,0,-14,0,0,7047,6,50491,"WAT","HY" 11,23,1,1,,37,240,"CENTRAL MAINE POWER CO","HILL MILL",0,,3266,"0M",1294,,,95,-3,0,0,-2,0,0,183,0,0,-6,0,0,60,0,0,2,0,0,1,0,0,0,0,0,1,0,0,105,0,0,467,0,0,-6,0,0,7048,6,50491,"WAT","HY" 11,23,1,1,,37,245,"CENTRAL MAINE POWER CO","C E MONTY",0,,3266,"0M",1294,,,95,11840,0,0,10124,0,0,14280,0,0,13297,0,0,13808,0,0,8324,0,0,5496,0,0,4271,0,0,3199,0,0,9333,0,0,15686,0,0,12247,0,0,805,6,50491,"WAT","HY" 11,23,1,1,,37,250,"CENTRAL MAINE POWER CO","SMELT HILL",0,,3266,"0M",294,"A",,95,0,0,0,400,0,0,352,0,0,239,0,0,180,0,0,162,0,0,191,0,0,178,0,0,-608,0,0,766,0,0,224,0,0,283,0,0,7514,6,50491,"WAT","HY" 11,23,1,2,"B",37,255,"CENTRAL MAINE POWER CO","AROOSTOOK V",0,"WOOD",3266,"0M",294,"A",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,165,0,0,134,0,0,0,0,0,0,0,0,7513,6,50491,"WD","ST" 11,23,1,1,,94,5,"MAINE PUBLIC SERVICE CO","CARIBOU",0,,11522,"0M",1294,,,95,454,0,0,469,0,0,519,0,0,451,0,0,454,0,0,410,0,0,48,0,0,1,0,0,-2,0,0,178,0,0,536,0,0,504,0,0,1513,6,51747,"WAT","HY" 11,23,1,2,3,94,5,"MAINE PUBLIC SERVICE CO","CARIBOU",0,"HEAVY OIL",11522,"0M",1294,,,95,343,903,9375,592,1410,7984,-32,0,8005,-29,0,7995,-26,6,8015,-27,4,8057,-26,0,8067,222,644,7448,-28,0,7396,-29,0,7390,857,1841,5557,2237,4973,2370,1513,6,51747,"FO6","ST" 11,23,1,3,2,94,5,"MAINE PUBLIC SERVICE CO","CARIBOU",0,"LIGHT OIL",11522,"0M",1294,,,95,50,251,1746,5,143,1693,-65,0,1583,78,225,1932,-18,17,1865,-9,6,1829,38,115,1683,233,500,1802,86,210,1776,-6,65,2071,-56,28,1948,244,599,2098,1513,6,51747,"FO2","IC" 11,23,1,1,,94,10,"MAINE PUBLIC SERVICE CO","SQUA PAN",0,,11522,"0M",1294,,,95,115,0,0,363,0,0,152,0,0,-10,0,0,-7,0,0,-3,0,0,-3,0,0,-4,0,0,-6,0,0,-7,0,0,3,0,0,223,0,0,1516,6,51747,"WAT","HY" 11,23,1,3,2,94,23,"MAINE PUBLIC SERVICE CO","FLOS INN",0,"LIGHT OIL",11522,"0M",1294,,,95,27,115,314,19,82,232,-29,0,232,19,79,373,-23,2,371,-16,0,371,13,80,290,124,284,232,74,135,323,-3,51,272,-25,8,264,217,451,388,1514,6,51747,"FO2","IC" 11,23,1,3,2,94,25,"MAINE PUBLIC SERVICE CO","HOULTON",0,"LIGHT OIL",11522,"0M",1294,,,95,6,28,13,-8,1,12,-8,2,10,-8,0,10,-6,0,10,-3,0,10,-2,0,10,-3,0,10,-3,0,10,-4,0,11,-4,2,8,14,34,6,1515,6,51747,"FO2","IC" 11,23,1,2,1,97,1,"MAINE YANKEE ATOMIC PWR C","MAIN YANKEE",0,"NUCLEAR",11525,"0M",1294,,,95,197577,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1517,6,51748,"UR","ST" 11,23,1,3,2,116,10,"PUB SERV CO OF NEW HAMP","SWANS FALLS",0,"LIGHT OIL",15472,"0M",1294,"R",180,95,-7,0,2,-7,0,2,-6,0,2,-3,0,2,-2,0,2,-1,0,2,-1,0,2,-1,0,2,-1,0,2,-1,0,2,-3,0,2,0,0,0,1518,6,52411,"FO2","IC" 11,23,5,1,,525,1,"LEWISTON (CITY OF)","ANDRO UPPER",0,,10963,"0A",1294,,,95,296,0,0,378,0,0,310,0,0,424,0,0,264,0,0,390,0,0,256,0,0,258,0,0,304,0,0,270,0,0,342,0,0,324,0,0,7046,6,54168,"WAT","HY" 11,23,5,1,,566,1,"MADISON (CITY OF)","NORRIDGEWCK",0,,11477,"0A",1294,,,95,306,0,0,241,0,0,261,0,0,291,0,0,379,0,0,277,0,0,75,0,0,0,0,0,26,0,0,121,0,0,197,0,0,224,0,0,6701,6,51737,"WAT","HY" 11,23,8,3,2,835,5,"EASTERN MAINE ELEC COOP","PORTABLE",0,"LIGHT OIL",5609,"0A",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,6366,6,50848,"FO2","IC" 11,23,8,3,2,940,1,"SWANS ISLAND ELEC COOP","MINTURN",0,"LIGHT OIL",18368,"0A",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1550,6,52863,"FO2","IC" 12,33,1,1,,106,5,"NEW ENGLAND POWER CO","COMERFORD",0,,13433,"0M",1294,,90,95,34273,0,0,19125,0,0,43429,0,0,11874,0,0,22700,0,0,13853,0,0,5565,0,0,11061,0,0,5412,0,0,30636,0,0,45527,0,0,18948,0,0,2349,6,52007,"WAT","HY" 12,33,1,1,,106,10,"NEW ENGLAND POWER CO","MCINDOES",0,,13433,"0M",1294,,90,95,4420,0,0,3434,0,0,6350,0,0,3330,0,0,4648,0,0,2664,0,0,1453,0,0,2497,0,0,1353,0,0,4755,0,0,7050,0,0,3740,0,0,6483,6,52007,"WAT","HY" 12,33,1,1,,106,13,"NEW ENGLAND POWER CO","S C MOORE",0,,13433,"0M",1294,,90,95,29434,0,0,15866,0,0,34014,0,0,9521,0,0,19359,0,0,12124,0,0,4787,0,0,9805,0,0,4357,0,0,27013,0,0,40020,0,0,16551,0,0,2351,6,52007,"WAT","HY" 12,33,1,1,,106,15,"NEW ENGLAND POWER CO","VERNON",0,,13433,"0M",1294,,90,95,7120,0,0,5523,0,0,9186,0,0,7993,0,0,7582,0,0,3197,0,0,1355,0,0,2525,0,0,19,0,0,5912,0,0,9702,0,0,7342,0,0,2352,6,52007,"WAT","HY" 12,33,1,1,,106,20,"NEW ENGLAND POWER CO","WILDER",0,,13433,"0M",1294,,90,95,1974,0,0,3326,0,0,18722,0,0,7773,0,0,8911,0,0,4713,0,0,4047,0,0,5176,0,0,2849,0,0,9330,0,0,12667,0,0,7471,0,0,2353,6,52007,"WAT","HY" 12,33,1,2,1,123,1,"PUB SERV CO OF NEW HAMP","SEABROOK",0,"NUCLEAR",15472,"0M",1294,,180,95,857441,0,0,778373,0,0,863021,0,0,832472,0,0,865152,0,0,495425,0,0,690261,0,0,805711,0,0,800410,0,0,828658,0,0,60958,0,0,501494,0,0,6115,6,52411,"UR","ST" 12,33,1,1,,123,4,"PUB SERV CO OF NEW HAMP","AMOSKEAG",0,,15472,"0M",1294,,180,95,10690,0,0,7028,0,0,11425,0,0,749,0,0,15769,0,0,4245,0,0,2251,0,0,3257,0,0,434,0,0,5760,0,0,11044,0,0,6264,0,0,2354,6,52411,"WAT","HY" 12,33,1,1,,123,6,"PUB SERV CO OF NEW HAMP","AYERS IS",0,,15472,"0M",1294,,180,95,3909,0,0,2249,0,0,4743,0,0,3555,0,0,4487,0,0,1520,0,0,1448,0,0,1727,0,0,380,0,0,3303,0,0,5711,0,0,2632,0,0,2355,6,52411,"WAT","HY" 12,33,1,1,,123,16,"PUB SERV CO OF NEW HAMP","EASTMAN FLS",0,,15472,"0M",1294,,180,95,2843,0,0,1293,0,0,2781,0,0,2587,0,0,2725,0,0,1214,0,0,1763,0,0,10079,0,0,-9794,0,0,1729,0,0,3266,0,0,1701,0,0,2356,6,52411,"WAT","HY" 12,33,1,1,,123,20,"PUB SERV CO OF NEW HAMP","GARVIN FLS",0,,15472,"0M",1294,,180,95,5209,0,0,3143,0,0,5693,0,0,4388,0,0,3956,0,0,2019,0,0,755,0,0,1667,0,0,350,0,0,3233,0,0,6336,0,0,3913,0,0,2357,6,52411,"WAT","HY" 12,33,1,1,,123,22,"PUB SERV CO OF NEW HAMP","GORHAM",0,,15472,"0M",1294,,180,95,989,0,0,1031,0,0,1249,0,0,885,0,0,1193,0,0,756,0,0,568,0,0,530,0,0,580,0,0,864,0,0,1116,0,0,1202,0,0,2358,6,52411,"WAT","HY" 12,33,1,1,,123,28,"PUB SERV CO OF NEW HAMP","HOOKSETT",0,,15472,"0M",1294,,180,95,787,0,0,865,0,0,912,0,0,1164,0,0,1141,0,0,791,0,0,156,0,0,317,0,0,43,0,0,751,0,0,952,0,0,776,0,0,2359,6,52411,"WAT","HY" 12,33,1,1,,123,30,"PUB SERV CO OF NEW HAMP","JACKMAN",0,,15472,"0M",1294,,180,95,1997,0,0,535,0,0,1239,0,0,236,0,0,557,0,0,305,0,0,191,0,0,722,0,0,-8,0,0,1339,0,0,2326,0,0,864,0,0,2360,6,52411,"WAT","HY" 12,33,1,1,,123,50,"PUB SERV CO OF NEW HAMP","SMITH STA",0,,15472,"0M",1294,,180,95,8143,0,0,9737,0,0,11648,0,0,6108,0,0,8349,0,0,6172,0,0,4454,0,0,4871,0,0,3742,0,0,6861,0,0,10860,0,0,10308,0,0,2368,6,52411,"WAT","HY" 12,33,1,4,2,123,57,"PUB SERV CO OF NEW HAMP","LOST NATION",0,"LIGHT OIL",15472,"0M",1294,,180,95,-15,0,2159,79,306,1853,-15,0,1853,-12,0,1853,42,125,1728,50,140,1587,209,595,1527,275,828,1235,-11,0,1235,-11,0,1235,-10,0,1235,111,338,1076,2362,6,52411,"FO2","GT" 12,33,1,2,2,123,59,"PUB SERV CO OF NEW HAMP","MERRIMACK",0,"LIGHT OIL",15472,"0M",1294,,180,95,27,45,275,16,29,156,22,38,180,23,38,218,0,0,0,29,52,151,6,14,205,30,55,180,52,96,222,62,108,185,57,96,176,20,35,176,2364,6,52411,"FO2","ST" 12,33,1,2,6,123,59,"PUB SERV CO OF NEW HAMP","MERRIMACK",0,"BIT COAL",15472,"0M",1294,,180,95,266403,101539,253077,274308,103830,266334,256612,98157,263978,216443,80934,278945,76504,17154,315133,246563,95683,297713,281671,111493,247571,263463,95839,235114,181335,71786,264069,207269,81066,275589,253852,96425,269715,287608,108204,247069,2364,6,52411,"BIT","ST" 12,33,1,4,2,123,59,"PUB SERV CO OF NEW HAMP","MERRIMACK",0,"LIGHT OIL",15472,"0M",1294,,180,95,-47,0,3032,411,1048,3032,-21,0,1984,-18,0,1984,112,282,1702,122,334,1367,613,1576,1494,582,1554,2033,-14,0,2033,-11,20,2013,-20,0,2013,242,603,1411,2364,6,52411,"FO2","GT" 12,33,1,2,3,123,63,"PUB SERV CO OF NEW HAMP","SCHILLER",0,"HEAVY OIL",15472,"0M",1294,,180,95,1350,2702,31413,820,1554,92325,2073,4352,187620,1454,2823,184796,1826,3479,189663,2478,4626,184835,4062,7903,176932,2011,4193,53637,1321,2911,170000,1885,4329,165671,5233,10859,154812,3538,6785,118334,2367,6,52411,"FO6","ST" 12,33,1,2,6,123,63,"PUB SERV CO OF NEW HAMP","SCHILLER",0,"BIT COAL",15472,"0M",1294,,180,95,53534,27148,87087,68779,32692,50318,47008,24972,52027,65230,33724,53967,55312,27020,32185,49976,24400,75043,55074,26887,62380,30313,18396,42154,18241,9931,51974,16092,9642,54786,30357,16856,90418,65541,32424,72200,2367,6,52411,"BIT","ST" 12,33,1,4,2,123,63,"PUB SERV CO OF NEW HAMP","SCHILLER",0,"LIGHT OIL",15472,"0M",1294,,180,95,-13,0,804,95,260,723,-12,0,723,-9,0,723,57,118,604,-7,0,604,90,262,723,242,963,714,-7,0,714,0,0,714,-9,0,714,120,301,794,2367,6,52411,"FO2","GT" 12,33,1,4,9,123,63,"PUB SERV CO OF NEW HAMP","SCHILLER",0,"NAT GAS",15472,"0M",1294,,180,95,19,240,0,12,140,0,24,310,0,25,300,0,22,264,0,17,210,0,219,2700,0,121,2803,0,14,190,0,15,220,0,24,320,0,22,260,0,2367,6,52411,"NG","GT" 12,33,1,4,2,123,70,"PUB SERV CO OF NEW HAMP","WHITE LAKE",0,"LIGHT OIL",15472,"0M",1294,,180,95,-17,0,2383,97,350,2033,-14,4,2029,-7,0,2029,48,94,1935,136,341,1595,147,405,1763,357,924,1410,-3,0,1410,-3,0,1410,-13,0,1410,-6,129,1281,2369,6,52411,"FO2","GT" 12,33,1,2,2,123,72,"PUB SERV CO OF NEW HAMP","NEWINGTON",0,"LIGHT OIL",15472,"0M",1294,,180,95,2141,4247,1577,1729,3274,1766,1111,2327,1824,1584,4149,1209,1580,3072,1209,1589,3168,1640,1162,2239,1856,1703,3313,1598,1134,2258,1388,173,817,1751,1894,3703,1630,507,3096,1651,8002,6,52411,"FO2","ST" 12,33,1,2,3,123,72,"PUB SERV CO OF NEW HAMP","NEWINGTON",0,"HEAVY OIL",15472,"0M",1294,,180,95,73391,138116,328850,119485,206586,321529,32827,62816,434361,89003,159420,245596,100291,177704,321055,73382,134661,317462,125529,216497,100965,57182,118647,2305699,45699,82009,405756,1560,6611,399144,100544,177099,222046,136392,231245,388270,8002,6,52411,"FO6","ST" 12,33,1,2,9,123,72,"PUB SERV CO OF NEW HAMP","NEWINGTON",0,"NAT GAS",15472,"0M",1294,,180,95,1463,17053,0,0,0,0,0,0,0,0,0,0,35353,394385,0,45744,527451,0,57696,624462,0,48968,544320,0,10747,122302,0,57,1545,0,742,8312,0,0,0,0,8002,6,52411,"NG","ST" 13,50,1,1,,22,2,"CENTRAL VT PUB SERV CORP","ARNOLD FLS",0,,3292,"0A",1294,,350,95,112,0,0,27,0,0,168,0,0,290,0,0,100,0,0,18,0,0,33,0,0,37,0,0,17,0,0,172,0,0,245,0,0,135,0,0,3707,6,50503,"WAT","HY" 13,50,1,1,,22,10,"CENTRAL VT PUB SERV CORP","CAVENDISH",0,,3292,"0A",1294,,350,95,534,0,0,309,0,0,847,0,0,607,0,0,267,0,0,83,0,0,0,0,0,134,0,0,-3,0,0,391,0,0,928,0,0,383,0,0,3710,6,50503,"WAT","HY" 13,50,1,1,,22,11,"CENTRAL VT PUB SERV CORP","CLARKS FLS",0,,3292,"0A",1294,,350,95,1404,0,0,1026,0,0,1689,0,0,1865,0,0,1729,0,0,855,0,0,596,0,0,1076,0,0,567,0,0,1648,0,0,1970,0,0,1412,0,0,3711,6,50503,"WAT","HY" 13,50,1,1,,22,15,"CENTRAL VT PUB SERV CORP","FAIRFAX",0,,3292,"0A",1294,,350,95,1873,0,0,1589,0,0,2321,0,0,2516,0,0,2499,0,0,1241,0,0,878,0,0,1432,0,0,744,0,0,2114,0,0,2573,0,0,2233,0,0,3712,6,50503,"WAT","HY" 13,50,1,1,,22,16,"CENTRAL VT PUB SERV CORP","GAGE",0,,3292,"0A",1294,,350,95,221,0,0,24,0,0,244,0,0,307,0,0,290,0,0,73,0,0,85,0,0,38,0,0,48,0,0,305,0,0,523,0,0,226,0,0,3713,6,50503,"WAT","HY" 13,50,1,1,,22,18,"CENTRAL VT PUB SERV CORP","GLEN",0,,3292,"0A",1294,,350,95,1041,0,0,605,0,0,731,0,0,367,0,0,238,0,0,98,0,0,83,0,0,323,0,0,183,0,0,629,0,0,1307,0,0,401,0,0,3714,6,50503,"WAT","HY" 13,50,1,1,,22,22,"CENTRAL VT PUB SERV CORP","LW MIDLEBRY",0,,3292,"0A",1294,,350,95,725,0,0,534,0,0,1054,0,0,920,0,0,550,0,0,286,0,0,79,0,0,150,0,0,104,0,0,524,0,0,1220,0,0,492,0,0,3716,6,50503,"WAT","HY" 13,50,1,1,,22,26,"CENTRAL VT PUB SERV CORP","MILTON",0,,3292,"0A",1294,,350,95,3538,0,0,2446,0,0,4215,0,0,4336,0,0,3864,0,0,1806,0,0,1204,0,0,2514,0,0,1210,0,0,4046,0,0,4879,0,0,3192,0,0,3717,6,50503,"WAT","HY" 13,50,1,1,,22,28,"CENTRAL VT PUB SERV CORP","PASSUMPSIC",0,,3292,"0A",1294,,350,95,315,0,0,97,0,0,378,0,0,435,0,0,415,0,0,90,0,0,51,0,0,150,0,0,94,0,0,370,0,0,434,0,0,44,0,0,3718,6,50503,"WAT","HY" 13,50,1,1,,22,30,"CENTRAL VT PUB SERV CORP","PATCH",0,,3292,"0A",1294,,350,95,107,0,0,58,0,0,59,0,0,21,0,0,7,0,0,5,0,0,5,0,0,28,0,0,7,0,0,42,0,0,158,0,0,30,0,0,3719,6,50503,"WAT","HY" 13,50,1,1,,22,34,"CENTRAL VT PUB SERV CORP","PIERCE MLS",0,,3292,"0A",1294,,350,95,113,0,0,81,0,0,121,0,0,180,0,0,161,0,0,59,0,0,47,0,0,47,0,0,17,0,0,102,0,0,181,0,0,116,0,0,3721,6,50503,"WAT","HY" 13,50,1,1,,22,36,"CENTRAL VT PUB SERV CORP","PITTSFORD",0,,3292,"0A",1294,,350,95,1275,0,0,941,0,0,158,0,0,47,0,0,-2,0,0,9,0,0,0,0,0,489,0,0,354,0,0,726,0,0,1999,0,0,679,0,0,3722,6,50503,"WAT","HY" 13,50,1,1,,22,38,"CENTRAL VT PUB SERV CORP","SALISBURY",0,,3292,"0A",1294,,350,95,325,0,0,210,0,0,191,0,0,62,0,0,141,0,0,65,0,0,25,0,0,72,0,0,111,0,0,88,0,0,-6,0,0,303,0,0,3724,6,50503,"WAT","HY" 13,50,1,1,,22,40,"CENTRAL VT PUB SERV CORP","SILVER LAKE",0,,3292,"0A",1294,,350,95,800,0,0,508,0,0,722,0,0,405,0,0,402,0,0,227,0,0,103,0,0,275,0,0,84,0,0,500,0,0,973,0,0,535,0,0,3725,6,50503,"WAT","HY" 13,50,1,1,,22,41,"CENTRAL VT PUB SERV CORP","TAFTSVILLE",0,,3292,"0A",1294,,350,95,150,0,0,135,0,0,208,0,0,200,0,0,119,0,0,12,0,0,0,0,0,17,0,0,-1,0,0,55,0,0,175,0,0,162,0,0,3727,6,50503,"WAT","HY" 13,50,1,1,,22,44,"CENTRAL VT PUB SERV CORP","WEYBRIDGE",0,,3292,"0A",1294,,350,95,1391,0,0,616,0,0,1819,0,0,1459,0,0,991,0,0,370,0,0,156,0,0,354,0,0,167,0,0,1042,0,0,2031,0,0,856,0,0,3728,6,50503,"WAT","HY" 13,50,1,1,,22,45,"CENTRAL VT PUB SERV CORP","PETERSON",0,,3292,"0A",1294,,350,95,2522,0,0,1281,0,0,3601,0,0,3092,0,0,2335,0,0,1090,0,0,702,0,0,1605,0,0,681,0,0,2814,0,0,4021,0,0,1742,0,0,3720,6,50503,"WAT","HY" 13,50,1,4,2,22,48,"CENTRAL VT PUB SERV CORP","RUTLAND",0,"LIGHT OIL",3292,"0A",1294,,350,95,13,125,4525,45,327,4198,40,218,3979,19,143,3836,20,127,3709,101,381,3328,272,898,2430,277,932,1498,34,167,3475,-8,46,3429,32,195,3234,152,651,2583,3723,6,50503,"FO2","GT" 13,50,1,4,2,22,49,"CENTRAL VT PUB SERV CORP","ASCUTNEY",0,"LIGHT OIL",3292,"0A",1294,,350,95,27,136,2572,77,326,2246,69,300,1946,18,96,1851,8,65,1786,41,144,1641,268,895,2175,226,765,1409,-1,38,3277,-15,0,3277,-3,71,3206,88,353,2853,3708,6,50503,"FO2","GT" 13,50,1,3,2,22,60,"CENTRAL VT PUB SERV CORP","ST ALBANS",0,"LIGHT OIL",3292,"0A",1294,,350,95,-14,0,89,5,38,214,-11,4,210,-10,5,205,7,17,188,21,40,148,72,149,234,59,123,111,-1,2,110,-3,0,110,-6,0,108,9,42,236,3726,6,50503,"FO2","IC" 13,50,1,1,,22,65,"CENTRAL VT PUB SERV CORP","SMITH",0,,3292,"0A",1294,,350,95,361,0,0,154,0,0,495,0,0,658,0,0,519,0,0,163,0,0,121,0,0,123,0,0,72,0,0,258,0,0,692,0,0,170,0,0,3709,6,50503,"WAT","HY" 13,50,1,1,,22,70,"CENTRAL VT PUB SERV CORP","EAST BARNET",0,,3292,"0A",1294,,350,95,595,0,0,399,0,0,900,0,0,1046,0,0,922,0,0,325,0,0,322,0,0,358,0,0,203,0,0,790,0,0,1148,0,0,702,0,0,788,6,50503,"WAT","HY" 13,50,1,1,,24,5,"CITIZENS UTILITIES CO","CHARLESTON",0,,3611,"0A",1294,,,95,339,0,0,244,0,0,393,0,0,445,0,0,409,0,0,252,0,0,154,0,0,192,0,0,90,0,0,382,0,0,461,0,0,314,0,0,3729,6,50560,"WAT","HY" 13,50,1,1,,24,10,"CITIZENS UTILITIES CO","NEWPORT",0,,3611,"0A",1294,,,95,1625,0,0,946,0,0,1961,0,0,1655,0,0,1645,0,0,917,0,0,474,0,0,1107,0,0,331,0,0,1614,0,0,2652,0,0,1235,0,0,3731,6,50560,"WAT","HY" 13,50,1,3,2,24,15,"CITIZENS UTILITIES CO","NEWPORT DSL",0,"LIGHT OIL",3611,"0A",1294,,,95,0,0,377,16,33,290,0,0,259,0,0,229,0,0,206,0,0,206,0,0,206,7,12,194,8,16,177,0,0,177,0,0,137,0,0,85,3730,6,50560,"FO2","IC" 13,50,1,1,,24,20,"CITIZENS UTILITIES CO","TROY",0,,3611,"0A",1294,,,95,150,0,0,72,0,0,150,0,0,267,0,0,209,0,0,71,0,0,28,0,0,30,0,0,3,0,0,74,0,0,244,0,0,128,0,0,3733,6,50560,"WAT","HY" 13,50,1,1,,47,10,"GREEN MOUNTAIN POWER CORP","ESSEX 19",0,,7601,"0M",1294,,,95,2888,0,0,2870,0,0,4338,0,0,3931,0,0,3261,0,0,980,0,0,333,0,0,1531,0,0,936,0,0,2161,0,0,3540,0,0,2964,0,0,3737,6,51169,"WAT","HY" 13,50,1,3,2,47,10,"GREEN MOUNTAIN POWER CORP","ESSEX 19",0,"LIGHT OIL",7601,"0M",1294,,,95,0,0,311,11,27,284,1,1,283,0,0,283,7,16,267,28,61,385,45,85,300,33,65,235,9,19,394,0,0,394,0,0,394,12,25,369,3737,6,51169,"FO2","IC" 13,50,1,1,,47,15,"GREEN MOUNTAIN POWER CORP","GORGE NO 18",0,,7601,"0M",1294,,,95,901,0,0,986,0,0,1573,0,0,1661,0,0,1125,0,0,122,0,0,113,0,0,692,0,0,0,0,0,0,0,0,0,0,0,0,0,0,6475,6,51169,"WAT","HY" 13,50,1,1,,47,20,"GREEN MOUNTAIN POWER CORP","MARSHFIELD6",0,,7601,"0M",1294,,,95,891,0,0,1188,0,0,245,0,0,107,0,0,0,0,0,3,0,0,2,0,0,54,0,0,53,0,0,604,0,0,1300,0,0,430,0,0,3739,6,51169,"WAT","HY" 13,50,1,1,,47,25,"GREEN MOUNTAIN POWER CORP","MIDDLESEX 2",0,,7601,"0M",1294,,,95,1134,0,0,848,0,0,1580,0,0,1697,0,0,1156,0,0,150,0,0,111,0,0,717,0,0,45,0,0,1158,0,0,2061,0,0,1133,0,0,3740,6,51169,"WAT","HY" 13,50,1,1,,47,40,"GREEN MOUNTAIN POWER CORP","VERGENNES 9",0,,7601,"0M",1294,,,95,972,0,0,799,0,0,1171,0,0,1224,0,0,968,0,0,441,0,0,247,0,0,499,0,0,318,0,0,590,0,0,1307,0,0,899,0,0,6519,6,51169,"WAT","HY" 13,50,1,3,2,47,40,"GREEN MOUNTAIN POWER CORP","VERGENNES 9",0,"LIGHT OIL",7601,"0M",1294,,,95,15,27,282,68,118,164,15,24,319,5,8,311,4,25,465,108,264,200,174,319,417,163,302,294,20,35,437,3,2,436,2,4,432,35,62,370,6519,6,51169,"FO2","IC" 13,50,1,1,,47,53,"GREEN MOUNTAIN POWER CORP","WATRBRY 22",0,,7601,"0M",1294,,,95,2101,0,0,2029,0,0,1441,0,0,318,0,0,823,0,0,444,0,0,464,0,0,1190,0,0,485,0,0,2251,0,0,2609,0,0,1566,0,0,6520,6,51169,"WAT","HY" 13,50,1,1,,47,55,"GREEN MOUNTAIN POWER CORP","W DANVIL 15",0,,7601,"0M",1294,,,95,445,0,0,146,0,0,507,0,0,509,0,0,301,0,0,77,0,0,87,0,0,220,0,0,103,0,0,544,0,0,661,0,0,151,0,0,3743,6,51169,"WAT","HY" 13,50,1,4,2,47,58,"GREEN MOUNTAIN POWER CORP","BERLIN NO 5",0,"LIGHT OIL",7601,"0M",1294,,,95,32,270,10962,606,1501,9460,21,72,9388,0,0,9338,254,677,8711,731,1834,7632,1214,3039,11011,1354,3377,12369,189,463,14376,681,1521,12855,79,209,12646,389,879,11767,3734,6,51169,"FO2","GT" 13,50,1,4,2,47,60,"GREEN MOUNTAIN POWER CORP","COLCHSTR 16",0,"LIGHT OIL",7601,"0M",1294,,,95,7,28,1071,86,296,775,5,25,750,0,0,750,9,33,717,6,26,1583,117,472,1112,76,320,791,0,0,1506,0,0,1506,0,0,1507,0,0,1506,3735,6,51169,"FO2","GT" 13,50,1,1,,47,65,"GREEN MOUNTAIN POWER CORP","BOLTON FALL",0,,7601,"0M",1294,,,95,3020,0,0,2253,0,0,3823,0,0,2884,0,0,2258,0,0,636,0,0,502,0,0,1603,0,0,428,0,0,2596,0,0,4478,0,0,2430,0,0,7056,6,51169,"WAT","HY" 13,50,1,7,"D",47,70,"GREEN MOUNTAIN POWER CORP","CARTHUSIANS",0,"N/A",7601,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,7260,6,51169,"WI","WI" 13,50,1,1,,73,5,"NEW ENGLAND POWER CO","BELLOWS FLS",0,,13433,"0M",1294,,90,95,22299,0,0,16448,0,0,28735,0,0,22260,0,0,21635,0,0,10244,0,0,6175,0,0,10541,0,0,3991,0,0,19464,0,0,30239,0,0,18843,0,0,3745,6,52007,"WAT","HY" 13,50,1,1,,73,10,"NEW ENGLAND POWER CO","HARRIMAN",0,,13433,"0M",1294,,90,95,14391,0,0,13610,0,0,13092,0,0,2630,0,0,807,0,0,1394,0,0,2040,0,0,2968,0,0,2416,0,0,10136,0,0,16468,0,0,11713,0,0,3746,6,52007,"WAT","HY" 13,50,1,1,,73,15,"NEW ENGLAND POWER CO","SEARSBURG",0,,13433,"0M",1294,,90,95,3120,0,0,2878,0,0,3094,0,0,1942,0,0,1012,0,0,853,0,0,152,0,0,1319,0,0,954,0,0,2077,0,0,3042,0,0,2675,0,0,6529,6,52007,"WAT","HY" 13,50,1,1,,73,18,"NEW ENGLAND POWER CO","VERNON",0,,13433,"0M",1294,,90,95,4592,0,0,4182,0,0,5197,0,0,4922,0,0,4427,0,0,2397,0,0,1604,0,0,3525,0,0,1667,0,0,3876,0,0,4946,0,0,3693,0,0,8904,6,52007,"WAT","HY" 13,50,1,1,,73,20,"NEW ENGLAND POWER CO","WILDER",0,,13433,"0M",1294,,90,95,9053,0,0,5888,0,0,8525,0,0,1765,0,0,2559,0,0,1204,0,0,21,0,0,1756,0,0,407,0,0,4556,0,0,8802,0,0,2669,0,0,8905,6,52007,"WAT","HY" 13,50,1,1,,98,5,"PUB SERV CO OF NEW HAMP","CANAAN",0,,15472,"0M",1294,,180,95,729,0,0,718,0,0,805,0,0,483,0,0,569,0,0,345,0,0,252,0,0,190,0,0,195,0,0,728,0,0,765,0,0,738,0,0,3750,6,52411,"WAT","HY" 13,50,1,2,1,135,1,"VT YANKEE NUCLEAR PR CORP","VT YANKEE",0,"NUCLEAR",19796,"0M",1294,,,95,384928,0,0,346136,0,0,192519,0,0,0,0,0,335965,0,0,365673,0,0,371198,0,0,375476,0,0,363210,0,0,389313,0,0,379730,0,0,354361,0,0,3751,6,53128,"UR","ST" 13,50,1,1,,304,1,"VERMONT MARBLE CO","PROCTOR",0,,19794,"0A",1294,,,95,3213,0,0,2009,0,0,3559,0,0,3058,0,0,2032,0,0,1143,0,0,395,0,0,893,0,0,294,0,0,1839,0,0,3796,0,0,1853,0,0,6450,6,53127,"WAT","HY" 13,50,1,1,,304,5,"VERMONT MARBLE CO","CTR RUTLAND",0,,19794,"0A",1294,,,95,161,0,0,164,0,0,188,0,0,211,0,0,211,0,0,121,0,0,26,0,0,62,0,0,19,0,0,85,0,0,190,0,0,184,0,0,6453,6,53127,"WAT","HY" 13,50,1,1,,304,10,"VERMONT MARBLE CO","BELDENS",0,,19794,"0A",1294,,,95,2174,0,0,1009,0,0,2729,0,0,1624,0,0,972,0,0,405,0,0,95,0,0,369,0,0,149,0,0,1679,0,0,2997,0,0,1013,0,0,6451,6,53127,"WAT","HY" 13,50,1,4,2,304,15,"VERMONT MARBLE CO","FLORENCE",0,"LIGHT OIL",19794,"0A",1294,,,95,-2,95,12708,118,200,12076,184,475,11934,674,1762,7457,74,191,4607,157,358,9260,354,1040,6925,210,559,6363,167,435,4707,-11,3,10761,-13,60,8428,167,550,7887,7337,6,53127,"FO2","GT" 13,50,5,1,,520,1,"BARTON (VILLAGE OF)","W CHARLESTN",0,,1299,"0A",1294,,,95,477,0,0,231,0,0,556,0,0,533,0,0,570,0,0,256,0,0,132,0,0,351,0,0,83,0,0,382,0,0,680,0,0,196,0,0,3753,6,50178,"WAT","HY" 13,50,5,3,2,520,1,"BARTON (VILLAGE OF)","W CHARLESTN",0,"LIGHT OIL",1299,"0A",1294,,,95,0,0,206,14,34,172,0,0,172,0,0,172,1,3,169,19,51,118,39,103,190,42,112,78,7,19,59,0,0,59,0,0,118,10,86,32,3753,6,50178,"FO2","IC" 13,50,5,4,2,536,1,"BURLINGTON (CITY OF)","GAS TURB",0,"LIGHT OIL",2548,"0M",1294,,,95,0,1,1628,248,707,868,0,4,2022,0,0,2015,19,66,1949,459,1365,1742,608,1830,1698,485,1472,1476,56,189,1287,0,0,1285,84,242,1001,165,472,1772,3754,6,50375,"FO2","GT" 13,50,5,2,"B",536,10,"BURLINGTON (CITY OF)","J C MC NEIL",0,"WOD CHIPS",2548,"0M",1294,,,95,7742,0,0,12138,0,0,4790,0,0,12108,0,0,15618,0,0,11949,0,0,14425,0,0,8887,0,0,5359,0,0,3746,0,0,10817,0,0,19589,0,0,589,6,50375,"WOD","ST" 13,50,5,2,2,536,10,"BURLINGTON (CITY OF)","J C MC NEIL",0,"LIGHT OIL",2548,"0M",1294,,,95,136,326,2416,132,350,1989,41,99,1826,0,216,1559,0,39,1448,0,22,1351,4,23,1264,0,81,1183,0,52,1021,0,40,945,19,99,3170,24,98,2994,589,6,50375,"FO2","ST" 13,50,5,2,9,536,10,"BURLINGTON (CITY OF)","J C MC NEIL",0,"NAT GAS",2548,"0M",1294,,,95,1750,24386,0,816,12632,0,1337,18689,0,0,2252,0,0,3244,0,0,3721,0,177,4800,0,0,2471,0,0,2396,0,0,2708,0,449,13380,0,2064,47618,0,589,6,50375,"NG","ST" 13,50,5,1,,551,5,"ENOSBURG FALLS (VILLAGE)","KENDALL",0,,5915,"0A",1294,,,95,52,0,0,126,0,0,145,0,0,160,0,0,164,0,0,130,0,0,102,0,0,121,0,0,68,0,0,109,0,0,147,0,0,64,0,0,3757,6,50910,"WAT","HY" 13,50,5,3,2,551,10,"ENOSBURG FALLS (VILLAGE)","DIESEL PLT",0,"LIGHT OIL",5915,"0A",1294,,,95,1,5,320,14,24,296,0,1,296,1,3,293,4,13,280,16,34,246,20,37,351,23,44,307,2,6,301,0,0,301,0,0,0,12,21,279,4247,6,50910,"FO2","IC" 13,50,5,1,,551,15,"ENOSBURG FALLS (VILLAGE)","VILLAGE PLT",0,,5915,"0A",1294,,,95,370,0,0,204,0,0,298,0,0,433,0,0,408,0,0,218,0,0,87,0,0,140,0,0,45,0,0,324,0,0,364,0,0,395,0,0,4246,6,50910,"WAT","HY" 13,50,5,1,,567,1,"HARDWICK (VILLAGE OF)","WOLCOTT",0,,8104,"0A",1294,,,95,228,0,0,139,0,0,381,0,0,480,0,0,332,0,0,55,0,0,41,0,0,20,0,0,22,0,0,331,0,0,526,0,0,262,0,0,6477,6,51238,"WAT","HY" 13,50,5,3,2,567,5,"HARDWICK (VILLAGE OF)","HARDWICK",0,"LIGHT OIL",8104,"0A",1294,,,95,0,0,451,0,0,451,0,0,451,0,0,451,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,6476,6,51238,"FO2","IC" 13,50,5,1,,644,5,"LYNDONVILLE (CITY OF)","GREAT FALLS",0,,11359,"0A",1294,,,95,160,0,0,115,0,0,308,0,0,489,0,0,746,0,0,350,0,0,273,0,0,122,0,0,171,0,0,457,0,0,558,0,0,437,0,0,3762,6,51721,"WAT","HY" 13,50,5,1,,644,10,"LYNDONVILLE (CITY OF)","VAIL",0,,11359,"0A",1294,,,95,100,0,0,71,0,0,99,0,0,123,0,0,225,0,0,93,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,107,0,0,3763,6,51721,"WAT","HY" 13,50,5,1,,659,5,"MORRISVILLE (VILLAGE OF)","CADYS FALLS",0,,12989,"0A",1294,,,95,396,0,0,268,0,0,387,0,0,226,0,0,403,0,0,133,0,0,101,0,0,2,0,0,71,0,0,356,0,0,337,0,0,160,0,0,3765,6,51943,"WAT","HY" 13,50,5,1,,659,10,"MORRISVILLE (VILLAGE OF)","MORRISVILLE",0,,12989,"0A",1294,,,95,250,0,0,312,0,0,619,0,0,801,0,0,581,0,0,131,0,0,-1,0,0,-1,0,0,-1,0,0,-1,0,0,-2,0,0,227,0,0,3764,6,51943,"WAT","HY" 13,50,5,1,,659,15,"MORRISVILLE (VILLAGE OF)","W K SANDERS",0,,12989,"0A",1294,,,95,-5,0,0,114,0,0,24,0,0,13,0,0,33,0,0,10,0,0,-1,0,0,38,0,0,-2,0,0,83,0,0,177,0,0,7,0,0,678,6,51943,"WAT","HY" 13,50,5,1,,737,5,"SWANTON (VILLAGE OF)","HIGHGATE FL",0,,18371,"0A",1294,,,95,3846,0,0,2084,0,0,5329,0,0,5012,0,0,4484,0,0,2556,0,0,711,0,0,1431,0,0,444,0,0,4486,0,0,6056,0,0,2920,0,0,6618,6,52864,"WAT","HY" 13,50,8,1,,800,5,"VERMONT ELECTRIC COOP","N HARTLAND",0,,19791,"0A",1294,,,95,1260,0,0,415,0,0,212,0,0,990,0,0,623,0,0,190,0,0,90,0,0,4,0,0,8,0,0,484,0,0,1466,0,0,734,0,0,590,6,53125,"WAT","HY" 13,50,8,1,,810,5,"WASHINGTON ELECTRIC COOP","WRIGHTSVILE",0,,20151,"0A",1294,,,95,270,0,0,88,0,0,334,0,0,327,0,0,246,0,0,50,0,0,54,0,0,128,0,0,47,0,0,3224,0,0,418,0,0,153,0,0,7051,6,58100,"WAT","HY" 14,25,1,2,1,23,1,"BOSTON EDISON CO","PILGRIM",0,"NUCLEAR",1998,"0M",1294,,,95,494219,0,0,433548,0,0,370903,0,0,0,0,0,0,0,0,313826,0,0,476983,0,0,486906,0,0,466384,0,0,470820,0,0,479805,0,0,492451,0,0,1590,6,50300,"UR","ST" 14,25,1,4,2,23,15,"BOSTON EDISON CO","EDGAR",0,"LIGHT OIL",1998,"0M",1294,,,95,43,139,1048,160,393,893,25,79,1053,64,124,929,28,74,855,110,379,953,323,950,955,245,760,910,38,108,1040,37,107,933,56,139,1032,134,337,934,1585,6,50300,"FO2","GT" 14,25,1,4,2,23,17,"BOSTON EDISON CO","FRAMINGHAM",0,"LIGHT OIL",1998,"0M",1294,,,95,141,378,1770,276,681,1804,67,203,1601,44,165,1674,70,215,1698,449,1329,1559,788,2383,1819,766,2306,1658,95,258,1630,53,142,1734,74,277,1695,278,761,1649,1586,6,50300,"FO2","GT" 14,25,1,4,2,23,20,"BOSTON EDISON CO","L STREET",0,"LIGHT OIL",1998,"0M",1294,,,95,18,71,606,223,524,481,31,74,586,101,254,571,64,181,628,302,790,611,232,657,597,450,1241,537,70,195,581,33,121,579,41,95,603,202,478,601,1587,6,50300,"FO2","GT" 14,25,1,2,2,23,25,"BOSTON EDISON CO","MYSTIC",0,"LIGHT OIL",1998,"0M",1294,,,95,251,519,1723,2082,3518,560,0,0,2480,874,1565,1748,1508,2858,1987,1285,2470,2852,2284,4277,1789,1325,2537,1992,119,230,1762,111,219,2019,220,439,1580,238,420,1327,1588,6,50300,"FO2","ST" 14,25,1,2,3,23,25,"BOSTON EDISON CO","MYSTIC",0,"HEAVY OIL",1998,"0M",1294,,,95,112692,212897,634701,250006,389639,396000,28170,35809,578539,46219,75659,622498,47350,81843,540595,74633,131731,529651,114158,195470,453259,65504,114254,339850,9543,16899,623019,18574,33314,589243,137777,234264,549412,333744,539006,466193,1588,6,50300,"FO6","ST" 14,25,1,2,9,23,25,"BOSTON EDISON CO","MYSTIC",0,"NAT GAS",1998,"0M",1294,,,95,54301,611365,0,41760,387451,0,199825,2260608,0,223483,2242300,0,121095,1295784,0,76698,835115,0,229079,2424349,0,221936,2420968,0,166749,1844575,0,138588,1545200,0,1185,12271,0,4690,47014,0,1588,6,50300,"NG","ST" 14,25,1,4,2,23,25,"BOSTON EDISON CO","MYSTIC",0,"LIGHT OIL",1998,"0M",1294,,,95,27,56,491,103,175,435,20,57,497,61,110,506,37,71,435,192,369,532,279,524,365,264,506,455,27,53,523,26,52,471,36,92,498,52,92,444,1588,6,50300,"FO2","GT" 14,25,1,2,2,23,30,"BOSTON EDISON CO","NEW BOSTON",0,"LIGHT OIL",1998,"0M",1294,,,95,0,0,60,0,0,60,0,0,60,0,0,60,0,0,60,0,0,60,0,0,60,0,0,60,0,0,60,0,0,60,0,0,60,0,0,60,1589,6,50300,"FO2","ST" 14,25,1,2,3,23,30,"BOSTON EDISON CO","NEW BOSTON",0,"HEAVY OIL",1998,"0M",1294,,,95,215120,320592,70394,155709,225131,71506,167349,258313,38374,0,0,38374,0,0,38374,0,0,38374,0,0,38403,0,0,38403,0,0,38403,0,0,38808,0,0,73197,633,1026,94600,1589,6,50300,"FO6","ST" 14,25,1,2,9,23,30,"BOSTON EDISON CO","NEW BOSTON",0,"NAT GAS",1998,"0M",1294,,,95,0,0,0,151,1334,0,2301,23751,0,201560,2042478,0,231080,2303282,0,366745,3613841,0,376840,3697457,0,381210,3746576,0,337660,3311625,0,328300,3254233,0,343010,3322669,0,159417,1573389,0,1589,6,50300,"NG","ST" 14,25,1,4,2,23,40,"BOSTON EDISON CO","WEST MEDWAY",0,"LIGHT OIL",1998,"0M",1294,,,95,532,1305,6724,2615,5858,6588,305,882,6659,441,1064,6548,648,1783,6907,1922,5806,5619,2304,7193,6789,2376,1139,6841,43,153,6688,33,101,6587,199,636,6665,2492,6199,6929,1592,6,50300,"FO2","GT" 14,25,1,4,9,23,40,"BOSTON EDISON CO","WEST MEDWAY",0,"NAT GAS",1998,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,963,16262,0,363,42170,0,305,906,0,134,2149,0,0,0,0,0,0,0,1592,6,50300,"NG","GT" 14,25,1,2,3,25,5,"COMMONWEALTH ENERGY SYS","BLACKSTONE",0,"HEAVY OIL",4120,"0M",1294,,80,95,12,9,1622,622,891,254,0,0,0,12,11,3277,4,9,3067,8,31,3303,19,66,3122,71,286,2313,8,25,2707,0,0,2900,388,267,2375,216,151,3016,1594,6,50412,"FO6","ST" 14,25,1,2,9,25,5,"COMMONWEALTH ENERGY SYS","BLACKSTONE",0,"NAT GAS",4120,"0M",1294,,80,95,643,3052,0,809,7234,0,0,0,0,329,1924,0,176,2782,0,306,7064,0,840,18553,0,641,16359,0,98,2009,0,0,0,0,26,113,0,3,12,0,1594,6,50412,"NG","ST" 14,25,1,2,3,25,10,"COMMONWEALTH ENERGY SYS","KENDALL SQ",0,"HEAVY OIL",4120,"0M",1294,,80,95,1966,3331,44639,4440,7426,46357,571,1025,43350,551,1184,40895,279,518,39729,76,146,39422,226,384,45928,178,367,45253,473,969,43288,91,206,42859,6937,10643,43043,10035,14044,33074,1595,6,50412,"FO6","ST" 14,25,1,2,9,25,10,"COMMONWEALTH ENERGY SYS","KENDALL SQ",0,"NAT GAS",4120,"0M",1294,,80,95,8305,87563,0,5498,57215,0,7487,85115,0,6963,94695,0,6096,81153,0,7445,90078,0,8638,93009,0,7941,103714,0,6154,79756,0,5898,84299,0,580,5629,0,447,3954,0,1595,6,50412,"NG","ST" 14,25,1,4,2,25,10,"COMMONWEALTH ENERGY SYS","KENDALL SQ",0,"LIGHT OIL",4120,"0M",1294,,80,95,0,0,1889,173,442,1930,0,0,1930,10,26,1904,381,951,1671,340,886,1969,587,1240,1863,822,2088,2078,160,754,1323,0,0,1561,0,0,1561,183,453,1925,1595,6,50412,"FO2","GT" 14,25,1,2,3,25,15,"COMMONWEALTH ENERGY SYS","CANAL",0,"HEAVY OIL",4120,"0M",1294,,80,95,162391,279085,64428,147412,254620,37606,178077,310890,35916,210807,342420,34150,172965,296386,68134,149960,274442,64297,204907,357210,66759,386648,623547,65078,202416,316252,66152,59087,109907,66707,307766,492512,64272,421791,645524,63446,1599,6,50412,"FO6","ST" 14,25,1,3,2,25,25,"COMMONWEALTH ENERGY SYS","OAK BLUFFS",0,"LIGHT OIL",4120,"0M",1294,,80,95,0,0,1131,70,125,1006,0,0,1006,3,6,1000,58,98,1011,55,97,1035,183,321,1005,196,350,1036,1,4,1032,0,0,1159,6,15,1144,63,118,1026,1597,6,50412,"FO2","IC" 14,25,1,3,2,25,30,"COMMONWEALTH ENERGY SYS","W TISBURY",0,"LIGHT OIL",4120,"0M",1294,,80,95,0,0,2023,42,87,1936,0,0,1936,2,4,1932,38,68,1918,40,70,1848,243,439,1711,204,373,1827,0,0,1827,0,0,2044,5,18,2026,47,98,1928,6049,6,50412,"FO2","IC" 14,25,1,3,2,25,35,"COMMONWEALTH ENERGY SYS","AIRPORT DIE",0,"LIGHT OIL",4120,"0M",1294,,80,95,2,4,65,20,32,57,6,9,48,14,26,23,3,17,6,0,6,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,7184,6,50412,"FO2","IC" 14,25,1,4,2,46,1,"FITCHBURG GAS & ELEC LGT","FITCHBURG",0,"LIGHT OIL",6374,"0M",1294,,,95,113,320,1233,544,1372,812,0,0,1289,68,210,1079,120,416,1139,539,1444,1109,663,1798,2154,708,1974,1126,70,191,2125,49,166,1960,0,0,1960,461,1173,2216,1601,6,50990,"FO2","GT" 14,25,1,1,,59,5,"HOLYOKE WTR PWR CO","BB HOLBROOK",0,,8779,"0M",1294,,554,95,215,0,0,12,0,0,439,0,0,48,0,0,0,0,0,-4,0,0,-2,0,0,111,0,0,7,0,0,88,0,0,177,0,0,95,0,0,1602,6,51327,"WAT","HY" 14,25,1,1,,59,7,"HOLYOKE WTR PWR CO","CHEMICAL",0,,8779,"0M",1294,,554,95,390,0,0,65,0,0,264,0,0,560,0,0,1378,0,0,-3,0,0,-2,0,0,33,0,0,-2,0,0,199,0,0,228,0,0,152,0,0,1604,6,51327,"WAT","HY" 14,25,1,1,,59,10,"HOLYOKE WTR PWR CO","HADLEY FLLS",0,,8779,"0M",1294,,554,95,19318,0,0,16252,0,0,20835,0,0,17997,0,0,1047,0,0,10005,0,0,4815,0,0,8945,0,0,1536,0,0,13795,0,0,19251,0,0,19209,0,0,1605,6,51327,"WAT","HY" 14,25,1,1,,59,15,"HOLYOKE WTR PWR CO","RIVERSIDE",0,,8779,"0M",1294,,554,95,2283,0,0,798,0,0,2407,0,0,2806,0,0,1058,0,0,-32,0,0,-28,0,0,236,0,0,-31,0,0,991,0,0,1475,0,0,1658,0,0,1607,6,51327,"WAT","HY" 14,25,1,1,,59,20,"HOLYOKE WTR PWR CO","BOATLOCK",0,,8779,"0M",1294,,554,95,1401,0,0,440,0,0,1465,0,0,1749,0,0,-1985,0,0,-45,0,0,34,0,0,364,0,0,188,0,0,1015,0,0,1030,0,0,1719,0,0,1603,6,51327,"WAT","HY" 14,25,1,1,,59,21,"HOLYOKE WTR PWR CO","SKINNER",0,,8779,"0M",1294,,554,95,1087,0,0,-990,0,0,135,0,0,122,0,0,0,0,0,-3,0,0,-3,0,0,10,0,0,-5,0,0,48,0,0,88,0,0,144,0,0,1608,6,51327,"WAT","HY" 14,25,1,2,2,59,23,"HOLYOKE WTR PWR CO","MT TOM",0,"LIGHT OIL",8779,"0M",1294,,554,95,253,312,334,85,74,223,86,144,363,96,161,0,210,338,471,128,216,400,63,106,0,319,575,0,148,244,0,283,596,339,311,528,442,268,461,289,1606,6,51327,"FO2","ST" 14,25,1,2,6,59,23,"HOLYOKE WTR PWR CO","MT TOM",0,"BIT COAL",8779,"0M",1294,,554,95,83436,31625,65901,94304,36568,48767,100316,38568,48417,92219,34981,57613,86828,32256,68520,89522,33641,55040,96838,37232,50903,67013,26869,64337,58083,21428,72102,20300,9635,85211,75120,28714,96373,83498,33548,87268,1606,6,51327,"BIT","ST" 14,25,1,2,3,85,1,"MONTAUP ELECTRIC COMPANY","SOMERSET",0,"HEAVY OIL",12833,"0M",1294,,,95,5362,8778,70647,3605,6271,64376,3682,6389,57987,572,894,57093,4068,7388,49705,3861,6474,101371,1808,3090,98281,1729,8455,89825,4071,6826,83000,7484,12748,70251,8762,14647,55605,1259,3587,97942,1613,6,56511,"FO6","ST" 14,25,1,2,6,85,1,"MONTAUP ELECTRIC COMPANY","SOMERSET",0,"BIT COAL",12833,"0M",1294,,,95,57318,21462,76767,61443,26125,64290,61730,25219,52529,14739,5125,47404,25607,10149,50811,58410,21998,42203,65563,26654,42553,52228,21241,48670,53057,20314,65856,44642,17190,76089,48433,18499,83931,70559,26084,98563,1613,6,56511,"BIT","ST" 14,25,1,4,2,85,1,"MONTAUP ELECTRIC COMPANY","SOMERSET",0,"LIGHT OIL",12833,"0M",1294,,,95,143,374,5116,433,1118,3998,115,229,3769,65,186,3583,285,740,4510,629,1593,4110,1349,3410,5229,1777,4429,5348,136,348,5000,0,0,4999,5,26,5687,653,1369,4318,1613,6,56511,"FO2","GT" 14,25,1,3,2,90,15,"NANTUCKET ELEC CO","NANTUCKET",0,"LIGHT OIL",13206,"0M",1294,,,95,7539,12658,2602,7625,13184,8503,7218,12056,5494,6969,12757,2261,7465,13354,7937,7820,14759,9687,10453,19444,7486,10644,19689,5848,7894,13523,10626,6823,12246,7898,7832,14492,3042,9557,16800,2912,1615,6,51977,"FO2","IC" 14,25,1,1,,96,5,"NEW ENGLAND POWER CO","DEERFIELD 2",0,,13433,"0M",1294,,90,95,3908,0,0,2952,0,0,3971,0,0,2045,0,0,1064,0,0,520,0,0,442,0,0,617,0,0,404,0,0,2016,0,0,3583,0,0,2747,0,0,6047,6,52007,"WAT","HY" 14,25,1,1,,96,10,"NEW ENGLAND POWER CO","DEERFIELD 3",0,,13433,"0M",1294,,90,95,4040,0,0,3243,0,0,4233,0,0,2293,0,0,1182,0,0,848,0,0,445,0,0,722,0,0,460,0,0,1885,0,0,3570,0,0,3116,0,0,6083,6,52007,"WAT","HY" 14,25,1,1,,96,15,"NEW ENGLAND POWER CO","DEERFIELD 4",0,,13433,"0M",1294,,90,95,3691,0,0,2835,0,0,3555,0,0,1674,0,0,865,0,0,673,0,0,414,0,0,621,0,0,420,0,0,1920,0,0,3135,0,0,2638,0,0,6119,6,52007,"WAT","HY" 14,25,1,1,,96,20,"NEW ENGLAND POWER CO","DEERFIELD 5",0,,13433,"0M",1294,,90,95,8684,0,0,6946,0,0,8699,0,0,2314,0,0,807,0,0,564,0,0,515,0,0,177,0,0,0,0,0,0,0,0,3382,0,0,5810,0,0,1620,6,52007,"WAT","HY" 14,25,1,1,,96,25,"NEW ENGLAND POWER CO","SHERMAN",0,,13433,"0M",1294,,90,95,4117,0,0,3467,0,0,4264,0,0,1151,0,0,407,0,0,439,0,0,377,0,0,602,0,0,527,0,0,2183,0,0,3889,0,0,2917,0,0,6012,6,52007,"WAT","HY" 14,25,1,2,3,96,27,"NEW ENGLAND POWER CO","BRAYTON PT",0,"HEAVY OIL",13433,"0M",1294,,90,95,40093,74054,435541,65951,116563,318656,49098,75749,438283,41100,69916,368366,2212,5326,519600,0,0,519442,0,0,519401,488,4266,515767,0,0,516617,0,0,516584,7553,10954,505630,71672,125949,379784,1619,6,52007,"FO6","ST" 14,25,1,2,6,96,27,"NEW ENGLAND POWER CO","BRAYTON PT",0,"BIT COAL",13433,"0M",1294,,90,95,657136,245754,255528,538158,200282,277893,335153,130042,379361,336389,128159,523785,552184,203304,520224,709319,259373,461575,714608,267126,390587,681408,256270,431828,600517,222478,518312,676108,250140,322224,643066,226804,159986,692743,256541,166201,1619,6,52007,"BIT","ST" 14,25,1,2,9,96,27,"NEW ENGLAND POWER CO","BRAYTON PT",0,"NAT GAS",13433,"0M",1294,,90,95,2475,65992,0,19895,234494,0,87264,1046891,0,115149,1305242,0,165738,1925331,0,192541,2159965,0,121121,1465806,0,138514,1578722,0,90677,1067560,0,7950,208839,0,642,50267,0,499,65467,0,1619,6,52007,"NG","ST" 14,25,1,3,2,96,27,"NEW ENGLAND POWER CO","BRAYTON PT",0,"LIGHT OIL",13433,"0M",1294,,90,95,48,91,0,168,321,0,49,91,0,66,120,0,149,212,0,229,427,0,434,803,0,429,813,0,49,97,0,17,33,0,0,0,0,122,221,0,1619,6,52007,"FO2","IC" 14,25,1,2,3,96,33,"NEW ENGLAND POWER CO","SALEM HABR",0,"HEAVY OIL",13433,"0M",1294,,90,95,4216,6811,427550,19621,51462,372000,43825,80929,296042,52176,100975,196885,88546,157427,294207,74155,134469,405510,143472,245061,157683,78033,135040,315193,15952,29894,481681,10242,22800,451257,31856,63264,446411,130138,177251,300301,1626,6,52007,"FO6","ST" 14,25,1,2,6,96,33,"NEW ENGLAND POWER CO","SALEM HABR",0,"BIT COAL",13433,"0M",1294,,90,95,170230,67910,116594,174526,68827,87604,182421,75469,107334,180983,73494,87888,123760,53441,145441,149482,64633,132065,157915,67184,148469,169338,69504,116124,140768,59871,93091,133365,56779,72780,147538,65216,99054,158287,70574,72828,1626,6,52007,"BIT","ST" 14,25,1,3,2,96,40,"NEW ENGLAND POWER CO","GLOUCESTER",0,"LIGHT OIL",13433,"0M",1294,,90,95,180,400,1027,365,1056,1255,495,500,1183,191,320,863,798,1430,1148,331,615,1333,398,757,1219,767,1957,1197,100,165,1033,0,0,1031,2,3,1465,491,918,1190,1624,6,52007,"FO2","IC" 14,25,1,3,2,96,50,"NEW ENGLAND POWER CO","NEWBURYPORT",0,"LIGHT OIL",13433,"0M",1294,,90,95,23,31,898,242,431,942,1,0,943,124,222,720,79,135,986,279,516,828,384,714,746,466,834,770,24,47,723,5,10,715,0,0,929,200,360,998,1625,6,52007,"FO2","IC" 14,25,1,1,,96,55,"NEW ENGLAND POWER CO","FIFE BROOK",0,,13433,"0M",1294,,90,95,4107,0,0,3775,0,0,4880,0,0,1321,0,0,312,0,0,338,0,0,198,0,0,494,0,0,291,0,0,2274,0,0,4150,0,0,3161,0,0,8004,6,52007,"WAT","HY" 14,25,1,1,,96,60,"NEW ENGLAND POWER CO","BEAR SWAMP",0,"P-PUMPSTG",13433,"0M",1294,,90,95,-17861,61325,0,-15324,57381,0,-16082,58258,0,-15241,53916,0,-14630,56226,0,-16812,61971,0,-18159,63682,0,-15902,62948,0,-16995,61404,0,-17477,62001,0,-15650,58713,0,-16215,58454,0,8005,6,52007,"WAT","HY" 14,25,1,1,,145,5,"W MASSACHUSETTS ELEC CO","CABOT",0,,20455,"0M",1294,,555,95,27350,0,0,20962,0,0,33562,0,0,28813,0,0,2450,0,0,11373,0,0,5730,0,0,10888,0,0,1060,0,0,21360,0,0,32264,0,0,23532,0,0,1629,6,53266,"WAT","HY" 14,25,1,1,,145,10,"W MASSACHUSETTS ELEC CO","COBBLE MT",0,,20455,"0M",1294,,555,95,2687,0,0,2401,0,0,3134,0,0,1490,0,0,613,0,0,1371,0,0,1579,0,0,2606,0,0,404,0,0,934,0,0,679,0,0,2257,0,0,1630,6,53266,"WAT","HY" 14,25,1,1,,145,12,"W MASSACHUSETTS ELEC CO","DWIGHT",0,,20455,"0M",1294,,555,95,541,0,0,520,0,0,744,0,0,709,0,0,972,0,0,422,0,0,241,0,0,219,0,0,137,0,0,316,0,0,187,0,0,450,0,0,6378,6,53266,"WAT","HY" 14,25,1,1,,145,20,"W MASSACHUSETTS ELEC CO","GARDER FLS",0,,20455,"0M",1294,,555,95,1535,0,0,1501,0,0,2140,0,0,1273,0,0,591,0,0,393,0,0,159,0,0,373,0,0,244,0,0,740,0,0,1394,0,0,1292,0,0,1634,6,53266,"WAT","HY" 14,25,1,1,,145,30,"W MASSACHUSETTS ELEC CO","IND ORCHARD",0,,20455,"0M",1294,,555,95,1913,0,0,854,0,0,1614,0,0,786,0,0,661,0,0,177,0,0,8,0,0,59,0,0,4,0,0,434,0,0,1375,0,0,741,0,0,6379,6,53266,"WAT","HY" 14,25,1,1,,145,32,"W MASSACHUSETTS ELEC CO","PUTTS BRDGE",0,,20455,"0M",1294,,555,95,224,0,0,252,0,0,1368,0,0,249,0,0,550,0,0,741,0,0,249,0,0,393,0,0,186,0,0,1233,0,0,1150,0,0,251,0,0,1637,6,53266,"WAT","HY" 14,25,1,1,,145,33,"W MASSACHUSETTS ELEC CO","RED BRIDGE",0,,20455,"0M",1294,,555,95,2265,0,0,1259,0,0,1699,0,0,1592,0,0,1025,0,0,689,0,0,212,0,0,256,0,0,150,0,0,1248,0,0,7724,0,0,1271,0,0,1638,6,53266,"WAT","HY" 14,25,1,1,,145,35,"W MASSACHUSETTS ELEC CO","TURNERS FL",0,,20455,"0M",1294,,555,95,1180,0,0,-9,0,0,2580,0,0,457,0,0,2357,0,0,3,0,0,320,0,0,753,0,0,1529,0,0,1437,0,0,3487,0,0,96,0,0,6388,6,53266,"WAT","HY" 14,25,1,1,,145,37,"W MASSACHUSETTS ELEC CO","NORTHFLD MT",0,"P-PUMPSTG",20455,"0M",1294,,555,95,-40582,142177,0,-33131,122422,0,-34507,127754,0,-38191,123876,0,-53574,130653,0,-54650,139615,0,-65287,149806,0,-58299,150495,0,-60095,144418,0,-65178,152081,0,-51403,135668,0,-54958,140849,0,547,6,53266,"WAT","HY" 14,25,1,4,2,145,38,"W MASSACHUSETTS ELEC CO","DOREEN",0,"LIGHT OIL",20455,"0M",1294,,555,95,50,156,956,319,789,738,14,84,997,11,135,1029,31,63,967,166,460,863,117,360,1099,422,1231,1099,69,204,1073,-10,0,1073,34,122,951,162,418,771,1631,6,53266,"FO2","GT" 14,25,1,2,2,145,55,"W MASSACHUSETTS ELEC CO","W SPRINGFLD",0,"LIGHT OIL",20455,"0M",1294,,555,95,0,0,533,101,224,458,0,0,458,19,36,411,0,0,411,0,0,411,0,0,411,0,0,411,0,0,411,0,0,411,0,0,411,0,0,379,1642,6,53266,"FO2","ST" 14,25,1,2,3,145,55,"W MASSACHUSETTS ELEC CO","W SPRINGFLD",0,"HEAVY OIL",20455,"0M",1294,,555,95,3033,6175,75421,4119,8425,75374,344,607,80604,1867,3252,77352,19,33,77318,750,1321,75997,1456,2596,73401,758,1343,72058,0,0,72058,0,0,72923,2320,5181,76520,13739,24402,55074,1642,6,53266,"FO6","ST" 14,25,1,2,9,145,55,"W MASSACHUSETTS ELEC CO","W SPRINGFLD",0,"NAT GAS",20455,"0M",1294,,555,95,2167,27681,0,81,1046,0,24872,278755,0,28674,316564,0,33801,372726,0,33691,376470,0,34950,395433,0,39329,440670,0,21443,242289,0,3420,45099,0,110,1547,0,158,1773,0,1642,6,53266,"NG","ST" 14,25,1,4,2,145,55,"W MASSACHUSETTS ELEC CO","W SPRINGFLD",0,"LIGHT OIL",20455,"0M",1294,,555,95,45,159,682,84,220,801,-17,0,801,-12,0,801,-3,12,789,108,297,6777,282,717,1096,319,633,977,0,0,977,0,0,977,0,0,977,0,0,977,1642,6,53266,"FO2","GT" 14,25,1,4,2,145,60,"W MASSACHUSETTS ELEC CO","WOODLAND RD",0,"LIGHT OIL",20455,"0M",1294,,555,95,38,127,1027,218,623,814,3,20,1144,11,96,1048,22,56,992,219,604,924,341,963,1130,373,1030,1017,32,105,1090,-7,0,1090,5,59,1032,156,398,534,1643,6,53266,"FO2","GT" 14,25,5,3,2,532,5,"BRAINTREE (CITY OF)","POTTER",0,"LIGHT OIL",2144,"0M",1294,,,95,1,3,0,40,86,0,2,4,0,8,15,0,18,33,0,0,0,0,66,37,0,90,173,0,8,15,0,16,29,0,0,0,0,47,86,0,1660,6,50315,"FO2","IC" 14,25,5,5,9,532,5,"BRAINTREE (CITY OF)","POTTER",0,"WASTE HT",2144,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1660,6,50315,"NG","CC" 14,25,5,6,2,532,5,"BRAINTREE (CITY OF)","POTTER",0,"LIGHT OIL",2144,"0M",1294,,,95,597,1163,3860,1950,3916,4922,529,946,3897,722,1243,2632,0,0,2595,0,0,2595,0,0,0,0,0,0,0,0,0,418,803,0,0,0,0,563,1271,0,1660,6,50315,"FO2","CT" 14,25,5,6,9,532,5,"BRAINTREE (CITY OF)","POTTER",0,"NAT GAS",2144,"0M",1294,,,95,6985,76876,0,16116,164048,0,4161,42418,0,25648,268544,0,6647,61554,0,0,0,0,6439,68107,0,22225,231091,0,11633,125960,0,2826,30097,0,605,6473,0,2795,30378,0,1660,6,50315,"NG","CT" 14,25,5,1,,597,5,"HOLYOKE (CITY OF)","HOLYOKE",0,,8776,"0M",1294,,,95,1039,0,0,94,0,0,1200,0,0,538,0,0,244,0,0,216,0,0,169,0,0,308,0,0,243,0,0,308,0,0,843,0,0,63,0,0,9864,6,51325,"WAT","HY" 14,25,5,2,3,597,5,"HOLYOKE (CITY OF)","HOLYOKE",0,"HEAVY OIL",8776,"0M",1294,,,95,-34,8,21223,-7,161,18597,-32,0,17335,-149,242,9944,-157,0,11105,-26,144,12014,197,918,10400,173,751,10383,0,0,21744,-26,2,23445,-45,21,21407,48,571,24539,9864,6,51325,"FO6","ST" 14,25,5,2,9,597,5,"HOLYOKE (CITY OF)","HOLYOKE",0,"NAT GAS",8776,"0M",1294,,,95,-406,548,0,-47,7095,0,-432,0,0,-151,1508,0,-180,0,0,-82,2775,0,358,10343,0,495,13260,0,-282,0,0,-300,136,0,-310,907,0,116,8617,0,9864,6,51325,"NG","ST" 14,25,5,3,2,602,1,"HUDSON (CITY OF)","CHERRY ST",0,"LIGHT OIL",8973,"0A",1294,,,95,126,216,6535,468,801,5733,24,47,5687,49,79,5608,60,99,5509,136,242,5267,334,576,4687,237,442,10028,21,36,9992,0,0,9992,0,0,9992,0,613,9379,9038,6,51362,"FO2","IC" 14,25,5,3,9,602,1,"HUDSON (CITY OF)","CHERRY ST",0,"NAT GAS",8973,"0A",1294,,,95,16,177,0,0,0,0,0,0,0,27,276,0,223,2327,0,514,5353,0,813,8555,0,1067,10973,0,248,2679,0,0,0,0,0,0,0,0,0,0,9038,6,51362,"NG","IC" 14,25,5,3,2,613,1,"IPSWICH (CITY OF)","IPSWICH",0,"LIGHT OIL",9442,"0A",1294,,,95,3,144,1524,185,504,1020,-44,84,928,26,97,839,45,81,751,112,229,1817,221,430,1388,171,335,1053,42,71,981,0,0,1991,0,13,1901,70,285,1616,1670,6,51411,"FO2","IC" 14,25,5,3,9,613,1,"IPSWICH (CITY OF)","IPSWICH",0,"NAT GAS",9442,"0A",1294,,,95,0,0,0,0,0,0,-7,91,0,26,564,0,193,2049,0,356,4180,0,540,6225,0,488,5467,0,218,2149,0,0,0,0,0,164,0,0,0,0,1670,6,51411,"NG","IC" 14,25,5,3,2,630,20,"MARBLEHEAD (CITY OF)","COMM ST 2",0,"LIGHT OIL",11624,"0A",1294,,,95,0,0,134,30,54,153,0,0,124,1,4,109,8,23,86,22,43,163,30,67,96,40,77,139,3,3,134,0,0,129,0,0,107,16,31,153,6585,6,51769,"FO2","IC" 14,25,5,3,2,630,25,"MARBLEHEAD (CITY OF)","WILKINS STA",0,"LIGHT OIL",11624,"0A",1294,,,95,24,42,422,242,404,495,3,4,490,17,25,466,41,67,398,140,249,387,184,331,532,214,384,390,17,34,833,0,0,831,0,0,833,105,187,646,6586,6,51769,"FO2","IC" 14,25,5,4,2,640,5,"MASS MUN WHOLESALE ELEC","STONY BROOK",0,"LIGHT OIL",11806,"0M",1294,,,95,868,1812,0,3250,6760,0,1070,2159,0,1016,2152,0,1531,3641,0,3583,7206,0,6923,15010,0,5440,12228,0,1296,2825,0,251,525,0,0,0,0,2081,4355,0,6081,6,56516,"FO2","GT" 14,25,5,5,2,640,5,"MASS MUN WHOLESALE ELEC","STONY BROOK",0,"LIGHT OIL",11806,"0M",1294,,,95,4867,0,0,4882,0,0,1895,0,0,0,0,0,1645,0,0,1298,0,0,2909,0,0,2231,0,0,542,0,0,137,0,0,778,0,0,7866,0,0,6081,6,56516,"FO2","CC" 14,25,5,5,9,640,5,"MASS MUN WHOLESALE ELEC","STONY BROOK",0,"WASTE HT",11806,"0M",1294,,,95,667,6409,0,33,225,0,713,7903,0,38860,226425,0,32080,282829,0,30410,271547,0,30355,268417,0,22281,199679,0,16911,152536,0,13731,126250,0,649,6336,0,0,0,0,6081,6,56516,"NG","CC" 14,25,5,6,2,640,5,"MASS MUN WHOLESALE ELEC","STONY BROOK",0,"LIGHT OIL",11806,"0M",1294,,,95,16765,34499,275954,17076,35625,171066,1732,3145,164811,15194,31318,130811,4458,10049,117055,3259,6474,203614,7129,14689,223923,5719,12097,199458,1427,2966,193410,406,852,191674,2974,6318,192851,24527,50346,140778,6081,6,56516,"FO2","CT" 14,25,5,6,9,640,5,"MASS MUN WHOLESALE ELEC","STONY BROOK",0,"NAT GAS",11806,"0M",1294,,,95,2298,22081,0,33,225,0,7123,78947,0,38860,226425,0,85133,750563,0,75927,677993,0,74156,655728,0,57044,511219,0,44278,399380,0,38588,354794,0,2475,24166,0,0,0,0,6081,6,56516,"NG","CT" 14,25,5,4,2,668,10,"PEABODY (CITY OF)","WATERS RIVR",0,"LIGHT OIL",14605,"0M",1294,,,95,4,11,7009,461,990,6019,3,13,6006,114,218,5789,218,411,5378,259,572,4806,1447,3081,5724,79,204,5787,0,0,5770,0,0,5770,0,0,5770,751,1304,4214,1678,6,52270,"FO2","GT" 14,25,5,4,9,668,10,"PEABODY (CITY OF)","WATERS RIVR",0,"NAT GAS",14605,"0M",1294,,,95,71,948,0,818,8676,0,0,0,0,298,3898,0,500,6079,0,1161,14052,0,735,10563,0,2810,34245,0,871,10971,0,16,244,0,0,0,0,136,1612,0,1678,6,52270,"NG","GT" 14,25,5,3,2,695,1,"SHREWSBURY (CITY OF)","SHREWSBURY",0,"LIGHT OIL",17127,"0A",1294,,,95,-48,53,1717,-20,96,1621,-72,0,1621,-59,0,1621,-27,43,1577,28,133,1444,206,450,994,393,793,1630,-12,58,1571,-52,4,1568,-66,0,1568,5,146,1421,6125,6,52653,"FO2","IC" 14,25,5,2,3,711,10,"TAUNTON (CITY OF)","CLRY FLOOD",0,"HEAVY OIL",18488,"0M",1294,,,95,707,1487,45484,117,274,41056,124,1171,40232,227,881,38944,154,338,18232,1782,3821,13122,1997,4404,13146,1671,3714,26632,1017,1981,30701,285,1042,41468,209,665,43572,1269,2308,3691,1682,6,52885,"FO6","ST" 14,25,5,5,3,711,10,"TAUNTON (CITY OF)","CLRY FLOOD",0,"HEAVY OIL",18488,"0M",1294,,,95,2588,4259,0,3074,4987,0,7,71,0,264,1016,0,10569,21610,0,5376,8750,0,7132,10296,0,7761,11325,0,6430,8473,0,269,1218,0,135,435,0,7563,7563,0,1682,6,52885,"FO6","CC" 14,25,5,5,9,711,10,"TAUNTON (CITY OF)","CLRY FLOOD",0,"NAT GAS",18488,"0M",1294,,,95,0,0,0,88,2162,0,0,0,0,0,7,0,70,898,0,11828,118101,0,7953,72245,0,11517,102477,0,3409,38796,0,275,3743,0,0,0,0,0,0,0,1682,6,52885,"NG","CC" 14,25,5,6,2,711,10,"TAUNTON (CITY OF)","CLRY FLOOD",0,"LIGHT OIL",18488,"0M",1294,,,95,600,1721,500,1175,3321,414,0,10,405,0,0,405,23,155,250,230,719,0,424,1426,393,75,247,983,20,69,920,0,0,922,172,601,798,1596,4611,881,1682,6,52885,"FO2","CT" 14,25,5,6,3,711,10,"TAUNTON (CITY OF)","CLRY FLOOD",0,"HEAVY OIL",18488,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1682,6,52885,"FO6","CT" 14,25,5,6,9,711,10,"TAUNTON (CITY OF)","CLRY FLOOD",0,"NAT GAS",18488,"0M",1294,,,95,215,3547,0,0,0,0,0,0,0,9,220,0,91,2523,0,3269,55134,0,3573,59309,0,4974,79500,0,4776,58796,0,188,2751,0,2,41,0,0,0,0,1682,6,52885,"NG","CT" 15,44,1,3,2,59,1,"BLOCK ISLAND POWER CO","BLOCK ISL",0,"LIGHT OIL",1857,"0A",1294,,,95,640,929,1894,560,757,1368,454,801,1953,666,926,2412,871,1183,2384,728,1492,1815,1748,2173,1258,1686,2317,1251,852,1532,1104,890,1214,1044,683,904,1044,537,1042,1378,6567,6,50270,"FO2","IC" 15,44,1,2,3,60,5,"NEW ENGLAND POWER CO","MANCHSTR ST",0,"HEAVY OIL",13433,"0M",1294,,90,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,6954,6984,12805,21121,8031,15471,21089,11950,17787,9381,10642,17134,20900,3236,6,52007,"FO6","ST" 15,44,1,2,6,60,5,"NEW ENGLAND POWER CO","MANCHSTR ST",0,"BIT COAL",13433,"0M",1294,,90,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,3236,6,52007,"BIT","ST" 15,44,1,2,9,60,5,"NEW ENGLAND POWER CO","MANCHSTR ST",0,"NAT GAS",13433,"0M",1294,,90,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,185,6790,0,5496,108488,0,22180,283931,0,57696,544903,0,43911,426261,0,200212,1571059,0,273062,2060878,0,3236,6,52007,"NG","ST" 15,44,1,3,2,71,5,"NEWPORT ELECTRIC CORP","ELDRED",0,"LIGHT OIL",13549,"0A",1294,,,95,0,0,912,146,241,919,0,0,916,14,24,893,280,476,872,38,285,806,254,445,603,431,759,765,53,97,884,0,0,884,30,55,818,186,311,942,3240,6,52046,"FO2","IC" 15,44,1,3,2,71,15,"NEWPORT ELECTRIC CORP","JEPSON",0,"LIGHT OIL",13549,"0A",1294,,,95,10,19,1047,104,179,864,0,0,1112,13,24,1094,58,103,998,35,303,926,228,421,966,339,620,1037,31,56,977,0,0,977,0,0,977,162,273,920,3241,6,52046,"FO2","IC" 15,44,5,1,,600,1,"PROVIDENCE (CITY OF)","PROVIDENCE",0,,15440,"0A",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,3245,6,52404,"WAT","HY" 16,9,1,1,,21,1,"GILMAN BROTHERS CO","GILMAN",0,,6885,"0A",1294,"R",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,536,6,50309,"WAT","HY" 16,9,1,1,,37,5,"CONNECTICUT LGT & PWR CO","BULLS BRDGE",0,,4176,"0M",1294,,550,95,4542,0,0,3859,0,0,4535,0,0,4526,0,0,711,0,0,1545,0,0,596,0,0,576,0,0,83,0,0,3291,0,0,5258,0,0,4512,0,0,541,6,50651,"WAT","HY" 16,9,1,1,,37,15,"CONNECTICUT LGT & PWR CO","ROBERTSVLE",0,,4176,"0M",1294,,550,95,228,0,0,144,0,0,74,0,0,117,0,0,0,0,0,23,0,0,4,0,0,14,0,0,1,0,0,58,0,0,0,0,0,7,0,0,549,6,50651,"WAT","HY" 16,9,1,1,,37,20,"CONNECTICUT LGT & PWR CO","ROCKY RIVER",0,"C-PUMPSTG",4176,"0M",1294,,550,95,-532,573,0,-108,831,0,-5011,4942,0,-3890,3881,0,-2483,2464,0,-30,0,0,-50,160,0,-45,941,0,-34,0,0,-295,262,0,3242,0,0,3543,0,0,539,6,50651,"WAT","HY" 16,9,1,1,,37,25,"CONNECTICUT LGT & PWR CO","SCOTLAND DM",0,,4176,"0M",1294,,550,95,1196,0,0,762,0,0,1285,0,0,753,0,0,65,0,0,169,0,0,32,0,0,83,0,0,9,0,0,401,0,0,43,0,0,524,0,0,551,6,50651,"WAT","HY" 16,9,1,1,,37,28,"CONNECTICUT LGT & PWR CO","SHEPAUG",0,,4176,"0M",1294,,550,95,19987,0,0,8510,0,0,16746,0,0,8668,0,0,479,0,0,3113,0,0,1323,0,0,1665,0,0,561,0,0,4280,0,0,17593,0,0,9586,0,0,552,6,50651,"WAT","HY" 16,9,1,1,,37,30,"CONNECTICUT LGT & PWR CO","STEVENSON",0,,4176,"0M",1294,,550,95,14594,0,0,6873,0,0,12878,0,0,7022,0,0,5946,0,0,2333,0,0,1155,0,0,1565,0,0,585,0,0,7574,0,0,15018,0,0,7269,0,0,553,6,50651,"WAT","HY" 16,9,1,1,,37,33,"CONNECTICUT LGT & PWR CO","TAFTVILLE",0,,4176,"0M",1294,,550,95,1047,0,0,773,0,0,1181,0,0,662,0,0,0,0,0,286,0,0,106,0,0,168,0,0,58,0,0,376,0,0,802,0,0,539,0,0,554,6,50651,"WAT","HY" 16,9,1,1,,37,35,"CONNECTICUT LGT & PWR CO","TUNNEL",0,,4176,"0M",1294,,550,95,1344,0,0,790,0,0,1127,0,0,808,0,0,808,0,0,130,0,0,51,0,0,62,0,0,13,0,0,528,0,0,1238,0,0,756,0,0,557,6,50651,"WAT","HY" 16,9,1,4,2,37,35,"CONNECTICUT LGT & PWR CO","TUNNEL",0,"LIGHT OIL",4176,"0M",1294,,550,95,92,241,1121,148,413,1052,-10,0,1052,8,34,1017,-9,0,1017,174,492,1054,399,1075,1028,391,1123,1060,-10,0,1060,-9,0,1060,-8,0,1060,247,642,1013,557,6,50651,"FO2","GT" 16,9,1,4,2,37,37,"CONNECTICUT LGT & PWR CO","COS COB",0,"LIGHT OIL",4176,"0M",1294,,550,95,338,879,6366,1004,2550,5530,-6,0,6730,61,328,6402,100,252,6836,1043,2766,6164,1606,4183,6744,1574,4512,6417,89,372,6045,10,115,5931,-7,47,5884,478,1250,6205,542,6,50651,"FO2","GT" 16,9,1,2,2,37,40,"CONNECTICUT LGT & PWR CO","DEVON",0,"LIGHT OIL",4176,"0M",1294,,550,95,4,7,607,26,48,738,10,19,719,8,14,705,6,12,693,5,10,683,12,21,662,5,10,652,35,67,586,12,21,564,10,19,545,126,250,652,544,6,50651,"FO2","ST" 16,9,1,2,3,37,40,"CONNECTICUT LGT & PWR CO","DEVON",0,"HEAVY OIL",4176,"0M",1294,,550,95,1691,2896,140820,5317,8938,131882,6310,10503,160145,2309,3909,156236,1040,1748,154488,1026,1746,152742,366,624,152118,0,0,152118,0,0,152118,1119,1895,186866,0,0,223227,52715,95704,164704,544,6,50651,"FO6","ST" 16,9,1,2,9,37,40,"CONNECTICUT LGT & PWR CO","DEVON",0,"NAT GAS",4176,"0M",1294,,550,95,139882,1480772,0,125833,1333372,0,140034,1484076,0,74718,805341,0,129292,1364215,0,113222,1209824,0,134347,1440396,0,141005,1520883,0,84240,919763,0,92690,988325,0,85651,910220,0,1027,11734,0,544,6,50651,"NG","ST" 16,9,1,4,2,37,40,"CONNECTICUT LGT & PWR CO","DEVON",0,"LIGHT OIL",4176,"0M",1294,,550,95,-8,0,826,52,143,1016,-6,0,1016,11,41,975,15,50,924,93,252,873,213,464,899,323,840,1155,12,42,1113,14,46,864,-8,0,864,126,312,755,544,6,50651,"FO2","GT" 16,9,1,2,2,37,45,"CONNECTICUT LGT & PWR CO","MONTVILLE",0,"LIGHT OIL",4176,"0M",1294,,550,95,79,187,224,71,184,282,0,0,277,35,81,316,26,52,254,126,275,254,225,460,205,169,342,281,13,78,193,-9,27,344,11,35,57,248,530,404,546,6,50651,"FO2","ST" 16,9,1,2,3,37,45,"CONNECTICUT LGT & PWR CO","MONTVILLE",0,"HEAVY OIL",4176,"0M",1294,,550,95,19404,42123,179930,11903,28403,229734,496,984,267130,8852,18669,287361,73,131,287230,16090,31789,255441,33046,60820,194621,29759,54794,250449,448,2452,286041,-459,1261,284780,4782,14127,272628,50192,96782,219079,546,6,50651,"FO6","ST" 16,9,1,2,9,37,45,"CONNECTICUT LGT & PWR CO","MONTVILLE",0,"NAT GAS",4176,"0M",1294,,550,95,2644,35575,0,1337,19886,0,14239,177907,0,15760,209674,0,26332,300080,0,15321,191070,0,33080,384304,0,29657,341116,0,660,22744,0,-410,7132,0,948,17617,0,2622,31910,0,546,6,50651,"NG","ST" 16,9,1,3,2,37,45,"CONNECTICUT LGT & PWR CO","MONTVILLE",0,"LIGHT OIL",4176,"0M",1294,,550,95,5,11,429,51,91,429,3,5,429,21,47,429,5,10,429,32,60,429,47,88,429,44,82,429,5,10,429,0,0,429,7,15,429,14,27,429,546,6,50651,"FO2","IC" 16,9,1,2,2,37,46,"CONNECTICUT LGT & PWR CO","NORWALK HAR",0,"LIGHT OIL",4176,"0M",1294,,550,95,1942,3751,1166,1049,1831,1166,1411,2570,1166,801,1409,746,830,1566,1275,1306,2393,1275,1212,2164,1208,1005,1793,1129,448,996,1090,743,1549,1201,1863,3623,816,1573,2830,1073,548,6,50651,"FO2","ST" 16,9,1,2,3,37,46,"CONNECTICUT LGT & PWR CO","NORWALK HAR",0,"HEAVY OIL",4176,"0M",1294,,550,95,61485,109340,281515,116317,186438,251428,53269,89422,277523,112195,177490,244461,49615,86635,387526,72024,117143,423659,87276,142042,395624,69104,110519,365065,12764,26032,444868,12966,24423,458286,56112,97835,437824,98414,160154,343905,548,6,50651,"FO6","ST" 16,9,1,4,2,37,46,"CONNECTICUT LGT & PWR CO","NORWALK HAR",0,"LIGHT OIL",4176,"0M",1294,"R",550,95,0,0,0,0,0,0,-12,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,548,6,50651,"FO2","GT" 16,9,1,1,,37,60,"CONNECTICUT LGT & PWR CO","BANTAM",0,,4176,"0M",1294,,550,95,166,0,0,122,0,0,177,0,0,99,0,0,0,0,0,24,0,0,2,0,0,9,0,0,0,0,0,66,0,0,182,0,0,126,0,0,6457,6,50651,"WAT","HY" 16,9,1,1,,37,65,"CONNECTICUT LGT & PWR CO","FLS VILLAGE",0,,4176,"0M",1294,,550,95,6485,0,0,3067,0,0,6148,0,0,4269,0,0,57,0,0,1043,0,0,359,0,0,386,0,0,86,0,0,3283,0,0,6134,0,0,3241,0,0,560,6,50651,"WAT","HY" 16,9,1,4,2,37,70,"CONNECTICUT LGT & PWR CO","FRANKLIN DR",0,"LIGHT OIL",4176,"0M",1294,,550,95,87,251,1073,112,303,770,-21,0,770,6,41,429,9,45,1229,156,508,1033,386,937,931,385,1480,880,-11,0,808,-12,0,808,-14,0,0,109,306,1000,561,6,50651,"FO2","GT" 16,9,1,2,2,37,75,"CONNECTICUT LGT & PWR CO","MIDDLETOWN",0,"LIGHT OIL",4176,"0M",1294,,550,95,52,116,72,106,200,205,37,72,134,69,119,181,93,171,177,62,115,62,142,274,121,143,283,195,159,331,184,25,61,123,89,174,116,58,124,159,562,6,50651,"FO2","ST" 16,9,1,2,3,37,75,"CONNECTICUT LGT & PWR CO","MIDDLETOWN",0,"HEAVY OIL",4176,"0M",1294,,550,95,28156,57773,619646,82338,144562,470965,28954,52136,494722,112799,180932,367774,91771,154447,321716,103385,178821,285273,180564,315539,192342,120265,219668,308678,14240,27382,395204,9172,20697,432521,29631,53865,465010,116423,197687,379501,562,6,50651,"FO6","ST" 16,9,1,4,2,37,75,"CONNECTICUT LGT & PWR CO","MIDDLETOWN",0,"LIGHT OIL",4176,"0M",1294,,550,95,0,0,986,60,155,998,2,12,986,0,0,986,18,56,1096,133,235,803,220,518,962,326,864,969,6,21,948,0,0,946,0,0,936,0,0,936,562,6,50651,"FO2","GT" 16,9,1,2,"C",37,80,"CONNECTICUT LGT & PWR CO","S MEADOW",0,"REFUSE",4176,"0M",1294,,550,95,36668,0,0,31584,0,0,30750,0,0,36558,0,0,4988,0,0,38064,0,0,35273,0,0,35840,0,0,37803,0,0,39379,0,0,36583,0,0,40236,0,0,563,6,50651,"GEO","ST" 16,9,1,4,2,37,80,"CONNECTICUT LGT & PWR CO","S MEADOW",0,"LIGHT OIL",4176,"0M",1294,,550,95,547,1286,33605,2263,5797,27807,-4,195,27613,257,794,4952,465,1373,43574,2527,6621,35953,4081,8784,28189,3486,11650,34410,234,1143,29931,-49,0,29931,56,271,29660,2479,6072,23588,563,6,50651,"FO2","GT" 16,9,1,4,2,37,85,"CONNECTICUT LGT & PWR CO","TORRINGTN T",0,"LIGHT OIL",4176,"0M",1294,,550,95,80,183,802,-19,0,802,9,49,753,4,24,729,-6,0,1062,163,373,867,4081,6864,28189,583,1059,947,4,16,931,-7,0,931,-8,0,931,173,446,1006,565,6,50651,"FO2","GT" 16,9,1,4,2,37,90,"CONNECTICUT LGT & PWR CO","BRANFORD",0,"LIGHT OIL",4176,"0M",1294,,550,95,-23,0,993,-11,0,993,-12,0,983,-9,0,993,-12,0,993,-15,0,963,303,888,1170,580,1248,981,112,115,1073,-7,12,1061,12,62,999,103,312,1042,540,6,50651,"FO2","GT" 16,9,1,2,1,45,1,"CONN YANKEE ATOMIC PWR CO","HADDAM NECK",0,"NUCLEAR",4187,"0M",1294,,551,95,349804,0,0,-2724,0,0,-2714,0,0,80321,0,0,411060,0,0,385019,0,0,346822,0,0,397229,0,0,404771,0,0,427136,0,0,421633,0,0,435253,0,0,558,6,50652,"UR","ST" 16,9,1,1,,70,1,"FARMINGTON RIVER POWER CO","RAINBOW",0,,6207,"0A",1294,,,95,4465,0,0,2602,0,0,3654,0,0,2574,0,0,1712,0,0,1108,0,0,787,0,0,842,0,0,700,0,0,2530,0,0,4222,0,0,2756,0,0,559,6,50970,"WAT","HY" 16,9,1,2,1,85,1,"NORTHEAST NUCL ENERGY CO","MILLSTONE",0,"NUCLEAR",21687,"0M",1294,,553,95,474794,0,0,424364,0,0,479164,0,0,452923,0,0,470915,0,0,397551,0,0,307242,0,0,369216,0,0,459416,0,0,478184,0,0,46176,0,0,-2630,0,0,566,6,50005,"UR","ST" 16,9,1,2,1,85,2,"NORTHEAST NUCL ENERGY CO","MILLSTONE",0,"NUCLEAR",21687,"0M",1294,,553,95,-2968,0,0,-3117,0,0,-2841,0,0,12840,0,0,0,0,0,0,0,0,-8427,0,0,340333,0,0,625348,0,0,645987,0,0,618792,0,0,511064,0,0,566,6,50005,"UR","ST" 16,9,1,2,1,85,3,"NORTHEAST NUCL ENERGY CO","MILLSTONE",0,"NUCLEAR",21687,"0M",1294,,553,95,853882,0,0,758672,0,0,851613,0,0,328284,0,0,0,0,0,594786,0,0,853005,0,0,844847,0,0,822134,0,0,852985,0,0,817800,0,0,422956,0,0,566,6,50005,"UR","ST" 16,9,1,2,2,159,3,"UNITED ILLUMINATING CO","BRDGEPT HBR",0,"LIGHT OIL",19497,"0M",1294,,,95,289,498,533,83,144,555,103,183,538,278,575,297,94,164,466,159,276,523,127,224,632,239,436,363,60,105,591,207,368,557,52,92,465,58,101,530,568,6,53003,"FO2","ST" 16,9,1,2,3,159,3,"UNITED ILLUMINATING CO","BRDGEPT HBR",0,"HEAVY OIL",19497,"0M",1294,,,95,12678,20036,157706,31465,49414,142873,1716,2749,140124,28015,51807,143380,11615,18496,124884,34707,55499,150609,43253,69685,122107,18699,30642,149294,6814,10677,163242,4908,7842,155400,4195,6665,148735,54634,86347,0,568,6,53003,"FO6","ST" 16,9,1,2,6,159,3,"UNITED ILLUMINATING CO","BRDGEPT HBR",0,"BIT COAL",19497,"0M",1294,,,95,193441,73716,182983,223214,85285,166858,221070,86802,148636,4755,2176,201542,224862,86475,170775,217578,84500,168741,225684,88542,121774,166492,67303,123827,199715,77070,157924,143992,56780,199095,198867,77375,176894,249682,95223,163986,568,6,53003,"BIT","ST" 16,9,1,4,2,159,3,"UNITED ILLUMINATING CO","BRDGEPT HBR",0,"LIGHT OIL",19497,"0M",1294,,,95,4,8,549,151,259,469,0,0,647,5,12,635,10,18,617,12,22,595,145,256,696,308,560,493,63,111,560,0,0,560,9,16,545,75,130,594,568,6,53003,"FO2","GT" 16,9,1,2,2,159,5,"UNITED ILLUMINATING CO","ENGLISH",0,"LIGHT OIL",19497,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,569,6,53003,"FO2","ST" 16,9,1,2,3,159,5,"UNITED ILLUMINATING CO","ENGLISH",0,"HEAVY OIL",19497,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,569,6,53003,"FO6","ST" 16,9,1,2,2,159,12,"UNITED ILLUMINATING CO","N HAVEN HBR",0,"LIGHT OIL",19497,"0M",1294,,,95,876,1540,484,437,731,468,424,737,445,327,564,583,511,892,406,254,441,667,361,632,570,401,702,762,359,651,646,23,502,680,959,1741,546,779,1314,482,6156,6,53003,"FO2","ST" 16,9,1,2,3,159,12,"UNITED ILLUMINATING CO","N HAVEN HBR",0,"HEAVY OIL",19497,"0M",1294,,,95,104071,166097,286634,171042,260046,151260,95848,151028,241794,147390,227183,379543,69013,110799,306351,74009,117219,286218,97251,153426,333078,88533,139665,374595,39346,64393,310202,163,3184,307018,72476,120773,186245,162959,252660,0,6156,6,53003,"FO6","ST" 16,9,1,2,9,159,12,"UNITED ILLUMINATING CO","N HAVEN HBR",0,"NAT GAS",19497,"0M",1294,,,95,0,0,0,0,0,0,31250,307224,0,64504,630374,0,76077,749979,0,81590,800742,0,99404,985733,0,49501,489902,0,13044,134068,0,34,4180,0,0,0,0,0,0,0,6156,6,53003,"NG","ST" 16,9,5,1,,556,5,"NORWICH (CITY OF)","SECOND ST",0,,13831,"0A",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,5,0,0,174,0,0,101,0,0,67,0,0,17,0,0,180,0,0,272,0,0,324,0,0,580,6,52123,"WAT","HY" 16,9,5,1,,556,10,"NORWICH (CITY OF)","OCCUM",0,,13831,"0A",1294,,,95,516,0,0,356,0,0,529,0,0,370,0,0,225,0,0,257,0,0,63,0,0,95,0,0,42,0,0,215,0,0,420,0,0,292,0,0,582,6,52123,"WAT","HY" 16,9,5,1,,556,13,"NORWICH (CITY OF)","TENTH ST",0,,13831,"0A",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,83,0,0,0,0,0,113,0,0,54,0,0,255,0,0,534,0,0,636,0,0,583,6,52123,"WAT","HY" 16,9,5,4,2,556,20,"NORWICH (CITY OF)","N MAIN ST",0,"LIGHT OIL",13831,"0A",1294,,,95,0,0,1935,53,168,1767,0,0,1767,0,0,1767,23,56,1711,62,161,1550,402,1007,1693,531,1325,1518,0,0,1518,0,0,1518,0,0,1518,117,296,2388,581,6,52123,"FO2","GT" 16,9,5,3,2,560,1,"SOUTH NORWALK (CITY OF)","SO NORWALK",0,"LIGHT OIL",17569,"0A",1294,,,95,50,90,1114,84,147,1614,27,49,1523,27,45,1455,71,123,1331,70,125,1235,242,444,819,209,351,1604,20,34,1570,2,4,1736,9,13,1671,98,158,1418,6598,6,52704,"FO2","IC" 16,9,5,2,3,567,1,"WALLINGFORD (CITY OF)","PIERCE",0,"HEAVY OIL",20038,"0A",1294,,,95,0,15,1540,368,1067,2318,0,0,2318,0,0,2318,0,0,2318,0,0,2318,0,0,2318,0,0,2318,146,445,1873,0,0,1873,0,0,1873,0,0,1873,6635,6,53175,"FO6","ST" 21,36,1,1,,35,10,"CENTRAL HUDSON GAS & ELEC","DASHVILLE",0,,3249,"0M",1294,,,95,2381,0,0,502,0,0,1130,0,0,814,0,0,844,0,0,273,0,0,156,0,0,52,0,0,6,0,0,1173,0,0,1735,0,0,901,0,0,2481,6,50484,"WAT","HY" 21,36,1,1,,35,18,"CENTRAL HUDSON GAS & ELEC","NEVERSINK",0,,3249,"0M",1294,,,95,4408,0,0,4221,0,0,4645,0,0,2716,0,0,2618,0,0,2849,0,0,10968,0,0,9289,0,0,3298,0,0,2724,0,0,2482,0,0,4970,0,0,2483,6,50484,"WAT","HY" 21,36,1,1,,35,20,"CENTRAL HUDSON GAS & ELEC","STURGEON PL",0,,3249,"0M",1294,,,95,9300,0,0,4140,0,0,8251,0,0,4665,0,0,3127,0,0,1123,0,0,872,0,0,359,0,0,111,0,0,5834,0,0,7954,0,0,3663,0,0,2486,6,50484,"WAT","HY" 21,36,1,2,3,35,25,"CENTRAL HUDSON GAS & ELEC","DANSKAMMER",0,"HEAVY OIL",3249,"0M",1294,,,95,0,0,10567,2887,4585,13091,0,0,13091,0,0,13091,377,619,12472,1176,2123,10349,198,406,9943,0,0,9943,0,0,9943,0,0,9943,16,30,9913,0,0,9913,2480,6,50484,"FO6","ST" 21,36,1,2,6,35,25,"CENTRAL HUDSON GAS & ELEC","DANSKAMMER",0,"BIT COAL",3249,"0M",1294,,,95,180547,67912,176943,208851,77841,149786,144579,54893,173619,180437,67955,164986,58267,23110,161831,149627,57630,163884,131893,51114,152154,127793,49654,170960,144488,55872,134561,60315,24424,150152,137406,60589,138420,208309,77898,129136,2480,6,50484,"BIT","ST" 21,36,1,2,9,35,25,"CENTRAL HUDSON GAS & ELEC","DANSKAMMER",0,"NAT GAS",3249,"0M",1294,,,95,12788,136338,0,5348,58875,0,52133,554622,0,1003,12881,0,26410,269381,0,9355,110458,0,50047,563362,0,64005,727957,0,42268,475832,0,72329,806049,0,21208,238996,0,526,5007,0,2480,6,50484,"NG","ST" 21,36,1,3,2,35,25,"CENTRAL HUDSON GAS & ELEC","DANSKAMMER",0,"LIGHT OIL",3249,"0M",1294,,,95,38,70,119,10,15,278,29,38,240,10,9,231,5,9,222,30,55,167,29,60,281,48,81,200,48,99,274,48,83,191,38,76,289,9,16,273,2480,6,50484,"FO2","IC" 21,36,1,4,2,35,35,"CENTRAL HUDSON GAS & ELEC","SOUTH CAIRO",0,"LIGHT OIL",3249,"0M",1294,,,95,74,178,2486,0,0,2486,0,0,2486,0,0,2486,13,31,2455,198,577,1878,16,34,1844,70,197,1647,0,0,2719,0,0,2719,39,93,2626,18,49,2577,2485,6,50484,"FO2","GT" 21,36,1,4,2,35,40,"CENTRAL HUDSON GAS & ELEC","W COXSACKIE",0,"LIGHT OIL",3249,"0M",1294,,,95,0,0,2176,0,0,2176,0,0,2176,0,0,2176,0,0,2176,0,0,2176,0,0,2176,0,0,2176,0,0,2176,0,0,2176,0,0,2176,0,0,2176,2487,6,50484,"FO2","GT" 21,36,1,4,9,35,40,"CENTRAL HUDSON GAS & ELEC","W COXSACKIE",0,"NAT GAS",3249,"0M",1294,,,95,90,1181,0,32,427,0,0,0,0,45,632,0,59,962,0,631,9351,0,109,1557,0,530,7243,0,0,0,0,52,789,0,180,2430,0,69,1043,0,2487,6,50484,"NG","GT" 21,36,1,2,2,35,45,"CENTRAL HUDSON GAS & ELEC","ROSETON JO",0,"LIGHT OIL",3249,"0M",1294,,,95,1744,3069,2289,782,1361,3014,1071,2036,2369,0,0,2542,0,0,2542,0,0,2542,0,0,2542,0,0,2542,0,0,2542,0,17,2525,654,2512,1229,581,1004,2137,8006,6,50484,"FO2","ST" 21,36,1,2,3,35,45,"CENTRAL HUDSON GAS & ELEC","ROSETON JO",0,"HEAVY OIL",3249,"0M",1294,,,95,49649,80148,781308,157108,249990,495225,13890,23984,478029,0,0,478029,0,0,478029,0,0,604069,0,0,604069,0,0,604069,0,0,604069,0,0,589640,1356,4755,599314,189513,299562,451927,8006,6,50484,"FO6","ST" 21,36,1,2,9,35,45,"CENTRAL HUDSON GAS & ELEC","ROSETON JO",0,"NAT GAS",3249,"0M",1294,,,95,33526,336575,0,69660,692555,0,24026,260204,0,0,0,0,177930,1880760,0,186946,1950511,0,310122,3310810,0,247281,2627847,0,0,0,0,0,0,0,2849,61824,0,7068,69278,0,8006,6,50484,"NG","ST" 21,36,1,1,,35,50,"CENTRAL HUDSON GAS & ELEC","HIGH FALLS",0,,3249,"0M",1294,,,95,1184,0,0,92,0,0,1122,0,0,69,0,0,143,0,0,23,0,0,26,0,0,0,0,0,0,0,0,340,0,0,1057,0,0,170,0,0,579,6,50484,"WAT","HY" 21,36,1,1,,37,5,"CENTRAL VT PUB SERV CORP","CARVERS FLS",0,,3292,"0A",1294,,350,95,921,0,0,597,0,0,1182,0,0,1121,0,0,691,0,0,250,0,0,18,0,0,58,0,0,0,0,0,391,0,0,1196,0,0,502,0,0,6456,6,50503,"WAT","HY" 21,36,1,2,3,40,1,"CONSOL EDISON CO N Y INC","ARTHUR KILL",0,"HEAVY OIL",4226,"0M",1294,,,95,0,0,5711,0,0,5711,0,0,5711,0,0,5711,0,0,5711,0,0,5711,0,0,5711,7328,11940,18519,0,0,18519,0,0,18519,0,0,18513,0,0,18513,2490,6,50653,"FO6","ST" 21,36,1,2,9,40,1,"CONSOL EDISON CO N Y INC","ARTHUR KILL",0,"NAT GAS",4226,"0M",1294,,,95,-1408,17220,0,-1393,16473,0,-1276,5546,0,42517,495291,0,55216,582417,0,194234,1938196,0,301093,2957985,0,278373,2754690,0,147636,1480827,0,-1783,3561,0,-1398,5,0,-1433,5,0,2490,6,50653,"NG","ST" 21,36,1,4,2,40,1,"CONSOL EDISON CO N Y INC","ARTHUR KILL",0,"LIGHT OIL",4226,"0M",1294,,,95,13,44,1913,67,194,1823,0,0,1823,36,79,1744,215,635,1882,298,918,2083,566,1739,2154,371,1201,1884,0,0,0,0,0,0,0,0,0,0,0,0,2490,6,50653,"FO2","GT" 21,36,1,2,1,40,2,"CONSOL EDISON CO N Y INC","INDIAN PT",0,"NUCLEAR",4226,"0M",1294,,,95,562851,0,0,52711,0,0,-6970,0,0,-3790,0,0,-13730,0,0,241777,0,0,674078,0,0,678357,0,0,681364,0,0,661697,0,0,694091,0,0,636105,0,0,2497,6,50653,"UR","ST" 21,36,1,2,3,40,3,"CONSOL EDISON CO N Y INC","ASTORIA",0,"HEAVY OIL",4226,"0M",1294,,,95,44284,69523,204071,87234,136417,162405,51168,80603,150832,37361,58624,135192,36339,59441,192317,36196,59149,130130,89762,143025,106180,87335,138221,98117,59995,93814,117887,54037,87216,125085,64568,101738,117638,289554,461968,161157,8906,6,50653,"FO6","ST" 21,36,1,2,9,40,3,"CONSOL EDISON CO N Y INC","ASTORIA",0,"NAT GAS",4226,"0M",1294,,,95,270672,2666431,0,244705,2376465,0,354262,3528212,0,241575,2383868,0,275033,2732177,0,466083,4630924,0,417404,4132582,0,422777,4216725,0,331846,3235732,0,333120,3377003,0,267480,2653281,0,78615,787377,0,8906,6,50653,"NG","ST" 21,36,1,4,2,40,3,"CONSOL EDISON CO N Y INC","ASTORIA",0,"LIGHT OIL",4226,"0M",1294,,,95,1484,3523,70541,935,2176,68112,695,1314,66869,1270,3125,63744,1033,2385,61076,1517,3666,57410,5121,12698,44790,1655,4191,48468,794,1989,67296,758,1842,65454,651,1541,63965,4785,11328,52945,8906,6,50653,"FO2","GT" 21,36,1,4,9,40,3,"CONSOL EDISON CO N Y INC","ASTORIA",0,"NAT GAS",4226,"0M",1294,,,95,1238,16825,0,4723,63317,0,9436,102713,0,19761,279920,0,13199,175023,0,14602,203072,0,50641,721027,0,30754,443611,0,22755,324431,0,10683,150198,0,29807,410036,0,1300,17862,0,8906,6,50653,"NG","GT" 21,36,1,2,3,40,5,"CONSOL EDISON CO N Y INC","EAST RIVER",0,"HEAVY OIL",4226,"0M",1294,,,95,48411,100447,260377,52328,112594,251467,22577,46041,196293,14368,29471,111609,10915,20599,75923,9443,18148,129321,17347,33410,143239,17145,35799,154704,57,119,208820,391,883,155405,24581,53489,125358,26299,56899,135819,2493,6,50653,"FO6","ST" 21,36,1,2,9,40,5,"CONSOL EDISON CO N Y INC","EAST RIVER",0,"NAT GAS",4226,"0M",1294,,,95,22936,297706,0,16423,222129,0,33740,432005,0,32894,424765,0,83114,976015,0,52018,626673,0,74759,901280,0,43540,571392,0,62070,814818,0,38780,549257,0,26334,362630,0,4079,55677,0,2493,6,50653,"NG","ST" 21,36,1,2,3,40,8,"CONSOL EDISON CO N Y INC","59TH STREET",0,"HEAVY OIL",4226,"0M",1294,,,95,134,711,28019,-168,0,13932,-186,0,17029,-180,0,14663,-186,0,16921,-180,0,14962,-186,0,34238,-186,0,28013,0,0,18655,-186,0,24175,-180,0,21506,-186,0,15408,2503,6,50653,"FO6","ST" 21,36,1,2,9,40,8,"CONSOL EDISON CO N Y INC","59TH STREET",0,"NAT GAS",4226,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,-180,0,0,0,0,0,0,0,0,0,0,0,2503,6,50653,"NG","ST" 21,36,1,4,2,40,8,"CONSOL EDISON CO N Y INC","59TH STREET",0,"LIGHT OIL",4226,"0M",1294,,,95,0,0,2421,12,43,2379,0,0,2379,34,63,2315,382,920,2169,220,532,2101,517,1422,2132,154,399,2018,0,0,2018,0,0,2018,0,0,2019,0,0,2019,2503,6,50653,"FO2","GT" 21,36,1,4,2,40,10,"CONSOL EDISON CO N Y INC","GOWANUS",0,"LIGHT OIL",4226,"0M",1294,,,95,3431,10187,54995,3032,8863,61517,3332,9885,51514,5596,16946,54888,9656,30399,58173,10867,35156,51183,35078,112111,54362,18095,69179,54055,9925,32320,51120,3062,9091,61678,11850,35551,63660,11082,31386,52408,2494,6,50653,"FO2","GT" 21,36,1,4,2,40,17,"CONSOL EDISON CO N Y INC","INDIAN PT",0,"LIGHT OIL",4226,"0M",1294,,,95,10,470,1357,110,334,1476,0,0,1438,10,26,1387,190,648,1553,120,502,1367,618,1994,1429,339,1276,1561,10,65,1518,10,49,1466,70,568,1361,10,79,1524,2497,6,50653,"FO2","GT" 21,36,1,2,3,40,18,"CONSOL EDISON CO N Y INC","HUDSON AVE",0,"HEAVY OIL",4226,"0M",1294,,,95,13942,16640,116475,22892,27677,121761,19571,25683,88715,5881,7513,112117,13579,17821,145862,8960,11221,121321,17004,23012,156902,16358,21789,184711,8488,11589,233738,9039,12876,207818,15377,22058,190563,21649,30797,210122,2496,6,50653,"FO6","ST" 21,36,1,4,2,40,18,"CONSOL EDISON CO N Y INC","HUDSON AVE",0,"LIGHT OIL",4226,"0M",1294,,,95,32,106,3790,262,520,3270,24,63,4088,0,0,4088,318,932,4131,366,1254,4363,1154,3982,3948,684,2253,4361,44,148,4212,7,28,4185,255,954,4157,0,0,4471,2496,6,50653,"FO2","GT" 21,36,1,4,2,40,23,"CONSOL EDISON CO N Y INC","NARROWS BAY",0,"LIGHT OIL",4226,"0M",1294,,,95,1815,5002,70995,2374,6488,64363,3121,8503,70742,4829,13085,57595,4696,13259,61188,7112,20641,70359,14360,43802,86922,0,0,86754,113,310,61193,358,1046,60146,2527,7040,53007,5977,17365,64411,2499,6,50653,"FO2","GT" 21,36,1,4,9,40,23,"CONSOL EDISON CO N Y INC","NARROWS BAY",0,"NAT GAS",4226,"0M",1294,,,95,160,2545,0,0,0,0,1437,23105,0,3151,50378,0,5478,91177,0,7841,132409,0,26727,472807,0,23321,410674,0,8725,137237,0,6684,112244,0,14121,266734,0,726,12168,0,2499,6,50653,"NG","GT" 21,36,1,2,3,40,25,"CONSOL EDISON CO N Y INC","RAVENSWOOD",0,"HEAVY OIL",4226,"0M",1294,,,95,56562,96769,43835,156038,248776,28947,15866,27428,34677,22910,42845,42500,30055,54093,37926,31922,55970,39660,31596,55334,44269,54612,90412,42941,11656,19796,32055,4144,7555,26939,45172,77641,44297,97823,181018,43354,2500,6,50653,"FO6","ST" 21,36,1,2,9,40,25,"CONSOL EDISON CO N Y INC","RAVENSWOOD",0,"NAT GAS",4226,"0M",1294,,,95,209768,2234824,0,193780,1928735,0,161992,1747544,0,161776,1895581,0,200509,2260799,0,241862,2659354,0,377330,4132582,0,492580,5112387,0,269868,2872681,0,121326,1378858,0,190022,2065045,0,34903,408143,0,2500,6,50653,"NG","ST" 21,36,1,4,2,40,25,"CONSOL EDISON CO N Y INC","RAVENSWOOD",0,"LIGHT OIL",4226,"0M",1294,,,95,317,1144,40469,1114,3166,37304,412,1109,36195,1364,3752,32443,0,0,32613,292,765,31848,1020,2785,39004,707,2001,37003,43,116,38759,232,819,37940,91,256,37684,3105,8078,40525,2500,6,50653,"FO2","GT" 21,36,1,4,9,40,25,"CONSOL EDISON CO N Y INC","RAVENSWOOD",0,"NAT GAS",4226,"0M",1294,,,95,699,14506,0,461,7543,0,1614,25061,0,3849,61087,0,2639,36379,0,6191,93115,0,11215,178768,0,7292,120354,0,2766,43431,0,1873,38571,0,2782,45521,0,533,8123,0,2500,6,50653,"NG","GT" 21,36,1,2,3,40,30,"CONSOL EDISON CO N Y INC","74TH STREET",0,"HEAVY OIL",4226,"0M",1294,,,95,4001,11849,37330,7337,16422,1428,4042,7539,1190,6302,7774,1190,11192,14181,1190,8567,12004,1190,7521,9483,1190,3846,5472,1365,3937,4892,1428,-949,0,1429,3253,6242,1429,3602,5677,1429,2504,6,50653,"FO6","ST" 21,36,1,4,2,40,30,"CONSOL EDISON CO N Y INC","74TH STREET",0,"LIGHT OIL",4226,"0M",1294,,,95,-13,0,1690,-11,0,2143,-12,0,2083,-12,0,1952,-3,12,1881,-12,0,1762,-12,24,1738,-13,0,1747,-12,0,1548,-12,0,1524,-12,0,1595,-12,0,2202,2504,6,50653,"FO2","GT" 21,36,1,2,3,40,40,"CONSOL EDISON CO N Y INC","WATERSIDE",0,"HEAVY OIL",4226,"0M",1294,,,95,3119,5797,0,25178,41438,0,1003,1798,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,146,266,0,2502,6,50653,"FO6","ST" 21,36,1,2,9,40,40,"CONSOL EDISON CO N Y INC","WATERSIDE",0,"NAT GAS",4226,"0M",1294,,,95,59934,697096,0,47441,490868,0,53623,603408,0,39082,449151,0,37250,448243,0,36423,288224,0,55999,633276,0,55829,627391,0,38346,480259,0,35286,396996,0,48220,540897,0,63071,723341,0,2502,6,50653,"NG","ST" 21,36,1,2,3,40,50,"CONSOL EDISON CO N Y INC","OIL STORAGE",0,"HEAVY OIL",4226,"0M",1294,,,95,0,0,2766499,0,0,2324286,0,0,2545579,0,0,2254272,0,0,1899927,0,0,1649376,0,0,1484314,0,0,1332860,0,0,1420463,0,0,1532278,0,0,1814997,0,0,1473629,8801,6,50653,"FO6","ST" 21,36,1,4,2,40,60,"CONSOL EDISON CO N Y INC","OIL STORAGE",0,"LIGHT OIL",4226,"0M",1294,,,95,0,0,204071,0,0,265070,0,0,259969,0,0,242953,0,0,247234,0,0,245330,0,0,259288,0,0,251578,0,0,241219,0,0,257945,0,0,250930,0,0,243796,8802,6,50653,"FO2","GT" 21,36,1,4,2,40,65,"CONSOL EDISON CO N Y INC","BUCHANAN",0,"LIGHT OIL",4226,"0M",1294,,,95,55,213,3746,295,599,4326,12,22,4481,20,42,4440,199,586,4211,634,1857,4497,979,2573,4452,907,2783,4475,35,172,4303,63,247,4282,398,1093,4230,56,191,4039,4233,6,50653,"FO2","GT" 21,36,1,1,,49,5,"HYDRO DEV GROUP INC","DEXTER",0,,9145,"0A",1294,,,95,2082,0,0,1260,0,0,2412,0,0,1860,0,0,1134,0,0,690,0,0,834,0,0,558,0,0,666,0,0,1998,0,0,2619,0,0,1908,0,0,2505,6,50785,"WAT","HY" 21,36,1,1,,49,10,"HYDRO DEV GROUP INC","PYRITES #1",0,,9145,"0A",1294,,,95,228,0,0,53,0,0,337,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2506,6,50785,"WAT","HY" 21,36,1,1,,49,12,"HYDRO DEV GROUP INC","PYRITES #2",0,,9145,"0A",1294,,,95,2658,0,0,1453,0,0,3335,0,0,2856,0,0,2370,0,0,1044,0,0,630,0,0,678,0,0,606,0,0,2458,0,0,3186,0,0,2166,0,0,7031,6,50785,"WAT","HY" 21,36,1,1,,49,15,"HYDRO DEV GROUP INC","HAILESBORO",0,,9145,"0A",1294,,,95,1037,0,0,706,0,0,1087,0,0,1097,0,0,854,0,0,509,0,0,415,0,0,624,0,0,389,0,0,982,0,0,1159,0,0,780,0,0,6573,6,50785,"WAT","HY" 21,36,1,1,,49,20,"HYDRO DEV GROUP INC","FOWLER",0,,9145,"0A",1294,,,95,426,0,0,394,0,0,515,0,0,491,0,0,515,0,0,316,0,0,245,0,0,349,0,0,250,0,0,398,0,0,507,0,0,434,0,0,6572,6,50785,"WAT","HY" 21,36,1,1,,49,25,"HYDRO DEV GROUP INC","#6 MILL",0,,9145,"0A",1294,,,95,471,0,0,407,0,0,463,0,0,491,0,0,394,0,0,231,0,0,201,0,0,313,0,0,208,0,0,384,0,0,494,0,0,499,0,0,453,6,50785,"WAT","HY" 21,36,1,1,,49,50,"HYDRO DEV GROUP INC","COPENHAGEN",0,,9145,"0A",1294,,,95,1176,0,0,560,0,0,1460,0,0,1532,0,0,460,0,0,108,0,0,360,0,0,112,0,0,312,0,0,1396,0,0,1884,0,0,924,0,0,742,6,50785,"WAT","HY" 21,36,1,1,,49,55,"HYDRO DEV GROUP INC","DIAMOND IS",0,,9145,"0A",1294,,,95,665,0,0,468,0,0,733,0,0,702,0,0,504,0,0,251,0,0,228,0,0,190,0,0,239,0,0,583,0,0,773,0,0,616,0,0,2553,6,50785,"WAT","HY" 21,36,1,1,,49,60,"HYDRO DEV GROUP INC","THERESA",0,,9145,"0A",1294,,,95,752,0,0,606,0,0,800,0,0,836,0,0,556,0,0,150,0,0,78,0,0,202,0,0,34,0,0,710,0,0,842,0,0,794,0,0,2618,6,50785,"WAT","HY" 21,36,1,1,,49,70,"HYDRO DEV GROUP INC","#3 MILL",0,,9145,"0A",1294,,,95,456,0,0,350,0,0,485,0,0,483,0,0,398,0,0,240,0,0,157,0,0,294,0,0,180,0,0,283,0,0,456,0,0,346,0,0,743,6,50785,"WAT","HY" 21,36,1,1,,49,75,"HYDRO DEV GROUP INC","GOODYEAR LK",0,,9145,"0A",1294,,,95,640,0,0,400,0,0,757,0,0,542,0,0,315,0,0,166,0,0,49,0,0,25,0,0,19,0,0,171,0,0,575,0,0,550,0,0,7358,6,50785,"WAT","HY" 21,36,1,3,2,59,1,"FISHERS IS ELEC CORP (THE","FISHERS ISL",0,"LIGHT OIL",6369,"0A",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,6575,6,50989,"FO2","IC" 21,36,1,4,2,87,1,"LONG ISLAND LIGHTING CO","W BABYLON",0,"LIGHT OIL",11172,"0M",1294,,,95,-9,0,10978,184,398,10580,-10,0,10580,-8,0,10580,-10,0,10580,-10,0,10580,1589,3799,6781,1012,2525,9994,-8,0,9994,23,63,9931,12,52,9878,-6,0,9878,2521,6,51685,"FO2","GT" 21,36,1,2,2,87,2,"LONG ISLAND LIGHTING CO","E F BARRETT",0,"LIGHT OIL",11172,"0M",1294,,,95,0,0,382,0,0,382,0,0,382,0,0,382,0,0,382,0,0,382,0,0,382,0,0,382,189,351,31,0,0,31,0,0,0,0,0,0,2511,6,51685,"FO2","ST" 21,36,1,2,3,87,2,"LONG ISLAND LIGHTING CO","E F BARRETT",0,"HEAVY OIL",11172,"0M",1294,,,95,7679,13204,183912,19277,32691,151221,6888,12026,167809,7622,13054,154755,21364,35883,118872,5001,8521,110351,0,0,100351,0,0,150055,0,0,176621,0,0,176621,4499,7876,168745,30931,52133,130983,2511,6,51685,"FO6","ST" 21,36,1,2,9,87,2,"LONG ISLAND LIGHTING CO","E F BARRETT",0,"NAT GAS",11172,"0M",1294,,,95,88641,923891,0,72376,743992,0,119516,1265049,0,108791,1129535,0,161464,1644681,0,176300,1817157,0,201713,2124759,0,207176,2182914,0,194067,2023621,0,176719,1855067,0,152642,1622397,0,111293,1143313,0,2511,6,51685,"NG","ST" 21,36,1,4,2,87,2,"LONG ISLAND LIGHTING CO","E F BARRETT",0,"LIGHT OIL",11172,"0M",1294,,,95,0,0,21322,0,0,21322,0,0,21322,0,0,21322,0,0,21322,0,0,21322,0,0,21322,0,0,21322,0,0,21322,0,0,21322,0,0,21322,89,272,21050,2511,6,51685,"FO2","GT" 21,36,1,4,9,87,2,"LONG ISLAND LIGHTING CO","E F BARRETT",0,"NAT GAS",11172,"0M",1294,,,95,2584,48858,0,2455,39578,0,396,9580,0,7540,115964,0,15423,241318,0,13024,203027,0,13183,202506,0,13611,214090,0,2215,41056,0,3367,60239,0,3070,49795,0,1324,23100,0,2511,6,51685,"NG","GT" 21,36,1,2,3,87,5,"LONG ISLAND LIGHTING CO","FAR ROCKWAY",0,"HEAVY OIL",11172,"0M",1294,,,95,0,0,630,0,0,630,0,0,630,0,0,630,0,0,630,0,0,630,0,0,630,0,0,630,0,0,630,0,0,630,0,0,630,0,0,630,2513,6,51685,"FO6","ST" 21,36,1,2,9,87,5,"LONG ISLAND LIGHTING CO","FAR ROCKWAY",0,"NAT GAS",11172,"0M",1294,,,95,35652,370173,0,-382,0,0,37901,413154,0,47344,499677,0,39814,418408,0,43785,454694,0,44918,522402,0,46370,490439,0,46043,485717,0,32114,356625,0,40424,437203,0,48243,507731,0,2513,6,51685,"NG","ST" 21,36,1,2,3,87,15,"LONG ISLAND LIGHTING CO","GLENWOOD",0,"HEAVY OIL",11172,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2514,6,51685,"FO6","ST" 21,36,1,2,9,87,15,"LONG ISLAND LIGHTING CO","GLENWOOD",0,"NAT GAS",11172,"0M",1294,,,95,57152,656357,0,88875,989013,0,43090,513102,0,64609,758501,0,65972,764067,0,85437,987225,0,91585,1053103,0,91614,1044546,0,87436,984844,0,70615,831640,0,65930,771090,0,72860,814525,0,2514,6,51685,"NG","ST" 21,36,1,4,2,87,15,"LONG ISLAND LIGHTING CO","GLENWOOD",0,"LIGHT OIL",11172,"0M",1294,,,95,-13,0,28987,348,833,28155,-2,113,28042,-10,0,28042,-15,0,28042,308,112,27929,1020,3353,24576,1330,3635,20941,-16,0,20941,52,122,20819,-18,0,20787,-15,0,20787,2514,6,51685,"FO2","GT" 21,36,1,3,2,87,17,"LONG ISLAND LIGHTING CO","E HAMPTON",0,"LIGHT OIL",11172,"0M",1294,,,95,-6,0,971,33,69,902,-4,4,898,-6,0,898,-1,8,890,2,12,878,464,935,369,527,862,816,51,112,705,-6,0,705,-1,4,915,0,3,911,2512,6,51685,"FO2","IC" 21,36,1,4,2,87,17,"LONG ISLAND LIGHTING CO","E HAMPTON",0,"LIGHT OIL",11172,"0M",1294,,,95,-17,0,2876,-11,17,2859,-15,0,2859,-9,0,2859,-4,25,2834,34,116,2718,2330,5851,265,2246,5851,2259,76,212,2471,-10,0,2471,27,113,2789,-12,0,2789,2512,6,51685,"FO2","GT" 21,36,1,4,2,87,18,"LONG ISLAND LIGHTING CO","SOUTHOLD",0,"LIGHT OIL",11172,"0M",1294,,,95,-8,0,2716,-15,0,2716,-15,0,2716,-11,0,2716,-9,0,2716,14,79,2637,79,316,2534,39,174,2784,-8,0,2784,-8,0,2784,33,160,2624,-15,0,2624,2520,6,51685,"FO2","GT" 21,36,1,2,2,87,21,"LONG ISLAND LIGHTING CO","NORTHPORT",0,"LIGHT OIL",11172,"0M",1294,,,95,393,703,2446,1919,3360,10568,787,1448,10918,244,438,10694,0,0,10694,1255,2346,10708,543,987,10787,859,1604,10653,1224,1286,10857,0,0,11070,42,78,10992,866,1558,10948,2516,6,51685,"FO2","ST" 21,36,1,2,3,87,21,"LONG ISLAND LIGHTING CO","NORTHPORT",0,"HEAVY OIL",11172,"0M",1294,,,95,251839,410183,917940,419721,669714,545119,137170,230153,627264,93546,156459,751601,4614,7948,743653,138528,235371,730114,232571,387065,831393,198326,339587,780654,65679,111985,948390,0,0,1048629,13006,22156,1026473,263245,435054,787488,2516,6,51685,"FO6","ST" 21,36,1,2,9,87,21,"LONG ISLAND LIGHTING CO","NORTHPORT",0,"NAT GAS",11172,"0M",1294,,,95,161173,1656185,0,109357,1099738,0,179917,1902183,0,179876,1858552,0,249772,2620522,0,277680,2980882,0,392501,4094975,0,395601,4243388,0,332956,3533654,0,339896,3613412,0,310631,3313635,0,259449,2673147,0,2516,6,51685,"NG","ST" 21,36,1,4,2,87,21,"LONG ISLAND LIGHTING CO","NORTHPORT",0,"LIGHT OIL",11172,"0M",1294,,,95,-16,0,2030,-16,0,2030,11,87,1943,-13,0,1943,-12,0,1943,-8,15,1928,10,25,1904,24,175,1729,-2,17,1712,-7,0,0,-15,0,1290,-10,0,1506,2516,6,51685,"FO2","GT" 21,36,1,3,2,87,23,"LONG ISLAND LIGHTING CO","SHOREHAM",0,"LIGHT OIL",11172,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2518,6,51685,"FO2","IC" 21,36,1,4,2,87,23,"LONG ISLAND LIGHTING CO","SHOREHAM",0,"LIGHT OIL",11172,"0M",1294,,,95,-4,0,10375,81,259,11414,11,38,11377,-7,0,11377,340,528,10848,91,128,10720,441,1417,9303,551,846,15679,5,41,15638,18,32,15605,-4,0,15605,-7,3,15602,2518,6,51685,"FO2","GT" 21,36,1,2,2,87,24,"LONG ISLAND LIGHTING CO","P JEFFERSON",0,"LIGHT OIL",11172,"0M",1294,,,95,505,940,248,368,651,173,451,865,267,430,769,71,340,624,210,273,507,271,308,573,265,205,379,265,120,230,224,260,511,310,181,337,162,173,317,229,2517,6,51685,"FO2","ST" 21,36,1,2,3,87,24,"LONG ISLAND LIGHTING CO","P JEFFERSON",0,"HEAVY OIL",11172,"0M",1294,,,95,83231,142447,374658,116002,187180,292517,84682,149701,363973,88134,146337,217636,86246,147673,240914,86540,147162,367784,119762,202643,388397,116504,197519,283029,62653,110443,267311,37059,67418,404544,57551,98596,305948,73017,122780,291514,2517,6,51685,"FO6","ST" 21,36,1,4,2,87,24,"LONG ISLAND LIGHTING CO","P JEFFERSON",0,"LIGHT OIL",11172,"0M",1294,,,95,14,70,2055,36,150,1905,-16,0,1905,-11,0,1905,30,100,1805,15,79,1726,94,282,1444,49,175,2118,-8,0,2118,2,49,2069,-12,0,2069,-14,0,2069,2517,6,51685,"FO2","GT" 21,36,1,4,2,87,26,"LONG ISLAND LIGHTING CO","SOUTHAMPTON",0,"LIGHT OIL",11172,"0M",1294,,,95,-16,0,2575,22,137,2438,-17,0,2438,-9,0,2438,-4,9,2430,36,153,2277,200,649,2266,170,698,2628,-11,0,2628,-8,0,2628,-2,0,2628,-18,0,2628,2519,6,51685,"FO2","GT" 21,36,1,3,2,87,29,"LONG ISLAND LIGHTING CO","MONTAUK",0,"LIGHT OIL",11172,"0M",1294,,,95,-6,0,685,34,66,619,-6,0,619,-6,0,619,0,0,619,2,46,572,274,574,424,184,319,529,57,109,420,-6,0,420,0,23,611,-6,0,611,2515,6,51685,"FO2","IC" 21,36,1,4,2,87,30,"LONG ISLAND LIGHTING CO","HOLTSVILLE",0,"LIGHT OIL",11172,"0M",1294,,,95,3418,7966,65483,2730,6945,98989,1349,3183,95807,3573,8991,86815,1220,3009,83806,4957,12317,71489,13538,28073,71475,15481,41712,89159,785,2396,86763,-94,234,86529,427,1487,85042,2296,5778,79264,8007,6,51685,"FO2","GT" 21,36,1,4,2,87,35,"LONG ISLAND LIGHTING CO","BROOKHAVEN",0,"LIGHT OIL",11172,"0M",1294,,,95,2290,4982,38416,2652,6010,38901,226,279,38622,3165,6704,37310,6210,13571,28376,6235,12488,40846,9816,21210,30472,9736,19194,39142,-52,0,39142,113,688,40071,528,1470,40751,2660,5996,37572,7146,6,51685,"FO2","GT" 21,36,1,1,,100,1,"N Y STATE ELEC & GAS CORP","CADYVILLE",0,,13511,"0M",1294,,,95,2289,0,0,1760,0,0,2697,0,0,2249,0,0,2033,0,0,1277,0,0,1043,0,0,1271,0,0,873,0,0,1835,0,0,2411,0,0,1256,0,0,2522,6,52036,"WAT","HY" 21,36,1,1,,100,3,"N Y STATE ELEC & GAS CORP","MILL 'C'",0,,13511,"0M",1294,,,95,1082,0,0,1120,0,0,1325,0,0,1217,0,0,1424,0,0,918,2,0,782,0,0,1153,0,0,591,0,0,1982,0,0,2696,0,0,728,0,0,6486,6,52036,"WAT","HY" 21,36,1,1,,100,8,"N Y STATE ELEC & GAS CORP","HIGH FALLS",0,,13511,"0M",1294,,,95,8036,0,0,6467,0,0,9348,0,0,7548,0,0,6945,0,0,4111,0,0,3127,0,0,4402,0,0,2270,0,0,1885,0,0,8998,0,0,6023,0,0,2530,6,52036,"WAT","HY" 21,36,1,1,,100,9,"N Y STATE ELEC & GAS CORP","KENT FALLS",0,,13511,"0M",1294,,,95,4267,0,0,3614,0,0,5729,0,0,4500,0,0,4403,0,0,2459,0,0,1821,0,0,2011,0,0,1112,0,0,2429,0,0,0,0,0,2462,0,0,2532,6,52036,"WAT","HY" 21,36,1,1,,100,11,"N Y STATE ELEC & GAS CORP","KEUKA",0,,13511,"0M",1294,,,95,479,0,0,618,0,0,1104,0,0,424,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,246,0,0,368,0,0,87,0,0,2533,6,52036,"WAT","HY" 21,36,1,1,,100,18,"N Y STATE ELEC & GAS CORP","RAINBOW FLS",0,,13511,"0M",1294,,,95,844,0,0,484,0,0,1136,0,0,1424,0,0,2008,0,0,1044,0,0,972,0,0,828,0,0,572,0,0,920,0,0,1432,0,0,800,0,0,6526,6,52036,"WAT","HY" 21,36,1,1,,100,20,"N Y STATE ELEC & GAS CORP","SENECA FLS",0,,13511,"0M",1294,,,95,929,0,0,0,0,0,237,0,0,418,0,0,57,0,0,12,0,0,35,0,0,0,0,0,0,0,0,144,0,0,1097,0,0,1515,0,0,6525,6,52036,"WAT","HY" 21,36,1,1,,100,26,"N Y STATE ELEC & GAS CORP","WATERLOO",0,,13511,"0M",1294,,,95,218,0,0,0,0,0,91,0,0,167,0,0,47,0,0,38,0,0,63,0,0,15,0,0,0,0,0,28,0,0,273,0,0,435,0,0,2538,6,52036,"WAT","HY" 21,36,1,2,2,100,28,"N Y STATE ELEC & GAS CORP","GOUDEY",0,"LIGHT OIL",13511,"0M",1294,,,95,4,6,902,7,12,922,38,860,816,166,1093,889,115,412,787,23,40,755,14,25,726,19,34,1012,88,159,674,17,29,652,15,27,781,57,99,755,2526,6,52036,"FO2","ST" 21,36,1,2,6,100,28,"N Y STATE ELEC & GAS CORP","GOUDEY",0,"BIT COAL",13511,"0M",1294,,,95,49140,18404,38386,47957,17309,33487,38535,14154,31196,29944,11570,19706,47570,19243,17396,46082,17833,16951,48114,18609,8401,48907,19270,14458,47509,18547,11816,46734,17563,21803,47743,17962,29205,49938,18814,16951,2526,6,52036,"BIT","ST" 21,36,1,2,2,100,30,"N Y STATE ELEC & GAS CORP","GREENIDGE",0,"LIGHT OIL",13511,"0M",1294,,,95,49,84,1482,143,249,1673,49,85,1663,69,118,1503,97,194,1276,101,268,963,140,255,1024,312,565,929,134,232,1184,28,65,1082,27,47,1003,135,254,963,2527,6,52036,"FO2","ST" 21,36,1,2,6,100,30,"N Y STATE ELEC & GAS CORP","GREENIDGE",0,"BIT COAL",13511,"0M",1294,,,95,59064,22369,46139,64896,24628,34337,56536,21560,33567,61588,23327,27754,60141,23147,16512,44718,17812,44179,56844,23346,35975,63282,25535,39483,33115,12718,51031,52461,19935,48906,51733,19814,48981,79778,32545,44179,2527,6,52036,"BIT","ST" 21,36,1,2,6,100,32,"N Y STATE ELEC & GAS CORP","HICKLING",0,"BIT COAL",13511,"0M",1294,,,95,29937,25353,59845,37278,28317,42388,31428,24287,26231,36848,29367,9739,25540,20965,7417,26619,21486,11619,19927,15033,13417,19292,17747,12211,16109,14260,19398,15799,13125,25995,15584,11444,38506,16518,14020,11619,2529,6,52036,"BIT","ST" 21,36,1,2,"B",100,34,"N Y STATE ELEC & GAS CORP","JENNISON",0,"WOOD CHIP",13511,"0M",1294,,,95,1937,0,0,2506,0,0,1706,0,0,446,0,0,510,0,0,631,0,0,0,0,0,966,0,0,1443,0,0,1357,0,0,215,0,0,517,0,0,2531,6,52036,"WOD","ST" 21,36,1,2,6,100,34,"N Y STATE ELEC & GAS CORP","JENNISON",0,"BIT COAL",13511,"0M",1294,,,95,18813,12027,31771,27918,18374,13300,18598,13682,9272,12405,9568,1166,10568,8258,1035,8066,6810,737,10639,7167,2889,9803,7780,5121,7664,6371,9926,7104,5362,9933,11173,7198,8195,18436,12369,737,2531,6,52036,"BIT","ST" 21,36,1,2,2,100,35,"N Y STATE ELEC & GAS CORP","MILLIKEN",0,"LIGHT OIL",13511,"0M",1294,,,95,206,337,1812,188,320,1856,273,465,1873,142,244,1879,53,94,1978,249,452,1841,116,209,1815,158,288,1863,211,385,1831,258,462,1670,59,105,1738,26,47,1841,2535,6,52036,"FO2","ST" 21,36,1,2,6,100,35,"N Y STATE ELEC & GAS CORP","MILLIKEN",0,"BIT COAL",13511,"0M",1294,,,95,192258,68792,79141,180255,67185,80127,183681,68408,89806,153861,58397,69230,98273,37927,98714,132074,52498,118633,185234,73165,90889,184163,73756,101056,131693,53020,97110,185372,73940,102961,167135,65625,99048,191784,76075,118633,2535,6,52036,"BIT","ST" 21,36,1,3,2,100,35,"N Y STATE ELEC & GAS CORP","MILLIKEN",0,"LIGHT OIL",13511,"0M",1294,,,95,0,1,0,20,38,0,3,84,0,104,107,0,54,144,0,1,38,0,-64,39,0,10,20,0,0,1,0,12,39,0,11,44,0,17,32,0,2535,6,52036,"FO2","IC" 21,36,1,3,2,100,40,"N Y STATE ELEC & GAS CORP","HARRIS LAKE",0,"LIGHT OIL",13511,"0M",1294,,,95,-11,0,405,0,0,349,0,0,0,-4,0,313,0,0,260,0,0,242,64,122,269,12,25,244,2,0,436,0,0,357,0,0,290,-13,0,242,2528,6,52036,"FO2","IC" 21,36,1,1,,100,43,"N Y STATE ELEC & GAS CORP","MECHANICVLE",0,,13511,"0M",1294,,,95,9072,0,0,6867,0,0,9702,0,0,6867,0,0,4347,0,0,2961,0,0,1134,0,0,2331,0,0,1953,0,0,5670,0,0,12663,0,0,8946,0,0,625,6,52036,"WAT","HY" 21,36,1,2,2,100,50,"N Y STATE ELEC & GAS CORP","KINTIGH",0,"LIGHT OIL",13511,"0M",1294,,,95,219,378,4169,770,1322,2904,474,811,3335,953,1656,3113,165,283,2839,314,543,2288,879,1523,3426,394,685,2738,627,1087,4124,1183,2162,2118,626,1094,4657,509,873,2288,6082,6,52036,"FO2","ST" 21,36,1,2,6,100,50,"N Y STATE ELEC & GAS CORP","KINTIGH",0,"BIT COAL",13511,"0M",1294,,,95,429496,166336,132032,393694,148405,142690,419527,160683,178911,416807,160659,178855,418612,159916,174957,381565,146069,162034,348178,133246,124345,413546,158604,73112,376458,141570,75380,181079,73253,130474,363691,142233,133771,423315,159637,162034,6082,6,52036,"BIT","ST" 21,36,1,2,1,105,1,"NIAGARA MOHAWK POWER CORP","NINE MILE P",0,"NUCLEAR",13573,"0M",1294,,190,95,368414,0,0,58742,0,0,0,0,0,332154,0,0,459193,0,0,439571,0,0,434942,0,0,437261,0,0,420930,0,0,452099,0,0,441551,0,0,459844,0,0,2589,6,52053,"UR","ST" 21,36,1,2,1,105,2,"NIAGARA MOHAWK POWER CORP","NINE MILE P",0,"NUCLEAR",13573,"0M",1294,,190,95,694823,0,0,533574,0,0,742888,0,0,149501,0,0,0,0,0,575400,0,0,821880,0,0,766368,0,0,443850,0,0,845303,0,0,824493,0,0,841323,0,0,2589,6,52053,"UR","ST" 21,36,1,1,,105,5,"NIAGARA MOHAWK POWER CORP","ALLENS FLS",0,,13573,"0M",1294,,190,95,2087,0,0,1758,0,0,2479,0,0,2662,0,0,2344,0,0,1289,0,0,1268,0,0,1240,0,0,1099,0,0,2308,0,0,2305,0,0,2092,0,0,2540,6,52053,"WAT","HY" 21,36,1,1,,105,10,"NIAGARA MOHAWK POWER CORP","BALDWINSVLE",0,,13573,"0M",1294,,190,95,205,0,0,112,0,0,221,0,0,171,0,0,60,0,0,7,0,0,-3,0,0,16,0,0,1,0,0,57,0,0,217,0,0,140,0,0,2542,6,52053,"WAT","HY" 21,36,1,1,,105,15,"NIAGARA MOHAWK POWER CORP","BELFORT",0,,13573,"0M",1294,,190,95,861,0,0,751,0,0,805,0,0,464,0,0,550,0,0,561,0,0,714,0,0,764,0,0,730,0,0,557,0,0,1171,0,0,1354,0,0,2544,6,52053,"WAT","HY" 21,36,1,1,,105,20,"NIAGARA MOHAWK POWER CORP","BENNETTS B",0,,13573,"0M",1294,,190,95,10231,0,0,5759,0,0,9838,0,0,5346,0,0,4404,0,0,1938,0,0,-33,0,0,313,0,0,5443,0,0,9001,0,0,13335,0,0,6313,0,0,2545,6,52053,"WAT","HY" 21,36,1,1,,105,25,"NIAGARA MOHAWK POWER CORP","BLACK RIVER",0,,13573,"0M",1294,,190,95,3477,0,0,2422,0,0,3823,0,0,3907,0,0,2562,0,0,1270,0,0,1501,0,0,948,0,0,1559,0,0,3563,0,0,4456,0,0,3477,0,0,2546,6,52053,"WAT","HY" 21,36,1,1,,105,30,"NIAGARA MOHAWK POWER CORP","BLAKE",0,,13573,"0M",1294,,190,95,6604,0,0,6486,0,0,5072,0,0,2962,0,0,3721,0,0,3715,0,0,672,0,0,2828,0,0,1682,0,0,3534,0,0,9144,0,0,6300,0,0,2547,6,52053,"WAT","HY" 21,36,1,1,,105,35,"NIAGARA MOHAWK POWER CORP","BROWNS FLS",0,,13573,"0M",1294,,190,95,6785,0,0,3738,0,0,4510,0,0,1724,0,0,1746,0,0,1866,0,0,545,0,0,2901,0,0,1160,0,0,4896,0,0,7492,0,0,3767,0,0,2548,6,52053,"WAT","HY" 21,36,1,1,,105,40,"NIAGARA MOHAWK POWER CORP","CHASM",0,,13573,"0M",1294,,190,95,1902,0,0,1138,0,0,1426,0,0,1777,0,0,1751,0,0,1323,0,0,994,0,0,1236,0,0,1014,0,0,1752,0,0,1795,0,0,1489,0,0,2550,6,52053,"WAT","HY" 21,36,1,1,,105,45,"NIAGARA MOHAWK POWER CORP","COLTON",0,,13573,"0M",1294,,190,95,20600,0,0,18761,0,0,20043,0,0,13701,0,0,15937,0,0,15548,0,0,9456,0,0,14510,0,0,7469,0,0,15049,0,0,2073,0,0,19935,0,0,2551,6,52053,"WAT","HY" 21,36,1,1,,105,50,"NIAGARA MOHAWK POWER CORP","DEFERIET",0,,13573,"0M",1294,,190,95,4478,0,0,3495,0,0,5869,0,0,5234,0,0,3642,0,0,1740,0,0,1638,0,0,1204,0,0,1248,0,0,5355,0,0,7027,0,0,4656,0,0,2552,6,52053,"WAT","HY" 21,36,1,1,,105,65,"NIAGARA MOHAWK POWER CORP","EAGLE",0,,13573,"0M",1294,,190,95,2653,0,0,2021,0,0,2505,0,0,1200,0,0,1421,0,0,1737,0,0,2331,0,0,1979,0,0,2045,0,0,1398,0,0,3203,0,0,3777,0,0,2555,6,52053,"WAT","HY" 21,36,1,1,,105,70,"NIAGARA MOHAWK POWER CORP","EEL WEIR",0,,13573,"0M",1294,,190,95,866,0,0,622,0,0,964,0,0,803,0,0,524,0,0,203,0,0,115,0,0,125,0,0,7,0,0,655,0,0,1332,0,0,994,0,0,2556,6,52053,"WAT","HY" 21,36,1,1,,105,75,"NIAGARA MOHAWK POWER CORP","EFFLEY",0,,13573,"0M",1294,,190,95,1093,0,0,986,0,0,1153,0,0,580,0,0,694,0,0,845,0,0,905,0,0,982,0,0,900,0,0,740,0,0,1558,0,0,1767,0,0,2557,6,52053,"WAT","HY" 21,36,1,1,,105,80,"NIAGARA MOHAWK POWER CORP","ELMER",0,,13573,"0M",1294,,190,95,812,0,0,575,0,0,796,0,0,380,0,0,439,0,0,552,0,0,441,0,0,640,0,0,593,0,0,496,0,0,1010,0,0,1135,0,0,2559,6,52053,"WAT","HY" 21,36,1,1,,105,85,"NIAGARA MOHAWK POWER CORP","ET NORFOLK",0,,13573,"0M",1294,,190,95,2479,0,0,1995,0,0,2559,0,0,1703,0,0,1975,0,0,1859,0,0,1059,0,0,1731,0,0,851,0,0,1883,0,0,2471,0,0,2519,0,0,2561,6,52053,"WAT","HY" 21,36,1,1,,105,90,"NIAGARA MOHAWK POWER CORP","FIVE FALLS",0,,13573,"0M",1294,,190,95,10795,0,0,10405,0,0,8347,0,0,4782,0,0,5926,0,0,5896,0,0,3396,0,0,5619,0,0,2631,0,0,5807,0,0,14654,0,0,10198,0,0,2562,6,52053,"WAT","HY" 21,36,1,1,,105,95,"NIAGARA MOHAWK POWER CORP","FLAT ROCK",0,,13573,"0M",1294,,190,95,1503,0,0,871,0,0,1489,0,0,592,0,0,450,0,0,401,0,0,136,0,0,528,0,0,169,0,0,1414,0,0,1912,0,0,876,0,0,2563,6,52053,"WAT","HY" 21,36,1,1,,105,98,"NIAGARA MOHAWK POWER CORP","FRANKLIN F",0,,13573,"0M",1294,,190,95,775,0,0,767,0,0,1052,0,0,613,0,0,385,0,0,496,0,0,336,0,0,352,0,0,-1,0,0,-1,0,0,-1,0,0,-1,0,0,2564,6,52053,"WAT","HY" 21,36,1,1,,105,100,"NIAGARA MOHAWK POWER CORP","FULTON",0,,13573,"0M",1294,,190,95,464,0,0,333,0,0,608,0,0,437,0,0,459,0,0,300,0,0,406,0,0,363,0,0,304,0,0,474,0,0,653,0,0,625,0,0,2566,6,52053,"WAT","HY" 21,36,1,1,,105,105,"NIAGARA MOHAWK POWER CORP","GRANBY",0,,13573,"0M",1294,,190,95,5845,0,0,3502,0,0,6558,0,0,1324,0,0,640,0,0,477,0,0,-38,0,0,491,0,0,-42,0,0,3025,0,0,5404,0,0,5157,0,0,2569,6,52053,"WAT","HY" 21,36,1,1,,105,110,"NIAGARA MOHAWK POWER CORP","HANNAWA",0,,13573,"0M",1294,,190,95,5253,0,0,4772,0,0,5248,0,0,3332,0,0,4051,0,0,3941,0,0,2329,0,0,3797,0,0,1747,0,0,1086,0,0,2696,0,0,5321,0,0,2571,6,52053,"WAT","HY" 21,36,1,1,,105,115,"NIAGARA MOHAWK POWER CORP","HERRINGS",0,,13573,"0M",1294,,190,95,1980,0,0,1586,0,0,2151,0,0,2116,0,0,1509,0,0,629,0,0,705,0,0,371,0,0,337,0,0,1747,0,0,2341,0,0,2187,0,0,2572,6,52053,"WAT","HY" 21,36,1,1,,105,120,"NIAGARA MOHAWK POWER CORP","HEUVELTON",0,,13573,"0M",1294,,190,95,458,0,0,468,0,0,484,0,0,556,0,0,455,0,0,254,0,0,195,0,0,277,0,0,149,0,0,433,0,0,506,0,0,588,0,0,2573,6,52053,"WAT","HY" 21,36,1,1,,105,125,"NIAGARA MOHAWK POWER CORP","HIGH DAM 6",0,,13573,"0M",1294,,190,95,0,0,0,0,0,0,1863,0,0,2023,0,0,1494,0,0,922,0,0,725,0,0,989,0,0,179,0,0,2024,0,0,2607,0,0,3766,0,0,2574,6,52053,"WAT","HY" 21,36,1,1,,105,126,"NIAGARA MOHAWK POWER CORP","HIGH FALLS",0,,13573,"0M",1294,,190,95,2622,0,0,1900,0,0,2648,0,0,1268,0,0,1439,0,0,1814,0,0,2106,0,0,1998,0,0,1847,0,0,1571,0,0,3045,0,0,3527,0,0,2575,6,52053,"WAT","HY" 21,36,1,1,,105,130,"NIAGARA MOHAWK POWER CORP","HIGLEY",0,,13573,"0M",1294,,190,95,3414,0,0,2999,0,0,3075,0,0,1774,0,0,2177,0,0,2037,0,0,1416,0,0,2086,0,0,1120,0,0,2315,0,0,3556,0,0,3242,0,0,2576,6,52053,"WAT","HY" 21,36,1,1,,105,135,"NIAGARA MOHAWK POWER CORP","HOGANSBURG",0,,13573,"0M",1294,,190,95,98,0,0,143,0,0,192,0,0,192,0,0,148,0,0,129,0,0,87,0,0,146,0,0,79,0,0,113,0,0,186,0,0,218,0,0,2577,6,52053,"WAT","HY" 21,36,1,1,,105,140,"NIAGARA MOHAWK POWER CORP","KAMARGO",0,,13573,"0M",1294,,190,95,2374,0,0,1857,0,0,2750,0,0,2638,0,0,1924,0,0,960,0,0,1034,0,0,398,0,0,612,0,0,2497,0,0,3433,0,0,1788,0,0,2581,6,52053,"WAT","HY" 21,36,1,1,,105,145,"NIAGARA MOHAWK POWER CORP","LIGHTHOUSE",0,,13573,"0M",1294,,190,95,2431,0,0,1342,0,0,2514,0,0,1178,0,0,925,0,0,399,0,0,-14,0,0,-14,0,0,1080,0,0,1999,0,0,3282,0,0,1507,0,0,2582,6,52053,"WAT","HY" 21,36,1,1,,105,155,"NIAGARA MOHAWK POWER CORP","MACOMB",0,,13573,"0M",1294,,190,95,434,0,0,398,0,0,641,0,0,569,0,0,481,0,0,319,0,0,-4,0,0,-4,0,0,132,0,0,534,0,0,627,0,0,520,0,0,2583,6,52053,"WAT","HY" 21,36,1,1,,105,160,"NIAGARA MOHAWK POWER CORP","MINETTO",0,,13573,"0M",1294,,190,95,3847,0,0,2604,0,0,4467,0,0,2022,0,0,1607,0,0,940,0,0,602,0,0,800,0,0,427,0,0,1690,0,0,4151,0,0,4554,0,0,2586,6,52053,"WAT","HY" 21,36,1,1,,105,165,"NIAGARA MOHAWK POWER CORP","MOSHIER",0,,13573,"0M",1294,,190,95,2698,0,0,2561,0,0,2447,0,0,1064,0,0,1751,0,0,2554,0,0,2993,0,0,2896,0,0,2791,0,0,736,0,0,3994,0,0,5506,0,0,2588,6,52053,"WAT","HY" 21,36,1,1,,105,170,"NIAGARA MOHAWK POWER CORP","NORFOLK",0,,13573,"0M",1294,,190,95,2391,0,0,2156,0,0,2979,0,0,1872,0,0,2207,0,0,2139,0,0,1223,0,0,2018,0,0,958,0,0,2054,0,0,3088,0,0,2630,0,0,2590,6,52053,"WAT","HY" 21,36,1,1,,105,175,"NIAGARA MOHAWK POWER CORP","NORWOOD",0,,13573,"0M",1294,,190,95,1536,0,0,1408,0,0,1536,0,0,938,0,0,1146,0,0,1136,0,0,605,0,0,1104,0,0,480,0,0,1072,0,0,1232,0,0,1488,0,0,2591,6,52053,"WAT","HY" 21,36,1,1,,105,180,"NIAGARA MOHAWK POWER CORP","OSWEGATCHIE",0,,13573,"0M",1294,,190,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2593,6,52053,"WAT","HY" 21,36,1,1,,105,182,"NIAGARA MOHAWK POWER CORP","OSWEGO FL E",0,,13573,"0M",1294,,190,95,2890,0,0,2449,0,0,2510,0,0,1688,0,0,1604,0,0,996,0,0,637,0,0,679,0,0,550,0,0,1991,0,0,2836,0,0,2816,0,0,2595,6,52053,"WAT","HY" 21,36,1,1,,105,183,"NIAGARA MOHAWK POWER CORP","OSWEGO FL W",0,,13573,"0M",1294,,190,95,1223,0,0,423,0,0,1212,0,0,176,0,0,-1,0,0,28,0,0,-2,0,0,47,0,0,14,0,0,385,0,0,730,0,0,1172,0,0,2596,6,52053,"WAT","HY" 21,36,1,1,,105,185,"NIAGARA MOHAWK POWER CORP","PARISHVILLE",0,,13573,"0M",1294,,190,95,0,0,0,690,0,0,1562,0,0,1603,0,0,1516,0,0,848,0,0,849,0,0,763,0,0,749,0,0,1395,0,0,1488,0,0,1298,0,0,2597,6,52053,"WAT","HY" 21,36,1,1,,105,187,"NIAGARA MOHAWK POWER CORP","PIERCEFIELD",0,,13573,"0M",1294,,190,95,1488,0,0,1283,0,0,1529,0,0,1482,0,0,1341,0,0,627,0,0,429,0,0,881,0,0,370,0,0,1195,0,0,1783,0,0,1527,0,0,2598,6,52053,"WAT","HY" 21,36,1,1,,105,192,"NIAGARA MOHAWK POWER CORP","PROSPECT",0,,13573,"0M",1294,,190,95,1704,0,0,0,0,0,4257,0,0,5788,0,0,3672,0,0,2881,0,0,2386,0,0,1689,0,0,184,0,0,6691,0,0,11309,0,0,6904,0,0,2599,6,52053,"WAT","HY" 21,36,1,1,,105,195,"NIAGARA MOHAWK POWER CORP","RAINBOW",0,,13573,"0M",1294,,190,95,10771,0,0,10270,0,0,8298,0,0,4779,0,0,5959,0,0,5843,0,0,3452,0,0,5583,0,0,2641,0,0,5774,0,0,14120,0,0,9950,0,0,2600,6,52053,"WAT","HY" 21,36,1,1,,105,200,"NIAGARA MOHAWK POWER CORP","RAYMONDVLE",0,,13573,"0M",1294,,190,95,932,0,0,816,0,0,1452,0,0,926,0,0,670,0,0,1102,0,0,674,0,0,1036,0,0,530,0,0,1056,0,0,1404,0,0,1120,0,0,2601,6,52053,"WAT","HY" 21,36,1,1,,105,210,"NIAGARA MOHAWK POWER CORP","S EDWARDS",0,,13573,"0M",1294,,190,95,1404,0,0,1076,0,0,1387,0,0,973,0,0,1018,0,0,736,0,0,427,0,0,1020,0,0,558,0,0,1359,0,0,1919,0,0,1392,0,0,2604,6,52053,"WAT","HY" 21,36,1,1,,105,215,"NIAGARA MOHAWK POWER CORP","SEWALLS",0,,13573,"0M",1294,,190,95,1372,0,0,889,0,0,1518,0,0,1486,0,0,1205,0,0,544,0,0,246,0,0,320,0,0,319,0,0,1211,0,0,1489,0,0,1514,0,0,2608,6,52053,"WAT","HY" 21,36,1,1,,105,220,"NIAGARA MOHAWK POWER CORP","SOFT MAPLE",0,,13573,"0M",1294,,190,95,2633,0,0,1616,0,0,2359,0,0,882,0,0,1236,0,0,1714,0,0,2341,0,0,1918,0,0,1850,0,0,1760,0,0,3432,0,0,4125,0,0,2610,6,52053,"WAT","HY" 21,36,1,1,,105,225,"NIAGARA MOHAWK POWER CORP","SOTH COLTON",0,,13573,"0M",1294,,190,95,8860,0,0,8292,0,0,6906,0,0,3510,0,0,4607,0,0,4842,0,0,2861,0,0,4595,0,0,2211,0,0,4731,0,0,12247,0,0,8305,0,0,2611,6,52053,"WAT","HY" 21,36,1,1,,105,230,"NIAGARA MOHAWK POWER CORP","STARK",0,,13573,"0M",1294,,190,95,10035,0,0,10162,0,0,7531,0,0,4401,0,0,5629,0,0,5788,0,0,3281,0,0,5363,0,0,2475,0,0,5187,0,0,14852,0,0,9960,0,0,2613,6,52053,"WAT","HY" 21,36,1,1,,105,235,"NIAGARA MOHAWK POWER CORP","SUGAR IS",0,,13573,"0M",1294,,190,95,2908,0,0,2519,0,0,2995,0,0,2818,0,0,2884,0,0,2757,0,0,1893,0,0,2754,0,0,1376,0,0,2667,0,0,2781,0,0,2983,0,0,2616,6,52053,"WAT","HY" 21,36,1,1,,105,240,"NIAGARA MOHAWK POWER CORP","TAYLORVILLE",0,,13573,"0M",1294,,190,95,2219,0,0,1663,0,0,2176,0,0,1051,0,0,1247,0,0,1560,0,0,1566,0,0,1692,0,0,1630,0,0,1392,0,0,2700,0,0,3109,0,0,2617,6,52053,"WAT","HY" 21,36,1,1,,105,250,"NIAGARA MOHAWK POWER CORP","TRENTON",0,,13573,"0M",1294,,190,95,12363,0,0,10763,0,0,12685,0,0,10309,0,0,6711,0,0,6004,0,0,5262,0,0,4565,0,0,3995,0,0,8295,0,0,14603,0,0,11617,0,0,2619,6,52053,"WAT","HY" 21,36,1,1,,105,255,"NIAGARA MOHAWK POWER CORP","VARICK",0,,13573,"0M",1294,,190,95,3510,0,0,2348,0,0,3552,0,0,1467,0,0,836,0,0,546,0,0,363,0,0,629,0,0,211,0,0,2344,0,0,3490,0,0,3553,0,0,2621,6,52053,"WAT","HY" 21,36,1,1,,105,265,"NIAGARA MOHAWK POWER CORP","YALEVILLE",0,,13573,"0M",1294,,190,95,293,0,0,255,0,0,406,0,0,320,0,0,373,0,0,341,0,0,243,0,0,407,0,0,242,0,0,346,0,0,275,0,0,248,0,0,2624,6,52053,"WAT","HY" 21,36,1,3,2,105,270,"NIAGARA MOHAWK POWER CORP","NINE MILE P",0,"LIGHT OIL",13573,"0M",1294,,190,95,6,136,4435,3,121,4470,11,87,4380,0,100,4256,13,323,4316,10,36,4349,6,164,4288,7,218,4320,6,11,535,6,12,573,6,13,557,6,12,543,2589,6,52053,"FO2","IC" 21,36,1,2,3,105,275,"NIAGARA MOHAWK POWER CORP","OSWEGO",0,"HEAVY OIL",13573,"0M",1294,,190,95,0,0,632933,120407,215553,417380,0,0,417380,26504,46741,370639,0,0,370639,1371,4130,366508,44092,30232,330715,13690,33269,298197,9883,21973,276183,0,0,276183,0,0,542213,0,0,542213,2594,6,52053,"FO6","ST" 21,36,1,2,9,105,275,"NIAGARA MOHAWK POWER CORP","OSWEGO",0,"NAT GAS",13573,"0M",1294,,190,95,999,22854,0,10635,117884,0,0,0,0,0,0,0,0,0,0,0,0,0,108,461,0,38513,570000,0,15497,213000,0,0,0,0,0,0,0,0,0,0,2594,6,52053,"NG","ST" 21,36,1,3,2,105,275,"NIAGARA MOHAWK POWER CORP","OSWEGO",0,"LIGHT OIL",13573,"0M",1294,,190,95,0,0,2149,0,0,2149,0,0,2149,0,0,2149,0,0,2149,0,0,2149,0,0,2149,0,0,2149,4,11,2138,0,0,2138,0,0,2138,0,0,2138,2594,6,52053,"FO2","IC" 21,36,1,1,,105,285,"NIAGARA MOHAWK POWER CORP","BEARDSLEE F",0,,13573,"0M",1294,,190,95,5266,0,0,1946,0,0,6556,0,0,4417,0,0,2463,0,0,1946,0,0,895,0,0,759,0,0,741,0,0,5400,0,0,6369,0,0,2631,0,0,2543,6,52053,"WAT","HY" 21,36,1,1,,105,290,"NIAGARA MOHAWK POWER CORP","BAKER FALLS",0,,13573,"0M",1294,"R",190,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2541,6,52053,"WAT","HY" 21,36,1,1,,105,300,"NIAGARA MOHAWK POWER CORP","EL J WEST",0,,13573,"0M",1294,,190,95,5989,0,0,5250,0,0,1580,0,0,972,0,0,1241,0,0,3218,0,0,3059,0,0,2326,0,0,4257,0,0,1425,0,0,10684,0,0,8834,0,0,6527,6,52053,"WAT","HY" 21,36,1,1,,105,305,"NIAGARA MOHAWK POWER CORP","EPHRATAH",0,,13573,"0M",1294,,190,95,2045,0,0,902,0,0,1493,0,0,780,0,0,337,0,0,463,0,0,97,0,0,147,0,0,127,0,0,1599,0,0,1298,0,0,1198,0,0,2560,6,52053,"WAT","HY" 21,36,1,1,,105,315,"NIAGARA MOHAWK POWER CORP","GLEN FALLS",0,,13573,"0M",1294,,190,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2567,6,52053,"WAT","HY" 21,36,1,1,,105,317,"NIAGARA MOHAWK POWER CORP","GREEN ISL",0,,13573,"0M",1294,,190,95,3672,0,0,3067,0,0,3470,0,0,3478,0,0,2678,0,0,2110,0,0,1303,0,0,1440,0,0,1476,0,0,2837,0,0,2513,0,0,3722,0,0,6528,6,52053,"WAT","HY" 21,36,1,1,,105,320,"NIAGARA MOHAWK POWER CORP","INGHAMS",0,,13573,"0M",1294,,190,95,2951,0,0,1446,0,0,3570,0,0,3006,0,0,1806,0,0,1403,0,0,605,0,0,518,0,0,480,0,0,2716,0,0,3695,0,0,1829,0,0,2579,6,52053,"WAT","HY" 21,36,1,1,,105,325,"NIAGARA MOHAWK POWER CORP","JOHNSONVLE",0,,13573,"0M",1294,,190,95,783,0,0,709,0,0,698,0,0,730,0,0,706,0,0,415,0,0,84,0,0,196,0,0,71,0,0,754,0,0,1347,0,0,777,0,0,2580,6,52053,"WAT","HY" 21,36,1,1,,105,340,"NIAGARA MOHAWK POWER CORP","MOREAU",0,,13573,"0M",1294,"R",190,95,0,0,0,2501,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2587,6,52053,"WAT","HY" 21,36,1,1,,105,350,"NIAGARA MOHAWK POWER CORP","SCH ST COHS",0,,13573,"0M",1294,,190,95,17365,0,0,13801,0,0,18549,0,0,16246,0,0,8330,0,0,6836,0,0,4087,0,0,3410,0,0,3303,0,0,14028,0,0,23804,0,0,15352,0,0,2605,6,52053,"WAT","HY" 21,36,1,1,,105,355,"NIAGARA MOHAWK POWER CORP","SCHAGHTICKE",0,,13573,"0M",1294,,190,95,6959,0,0,4628,0,0,1779,0,0,7008,0,0,3998,0,0,2703,0,0,925,0,0,1694,0,0,513,0,0,4157,0,0,7065,0,0,4122,0,0,2606,6,52053,"WAT","HY" 21,36,1,1,,105,360,"NIAGARA MOHAWK POWER CORP","SCHUYLERVLE",0,,13573,"0M",1294,,190,95,766,0,0,454,0,0,951,0,0,408,0,0,291,0,0,185,0,0,26,0,0,77,0,0,-5,0,0,527,0,0,1089,0,0,771,0,0,2607,6,52053,"WAT","HY" 21,36,1,1,,105,365,"NIAGARA MOHAWK POWER CORP","SHERMAN",0,,13573,"0M",1294,,190,95,14937,0,0,11480,0,0,11483,0,0,9158,0,0,6495,0,0,5892,0,0,5453,0,0,6179,0,0,6999,0,0,9121,0,0,7996,0,0,9198,0,0,2609,6,52053,"WAT","HY" 21,36,1,1,,105,370,"NIAGARA MOHAWK POWER CORP","SPIER FALLS",0,,13573,"0M",1294,,190,95,22054,0,0,16130,0,0,18521,0,0,13202,0,0,8844,0,0,7373,0,0,6467,0,0,7246,0,0,8844,0,0,15741,0,0,12177,0,0,20353,0,0,2612,6,52053,"WAT","HY" 21,36,1,1,,105,380,"NIAGARA MOHAWK POWER CORP","STEWARTS BR",0,,13573,"0M",1294,,190,95,10770,0,0,11203,0,0,3959,0,0,1818,0,0,5172,0,0,2348,0,0,5366,0,0,4271,0,0,7737,0,0,2666,0,0,19084,0,0,17328,0,0,2614,6,52053,"WAT","HY" 21,36,1,1,,105,385,"NIAGARA MOHAWK POWER CORP","STUYVESANT",0,,13573,"0M",1294,,190,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2615,6,52053,"WAT","HY" 21,36,1,2,2,105,395,"NIAGARA MOHAWK POWER CORP","ALBANY",0,"LIGHT OIL",13573,"0M",1294,,190,95,0,0,220,0,0,220,0,0,220,0,0,220,0,0,220,0,0,220,0,0,201,0,0,201,0,0,195,0,0,192,0,0,189,0,0,185,2539,6,52053,"FO2","ST" 21,36,1,2,3,105,395,"NIAGARA MOHAWK POWER CORP","ALBANY",0,"HEAVY OIL",13573,"0M",1294,,190,95,58267,97691,332532,62750,94595,237938,5641,8097,184840,0,0,184840,0,0,184840,1711,4230,180610,0,0,180610,0,0,180610,0,0,180610,0,0,180610,18591,30657,149952,25930,42050,107902,2539,6,52053,"FO6","ST" 21,36,1,2,9,105,395,"NIAGARA MOHAWK POWER CORP","ALBANY",0,"NAT GAS",13573,"0M",1294,,190,95,57789,665226,0,58253,669709,0,144263,1550322,0,53054,571524,0,31237,333909,0,47841,524896,0,130139,1434248,0,147338,1604315,0,50979,541649,0,49257,521886,0,6001,121469,0,5994,104410,0,2539,6,52053,"NG","ST" 21,36,1,3,2,105,395,"NIAGARA MOHAWK POWER CORP","ALBANY",0,"LIGHT OIL",13573,"0M",1294,,190,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2539,6,52053,"FO2","IC" 21,36,1,4,2,105,395,"NIAGARA MOHAWK POWER CORP","ALBANY",0,"LIGHT OIL",13573,"0M",1294,,190,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2539,6,52053,"FO2","GT" 21,36,1,4,9,105,395,"NIAGARA MOHAWK POWER CORP","ALBANY",0,"NAT GAS",13573,"0M",1294,,190,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2539,6,52053,"NG","GT" 21,36,1,1,,105,420,"NIAGARA MOHAWK POWER CORP","GLENWOOD",0,,13573,"0M",1294,,190,95,584,0,0,584,0,0,712,0,0,35,0,0,602,0,0,501,0,0,510,0,0,499,0,0,459,0,0,493,0,0,412,0,0,213,0,0,2568,6,52053,"WAT","HY" 21,36,1,1,,105,425,"NIAGARA MOHAWK POWER CORP","HYDRAULIC R",0,,13573,"0M",1294,,190,95,0,0,0,0,0,0,0,0,0,247,0,0,1980,0,0,1737,0,0,1757,0,0,1761,0,0,1655,0,0,1715,0,0,209,0,0,0,0,0,2578,6,52053,"WAT","HY" 21,36,1,1,,105,440,"NIAGARA MOHAWK POWER CORP","WATERPORT",0,,13573,"0M",1294,,190,95,1372,0,0,1372,0,0,1447,0,0,69,0,0,924,0,0,779,0,0,723,0,0,727,0,0,684,0,0,922,0,0,936,0,0,428,0,0,2623,6,52053,"WAT","HY" 21,36,1,2,2,105,445,"NIAGARA MOHAWK POWER CORP","DUNKIRK",0,"LIGHT OIL",13573,"0M",1294,,190,95,1601,2790,0,653,1081,0,675,1178,0,599,1017,0,1403,2417,0,539,896,0,638,1090,0,1031,1725,0,723,1216,0,997,1731,0,914,1625,0,396,651,0,2554,6,52053,"FO2","ST" 21,36,1,2,6,105,445,"NIAGARA MOHAWK POWER CORP","DUNKIRK",0,"BIT COAL",13573,"0M",1294,,190,95,254022,99455,112963,311173,114689,97723,298538,114582,80138,317020,119632,52831,259603,99967,52456,255038,95545,74556,311521,120965,80149,307244,117398,77577,307482,116339,76599,257442,99939,138351,253614,100750,153571,354614,131876,151153,2554,6,52053,"BIT","ST" 21,36,1,3,2,105,445,"NIAGARA MOHAWK POWER CORP","DUNKIRK",0,"LIGHT OIL",13573,"0M",1294,,190,95,0,0,1079,0,0,1334,0,0,1300,0,0,1323,0,0,635,0,0,1174,0,0,1343,0,0,1234,0,0,1317,0,0,1090,0,0,1325,0,0,1484,2554,6,52053,"FO2","IC" 21,36,1,2,2,105,450,"NIAGARA MOHAWK POWER CORP","C R HUNTLEY",0,"LIGHT OIL",13573,"0M",1294,,190,95,681,1256,1160,349,688,1247,690,1294,1076,1705,3207,1221,704,1326,1175,1004,1818,1727,1072,1981,1452,554,1037,1301,324,570,1193,1215,2237,1180,832,1567,1213,253,461,1135,2549,6,52053,"FO2","ST" 21,36,1,2,6,105,450,"NIAGARA MOHAWK POWER CORP","C R HUNTLEY",0,"BIT COAL",13573,"0M",1294,,190,95,272246,110975,103175,276497,121255,106086,220640,91915,179212,270614,112094,162277,265384,109603,157439,267756,107734,190733,286378,118727,131748,337035,139658,120591,316597,122391,136393,245260,100618,129570,236599,99435,197282,339259,137453,168549,2549,6,52053,"BIT","ST" 21,36,1,3,2,105,450,"NIAGARA MOHAWK POWER CORP","C R HUNTLEY",0,"LIGHT OIL",13573,"0M",1294,,190,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2549,6,52053,"FO2","IC" 21,36,1,1,,105,460,"NIAGARA MOHAWK POWER CORP","OAK ORCHARD",0,,13573,"0M",1294,,190,95,0,0,0,0,0,0,0,0,0,0,0,0,178,0,0,186,0,0,185,0,0,187,0,0,174,0,0,176,0,0,46,0,0,0,0,0,2592,6,52053,"WAT","HY" 21,36,1,1,,105,465,"NIAGARA MOHAWK POWER CORP","BEEBEE IS",0,,13573,"0M",1294,,190,95,3633,0,0,2768,0,0,5208,0,0,4383,0,0,3010,0,0,1959,0,0,2292,0,0,1754,0,0,2115,0,0,4754,0,0,5881,0,0,3959,0,0,6434,6,52053,"WAT","HY" 21,36,1,1,,105,470,"NIAGARA MOHAWK POWER CORP","FEEDER DAM",0,,13573,"0M",1294,,190,95,3058,0,0,0,0,0,2491,0,0,1680,0,0,1085,0,0,869,0,0,595,0,0,648,0,0,1046,0,0,1795,0,0,3058,0,0,2885,0,0,2666,6,52053,"WAT","HY" 21,36,1,1,,115,3,"ORANGE & ROCKLAND UTL INC","GRAHAMSVILE",0,,14154,"0M",1294,,,95,7995,0,0,10213,0,0,10828,0,0,5471,0,0,3765,0,0,6843,0,0,11715,0,0,11385,0,0,6049,0,0,6915,0,0,5017,0,0,7158,0,0,2627,6,52181,"WAT","HY" 21,36,1,1,,115,5,"ORANGE & ROCKLAND UTL INC","MONGAUP FLS",0,,14154,"0M",1294,,,95,1849,0,0,830,0,0,1994,0,0,1152,0,0,218,0,0,502,0,0,749,0,0,605,0,0,91,0,0,475,0,0,1859,0,0,1637,0,0,2630,6,52181,"WAT","HY" 21,36,1,1,,115,10,"ORANGE & ROCKLAND UTL INC","RIO",0,,14154,"0M",1294,,,95,4380,0,0,1792,0,0,4911,0,0,2578,0,0,759,0,0,986,0,0,1125,0,0,978,0,0,116,0,0,1041,0,0,4467,0,0,3352,0,0,2631,6,52181,"WAT","HY" 21,36,1,1,,115,15,"ORANGE & ROCKLAND UTL INC","SWING BR 1",0,,14154,"0M",1294,,,95,1041,0,0,442,0,0,1445,0,0,608,0,0,266,0,0,374,0,0,391,0,0,409,0,0,76,0,0,299,0,0,1316,0,0,873,0,0,2633,6,52181,"WAT","HY" 21,36,1,1,,115,20,"ORANGE & ROCKLAND UTL INC","SWING BR 2",0,,14154,"0M",1294,,,95,687,0,0,340,0,0,661,0,0,428,0,0,16,0,0,-84,0,0,164,0,0,42,0,0,-68,0,0,68,0,0,889,0,0,593,0,0,2634,6,52181,"WAT","HY" 21,36,1,2,3,115,25,"ORANGE & ROCKLAND UTL INC","BOWLINE PT",0,"HEAVY OIL",14154,"0M",1294,,,95,43906,73730,656595,138605,222519,509921,36874,60431,690856,47123,77864,612992,171664,281797,399693,132603,218077,395393,121658,204130,412273,93622,159538,457749,16475,28676,564249,22772,39554,562775,23802,41159,590697,87447,145316,516559,2625,6,52181,"FO6","ST" 21,36,1,2,9,115,25,"ORANGE & ROCKLAND UTL INC","BOWLINE PT",0,"NAT GAS",14154,"0M",1294,,,95,168974,1723560,0,82272,1239913,0,246716,2463200,0,218627,2199380,0,99656,966090,0,197607,1984380,0,277722,2939140,0,259468,2692570,0,188365,2000250,0,195838,2071510,0,142378,1499610,0,41983,424600,0,2625,6,52181,"NG","ST" 21,36,1,2,3,115,30,"ORANGE & ROCKLAND UTL INC","LOVETT",0,"HEAVY OIL",14154,"0M",1294,,,95,8,15,100319,1955,3363,96956,1,1,96927,0,0,96968,162,289,96714,7,13,96701,10,18,96682,5,10,96706,6,11,96717,0,0,96732,0,0,96732,5,10,96723,2629,6,52181,"FO6","ST" 21,36,1,2,6,115,30,"ORANGE & ROCKLAND UTL INC","LOVETT",0,"BIT COAL",14154,"0M",1294,,,95,111799,49067,63359,155251,65603,75519,116513,50062,70545,69873,29960,67950,67316,29174,75567,80224,36666,84715,138923,58882,82515,118307,52178,76055,140703,61690,59229,113469,49704,60388,125569,51656,62679,132749,58514,56774,2629,6,52181,"BIT","ST" 21,36,1,2,9,115,30,"ORANGE & ROCKLAND UTL INC","LOVETT",0,"NAT GAS",14154,"0M",1294,,,95,29773,323525,0,26698,280445,0,15824,169812,0,33214,357965,0,35392,384353,0,65900,754578,0,47901,513697,0,42001,470557,0,20369,222754,0,24743,268834,0,21096,220661,0,31665,346005,0,2629,6,52181,"NG","ST" 21,36,1,4,2,115,35,"ORANGE & ROCKLAND UTL INC","HILLBURN",0,"LIGHT OIL",14154,"0M",1294,,,95,0,0,4238,0,0,4238,0,0,4238,0,0,4238,0,9,4229,0,0,4229,52,164,4065,108,334,3731,0,0,3731,0,0,3731,0,0,3731,0,0,3731,2628,6,52181,"FO2","GT" 21,36,1,4,9,115,35,"ORANGE & ROCKLAND UTL INC","HILLBURN",0,"NATURAL G",14154,"0M",1294,,,95,44,1217,0,0,0,0,37,1143,0,565,8996,0,-13,1208,0,256,5250,0,276,4745,0,945,15862,0,444,6906,0,-18,82,0,-27,456,0,24,430,0,2628,6,52181,"NG","GT" 21,36,1,4,2,115,40,"ORANGE & ROCKLAND UTL INC","SHOEMAKER",0,"LIGHT OIL",14154,"0M",1294,,,95,0,0,4599,73,30,4569,29,103,4466,-1,30,4485,1,2,4463,45,124,4068,0,0,4068,1,3,4065,0,0,4065,22,81,3984,84,247,3738,0,0,3738,2632,6,52181,"FO2","GT" 21,36,1,4,9,115,40,"ORANGE & ROCKLAND UTL INC","SHOEMAKER",0,"NAT GAS",14154,"0M",1294,,,95,217,4023,0,342,7789,0,599,11559,0,-31,207,0,1856,30143,0,3256,49008,0,4402,75566,0,4597,74746,0,2492,42150,0,713,14586,0,45,456,0,53,1654,0,2632,6,52181,"NG","GT" 21,36,1,2,1,135,1,"ROCHESTER GAS & ELEC CORP","GINNA",0,"NUCLEAR",16183,"0M",1294,,,95,351805,0,0,321771,0,0,293087,0,0,-2750,0,0,299117,0,0,334397,0,0,342637,0,0,305248,0,0,336763,0,0,353447,0,0,342871,0,0,354889,0,0,6122,6,52501,"UR","ST" 21,36,1,1,,135,5,"ROCHESTER GAS & ELEC CORP","MILLS M 172",0,,16183,"0M",1294,,,95,68,0,0,0,0,0,79,0,0,31,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2636,6,52501,"WAT","HY" 21,36,1,1,,135,10,"ROCHESTER GAS & ELEC CORP","MT MORR 160",0,,16183,"0M",1294,,,95,0,0,0,75,0,0,0,0,0,0,0,0,49,0,0,121,0,0,87,0,0,44,0,0,16,0,0,124,0,0,132,0,0,67,0,0,2637,6,52501,"WAT","HY" 21,36,1,1,,135,15,"ROCHESTER GAS & ELEC CORP","ROCHESTER 2",0,,16183,"0M",1294,,,95,3983,0,0,3890,0,0,4861,0,0,4119,0,0,4073,0,0,2681,0,0,1898,0,0,1483,0,0,708,0,0,3228,0,0,4230,0,0,3509,0,0,2639,6,52501,"WAT","HY" 21,36,1,1,,135,25,"ROCHESTER GAS & ELEC CORP","ROCHESTER 5",0,,16183,"0M",1294,,,95,18727,0,0,8869,0,0,21670,0,0,13445,0,0,7303,0,0,4173,0,0,5885,0,0,2422,0,0,1347,0,0,9730,0,0,15462,0,0,12738,0,0,2641,6,52501,"WAT","HY" 21,36,1,1,,135,28,"ROCHESTER GAS & ELEC CORP","RCHESTER 26",0,,16183,"0M",1294,,,95,596,0,0,1040,0,0,1215,0,0,1302,0,0,1083,0,0,420,0,0,405,0,0,282,0,0,135,0,0,726,0,0,1174,0,0,1054,0,0,2638,6,52501,"WAT","HY" 21,36,1,1,,135,35,"ROCHESTER GAS & ELEC CORP","WISCOY 170",0,,16183,"0M",1294,,,95,517,0,0,408,0,0,590,0,0,391,0,0,204,0,0,97,0,0,121,0,0,83,0,0,55,0,0,240,0,0,470,0,0,462,0,0,2646,6,52501,"WAT","HY" 21,36,1,2,2,135,45,"ROCHESTER GAS & ELEC CORP","ROCHESTER 3",0,"LIGHT OIL",16183,"0M",394,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,102,143,2305,77,143,2008,122,214,1718,91,167,1882,68,119,1700,27,58,1645,2640,6,52501,"FO2","ST" 21,36,1,2,3,135,45,"ROCHESTER GAS & ELEC CORP","ROCHESTER 3",0,"HEAVY OIL",16183,"0M",1294,"R",,95,27,48,2860,14,24,2809,14,24,2745,14,24,2703,0,0,2703,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2640,6,52501,"FO6","ST" 21,36,1,2,6,135,45,"ROCHESTER GAS & ELEC CORP","ROCHESTER 3",0,"BIT COAL",16183,"0M",1294,,,95,36334,13900,770,42264,15300,1458,40715,15300,1556,45572,16900,817,17481,6500,1591,36715,14100,1438,41179,15700,936,37637,15017,1800,37010,13802,1800,27740,10832,1630,33466,12558,1431,34731,13210,1105,2640,6,52501,"BIT","ST" 21,36,1,4,2,135,45,"ROCHESTER GAS & ELEC CORP","ROCHESTER 3",0,"LIGHT OIL",16183,"0M",1294,,,95,26,81,0,4,27,0,13,41,0,3,18,0,0,0,0,6,34,0,4,6,0,46,154,0,25,76,0,8,26,0,13,63,0,1,7,0,2640,6,52501,"FO2","GT" 21,36,1,2,2,135,50,"ROCHESTER GAS & ELEC CORP","ROCHESTER 7",0,"LIGHT OIL",16183,"0M",1294,,,95,299,571,1111,90,167,1127,375,690,1162,173,310,1211,249,452,1299,566,1071,1121,331,643,1190,434,833,1065,37,71,1065,373,738,1065,345,643,958,311,571,1102,2642,6,52501,"FO2","ST" 21,36,1,2,6,135,50,"ROCHESTER GAS & ELEC CORP","ROCHESTER 7",0,"BIT COAL",16183,"0M",1294,,,95,66357,27700,114902,86515,35300,90431,90609,36600,83204,137634,53400,75835,121093,47500,85250,104898,43000,113923,112687,47700,112973,116634,48507,127749,110993,45157,153399,77990,33362,173353,81051,33064,173047,90029,35948,150667,2642,6,52501,"BIT","ST" 21,36,1,4,2,135,60,"ROCHESTER GAS & ELEC CORP","ROCHESTER 9",0,"LIGHT OIL",16183,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2644,6,52501,"FO2","GT" 21,36,1,4,9,135,60,"ROCHESTER GAS & ELEC CORP","ROCHESTER 9",0,"NAT GAS",16183,"0M",1294,,,95,26,383,0,2,74,0,14,216,0,4,174,0,0,0,0,8,290,0,17,280,0,3,89,0,24,381,0,0,0,0,3,98,0,8,143,0,2644,6,52501,"NG","GT" 21,36,5,3,2,578,5,"FREEPORT (VILLAGE OF)","PLANT NO 2",0,"LIGHT OIL",6775,"0M",1294,,,95,1463,3067,3172,1434,3271,2622,413,1557,2551,-162,121,3525,-118,217,5782,984,2264,6164,3712,7100,3595,3729,7301,5720,584,1625,6684,895,1423,5789,787,2037,3752,1869,3903,3213,2679,6,51057,"FO2","IC" 21,36,5,4,2,578,5,"FREEPORT (VILLAGE OF)","PLANT NO 2",0,"LIGHT OIL",6775,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2,12,0,13,58,0,18,95,0,0,0,0,0,0,0,0,0,0,0,0,0,2679,6,51057,"FO2","GT" 21,36,5,3,2,578,10,"FREEPORT (VILLAGE OF)","PLANT NO 1",0,"LIGHT OIL",6775,"0M",1294,,,95,182,658,1479,376,1032,1630,468,1254,1391,320,920,1697,251,803,1542,452,1093,1119,571,1281,1220,740,1757,1321,639,1551,1424,175,575,1295,402,1078,1704,465,1231,1436,2678,6,51057,"FO2","IC" 21,36,5,1,,586,1,"GOUVERNEUR (CITY OF)","GOUVERNEUR",0,,7422,"0A",1294,,,95,46,0,0,92,0,0,47,0,0,50,0,0,50,0,0,38,0,0,13,0,0,45,0,0,29,0,0,20,0,0,26,0,0,41,0,0,2680,6,51137,"WAT","HY" 21,36,5,3,2,599,1,"GREENPORT (CITY OF)","GREENPORT",0,"LIGHT OIL",7630,"0A",1294,,,95,-32,0,183,-32,0,183,-27,0,183,0,2,181,0,0,0,0,1,180,-20,0,180,-4,28,152,-10,14,182,-19,0,182,0,0,182,-1,26,181,2681,6,51177,"FO2","IC" 21,36,5,2,2,624,1,"JAMESTOWN (CITY OF)","S A CARLSON",0,"LIGHT OIL",9645,"0M",1294,,,95,105,273,377,41,102,275,21,59,394,24,59,335,20,54,281,26,64,394,57,144,250,59,144,281,26,66,215,26,69,323,44,114,209,51,136,250,2682,6,51437,"FO2","ST" 21,36,5,2,6,624,1,"JAMESTOWN (CITY OF)","S A CARLSON",0,"BIT COAL",9645,"0M",1294,,,95,17974,10638,3526,17648,10013,3826,11794,7305,3597,9844,5439,3428,9879,6006,2629,11487,6255,2811,13511,7717,2530,13208,7291,3578,9538,5398,3370,10505,6096,2827,12704,7245,3946,16956,10165,3924,2682,6,51437,"BIT","ST" 21,36,5,3,2,675,1,"ROCKVILLE CTR(VILLAGE OF)","ROCKVILLE C",0,"LIGHT OIL",16217,"0M",1294,,,95,105,294,2332,321,741,2091,43,283,1808,-60,82,1726,-18,114,2338,244,637,2368,957,2138,1919,2160,4073,1884,560,1129,2277,20,216,2061,38,213,2151,101,381,1770,2695,6,52509,"FO2","IC" 21,36,5,3,9,675,1,"ROCKVILLE CTR(VILLAGE OF)","ROCKVILLE C",0,"NAT GAS",16217,"0M",1294,,,95,642,7257,0,510,5912,0,15,471,0,0,325,0,-11,282,0,1931,20033,0,4455,46010,0,2523,26516,0,352,4031,0,47,1369,0,46,1025,0,450,5750,0,2695,6,52509,"NG","IC" 21,36,5,3,2,700,5,"SKANEATELES VILLAGE OF","SKANEATELES",0,"LIGHT OIL",17280,"0A",1294,"R",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2697,6,52670,"FO2","IC" 21,36,5,1,,712,1,"SPRINGVILLE (CITY OF)","SPRINGVILLE",0,,17846,"0A",1294,,,95,145,0,0,118,0,0,104,0,0,166,0,0,172,0,0,129,0,0,84,0,0,63,0,0,12,0,0,39,0,0,110,0,0,124,0,0,2698,6,52772,"WAT","HY" 21,36,5,1,,725,1,"WATERTOWN (CITY OF)","WATERTOWN",0,,20188,"0A",1294,,,95,2508,0,0,1826,0,0,2861,0,0,2520,0,0,2042,0,0,715,0,0,684,0,0,252,0,0,458,0,0,1925,0,0,2671,0,0,2141,0,0,2700,6,53199,"WAT","HY" 21,36,9,1,,668,1,"POWER AUTHY OF ST OF N Y","LEWISTON PG",0,"C-PUMPSTG",15296,"0M",1294,,,95,-23392,48481,0,-16321,48107,0,-18062,52914,0,-34170,75041,0,-32754,81523,0,-35246,84639,0,-35971,80543,0,-31970,78905,0,-33926,76500,0,-34404,82531,0,-25619,66689,0,-26848,63831,0,2692,6,52375,"WAT","HY" 21,36,9,2,1,668,1,"POWER AUTHY OF ST OF N Y","FITZPATRICK",0,"NUCLEAR",15296,"0M",1294,,,95,0,0,0,0,0,0,34055,0,0,544665,0,0,562170,0,0,384520,0,0,579310,0,0,577530,0,0,402855,0,0,590100,0,0,572680,0,0,580835,0,0,6110,6,52375,"UR","ST" 21,36,9,1,,668,3,"POWER AUTHY OF ST OF N Y","MOSES NIAG",0,,15296,"0M",1294,,,95,1463973,0,0,1230590,0,0,1418230,0,0,1163933,0,0,1279083,0,0,1132981,0,0,1197133,0,0,1148436,0,0,1021706,0,0,1145560,0,0,1382957,0,0,1354956,0,0,2693,6,52375,"WAT","HY" 21,36,9,2,1,668,3,"POWER AUTHY OF ST OF N Y","INDIAN PT 3",0,"NUCLEAR",15296,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,17,0,0,434533,0,0,716433,0,0,320544,0,0,0,0,0,0,0,0,-2,0,0,8907,6,52375,"UR","ST" 21,36,9,1,,668,5,"POWER AUTHY OF ST OF N Y","MOSES PR DM",0,,15296,"0M",1294,,,95,524759,0,0,481624,0,0,585412,0,0,549618,0,0,532348,0,0,526743,0,0,545520,0,0,559232,0,0,538635,0,0,554432,0,0,576778,0,0,569302,0,0,2694,6,52375,"WAT","HY" 21,36,9,1,,668,8,"POWER AUTHY OF ST OF N Y","BLENHEIM G",0,"P-PUMPSTG",15296,"0M",1294,,,95,-80117,223900,0,-66116,187582,0,-64757,198518,0,-71547,180530,0,-58305,185571,0,-61293,196731,0,-78558,215353,0,-75753,237341,0,-63547,183628,0,-66325,194141,0,-57795,177791,0,-70135,192222,0,2691,6,52375,"WAT","HY" 21,36,9,2,3,668,15,"POWER AUTHY OF ST OF N Y","POLETTI",0,"HEAVY OIL",15296,"0M",1294,,,95,33400,61649,303226,126069,209523,203682,20403,35475,168236,17269,37577,130679,19806,35708,94972,47803,62254,32718,36004,60668,68293,14149,23707,150452,35247,61190,430389,17481,30727,459549,62862,110242,349307,252627,421942,245156,2491,6,52375,"FO6","ST" 21,36,9,2,9,668,15,"POWER AUTHY OF ST OF N Y","POLETTI",0,"NAT GAS",15296,"0M",1294,,,95,99454,1128061,0,99940,1020449,0,202945,2167293,0,211435,2738075,0,258894,2862705,0,324525,2604689,0,262599,2721610,0,310920,3222176,0,205757,2168448,0,224611,2374781,0,128580,1368464,0,2466,25078,0,2491,6,52375,"NG","ST" 21,36,9,1,,668,20,"POWER AUTHY OF ST OF N Y","ASHOKAN",0,,15296,"0M",1294,,,95,1615,0,0,587,0,0,1045,0,0,2214,0,0,2450,0,0,2277,0,0,2117,0,0,2126,0,0,1756,0,0,1286,0,0,1083,0,0,1303,0,0,88,6,52375,"WAT","HY" 21,36,9,1,,668,25,"POWER AUTHY OF ST OF N Y","KENSICO",0,,15296,"0M",1294,,,95,802,0,0,73,0,0,0,0,0,1521,0,0,150,0,0,271,0,0,1411,0,0,1244,0,0,1418,0,0,1191,0,0,880,0,0,0,0,0,650,6,52375,"WAT","HY" 21,36,9,1,,668,30,"POWER AUTHY OF ST OF N Y","JARVIS",0,,15296,"0M",1294,,,95,4048,0,0,2165,0,0,2416,0,0,2485,0,0,1720,0,0,1501,0,0,1162,0,0,1003,0,0,575,0,0,2833,0,0,5091,0,0,2476,0,0,808,6,52375,"WAT","HY" 21,36,9,1,,668,35,"POWER AUTHY OF ST OF N Y","CRESCENT",0,,15296,"0M",1294,,,95,6303,0,0,4034,0,0,7316,0,0,4624,0,0,3019,0,0,2031,0,0,104,0,0,713,0,0,703,0,0,3132,0,0,6120,0,0,4690,0,0,2685,6,52375,"WAT","HY" 21,36,9,1,,668,40,"POWER AUTHY OF ST OF N Y","VISCHER FER",0,,15296,"0M",1294,,,95,5945,0,0,3714,0,0,6024,0,0,4504,0,0,2789,0,0,1833,0,0,986,0,0,123,0,0,654,0,0,2259,0,0,5980,0,0,4591,0,0,2686,6,52375,"WAT","HY" 21,36,9,5,9,668,45,"POWER AUTHY OF ST OF N Y","FLYNN",0,"WASTE HT",15296,"0M",1294,,,95,24819,192100,0,17369,134483,0,27383,211172,0,18948,146928,0,26056,199854,0,24430,188777,0,23492,184084,0,25126,194127,0,24424,188668,0,23749,183457,0,20261,158951,0,19720,154115,0,7314,6,52375,"WH","CC" 21,36,9,6,2,668,45,"POWER AUTHY OF ST OF N Y","FLYNN",0,"LIGHT OIL",15296,"0M",1294,,,95,7722,10369,101959,21462,28859,72145,0,0,72242,14,20,72083,0,0,72104,0,0,72094,0,0,72044,0,0,72052,0,0,72062,157,211,71873,9447,12866,58992,27271,36998,78070,7314,6,52375,"FO2","CT" 21,36,9,6,9,668,45,"POWER AUTHY OF ST OF N Y","FLYNN",0,"NAT GAS",15296,"0M",1294,,,95,74458,576302,0,52111,403450,0,82153,633518,0,56849,440785,0,78170,599562,0,73293,566331,0,71470,552251,0,75381,582382,0,73276,566005,0,71251,550371,0,60784,476853,0,59162,462344,0,7314,6,52375,"NG","CT" 22,34,1,2,2,24,1,"ATLANTIC CITY ELEC CO","DEEPWATER",0,"LIGHT OIL",963,"0M",1294,,181,95,0,0,123,81,130,93,0,0,131,0,0,138,14,28,165,67,129,202,80,160,147,5,10,137,40,91,189,0,29,160,0,29,131,4,8,123,2384,3,56513,"FO2","ST" 22,34,1,2,3,24,1,"ATLANTIC CITY ELEC CO","DEEPWATER",0,"HEAVY OIL",963,"0M",1294,,181,95,1345,2425,95467,4563,6516,88951,0,0,88951,0,0,88261,0,0,88261,1177,2026,86235,3361,5958,80277,5273,9351,70926,5555,8624,62302,0,0,62302,0,0,62302,0,0,62302,2384,3,56513,"FO6","ST" 22,34,1,2,6,24,1,"ATLANTIC CITY ELEC CO","DEEPWATER",0,"BIT COAL",963,"0M",1294,,181,95,29945,12519,39313,35838,15203,23710,8276,3561,20149,0,0,34389,5810,3059,52665,34469,14723,52014,42129,18253,40567,44451,19515,27979,11926,4625,44084,33654,13941,51248,53859,21346,70836,57721,22974,63900,2384,3,56513,"BIT","ST" 22,34,1,2,9,24,1,"ATLANTIC CITY ELEC CO","DEEPWATER",0,"NAT GAS",963,"0M",1294,,181,95,1491,16310,0,0,0,0,944,9940,0,1878,22040,0,11307,122240,0,11062,117040,0,27862,302860,0,29442,321050,0,12534,120040,0,807,8090,0,1552,15370,0,0,0,0,2384,3,56513,"NG","ST" 22,34,1,4,2,24,1,"ATLANTIC CITY ELEC CO","DEEPWATER",0,"LIGHT OIL",963,"0M",1294,,181,95,-8,0,770,27,44,729,14,39,690,20,103,587,0,0,587,0,0,587,0,0,587,0,0,587,0,0,587,0,0,587,0,0,587,0,0,0,2384,3,56513,"FO2","GT" 22,34,1,4,9,24,1,"ATLANTIC CITY ELEC CO","DEEPWATER",0,"NAT GAS",963,"0M",1294,,181,95,-8,0,0,0,0,0,0,0,0,0,0,0,0,0,0,629,6657,0,3831,41649,0,3649,39793,0,1027,14649,0,628,9167,0,1061,10505,0,694,6875,0,2384,3,56513,"NG","GT" 22,34,1,4,2,24,2,"ATLANTIC CITY ELEC CO","MISSOURI AV",0,"LIGHT OIL",963,"0M",1294,,181,95,-4,100,9869,278,791,9635,3,53,9582,-21,5,9576,-17,8,9568,177,455,9113,2101,5546,7361,1882,5382,8451,605,2439,10201,-18,16,10185,-16,19,10167,2,70,10097,2383,3,56513,"FO2","GT" 22,34,1,2,2,24,5,"ATLANTIC CITY ELEC CO","B L ENGLAND",0,"LIGHT OIL",963,"0M",1294,,181,95,510,999,1734,317,596,1818,213,395,1756,107,200,1734,125,224,1843,424,778,1734,424,814,1508,552,1027,1647,500,1086,1588,450,958,1654,643,1122,1377,242,442,1435,2378,3,56513,"FO2","ST" 22,34,1,2,3,24,5,"ATLANTIC CITY ELEC CO","B L ENGLAND",0,"HEAVY OIL",963,"0M",1294,,181,95,4583,8307,99579,7833,13643,103560,0,0,103560,0,0,103560,0,0,103560,8731,14731,88829,37756,66914,51324,29729,50813,69931,850,2842,113855,18800,33751,80103,0,0,80103,15770,26499,87607,2378,3,56513,"FO6","ST" 22,34,1,2,6,24,5,"ATLANTIC CITY ELEC CO","B L ENGLAND",0,"BIT COAL",963,"0M",1294,,181,95,68381,30282,165387,127521,54088,125492,123787,53379,95025,85963,36061,88754,176115,72435,61413,155554,64926,62658,185411,80134,49009,173888,73305,41509,130330,53650,71904,83030,32962,118367,145947,62033,109160,196038,81549,81843,2378,3,56513,"BIT","ST" 22,34,1,3,2,24,5,"ATLANTIC CITY ELEC CO","B L ENGLAND",0,"LIGHT OIL",963,"0M",1294,,181,95,0,0,0,5,11,0,0,0,0,0,0,0,0,0,0,12,23,0,133,257,0,321,597,0,5,10,0,0,0,0,0,0,0,0,0,0,2378,3,56513,"FO2","IC" 22,34,1,4,2,24,20,"ATLANTIC CITY ELEC CO","MIDDLE STA",0,"LIGHT OIL",963,"0M",1294,,181,95,-834,144,15410,-227,1590,15128,-1342,459,14669,-815,159,14510,-333,16,14494,-558,315,9113,2009,5421,12193,2243,7786,14637,-670,677,15327,-729,232,15284,-745,423,15069,-730,254,14814,2382,3,56513,"FO2","GT" 22,34,1,4,2,24,25,"ATLANTIC CITY ELEC CO","CEDAR STA",0,"LIGHT OIL",963,"0M",1294,,181,95,-474,179,21675,-321,918,21875,-42,70,21804,-546,56,21748,-110,38,21710,62,61,21650,3843,9672,14702,3756,10444,18151,-253,1075,20407,-631,431,21246,-535,219,21027,-679,322,20705,2380,3,56513,"FO2","GT" 22,34,1,4,2,24,30,"ATLANTIC CITY ELEC CO","CARLL CORNR",0,"LIGHT OIL",963,"0M",1294,,181,95,-28,8,13554,78,379,13175,-43,0,13175,-20,0,13175,-965,8,13167,-121,166,13002,1394,2899,10102,1615,4499,9171,-32,0,13713,-16,0,14849,-44,0,14849,49,332,14517,2379,3,56513,"FO2","GT" 22,34,1,4,9,24,30,"ATLANTIC CITY ELEC CO","CARLL CORNR",0,"NAT GAS",963,"0M",1294,,181,95,35,1120,0,452,8170,0,-76,50,0,-19,1010,0,73,2450,0,835,15970,0,6072,93380,0,5324,82370,0,-117,28460,0,861,14250,0,-44,7170,0,172,150,0,2379,3,56513,"NG","GT" 22,34,1,4,2,24,32,"ATLANTIC CITY ELEC CO","MICKETON ST",0,"LIGHT OIL",963,"0M",1294,,181,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,8008,3,56513,"FO2","GT" 22,34,1,4,9,24,32,"ATLANTIC CITY ELEC CO","MICKETON ST",0,"NAT GAS",963,"0M",1294,,181,95,665,11020,0,1084,16250,0,714,11030,0,1017,15170,0,334,6070,0,2355,35610,0,9801,143090,0,8665,129480,0,2856,42750,0,30,1480,0,2277,33340,0,276,5380,0,8008,3,56513,"NG","GT" 22,34,1,4,2,24,33,"ATLANTIC CITY ELEC CO","CUMBERLAND",0,"LIGHT OIL",963,"0M",1294,,181,95,-76,0,18141,-10,0,18141,-38,0,18141,-31,0,18141,-30,0,18141,0,0,18141,5894,12888,17367,7323,16647,12470,3,249,14661,0,0,17077,-158,198,17249,60,412,16838,5083,3,56513,"FO2","GT" 22,34,1,4,9,24,33,"ATLANTIC CITY ELEC CO","CUMBERLAND",0,"NAT GAS",963,"0M",1294,,181,95,-76,0,0,-10,0,0,-38,0,0,-31,0,0,0,0,0,-27,130,0,342,4020,0,16,200,0,1,380,0,-93,0,0,0,0,0,101,3810,0,5083,3,56513,"NG","GT" 22,34,1,4,2,24,35,"ATLANTIC CITY ELEC CO","MANTU DEPOT",0,"LIGHT OIL",963,"0M",1294,,181,95,0,0,53843,0,0,50861,0,0,80853,0,0,80853,0,0,80853,0,0,80853,0,0,58245,0,0,12871,0,0,12871,0,0,52645,0,0,52645,0,0,82122,8803,3,56513,"FO2","GT" 22,34,1,4,3,24,40,"ATLANTIC CITY ELEC CO","MANTU DEPOT",0,"HEAVY OIL",963,"0M",1294,,181,95,0,0,128847,0,0,111223,0,0,111223,0,0,111223,0,0,111223,0,0,111223,0,0,81814,0,0,111865,0,0,111865,0,0,115694,0,0,115694,0,0,131074,8804,3,56513,"FO6","GT" 22,34,1,4,2,24,45,"ATLANTIC CITY ELEC CO","SHERMAN AVE",0,"LIGHT OIL",963,"0M",1294,,181,95,70,186,14708,-45,0,14708,-30,0,14708,0,0,14708,-11,0,14708,0,0,14708,0,0,14708,-190,0,14708,0,0,14708,0,0,14708,76,193,14515,232,590,14513,7288,3,56513,"FO2","GT" 22,34,1,4,9,24,45,"ATLANTIC CITY ELEC CO","SHERMAN AVE",0,"NAT GAS",963,"0M",1294,,181,95,1386,19950,0,-45,0,0,-30,0,0,0,0,0,0,0,0,0,0,0,0,0,0,-190,0,0,0,0,0,0,0,0,1704,23780,0,2984,41500,0,7288,3,56513,"NG","GT" 22,34,1,2,1,50,1,"GPU NUCLEAR CORP","OYSTER CRK",0,"NUCLEAR",7423,"0M",1294,,,95,471880,0,0,400185,0,0,466040,0,0,457427,0,0,440064,0,0,447364,0,0,438119,0,0,420825,0,0,447572,0,0,468215,0,0,428423,0,0,307964,0,0,2388,3,58850,"UR","ST" 22,34,1,1,,78,5,"JERSEY CENTRAL PWR & LGT","YARDS CR JO",0,"P-PUMPSTG",9726,"0M",1294,,,95,-9476,31075,0,-6121,19602,0,-8606,30644,0,-9596,30043,0,-9800,36086,0,-15417,52655,0,-13938,46076,0,-11848,42668,0,-7525,27636,0,0,0,0,0,0,0,-2205,5358,0,6522,3,56512,"WAT","HY" 22,34,1,4,2,78,7,"JERSEY CENTRAL PWR & LGT","GLEN GARDNR",0,"LIGHT OIL",9726,"0M",1294,,,95,357,1074,17830,457,1242,16588,29,247,16340,30,141,16199,0,0,16199,360,1062,15138,0,0,15138,0,0,15138,149,445,14693,21,60,14633,69,223,14409,10,63,16838,8227,3,56512,"FO2","GT" 22,34,1,4,9,78,7,"JERSEY CENTRAL PWR & LGT","GLEN GARDNR",0,"NAT GAS",9726,"0M",1294,,,95,1,10,0,31,485,0,2,90,0,0,0,0,0,0,0,698,11690,0,15562,248730,0,18982,309960,0,4246,71580,0,3046,50662,0,1111,20594,0,10,377,0,8227,3,56512,"NG","GT" 22,34,1,2,3,78,9,"JERSEY CENTRAL PWR & LGT","GILBERT",0,"HEAVY OIL",9726,"0M",1294,,,95,268,611,153901,2150,4403,149484,0,0,149488,0,0,149544,0,0,149379,0,0,150080,0,0,150051,0,0,149974,0,0,150075,0,0,149949,0,0,149926,8990,12417,137518,2393,3,56512,"FO6","ST" 22,34,1,2,9,78,9,"JERSEY CENTRAL PWR & LGT","GILBERT",0,"NAT GAS",9726,"0M",1294,,,95,1658,32084,0,198,3865,0,-452,0,0,-364,0,0,-363,0,0,6011,80854,0,28213,364986,0,24888,306021,0,915,14545,0,340,8670,0,825,13717,0,331,2840,0,2393,3,56512,"NG","ST" 22,34,1,4,2,78,9,"JERSEY CENTRAL PWR & LGT","GILBERT",0,"LIGHT OIL",9726,"0M",1294,,,95,150,431,0,803,2747,0,39,127,0,0,0,0,0,0,0,1,8,0,1,3,0,791,2604,0,31,88,0,0,0,0,0,0,0,0,0,0,2393,3,56512,"FO2","GT" 22,34,1,4,9,78,9,"JERSEY CENTRAL PWR & LGT","GILBERT",0,"NAT GAS",9726,"0M",1294,,,95,1,16,0,0,0,0,1,15,0,0,0,0,0,0,0,3,79,0,2862,50800,0,6493,121452,0,911,15880,0,4,174,0,979,364,0,29,249,0,2393,3,56512,"NG","GT" 22,34,1,5,2,78,9,"JERSEY CENTRAL PWR & LGT","GILBERT",0,"LIGHT OIL",9726,"0M",1294,,,95,728,0,0,3136,0,0,1259,0,0,1612,0,0,-587,0,0,5741,0,0,26058,0,0,28272,0,0,20554,0,0,8047,0,0,19296,0,0,18926,0,0,2393,3,56512,"FO2","CC" 22,34,1,5,9,78,9,"JERSEY CENTRAL PWR & LGT","GILBERT",0,"WASTE HT",9726,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2393,3,56512,"NG","CC" 22,34,1,6,2,78,9,"JERSEY CENTRAL PWR & LGT","GILBERT",0,"LIGHT OIL",9726,"0M",1294,,,95,1147,2566,252704,5572,11989,236313,1136,2545,232067,367,826,230086,0,0,229824,2660,6112,221348,82,189,219853,2038,4709,211204,942,1977,207539,163,373,205587,83,183,203671,5739,8660,193069,2393,3,56512,"FO2","CT" 22,34,1,6,9,78,9,"JERSEY CENTRAL PWR & LGT","GILBERT",0,"NAT GAS",9726,"0M",1294,,,95,5385,68331,0,8729,106467,0,6306,80671,0,7352,94029,0,-100,0,0,15594,203104,0,61026,877903,0,70864,931070,0,54572,701754,0,24094,329931,0,60664,796524,0,81101,693848,0,2393,3,56512,"NG","CT" 22,34,1,2,3,78,10,"JERSEY CENTRAL PWR & LGT","SAYREVILLE",0,"HEAVY OIL",9726,"0M",1294,,,95,4224,7914,90214,19448,37587,72103,7,16,72200,0,0,72163,792,1710,90373,6448,15362,75189,42812,86857,27305,24793,50118,55888,1650,3646,52242,0,0,71301,7,18,90540,10844,23847,66865,2390,3,56512,"FO6","ST" 22,34,1,2,9,78,10,"JERSEY CENTRAL PWR & LGT","SAYREVILLE",0,"NAT GAS",9726,"0M",1294,,,95,20137,245800,0,2651,32100,0,6917,89800,0,-727,100,0,-407,2800,0,141,2100,0,224,4900,0,16338,199000,0,1429,25400,0,-704,0,0,2904,47900,0,306,4100,0,2390,3,56512,"NG","ST" 22,34,1,4,2,78,10,"JERSEY CENTRAL PWR & LGT","SAYREVILLE",0,"LIGHT OIL",9726,"0M",1294,,,95,93,224,31996,752,2238,29758,0,0,29758,0,0,29758,139,640,29118,0,0,29118,0,0,29118,0,0,29118,0,0,29118,0,0,29118,0,0,29118,0,0,29118,2390,3,56512,"FO2","GT" 22,34,1,4,9,78,10,"JERSEY CENTRAL PWR & LGT","SAYREVILLE",0,"NAT GAS",9726,"0M",1294,,,95,1500,19800,0,1294,21300,0,831,12100,0,898,13300,0,187,4800,0,2507,37100,0,16534,266200,0,24165,379300,0,3245,51100,0,2451,37300,0,265,3800,0,22,300,0,2390,3,56512,"NG","GT" 22,34,1,2,3,78,15,"JERSEY CENTRAL PWR & LGT","WERNER",0,"HEAVY OIL",9726,"0M",1294,,,95,259,628,28845,5405,11437,18060,1926,4703,13792,-265,311,13764,-275,69,13780,1352,3366,28845,10346,20351,28459,7922,15595,12784,55,70,13159,-271,197,32022,-298,546,32144,3509,7954,24818,2385,3,56512,"FO6","ST" 22,34,1,4,2,78,15,"JERSEY CENTRAL PWR & LGT","WERNER",0,"LIGHT OIL",9726,"0M",1294,,,95,44,115,40240,398,1664,37864,88,236,37615,0,0,37379,13,702,36473,348,618,35855,2640,8238,27453,4764,13326,33888,215,290,33598,10,269,33202,0,25,42792,3,278,41910,2385,3,56512,"FO2","GT" 22,34,1,4,2,78,20,"JERSEY CENTRAL PWR & LGT","FORKED RVR",0,"LIGHT OIL",9726,"0M",1294,,,95,0,0,16388,1066,2219,17602,713,1618,15984,0,0,15971,0,0,15989,0,0,15969,0,0,15974,0,0,15980,0,0,15980,5,12,15970,0,0,15994,221,489,15505,7138,3,56512,"FO2","GT" 22,34,1,4,9,78,20,"JERSEY CENTRAL PWR & LGT","FORKED RVR",0,"NAT GAS",9726,"0M",1294,,,95,364,4569,0,160,1908,0,1306,15609,0,1647,20147,0,1120,14174,0,2225,28309,0,12875,162923,0,11844,149957,0,4227,53220,0,1880,23454,0,1759,25611,0,749,9475,0,7138,3,56512,"NG","GT" 22,34,1,2,1,131,1,"PUBLIC SERV ELEC & GAS CO","SALEM",0,"NUCLEAR",15477,"0M",1294,,,95,818199,0,0,47631,0,0,687443,0,0,753981,0,0,247176,0,0,-8310,0,0,-7985,0,0,-5500,0,0,-3133,0,0,-2112,0,0,-2002,0,0,-2639,0,0,2410,3,52414,"UR","ST" 22,34,1,2,1,131,1,"PUBLIC SERV ELEC & GAS CO","HOPE CREEK",0,"NUCLEAR",15477,"0M",1294,,,95,778188,0,0,711976,0,0,566874,0,0,750262,0,0,767051,0,0,742345,0,0,309223,0,0,760021,0,0,742281,0,0,733449,0,0,210606,0,0,-8357,0,0,6118,3,52414,"UR","ST" 22,34,1,2,1,131,2,"PUBLIC SERV ELEC & GAS CO","SALEM",0,"NUCLEAR",15477,"0M",1294,,,95,-17867,0,0,12090,0,0,369001,0,0,767911,0,0,765246,0,0,157494,0,0,-5523,0,0,-7400,0,0,-4042,0,0,-4499,0,0,-4002,0,0,-3638,0,0,2410,3,52414,"UR","ST" 22,34,1,4,2,131,2,"PUBLIC SERV ELEC & GAS CO","BAYONNE 1",0,"LIGHT OIL",15477,"0M",1294,,,95,-19,40,3837,74,282,453,-9,0,453,-44,0,1097,-18,0,3930,-2,0,3930,252,805,3125,134,585,2744,-24,0,3373,-42,0,3744,0,26,3744,-33,25,3898,2397,3,52414,"FO2","GT" 22,34,1,2,9,131,3,"PUBLIC SERV ELEC & GAS CO","BERGEN",0,"NAT GAS",15477,"0M",1294,,,95,-2112,0,0,-2514,3702,0,8759,159907,0,3706,93882,0,82739,754972,0,167861,1271630,0,281448,2131152,0,334990,2488678,0,184434,1379778,0,154884,1248547,0,151551,1232638,0,151368,1176288,0,2398,3,52414,"NG","ST" 22,34,1,4,2,131,3,"PUBLIC SERV ELEC & GAS CO","BERGEN",0,"LIGHT OIL",15477,"0M",1294,,,95,0,0,0,0,0,21622,0,0,21622,0,0,38592,0,0,38592,0,0,61623,2310,3197,102565,0,0,118429,0,0,118396,3765,5367,113029,4832,7091,116664,465,652,117805,2398,3,52414,"FO2","GT" 22,34,1,4,9,131,3,"PUBLIC SERV ELEC & GAS CO","BERGEN",0,"NAT GAS",15477,"0M",1294,,,95,-13,0,0,0,0,0,-6,664,0,-6,644,0,-9,0,0,0,0,0,347,35845,0,505,5090,0,0,0,0,-7,0,0,-7,0,0,-8,0,0,2398,3,52414,"NG","GT" 22,34,1,2,2,131,5,"PUBLIC SERV ELEC & GAS CO","BURLINGTON",0,"LIGHT OIL",15477,"0M",1294,,,95,922,1740,0,1014,1683,0,707,1131,0,668,1366,0,0,0,0,911,1528,0,1631,2761,0,200,501,0,0,0,0,0,0,0,0,0,0,0,0,0,2399,3,52414,"FO2","ST" 22,34,1,2,3,131,5,"PUBLIC SERV ELEC & GAS CO","BURLINGTON",0,"HEAVY OIL",15477,"0M",1294,,,95,9046,15688,55522,11250,17153,88452,0,0,88452,0,0,88452,-534,0,88437,2949,4515,83916,25958,40320,43596,1803,5025,88868,-545,0,88868,-541,0,88868,-541,0,88868,-573,0,88868,2399,3,52414,"FO6","ST" 22,34,1,4,2,131,5,"PUBLIC SERV ELEC & GAS CO","BURLINGTON",0,"LIGHT OIL",15477,"0M",1294,,,95,1176,2221,83444,10436,17314,64340,158,253,93381,55,114,91811,-75,14,91811,57,96,90581,102,173,81026,4040,11276,88868,-82,16,87601,-75,58,86367,29,348,84382,4578,8912,83631,2399,3,52414,"FO2","GT" 22,34,1,4,9,131,5,"PUBLIC SERV ELEC & GAS CO","BURLINGTON",0,"NAT GAS",15477,"0M",1294,,,95,60222,642634,0,62039,580691,0,60695,548854,0,9404,108237,0,42361,363894,0,31693,299006,0,63357,605299,0,60174,537745,0,21155,187254,0,17575,158420,0,24156,217635,0,18363,172905,0,2399,3,52414,"NG","GT" 22,34,1,6,2,131,5,"PUBLIC SERV ELEC & GAS CO","BURLINGTON",0,"LIGHT OIL",15477,"0M",894,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,144,235,0,0,0,0,0,0,0,0,0,0,0,0,0,2399,3,52414,"FO2","CT" 22,34,1,4,2,131,7,"PUBLIC SERV ELEC & GAS CO","EDISON",0,"LIGHT OIL",15477,"0M",1294,,,95,152,366,106308,281,513,105795,252,403,105392,7,135,105257,0,0,105257,88,644,104610,675,1783,102827,687,1976,100851,0,0,110803,0,0,110803,126,444,110359,742,2206,108153,2400,3,52414,"FO2","GT" 22,34,1,4,9,131,7,"PUBLIC SERV ELEC & GAS CO","EDISON",0,"NAT GAS",15477,"0M",1294,,,95,-33,582,0,70,992,0,-80,345,0,0,0,0,-162,750,0,0,0,0,3046,44211,0,2441,36716,0,-100,537,0,120,3310,0,89,2079,0,28,428,0,2400,3,52414,"NG","GT" 22,34,1,4,2,131,8,"PUBLIC SERV ELEC & GAS CO","ESSEX",0,"LIGHT OIL",15477,"0M",1294,,,95,0,0,112211,4598,10660,104446,0,0,104446,0,0,103802,0,0,96326,4,10,91990,0,0,91990,0,0,91990,0,0,112914,2,185,112914,234,400,112327,894,2118,110210,2401,3,52414,"FO2","GT" 22,34,1,4,9,131,8,"PUBLIC SERV ELEC & GAS CO","ESSEX",0,"NAT GAS",15477,"0M",1294,,,95,20171,250330,0,38746,466002,0,28312,330527,0,6195,75506,0,7086,87770,0,17745,236062,0,65291,864255,0,62756,803138,0,18682,243317,0,3599,40505,0,3163,40505,0,1420,2118,0,2401,3,52414,"NG","GT" 22,34,1,2,2,131,13,"PUBLIC SERV ELEC & GAS CO","HUDSON",0,"LIGHT OIL",15477,"0M",1294,,,95,119,251,0,0,0,0,0,0,0,0,0,0,0,0,0,3,6,0,4,9,0,4,9,0,0,0,0,0,0,0,0,0,0,0,0,0,2403,3,52414,"FO2","ST" 22,34,1,2,3,131,13,"PUBLIC SERV ELEC & GAS CO","HUDSON",0,"HEAVY OIL",15477,"0M",1294,,,95,11188,21576,147242,40039,87268,59974,0,0,59974,158,379,13064,0,0,13064,0,0,13064,0,0,13064,0,0,0,0,0,0,0,0,0,0,0,0,-2401,3164,109182,2403,3,52414,"FO6","ST" 22,34,1,2,6,131,13,"PUBLIC SERV ELEC & GAS CO","HUDSON",0,"BIT COAL",15477,"0M",1294,,,95,0,0,239403,0,0,239403,46093,19713,219690,82549,35226,208484,158939,68702,225010,141427,62425,162585,235608,99546,193639,263396,110928,173063,10310,4383,258904,0,0,349753,57703,21908,369380,339660,132744,293504,2403,3,52414,"BIT","ST" 22,34,1,2,9,131,13,"PUBLIC SERV ELEC & GAS CO","HUDSON",0,"NAT GAS",15477,"0M",1294,,,95,30599,362930,0,7194,97478,0,122788,1378604,0,43966,500739,0,16188,203737,0,20750,232325,0,137870,1458255,0,96187,1102638,0,1254,45160,0,-3375,2793,0,356,3383,0,1493,16683,0,2403,3,52414,"NG","ST" 22,34,1,4,2,131,13,"PUBLIC SERV ELEC & GAS CO","HUDSON",0,"LIGHT OIL",15477,"0M",1294,,,95,119,251,352215,256,609,34606,-63,0,34606,-54,0,34597,-48,0,34597,0,0,34597,1239,2320,32262,396,2283,29962,-50,0,29962,-46,0,29962,-55,0,29962,-71,0,29959,2403,3,52414,"FO2","GT" 22,34,1,4,9,131,13,"PUBLIC SERV ELEC & GAS CO","HUDSON",0,"NAT GAS",15477,"0M",1294,,,95,0,0,0,7,103,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,3,38,0,0,0,0,0,0,0,0,0,0,0,0,0,2403,3,52414,"NG","GT" 22,34,1,2,2,131,16,"PUBLIC SERV ELEC & GAS CO","KEARNY",0,"LIGHT OIL",15477,"0M",1294,,,95,0,0,0,47,160,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2404,3,52414,"FO2","ST" 22,34,1,2,3,131,16,"PUBLIC SERV ELEC & GAS CO","KEARNY",0,"HEAVY OIL",15477,"0M",1294,,,95,-1419,0,47358,3162,9747,46218,-1264,0,46218,-811,0,43218,-763,0,46218,2322,7151,47602,25660,53229,45133,22324,46979,41775,-837,0,41775,-758,0,41755,-1135,0,41775,-1308,0,46698,2404,3,52414,"FO6","ST" 22,34,1,4,2,131,16,"PUBLIC SERV ELEC & GAS CO","KEARNY",0,"LIGHT OIL",15477,"0M",1294,,,95,375,941,65441,656,2205,61502,0,175,60444,-48,459,59831,-54,459,66419,-11,40,64109,2241,5425,58552,1592,6227,53502,-37,0,73227,-117,0,73054,-84,226,71810,-19,331,69761,2404,3,52414,"FO2","GT" 22,34,1,4,9,131,16,"PUBLIC SERV ELEC & GAS CO","KEARNY",0,"NAT GAS",15477,"0M",1294,,,95,778,10891,0,531,10070,0,-183,586,0,-132,928,0,-131,324,0,1324,24641,0,4064,67350,0,6293,99804,0,-119,0,0,-6,0,0,-8,139,0,-23,0,0,2404,3,52414,"NG","GT" 22,34,1,2,3,131,18,"PUBLIC SERV ELEC & GAS CO","LINDEN",0,"HEAVY OIL",15477,"0M",1294,,,95,-2975,0,169370,18699,47791,121579,1724,8149,41900,-1941,0,88431,-2550,0,88431,1771,15138,11078,59268,130643,95281,51534,115049,125814,-2711,0,128815,-1641,0,126134,-2551,10434,115700,-1747,0,115700,2406,3,52414,"FO6","ST" 22,34,1,4,2,131,18,"PUBLIC SERV ELEC & GAS CO","LINDEN",0,"LIGHT OIL",15477,"0M",1294,,,95,26,253,53370,313,1361,52009,448,1157,50882,3498,6627,44255,6478,14170,30085,0,0,30085,0,0,30085,564,1160,28925,0,0,49924,-37,195,49604,202,372,49037,451,1756,51571,2406,3,52414,"FO2","GT" 22,34,1,4,9,131,18,"PUBLIC SERV ELEC & GAS CO","LINDEN",0,"NAT GAS",15477,"0M",1294,,,95,-96,0,0,43,2616,0,3961,49847,0,1854,18696,0,15141,180135,0,13553,160573,0,33255,393680,0,32192,409006,0,8666,121819,0,8374,103539,0,3980,41596,0,1468,15561,0,2406,3,52414,"NG","GT" 22,34,1,2,6,131,22,"PUBLIC SERV ELEC & GAS CO","MERCER",0,"BIT COAL",15477,"0M",1294,,,95,260338,90961,263541,283481,98338,252219,105820,38401,312566,69927,25278,364038,58034,23857,399943,121372,47152,419711,144178,55677,392291,111773,44297,360087,169493,64917,301841,40666,17201,334307,135703,47712,346850,209008,71876,359245,2408,3,52414,"BIT","ST" 22,34,1,2,9,131,22,"PUBLIC SERV ELEC & GAS CO","MERCER",0,"NAT GAS",15477,"0M",1294,,,95,15072,160572,0,10698,100608,0,12860,134613,0,17393,171693,0,23606,242604,0,33578,373796,0,130882,1357300,0,110572,1186167,0,12727,142016,0,7184,77196,0,1387,12188,0,362,30224,0,2408,3,52414,"NG","ST" 22,34,1,4,2,131,22,"PUBLIC SERV ELEC & GAS CO","MERCER",0,"LIGHT OIL",15477,"0M",1294,,,95,58,452,0,99,166,0,-80,45,0,-80,22,0,-90,0,0,-84,0,0,174,1003,0,1250,2375,0,-74,0,0,-89,0,0,-86,0,0,65,504,0,2408,3,52414,"FO2","GT" 22,34,1,4,9,131,22,"PUBLIC SERV ELEC & GAS CO","MERCER",0,"NAT GAS",15477,"0M",1294,,,95,0,0,0,11,107,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,23,252,0,0,0,0,0,0,0,0,0,0,0,0,0,2408,3,52414,"NG","GT" 22,34,1,4,2,131,24,"PUBLIC SERV ELEC & GAS CO","NATIONAL PK",0,"LIGHT OIL",15477,"0M",1294,,,95,-7,0,2850,-5,0,2850,-6,0,168,-6,0,167,-7,0,1390,-6,0,3548,-6,0,3548,33,67,3481,-6,0,3481,3,25,3456,2,22,3434,-6,0,3434,2409,3,52414,"FO2","GT" 22,34,1,2,3,131,25,"PUBLIC SERV ELEC & GAS CO","SEWAREN",0,"HEAVY OIL",15477,"0M",1294,,,95,915,2021,98313,16425,33366,104241,341,778,103613,0,0,103613,1016,2372,101241,0,0,101241,128,279,100962,2211,4787,96175,4969,9343,86832,2764,7861,78971,2025,6536,72435,11423,30324,105394,2411,3,52414,"FO6","ST" 22,34,1,2,9,131,25,"PUBLIC SERV ELEC & GAS CO","SEWAREN",0,"NAT GAS",15477,"0M",1294,,,95,30968,435199,0,63113,771440,0,13222,183529,0,3478,58360,0,10032,124996,0,30077,426413,0,86401,1129748,0,69754,958979,0,7865,101861,0,-868,15021,0,1354,26896,0,943,15389,0,2411,3,52414,"NG","ST" 22,34,1,4,2,131,25,"PUBLIC SERV ELEC & GAS CO","SEWAREN",0,"LIGHT OIL",15477,"0M",1294,,,95,51,704,34543,121,263,34280,-71,0,34280,-133,0,34280,-130,0,34280,-22,30,38575,438,1523,37052,831,2943,34109,-123,0,34109,-124,0,34109,23,82,34027,80,208,33819,2411,3,52414,"FO2","GT" 22,34,1,4,9,131,25,"PUBLIC SERV ELEC & GAS CO","SEWAREN",0,"NAT GAS",15477,"0M",1294,,,95,0,0,0,2,31,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,16,0,0,0,0,2411,3,52414,"NG","GT" 22,34,1,4,2,131,27,"PUBLIC SERV ELEC & GAS CO","SALEM JO",0,"LIGHT OIL",15477,"0M",1294,,,95,-18,3,16640,85,264,16528,-5,49,16528,-14,28,17721,-15,0,17581,0,0,17581,398,125,32262,152,455,31807,-6,0,16295,2764,7861,78971,-14,0,14970,54,170,12261,2410,3,52414,"FO2","GT" 22,34,5,2,3,645,1,"VINELAND (CITY OF)","HOWARD DOWN",0,"HEAVY OIL",19856,"0M",1294,,,95,0,0,24261,803,2139,23900,486,1664,22238,294,1029,21209,2656,6649,16338,890,2102,21318,4629,11673,9645,3246,7549,10200,0,0,10347,0,0,10397,0,0,10320,2429,6628,6595,2434,3,53140,"FO6","ST" 22,34,5,2,6,645,1,"VINELAND (CITY OF)","HOWARD DOWN",0,"BIT COAL",19856,"0M",1294,,,95,7844,4284,7953,7472,4143,6788,3415,1988,9938,0,0,9849,2186,1111,8737,7260,3928,6843,6950,3861,9709,3584,3042,7673,388,209,9251,1581,798,8709,5259,2954,5755,3724,2035,5931,2434,3,53140,"BIT","ST" 22,34,5,4,2,645,10,"VINELAND (CITY OF)","WEST",0,"LIGHT OIL",19856,"0M",1294,,,95,74,199,9430,353,887,8543,45,128,8417,0,0,8417,0,0,8417,315,901,7389,2079,6227,5808,2543,5808,3568,151,900,3206,36,73,3061,6,80,2981,129,339,2818,6776,3,53140,"FO2","GT" 23,42,1,2,1,52,1,"DUQUESNE LGT CO","B VALLEY",0,"NUCLEAR",5487,"0M",1294,,,95,17240,0,0,-6300,0,0,367420,0,0,596300,0,0,615700,0,0,589500,0,0,604900,0,0,561482,0,0,591490,0,0,614130,0,0,582150,0,0,452460,0,0,6040,1,50827,"UR","ST" 23,42,1,2,1,52,2,"DUQUESNE LGT CO","B VALLEY",0,"NUCLEAR",5487,"0M",1294,,,95,610052,0,0,558397,0,0,377306,0,0,-2502,0,0,358108,0,0,592883,0,0,609130,0,0,296500,0,0,598381,0,0,622939,0,0,557126,0,0,601216,0,0,6040,1,50827,"UR","ST" 23,42,1,2,6,52,5,"DUQUESNE LGT CO","CHESWICK",0,"BIT COAL",5487,"0M",1294,,,95,355392,137291,317861,331090,126419,307477,249582,96410,291500,17430,8507,318494,299247,119774,288017,339756,132948,261655,256633,102182,276100,296500,118467,263069,297357,118900,201464,311698,126308,186349,351416,139379,173501,306740,121467,188856,8226,1,50827,"BIT","ST" 23,42,1,2,9,52,5,"DUQUESNE LGT CO","CHESWICK",0,"NAT GAS",5487,"0M",1294,,,95,1427,13928,0,331,3531,0,1002,9220,0,1172,14418,0,1806,18532,0,1364,13508,0,1549,14158,0,2639,26716,0,2701,26104,0,1881,19412,0,1411,14459,0,1232,12044,0,8226,1,50827,"NG","ST" 23,42,1,2,2,52,13,"DUQUESNE LGT CO","ELRAMA",0,"LIGHT OIL",5487,"0M",1294,,,95,1941,3768,1508,1330,2779,1204,1589,3262,979,1253,2681,1633,1006,2112,1445,803,1634,1382,1389,3062,1487,1368,2719,1591,1136,2443,1644,986,1991,1570,898,1981,1539,1195,2526,782,3098,1,50827,"FO2","ST" 23,42,1,2,6,52,13,"DUQUESNE LGT CO","ELRAMA",0,"BIT COAL",5487,"0M",1294,,,95,240736,111790,172599,220356,101044,171860,197080,90684,191628,207597,94541,190808,200161,89633,171686,159939,73949,169611,197010,95313,150545,226664,107371,139013,188236,90982,151708,97661,45101,189092,223530,101521,181601,237771,106889,154459,3098,1,50827,"BIT","ST" 23,42,1,2,2,52,15,"DUQUESNE LGT CO","F PHILLIPS",0,"LIGHT OIL",5487,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,3099,1,50827,"FO2","ST" 23,42,1,2,6,52,15,"DUQUESNE LGT CO","F PHILLIPS",0,"BIT COAL",5487,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,3099,1,50827,"BIT","ST" 23,42,1,4,2,52,27,"DUQUESNE LGT CO","BRUNOT ILND",0,"LIGHT OIL",5487,"0M",1294,,,95,-733,567,24237,-801,692,23545,-848,9,23536,-662,220,23316,-662,0,23316,-579,460,22856,1005,4706,18150,5198,15710,17539,-587,0,19993,-604,0,19993,-808,0,19993,-777,582,20583,3096,1,50827,"FO2","GT" 23,42,1,5,2,52,27,"DUQUESNE LGT CO","BRUNOT ILND",0,"LIGHT OIL",5487,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,3096,1,50827,"FO2","CC" 23,42,1,6,2,52,27,"DUQUESNE LGT CO","BRUNOT ILND",0,"LIGHT OIL",5487,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,3096,1,50827,"FO2","CT" 23,42,1,2,1,100,1,"GPU NUCLEAR CORP","3 MI ISLAND",0,"NUCLEAR",7423,"0M",1294,,,95,611412,0,0,552321,0,0,609022,0,0,586279,0,0,599986,0,0,573186,0,0,584601,0,0,586748,0,0,144888,0,0,338797,0,0,590553,0,0,610193,0,0,8011,3,58850,"UR","ST" 23,42,1,1,,114,15,"METROPOLITAN EDISON CO","YORK HAVEN",0,,12390,"0M",1294,,,95,8890,0,0,9724,0,0,12867,0,0,10005,0,0,12383,0,0,12781,0,0,10950,0,0,1654,0,0,3141,0,0,8336,0,0,12409,0,0,9435,0,0,3117,3,54020,"WAT","HY" 23,42,1,4,2,114,24,"METROPOLITAN EDISON CO","HAMILTON",0,"LIGHT OIL",12390,"0M",1294,,,95,0,44,4643,342,858,4499,38,102,4397,28,68,4330,-2,0,4330,0,0,4330,432,1398,2932,1179,2884,2369,143,356,3085,0,0,3085,47,129,3491,190,511,4606,3109,3,54020,"FO2","GT" 23,42,1,4,2,114,25,"METROPOLITAN EDISON CO","HUNTERSTOWN",0,"LIGHT OIL",12390,"0M",1294,,,95,44,117,8244,904,2365,9808,139,361,9448,53,150,8583,0,1,8583,0,0,8582,1,3,8579,16,42,8895,2,7,9067,19,50,9017,7,22,8995,281,706,8304,3110,3,54020,"FO2","GT" 23,42,1,4,9,114,25,"METROPOLITAN EDISON CO","HUNTERSTOWN",0,"NAT GAS",12390,"0M",1294,,,95,1133,17680,0,1048,17830,0,7,180,0,729,13320,0,504,8500,0,1339,19320,0,3546,41940,0,6556,84500,0,3434,53290,0,1503,23470,0,1262,20430,0,1780,27282,0,3110,3,54020,"NG","GT" 23,42,1,4,2,114,27,"METROPOLITAN EDISON CO","MOUNTAIN",0,"LIGHT OIL",12390,"0M",1294,,,95,71,188,6429,964,2523,5157,48,126,5031,4,12,5912,0,0,5912,0,1,5911,0,2,5910,0,0,5910,36,175,5913,0,0,6270,0,2,6804,367,1234,6575,3111,3,54020,"FO2","GT" 23,42,1,4,9,114,27,"METROPOLITAN EDISON CO","MOUNTAIN",0,"NATURAL G",12390,"0M",1294,,,95,297,5940,0,476,8360,0,443,6390,0,469,7770,0,208,3710,0,328,5630,0,1743,26610,0,3541,53620,0,894,14500,0,170,2840,0,572,8810,0,1301,18260,0,3111,3,54020,"NG","GT" 23,42,1,4,2,114,31,"METROPOLITAN EDISON CO","ORRTANNA",0,"LIGHT OIL",12390,"0M",1294,,,95,48,116,4401,346,875,4418,88,218,4200,26,66,4135,0,0,4135,0,0,4135,593,1575,2917,1316,3402,1824,159,409,2667,26,65,3674,0,7,5453,229,581,4898,3112,3,54020,"FO2","GT" 23,42,1,2,2,114,32,"METROPOLITAN EDISON CO","PORTLAND",0,"LIGHT OIL",12390,"0M",1294,,,95,1210,2219,56721,612,1085,51313,671,1307,49944,1587,3013,45429,432,812,42830,190,349,41500,955,1701,39591,434,783,37499,499,951,35882,161,335,60358,2066,4127,57233,222,397,56872,3113,3,54020,"FO2","ST" 23,42,1,2,6,114,32,"METROPOLITAN EDISON CO","PORTLAND",0,"BIT COAL",12390,"0M",1294,,,95,132808,53399,109521,182821,71489,66961,66747,28478,108572,54477,22914,130642,57698,23989,150827,144768,58703,134821,179344,71804,85267,178789,70856,51093,83228,35019,46481,11852,5425,93489,58689,25583,120272,183470,71507,85462,3113,3,54020,"BIT","ST" 23,42,1,4,2,114,32,"METROPOLITAN EDISON CO","PORTLAND",0,"LIGHT OIL",12390,"0M",1294,,,95,77,142,2671,1704,3020,3973,50,98,3938,790,1501,3938,951,1787,3938,662,1215,3705,281,501,3412,727,1310,3410,2125,4049,3409,1,3,3407,122,245,3406,1839,3288,3291,3113,3,54020,"FO2","GT" 23,42,1,4,9,114,32,"METROPOLITAN EDISON CO","PORTLAND",0,"NAT GAS",12390,"0M",1294,,,95,7,72,0,1596,15661,0,2973,32178,0,2051,22130,0,3978,42351,0,12035,125176,0,33248,336088,0,28922,295790,0,5224,56353,0,750,8818,0,2029,22553,0,597,5955,0,3113,3,54020,"NG","GT" 23,42,1,4,2,114,34,"METROPOLITAN EDISON CO","SHAWNEE",0,"LIGHT OIL",12390,"0M",1294,,,95,73,171,6099,265,687,6483,16,27,6472,20,60,6412,44,112,6301,35,90,6211,135,371,5839,869,2245,3594,68,177,3417,0,0,4845,68,117,5622,0,0,5679,3114,3,54020,"FO2","GT" 23,42,1,2,2,114,35,"METROPOLITAN EDISON CO","TITUS",0,"LIGHT OIL",12390,"0M",1294,,,95,102,198,885,73,138,926,387,772,869,487,933,1186,472,874,1205,168,334,1228,294,559,1026,220,409,617,291,530,803,369,699,998,321,614,560,227,431,880,3115,3,54020,"FO2","ST" 23,42,1,2,6,114,35,"METROPOLITAN EDISON CO","TITUS",0,"BIT COAL",12390,"0M",1294,,,95,73788,31030,99475,51570,21149,100003,47245,20126,101173,38103,15904,107895,66063,26455,103387,95872,40846,84743,118659,48529,57453,118052,46687,37871,105060,41177,26170,83805,34936,50826,103029,42373,57757,128752,52966,41217,3115,3,54020,"BIT","ST" 23,42,1,4,2,114,35,"METROPOLITAN EDISON CO","TITUS",0,"LIGHT OIL",12390,"0M",1294,,,95,58,114,4000,793,1492,4117,0,0,4117,1,2,4115,0,0,4115,4,8,4106,65,124,3983,133,248,3983,0,0,3983,131,248,3734,20,39,3695,0,0,3755,3115,3,54020,"FO2","GT" 23,42,1,4,9,114,35,"METROPOLITAN EDISON CO","TITUS",0,"NAT GAS",12390,"0M",1294,,,95,53,575,0,23,240,0,80,890,0,60,640,0,52,541,0,22,250,0,1587,16770,0,2936,30250,0,319,3230,0,110,1190,0,149,1590,0,5,60,0,3115,3,54020,"NG","GT" 23,42,1,4,2,114,38,"METROPOLITAN EDISON CO","TOLNA",0,"LIGHT OIL",12390,"0M",1294,,,95,68,175,6400,563,1516,6278,90,224,6054,0,1,6053,0,0,6053,0,0,6053,759,2033,4020,2323,6134,2677,164,447,5438,64,349,6339,62,101,6238,114,281,6229,3116,3,54020,"FO2","GT" 23,42,1,2,2,133,1,"PENNSYLVANIA ELEC CO","CONMAUGH JO",0,"LIGHT OIL",14711,"0M",1294,,250,95,514,827,5361,559,930,4122,454,736,6813,810,1319,5181,459,747,4344,78,121,4153,878,1456,2385,538,892,3017,74,121,5479,0,0,5356,3148,5217,7748,383,627,6559,3118,3,54025,"FO2","ST" 23,42,1,2,6,133,1,"PENNSYLVANIA ELEC CO","CONMAUGH JO",0,"BIT COAL",14711,"0M",1294,,250,95,1122156,419851,722958,925303,359096,640938,1076935,406220,574117,992331,375372,600365,1073542,404411,660222,1082614,409954,586984,1087889,419782,543363,1144736,439047,524854,727433,274855,587632,579871,221827,735222,799742,308937,733868,1107177,421853,608881,3118,3,54025,"BIT","ST" 23,42,1,2,9,133,1,"PENNSYLVANIA ELEC CO","CONMAUGH JO",0,"NAT GAS",14711,"0M",1294,,250,95,1516,13798,0,1026,9654,0,566,5184,0,1707,15719,0,1710,15719,0,264,2319,0,2347,22035,0,3446,32313,0,452,4120,0,258,2408,0,2434,22766,0,571,5283,0,3118,3,54025,"NG","ST" 23,42,1,3,2,133,1,"PENNSYLVANIA ELEC CO","CONMAUGH JO",0,"LIGHT OIL",14711,"0M",1294,,250,95,59,96,0,34,57,0,59,97,0,181,295,0,54,89,0,45,71,0,187,311,0,146,243,0,46,75,0,31,52,0,78,130,0,46,76,0,3118,3,54025,"FO2","IC" 23,42,1,1,,133,5,"PENNSYLVANIA ELEC CO","PINEY",0,,14711,"0M",1294,,250,95,7087,0,0,2980,0,0,8315,0,0,7025,0,0,7405,0,0,7866,0,0,1807,0,0,900,0,0,618,0,0,1506,0,0,5259,0,0,4760,0,0,3124,3,54025,"WAT","HY" 23,42,1,1,,133,13,"PENNSYLVANIA ELEC CO","SENECA JO",0,"C-PUMPSTG",14711,"0M",1294,,250,95,-18038,60718,0,-12762,44459,0,-13759,53339,0,-14476,46086,0,-10189,43886,0,-20535,71955,0,-32632,124316,0,-31819,130160,0,-23462,98242,0,-26851,110227,0,-17180,96885,0,-19235,101307,0,8225,3,54025,"WAT","HY" 23,42,1,4,9,133,17,"PENNSYLVANIA ELEC CO","BLOSSBURG",0,"NAT GAS",14711,"0M",1294,,250,95,-5,0,0,248,3769,0,-4,0,0,0,0,0,0,0,0,0,0,0,502,7485,0,846,9556,0,243,7354,0,-5,0,0,-4,0,0,-4,0,0,3120,3,54025,"NG","GT" 23,42,1,2,2,133,25,"PENNSYLVANIA ELEC CO","HOMER CTYJO",0,"LIGHT OIL",14711,"0M",1294,,250,95,724,1106,10724,239,368,10825,1397,2089,8613,678,1026,8717,2469,3709,5517,3227,5084,7324,1158,1765,5736,474,737,6933,1569,3909,7274,769,1187,8528,7523,12170,9104,4070,6343,6965,3122,3,54025,"FO2","ST" 23,42,1,2,6,133,25,"PENNSYLVANIA ELEC CO","HOMER CTYJO",0,"BIT COAL",14711,"0M",1294,,250,95,1185616,454082,568142,1188794,455176,479305,1210546,457862,391125,1087359,409749,340123,685495,258590,520058,1050104,414471,562956,1147586,445483,356766,1213094,474606,228657,448257,271599,331273,758425,290978,460056,823682,334855,431770,991225,388795,409243,3122,3,54025,"BIT","ST" 23,42,1,2,2,133,45,"PENNSYLVANIA ELEC CO","SEWARD",0,"LIGHT OIL",14711,"0M",1294,,250,95,662,1281,675,306,595,618,281,535,616,145,261,535,122,305,409,432,940,535,285,552,414,274,531,585,416,789,657,463,878,671,432,834,724,340,657,600,3130,3,54025,"FO2","ST" 23,42,1,2,6,133,45,"PENNSYLVANIA ELEC CO","SEWARD",0,"BIT COAL",14711,"0M",1294,,250,95,101596,46820,104963,110101,50567,86392,110470,50520,76721,54307,23628,78208,29270,17347,91227,52721,27510,83682,115539,53769,77789,119322,55517,67991,102723,46904,73094,107866,49063,74467,105367,48397,85472,116951,53923,61526,3130,3,54025,"BIT","ST" 23,42,1,2,2,133,48,"PENNSYLVANIA ELEC CO","SHAWVILLE",0,"LIGHT OIL",14711,"0M",1294,,250,95,1123,1920,8833,2602,4605,6882,3250,5700,8490,1312,2317,8459,872,1542,9545,917,1633,7965,912,1584,7411,1122,2141,8065,1665,3195,7890,1607,2973,8086,2444,4275,8035,3504,6399,6379,3131,3,54025,"FO2","ST" 23,42,1,2,6,133,48,"PENNSYLVANIA ELEC CO","SHAWVILLE",0,"BIT COAL",14711,"0M",1294,,250,95,269348,109338,102763,256827,107901,105884,326710,136132,96046,350160,145852,80632,328883,137262,84982,336010,141689,79617,350851,144610,79435,304942,138068,76369,248206,112475,83476,317261,138069,65107,346273,142913,61290,323453,141293,48123,3131,3,54025,"BIT","ST" 23,42,1,3,2,133,48,"PENNSYLVANIA ELEC CO","SHAWVILLE",0,"LIGHT OIL",14711,"0M",1294,,250,95,31,54,764,42,75,689,26,47,797,22,39,757,20,37,721,29,52,669,42,74,740,203,388,705,22,43,662,24,46,763,18,32,731,24,44,819,3131,3,54025,"FO2","IC" 23,42,1,2,2,133,60,"PENNSYLVANIA ELEC CO","WARREN",0,"LIGHT OIL",14711,"0M",1294,,250,95,101,246,375,38,94,281,58,147,313,65,158,336,29,123,391,38,93,297,45,104,725,30,76,657,8,20,637,47,126,511,41,109,402,38,97,482,3132,3,54025,"FO2","ST" 23,42,1,2,6,133,60,"PENNSYLVANIA ELEC CO","WARREN",0,"BIT COAL",14711,"0M",1294,,250,95,23223,13460,34201,30943,18008,26672,17000,10379,34033,20947,11998,35372,16865,16419,30837,28698,16502,23133,35556,19496,14235,32084,18799,17943,18322,10742,21117,17556,10786,25392,16779,10295,31120,32207,19202,23049,3132,3,54025,"BIT","ST" 23,42,1,4,2,133,60,"PENNSYLVANIA ELEC CO","WARREN",0,"LIGHT OIL",14711,"0M",1294,,250,95,2,7,9205,924,2260,9835,124,314,9521,0,1,9519,94,389,9130,154,374,8757,2078,4788,7154,3447,8693,6033,514,1272,7934,0,0,7934,105,276,7658,393,986,9466,3132,3,54025,"FO2","GT" 23,42,1,4,9,133,60,"PENNSYLVANIA ELEC CO","WARREN",0,"NAT GAS",14711,"0M",1294,,250,95,0,10,0,0,10,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,3132,3,54025,"NG","GT" 23,42,1,3,2,133,75,"PENNSYLVANIA ELEC CO","BENTON",0,"LIGHT OIL",14711,"0M",1294,"R",250,95,-3,0,0,-2,0,0,-3,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,3119,3,54025,"FO2","IC" 23,42,1,4,2,133,87,"PENNSYLVANIA ELEC CO","WAYNE",0,"LIGHT OIL",14711,"0M",1294,,250,95,-99,18,20263,508,1505,18758,-92,0,18758,-86,0,18758,-70,1,18757,-54,0,18757,1349,3469,15288,3798,9355,11397,490,1027,13199,-52,0,13199,141,1098,14037,154,691,18031,3134,3,54025,"FO2","GT" 23,42,1,2,2,133,90,"PENNSYLVANIA ELEC CO","KEYSTONE JO",0,"LIGHT OIL",14711,"0M",1294,,250,95,2244,3690,6503,1272,2084,8137,0,0,8969,4533,7554,9207,714,1204,9434,965,1623,9346,2145,3684,9013,3083,5243,9005,923,1553,9324,753,1254,8496,1264,2066,8810,0,0,8724,3136,3,54025,"FO2","ST" 23,42,1,2,6,133,90,"PENNSYLVANIA ELEC CO","KEYSTONE JO",0,"BIT COAL",14711,"0M",1294,,250,95,1102214,423987,311858,582793,225211,453587,563417,222247,605342,809149,315890,648804,1078337,426399,648546,1084349,429852,601163,1034268,420581,454702,938657,378854,582342,1033031,410618,649687,1088547,426659,795799,1058746,408591,711979,1180880,456067,560683,3136,3,54025,"BIT","ST" 23,42,1,3,2,133,90,"PENNSYLVANIA ELEC CO","KEYSTONE JO",0,"LIGHT OIL",14711,"0M",1294,,250,95,349,575,0,349,573,0,34,59,0,204,341,0,100,170,0,35,60,0,207,356,0,870,1480,0,155,262,0,66,110,0,178,291,0,46,86,0,3136,3,54025,"FO2","IC" 23,42,1,2,2,135,1,"PENNSYLVANIA POWER CO","NEW CASTLE",0,"LIGHT OIL",14716,"0M",1294,,,95,157,295,104,61,118,158,276,532,107,184,352,158,327,657,138,250,493,138,176,344,140,152,297,106,171,327,131,192,372,116,117,218,145,156,288,161,3138,1,52289,"FO2","ST" 23,42,1,2,6,135,1,"PENNSYLVANIA POWER CO","NEW CASTLE",0,"BIT COAL",14716,"0M",1294,,,95,167856,72057,99647,154279,67443,98213,130534,58811,77871,125682,55847,86191,67772,31976,90113,98557,45757,95531,118202,53998,90022,140629,64008,74786,116270,52148,73949,88872,40250,91385,140709,61724,82726,150687,61716,63171,3138,1,52289,"BIT","ST" 23,42,1,3,2,135,1,"PENNSYLVANIA POWER CO","NEW CASTLE",0,"LIGHT OIL",14716,"0M",1294,,,95,22,56,1012,6,7,1012,7,22,863,1,3,991,4,9,875,1,7,1095,68,120,980,348,650,769,21,48,895,12,25,914,9,4,978,1,5,846,3138,1,52289,"FO2","IC" 23,42,1,2,2,135,12,"PENNSYLVANIA POWER CO","MANSFLD JO",0,"LIGHT OIL",14716,"0M",1294,,,95,1007,1692,29171,723,1155,27861,1506,2563,20232,2103,3540,37005,3377,5991,30895,1363,2382,49447,1396,2364,47084,1578,2757,44327,1128,2011,40209,852,1442,3868,625,1076,37528,5978,10675,26852,6094,1,52289,"FO2","ST" 23,42,1,2,6,135,12,"PENNSYLVANIA POWER CO","MANSFLD JO",0,"BIT COAL",14716,"0M",1294,,,95,1000025,404047,691181,900788,348267,715644,764097,314521,842427,1018498,413184,894368,1102944,466816,876286,1268001,530524,794307,1358940,556273,756092,1346419,567300,719388,816664,349651,802659,889136,365870,922037,897824,373667,888666,766127,330985,1035343,6094,1,52289,"BIT","ST" 23,42,1,2,1,137,1,"PENNSYLVANIA PWR & LGT CO","SUSQUEHANNA",0,"NUCLEAR",14715,"0M",1294,,,95,784581,0,0,707744,0,0,597267,0,0,-6623,0,0,455272,0,0,764570,0,0,800626,0,0,807866,0,0,781516,0,0,816456,0,0,256044,0,0,663200,0,0,6103,3,52288,"UR","ST" 23,42,1,2,1,137,2,"PENNSYLVANIA PWR & LGT CO","SUSQUEHANNA",0,"NUCLEAR",14715,"0M",1294,,,95,819260,0,0,744537,0,0,809836,0,0,572523,0,0,800757,0,0,763767,0,0,784244,0,0,790491,0,0,327567,0,0,158303,0,0,801099,0,0,820399,0,0,6103,3,52288,"UR","ST" 23,42,1,1,,137,8,"PENNSYLVANIA PWR & LGT CO","HOLTWOOD",0,,14715,"0M",1294,,,95,63368,0,0,44815,0,0,66767,0,0,61784,0,0,47914,0,0,44060,0,0,38745,0,0,15029,0,0,8892,0,0,3395,0,0,54454,0,0,52183,0,0,3145,3,52288,"WAT","HY" 23,42,1,2,2,137,8,"PENNSYLVANIA PWR & LGT CO","HOLTWOOD",0,"LIGHT OIL",14715,"0M",1294,,,95,2,293,307,92,564,453,76,299,502,6,12,486,9,103,375,64,316,412,48,185,402,32,69,513,156,340,542,105,324,374,44,96,457,71,158,639,3145,3,52288,"FO2","ST" 23,42,1,2,4,137,8,"PENNSYLVANIA PWR & LGT CO","HOLTWOOD",0,"ANTH COAL",14715,"0M",1294,,,95,16657,10967,92177,28295,20094,81874,38352,28374,83310,37995,26901,93553,28887,20504,97262,21957,15483,110941,27038,19535,107719,38254,26848,105902,36692,25935,106839,27783,20333,110563,38411,27438,93901,40473,29360,79473,3145,3,52288,"ANT","ST" 23,42,1,2,5,137,8,"PENNSYLVANIA PWR & LGT CO","HOLTWOOD",0,"COKE",14715,"0M",1294,,,95,5600,3687,7954,10386,7347,6463,12376,9136,6569,13390,9479,6750,10455,7419,8863,7778,5469,5689,9256,6676,3115,13170,9235,2168,11989,8438,3400,7495,5464,2289,8623,7102,1550,11704,5956,0,3145,3,52288,"PC","ST" 23,42,1,1,,137,14,"PENNSYLVANIA PWR & LGT CO","WALLENPAUPK",0,,14715,"0M",1294,,,95,12278,0,0,38773,0,0,4171,0,0,-24207,0,0,735,0,0,560,0,0,5204,0,0,2717,0,0,244,0,0,24,0,0,11908,0,0,11545,0,0,3153,3,52288,"WAT","HY" 23,42,1,4,2,137,15,"PENNSYLVANIA PWR & LGT CO","ALLENTOWN",0,"LIGHT OIL",14715,"0M",1294,,,95,64,195,4597,200,523,4444,0,0,4446,40,90,4355,0,0,4356,122,333,4024,199,561,4006,2797,7611,4017,44,168,4389,12,34,4355,0,0,4351,134,369,4531,3139,3,52288,"FO2","GT" 23,42,1,2,2,137,20,"PENNSYLVANIA PWR & LGT CO","BRUNNER ISL",0,"LIGHT OIL",14715,"0M",1294,,,95,5215,9667,5220,2811,6985,2945,2623,7457,4341,1006,3274,4688,1673,5855,4747,623,3511,4635,1145,3027,3800,192,491,4638,1850,4455,1752,956,1998,4421,1497,3195,3955,6348,15226,4765,3140,3,52288,"FO2","ST" 23,42,1,2,6,137,20,"PENNSYLVANIA PWR & LGT CO","BRUNNER ISL",0,"BIT COAL",14715,"0M",1294,,,95,726861,278333,624176,797416,299207,615563,638681,243796,659948,618218,235042,726562,483331,182515,843219,636052,246917,774595,729927,280541,565746,770922,293672,454478,661164,258193,418744,632910,240757,448356,500569,201629,451028,542332,211139,476821,3140,3,52288,"BIT","ST" 23,42,1,3,2,137,20,"PENNSYLVANIA PWR & LGT CO","BRUNNER ISL",0,"LIGHT OIL",14715,"0M",1294,,,95,43,75,0,27,35,0,29,50,0,11,33,0,29,50,0,27,47,0,38,66,0,41,123,0,30,52,0,27,47,0,21,37,0,28,47,0,3140,3,52288,"FO2","IC" 23,42,1,4,2,137,26,"PENNSYLVANIA PWR & LGT CO","FISHBACH",0,"LIGHT OIL",14715,"0M",1294,,,95,0,0,2203,37,115,2088,0,0,2076,11,33,2043,0,0,2039,16,52,1987,102,265,2080,1274,3289,1978,63,218,2105,0,0,2095,0,0,2105,13,33,2071,3142,3,52288,"FO2","GT" 23,42,1,4,2,137,28,"PENNSYLVANIA PWR & LGT CO","HARWOOD",0,"LIGHT OIL",14715,"0M",1294,,,95,0,0,2216,83,240,2157,0,0,2152,44,152,2171,0,0,2171,13,61,2272,289,883,2098,1064,3093,1958,134,415,2230,60,205,2217,0,0,2217,0,0,2208,3144,3,52288,"FO2","GT" 23,42,1,4,2,137,29,"PENNSYLVANIA PWR & LGT CO","HARRISBURG",0,"LIGHT OIL",14715,"0M",1294,,,95,0,0,4184,328,916,4530,0,0,4528,34,103,4425,7,31,4394,111,326,4426,221,659,4486,3286,9229,3610,329,960,4424,0,0,4424,8,0,4410,101,283,4486,3143,3,52288,"FO2","GT" 23,42,1,2,2,137,32,"PENNSYLVANIA PWR & LGT CO","MARTINS CRK",0,"LIGHT OIL",14715,"0M",1294,,,95,1397,3966,1367,1654,3961,905,487,1818,1153,845,3118,1197,886,4111,1282,1222,4052,1400,1679,4825,803,2026,5349,775,303,753,1408,633,2680,1365,1511,3919,1485,2510,5735,1078,3148,3,52288,"FO2","ST" 23,42,1,2,3,137,32,"PENNSYLVANIA PWR & LGT CO","MARTINS CRK",0,"HEAVY OIL",14715,"0M",1294,,,95,3313,20105,1792976,137098,246817,1537637,4594,16136,1518993,7837,26024,1486208,0,0,1482804,46574,94076,1387076,225007,410380,970823,241933,469387,1094662,32635,57250,1132457,11373,23775,1505839,59422,125764,1590347,265457,506756,1125474,3148,3,52288,"FO6","ST" 23,42,1,2,6,137,32,"PENNSYLVANIA PWR & LGT CO","MARTINS CRK",0,"BIT COAL",14715,"0M",1294,,,95,77736,33553,94127,107453,45145,78631,33245,15373,94972,56476,25532,79013,56350,25210,63411,56558,24356,57931,77903,34985,45157,72539,34251,53601,19134,10553,62015,28384,12765,56271,68305,31511,46146,107135,53235,34362,3148,3,52288,"BIT","ST" 23,42,1,3,2,137,32,"PENNSYLVANIA PWR & LGT CO","MARTINS CRK",0,"LIGHT OIL",14715,"0M",1294,,,95,19,33,0,53,92,0,70,124,0,63,90,0,15,57,0,18,30,0,7,12,0,39,74,0,10,20,0,7,13,0,4,7,0,20,9,0,3148,3,52288,"FO2","IC" 23,42,1,4,2,137,32,"PENNSYLVANIA PWR & LGT CO","MARTINS CRK",0,"LIGHT OIL",14715,"0M",1294,,,95,0,0,5154,253,713,4491,0,0,4487,23,66,4408,0,0,4408,97,271,4056,301,924,3141,2928,8451,3433,332,1023,4044,0,0,4797,34,92,6619,47,134,6156,3148,3,52288,"FO2","GT" 23,42,1,4,2,137,34,"PENNSYLVANIA PWR & LGT CO","JENKINS",0,"LIGHT OIL",14715,"0M",1294,,,95,0,0,2287,49,143,2325,0,0,2326,12,59,2267,0,0,2265,0,0,2261,285,831,1773,1377,3617,2093,62,169,2280,17,50,2230,0,0,2177,0,0,2170,3146,3,52288,"FO2","GT" 23,42,1,4,2,137,36,"PENNSYLVANIA PWR & LGT CO","LOCK HAVEN",0,"LIGHT OIL",14715,"0M",1294,,,95,2,17,2072,0,0,2072,0,0,2071,0,0,2072,0,0,2231,19,50,2181,47,187,2160,309,776,1940,29,62,2234,0,0,2233,0,0,2229,0,0,2223,3147,3,52288,"FO2","GT" 23,42,1,2,2,137,38,"PENNSYLVANIA PWR & LGT CO","MONTOUR",0,"LIGHT OIL",14715,"0M",1294,,,95,5284,3061,15269,1120,9829,7128,603,1538,7267,606,3951,8198,13,2000,6913,5227,30521,8337,1368,7253,4923,878,2071,5843,1573,7626,7055,7633,17598,7723,1969,8730,7062,7059,10859,7500,3149,3,52288,"FO2","ST" 23,42,1,2,6,137,38,"PENNSYLVANIA PWR & LGT CO","MONTOUR",0,"BIT COAL",14715,"0M",1294,,,95,847074,335924,519372,875346,340631,445625,780698,304571,380887,372505,141113,452083,435583,162563,503087,625764,248102,531404,836431,328954,481373,911902,352540,306054,690630,264412,407406,817637,314073,299288,838531,328858,291789,880367,352324,220532,3149,3,52288,"BIT","ST" 23,42,1,2,2,137,40,"PENNSYLVANIA PWR & LGT CO","SUNBURY",0,"LIGHT OIL",14715,"0M",1294,,,95,120,1018,953,89,415,868,270,1417,1025,212,1169,913,362,1349,784,121,240,1084,94,305,938,95,427,967,167,1398,1038,316,896,961,315,1038,893,516,1056,864,3152,3,52288,"FO2","ST" 23,42,1,2,4,137,40,"PENNSYLVANIA PWR & LGT CO","SUNBURY",0,"ANTH COAL",14715,"0M",1294,,,95,59791,48178,418732,52800,43904,407593,42379,34783,387855,56229,44534,380823,54876,44151,401119,43071,35250,457310,34960,27900,513983,38518,30044,586494,54062,41683,635399,58158,44699,652259,58144,45249,613424,56311,42856,591156,3152,3,52288,"ANT","ST" 23,42,1,2,5,137,40,"PENNSYLVANIA PWR & LGT CO","SUNBURY",0,"COKE",14715,"0M",1294,,,95,32080,14266,18014,37875,17579,8930,34489,14591,2989,39190,17032,15602,35966,15206,24516,28052,11818,24368,21736,9175,21882,27009,11174,25559,37827,15339,20820,35544,14870,22116,40820,17176,11347,43815,18422,22426,3152,3,52288,"PC","ST" 23,42,1,2,6,137,40,"PENNSYLVANIA PWR & LGT CO","SUNBURY",0,"BIT COAL",14715,"0M",1294,,,95,38602,20937,145827,50229,27422,136935,127350,62833,126363,110076,53702,131074,110470,54187,128876,117078,56381,126273,137002,67568,99984,129986,64144,93470,121920,58717,95585,117436,55949,93435,118781,56941,78649,145641,68789,57848,3152,3,52288,"BIT","ST" 23,42,1,3,2,137,40,"PENNSYLVANIA PWR & LGT CO","SUNBURY",0,"LIGHT OIL",14715,"0M",1294,,,95,29,54,0,17,32,0,22,41,0,12,22,0,18,33,0,15,28,0,10,19,0,41,76,0,14,26,0,21,39,0,16,30,0,15,28,0,3152,3,52288,"FO2","IC" 23,42,1,4,2,137,40,"PENNSYLVANIA PWR & LGT CO","SUNBURY",0,"LIGHT OIL",14715,"0M",1294,,,95,0,0,4196,0,0,4357,0,0,4367,0,0,4367,0,0,4367,12,34,4284,56,161,4122,1269,3772,3896,136,375,4425,0,0,4425,0,0,4304,59,188,4116,3152,3,52288,"FO2","GT" 23,42,1,4,2,137,41,"PENNSYLVANIA PWR & LGT CO","WEST SHORE",0,"LIGHT OIL",14715,"0M",1294,,,95,0,0,1981,146,397,2124,0,0,2125,23,63,2063,0,0,2063,27,85,2157,93,275,2060,1581,3944,1664,97,247,1948,0,0,1948,0,0,1943,0,0,1936,3154,3,52288,"FO2","GT" 23,42,1,4,2,137,42,"PENNSYLVANIA PWR & LGT CO","WILLIAMPORT",0,"LIGHT OIL",14715,"0M",1294,,,95,11,25,2095,108,303,2299,33,89,2120,24,80,2130,0,0,1062,31,83,2085,166,469,2282,1685,4637,1796,229,615,2348,0,1,2347,0,0,2347,47,129,2218,3155,3,52288,"FO2","GT" 23,42,1,2,4,137,44,"PENNSYLVANIA PWR & LGT CO","COAL STORAG",0,"ANTH COAL",14715,"0M",1294,,,95,0,0,4326102,0,0,4287048,0,0,4250306,0,0,4192077,0,0,4116068,0,0,4024607,0,0,3949307,0,0,3858966,0,0,3770991,0,0,3712178,0,0,3655315,0,0,3627389,8805,3,52288,"ANT","ST" 23,42,1,2,1,144,1,"PECO ENERGY CO","LIMERICK",0,"NUCLEAR",14940,"0M",1294,,260,95,758738,0,0,649503,0,0,788638,0,0,741991,0,0,644273,0,0,749037,0,0,735331,0,0,472319,0,0,293869,0,0,781359,0,0,758883,0,0,774008,0,0,6105,3,52304,"UR","ST" 23,42,1,2,1,144,2,"PECO ENERGY CO","LIMERICK",0,"NUCLEAR",14940,"0M",1294,,260,95,305997,0,0,145495,0,0,841460,0,0,792169,0,0,828631,0,0,759339,0,0,812705,0,0,648469,0,0,793584,0,0,839715,0,0,794719,0,0,838665,0,0,6105,3,52304,"UR","ST" 23,42,1,2,1,144,2,"PECO ENERGY CO","PEACHBOTTOM",0,"NUCLEAR",14940,"0M",1294,,260,95,835865,0,0,758077,0,0,833805,0,0,783656,0,0,813085,0,0,767048,0,0,814131,0,0,781700,0,0,787889,0,0,812587,0,0,755502,0,0,620649,0,0,3166,3,52304,"UR","ST" 23,42,1,1,,144,3,"PECO ENERGY CO","MUDDY RUN",0,"P-PUMPSTG",14940,"0M",1294,,260,95,-58588,197635,0,-48050,161907,0,-57936,201052,0,-62063,184331,0,-54454,193555,0,-64502,219733,0,-77254,238571,0,-71435,248510,0,-71632,228867,0,-151911,225998,0,-140643,200522,0,-140747,207063,0,3164,3,52304,"WAT","HY" 23,42,1,2,1,144,3,"PECO ENERGY CO","PEACHBOTTOM",0,"NUCLEAR",14940,"0M",1294,,260,95,777483,0,0,711496,0,0,640321,0,0,740258,0,0,699846,0,0,588449,0,0,497410,0,0,423621,0,0,284823,0,0,314451,0,0,800042,0,0,695148,0,0,3166,3,52304,"UR","ST" 23,42,1,4,2,144,10,"PECO ENERGY CO","CHESTER",0,"LIGHT OIL",14940,"0M",1294,,260,95,40,143,6303,283,871,5973,4,13,5960,0,0,5960,0,0,5960,134,251,5709,1965,3097,5088,2547,9094,4622,135,622,5417,6,46,5371,9,117,5615,0,0,5615,3157,3,52304,"FO2","GT" 23,42,1,2,2,144,18,"PECO ENERGY CO","CROMBY",0,"LIGHT OIL",14940,"0M",1294,,260,95,552,1065,739,136,247,742,559,972,675,596,1108,639,800,1555,694,542,1023,717,107,204,786,442,846,656,532,1027,700,390,751,648,1349,2625,514,669,1263,679,3159,3,52304,"FO2","ST" 23,42,1,2,3,144,18,"PECO ENERGY CO","CROMBY",0,"HEAVY OIL",14940,"0M",1294,,260,95,2359,4204,37192,40300,66566,38230,6132,9753,28477,2439,4170,38531,1755,3147,35384,2326,3992,31392,2427,4219,27173,2684,4698,32767,5362,9562,23250,2962,5168,40075,2887,5164,35070,3164,5422,36172,3159,3,52304,"FO6","ST" 23,42,1,2,6,144,18,"PECO ENERGY CO","CROMBY",0,"BIT COAL",14940,"0M",1294,,260,95,74489,31603,37801,84553,33984,30569,59404,28393,32942,68130,28446,39783,56042,24391,55616,62095,25757,51736,68743,28828,37015,81385,34554,29542,73288,31653,35675,82081,34906,31898,75734,32689,34891,88164,36436,31030,3159,3,52304,"BIT","ST" 23,42,1,2,9,144,18,"PECO ENERGY CO","CROMBY",0,"NAT GAS",14940,"0M",1294,,260,95,71643,785884,0,61834,634083,0,79727,785913,0,51172,541950,0,54177,597370,0,81502,865110,0,111181,1192120,0,110008,1192120,0,68568,752990,0,0,0,0,0,0,0,69,740,0,3159,3,52304,"NG","ST" 23,42,1,3,2,144,18,"PECO ENERGY CO","CROMBY",0,"LIGHT OIL",14940,"0M",1294,,260,95,0,0,425,2,5,382,1,2,380,1,3,377,0,0,377,0,1,376,6,13,363,0,0,363,2,5,358,0,0,358,3,6,352,0,0,352,3159,3,52304,"FO2","IC" 23,42,1,2,2,144,20,"PECO ENERGY CO","DELAWARE",0,"LIGHT OIL",14940,"0M",1294,,260,95,83,167,285,230,443,159,379,1037,262,0,1258,270,63,112,285,407,948,313,503,939,296,248,512,251,125,311,303,0,535,306,0,1886,292,1548,3097,274,3160,3,52304,"FO2","ST" 23,42,1,2,3,144,20,"PECO ENERGY CO","DELAWARE",0,"HEAVY OIL",14940,"0M",1294,,260,95,7566,13842,54536,40968,72617,57755,6149,15501,61363,-988,853,60510,1023,1674,58836,10372,22370,60784,73226,125872,59240,61586,116298,48551,3817,8670,64382,-880,0,64382,-848,109,64273,42071,77005,46160,3160,3,52304,"FO6","ST" 23,42,1,3,2,144,20,"PECO ENERGY CO","DELAWARE",0,"LIGHT OIL",14940,"0M",1294,,260,95,4,8,0,6,12,0,0,0,0,8,4,0,0,0,0,0,0,0,0,0,0,5,12,0,0,0,0,0,0,0,3,6,0,0,0,0,3160,3,52304,"FO2","IC" 23,42,1,4,2,144,20,"PECO ENERGY CO","DELAWARE",0,"LIGHT OIL",14940,"0M",1294,,260,95,14,29,4606,471,908,4510,16,46,5120,42,103,4834,0,0,5221,137,321,4998,1693,3157,5919,4022,8277,4823,175,434,5097,11,64,4495,0,0,4139,3,6,3960,3160,3,52304,"FO2","GT" 23,42,1,2,2,144,23,"PECO ENERGY CO","EDDYSTONE",0,"LIGHT OIL",14940,"0M",1294,,260,95,2860,5785,8309,7265,14150,6730,691,1392,5338,656,1353,6842,1090,2439,5446,1497,2992,3502,265,545,7647,1122,2234,5367,200,403,4943,1397,2645,5855,940,1740,11279,4634,8834,12016,3161,3,52304,"FO2","ST" 23,42,1,2,3,144,23,"PECO ENERGY CO","EDDYSTONE",0,"HEAVY OIL",14940,"0M",1294,,260,95,28189,52308,219884,149450,269038,232369,3289,6168,226201,212,405,225796,779,1602,224194,12605,22920,225716,34139,63954,190796,58828,107390,228949,6004,24353,228406,13370,23208,205198,25814,43623,161575,159697,281810,186014,3161,3,52304,"FO6","ST" 23,42,1,2,6,144,23,"PECO ENERGY CO","EDDYSTONE",0,"BIT COAL",14940,"0M",1294,,260,95,230611,102377,114701,145600,63304,115351,142036,63132,95986,141196,64796,114142,75987,37394,136129,72749,31969,156190,38241,17251,161746,115645,50809,196139,101095,70609,237844,255413,106924,214128,279475,114586,204428,343647,144382,154263,3161,3,52304,"BIT","ST" 23,42,1,2,9,144,23,"PECO ENERGY CO","EDDYSTONE",0,"NAT GAS",14940,"0M",1294,,260,95,44577,509816,0,75572,836629,0,64058,732536,0,42770,502085,0,37425,473140,0,199205,2238826,0,248894,2876189,0,290649,3273871,0,116178,2028607,0,136486,1466691,0,26917,282787,0,17773,193338,0,3161,3,52304,"NG","ST" 23,42,1,4,2,144,23,"PECO ENERGY CO","EDDYSTONE",0,"LIGHT OIL",14940,"0M",1294,,260,95,88,179,7824,301,588,7236,23,47,7189,0,0,7189,59,133,7056,38,77,6979,2082,4276,7703,5802,11553,9393,213,2838,8159,40,77,8082,74,138,7944,162,310,8951,3161,3,52304,"FO2","GT" 23,42,1,2,3,144,25,"PECO ENERGY CO","OIL STORAGE",0,"HEAVY OIL",14940,"0M",1294,,260,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,8806,3,52304,"FO6","ST" 23,42,1,4,2,144,26,"PECO ENERGY CO","FALLS",0,"LIGHT OIL",14940,"0M",1294,,260,95,6,16,10772,174,460,10312,0,0,10312,0,0,10312,0,0,10312,323,626,9686,1716,2316,9307,2167,6952,8374,53,261,8289,8,112,8177,0,0,8503,0,0,8503,3162,3,52304,"FO2","GT" 23,42,1,4,2,144,27,"PECO ENERGY CO","MOSER",0,"LIGHT OIL",14940,"0M",1294,,260,95,62,154,10920,416,1304,10329,2,7,10322,0,0,10322,0,0,10322,174,159,10163,2401,3681,8582,3033,9617,8076,165,385,7691,0,0,7691,49,1948,8854,0,0,8854,3163,3,52304,"FO2","GT" 23,42,1,4,2,144,30,"PECO ENERGY CO","RICHMOND",0,"LIGHT OIL",14940,"0M",1294,,260,95,73,705,25225,1538,2518,24154,176,209,23945,0,0,23945,0,0,23945,546,1092,22853,7883,15050,19654,8358,22812,19604,1489,4282,16208,573,1391,19605,1780,4530,22192,2646,5558,20232,3168,3,52304,"FO2","GT" 23,42,1,2,2,144,35,"PECO ENERGY CO","SCHUYLKILL",0,"LIGHT OIL",14940,"0M",1294,,260,95,10,31,177,29,55,282,0,13,330,0,0,58,5,32,173,21,41,260,32,63,204,31,64,224,0,0,285,0,0,204,0,13,117,174,366,292,3169,3,52304,"FO2","ST" 23,42,1,2,3,144,35,"PECO ENERGY CO","SCHUYLKILL",0,"HEAVY OIL",14940,"0M",1294,,260,95,2569,7049,0,27433,47982,0,-514,221,0,-442,0,0,787,4441,0,7540,12988,0,45149,79435,0,40737,74952,0,2171,4408,0,-450,0,0,-487,0,0,33696,64594,0,3169,3,52304,"FO6","ST" 23,42,1,3,2,144,35,"PECO ENERGY CO","SCHUYLKILL",0,"LIGHT OIL",14940,"0M",1294,,260,95,0,0,0,11,21,0,1,6,0,0,0,0,0,0,0,0,0,0,0,0,0,4,9,0,2,8,0,0,0,0,0,0,0,0,0,0,3169,3,52304,"FO2","IC" 23,42,1,4,2,144,35,"PECO ENERGY CO","SCHUYLKILL",0,"LIGHT OIL",14940,"0M",1294,,260,95,0,0,4077,183,347,4272,0,0,4454,0,0,4454,16,102,4352,25,48,4304,1060,2033,4025,3086,6214,3655,57,113,3542,0,0,3542,0,0,4435,0,0,4435,3169,3,52304,"FO2","GT" 23,42,1,4,2,144,39,"PECO ENERGY CO","SOUTHWARK",0,"LIGHT OIL",14940,"0M",1294,,260,95,7,10,6164,245,786,6101,28,123,5978,0,0,5978,0,0,5978,21,33,5945,2299,3702,5765,2572,9427,4876,120,646,4593,9,18,4592,0,0,5461,12,32,5429,3170,3,52304,"FO2","GT" 23,42,1,4,2,144,62,"PECO ENERGY CO","CROYDON",0,"LIGHT OIL",14940,"0M",1294,,260,95,908,1378,96105,5368,13129,82976,1206,2774,80202,185,1674,78528,-30,449,78079,2904,7166,70913,28748,58359,102954,34047,90855,75978,5816,17011,58967,4006,14190,124677,9344,33758,90919,20108,59103,81811,8012,3,52304,"FO2","GT" 23,42,1,1,,166,1,"SAFE HARBOR WATERPOWER CO","SAFE HARBOR",0,,16537,"0M",1294,,,95,143384,0,0,59393,0,0,126476,0,0,89759,0,0,63828,0,0,55553,0,0,43077,0,0,14256,0,0,7655,0,0,60191,0,0,112079,0,0,82918,0,0,3175,3,52553,"WAT","HY" 23,42,1,2,2,182,5,"UNITED GAS IMP CO (THE)","HUNLOCK CRK",0,"LIGHT OIL",19390,"0M",1294,,,95,513,820,149,94,161,167,202,328,185,435,618,244,11,18,226,1,2,224,140,230,170,0,0,170,514,892,135,73,127,175,21,35,140,24,41,99,3176,3,52988,"FO2","ST" 23,42,1,2,4,182,5,"UNITED GAS IMP CO (THE)","HUNLOCK CRK",0,"ANTH COAL",19390,"0M",1294,,,95,22922,15408,12384,27213,18489,14764,29884,19399,26578,8930,5383,44202,31976,21379,41110,31087,20919,40663,28632,19193,37106,32217,21657,39145,28079,19274,38194,32138,21308,38517,32139,20464,33331,30924,20327,26649,3176,3,52988,"ANT","ST" 23,42,1,2,2,187,1,"WEST PENN POWER CO","ARMSTRONG",0,"LIGHT OIL",20387,"0M",1294,,71,95,1137,2044,435,250,438,461,208,349,465,208,340,516,357,602,494,249,434,577,87,154,405,77,134,448,175,297,469,719,1212,478,755,1324,33,100,171,531,3178,1,54030,"FO2","ST" 23,42,1,2,6,187,1,"WEST PENN POWER CO","ARMSTRONG",0,"BIT COAL",20387,"0M",1294,,71,95,116602,48997,133134,169087,69152,118235,94695,37329,143043,106738,41224,154005,90547,35992,160453,93589,37605,145126,109058,44341,133889,108429,43934,141795,50453,20094,155423,132983,52637,143306,163282,66595,118118,227115,90923,97838,3178,1,54030,"BIT","ST" 23,42,1,2,2,187,5,"WEST PENN POWER CO","HATFIELD",0,"LIGHT OIL",20387,"0M",1294,,71,95,431,715,4466,429,677,4860,16,26,4860,109,176,5175,295,498,4642,232,393,4202,112,193,4003,116,200,3858,440,729,3846,625,1001,3653,200,324,4266,345,551,4530,3179,1,54030,"FO2","ST" 23,42,1,2,6,187,5,"WEST PENN POWER CO","HATFIELD",0,"BIT COAL",20387,"0M",1294,,71,95,924993,349235,573422,796344,286253,580468,654622,239981,562743,652050,240234,569141,751057,287421,561772,807472,310567,503117,873489,338429,425399,814220,315517,429242,611272,228129,438816,665375,244419,472140,717809,264457,471668,976850,352523,470255,3179,1,54030,"BIT","ST" 23,42,1,2,2,187,15,"WEST PENN POWER CO","MITCHELL",0,"LIGHT OIL",20387,"0M",1294,,71,95,1099,1660,62781,14264,26130,36652,9573,16358,20294,0,0,95,0,0,20294,0,0,20294,2975,5533,14761,9534,17307,37248,0,0,37248,370,623,36693,0,0,102,0,0,36712,3181,1,54030,"FO2","ST" 23,42,1,2,6,187,15,"WEST PENN POWER CO","MITCHELL",0,"BIT COAL",20387,"0M",1294,,71,95,133543,54702,81824,96423,41467,82859,153555,62524,77796,125039,49503,90740,49588,20363,93045,53622,23986,82955,92131,39751,72392,131370,55646,87997,44218,20045,99480,112797,45127,97501,86006,35430,95483,91125,37261,96203,3181,1,54030,"BIT","ST" 23,42,1,2,9,187,15,"WEST PENN POWER CO","MITCHELL",0,"NAT GAS",20387,"0M",1294,,71,95,997,8782,0,512,5468,0,649,6574,0,362,3518,0,98,1012,0,493,5639,0,384,4175,0,352,3732,0,608,6884,0,229,2287,0,632,6538,0,411,4215,0,3181,1,54030,"NG","ST" 23,42,1,2,3,187,25,"WEST PENN POWER CO","SPRINGDALE",0,"HEAVY OIL",20387,"0M",1294,"S",71,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,3182,1,54030,"FO6","ST" 23,42,8,1,,800,5,"ALLEGHENY ELECTRIC COOP","RAYSTOWN",0,,332,"0A",1294,,,95,10581,0,0,4872,0,0,10420,0,0,7145,0,0,9214,0,0,7292,0,0,7823,0,0,1871,0,0,1862,0,0,6232,0,0,13092,0,0,11263,0,0,7128,1,58500,"WAT","HY" 31,39,1,2,2,30,5,"CARDINAL OPERATING CO","CARDINAL",0,"LIGHT OIL",3006,"0M",1294,,365,95,1506,2512,16004,1987,3269,21891,793,1326,20561,810,1358,18998,750,1207,17783,5623,9537,7493,587,994,18460,1462,2531,15746,996,1682,14054,1293,2176,11850,586,984,10858,3751,6207,17605,2828,1,50359,"FO2","ST" 31,39,1,2,6,30,5,"CARDINAL OPERATING CO","CARDINAL",0,"BIT COAL",3006,"0M",1294,,365,95,964403,385031,651565,952635,371878,631820,970861,386058,589923,907026,357640,591393,523077,201759,670651,745173,300966,631446,1013299,410501,467099,1010121,415926,370224,984185,397240,345127,996339,400914,397108,987234,392815,487317,940659,377797,434608,2828,1,50359,"BIT","ST" 31,39,1,4,2,43,1,"CINCINNATI GAS ELEC CO","DICKS CREEK",0,"LIGHT OIL",3542,"0M",1294,,210,95,20,1175,6144,23,332,5811,9,35,5776,18,399,5377,0,0,5377,10,47,5330,233,987,4343,377,1342,3001,3,41,5373,8,49,5325,18,65,5260,1,7,5253,2831,1,50556,"FO2","GT" 31,39,1,4,9,43,1,"CINCINNATI GAS ELEC CO","DICKS CREEK",0,"NAT GAS",3542,"0M",1294,,210,95,74,4943,0,-217,0,0,17,13,0,-138,563,0,-109,0,0,227,871,0,3843,78877,0,4803,89226,0,-34,0,0,-101,1423,0,240,6693,0,672,17724,0,2831,1,50556,"NG","GT" 31,39,1,2,2,43,2,"CINCINNATI GAS ELEC CO","WC BECKJORD",0,"LIGHT OIL",3542,"0M",1294,,210,95,1063,1868,0,520,909,0,1246,2193,0,616,1040,0,909,1575,0,1694,2920,0,83,148,0,648,1175,0,673,1200,0,1185,2032,0,1335,2313,0,1124,2076,0,2830,1,50556,"FO2","ST" 31,39,1,2,6,43,2,"CINCINNATI GAS ELEC CO","WC BECKJORD",0,"BIT COAL",3542,"0M",1294,,210,95,376000,158991,137317,393834,167236,139827,297378,127194,171002,437582,181317,177440,274678,116442,192793,481664,200911,197721,528583,228082,195580,602321,260506,195850,213081,91113,206835,487454,202145,200676,427365,176777,196004,493746,218176,193234,2830,1,50556,"BIT","ST" 31,39,1,4,2,43,2,"CINCINNATI GAS ELEC CO","WC BECKJORD",0,"LIGHT OIL",3542,"0M",1294,,210,95,904,1589,30711,253,443,29179,30,54,26769,24,41,25499,30,53,23746,206,356,41971,10845,19305,22349,18056,32731,31385,523,933,29084,23,40,26796,38,67,23956,1551,2863,41821,2830,1,50556,"FO2","GT" 31,39,1,2,2,43,5,"CINCINNATI GAS ELEC CO","MIAMI FORT",0,"LIGHT OIL",3542,"0M",1294,,210,95,1008,1795,0,465,820,0,830,1457,0,436,757,0,862,1538,0,1665,3001,0,1804,3164,0,3368,6051,0,1292,2324,0,260,450,0,548,956,0,3202,5528,0,2832,1,50556,"FO2","ST" 31,39,1,2,6,43,5,"CINCINNATI GAS ELEC CO","MIAMI FORT",0,"BIT COAL",3542,"0M",1294,,210,95,637745,262491,294369,502865,207419,302760,559242,231277,318869,305741,124954,357678,414341,174583,369622,502174,211728,359534,599203,248510,325680,672906,285623,264937,557339,235511,249465,607306,250021,246891,553335,226505,248836,594845,241403,260437,2832,1,50556,"BIT","ST" 31,39,1,4,2,43,5,"CINCINNATI GAS ELEC CO","MIAMI FORT",0,"LIGHT OIL",3542,"0M",1294,,210,95,184,328,29994,104,184,28839,51,90,27190,104,182,26060,90,161,23971,260,470,20424,2604,4567,34307,5930,10654,29284,0,0,26912,56,98,26221,132,231,25022,4,7,19483,2832,1,50556,"FO2","GT" 31,39,1,2,2,43,10,"CINCINNATI GAS ELEC CO","W H ZIMMER",0,"LIGHT OIL",3542,"0M",1294,,210,95,387,627,43117,405,662,42455,266,437,42018,446,721,41297,544,908,40390,5437,9067,40610,3869,6259,34351,2406,3947,30404,654,1074,29331,0,0,28641,10375,17945,31644,228,326,31318,6019,1,50556,"FO2","ST" 31,39,1,2,6,43,10,"CINCINNATI GAS ELEC CO","W H ZIMMER",0,"BIT COAL",3542,"0M",1294,,210,95,945287,364436,470303,860575,334587,468422,931671,360276,429932,905494,345488,449089,895923,353208,433131,685071,269191,462164,813824,313887,471999,817013,315668,465279,858265,326707,439814,-6015,0,440306,643755,258809,446427,954218,369625,445092,6019,1,50556,"BIT","ST" 31,39,1,4,2,43,15,"CINCINNATI GAS ELEC CO","WOODSDALE",0,"PROPANE",3542,"0M",1294,,210,95,3264,17257,47281,251,6836,40445,206,1875,39359,655,3378,35981,0,2040,33941,765,1976,31965,599,1450,30515,128,307,30208,2,8,30200,22,122,30078,2291,8079,47000,9027,29590,47410,7158,1,50556,"FO2","GT" 31,39,1,4,9,43,15,"CINCINNATI GAS ELEC CO","WOODSDALE",0,"NAT GAS",3542,"0M",1294,,210,95,150,4500,0,6,900,0,329,16900,0,549,16100,0,-24,5400,0,8444,123700,0,78223,1073891,0,127374,1732000,0,11241,209600,0,798,24900,0,8079,161217,0,5288,98400,0,7158,1,50556,"NG","GT" 31,39,1,2,1,47,1,"CLEVELAND ELEC ILLUM CO","PERRY",0,"NUCLEAR",3755,"0M",1294,,,95,876776,0,0,768903,0,0,819283,0,0,488364,0,0,856246,0,0,825532,0,0,844484,0,0,836109,0,0,563058,0,0,867378,0,0,562127,0,0,802040,0,0,6020,1,50587,"UR","ST" 31,39,1,2,2,47,5,"CLEVELAND ELEC ILLUM CO","ASHTABULA",0,"LIGHT OIL",3755,"0M",1294,,,95,42,104,847,0,0,847,118,290,165,18,45,836,36,88,1105,993,2435,781,1126,2764,920,735,1805,1069,508,1246,1250,554,1359,961,372,912,1126,318,78,1063,2835,1,50587,"FO2","ST" 31,39,1,2,6,47,5,"CLEVELAND ELEC ILLUM CO","ASHTABULA",0,"BIT COAL",3755,"0M",1294,,,95,52796,31491,71024,49964,29829,71024,55761,34212,70589,75864,42918,70589,57256,34078,70589,75393,41494,70589,152351,73482,69602,185535,87655,62911,92554,48842,63273,134786,62671,50375,152108,70363,39853,183631,84228,39391,2835,1,50587,"BIT","ST" 31,39,1,2,2,47,10,"CLEVELAND ELEC ILLUM CO","AVON",0,"LIGHT OIL",3755,"0M",1294,,,95,545,1336,12357,217,533,11823,334,820,11003,71,175,13126,623,1529,11274,103,252,10337,204,501,9328,209,514,12564,219,537,11551,455,1117,10529,439,1076,9330,211,518,8657,2836,1,50587,"FO2","ST" 31,39,1,2,6,47,10,"CLEVELAND ELEC ILLUM CO","AVON",0,"BIT COAL",3755,"0M",1294,,,95,418792,166008,147432,412531,162705,122460,424163,169344,131476,363532,138488,180398,251231,98651,203325,203947,82859,218224,353614,137703,162497,424161,173437,95914,388690,173071,75855,373672,144052,89758,227150,92153,101135,197850,84233,81208,2836,1,50587,"BIT","ST" 31,39,1,4,2,47,10,"CLEVELAND ELEC ILLUM CO","AVON",0,"LIGHT OIL",3755,"0M",1294,,,95,-48,0,1833,46,308,1525,-44,0,1525,16,93,1432,-27,0,1432,51,171,1260,97,283,1453,726,2175,826,-20,0,1302,-23,0,1326,-40,0,1326,-55,0,1861,2836,1,50587,"FO2","GT" 31,39,1,2,2,47,15,"CLEVELAND ELEC ILLUM CO","EASTLAKE",0,"LIGHT OIL",3755,"0M",1294,,,95,1497,3674,9572,911,2234,8964,764,1874,9624,751,1842,8674,1166,2861,7850,1418,3479,8310,853,2092,5787,966,2369,13472,911,2234,13178,758,1860,11437,682,1673,13358,1121,2750,10965,2837,1,50587,"FO2","ST" 31,39,1,2,6,47,15,"CLEVELAND ELEC ILLUM CO","EASTLAKE",0,"BIT COAL",3755,"0M",1294,,,95,563066,214828,125324,531721,201833,127529,552063,214200,127558,603752,229103,113946,476696,183152,148312,528305,201681,134280,545020,211638,133115,580108,227637,126504,418750,164875,155538,237147,95621,161064,619540,234785,116588,554005,216330,121544,2837,1,50587,"BIT","ST" 31,39,1,4,2,47,15,"CLEVELAND ELEC ILLUM CO","EASTLAKE",0,"LIGHT OIL",3755,"0M",1294,,,95,-26,411,1392,-34,64,1328,-7,96,1232,-39,0,1232,-17,48,1184,80,272,913,110,487,2330,416,1227,1642,-21,0,1642,-29,0,1642,-48,0,1642,-62,0,1642,2837,1,50587,"FO2","GT" 31,39,1,2,2,47,20,"CLEVELAND ELEC ILLUM CO","LAKE SHORE",0,"LIGHT OIL",3755,"0M",1294,,,95,1807,4433,0,1095,2687,0,655,1878,10867,822,2016,9030,822,2016,9030,822,2016,9030,822,2016,9030,0,0,9030,0,0,9030,0,0,9030,0,0,9030,0,0,9030,2838,1,50587,"FO2","ST" 31,39,1,2,3,47,20,"CLEVELAND ELEC ILLUM CO","LAKE SHORE",0,"HEAVY OIL",3755,"0M",1294,,,95,-1345,0,0,-1121,0,0,-1101,0,0,-967,0,0,-1013,0,0,-1144,0,0,-1177,0,0,-1109,0,0,-1101,0,0,-886,0,0,-1113,0,0,-1190,0,0,2838,1,50587,"FO6","ST" 31,39,1,2,6,47,20,"CLEVELAND ELEC ILLUM CO","LAKE SHORE",0,"BIT COAL",3755,"0M",1294,,,95,-2869,0,0,-2051,0,0,-8655,0,0,-1765,0,0,-1630,0,0,-1592,0,0,-1511,0,0,-680,0,0,-664,0,0,-785,0,0,-839,0,0,-939,0,0,2838,1,50587,"BIT","ST" 31,39,1,3,2,47,20,"CLEVELAND ELEC ILLUM CO","LAKE SHORE",0,"LIGHT OIL",3755,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2838,1,50587,"FO2","IC" 31,39,1,2,2,50,5,"COLUMBUS SOUTHERN PWR CO","CONESVILLE",0,"LIGHT OIL",4062,"0M",1294,,369,95,781,1346,11167,848,1487,10088,1527,2569,9973,647,1108,10480,1150,1863,10818,808,1412,11137,1992,3195,10638,911,1520,12206,2980,5206,7444,848,1360,7419,1411,2362,6092,1247,2194,6515,2840,1,50633,"FO2","ST" 31,39,1,2,6,50,5,"COLUMBUS SOUTHERN PWR CO","CONESVILLE",0,"BIT COAL",4062,"0M",1294,,369,95,839897,361439,480236,776708,341510,409270,577474,241703,450938,516809,220156,545479,471259,188870,589930,540735,233443,590510,666114,292069,537443,960463,414977,380548,748475,319718,311923,775359,307972,333993,824448,339869,356943,594247,257598,411899,2840,1,50633,"BIT","ST" 31,39,1,2,2,50,15,"COLUMBUS SOUTHERN PWR CO","PICWAY",0,"LIGHT OIL",4062,"0M",1294,,369,95,77,157,318,80,151,162,0,0,158,0,0,163,0,0,150,271,581,410,67,164,258,153,329,279,86,168,293,52,109,355,102,206,330,71,149,354,2843,1,50633,"FO2","ST" 31,39,1,2,6,50,15,"COLUMBUS SOUTHERN PWR CO","PICWAY",0,"BIT COAL",4062,"0M",1294,,369,95,24098,12576,18902,17338,8355,10547,0,0,10547,0,0,10547,0,0,10547,12062,7059,8508,8499,5099,16411,33626,17892,7051,12493,6357,14305,11264,6148,20174,12256,6425,23762,14575,8110,25135,2843,1,50633,"BIT","ST" 31,39,1,3,2,56,15,"DAYTON PWR & LGT CO (THE)","FRANK TAIT",0,"LIGHT OIL",4922,"0M",1294,,,95,10,18,2118,30,55,1880,24,44,4879,67,123,5809,5,9,5601,0,0,8437,59,128,8308,638,1170,6968,8,15,6953,0,0,6953,4,31,12908,0,0,12704,2847,1,50752,"FO2","IC" 31,39,1,4,2,56,15,"DAYTON PWR & LGT CO (THE)","FRANK TAIT",0,"LIGHT OIL",4922,"0M",494,,,95,0,0,0,0,0,0,0,0,0,8,31,0,2615,5585,0,2094,4660,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,87,204,0,2847,1,50752,"FO2","GT" 31,39,1,4,9,56,15,"DAYTON PWR & LGT CO (THE)","FRANK TAIT",0,"NAT GAS",4922,"0M",494,,,95,0,0,0,0,0,0,0,0,0,206,4610,0,2453,30366,0,2250,29020,0,2757,33743,0,5899,80360,0,392,7740,0,65,1370,0,35,1210,0,1279,17010,0,2847,1,50752,"NG","GT" 31,39,1,2,6,56,20,"DAYTON PWR & LGT CO (THE)","HUTCHINGS",0,"BIT COAL",4922,"0M",1294,,,95,1189,1204,103680,11354,5882,97799,-864,0,97799,0,0,97799,-467,0,97799,38657,18515,85185,73119,34885,59277,140943,65371,20520,7427,3975,45638,4351,2521,84275,3553,2065,93826,62576,27616,66210,2848,1,50752,"BIT","ST" 31,39,1,2,9,56,20,"DAYTON PWR & LGT CO (THE)","HUTCHINGS",0,"NAT GAS",4922,"0M",1294,,,95,408,9899,0,595,6448,0,0,0,0,-804,48,0,4,164,0,1487,14801,0,2254,22264,0,5404,59821,0,688,9010,0,440,6133,0,353,5099,0,1464,15898,0,2848,1,50752,"NG","ST" 31,39,1,4,2,56,20,"DAYTON PWR & LGT CO (THE)","HUTCHINGS",0,"LIGHT OIL",4922,"0M",1294,,,95,71,303,1433,82,157,1275,0,1,1275,0,0,1275,0,0,1274,0,0,1274,0,0,1274,0,1,1274,0,0,1274,0,0,1274,58,147,1127,49,94,1395,2848,1,50752,"FO2","GT" 31,39,1,4,9,56,20,"DAYTON PWR & LGT CO (THE)","HUTCHINGS",0,"NAT GAS",4922,"0M",1294,,,95,0,10,0,0,0,0,5,1130,0,16,400,0,8,327,0,0,0,0,140,1384,0,423,4690,0,0,0,0,0,0,0,0,0,0,41,453,0,2848,1,50752,"NG","GT" 31,39,1,2,2,56,23,"DAYTON PWR & LGT CO (THE)","J M STUART",0,"LIGHT OIL",4922,"0M",1294,,,95,1332,2321,1749,646,1073,2134,623,1061,2140,1223,2081,1858,1631,2823,2062,975,1647,2197,223,358,2194,623,1047,2043,1054,1794,2183,2669,4498,2177,1035,1708,1924,2772,4191,2252,2850,1,50752,"FO2","ST" 31,39,1,2,6,56,23,"DAYTON PWR & LGT CO (THE)","J M STUART",0,"BIT COAL",4922,"0M",1294,,,95,1324209,556655,951299,1313535,540148,931841,981133,406226,1101726,963505,397393,1210633,1235488,518718,880851,1223521,506083,868835,1340550,537277,869585,1339861,554937,815555,984147,409972,981044,990034,409244,867049,1361690,549068,888832,1361213,508529,976472,2850,1,50752,"BIT","ST" 31,39,1,3,2,56,23,"DAYTON PWR & LGT CO (THE)","J M STUART",0,"LIGHT OIL",4922,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2850,1,50752,"FO2","IC" 31,39,1,4,2,56,28,"DAYTON PWR & LGT CO (THE)","YANKEE ST",0,"LIGHT OIL",4922,"0M",1294,,,95,392,1042,6368,143,449,7390,1,3,5791,0,0,5791,0,1,5790,0,2,5788,0,0,5788,0,2,6395,2,7,6388,0,1,6388,60,192,6195,298,738,6316,2854,1,50752,"FO2","GT" 31,39,1,4,9,56,28,"DAYTON PWR & LGT CO (THE)","YANKEE ST",0,"NAT GAS",4922,"0M",1294,,,95,10,160,0,62,1100,0,162,1963,0,84,1410,0,82,1499,0,110,1913,0,390,6135,0,2583,45005,0,16,299,0,118,2067,0,15,279,0,1,15,0,2854,1,50752,"NG","GT" 31,39,1,3,2,56,34,"DAYTON PWR & LGT CO (THE)","MONUMENT",0,"LIGHT OIL",4922,"0M",1294,,,95,48,88,666,38,70,596,24,44,749,8,15,735,20,37,698,0,0,698,0,0,698,868,1591,510,12,22,679,8,15,664,3,6,658,23,73,586,2851,1,50752,"FO2","IC" 31,39,1,3,2,56,38,"DAYTON PWR & LGT CO (THE)","SIDNEY",0,"LIGHT OIL",4922,"0M",1294,,,95,36,66,654,39,72,582,19,35,547,12,22,525,27,50,476,38,70,594,200,367,418,928,1701,298,12,22,467,14,26,441,11,20,599,27,50,550,2852,1,50752,"FO2","IC" 31,39,1,2,2,56,40,"DAYTON PWR & LGT CO (THE)","KILLEN",0,"LIGHT OIL",4922,"0M",1294,,,95,1515,2654,38401,2032,3512,34941,568,957,33906,811,1364,32383,2303,3935,28369,2103,3623,24697,1150,1949,22638,3905,6750,39224,3140,5527,33621,140,241,33352,1226,2214,31022,7796,9042,43816,6031,1,50752,"FO2","ST" 31,39,1,2,6,56,40,"DAYTON PWR & LGT CO (THE)","KILLEN",0,"BIT COAL",4922,"0M",1294,,,95,396655,162048,146219,299969,123570,141430,380134,154283,172985,326056,132202,166969,335211,138111,191956,337194,139038,170239,357281,145509,178055,407089,168349,129255,293108,123208,110897,435673,179182,98466,52201,22774,186101,115941,32572,227624,6031,1,50752,"BIT","ST" 31,39,1,2,2,133,10,"OHIO EDISON CO","EDGEWATER",0,"LIGHT OIL",13998,"0M",1294,"A",,95,0,0,0,0,0,0,255,723,33,159,366,33,0,0,0,308,793,33,68,152,33,5,124,33,27,86,33,7,17,33,1286,2860,33,3,6,33,2857,1,52154,"FO2","ST" 31,39,1,2,9,133,10,"OHIO EDISON CO","EDGEWATER",0,"NAT GAS",13998,"0M",394,,,95,0,0,0,0,0,0,7097,98907,0,15050,194824,0,0,0,0,5911,86537,0,13656,173637,0,24053,289252,0,13182,151945,0,7495,97750,0,13698,169535,0,9290,104799,0,2857,1,52154,"NG","ST" 31,39,1,4,2,133,10,"OHIO EDISON CO","EDGEWATER",0,"LIGHT OIL",13998,"0M",1294,,,95,39,51,10875,58,329,9555,-8,73,8938,-14,44,9839,0,0,9464,200,693,10736,984,3224,10487,1718,5378,9687,120,437,8935,-17,0,8918,15,18,8748,20,140,9834,2857,1,52154,"FO2","GT" 31,39,1,2,2,133,15,"OHIO EDISON CO","GORGE STEAM",0,"LIGHT OIL",13998,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2858,1,52154,"FO2","ST" 31,39,1,2,6,133,15,"OHIO EDISON CO","GORGE STEAM",0,"BIT COAL",13998,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2858,1,52154,"BIT","ST" 31,39,1,4,2,133,30,"OHIO EDISON CO","MAD RIVER",0,"LIGHT OIL",13998,"0M",1294,,,95,-78,0,15547,-26,273,15273,-54,0,15273,-54,0,15273,363,2822,15479,99,426,15053,1080,3857,14177,3295,9983,13051,179,602,14577,62,386,15260,60,421,14839,73,357,15562,2860,1,52154,"FO2","GT" 31,39,1,2,2,133,43,"OHIO EDISON CO","NILES",0,"LIGHT OIL",13998,"0M",1294,,,95,5,9,253,86,166,190,142,266,280,33,64,216,17,38,406,275,522,253,67,130,224,50,97,303,45,88,221,63,123,320,28,54,266,27,53,213,2861,1,52154,"FO2","ST" 31,39,1,2,6,133,43,"OHIO EDISON CO","NILES",0,"BIT COAL",13998,"0M",1294,,,95,123871,55965,73387,98573,45856,68795,100911,45527,84171,102317,46469,88241,6938,3797,109930,76341,34497,104722,105408,49207,76769,73326,33732,70283,103996,47562,47231,111221,52359,33613,108872,49872,33134,113766,51273,29923,2861,1,52154,"BIT","ST" 31,39,1,4,2,133,43,"OHIO EDISON CO","NILES",0,"LIGHT OIL",13998,"0M",1294,,,95,55,295,7474,75,333,7682,-36,56,7626,-41,0,7626,-25,30,7596,100,416,7180,647,2274,6851,1403,4579,5630,65,256,6970,-7,118,6852,3,124,6728,61,335,7293,2861,1,52154,"FO2","GT" 31,39,1,2,2,133,45,"OHIO EDISON CO","R E BURGER",0,"LIGHT OIL",13998,"0M",1294,,,95,101,204,570,57,119,629,70,132,675,95,173,502,63,117,562,95,188,374,81,156,558,51,100,633,44,83,549,46,91,458,2,3,632,119,296,336,2864,1,52154,"FO2","ST" 31,39,1,2,6,133,45,"OHIO EDISON CO","R E BURGER",0,"BIT COAL",13998,"0M",1294,,,95,220103,104240,157034,164294,78521,184267,126512,54034,193327,150997,63973,186573,81596,35961,201217,96775,43949,193287,127163,56391,181386,166656,74197,142563,130934,57102,99030,67387,30839,87088,93946,40429,64542,82572,48775,54306,2864,1,52154,"BIT","ST" 31,39,1,3,2,133,45,"OHIO EDISON CO","R E BURGER",0,"LIGHT OIL",13998,"0M",1294,,,95,7,10,1284,23,46,1417,9,11,1407,0,0,1407,0,0,1407,34,84,1323,236,429,1243,566,1044,904,17,35,1224,23,43,1181,0,0,1181,30,77,1647,2864,1,52154,"FO2","IC" 31,39,1,2,2,133,57,"OHIO EDISON CO","W H SAMMIS",0,"LIGHT OIL",13998,"0M",1294,,,95,1482,2546,867,528,903,1046,558,954,844,550,932,638,695,1199,912,544,955,1493,706,1274,1304,451,1354,1217,1142,2017,1181,1316,2293,1036,94,160,983,2104,3601,973,2866,1,52154,"FO2","ST" 31,39,1,2,6,133,57,"OHIO EDISON CO","W H SAMMIS",0,"BIT COAL",13998,"0M",1294,,,95,1276095,514756,525945,1279324,511426,457910,1239563,502275,472374,1278563,515393,459047,1160892,479648,563045,1211972,504994,605054,1203599,510803,549162,1367687,590999,470321,991825,414819,354704,1017793,422778,445492,1052538,422578,399901,1094820,447068,288610,2866,1,52154,"BIT","ST" 31,39,1,3,2,133,57,"OHIO EDISON CO","W H SAMMIS",0,"LIGHT OIL",13998,"0M",1294,,,95,21,47,2208,62,132,2422,24,52,2506,21,51,2619,18,49,2690,84,169,2569,424,916,2504,994,1895,1445,56,115,2687,17,62,1885,61,120,2363,49,78,2264,2866,1,52154,"FO2","IC" 31,39,1,5,2,133,80,"OHIO EDISON CO","W LORAIN JO",0,"LIGHT OIL",13998,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2869,1,52154,"FO2","CC" 31,39,1,6,2,133,80,"OHIO EDISON CO","W LORAIN JO",0,"LIGHT OIL",13998,"0M",1294,"A",,95,0,0,0,0,0,0,18,114,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2869,1,52154,"FO2","CT" 31,39,1,2,2,141,28,"OHIO POWER CO","MUSKINGUM R",0,"LIGHT OIL",14006,"0M",1294,,364,95,3882,6525,18086,2171,3713,17991,1663,2732,19038,2100,3500,20732,2616,4271,21458,2357,4274,22882,1323,2298,23072,3025,5284,24028,1082,2039,25141,1349,2367,24554,1527,2671,21638,6433,9974,10617,2872,1,54028,"FO2","ST" 31,39,1,2,6,141,28,"OHIO POWER CO","MUSKINGUM R",0,"BIT COAL",14006,"0M",1294,,364,95,535201,215186,421884,537048,220375,419768,597967,235236,427281,521184,207858,375208,449068,175136,430680,464394,194776,458208,580017,239178,402984,570215,237224,362814,265479,117802,367772,240284,100504,368567,286463,120853,342833,504050,190482,323803,2872,1,54028,"BIT","ST" 31,39,1,2,2,141,30,"OHIO POWER CO","GAVIN",0,"LIGHT OIL",14006,"0M",1294,,364,95,3763,6775,47403,769,1320,46083,4239,7491,38592,399,722,37870,719,1203,36667,2089,3543,33123,1042,1767,31357,1100,2128,29229,787,1372,39659,1447,2509,37150,1827,3076,34074,190,326,33748,8102,1,54028,"FO2","ST" 31,39,1,2,6,141,30,"OHIO POWER CO","GAVIN",0,"BIT COAL",14006,"0M",1294,,364,95,64858,30038,1931820,651490,284413,2186971,988276,436625,1888556,1196488,552083,1872871,1419448,615414,1838157,1182854,513910,1760692,1417031,613808,1615051,1643009,713610,1363516,1514789,657244,1159863,1269184,559173,1152059,1395530,601427,1176037,1375641,605361,1157372,8102,1,54028,"BIT","ST" 31,39,1,1,,141,35,"OHIO POWER CO","RACINE",0,,14006,"0M",1294,,364,95,18331,0,0,19396,0,0,21002,0,0,26318,0,0,19638,0,0,23776,0,0,16330,0,0,12023,0,0,7551,0,0,14526,0,0,23751,0,0,24817,0,0,6006,1,54028,"WAT","HY" 31,39,1,2,6,141,40,"OHIO POWER CO","TIDD",0,"BIT COAL",14006,"0M",1294,"S",364,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2874,1,54028,"BIT","ST" 31,39,1,2,2,147,1,"OHIO VALLEY ELEC CORP","KYGER CREEK",0,"LIGHT OIL",14015,"0M",1294,,506,95,214,364,1335,346,582,1079,478,772,930,80,131,1631,298,520,1248,203,342,1489,97,168,1464,0,0,1642,55,92,1550,582,973,577,236,390,1258,83,146,1373,2876,1,52156,"FO2","ST" 31,39,1,2,6,147,1,"OHIO VALLEY ELEC CORP","KYGER CREEK",0,"BIT COAL",14015,"0M",1294,,506,95,702913,271965,605907,555922,215202,643003,623778,230327,685798,645615,237897,675827,712862,278407,639864,676683,252935,580389,702720,270228,524058,722985,274975,470824,637930,231881,406765,609383,225508,431319,645928,235364,421426,715380,277692,649924,2876,1,52156,"BIT","ST" 31,39,1,2,1,168,1,"TOLEDO EDISON CO (THE)","DAVIS-BESSE",0,"NUCLEAR",18997,"0M",1294,,,95,658580,0,0,596841,0,0,657111,0,0,620608,0,0,643953,0,0,629968,0,0,645923,0,0,643124,0,0,630210,0,0,652469,0,0,633467,0,0,645496,0,0,6149,1,52927,"UR","ST" 31,39,1,2,2,168,9,"TOLEDO EDISON CO (THE)","ACME",0,"PROPANE",18997,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2877,1,52927,"FO2","ST" 31,39,1,2,6,168,9,"TOLEDO EDISON CO (THE)","ACME",0,"BIT COAL",18997,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2877,1,52927,"BIT","ST" 31,39,1,2,9,168,9,"TOLEDO EDISON CO (THE)","ACME",0,"NAT GAS",18997,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2877,1,52927,"NG","ST" 31,39,1,2,2,168,11,"TOLEDO EDISON CO (THE)","BAY SHORE",0,"LIGHT OIL",18997,"0M",1294,,,95,136,448,525,273,439,445,156,255,550,380,622,464,160,607,393,170,407,521,159,530,700,226,457,598,155,367,588,238,402,364,76,315,588,112,197,572,2878,1,52927,"FO2","ST" 31,39,1,2,6,168,11,"TOLEDO EDISON CO (THE)","BAY SHORE",0,"BIT COAL",18997,"0M",1294,,,95,271495,103216,169716,328463,121979,150035,259418,97335,167411,220548,81660,204738,228937,86543,252579,283830,108691,226673,265296,101256,155041,323077,180415,73781,309205,109740,75119,176674,67648,106761,254611,97258,111939,278242,107020,82847,2878,1,52927,"BIT","ST" 31,39,1,4,2,168,11,"TOLEDO EDISON CO (THE)","BAY SHORE",0,"LIGHT OIL",18997,"0M",1294,,,95,14,64,566,36,59,688,0,0,782,14,24,758,0,0,758,17,30,1086,46,267,997,175,646,886,8,62,825,2,5,820,0,19,979,1,53,926,2878,1,52927,"FO2","GT" 31,39,1,4,2,168,18,"TOLEDO EDISON CO (THE)","RICHLAND",0,"LIGHT OIL",18997,"0M",1294,,,95,0,40,2793,0,0,2793,0,0,2793,0,25,2768,0,3,2764,27,124,2641,49,260,2380,192,729,1652,0,0,1652,0,44,1607,0,0,2325,0,0,2325,2880,1,52927,"FO2","GT" 31,39,1,4,9,168,18,"TOLEDO EDISON CO (THE)","RICHLAND",0,"NAT GAS",18997,"0M",1294,,,95,0,276,0,0,594,0,0,324,0,0,621,0,0,756,0,25,675,0,71,2079,0,345,7385,0,0,215,0,0,3046,0,0,92,0,2,392,0,2880,1,52927,"NG","GT" 31,39,1,4,2,168,19,"TOLEDO EDISON CO (THE)","STRYKER",0,"LIGHT OIL",18997,"0M",1294,,,95,10,159,1191,0,0,1191,0,0,1191,0,0,1191,0,0,1191,0,0,1191,0,0,1191,0,8,1183,0,0,1183,16,41,1142,0,0,92,0,29,1113,2881,1,52927,"FO2","GT" 31,39,5,3,2,522,1,"ARCANUM (CITY OF)","ARCANUM",0,"LIGHT OIL",768,"0A",1294,,,95,27,51,203,49,90,186,15,31,155,4,8,148,3,5,143,17,33,110,14,27,82,52,101,101,4,8,93,3,6,87,4,13,74,8,21,171,2902,1,50096,"FO2","IC" 31,39,5,3,2,552,1,"BRYAN (CITY OF)","BRYAN",0,"LIGHT OIL",2439,"0M",1294,,,95,14,23,355,14,25,329,0,0,329,178,304,378,39,68,310,12,21,289,145,250,215,87,158,235,29,50,179,16,27,153,37,63,268,9,32,237,2903,1,50356,"FO2","IC" 31,39,5,4,2,552,1,"BRYAN (CITY OF)","BRYAN",0,"LIGHT OIL",2439,"0M",1294,,,95,22,50,6950,0,0,6950,2,156,6795,0,0,6790,0,0,6790,0,0,6790,0,0,6790,0,0,6790,0,0,6760,0,0,6720,6,12,6690,1,5,6682,2903,1,50356,"FO2","GT" 31,39,5,4,9,552,1,"BRYAN (CITY OF)","BRYAN",0,"NAT GAS",2439,"0M",1294,,,95,22,566,0,82,2330,0,0,0,0,254,4926,0,3992,62915,0,6018,86797,0,4936,89292,0,8968,190437,0,6094,104355,0,104,2299,0,132,2762,0,420,8161,0,2903,1,50356,"NG","GT" 31,39,5,4,2,561,2,"CLEVELAND (CITY OF)","COLLINWOOD",0,"LIGHT OIL",3762,"0M",1294,,,95,0,1,1070,0,4,1066,83,263,803,0,0,803,4,238,565,0,0,922,0,0,922,50,256,1022,0,0,1022,0,0,1022,0,0,1022,0,0,1022,2906,1,50589,"FO2","GT" 31,39,5,4,9,561,2,"CLEVELAND (CITY OF)","COLLINWOOD",0,"NAT GAS",3762,"0M",1294,,,95,27,729,0,0,0,0,1,32,0,0,33,0,0,0,0,674,8563,0,274,8962,0,32,941,0,17,380,0,0,3,0,0,7,0,0,4,0,2906,1,50589,"NG","GT" 31,39,5,2,2,561,10,"CLEVELAND (CITY OF)","LAKE ROAD",0,"LIGHT OIL",3762,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2908,1,50589,"FO2","ST" 31,39,5,2,6,561,10,"CLEVELAND (CITY OF)","LAKE ROAD",0,"BIT COAL",3762,"0M",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2908,1,50589,"BIT","ST" 31,39,5,4,2,561,20,"CLEVELAND (CITY OF)","W 41ST ST",0,"LIGHT OIL",3762,"0M",1294,,,95,0,1,1995,0,0,1994,0,0,1994,0,0,1993,0,0,1993,0,0,1992,0,1,1992,0,1,1991,0,0,1990,0,0,1990,0,1,1989,0,0,1989,2909,1,50589,"FO2","GT" 31,39,5,4,9,561,20,"CLEVELAND (CITY OF)","W 41ST ST",0,"NAT GAS",3762,"0M",1294,,,95,477,14950,0,526,10745,0,431,12673,0,247,6523,0,221,6443,0,340,8176,0,1197,15109,0,4074,94135,0,593,26459,0,537,13366,0,668,16240,0,628,17345,0,2909,1,50589,"NG","GT" 31,39,5,2,6,579,1,"DOVER (CITY OF)","DOVER",0,"BIT COAL",5336,"0M",1294,,,95,7510,5164,474,5838,3935,612,7700,4900,592,6987,4742,130,0,7,150,0,0,623,5223,3579,213,7330,5046,506,6122,4199,218,2658,1764,200,6852,5320,346,7262,4963,413,2914,1,50806,"BIT","ST" 31,39,5,2,9,579,1,"DOVER (CITY OF)","DOVER",0,"NAT GAS",5336,"0M",794,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,27,403,0,884,12716,0,410,6737,0,110,1163,0,663,9798,0,637,9130,0,2914,1,50806,"NG","ST" 31,39,5,3,2,579,1,"DOVER (CITY OF)","DOVER",0,"LIGHT OIL",5336,"0M",1294,,,95,0,0,66,0,0,66,4,9,61,0,0,66,0,0,57,18,228,79,36,74,109,29,75,101,0,0,101,0,0,101,0,0,101,0,0,101,2914,1,50806,"FO2","IC" 31,39,5,4,9,579,5,"DOVER (CITY OF)","DOVER",0,"NAT GAS",5336,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,65,1022,0,0,0,0,0,0,0,0,0,0,48,698,0,0,0,0,0,0,0,0,0,0,0,0,0,2914,1,50806,"NG","GT" 31,39,5,2,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT OIL",7977,"0M",1294,,,95,5,11,1751,1,3,1749,1,4,1747,1,5,1744,1,4,1743,4,10,1737,3,7,1734,4,9,1730,4,11,1724,1,4,1722,1,6,1719,7,16,1711,2917,1,51225,"FO2","ST" 31,39,5,2,6,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"BIT COAL",7977,"0M",1294,,,95,22703,11176,13737,252,146,15989,5474,3315,16142,8640,5428,12982,9803,5101,7881,11553,6584,1297,16363,9478,2000,22973,9375,5688,24478,13592,4621,4956,3752,6715,4870,4046,7024,23079,11772,7422,2917,1,51225,"BIT","ST" 31,39,5,2,9,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"NAT GAS",7977,"0M",1294,,,95,157,1874,0,13990,195116,0,5260,76784,0,483,7231,0,4563,57272,0,9310,123945,0,17338,207709,0,14384,141922,0,1816,24404,0,676,12116,0,270,5334,0,784,9339,0,2917,1,51225,"NG","ST" 31,39,5,4,2,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"LIGHT OIL",7977,"0M",1294,,,95,0,0,1751,0,0,1749,0,0,1748,0,0,1745,0,0,1742,0,0,1738,0,0,1735,0,0,1730,0,0,1725,0,0,1723,0,0,1719,0,0,1711,2917,1,51225,"FO2","GT" 31,39,5,4,9,605,1,"HAMILTON (CITY OF)","HAM MUN EL",0,"NAT GAS",7977,"0M",1294,,,95,11,142,0,174,2439,0,83,1220,0,26,393,0,18,234,0,55,745,0,1064,12754,0,1170,28673,0,18,250,0,134,2411,0,10,207,0,18,217,0,2917,1,51225,"NG","GT" 31,39,5,1,,605,5,"HAMILTON (CITY OF)","HMLTN HYDRO",0,,7977,"0M",1294,"R",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,7807,1,51225,"WAT","HY" 31,39,5,3,2,629,1,"LEBANON (CITY OF)","LEBANON",0,"LIGHT OIL",10830,"0M",1294,,,95,3,23,1067,0,0,1067,90,268,799,0,0,799,0,0,799,0,0,799,29,63,734,52,106,805,0,0,805,0,0,805,0,0,805,0,0,805,2921,1,51615,"FO2","IC" 31,39,5,4,2,629,1,"LEBANON (CITY OF)","LEBANON",0,"LIGHT OIL",10830,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2921,1,51615,"FO2","GT" 31,39,5,3,2,684,1,"OBERLIN (CITY OF)","OBERLIN",0,"LIGHT OIL",13949,"0A",1294,,,95,5,65,637,21,41,596,0,37,558,8,17,528,0,0,509,33,80,429,17,210,218,239,528,405,11,41,364,8,17,348,194,525,358,145,391,324,2933,1,52140,"FO2","IC" 31,39,5,3,9,684,1,"OBERLIN (CITY OF)","OBERLIN",0,"NAT GAS",13949,"0A",1294,,,95,275,2724,0,260,2802,0,5,1676,0,75,826,0,13,132,0,200,1734,0,339,3535,0,552,5958,0,39,487,0,82,884,0,969,9721,0,63,1533,0,2933,1,52140,"NG","IC" 31,39,5,2,6,689,1,"ORRVILLE (CITY OF)","ORRVILLE",0,"BIT COAL",14194,"0M",1294,,,95,30925,20332,2401,27128,23359,528,19190,7163,1721,22147,13962,524,29670,13038,1437,23583,15893,1741,24259,14697,2641,28372,19561,2485,22121,14691,1281,18235,13105,1557,28993,15643,959,24197,16177,783,2935,1,52192,"BIT","ST" 31,39,5,2,9,689,1,"ORRVILLE (CITY OF)","ORRVILLE",0,"NAT GAS",14194,"0M",1294,,,95,45,744,0,42,811,0,122,1020,0,127,1797,0,112,1116,0,51,780,0,63,856,0,72,1126,0,22,331,0,46,762,0,78,961,0,76,1181,0,2935,1,52192,"NG","ST" 31,39,5,2,2,691,1,"PAINESVILLE (CITY OF)","PAINESVILLE",0,"LIGHT OIL",14381,"0M",1294,,,95,0,0,1518,0,0,1518,0,0,1518,36,100,1776,5,13,1762,0,0,1048,0,0,1762,25,73,1689,25,73,1616,4,14,1602,17,53,1548,10,20,1528,2936,1,52227,"FO2","ST" 31,39,5,2,6,691,1,"PAINESVILLE (CITY OF)","PAINESVILLE",0,"BIT COAL",14381,"0M",1294,,,95,17099,10622,1607,15231,10037,2990,13188,8922,6467,12361,8060,7830,13138,7996,7962,15287,8544,8154,15901,9966,8093,12362,8310,8580,11176,7757,8780,11298,8213,9293,8336,6116,9293,7235,5099,7825,2936,1,52227,"BIT","ST" 31,39,5,2,9,691,1,"PAINESVILLE (CITY OF)","PAINESVILLE",0,"NAT GAS",14381,"0M",1294,,,95,16,258,0,29,464,0,152,2440,0,67,1072,0,27,394,0,18,254,0,42,658,0,113,1904,0,81,1386,0,46,839,0,100,1812,0,97,1715,0,2936,1,52227,"NG","ST" 31,39,5,2,2,700,10,"PIQUA (CITY OF)","PIQUA",0,"LIGHT OIL",15095,"0M",1294,,,95,0,1,33,1,9,24,0,0,35,1,7,27,0,0,32,0,1,31,0,1,30,0,0,30,0,0,30,0,4,26,0,3,23,1,6,36,2937,1,52334,"FO2","ST" 31,39,5,2,6,700,10,"PIQUA (CITY OF)","PIQUA",0,"BIT COAL",15095,"0M",1294,,,95,2963,3832,1560,2779,3526,1061,2427,2994,1038,1970,2648,582,2418,2789,195,1914,2556,734,1374,2211,15,1611,2421,41,1481,2312,382,2468,3140,627,2650,3515,1751,2688,3569,2090,2937,1,52334,"BIT","ST" 31,39,5,4,2,700,10,"PIQUA (CITY OF)","PIQUA",0,"LIGHT OIL",15095,"0M",1294,,,95,24,119,2949,51,239,3071,-37,127,2947,119,588,2896,109,897,3032,277,1359,2730,469,2758,2645,595,2956,2720,-11,101,2619,37,176,2979,59,288,3048,121,591,2992,2937,1,52334,"FO2","GT" 31,39,5,2,6,722,1,"SAINT MARYS (CITY OF)","ST MARYS",0,"BIT COAL",17891,"0M",1294,,,95,1250,698,645,3927,2565,332,4111,3269,140,0,0,150,0,0,150,1641,1050,490,5298,3368,489,222,149,638,1630,1068,419,4646,3274,449,4461,2807,449,4928,3119,495,2942,1,52789,"BIT","ST" 31,39,5,4,2,722,1,"SAINT MARYS (CITY OF)","ST MARYS",0,"LIGHT OIL",17891,"0M",1294,,,95,1,12,318,0,0,307,28,146,352,0,0,352,0,0,352,1,4,348,59,83,428,3,8,420,1,24,396,0,0,520,1,3,518,2,6,512,2942,1,52789,"FO2","GT" 31,39,5,2,6,726,1,"SHELBY (CITY OF)","SHELBY",0,"BIT COAL",17043,"0M",1294,,,95,8039,5710,300,7249,5098,300,7132,4852,300,6141,3985,300,6694,4389,300,8103,4859,300,6796,4831,300,7378,5266,0,6897,3944,300,6844,4580,300,7615,5188,300,8726,5206,300,2943,1,52637,"BIT","ST" 31,39,5,2,9,726,1,"SHELBY (CITY OF)","SHELBY",0,"NAT GAS",17043,"0M",1294,,,95,134,1996,0,47,686,0,36,517,0,9,134,0,0,0,0,30,381,0,96,1415,0,11,164,0,19,230,0,41,576,0,48,685,0,44,555,0,2943,1,52637,"NG","ST" 31,39,5,3,2,726,1,"SHELBY (CITY OF)","SHELBY",0,"LIGHT OIL",17043,"0M",1294,,,95,0,0,73,0,0,73,0,0,73,0,0,103,0,0,103,0,0,103,1,5,93,1,4,83,2,5,78,0,1,77,0,1,76,0,1,45,2943,1,52637,"FO2","IC" 31,39,5,3,9,726,1,"SHELBY (CITY OF)","SHELBY",0,"NAT GAS",17043,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2943,1,52637,"NG","IC" 31,39,5,3,2,774,1,"WOODSFIELD (CITY OF)","WOODSFIELD",0,"LIGHT OIL",20977,"0A",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2945,1,53350,"FO2","IC" 31,39,5,3,9,774,1,"WOODSFIELD (CITY OF)","WOODSFIELD",0,"NAT GAS",20977,"0A",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2945,1,53350,"NG","IC" 31,39,8,2,6,800,1,"AMER MUN POWER-OHIO INC","R GORSUCH",0,"BIT COAL",40577,"0M",1294,,,95,99037,64265,81413,104738,67228,84252,126378,79745,86718,63579,42733,100556,123281,76701,94920,115392,69307,101317,117333,72018,101225,121473,79176,86641,108722,66669,90892,126955,78956,87022,103717,67360,86260,126485,80616,78276,7286,1,58910,"BIT","ST" 31,39,8,2,9,800,1,"AMER MUN POWER-OHIO INC","R GORSUCH",0,"NAT GAS",40577,"0M",1294,,,95,1576,22702,0,1469,21157,0,638,9083,0,541,8226,0,767,10634,0,1094,14686,0,877,12191,0,505,7352,0,810,11188,0,528,7439,0,733,10544,0,821,11624,0,7286,1,58910,"NG","ST" 32,18,1,2,6,25,1,"COMMONWEALTH ED CO IND","STATE LINE",0,"BIT COAL",4111,"0M",1294,,101,95,111368,64033,111935,149730,82697,41943,169301,90886,94463,49952,30907,197006,107334,61118,203229,185763,102059,199201,147171,80912,167481,211732,117972,103696,93902,54629,131796,97942,56647,95060,141995,78255,74660,93050,52182,100094,981,4,54003,"BIT","ST" 32,18,1,2,9,25,1,"COMMONWEALTH ED CO IND","STATE LINE",0,"NAT GAS",4111,"0M",1294,,101,95,6077,64670,0,5326,53012,0,4895,48146,0,1349,14775,0,4538,48258,0,4988,51500,0,4470,45645,0,4498,45907,0,2972,32243,0,3706,39699,0,5098,51893,0,3793,39849,0,981,4,54003,"NG","ST" 32,18,1,2,2,45,1,"INDIANA-KENTUCKY EL CORP","CLIFTY CRK",0,"LIGHT OIL",9269,"0M",1294,,505,95,186,351,3905,152,276,3630,241,444,3700,377,692,3522,263,551,3142,200,360,3468,175,320,4005,93,171,4177,112,189,3988,183,330,3658,234,419,3925,187,321,3947,983,1,54010,"FO2","ST" 32,18,1,2,6,45,1,"INDIANA-KENTUCKY EL CORP","CLIFTY CRK",0,"BIT COAL",9269,"0M",1294,,505,95,680000,340288,711560,681685,332462,794224,771872,377298,719124,715568,349771,768331,774831,394798,790608,706890,347717,739042,846234,432529,698423,836401,439085,664104,841295,424266,608234,755940,378632,751924,859900,416889,759244,867253,423226,804472,983,1,54010,"BIT","ST" 32,18,1,1,,57,5,"INDIANA MICHIGAN POWER CO","ELKHART",0,,9324,"0M",1294,,363,95,1650,0,0,1194,0,0,1755,0,0,1250,0,0,1341,0,0,1179,0,0,1157,0,0,1230,0,0,728,0,0,610,0,0,606,0,0,1138,0,0,986,1,57745,"WAT","HY" 32,18,1,1,,57,15,"INDIANA MICHIGAN POWER CO","TWIN BRANCH",0,,9324,"0M",1294,,363,95,2749,0,0,2559,0,0,3177,0,0,3035,0,0,3169,0,0,2570,0,0,2394,0,0,2550,0,0,1769,0,0,1707,0,0,2868,0,0,2542,0,0,989,1,57745,"WAT","HY" 32,18,1,2,2,57,40,"INDIANA MICHIGAN POWER CO","TANNERS CRK",0,"LIGHT OIL",9324,"0M",1294,,363,95,1203,1922,5959,701,1134,5915,1180,2025,6714,1059,1682,6177,1112,1829,5848,1144,1978,6336,1259,2060,7095,1078,1912,5713,665,1191,4522,206,409,5361,886,1592,4308,1326,2011,4418,988,1,57745,"FO2","ST" 32,18,1,2,6,57,40,"INDIANA MICHIGAN POWER CO","TANNERS CRK",0,"BIT COAL",9324,"0M",1294,,363,95,432338,162155,420217,485332,183170,404434,427268,171172,375261,371083,146417,383926,364601,144830,374644,383224,158993,372917,442272,183537,275408,494886,200826,195877,151186,61682,248353,10073,4559,312659,189477,75997,327350,330050,118848,262047,988,1,57745,"BIT","ST" 32,18,1,4,2,57,55,"INDIANA MICHIGAN POWER CO","FOURTH ST",0,"LIGHT OIL",9324,"0M",1294,,363,95,0,0,90,0,0,90,0,0,90,0,0,90,0,0,90,0,0,90,0,0,90,0,0,90,0,0,90,0,0,90,0,0,90,0,0,90,1025,1,57745,"FO2","GT" 32,18,1,2,2,57,60,"INDIANA MICHIGAN POWER CO","ROCKPORT",0,"LIGHT OIL",9324,"0M",1294,,363,95,1253,2167,36532,1335,2320,34384,3886,6841,48740,4321,7609,41131,3580,6420,34711,5662,10180,45654,3887,6888,38767,4216,7569,31198,1478,2587,28611,1002,1634,26976,690,1194,25782,1723,4126,33355,6166,1,57745,"FO2","ST" 32,18,1,2,6,57,60,"INDIANA MICHIGAN POWER CO","ROCKPORT",0,"BIT COAL",9324,"0M",1294,,363,95,1749008,1032186,1725862,1579775,933220,1565332,1339465,797497,1717887,1321428,787392,1749794,910898,553161,1861348,1507665,916281,1691338,1420244,862282,1685879,1514621,918947,1761783,1599963,954251,1694782,1691163,933949,1738612,1640828,959611,1762887,1464158,854236,1918162,6166,1,57745,"BIT","ST" 32,18,1,2,2,63,5,"INDIANAPOLIS PWR & LGT CO","E W STOUT",0,"LIGHT OIL",9273,"0M",1294,,,95,566,1401,20541,856,1914,17945,116,609,17337,446,1143,15565,419,1038,14023,233,762,13073,334,805,11083,970,3484,18728,223,679,18049,471,1101,16948,1380,2012,14910,618,1456,13138,990,1,51394,"FO2","ST" 32,18,1,2,6,63,5,"INDIANAPOLIS PWR & LGT CO","E W STOUT",0,"BIT COAL",9273,"0M",1294,,,95,194584,90056,252587,180919,84581,279836,140480,66420,317709,160947,73882,318796,235268,109052,299888,217930,103073,287645,259644,122601,267666,349367,162431,221093,272895,126479,196285,244308,112170,197708,270443,125748,220391,253279,116842,274191,990,1,51394,"BIT","ST" 32,18,1,3,2,63,5,"INDIANAPOLIS PWR & LGT CO","E W STOUT",0,"LIGHT OIL",9273,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,990,1,51394,"FO2","IC" 32,18,1,4,2,63,5,"INDIANAPOLIS PWR & LGT CO","E W STOUT",0,"LIGHT OIL",9273,"0M",1294,,,95,1107,4856,0,-42,681,0,-50,0,0,112,628,0,182,504,0,-7,189,0,293,1179,0,349,1894,0,-35,0,0,-43,0,0,-50,26,0,-11,317,0,990,1,51394,"FO2","GT" 32,18,1,4,9,63,5,"INDIANAPOLIS PWR & LGT CO","E W STOUT",0,"NAT GAS",9273,"0M",1294,,,95,1286,11256,0,10,1339,0,-53,1880,0,93,2875,0,1102,18630,0,448,8470,0,4489,66365,0,11695,166046,0,-64,3722,0,-37,1618,0,3205,49273,0,3710,54428,0,990,1,51394,"NG","GT" 32,18,1,2,2,63,15,"INDIANAPOLIS PWR & LGT CO","PERRY K",0,"LIGHT OIL",9273,"0M",1294,,,95,0,0,4682,0,0,4553,0,0,4331,0,0,4301,0,0,4287,0,0,3841,0,0,3636,0,0,5062,0,0,5057,0,0,5051,0,0,5042,0,0,4762,992,1,51394,"FO2","ST" 32,18,1,2,6,63,15,"INDIANAPOLIS PWR & LGT CO","PERRY K",0,"BIT COAL",9273,"0M",1294,,,95,0,0,79574,-1610,0,80083,0,0,75101,0,0,73147,0,0,75348,0,0,76456,766,826,73924,340,352,74885,1152,1362,75776,0,0,74934,0,0,77090,0,0,71176,992,1,51394,"BIT","ST" 32,18,1,2,9,63,15,"INDIANAPOLIS PWR & LGT CO","PERRY K",0,"NAT GAS",9273,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,17,437,0,7,193,0,32,957,0,0,0,0,0,0,0,0,0,0,992,1,51394,"NG","ST" 32,18,1,5,9,63,15,"INDIANAPOLIS PWR & LGT CO","PERRY K",0,"WASTE HT",9273,"0M",1294,,,95,-782,0,0,0,0,0,1330,0,0,1056,0,0,2878,0,0,887,0,0,1971,0,0,1192,0,0,1301,0,0,1055,0,0,-372,0,0,-854,0,0,992,1,51394,"WT","CC" 32,18,1,2,2,63,20,"INDIANAPOLIS PWR & LGT CO","PERRY W",0,"LIGHT OIL",9273,"0M",1294,,,95,-49,0,697,-71,0,697,-71,0,697,-67,0,697,-59,0,697,-46,0,697,-51,0,697,-47,0,697,-42,0,697,-44,0,697,-59,0,697,-65,0,697,993,1,51394,"FO2","ST" 32,18,1,2,9,63,20,"INDIANAPOLIS PWR & LGT CO","PERRY W",0,"NAT GAS",9273,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,993,1,51394,"NG","ST" 32,18,1,5,9,63,20,"INDIANAPOLIS PWR & LGT CO","PERRY W",0,"WASTE HT",9273,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,993,1,51394,"WH","CC" 32,18,1,2,2,63,23,"INDIANAPOLIS PWR & LGT CO","PETERSBURG",0,"LIGHT OIL",9273,"0M",1294,,,95,610,1111,6386,445,819,5517,317,533,4940,401,748,8963,2218,4082,4553,637,1151,5787,377,687,4945,1822,3221,6367,801,1483,4763,545,999,3635,1447,2637,5880,1975,3581,4564,994,1,51394,"FO2","ST" 32,18,1,2,6,63,23,"INDIANAPOLIS PWR & LGT CO","PETERSBURG",0,"BIT COAL",9273,"0M",1294,,,95,1040025,481608,951198,910590,421941,973809,942914,432679,1023657,783657,368727,1096578,667135,315158,1184238,973163,448245,1179213,992610,460767,1051137,936517,439379,945966,722162,339012,925268,812107,376653,886087,794558,370468,820716,931266,431118,719090,994,1,51394,"BIT","ST" 32,18,1,3,2,63,23,"INDIANAPOLIS PWR & LGT CO","PETERSBURG",0,"LIGHT OIL",9273,"0M",1294,,,95,2,5,0,0,0,0,25,44,0,102,178,0,189,328,0,45,76,0,52,90,0,74,131,0,46,80,0,67,116,0,39,43,0,31,78,0,994,1,51394,"FO2","IC" 32,18,1,2,2,63,25,"INDIANAPOLIS PWR & LGT CO","H T PRTCHRD",0,"LIGHT OIL",9273,"0M",1294,,,95,318,680,5661,350,656,4975,104,195,4685,436,902,7879,417,829,7014,283,586,6386,443,914,5445,1802,3787,7417,307,627,7108,203,431,6547,316,654,5835,499,993,4785,991,1,51394,"FO2","ST" 32,18,1,2,6,63,25,"INDIANAPOLIS PWR & LGT CO","H T PRTCHRD",0,"BIT COAL",9273,"0M",1294,,,95,39918,21829,172846,38399,18739,164110,25730,13890,166007,31554,16614,192907,62657,32105,189004,38978,20477,189810,89346,46785,168301,129720,68988,123731,61410,31642,119624,29705,15920,161259,67519,35572,171574,68221,34547,157787,991,1,51394,"BIT","ST" 32,18,1,3,2,63,25,"INDIANAPOLIS PWR & LGT CO","H T PRTCHRD",0,"LIGHT OIL",9273,"0M",1294,,,95,10,18,0,10,18,0,11,19,0,10,19,0,10,19,0,10,18,0,9,18,0,10,18,0,9,18,0,3,5,0,10,11,0,10,16,0,991,1,51394,"FO2","IC" 32,18,1,1,,97,25,"NORTHERN IND PUB SERV CO","NORWAY",0,,13756,"0M",1294,,,95,2951,0,0,1754,0,0,3112,0,0,3813,0,0,3505,0,0,2903,0,0,2206,0,0,1230,0,0,509,0,0,-5,0,0,935,0,0,741,0,0,998,1,52101,"WAT","HY" 32,18,1,1,,97,30,"NORTHERN IND PUB SERV CO","OAKDALE",0,,13756,"0M",1294,,,95,4302,0,0,2658,0,0,4495,0,0,5358,0,0,4552,0,0,4225,0,0,3387,0,0,1840,0,0,1214,0,0,492,0,0,1566,0,0,1435,0,0,999,1,52101,"WAT","HY" 32,18,1,2,5,97,35,"NORTHERN IND PUB SERV CO","BAILLY",0,"COKE",13756,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,995,1,52101,"PC","ST" 32,18,1,2,6,97,35,"NORTHERN IND PUB SERV CO","BAILLY",0,"BIT COAL",13756,"0M",1294,,,95,255092,122559,79738,278804,133215,33213,188964,93227,81145,300874,140721,83750,249838,120767,64124,246937,117749,44162,235477,114020,45186,281196,134308,37119,206770,100042,54350,171878,84048,49037,248313,118863,34340,215434,105042,32995,995,1,52101,"BIT","ST" 32,18,1,2,9,97,35,"NORTHERN IND PUB SERV CO","BAILLY",0,"NAT GAS",13756,"0M",1294,,,95,2509,26046,0,1617,16709,0,6960,74244,0,364,3631,0,132,1380,0,473,4895,0,3976,41921,0,11155,116087,0,295,3099,0,9000,94567,0,731,7651,0,10008,106430,0,995,1,52101,"NG","ST" 32,18,1,4,2,97,35,"NORTHERN IND PUB SERV CO","BAILLY",0,"LIGHT OIL",13756,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,995,1,52101,"FO2","GT" 32,18,1,4,9,97,35,"NORTHERN IND PUB SERV CO","BAILLY",0,"NAT GAS",13756,"0M",1294,,,95,260,4325,0,239,4585,0,197,4652,0,73,729,0,0,0,0,128,2648,0,1309,27718,0,1556,27641,0,86,2797,0,94,990,0,0,0,0,0,0,0,995,1,52101,"NG","GT" 32,18,1,2,6,97,50,"NORTHERN IND PUB SERV CO","MICH CITY",0,"BIT COAL",13756,"0M",1294,,,95,236420,123317,103301,234123,120234,148075,251278,135807,162546,205743,116541,177892,112253,67389,170049,124057,76284,129959,232893,135633,114125,231506,135299,93596,234187,129907,86183,254454,138881,100596,227408,129965,87044,241351,131616,87326,997,1,52101,"BIT","ST" 32,18,1,2,9,97,50,"NORTHERN IND PUB SERV CO","MICH CITY",0,"NAT GAS",13756,"0M",1294,,,95,22888,245981,0,12315,127428,0,7313,77250,0,2223,23885,0,17374,195664,0,14491,167133,0,33790,372448,0,46983,516773,0,57,601,0,277,2894,0,14761,158089,0,7779,81844,0,997,1,52101,"NG","ST" 32,18,1,2,6,97,54,"NORTHERN IND PUB SERV CO","D MITCHELL",0,"BIT COAL",13756,"0M",1294,,,95,145857,82802,116751,116897,65893,113729,119863,69185,152487,141199,84936,154502,149654,87531,159194,148998,85732,121077,153374,92272,109798,153611,89672,90907,105137,61906,133520,134131,77926,126283,118138,72811,149593,119904,77033,120350,996,1,52101,"BIT","ST" 32,18,1,2,9,97,54,"NORTHERN IND PUB SERV CO","D MITCHELL",0,"NAT GAS",13756,"0M",1294,,,95,9050,99836,0,19988,219179,0,4693,51173,0,2044,22775,0,681,7679,0,15253,169699,0,31855,357533,0,49912,561059,0,1836,21192,0,688,7733,0,17585,198980,0,12007,137527,0,996,1,52101,"NG","ST" 32,18,1,4,2,97,54,"NORTHERN IND PUB SERV CO","D MITCHELL",0,"LIGHT OIL",13756,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,996,1,52101,"FO2","GT" 32,18,1,4,9,97,54,"NORTHERN IND PUB SERV CO","D MITCHELL",0,"NAT GAS",13756,"0M",1294,,,95,0,0,0,62,1005,0,19,314,0,61,972,0,59,947,0,23,381,0,1109,18451,0,787,13562,0,0,0,0,17,200,0,19,316,0,40,614,0,996,1,52101,"NG","GT" 32,18,1,2,2,97,60,"NORTHERN IND PUB SERV CO","SCHAHFER",0,"LIGHT OIL",13756,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,6085,1,52101,"FO2","ST" 32,18,1,2,5,97,60,"NORTHERN IND PUB SERV CO","SCHAHFER",0,"COKE",13756,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,5680,2361,3668,16726,6787,383,17831,7291,7,6085,1,52101,"PC","ST" 32,18,1,2,6,97,60,"NORTHERN IND PUB SERV CO","SCHAHFER",0,"BIT COAL",13756,"0M",1294,,,95,535261,312105,335057,389163,229937,440028,546548,302317,415959,448635,246990,395514,597050,350998,454670,756850,452731,337454,682007,398333,335076,754511,435319,290970,649742,383628,258615,683709,390480,291948,637992,357548,247219,681946,380639,238033,6085,1,52101,"BIT","ST" 32,18,1,2,9,97,60,"NORTHERN IND PUB SERV CO","SCHAHFER",0,"NAT GAS",13756,"0M",1294,,,95,3899,42407,0,6373,71396,0,4950,53485,0,5022,55321,0,9160,101163,0,8473,94946,0,11416,127138,0,11318,127241,0,6765,76948,0,5330,59832,0,10465,114654,0,16610,183389,0,6085,1,52101,"NG","ST" 32,18,1,4,2,97,60,"NORTHERN IND PUB SERV CO","SCHAHFER",0,"LIGHT OIL",13756,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,6085,1,52101,"FO2","GT" 32,18,1,4,9,97,60,"NORTHERN IND PUB SERV CO","SCHAHFER",0,"NAT GAS",13756,"0M",1294,,,95,723,10302,0,782,11325,0,1650,23018,0,308,4700,0,805,15657,0,1994,32783,0,15126,225451,0,13726,215839,0,142,2242,0,733,10618,0,280,4262,0,601,10905,0,6085,1,52101,"NG","GT" 32,18,1,1,,115,10,"PSI ENERGY, INC","MARKLAND",0,,15470,"0M",1294,,,95,25874,0,0,30535,0,0,30427,0,0,34190,0,0,21420,0,0,33483,0,0,37429,0,0,31238,0,0,21329,0,0,31723,0,0,32028,0,0,33480,0,0,1005,1,52410,"WAT","HY" 32,18,1,2,2,115,20,"PSI ENERGY, INC","CAYUGA",0,"LIGHT OIL",15470,"0M",1294,,,95,132,235,5513,571,1037,4367,530,968,3231,360,648,6046,1268,2286,3656,1673,3058,5188,191,340,4690,456,897,3714,450,808,2757,116,203,4365,648,1159,3695,1043,1890,4595,1001,1,52410,"FO2","ST" 32,18,1,2,6,115,20,"PSI ENERGY, INC","CAYUGA",0,"BIT COAL",15470,"0M",1294,,,95,560086,260374,595374,436002,205588,619769,507290,241920,579748,458167,216960,558238,273942,132145,579528,461324,222630,594519,529339,250671,586438,553167,264792,531310,481498,229472,498542,556861,260068,435186,538773,254635,379746,560196,264529,360124,1001,1,52410,"BIT","ST" 32,18,1,3,2,115,20,"PSI ENERGY, INC","CAYUGA",0,"LIGHT OIL",15470,"0M",1294,,,95,52,94,835,80,146,689,46,85,604,32,59,546,48,87,793,40,74,719,187,332,719,345,632,893,44,79,814,57,100,714,46,83,810,52,95,715,1001,1,52410,"FO2","IC" 32,18,1,4,2,115,20,"PSI ENERGY, INC","CAYUGA",0,"LIGHT OIL",15470,"0M",1294,,,95,94,169,5321,0,0,5313,0,0,5287,0,0,5295,9,17,5278,0,0,5274,0,0,5261,0,0,5256,0,0,5278,0,0,5291,0,0,5304,0,0,5321,1001,1,52410,"FO2","GT" 32,18,1,4,9,115,20,"PSI ENERGY, INC","CAYUGA",0,"NAT GAS",15470,"0M",1294,,,95,2346,23310,0,1913,19353,0,1506,15557,0,1635,16714,0,1240,12674,0,4044,41468,0,15842,159433,0,18202,212550,0,0,0,0,0,0,0,2097,21202,0,3527,35908,0,1001,1,52410,"NG","GT" 32,18,1,2,2,115,30,"PSI ENERGY, INC","EDWARDSPORT",0,"LIGHT OIL",15470,"0M",1294,,,95,209,496,4820,64,150,4672,155,373,4297,0,0,4295,0,0,4292,97,238,4052,689,1571,2481,2502,5818,2869,342,868,2002,0,0,2002,0,0,1997,147,370,1625,1004,1,52410,"FO2","ST" 32,18,1,2,6,115,30,"PSI ENERGY, INC","EDWARDSPORT",0,"BIT COAL",15470,"0M",1294,,,95,17730,11048,72080,19934,11948,70647,12688,8051,74559,-527,0,75232,-535,0,75232,15454,10259,64973,35050,21901,43072,52741,33340,15650,4173,2912,38766,-602,0,62015,-609,0,63195,16335,10947,52274,1004,1,52410,"BIT","ST" 32,18,1,2,2,115,32,"PSI ENERGY, INC","R GALLAGHER",0,"LIGHT OIL",15470,"0M",1294,,,95,2035,3891,1605,1454,2810,1394,1851,3297,1699,1757,3179,1643,2068,3708,1567,1765,3297,1717,1740,3339,1643,1698,3478,1699,628,1171,1662,1918,3473,1772,1054,1957,1432,2452,4557,1662,1008,1,52410,"FO2","ST" 32,18,1,2,6,115,32,"PSI ENERGY, INC","R GALLAGHER",0,"BIT COAL",15470,"0M",1294,,,95,228795,101724,280677,208492,94433,264483,157312,68908,321856,177541,78622,327010,219815,95103,325222,282888,123689,301473,287606,128632,273012,307948,143686,219622,142108,60394,233330,173570,72509,241738,224846,92953,254240,214410,90070,255848,1008,1,52410,"BIT","ST" 32,18,1,2,2,115,35,"PSI ENERGY, INC","NOBLESVILLE",0,"LIGHT OIL",15470,"0M",1294,,,95,51,112,562,83,160,505,48,112,674,66,152,531,0,0,490,110,229,643,81,169,664,55,117,548,22,64,674,58,167,474,0,43,548,34,71,476,1007,1,52410,"FO2","ST" 32,18,1,2,6,115,35,"PSI ENERGY, INC","NOBLESVILLE",0,"BIT COAL",15470,"0M",1294,,,95,11044,6031,55495,9455,4868,50627,3897,2460,49399,4036,2484,49078,-19,344,48734,11688,6456,42278,26318,14879,27399,34289,19561,18825,965,758,32438,3085,2324,49315,-104,155,61612,12274,6417,55744,1007,1,52410,"BIT","ST" 32,18,1,2,2,115,38,"PSI ENERGY, INC","WABASH RIVR",0,"LIGHT OIL",15470,"0M",1294,,,95,2430,4476,2106,1459,2739,2128,1389,2692,1967,1849,3579,2218,1434,2758,1631,681,1290,2176,1683,3263,2148,2465,4797,2269,945,1807,2338,1000,1900,2380,729,1435,2430,2010,3862,1720,1010,1,52410,"FO2","ST" 32,18,1,2,6,115,38,"PSI ENERGY, INC","WABASH RIVR",0,"BIT COAL",15470,"0M",1294,,,95,269453,126688,229629,237554,115161,230254,111825,56100,288778,84991,42415,325474,75621,37146,348471,305101,147377,290801,239625,122121,244288,280979,141633,160506,165651,82144,169356,117517,58071,210036,143505,72409,218547,185588,91761,206945,1010,1,52410,"BIT","ST" 32,18,1,3,2,115,38,"PSI ENERGY, INC","WABASH RIVR",0,"LIGHT OIL",15470,"0M",1294,,,95,22,41,295,6,12,283,29,57,226,36,71,155,22,43,283,17,33,250,46,91,336,25,50,286,1,2,283,16,31,37,14,29,343,5,10,333,1010,1,52410,"FO2","IC" 32,18,1,3,2,115,40,"PSI ENERGY, INC","MIAMI WBASH",0,"LIGHT OIL",15470,"0M",1294,,,95,-10,953,9190,166,743,8447,-197,894,7552,-39,60,7493,16,281,7212,81,612,6600,891,3627,5277,1034,3669,3913,-3,92,3821,-25,12,3809,-92,165,3644,-114,427,3217,1006,1,52410,"FO2","IC" 32,18,1,4,2,115,43,"PSI ENERGY, INC","CONNERSVILE",0,"LIGHT OIL",15470,"0M",1294,,,95,598,1430,6151,267,338,5812,185,528,5284,-1,88,5196,74,91,5105,363,946,4160,1734,3950,0,1728,5143,7132,123,299,6833,35,74,6797,36,197,6601,68,309,6291,1002,1,52410,"FO2","GT" 32,18,1,2,2,115,47,"PSI ENERGY, INC","GIBSON STA",0,"LIGHT OIL",15470,"0M",1294,,,95,3573,6225,8026,3627,6211,8525,2908,4962,6089,2299,3933,7385,2638,4537,9046,4608,8201,6236,1193,2069,8692,1020,1752,9495,2262,3909,8491,2394,4067,6679,1306,2237,7725,1788,3105,5067,6113,1,52410,"FO2","ST" 32,18,1,2,6,115,47,"PSI ENERGY, INC","GIBSON STA",0,"BIT COAL",15470,"0M",1294,,,95,1411040,662768,2861774,1615449,737476,2742578,1641475,746285,2737505,1326993,600387,2789580,1389674,630387,2844473,1353290,632853,2819275,1781130,810634,2543921,1880261,844888,2374175,1610199,724136,2280260,1401722,620957,2297336,1703790,761235,2101523,1647889,748548,1888232,6113,1,52410,"BIT","ST" 32,18,1,4,2,127,1,"SOUTHERN INDIANA G & E CO","BROADWAY",0,"LIGHT OIL",17633,"0M",1294,,,95,0,0,801,0,0,801,0,0,801,0,0,801,0,0,801,0,0,801,0,0,801,0,0,801,0,0,801,0,0,801,0,0,801,0,0,801,1011,1,52727,"FO2","GT" 32,18,1,4,9,127,1,"SOUTHERN INDIANA G & E CO","BROADWAY",0,"NAT GAS",17633,"0M",1294,,,95,108,1488,0,31,496,0,72,936,0,66,992,0,675,9932,0,358,9922,0,3822,54621,0,11701,173627,0,131,4946,0,181,9912,0,586,4959,0,0,0,0,1011,1,52727,"NG","GT" 32,18,1,2,2,127,3,"SOUTHERN INDIANA G & E CO","CULLEY",0,"LIGHT OIL",17633,"0M",1294,,,95,0,0,350,0,0,350,0,0,350,0,0,350,0,0,350,0,0,250,0,0,250,0,0,250,0,0,250,0,0,250,0,0,250,0,0,250,1012,1,52727,"FO2","ST" 32,18,1,2,6,127,3,"SOUTHERN INDIANA G & E CO","CULLEY",0,"BIT COAL",17633,"0M",1294,,,95,122067,60600,138140,167988,82419,159735,169634,79436,181228,114459,53639,191704,165848,81055,168418,184693,87570,154235,207611,100070,138520,218589,105190,134359,160446,77417,139667,174664,86907,135057,217251,106316,124021,205575,102713,115674,1012,1,52727,"BIT","ST" 32,18,1,2,9,127,3,"SOUTHERN INDIANA G & E CO","CULLEY",0,"NAT GAS",17633,"0M",1294,,,95,285,3090,0,126,1344,0,136,1410,0,300,3116,0,121,1311,0,107,1123,0,101,1082,0,285,3040,0,412,4406,0,312,3443,0,180,1935,0,153,1681,0,1012,1,52727,"NG","ST" 32,18,1,4,9,127,9,"SOUTHERN INDIANA G & E CO","NORTHEAST",0,"NAT GAS",17633,"0M",1294,,,95,24,992,0,48,5399,0,0,0,0,0,0,0,0,0,0,22,2492,0,0,0,0,562,10295,0,0,0,0,0,0,0,23,3023,0,26,4467,0,1013,1,52727,"NG","GT" 32,18,1,2,6,127,20,"SOUTHERN INDIANA G & E CO","WARRICK",0,"BIT COAL",17633,"0M",1294,,,95,95617,41510,100212,86572,39259,87257,96250,42312,89684,93020,40228,97629,96270,44344,83127,82739,38242,69870,89329,39892,44260,100497,44406,41656,97103,42826,35874,28941,12332,66823,92060,41077,55982,99718,45727,57793,6705,1,52727,"BIT","ST" 32,18,1,2,9,127,20,"SOUTHERN INDIANA G & E CO","WARRICK",0,"NAT GAS",17633,"0M",1294,,,95,27,261,0,112,1120,0,11,112,0,29,276,0,5,50,0,0,0,0,136,1318,0,83,796,0,0,0,0,295,2822,0,57,575,0,62,639,0,6705,1,52727,"NG","ST" 32,18,1,2,2,127,25,"SOUTHERN INDIANA G & E CO","BROWN",0,"LIGHT OIL",17633,"0M",1294,,,95,0,0,1712,0,0,1437,0,0,2186,0,0,2151,0,0,1998,0,0,1988,0,0,2336,0,0,2336,0,0,2336,0,0,2336,0,0,2175,0,0,2175,6137,1,52727,"FO2","ST" 32,18,1,2,6,127,25,"SOUTHERN INDIANA G & E CO","BROWN",0,"BIT COAL",17633,"0M",1294,,,95,217766,95613,450544,147685,72927,476200,218223,106171,479883,196964,85661,485255,182235,86959,499237,216954,101195,498135,247301,113099,429991,275892,131703,360852,177911,84026,286413,238026,112468,229493,139223,67172,246596,170321,82481,189492,6137,1,52727,"BIT","ST" 32,18,1,2,9,127,25,"SOUTHERN INDIANA G & E CO","BROWN",0,"NAT GAS",17633,"0M",1294,,,95,728,7231,0,709,7962,0,465,5154,0,1271,12486,0,681,7404,0,869,9196,0,829,8558,0,910,9792,0,91,976,0,1005,9912,0,462,4959,0,1013,10609,0,6137,1,52727,"NG","ST" 32,18,1,4,2,127,25,"SOUTHERN INDIANA G & E CO","BROWN",0,"LIGHT OIL",17633,"0M",1294,,,95,0,0,0,139,275,0,10,21,0,20,35,0,75,144,0,155,289,0,4,9,0,0,0,0,0,0,0,0,0,0,84,161,0,0,0,0,6137,1,52727,"FO2","GT" 32,18,1,4,9,127,25,"SOUTHERN INDIANA G & E CO","BROWN",0,"NAT GAS",17633,"0M",1294,,,95,371,3684,0,237,2668,0,72,799,0,244,2399,0,872,9478,0,725,7671,0,3499,36107,0,8313,89423,0,835,8917,0,0,0,0,0,0,0,115,1208,0,6137,1,52727,"NG","GT" 32,18,5,3,2,529,15,"BLUFFTON (CITY OF)","BLUFFTON",0,"LIGHT OIL",1896,"0A",1294,,,95,1,60,1391,2,67,1322,61,54,1600,8,70,1533,12,90,1444,17,90,1361,5,46,0,16,58,1746,9,46,1693,5,45,1674,1,9,1658,1,20,1637,1023,1,54077,"FO2","IC" 32,18,5,3,9,529,15,"BLUFFTON (CITY OF)","BLUFFTON",0,"NAT GAS",1896,"0A",1294,,,95,252,951,0,283,1047,0,187,936,0,252,888,0,327,1129,0,322,1124,0,21,749,0,165,1201,0,79,956,0,14,141,0,8,282,0,62,1131,0,1023,1,54077,"NG","IC" 32,18,5,2,6,552,1,"CRAWFORDSVILLE (CITY OF)","CRAWFRDVIL",0,"BIT COAL",4508,"M",1294,,,95,2633,2217,2514,2446,2032,2094,1890,1637,1012,0,12,1693,0,9,2211,497,408,1961,0,0,1961,1383,1034,1775,0,0,2801,0,0,2783,0,0,2783,2446,2070,2457,1024,1,50698,"BIT","ST" 32,18,5,2,9,552,1,"CTAWFORDSVILLE (CITY OF)","CRAWFRDVIL",0,"NAT GAS",4508,"M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,11,198,0,0,9,0,25,397,0,0,0,0,0,0,0,0,0,0,0,0,0,1024,1,50698,"NG","ST" 32,18,5,3,2,552,1,"CRAWFORDSVILLE (CITY OF)","CRAWFRDVIL",0,"LIGHT OIL",4508,"M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1024,1,50698,"FO2","IC" 32,18,5,2,6,601,1,"JASPER (CITY OF)","JASPER",0,"BIT COAL",9667,"0A",1294,,,95,5717,4616,631,5399,3895,631,5890,4398,631,2952,2186,631,3065,2373,631,5988,4375,631,5621,4191,631,2798,2138,631,0,0,1075,5001,3514,1051,5782,4146,1096,5466,4050,1096,6225,1,51443,"BIT","ST" 32,18,5,2,9,601,1,"JASPER (CITY OF)","JASPER",0,"NAT GAS",9667,"0A",1294,,,95,20,339,0,0,0,0,0,0,0,0,0,0,16,267,0,0,0,0,0,0,0,0,0,0,0,0,0,14,206,0,0,0,0,0,0,0,6225,1,51443,"NG","ST" 32,18,5,2,6,622,1,"LOGANSPORT (CITY OF)","LOGANSPORT",0,"BIT COAL",11142,"0M",1294,,,95,16294,10401,3093,15182,9658,2825,130,68,5257,0,0,7057,2842,2773,7049,15721,9566,3565,18496,9015,1600,18517,10895,1421,17032,9835,4095,8771,5557,5126,12606,7370,5733,23315,13078,934,1032,1,51681,"BIT","ST" 32,18,5,4,2,622,1,"LOGANSPORT (CITY OF)","LOGANSPORT",0,"LIGHT OIL",11142,"0M",1294,,,95,0,0,1887,0,0,1887,0,0,1887,0,0,1887,0,0,1887,0,0,1887,0,0,1887,0,0,1887,0,0,1887,0,0,1887,0,0,1887,0,0,1887,1032,1,51681,"FO2","GT" 32,18,5,4,9,622,1,"LOGANSPORT (CITY OF)","LOGANSPORT",0,"NAT GAS",11142,"0M",1294,,,95,127,2771,0,0,0,0,0,0,0,0,0,0,0,0,0,75,2842,0,0,0,0,217,5351,0,0,0,0,0,0,0,0,0,0,0,0,0,1032,1,51681,"NG","GT" 32,18,5,2,2,658,1,"PERU UTILITIES","PERU",0,"LIGHT OIL",14839,"0M",1294,,,95,2,7,60,0,0,40,0,0,29,0,0,45,0,0,42,0,0,89,0,0,89,28,62,123,2,6,104,0,0,104,0,0,64,0,0,58,1037,1,52298,"FO2","ST" 32,18,5,2,6,658,1,"PERU UTILITIES","PERU",0,"BIT COAL",14839,"0M",1294,,,95,597,409,462,0,0,462,0,0,462,0,0,462,0,0,462,0,0,664,0,0,664,4138,2475,1193,1602,1122,71,0,0,71,0,0,71,0,0,71,1037,1,52298,"BIT","ST" 32,18,5,3,2,666,1,"RENSSELAER (CITY OF)","RENSSELAER",0,"LIGHT OIL",15860,"0A",1294,,,95,0,5,507,0,4,492,0,0,385,0,0,376,42,89,635,0,0,624,11,22,610,10,24,577,13,25,557,13,33,523,18,34,485,12,25,448,1038,1,52461,"FO2","IC" 32,18,5,3,9,666,1,"RENSSELAER (CITY OF)","RENSSELAER",0,"NAT GAS",15860,"0A",1294,,,95,12,2242,0,5,609,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1038,1,52461,"NG","IC" 32,18,5,2,2,669,10,"RICHMOND (CITY OF)","WHITEWATER",0,"LIGHT OIL",15989,"0M",1294,,,95,66,135,651,4,9,642,11,23,618,36,75,544,43,89,455,36,75,380,33,65,315,24,51,800,38,79,721,40,84,637,125,241,754,33,67,866,1040,1,52479,"FO2","ST" 32,18,5,2,6,669,10,"RICHMOND (CITY OF)","WHITEWATER",0,"BIT COAL",15989,"0M",1294,,,95,52567,26931,66546,54464,27521,59857,50869,26046,61570,37981,19323,61813,34761,18221,70185,50812,25880,63189,54367,27836,58351,55464,28592,56536,47367,24058,57432,31433,16236,61431,49216,24827,57518,55122,27935,65411,1040,1,52479,"BIT","ST" 32,18,8,2,2,849,5,"HOOSIER ENERGY RURAL","RATTS",0,"LIGHT OIL",9267,"0M",1294,,,95,36,63,331,24,42,427,57,99,328,82,143,185,157,271,264,220,383,175,69,123,225,64,116,273,67,119,314,72,130,300,169,298,360,213,374,345,1043,1,51339,"FO2","ST" 32,18,8,2,6,849,5,"HOOSIER ENERGY RURAL","RATTS",0,"BIT COAL",9267,"0M",1294,,,95,152672,68804,12521,138850,61631,20613,120820,54271,33350,149240,67046,34059,138601,62960,37387,104185,47642,37604,152193,70371,29049,149047,69157,33970,133611,61143,30823,84154,38731,32856,131727,59094,30160,146986,66592,32432,1043,1,51339,"BIT","ST" 32,18,8,2,2,849,10,"HOOSIER ENERGY RURAL","MEROM",0,"LIGHT OIL",9267,"0M",1294,,,95,195,354,6014,19,38,10415,677,1227,9188,41,76,9112,1799,3447,5664,1764,3378,7059,771,1387,5672,508,946,4725,1207,2219,7281,584,1062,6218,468,838,10208,592,1063,9145,6213,1,51339,"FO2","ST" 32,18,8,2,6,849,10,"HOOSIER ENERGY RURAL","MEROM",0,"BIT COAL",9267,"0M",1294,,,95,462676,222254,448322,417644,215416,460946,384780,184640,471566,246060,116767,519358,230592,116155,570294,429927,213604,544280,462605,221660,492415,499492,244053,429843,353022,171326,433018,376476,178855,429945,480027,227666,396833,503880,236844,364841,6213,1,51339,"BIT","ST" 32,18,9,4,2,900,5,"INDIANA MUN POWER AGENCY","ANDERSON",0,"LIGHT OIL",9234,"0M",1294,,,95,19,44,5010,33,68,4942,40,82,4860,14,24,4835,7,12,4824,25,62,4762,0,1,4761,1,4,4757,0,0,4757,14,27,4730,3,9,4721,10,13,4708,7336,1,19234,"FO2","GT" 32,18,9,4,9,900,5,"INDIANA MUN POWER AGENCY","ANDERSON",0,"NAT GAS",9234,"0M",1294,,,95,53,772,0,54,717,0,199,2578,0,66,914,0,31,416,0,481,7593,0,2482,36348,0,6354,89340,0,94,1557,0,64,1343,0,36,450,0,47,750,0,7336,1,19234,"NG","GT" 33,17,1,2,2,29,5,"CENTRAL ILLINOIS LIGHT CO","E D EDWARDS",0,"LIGHT OIL",3252,"0M",1294,,,95,580,979,551,369,645,642,581,1050,511,539,979,621,777,1362,571,696,1201,688,793,1392,574,425,792,507,571,980,634,610,991,501,329,558,506,455,759,491,856,4,50485,"FO2","ST" 33,17,1,2,6,29,5,"CENTRAL ILLINOIS LIGHT CO","E D EDWARDS",0,"BIT COAL",3252,"0M",1294,,,95,278723,111505,170727,240983,94522,156151,283715,115017,142278,219332,90164,180893,314512,130292,145461,303524,124741,120263,294912,127410,143742,416665,181855,115286,215994,93604,136103,343831,139588,97044,284797,118784,138306,257830,101322,144327,856,4,50485,"BIT","ST" 33,17,1,4,9,29,12,"CENTRAL ILLINOIS LIGHT CO","STERLING AV",0,"NAT GAS",3252,"0M",1294,,,95,91,1361,0,30,486,0,29,443,0,29,495,0,28,483,0,114,1973,0,236,4614,0,495,8477,0,62,1057,0,60,926,0,32,555,0,79,1259,0,860,4,50485,"NG","GT" 33,17,1,2,2,29,20,"CENTRAL ILLINOIS LIGHT CO","DUCK CREEK",0,"LIGHT OIL",3252,"0M",1294,,,95,464,794,607,155,264,573,38,67,506,39,69,437,368,658,640,47,83,557,76,135,598,252,429,597,203,353,523,461,865,374,191,334,581,221,383,548,6016,4,50485,"FO2","ST" 33,17,1,2,6,29,20,"CENTRAL ILLINOIS LIGHT CO","DUCK CREEK",0,"BIT COAL",3252,"0M",1294,,,95,186107,88236,146013,184996,85972,174445,212342,99989,207941,178133,85191,199728,101736,49494,191824,209741,99840,163763,218825,104416,121412,182815,87426,161492,205874,98086,126656,49432,25199,182072,221479,104789,147984,208001,98018,120664,6016,4,50485,"BIT","ST" 33,17,1,2,9,29,25,"CENTRAL ILLINOIS LIGHT CO","MIDWEST GRN",0,"NAT GAS",3252,"0M",694,"A",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1987,12379,0,4809,36302,0,4873,33446,0,2693,19047,0,0,0,0,3046,22292,0,4051,25863,0,7384,4,50485,"NG","ST" 33,17,1,2,2,32,2,"CENTRAL ILL PUBLIC SER CO","COFFEEN",0,"LIGHT OIL",3253,"0M",1294,,,95,281,528,4129,159,291,4010,394,749,4105,523,1002,3949,771,1637,3876,506,903,4329,271,491,4241,39,71,3944,249,436,4034,521,930,3986,417,729,4572,962,1745,3927,861,4,50486,"FO2","ST" 33,17,1,2,6,32,2,"CENTRAL ILL PUBLIC SER CO","COFFEEN",0,"BIT COAL",3253,"0M",1294,,,95,365821,196265,250663,291393,151752,268915,248792,134522,254062,79012,43562,287270,49602,29698,377234,331239,171527,392358,397070,207104,345747,370867,195382,346249,139189,69530,387149,251535,126615,387760,291764,143554,406398,266300,137380,362886,861,4,50486,"BIT","ST" 33,17,1,2,2,32,5,"CENTRAL ILL PUBLIC SER CO","GRAND TOWER",0,"LIGHT OIL",3253,"0M",1294,,,95,146,294,559,222,423,494,139,267,578,60,171,742,-59,75,667,310,600,753,324,626,481,405,753,769,154,287,834,78,162,672,389,761,607,217,428,533,862,4,50486,"FO2","ST" 33,17,1,2,6,32,5,"CENTRAL ILL PUBLIC SER CO","GRAND TOWER",0,"BIT COAL",3253,"0M",1294,,,95,19817,10029,48685,18173,8634,59296,12650,6089,70908,3933,2772,73473,-503,161,78207,17238,8399,74696,44644,21400,58784,77238,35607,26412,11609,5363,31994,11150,5893,34133,57466,27803,19044,47800,23991,32368,862,4,50486,"BIT","ST" 33,17,1,2,2,32,10,"CENTRAL ILL PUBLIC SER CO","HUTSONVILLE",0,"LIGHT OIL",3253,"0M",1294,,,95,72,148,1592,254,501,1092,252,532,1126,117,284,1556,421,883,1560,398,781,1662,440,832,1760,236,429,1331,196,323,1008,158,382,1338,346,655,1437,140,264,1173,863,4,50486,"FO2","ST" 33,17,1,2,6,32,10,"CENTRAL ILL PUBLIC SER CO","HUTSONVILLE",0,"BIT COAL",3253,"0M",1294,,,95,17493,9580,55605,13103,6803,61393,11330,6319,65444,3457,2220,70186,6929,4012,73260,18641,9997,71065,43752,22295,48771,75386,37255,19363,5801,2524,33120,7107,4480,39773,44924,22754,26665,48938,24435,23714,863,4,50486,"BIT","ST" 33,17,1,3,2,32,10,"CENTRAL ILL PUBLIC SER CO","HUTSONVILLE",0,"LIGHT OIL",3253,"0M",1294,,,95,5,10,124,0,0,126,0,0,130,5,9,121,5,9,106,0,0,106,15,30,72,10,21,233,0,0,229,0,0,228,5,9,225,0,0,227,863,4,50486,"FO2","IC" 33,17,1,2,2,32,15,"CENTRAL ILL PUBLIC SER CO","MEREDOSIA",0,"LIGHT OIL",3253,"0M",1294,,,95,276,524,1245,240,455,1295,109,257,1541,576,1050,1518,264,464,1396,272,471,1722,478,864,1170,665,1188,1390,137,250,1672,104,202,1469,-609,0,1671,636,1140,1388,864,4,50486,"FO2","ST" 33,17,1,2,3,32,15,"CENTRAL ILL PUBLIC SER CO","MEREDOSIA",0,"HEAVY OIL",3253,"0M",1294,,,95,-878,0,41246,-869,0,41246,-953,0,41246,-789,0,41246,-6,0,41246,1105,5986,35342,1753,6017,29342,6547,17169,22153,-808,333,23977,-646,0,42084,996,1890,42084,-711,0,42084,864,4,50486,"FO6","ST" 33,17,1,2,6,32,15,"CENTRAL ILL PUBLIC SER CO","MEREDOSIA",0,"BIT COAL",3253,"0M",1294,,,95,66774,32586,105182,41839,21008,131939,15303,9402,148998,70146,32222,148546,91295,40883,144840,111244,50699,134953,137571,64325,109649,184516,85228,55561,77698,37291,62196,86881,43240,73623,78143,41045,82454,97009,48373,93368,864,4,50486,"BIT","ST" 33,17,1,2,2,32,20,"CENTRAL ILL PUBLIC SER CO","NEWTON",0,"LIGHT OIL",3253,"0M",1294,,,95,844,1577,4500,512,956,5160,1182,2043,4716,553,984,5869,379,679,5723,681,1231,5199,190,328,5578,942,1748,4784,746,1331,5217,282,508,5420,60,105,5315,649,3661,4337,6017,4,50486,"FO2","ST" 33,17,1,2,6,32,20,"CENTRAL ILL PUBLIC SER CO","NEWTON",0,"BIT COAL",3253,"0M",1294,,,95,556271,262272,366063,518547,246265,373901,546762,245831,417351,503402,237591,446819,516641,244361,536330,468640,219703,623301,560024,252360,476964,466441,225593,612105,491641,228921,632582,454181,204761,666122,359030,160358,746315,378431,180592,722338,6017,4,50486,"BIT","ST" 33,17,1,1,,41,1,"COMMONWEALTH EDISON CO","DIXON",0,,4110,"0M",1294,,100,95,1217,0,0,1001,0,0,1400,0,0,1473,0,0,1443,0,0,1109,0,0,1264,0,0,1341,0,0,1211,0,0,1365,0,0,1603,0,0,1067,0,0,868,4,50643,"WAT","HY" 33,17,1,2,1,41,1,"COMMONWEALTH EDISON CO","QUAD CITIES",0,"NUCLEAR",4110,"0M",1294,,100,95,265985,0,0,516483,0,0,563772,0,0,556271,0,0,570166,0,0,541658,0,0,537742,0,0,552522,0,0,533277,0,0,383182,0,0,293985,0,0,571167,0,0,880,4,50643,"UR","ST" 33,17,1,2,1,41,1,"COMMONWEALTH EDISON CO","BRAIDWOOD",0,"NUCLEAR",4110,"0M",1294,,100,95,845089,0,0,487988,0,0,443133,0,0,527594,0,0,838888,0,0,802928,0,0,825056,0,0,825520,0,0,701927,0,0,-9715,0,0,-10027,0,0,307159,0,0,6022,4,50643,"UR","ST" 33,17,1,2,1,41,1,"COMMONWEALTH EDISON CO","BYRON",0,"NUCLEAR",4110,"0M",1294,,100,95,766116,0,0,735235,0,0,817602,0,0,779568,0,0,804172,0,0,742334,0,0,790248,0,0,800198,0,0,786058,0,0,542611,0,0,-9310,0,0,142399,0,0,6023,4,50643,"UR","ST" 33,17,1,2,1,41,1,"COMMONWEALTH EDISON CO","LASALLE CTY",0,"NUCLEAR",4110,"0M",1294,,100,95,813809,0,0,531418,0,0,813835,0,0,788528,0,0,782478,0,0,561931,0,0,750639,0,0,609485,0,0,617973,0,0,773354,0,0,684375,0,0,641459,0,0,6026,4,50643,"UR","ST" 33,17,1,2,1,41,1,"COMMONWEALTH EDISON CO","ZION",0,"NUCLEAR",4110,"0M",1294,,100,95,777628,0,0,706122,0,0,778794,0,0,744367,0,0,679639,0,0,751346,0,0,778214,0,0,771971,0,0,190946,0,0,-8633,0,0,-8349,0,0,290089,0,0,885,4,50643,"UR","ST" 33,17,1,2,1,41,2,"COMMONWEALTH EDISON CO","ZION",0,"NUCLEAR",4110,"0M",1294,,100,95,62829,0,0,-7517,0,0,-8823,0,0,214602,0,0,763695,0,0,707962,0,0,768388,0,0,745403,0,0,742149,0,0,737928,0,0,708434,0,0,471011,0,0,885,4,50643,"UR","ST" 33,17,1,2,1,41,2,"COMMONWEALTH EDISON CO","LASALLE CTY",0,"NUCLEAR",4110,"0M",1294,,100,95,805795,0,0,433271,0,0,-8184,0,0,-8016,0,0,-8927,0,0,375943,0,0,773928,0,0,744199,0,0,446327,0,0,816638,0,0,792434,0,0,804502,0,0,6026,4,50643,"UR","ST" 33,17,1,2,1,41,2,"COMMONWEALTH EDISON CO","BYRON",0,"NUCLEAR",4110,"0M",1294,,100,95,753651,0,0,166639,0,0,50362,0,0,767250,0,0,824285,0,0,786866,0,0,797334,0,0,811901,0,0,764206,0,0,832898,0,0,804540,0,0,823838,0,0,6023,4,50643,"UR","ST" 33,17,1,2,1,41,2,"COMMONWEALTH EDISON CO","BRAIDWOOD",0,"NUCLEAR",4110,"0M",1294,,100,95,839335,0,0,759006,0,0,840028,0,0,777131,0,0,635751,0,0,794146,0,0,802182,0,0,795885,0,0,801537,0,0,846700,0,0,810185,0,0,831152,0,0,6022,4,50643,"UR","ST" 33,17,1,2,1,41,2,"COMMONWEALTH EDISON CO","QUAD CITIES",0,"NUCLEAR",4110,"0M",1294,,100,95,501116,0,0,453211,0,0,58157,0,0,-5752,0,0,-5952,0,0,-5994,0,0,-6618,0,0,93771,0,0,422180,0,0,318808,0,0,77988,0,0,571746,0,0,880,4,50643,"UR","ST" 33,17,1,2,1,41,2,"COMMONWEALTH EDISON CO","DRESDEN",0,"NUCLEAR",4110,"0M",1294,,100,95,535595,0,0,493244,0,0,81638,0,0,302574,0,0,449851,0,0,27639,0,0,-3615,0,0,-4287,0,0,-5566,0,0,-5704,0,0,-5672,0,0,-5963,0,0,869,4,50643,"UR","ST" 33,17,1,2,1,41,3,"COMMONWEALTH EDISON CO","DRESDEN",0,"NUCLEAR",4110,"0M",1294,,100,95,420814,0,0,506779,0,0,533907,0,0,467390,0,0,432429,0,0,-5060,0,0,-3401,0,0,-3807,0,0,41448,0,0,138092,0,0,358426,0,0,577978,0,0,869,4,50643,"UR","ST" 33,17,1,4,2,41,4,"COMMONWEALTH EDISON CO","BLOOM",0,"LIGHT OIL",4110,"0M",1294,,100,95,0,0,15589,0,0,15589,69,87,15502,0,0,15495,0,0,15495,0,0,15475,146,497,14951,792,2784,12167,0,0,15755,0,0,15755,0,0,15755,1,3,15739,865,4,50643,"FO2","GT" 33,17,1,4,2,41,6,"COMMONWEALTH EDISON CO","CALUMET",0,"LIGHT OIL",4110,"0M",1294,,100,95,0,0,16437,0,0,16437,0,0,16437,145,127,16310,0,0,16310,0,0,16310,593,2028,14281,508,1365,12917,0,0,15298,0,0,15298,0,0,15298,0,0,15298,866,4,50643,"FO2","GT" 33,17,1,4,9,41,6,"COMMONWEALTH EDISON CO","CALUMET",0,"NAT GAS",4110,"0M",1294,,100,95,0,0,0,68,1045,0,0,8,0,0,0,0,62,540,0,0,0,0,2902,56071,0,3743,56299,0,1,46,0,106,1474,0,29,760,0,0,0,0,866,4,50643,"NG","GT" 33,17,1,2,6,41,10,"COMMONWEALTH EDISON CO","CRAWFORD",0,"BIT COAL",4110,"0M",1294,,100,95,79127,52566,254284,56492,34236,247898,154770,96060,204338,157819,95401,178999,77964,50034,154295,195593,125311,78949,167051,106642,75986,220876,140947,52693,111791,74002,178401,100936,63677,173394,171688,108863,144620,107184,68961,169485,867,4,50643,"BIT","ST" 33,17,1,2,9,41,10,"COMMONWEALTH EDISON CO","CRAWFORD",0,"NAT GAS",4110,"0M",1294,,100,95,4191,46278,0,3822,41541,0,6151,66002,0,6881,74296,0,3205,34575,0,3676,39819,0,4307,47007,0,11765,128609,0,2943,33297,0,3202,34374,0,2534,27690,0,3684,42386,0,867,4,50643,"NG","ST" 33,17,1,4,2,41,10,"COMMONWEALTH EDISON CO","CRAWFORD",0,"LIGHT OIL",4110,"0M",1294,,100,95,39,239,11718,31,208,15427,7,85,15342,60,196,15146,0,0,15146,145,654,14492,207,1709,12783,90,287,12496,0,0,12495,0,0,12495,5,41,12453,0,0,12451,867,4,50643,"FO2","GT" 33,17,1,4,9,41,10,"COMMONWEALTH EDISON CO","CRAWFORD",0,"NAT GAS",4110,"0M",1294,,100,95,99,3367,0,462,10721,0,90,6128,0,496,8920,0,41,832,0,2338,60078,0,1956,92769,0,6353,117178,0,232,23469,0,130,22477,0,606,26280,0,716,38106,0,867,4,50643,"NG","GT" 33,17,1,2,2,41,16,"COMMONWEALTH EDISON CO","JOLIET",0,"LIGHT OIL",4110,"0M",1294,,100,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,874,4,50643,"FO2","ST" 33,17,1,2,6,41,16,"COMMONWEALTH EDISON CO","JOLIET",0,"BIT COAL",4110,"0M",1294,,100,95,122495,69041,120326,93234,54624,109729,118689,69742,107396,119799,68307,78398,7077,4459,86216,111744,65001,89393,128830,75618,81101,97034,56642,114450,105402,58755,119892,105052,56846,73967,38927,23143,87158,80786,46625,136310,874,4,50643,"BIT","ST" 33,17,1,2,9,41,16,"COMMONWEALTH EDISON CO","JOLIET",0,"NAT GAS",4110,"0M",1294,,100,95,2191,22095,0,1467,15220,0,2310,24340,0,2244,23500,0,166,1970,0,2208,24000,0,2239,22730,0,1106,11930,0,1732,18230,0,1439,14430,0,1402,15430,0,1598,17620,0,874,4,50643,"NG","ST" 33,17,1,3,2,41,16,"COMMONWEALTH EDISON CO","JOLIET",0,"LIGHT OIL",4110,"0M",1294,,100,95,28,24,0,19,36,0,26,24,0,38,121,0,42,65,0,45,88,0,191,342,0,177,323,0,43,60,8,25,36,0,50,114,0,33,48,0,874,4,50643,"FO2","IC" 33,17,1,4,2,41,16,"COMMONWEALTH EDISON CO","JOLIET",0,"LIGHT OIL",4110,"0M",1294,,100,95,0,0,12982,0,0,12946,0,0,13461,0,0,13339,0,0,11260,0,0,11071,56,101,11058,0,0,11182,0,0,11123,0,0,11087,0,0,11349,0,0,11301,874,4,50643,"FO2","GT" 33,17,1,4,9,41,16,"COMMONWEALTH EDISON CO","JOLIET",0,"NAT GAS",4110,"0M",1294,,100,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1395,27871,0,8945,90787,0,8183,223338,0,866,13196,0,229,3746,0,131,5138,0,234,3377,0,874,4,50643,"NG","GT" 33,17,1,2,2,41,17,"COMMONWEALTH EDISON CO","JOLIET 7&8",0,"LIGHT OIL",4110,"0M",1294,,100,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,384,4,50643,"FO2","ST" 33,17,1,2,6,41,17,"COMMONWEALTH EDISON CO","JOLIET 7&8",0,"BIT COAL",4110,"0M",1294,,100,95,520241,284540,251012,441016,243169,314690,475210,271066,278538,286729,169187,274394,417122,253105,368822,380291,234398,349806,434794,265270,338716,502962,304953,251022,375036,226403,245187,274949,166801,229512,204177,119561,295972,195022,118007,392005,384,4,50643,"BIT","ST" 33,17,1,2,9,41,17,"COMMONWEALTH EDISON CO","JOLIET 7&8",0,"NAT GAS",4110,"0M",1294,,100,95,11103,108953,0,8750,87209,0,12754,127880,0,12398,126498,0,15389,159604,0,14468,153070,0,34003,358096,0,38820,399592,0,12449,130392,0,5845,61103,0,9664,99401,0,15109,163833,0,384,4,50643,"NG","ST" 33,17,1,2,2,41,18,"COMMONWEALTH EDISON CO","KINCAID",0,"LIGHT OIL",4110,"0M",1294,,100,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,876,4,50643,"FO2","ST" 33,17,1,2,6,41,18,"COMMONWEALTH EDISON CO","KINCAID",0,"BIT COAL",4110,"0M",1294,,100,95,55770,32758,306574,225554,110119,355485,177700,87847,323621,111716,54633,362527,59730,40786,398523,326434,167542,321546,302831,139901,261736,370353,171207,168914,152028,76179,217203,146493,75067,252142,105685,62572,325669,303394,153078,287687,876,4,50643,"BIT","ST" 33,17,1,2,9,41,18,"COMMONWEALTH EDISON CO","KINCAID",0,"NAT GAS",4110,"0M",1294,,100,95,1202,16174,0,747,8607,0,913,10721,0,996,11458,0,1078,14934,0,450,5024,0,586,6470,0,981,10590,0,742,8548,0,1541,18276,0,2200,30312,0,917,10402,0,876,4,50643,"NG","ST" 33,17,1,4,2,41,19,"COMMONWEALTH EDISON CO","LOMBARD",0,"LIGHT OIL",4110,"0M",1294,,100,95,0,0,16204,0,0,16203,0,2,15828,0,0,15828,0,0,15471,0,0,15471,0,0,15471,0,0,15471,0,0,15471,0,0,15471,0,0,15471,0,0,15471,877,4,50643,"FO2","GT" 33,17,1,4,9,41,19,"COMMONWEALTH EDISON CO","LOMBARD",0,"NAT GAS",4110,"0M",1294,,100,95,0,0,0,0,0,0,216,9440,0,28,3677,0,45,1042,0,1545,52076,0,2695,90228,0,4011,66015,0,277,4570,0,110,2620,0,70,1556,0,6,1352,0,877,4,50643,"NG","GT" 33,17,1,4,2,41,22,"COMMONWEALTH EDISON CO","EL JUNCTION",0,"LIGHT OIL",4110,"0M",1294,,100,95,0,0,16029,0,0,16029,0,0,16029,0,0,16029,0,0,16029,0,0,16029,0,0,16029,0,0,16029,0,0,16029,0,0,16029,0,0,16029,0,0,16029,870,4,50643,"FO2","GT" 33,17,1,4,9,41,22,"COMMONWEALTH EDISON CO","EL JUNCTION",0,"NAT GAS",4110,"0M",1294,,100,95,45,1465,0,255,9385,0,433,17490,0,266,17646,0,201,1306,0,3974,165292,0,3141,117346,0,6577,120875,0,317,6236,0,0,0,0,0,0,0,0,0,0,870,4,50643,"NG","GT" 33,17,1,2,2,41,25,"COMMONWEALTH EDISON CO","POWERTON",0,"LIGHT OIL",4110,"0M",1294,,100,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,879,4,50643,"FO2","ST" 33,17,1,2,6,41,25,"COMMONWEALTH EDISON CO","POWERTON",0,"BIT COAL",4110,"0M",1294,,100,95,295687,209649,423935,447158,294017,440451,348046,239570,435308,212232,137447,636432,150582,105273,808681,358461,251527,710182,600064,381559,542202,449473,321219,483261,473891,314575,379942,711307,426764,426047,347462,223314,654319,369211,237119,790527,879,4,50643,"BIT","ST" 33,17,1,2,9,41,25,"COMMONWEALTH EDISON CO","POWERTON",0,"NAT GAS",4110,"0M",1294,,100,95,2163,27135,0,934,10806,0,1060,12568,0,352,4015,0,411,4960,0,1912,23178,0,1304,14277,0,344,4172,0,2982,34612,0,1175,12623,0,1089,12285,0,860,10186,0,879,4,50643,"NG","ST" 33,17,1,4,2,41,34,"COMMONWEALTH EDISON CO","SABROOKE",0,"LIGHT OIL",4110,"0M",1294,,100,95,0,0,10453,0,0,10453,0,0,10453,0,0,10453,0,0,10453,1060,4114,11113,2120,6610,10937,3819,12030,8749,0,0,10491,0,0,10491,92,332,10159,19,57,10102,882,4,50643,"FO2","GT" 33,17,1,2,6,41,35,"COMMONWEALTH EDISON CO","FISK ST",0,"BIT COAL",4110,"0M",1294,,100,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1258,2813,0,64730,37523,0,49452,31868,0,82828,51049,0,0,0,0,0,0,0,886,4,50643,"BIT","ST" 33,17,1,2,9,41,35,"COMMONWEALTH EDISON CO","FISK ST",0,"NAT GAS",4110,"0M",1294,,100,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,950,35700,0,6315,65190,0,4278,50522,0,3262,35967,0,0,0,0,0,0,0,886,4,50643,"NG","ST" 33,17,1,3,2,41,35,"COMMONWEALTH EDISON CO","FISK ST",0,"LIGHT OIL",4110,"0M",1294,,100,95,45,155,416,0,0,416,77,84,332,39,37,295,68,30,266,66,86,180,134,219,491,125,84,407,40,16,391,17,100,291,19,95,196,0,0,174,886,4,50643,"FO2","IC" 33,17,1,4,2,41,35,"COMMONWEALTH EDISON CO","FISK ST",0,"LIGHT OIL",4110,"0M",1294,,100,95,1,5,23532,47,93,23145,99,257,23261,297,889,22373,31,91,22630,3411,9368,21922,4887,12963,23223,4869,20375,20364,0,0,20364,0,0,20364,335,1236,19127,365,1339,17788,886,4,50643,"FO2","GT" 33,17,1,2,2,41,40,"COMMONWEALTH EDISON CO","WAUKEGAN",0,"LIGHT OIL",4110,"0M",1294,,100,95,895,1547,2815,3612,6129,2742,4931,8714,2873,777,1407,3668,959,1672,3660,3946,7104,2494,3955,7041,2217,5282,9737,2829,3119,5998,3784,2859,5228,2552,3518,6749,3529,1606,3513,2435,883,4,50643,"FO2","ST" 33,17,1,2,6,41,40,"COMMONWEALTH EDISON CO","WAUKEGAN",0,"BIT COAL",4110,"0M",1294,,100,95,297287,177180,273721,300831,175220,239888,317665,191650,286982,225455,141450,324935,256271,154756,392524,243529,150801,389581,310909,188184,335255,296518,187813,197729,119579,79260,209183,165704,104633,209690,128110,85584,284788,41660,30532,414595,883,4,50643,"BIT","ST" 33,17,1,2,9,41,40,"COMMONWEALTH EDISON CO","WAUKEGAN",0,"NAT GAS",4110,"0M",1294,,100,95,1435,14340,0,1745,16984,0,6345,64552,0,12306,127984,0,2631,26534,0,2700,27935,0,4475,45751,0,8173,86616,0,1604,17712,0,0,0,0,0,0,0,1606,20058,0,883,4,50643,"NG","ST" 33,17,1,4,2,41,40,"COMMONWEALTH EDISON CO","WAUKEGAN",0,"LIGHT OIL",4110,"0M",1294,,100,95,311,627,9084,81,252,8832,0,0,8832,62,220,8612,0,0,8612,2971,8993,7575,4093,8993,10099,3465,12846,8690,217,650,9693,15,46,9832,388,721,9111,455,101,8825,883,4,50643,"FO2","GT" 33,17,1,2,2,41,45,"COMMONWEALTH EDISON CO","WILL COUNTY",0,"LIGHT OIL",4110,"0M",1294,,100,95,1062,18762,3939,7295,13109,3758,10624,18496,3941,8221,14895,3199,9084,16531,4090,8920,16134,4050,10413,17507,4073,8717,15307,3888,6246,11354,3823,8028,14057,4581,13300,23039,4265,11454,20638,3742,884,4,50643,"FO2","ST" 33,17,1,2,6,41,45,"COMMONWEALTH EDISON CO","WILL COUNTY",0,"BIT COAL",4110,"0M",1294,,100,95,339333,214481,728644,276729,163281,493423,436182,242324,418178,363653,209416,394195,307990,182353,450891,397251,238256,419768,378522,212664,447725,475303,276214,354866,276771,166573,326404,319122,188012,314278,367545,210217,297641,236545,145482,315427,884,4,50643,"BIT","ST" 33,17,1,2,2,41,60,"COMMONWEALTH EDISON CO","COLLINS",0,"LIGHT OIL",4110,"0M",1294,,100,95,44,168,8953,149,398,8555,143,315,8240,46,189,8051,8,33,9226,37,94,9132,118,236,8896,161,333,8562,33,186,8376,121,346,8030,407,870,7160,418,907,6253,6025,4,50643,"FO2","ST" 33,17,1,2,3,41,60,"COMMONWEALTH EDISON CO","COLLINS",0,"HEAVY OIL",4110,"0M",1294,,100,95,10708,14958,858168,17136,41575,816594,22453,44431,829903,5094,19291,887973,1621,6324,924611,37801,79457,874073,46886,87834,814064,170809,316836,497228,8876,46988,565732,30191,78409,602644,60143,118667,704727,63549,126751,840744,6025,4,50643,"FO6","ST" 33,17,1,2,9,41,60,"COMMONWEALTH EDISON CO","COLLINS",0,"NAT GAS",4110,"0M",1294,,100,95,39831,890044,0,143526,2177150,0,287955,3565711,0,53575,1269470,0,42336,1034381,0,242662,3192054,0,342245,4012183,0,559661,6496563,0,22424,742913,0,72437,1176239,0,234867,2894481,0,189527,2361026,0,6025,4,50643,"NG","ST" 33,17,1,2,2,59,5,"ELECTRIC ENERGY INC","JOPPA STEAM",0,"LIGHT OIL",5748,"0M",1294,,,95,200,374,1123,39,70,1273,99,185,1072,621,1113,2510,355,632,917,223,421,1063,108,203,1046,324,609,1093,203,369,937,141,253,1041,23,42,874,163,297,1013,887,4,50877,"FO2","ST" 33,17,1,2,6,59,5,"ELECTRIC ENERGY INC","JOPPA STEAM",0,"BIT COAL",5748,"0M",1294,,,95,714619,413405,218343,620332,359921,257338,581511,352021,367649,615267,357331,494389,555217,326921,554836,664604,410139,566371,692201,431949,348896,616065,383985,389108,610216,368490,418929,705090,420489,495502,724030,433000,497231,719491,431637,526478,887,4,50877,"BIT","ST" 33,17,1,2,9,59,5,"ELECTRIC ENERGY INC","JOPPA STEAM",0,"NAT GAS",5748,"0M",1294,,,95,3,39,0,3,32,0,2,31,0,4,42,0,2,29,0,3,39,0,2,28,0,2,25,0,2,30,0,3,33,0,4,43,0,2,27,0,887,4,50877,"NG","ST" 33,17,1,2,1,72,1,"ILLINOIS POWER CO","CLINTON",0,"NUCLEAR",9208,"0M",1294,,,95,606581,0,0,556463,0,0,137066,0,0,-6903,0,0,405888,0,0,658164,0,0,673318,0,0,670862,0,0,558375,0,0,682367,0,0,659454,0,0,500645,0,0,204,4,51385,"UR","ST" 33,17,1,2,"C",72,20,"ILLINOIS POWER CO","BALDWIN",0,"TIRES",9208,"0M",294,"A",,95,0,0,0,1818,0,0,3181,0,0,7099,0,0,6807,0,0,5350,0,0,7244,0,0,3493,0,0,6277,0,0,7534,0,0,10681,0,0,7569,0,0,889,4,51385,"TIR","ST" 33,17,1,2,2,72,20,"ILLINOIS POWER CO","BALDWIN",0,"LIGHT OIL",9208,"0M",1294,,,95,1081,1918,2086,605,1061,2802,687,1177,4303,886,1546,2758,788,1102,2909,1035,1849,3333,1018,1819,2723,194,347,3603,519,926,3761,917,1661,2395,449,802,2830,719,1288,2830,889,4,51385,"FO2","ST" 33,17,1,2,6,72,20,"ILLINOIS POWER CO","BALDWIN",0,"BIT COAL",9208,"0M",1294,,,95,660540,312984,326606,560194,261218,347154,721218,332734,317839,1001149,461485,170294,940043,347817,194365,784737,373003,199111,952571,453263,98640,1114689,528001,10906,767993,364295,81430,684089,329233,150289,880194,419001,132828,809209,388865,132828,889,4,51385,"BIT","ST" 33,17,1,2,2,72,35,"ILLINOIS POWER CO","HAVANA",0,"LIGHT OIL",9208,"0M",1294,,,95,910,1948,1153,666,1365,840,307,580,1330,461,889,1682,716,1472,1237,733,1517,1451,606,1199,1513,905,1843,2122,693,1487,1847,988,1998,879,1035,1991,1192,678,1527,1192,891,4,51385,"FO2","ST" 33,17,1,2,3,72,35,"ILLINOIS POWER CO","HAVANA",0,"HEAVY OIL",9208,"0M",1294,,,95,0,0,11893,0,0,11893,0,0,11893,0,0,11893,0,0,11893,0,0,11893,0,0,11893,0,0,11893,0,0,11893,0,0,11893,0,0,362,0,0,362,891,4,51385,"FO6","ST" 33,17,1,2,6,72,35,"ILLINOIS POWER CO","HAVANA",0,"BIT COAL",9208,"0M",1294,,,95,98112,49256,30789,118979,58411,50159,224224,102634,40379,160060,74936,66818,118264,58880,70245,116146,58574,89918,115561,56674,118529,151230,75783,90549,71688,37378,112421,88892,44663,121996,115087,53793,99387,131730,71564,99387,891,4,51385,"BIT","ST" 33,17,1,2,9,72,35,"ILLINOIS POWER CO","HAVANA",0,"NAT GAS",9208,"0M",1294,,,95,1067,12979,0,440,5089,0,63,677,0,179,1951,0,351,4046,0,300,3543,0,463,5170,0,355,4086,0,402,4873,0,559,6392,0,891,9670,0,763,9698,0,891,4,51385,"NG","ST" 33,17,1,2,2,72,37,"ILLINOIS POWER CO","HENNEPIN",0,"LIGHT OIL",9208,"0M",1294,,,95,0,0,139,0,0,118,0,0,98,0,0,73,0,0,226,0,0,198,0,0,171,0,0,143,0,0,124,0,0,81,0,0,206,0,0,206,892,4,51385,"FO2","ST" 33,17,1,2,6,72,37,"ILLINOIS POWER CO","HENNEPIN",0,"BIT COAL",9208,"0M",1294,,,95,87360,41868,110995,113939,53993,91245,148496,70812,66931,128982,61958,52605,126965,61905,34055,114742,56218,13963,122662,60852,24745,143091,72106,29954,79631,39909,56695,59580,30905,81408,39508,20500,71977,116352,56957,71977,892,4,51385,"BIT","ST" 33,17,1,2,9,72,37,"ILLINOIS POWER CO","HENNEPIN",0,"NAT GAS",9208,"0M",1294,,,95,32318,326516,0,1234,12249,0,1222,12243,0,808,8187,0,416,4252,0,2050,20916,0,733,7579,0,551,5765,0,776,8044,0,87,951,0,169,1816,0,493,5034,0,892,4,51385,"NG","ST" 33,17,1,4,2,72,39,"ILLINOIS POWER CO","OGLESBY",0,"LIGHT OIL",9208,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,8629,0,0,8629,0,0,8629,0,0,8629,0,0,8629,0,0,8629,0,0,8629,0,0,8805,0,0,8805,894,4,51385,"FO2","GT" 33,17,1,4,9,72,39,"ILLINOIS POWER CO","OGLESBY",0,"NAT GAS",9208,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,2951,33996,0,2725,56764,0,0,0,0,110,1650,0,0,0,0,519,7497,0,894,4,51385,"NG","GT" 33,17,1,4,2,72,40,"ILLINOIS POWER CO","STALLINGS",0,"LIGHT OIL",9208,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,895,4,51385,"FO2","GT" 33,17,1,4,9,72,40,"ILLINOIS POWER CO","STALLINGS",0,"NAT GAS",9208,"0M",1294,,,95,-5,0,0,0,0,0,-188,0,0,-57,0,0,-40,0,0,-31,0,0,556,11621,0,1460,27572,0,-38,0,0,-159,0,0,0,0,0,40,1636,0,895,4,51385,"NG","GT" 33,17,1,2,2,72,45,"ILLINOIS POWER CO","VERMILION",0,"LIGHT OIL",9208,"0M",1294,,,95,115,249,624,91,198,602,191,417,364,236,549,361,18,38,279,0,0,257,0,0,333,0,0,327,0,0,327,0,0,284,0,0,284,0,0,284,897,4,51385,"FO2","ST" 33,17,1,2,6,72,45,"ILLINOIS POWER CO","VERMILION",0,"BIT COAL",9208,"0M",1294,,,95,30154,17048,27000,17324,9743,30113,23022,12947,17166,26005,15643,2483,5797,3221,2966,977,640,2326,0,0,2326,0,0,2326,0,0,2326,0,0,2326,-194,0,2326,0,0,2326,897,4,51385,"BIT","ST" 33,17,1,2,9,72,45,"ILLINOIS POWER CO","VERMILION",0,"NAT GAS",9208,"0M",794,"A",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,35157,523154,0,35815,280703,0,5530,63136,0,-181,425,0,0,0,0,0,0,0,897,4,51385,"NG","ST" 33,17,1,4,2,72,45,"ILLINOIS POWER CO","VERMILION",0,"LIGHT OIL",9208,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,-967,0,0,13,1679,0,0,0,0,0,0,0,897,4,51385,"FO2","GT" 33,17,1,2,"B",72,50,"ILLINOIS POWER CO","WOOD RIVER",0,"WOOD",9208,"0M",294,"A",,95,0,0,0,16,0,0,178,0,0,229,0,0,90,0,0,216,0,0,58,0,0,48,0,0,0,0,0,0,0,0,0,0,0,18,0,0,898,4,51385,"WD","ST" 33,17,1,2,2,72,50,"ILLINOIS POWER CO","WOOD RIVER",0,"LIGHT OIL",9208,"0M",1294,,,95,44,79,5600,23,43,5507,47,83,5347,40,74,5395,21,44,5332,24,48,5204,12,23,5294,49,90,5144,25,46,5028,38,67,5235,0,0,4820,0,0,4820,898,4,51385,"FO2","ST" 33,17,1,2,6,72,50,"ILLINOIS POWER CO","WOOD RIVER",0,"BIT COAL",9208,"0M",1294,,,95,179203,74998,45031,134748,57471,69498,189897,79401,76252,58215,25205,85871,13578,6765,84103,56995,25313,99570,176787,75799,113318,203949,86831,93346,141728,61520,85883,170165,70959,78358,166564,67877,95046,152328,67698,95046,898,4,51385,"BIT","ST" 33,17,1,2,9,72,50,"ILLINOIS POWER CO","WOOD RIVER",0,"NAT GAS",9208,"0M",1294,,,95,2917,29530,0,3161,32758,0,2112,21194,0,620,6474,0,455,5401,0,3940,43447,0,1042,11274,0,7813,79539,0,841,8463,0,2100,20806,0,1416,13732,0,3310,34114,0,898,4,51385,"NG","ST" 33,17,1,1,,76,5,"MIDAMERICAN ENERGY","MOLINE",0,,9438,"0M",1294,,50,95,867,0,0,502,0,0,693,0,0,501,0,0,751,0,0,1306,0,0,1909,0,0,1606,0,0,1628,0,0,1499,0,0,1295,0,0,824,0,0,899,5,51406,"WAT","HY" 33,17,1,4,2,76,5,"MIDAMERICAN ENERGY","MOLINE",0,"LIGHT OIL",9438,"0M",1294,,50,95,-104,1,1972,-89,0,1972,-80,0,1972,0,0,1972,0,0,1972,0,0,1972,0,0,1972,0,0,1972,-1,0,1972,-33,0,1972,-32,0,1972,-41,0,1972,899,5,51406,"FO2","GT" 33,17,1,4,9,76,5,"MIDAMERICAN ENERGY","MOLINE",0,"NAT GAS",9438,"0M",1294,,50,95,0,0,0,0,0,0,0,0,0,0,0,0,-61,2,0,1064,18944,0,1548,27660,0,1838,32171,0,-50,33,0,-34,0,0,-33,0,0,-42,0,0,899,5,51406,"NG","GT" 33,17,1,1,,107,1,"NATIONAL HYDRO","DAYTON",0,,9366,"0A",1294,,,95,1202,0,0,1122,0,0,1638,0,0,1567,0,0,992,0,0,1383,0,0,911,0,0,403,0,0,0,0,0,0,0,0,1259,0,0,1438,0,0,901,4,52081,"WAT","HY" 33,17,1,1,,134,1,"SO BELOIT WTR GAS & ELEC","ROCKTON",0,,17535,"0A",1294,,521,95,467,0,0,390,0,0,678,0,0,788,0,0,728,0,0,505,0,0,154,0,0,655,0,0,616,0,0,694,0,0,698,0,0,536,0,0,903,4,54026,"WAT","HY" 33,17,1,2,2,151,15,"UNION ELECTRIC CO","VENICE",0,"LIGHT OIL",19436,"0M",1294,,150,95,-14,55,40501,-148,624,39877,0,0,39877,0,0,39877,1716,6693,33184,1509,6175,27009,165,558,26451,1421,5295,29829,0,0,33009,0,0,33009,63,822,32186,-598,1970,30216,913,4,52997,"FO2","ST" 33,17,1,2,9,151,15,"UNION ELECTRIC CO","VENICE",0,"NAT GAS",19436,"0M",1294,,150,95,-1037,23078,0,-714,17082,0,745,29759,0,2615,70964,0,3881,85875,0,3694,85747,0,12175,233282,0,18970,400955,0,1254,9297,0,1125,26918,0,146,10894,0,-478,8990,0,913,4,52997,"NG","ST" 33,17,1,4,2,151,15,"UNION ELECTRIC CO","VENICE",0,"LIGHT OIL",19436,"0M",1294,,150,95,-67,27,1614,-28,163,2000,-35,94,1906,-28,27,1879,-20,89,1790,-20,0,1790,170,758,2114,425,1509,1672,-19,2,1670,-26,4,1666,-54,3,1664,-53,1,1663,913,4,52997,"FO2","GT" 33,17,5,2,2,528,1,"BREESE (CITY OF)","BREESE",0,"LIGHT OIL",2188,"0A",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,934,4,50322,"FO2","ST" 33,17,5,3,2,528,1,"BREESE (CITY OF)","BREESE",0,"LIGHT OIL",2188,"0A",1294,,,95,0,54,940,18,32,905,18,33,866,22,40,817,30,30,781,17,32,740,176,328,755,261,482,780,19,35,911,19,35,872,19,34,835,13,22,811,934,4,50322,"FO2","IC" 33,17,5,3,9,528,1,"BREESE (CITY OF)","BREESE",0,"NAT GAS",2188,"0A",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,934,4,50322,"NG","IC" 33,17,5,3,2,530,1,"BUSHNELL (CITY OF)","BUSHNELL",0,"LIGHT OIL",2634,"0A",1294,,,95,0,1,838,7,14,824,0,0,824,0,0,824,0,0,824,0,0,824,29,58,766,0,0,766,0,0,766,0,0,766,0,0,766,0,0,766,935,4,50383,"FO2","IC" 33,17,5,3,9,530,1,"BUSHNELL (CITY OF)","BUSHNELL",0,"NAT GAS",2634,"0A",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,935,4,50383,"NG","IC" 33,17,5,3,2,534,1,"CARLYLE (CITY OF)","CARLYLE",0,"LIGHT OIL",3037,"0A",1294,,,95,12,16,176,0,13,163,9,11,151,9,13,138,12,10,121,51,53,404,141,155,248,144,203,381,11,12,368,10,17,351,11,18,333,0,0,333,936,4,50438,"FO2","IC" 33,17,5,3,9,534,1,"CARLYLE (CITY OF)","CARLYLE",0,"NAT GAS",3037,"0A",1294,,,95,0,3,0,0,2,0,0,2,0,0,3,0,0,3,0,1,11,0,10,64,0,4,38,0,0,6,0,0,6,0,0,0,0,0,0,0,936,4,50438,"NG","IC" 33,17,5,3,2,537,1,"CARMI (CITY OF)","CARMI",0,"LIGHT OIL",3040,"0A",1294,,,95,16,38,765,95,45,720,10,19,700,7,19,681,5,21,660,5,32,627,5,12,616,9,15,600,18,53,722,9,20,702,10,22,702,61,90,590,937,4,50440,"FO2","IC" 33,17,5,3,9,537,1,"CARMI (CITY OF)","CARMI",0,"NAT GAS",3040,"0A",1294,,,95,70,720,0,25,1014,0,15,177,0,17,350,0,16,125,0,26,162,0,15,157,0,11,87,0,40,313,0,11,92,0,8,100,0,83,985,0,937,4,50440,"NG","IC" 33,17,5,2,6,559,1,"FAIRFIELD (CITY OF)","FAIRFIELD",0,"BIT COAL",6141,"0A",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,940,4,50941,"BIT","ST" 33,17,5,3,2,559,1,"FAIRFIELD (CITY OF)","FAIRFIELD",0,"LIGHT OIL",6141,"0A",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,940,4,50941,"FO2","IC" 33,17,5,3,9,559,1,"FAIRFIELD (CITY OF)","FAIRFIELD",0,"NAT GAS",6141,"0A",1294,"S",,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,940,4,50941,"NG","IC" 33,17,5,3,2,562,1,"FARMER (CITY OF)","FARMER CITY",0,"LIGHT OIL",6192,"0A",1294,,,95,1,3,227,0,0,227,0,0,227,0,0,227,1,2,230,10,20,208,7,23,186,38,71,283,4,4,279,0,0,279,0,0,274,0,0,274,941,4,50955,"FO2","IC" 33,17,5,3,9,562,1,"FARMER (CITY OF)","FARMER CITY",0,"NAT GAS",6192,"0A",1294,,,95,3,26,0,0,0,0,0,0,0,0,0,0,6,58,0,46,504,0,0,0,0,163,1723,0,0,0,0,0,0,0,0,0,0,0,0,0,941,4,50955,"NG","IC" 33,17,5,3,2,571,1,"FREEBURG (CITY OF)","FREEBURG",0,"LIGHT OIL",6764,"0A",1294,,,95,1,2,129,17,33,214,173,298,93,12,23,70,12,23,47,13,26,197,81,158,39,110,201,200,13,177,0,8,16,161,8,10,151,8,21,130,943,4,51056,"FO2","IC" 33,17,5,3,9,571,1,"FREEBURG (CITY OF)","FREEBURG",0,"NAT GAS",6764,"0A",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,943,4,51056,"NG","IC" 33,17,5,3,2,574,1,"GENESEO (CITY OF)","GENESEO",0,"LIGHT OIL",7095,"0A",1294,,,95,2,16,314,4,11,301,0,13,290,5,13,281,0,0,294,15,26,446,65,111,339,78,133,383,0,0,389,0,0,388,0,0,389,2,4,385,944,4,51093,"FO2","IC" 33,17,5,3,9,574,1,"GENESEO (CITY OF)","GENESEO",0,"NAT GAS",7095,"0A",1294,,,95,7,250,0,2,57,0,7,527,0,2,52,0,0,0,0,93,1716,0,562,6490,0,735,8338,0,0,0,0,0,0,0,0,0,0,0,1,0,944,4,51093,"NG","IC" 33,17,5,3,2,589,1,"HIGHLAND (CITY OF)","HIGHLAND",0,"LIGHT OIL",8573,"0A",1294,,,95,21,37,490,4,5,486,0,0,486,4,9,823,0,0,825,47,78,792,28,140,634,472,536,371,24,46,371,0,0,322,11,21,755,8,15,754,946,4,51298,"FO2","IC" 33,17,5,3,9,589,1,"HIGHLAND (CITY OF)","HIGHLAND",0,"NAT GAS",8573,"0A",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,946,4,51298,"NG","IC" 33,17,5,3,2,606,15,"MCLEANSBORO (CITY OF)","MCLEANSBORO",0,"LIGHT OIL",12167,"0A",1294,,,95,19,48,201,15,25,176,12,30,322,14,21,301,14,29,272,11,29,243,22,38,205,14,48,336,43,88,246,25,45,201,27,51,325,20,34,291,948,4,51812,"FO2","IC" 33,17,5,3,2,612,10,"MASCOUTAH (CITY OF)","MASCOUTAH",0,"LIGHT OIL",11790,"0A",1294,,,95,0,0,815,0,0,815,0,0,814,1,12,803,24,59,563,0,0,563,4,56,859,30,64,967,0,0,967,0,0,967,0,0,965,0,0,966,950,4,51789,"FO2","IC" 33,17,5,3,9,612,10,"MASCOUTAH (CITY OF)","MASCOUTAH",0,"NAT GAS",11790,"0A",1294,,,95,0,0,0,0,0,0,0,0,0,10,410,0,0,0,0,0,0,0,74,4890,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,950,4,51789,"NG","IC" 33,17,5,2,9,646,1,"PERU (CITY OF)","PERU",0,"NAT GAS",14840,"0M",1294,,,95,-15,0,0,-11,0,0,4,0,0,-13,0,0,-7,0,0,77,680,0,-9,0,0,-62,0,0,0,0,0,8,0,0,0,0,0,0,0,0,955,4,52299,"NG","ST" 33,17,5,3,2,646,1,"PERU (CITY OF)","PERU",0,"LIGHT OIL",14840,"0M",1294,,,95,-30,12,619,-13,24,595,-13,23,572,-6,24,548,-2,23,525,63,146,560,189,366,550,299,560,533,-14,0,533,-1,23,510,-22,12,498,-33,0,498,955,4,52299,"FO2","IC" 33,17,5,4,2,646,1,"PERU (CITY OF)","PERU",0,"LIGHT OIL",14840,"0M",1294,,,95,-17,5,621,-6,30,547,-28,31,516,-11,19,497,2,45,621,32,120,501,-5,0,501,78,277,563,-5,0,563,2,31,532,-6,34,498,-8,0,498,955,4,52299,"FO2","GT" 33,17,5,3,2,649,15,"PRINCETON (CITY OF)","PRINCETON",0,"LIGHT OIL",15388,"0M",1294,,,95,6,12,977,0,0,976,3,7,975,2,4,971,3,7,975,23,40,932,56,97,838,536,913,802,20,35,768,17,32,720,0,3,712,14,25,688,957,4,52397,"FO2","IC" 33,17,5,3,9,649,15,"PRINCETON (CITY OF)","PRINCETON",0,"NAT GAS",15388,"0M",1294,,,95,21,220,0,0,0,0,27,268,0,15,153,0,24,231,0,137,1308,0,636,6226,0,1790,17269,0,131,1265,0,82,827,0,0,106,0,75,752,0,957,4,52397,"NG","IC" 33,17,5,3,2,652,15,"RANTOUL (CITY OF)","RANTOUL",0,"LIGHT OIL",15686,"0A",1294,,,95,18,21,236,2,5,232,6,12,220,11,25,195,23,32,203,55,112,186,16,31,295,0,0,299,0,0,299,8,15,284,0,0,284,0,0,284,958,4,52436,"FO2","IC" 33,17,5,3,2,655,1,"RED BUD (CITY OF)","RED BUD",0,"LIGHT OIL",15772,"0A",1294,,,95,28,56,1047,2,5,1040,2,3,1034,0,1,1030,4,7,1021,15,26,993,6,9,981,14,25,956,0,0,956,0,0,953,0,0,949,0,0,948,959,4,52447,"FO2","IC" 33,17,5,3,9,655,1,"RED BUD (CITY OF)","RED BUD",0,"NAT GAS",15772,"0A",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,959,4,52447,"NG","IC" 33,17,5,3,2,661,5,"ROCHELLE (CITY OF)","N NINTH ST",0,"LIGHT OIL",16179,"0A",1294,,,95,0,0,0,5,15,779,0,0,0,3,0,771,0,0,764,12,23,741,59,110,631,112,214,527,0,0,416,0,0,415,0,24,711,0,25,686,960,4,52498,"FO2","IC" 33,17,5,3,9,661,5,"ROCHELLE (CITY OF)","N NINTH ST",0,"NAT GAS",16179,"0A",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,9,98,0,490,5142,0,1012,10917,0,0,0,0,0,0,0,0,1171,0,0,705,0,960,4,52498,"NG","IC" 33,17,5,2,6,661,10,"ROCHELLE (CITY OF)","S MAIN ST",0,"BIT COAL",16179,"0A",1294,,,95,182,283,317,0,0,1359,692,1123,1498,0,0,1498,0,0,1498,0,0,1498,0,0,1498,0,0,1498,0,0,1218,0,0,0,256,380,38,0,38,0,961,4,52498,"BIT","ST" 33,17,5,2,9,661,10,"ROCHELLE (CITY OF)","S MAIN ST",0,"NAT GAS",16179,"0A",1294,,,95,2606,84363,0,2941,19198,0,1831,61444,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,927,28450,0,0,0,0,961,4,52498,"NG","ST" 33,17,5,3,2,661,10,"ROCHELLE (CITY OF)","S MAIN ST",0,"LIGHT OIL",16179,"0A",1294,,,95,0,0,0,0,0,261,0,0,259,7,8,258,0,0,258,0,0,1498,0,0,1498,0,2,252,0,0,251,0,0,252,0,1,249,0,0,216,961,4,52498,"FO2","IC" 33,17,5,3,9,661,10,"ROCHELLE (CITY OF)","S MAIN ST",0,"NAT GAS",16179,"0A",1294,,,95,0,0,0,0,0,0,14,486,0,2,19,0,0,0,0,0,0,0,0,0,0,83,2186,0,0,0,0,0,0,0,10,323,0,0,0,0,961,4,52498,"NG","IC" 33,17,5,2,2,676,1,"SPRINGFIELD (CITY OF)","LAKESIDE",0,"LIGHT OIL",17828,"0M",1294,,,95,18,56,3309,-376,0,3847,35,123,3773,38,88,3309,8,21,2805,159,387,2233,123,292,1856,53,125,1641,42,111,1830,11,54,1641,16,39,2126,38,94,1910,964,4,52766,"FO2","ST" 33,17,5,2,6,676,1,"SPRINGFIELD (CITY OF)","LAKESIDE",0,"BIT COAL",17828,"0M",1294,,,95,1426,1194,2186,0,0,2186,1719,1619,3329,28971,18281,2724,3680,2612,1929,9405,6305,1526,17496,11431,1377,28851,18625,1401,2662,1934,379,394,523,1151,16922,10895,1211,7009,4720,1069,964,4,52766,"BIT","ST" 33,17,5,2,2,676,5,"SPRINGFIELD (CITY OF)","DALLMAN",0,"LIGHT OIL",17828,"0M",1294,,,95,300,585,0,76,148,0,85,123,0,184,376,0,278,544,0,98,185,0,43,85,0,46,90,0,194,381,0,69,134,0,98,191,0,62,121,0,963,4,52766,"FO2","ST" 33,17,5,2,6,676,5,"SPRINGFIELD (CITY OF)","DALLMAN",0,"BIT COAL",17828,"0M",1294,,,95,147822,79578,86892,139935,74982,79739,149373,60539,83519,84927,48213,88238,138529,75670,76947,148142,77066,75576,175826,96140,69655,181595,98487,70624,145723,79465,62150,147146,79567,66752,143295,77415,69089,189782,102492,71677,963,4,52766,"BIT","ST" 33,17,5,4,2,676,10,"SPRINGFIELD (CITY OF)","REYNOLDS",0,"LIGHT OIL",17828,"0M",1294,,,95,2,21,1499,1,19,1480,0,0,1480,22,120,1360,0,0,1360,12,77,1283,189,560,1401,222,713,1224,45,147,1077,0,0,1792,0,0,1792,21,66,1726,965,4,52766,"FO2","GT" 33,17,5,4,2,676,12,"SPRINGFIELD (CITY OF)","FACTORY",0,"LIGHT OIL",17828,"0M",1294,,,95,0,0,3559,57,277,3282,0,56,3226,0,0,3226,0,0,3226,0,15,3212,234,612,3502,337,1007,2674,0,0,0,1,40,2634,0,0,2634,6,18,2615,8016,4,52766,"FO2","GT" 33,17,5,3,2,685,1,"SULLIVAN (CITY OF)","SULLIVAN",0,"LIGHT OIL",18277,"0A",1294,,,95,64,126,1258,39,77,1181,15,30,1151,13,25,1301,205,430,1242,250,497,1265,287,569,1218,337,669,1235,211,418,1150,109,216,1446,94,187,1607,131,261,1346,969,4,52842,"FO2","IC" 33,17,5,3,9,685,1,"SULLIVAN (CITY OF)","SULLIVAN",0,"NAT GAS",18277,"0A",1294,,,95,417,4732,0,354,3991,0,175,2187,0,90,1200,0,2497,25139,0,3160,40149,0,3856,39252,0,4473,45978,0,2693,27195,0,1163,12837,0,1195,13294,0,1409,15384,0,969,4,52842,"NG","IC" 33,17,5,3,2,688,1,"WATERLOO (CITY OF)","WATERLOO",0,"LIGHT OIL",20180,"0A",1294,,,95,0,0,663,0,0,655,5,10,638,0,0,632,2,10,596,2,5,575,67,109,621,73,155,621,8,14,601,0,0,593,0,0,587,3,6,574,971,4,53196,"FO2","IC" 33,17,5,3,9,688,1,"WATERLOO (CITY OF)","WATERLOO",0,"NAT GAS",20180,"0A",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,2,17,0,3,26,0,77,912,0,83,788,0,0,0,0,0,0,0,0,0,0,0,0,0,971,4,53196,"NG","IC" 33,17,5,2,6,697,1,"WINNETKA (VILLAGE OF)","WINNEKA",0,"BIT COAL",20824,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,972,4,53319,"BIT","ST" 33,17,5,2,9,697,1,"WINNETKA (VILLAGE OF)","WINNEKA",0,"NAT GAS",20824,"0M",1294,,,95,76,1403,0,83,1602,0,0,0,0,61,1226,0,0,0,0,429,7918,0,1790,29451,0,3027,46315,0,83,1711,0,38,687,0,36,627,0,82,1282,0,972,4,53319,"NG","ST" 33,17,5,3,2,697,1,"WINNETKA (VILLAGE OF)","WINNEKA",0,"LIGHT OIL",20824,"0M",1294,,,95,9,15,1600,16,24,1576,15,27,2011,8,11,2038,15,27,2008,53,94,1879,81,146,1771,87,156,1614,39,65,1549,14,24,1525,21,36,1489,27,48,1441,972,4,53319,"FO2","IC" 33,17,8,3,2,835,5,"SOYLAND POWER COOP INC","PITTSFIELD",0,"LIGHT OIL",40307,"0M",1294,,,95,-86,19,362,-83,0,362,-84,0,362,-71,0,362,-22,0,362,-10,10,352,-13,0,352,-12,5,346,-10,0,346,-17,0,346,-27,0,346,-86,0,346,6237,4,53264,"FO2","IC" 33,17,8,3,2,835,10,"SOYLAND POWER COOP INC","WINCHESTER",0,"LIGHT OIL",40307,"0M",1294,"R",,95,-5,0,0,-4,0,0,-2,0,0,-4,0,0,-4,0,0,-3,0,0,-4,0,0,-4,0,0,-4,0,0,-3,0,0,-4,0,0,0,0,0,6236,4,53264,"FO2","IC" 33,17,8,2,2,835,20,"SOYLAND POWER COOP INC","PEARL",0,"LIGHT OIL",40307,"0M",1294,,,95,394,885,0,148,333,0,151,333,0,44,96,0,62,137,0,71,157,0,49,109,0,81,183,0,82,176,0,53,118,0,43,98,0,0,293,0,6238,4,53264,"FO2","ST" 33,17,8,2,6,835,20,"SOYLAND POWER COOP INC","PEARL",0,"BIT COAL",40307,"0M",1294,,,95,7480,4550,11696,6009,3668,13434,10811,6523,12395,9951,5859,11765,8686,5203,12183,10526,6310,12845,13881,8405,11170,12227,7501,11236,14144,8259,10522,14726,8807,6860,7789,4727,5629,-128,0,6213,6238,4,53264,"BIT","ST" 33,17,8,4,2,835,20,"SOYLAND POWER COOP INC","PEARL",0,"LIGHT OIL",40307,"0M",1294,,,95,0,0,3174,0,0,2841,0,0,2508,0,0,3312,0,0,3174,0,0,3018,198,439,4233,153,346,3704,0,0,3527,0,0,3410,0,0,3316,27,99,2920,6238,4,53264,"FO2","GT" 33,17,8,2,2,865,5,"SOUTHERN ILL PWR COOP","MARION",0,"LIGHT OIL",17632,"0M",1294,,,95,103,235,1930,398,937,1432,119,273,2109,54,114,1931,53,121,2200,40,89,1995,197,433,1909,516,982,1299,123,278,1355,138,291,1409,148,311,1983,116,228,2304,976,4,52726,"FO2","ST" 33,17,8,2,5,865,5,"SOUTHERN ILL PWR COOP","MARION",0,"COKE",17632,"0M",494,,,95,0,0,0,0,0,0,0,0,0,7100,5033,63,10577,7498,1080,12093,8573,883,18130,8251,340,24637,9801,5288,14975,6746,15187,18417,7751,15005,28435,11888,20057,29187,11536,36572,976,4,52726,"PC","ST" 33,17,8,2,6,865,5,"SOUTHERN ILL PWR COOP","MARION",0,"BIT COAL",17632,"0M",1294,,,95,99578,58899,343511,88921,53220,322269,67012,39679,313811,55683,32048,304374,67117,37520,306395,69155,37199,286872,84620,48755,270682,92636,56774,253743,47041,28911,281123,49349,30941,306445,68451,42435,291995,75427,45356,318016,976,4,52726,"BIT","ST" 34,26,1,2,1,21,1,"CONSUMERS POWER CO","BIG ROCK",0,"NUCLEAR",4254,"0M",1294,,95,95,49904,0,0,36125,0,0,47852,0,0,36194,0,0,51600,0,0,49866,0,0,50938,0,0,42590,0,0,45863,0,0,42825,0,0,30166,0,0,31731,0,0,1697,1,50658,"UR","ST" 34,26,1,2,1,21,1,"CONSUMERS POWER CO","PALISADES",0,"NUCLEAR",4254,"0M",1294,,95,95,583852,0,0,515599,0,0,577496,0,0,558296,0,0,349591,0,0,-2326,0,0,-2452,0,0,108144,0,0,474684,0,0,571773,0,0,561439,0,0,541156,0,0,1715,1,50658,"UR","ST" 34,26,1,1,,21,8,"CONSUMERS POWER CO","ALCONA",0,,4254,"0M",1294,,95,95,2490,0,0,1993,0,0,2704,0,0,2797,0,0,2622,0,0,1880,0,0,1902,0,0,2070,0,0,1760,0,0,2007,0,0,2376,0,0,2188,0,0,1693,1,50658,"WAT","HY" 34,26,1,1,,21,10,"CONSUMERS POWER CO","ALLEGAN",0,,4254,"0M",1294,,95,95,1357,0,0,1013,0,0,1394,0,0,1356,0,0,1410,0,0,981,0,0,946,0,0,1011,0,0,703,0,0,731,0,0,1154,0,0,994,0,0,1694,1,50658,"WAT","HY" 34,26,1,1,,21,19,"CONSUMERS POWER CO","C W TIPPY",0,,4254,"0M",1294,,95,95,5282,0,0,4150,0,0,6293,0,0,5440,0,0,5008,0,0,4326,0,0,4371,0,0,5203,0,0,4190,0,0,4573,0,0,5014,0,0,4570,0,0,1698,1,50658,"WAT","HY" 34,26,1,1,,21,25,"CONSUMERS POWER CO","COOKE",0,,4254,"0M",1294,,95,95,2367,0,0,1873,0,0,2687,0,0,2739,0,0,2539,0,0,1904,0,0,1946,0,0,2050,0,0,1790,0,0,2028,0,0,2329,0,0,2102,0,0,1700,1,50658,"WAT","HY" 34,26,1,1,,21,26,"CONSUMERS POWER CO","CROTON",0,,4254,"0M",1294,,95,95,4641,0,0,3300,0,0,4505,0,0,3399,0,0,3856,0,0,2193,0,0,2270,0,0,3054,0,0,2166,0,0,2146,0,0,3632,0,0,3031,0,0,1701,1,50658,"WAT","HY" 34,26,1,1,,21,28,"CONSUMERS POWER CO","FIVE CHANLS",0,,4254,"0M",1294,,95,95,2230,0,0,1812,0,0,2478,0,0,2479,0,0,2347,0,0,1784,0,0,1756,0,0,1920,0,0,1683,0,0,1895,0,0,2059,0,0,1961,0,0,1704,1,50658,"WAT","HY" 34,26,1,1,,21,29,"CONSUMERS POWER CO","FOOTE",0,,4254,"0M",1294,,95,95,2783,0,0,2213,0,0,3183,0,0,3182,0,0,2865,0,0,2239,0,0,2243,0,0,2387,0,0,2148,0,0,2381,0,0,2653,0,0,2564,0,0,1705,1,50658,"WAT","HY" 34,26,1,1,,21,32,"CONSUMERS POWER CO","HARDY",0,,4254,"0M",1294,,95,95,10721,0,0,6926,0,0,9337,0,0,6936,0,0,8622,0,0,4585,0,0,5199,0,0,7002,0,0,5021,0,0,5910,0,0,8935,0,0,6928,0,0,1707,1,50658,"WAT","HY" 34,26,1,1,,21,34,"CONSUMERS POWER CO","HODENPYL",0,,4254,"0M",1294,,95,95,3684,0,0,2846,0,0,4474,0,0,3916,0,0,3467,0,0,2500,0,0,2611,0,0,3740,0,0,2787,0,0,3279,0,0,4048,0,0,3474,0,0,1708,1,50658,"WAT","HY" 34,26,1,1,,21,38,"CONSUMERS POWER CO","LOUD",0,,4254,"0M",1294,,95,95,1690,0,0,1352,0,0,1882,0,0,1972,0,0,1822,0,0,1365,0,0,1424,0,0,1486,0,0,1265,0,0,1447,0,0,1654,0,0,1528,0,0,1712,1,50658,"WAT","HY" 34,26,1,1,,21,40,"CONSUMERS POWER CO","LD PUMP ST",0,"P-PUMPSTG",4254,"0M",1294,,95,95,-64589,233719,0,-57356,190758,0,-53950,195482,0,-71987,218971,0,-31897,115524,0,-60407,243003,0,-67008,223779,0,-77060,289960,0,-65130,213393,0,-70748,250623,0,-58089,197571,0,-53599,186916,0,1713,1,50658,"WAT","HY" 34,26,1,1,,21,42,"CONSUMERS POWER CO","MIO",0,,4254,"0M",1294,,95,95,1408,0,0,1113,0,0,1515,0,0,1563,0,0,1475,0,0,1064,0,0,1017,0,0,1161,0,0,991,0,0,1142,0,0,1213,0,0,1283,0,0,1714,1,50658,"WAT","HY" 34,26,1,1,,21,49,"CONSUMERS POWER CO","ROGERS",0,,4254,"0M",1294,,95,95,2752,0,0,1858,0,0,2142,0,0,2190,0,0,2657,0,0,1513,0,0,1706,0,0,2352,0,0,1808,0,0,1968,0,0,2874,0,0,2363,0,0,1716,1,50658,"WAT","HY" 34,26,1,1,,21,58,"CONSUMERS POWER CO","WEBBER",0,,4254,"0M",1294,,95,95,1914,0,0,1295,0,0,2105,0,0,2059,0,0,1759,0,0,836,0,0,748,0,0,1150,0,0,321,0,0,398,0,0,1321,0,0,928,0,0,1722,1,50658,"WAT","HY" 34,26,1,2,2,21,65,"CONSUMERS POWER CO","JH CAMPBELL",0,"LIGHT OIL",4254,"0M",1294,,95,95,376,598,4499,283,447,4052,1907,3068,3484,2100,3394,4019,519,835,7113,985,1571,5531,311,508,5023,954,1563,3460,1220,1999,3604,1817,2975,4007,1351,2181,3968,1278,2102,3566,1710,1,50658,"FO2","ST" 34,26,1,2,6,21,65,"CONSUMERS POWER CO","JH CAMPBELL",0,"BIT COAL",4254,"0M",1294,,95,95,688173,266958,245746,629424,250579,214312,554183,223280,253129,421848,167012,399301,597082,246292,477288,640613,258293,443746,603954,255371,374582,621938,269381,277933,502655,214049,299355,646510,274214,290900,687374,281291,323449,707593,291775,344669,1710,1,50658,"BIT","ST" 34,26,1,4,2,21,65,"CONSUMERS POWER CO","JH CAMPBELL",0,"LIGHT OIL",4254,"0M",1294,,95,95,3,18,3579,26,68,3511,5,2,3510,3,8,3501,14,105,3396,1,1,3395,89,352,3043,300,894,2816,0,0,2816,0,0,2780,12,29,2750,0,0,2750,1710,1,50658,"FO2","GT" 34,26,1,2,2,21,70,"CONSUMERS POWER CO","B C COBB",0,"LIGHT OIL",4254,"0M",1294,,95,95,119,201,0,106,183,0,15,25,0,151,260,0,15,25,0,11,20,0,1038,1787,0,616,1065,0,337,575,0,124,210,0,609,1027,0,116,197,0,1695,1,50658,"FO2","ST" 34,26,1,2,6,21,70,"CONSUMERS POWER CO","B C COBB",0,"BIT COAL",4254,"0M",1294,,95,95,171685,81705,303296,112559,55863,247433,173477,86683,160750,176230,89153,134091,171229,86036,137454,177787,81941,81399,152875,79003,128717,175209,87546,157003,143997,70790,171410,172337,82837,192966,174578,86518,170355,171682,85592,358752,1695,1,50658,"BIT","ST" 34,26,1,2,9,21,70,"CONSUMERS POWER CO","B C COBB",0,"NAT GAS",4254,"0M",1294,,95,95,921,9110,0,661,6660,0,735,7267,0,667,6715,0,387,3867,0,701,6993,0,490,4921,0,732,7388,0,377,3745,0,625,6179,0,826,8120,0,729,7244,0,1695,1,50658,"NG","ST" 34,26,1,4,9,21,71,"CONSUMERS POWER CO","B E MORROW",0,"NAT GAS",4254,"0M",1294,,95,95,21,1252,0,61,797,0,23,390,0,0,0,0,0,0,0,401,8324,0,371,9296,0,1149,25420,0,33,769,0,0,0,0,0,0,0,0,0,0,1696,1,50658,"NG","GT" 34,26,1,2,2,21,73,"CONSUMERS POWER CO","D E KARN",0,"LIGHT OIL",4254,"0M",1294,,95,95,95,155,4465,729,1211,3870,49,79,4192,1413,2315,3502,1471,2465,4192,323,528,4944,367,607,3918,3048,4972,4484,1078,1808,6755,441,718,5263,482,776,5343,208,340,5633,1702,1,50658,"FO2","ST" 34,26,1,2,3,21,73,"CONSUMERS POWER CO","D E KARN",0,"HEAVY OIL",4254,"0M",1294,,95,95,17263,41101,178646,32230,70799,144631,3259,14882,162100,3710,14639,204722,1348,4618,245418,27469,68422,203997,56064,119639,141693,95085,202123,111624,29250,66633,127707,-2403,604,148925,24960,66400,139076,24013,58612,178738,1702,1,50658,"FO6","ST" 34,26,1,2,6,21,73,"CONSUMERS POWER CO","D E KARN",0,"BIT COAL",4254,"0M",1294,,95,95,201703,83102,130505,120289,51141,110637,178823,75624,145086,292219,122156,106091,232390,98356,133690,313475,134010,126635,299344,128910,118120,335951,141190,65110,201053,86888,158744,293910,123720,122461,305821,124517,171638,315326,164076,152202,1702,1,50658,"BIT","ST" 34,26,1,2,9,21,73,"CONSUMERS POWER CO","D E KARN",0,"NAT GAS",4254,"0M",1294,,95,95,0,0,0,0,0,0,126,3486,0,7447,169068,0,10439,207703,0,12622,193255,0,50264,657734,0,101002,1316168,0,18325,257600,0,0,0,0,11460,187792,0,10071,152074,0,1702,1,50658,"NG","ST" 34,26,1,4,9,21,74,"CONSUMERS POWER CO","GAYLORD",0,"NAT GAS",4254,"0M",1294,,95,95,16,288,0,102,1836,0,15,332,0,0,0,0,0,0,0,515,9959,0,346,16592,0,3203,53480,0,4,2469,0,2,482,0,49,1700,0,0,0,0,1706,1,50658,"NG","GT" 34,26,1,4,9,21,79,"CONSUMERS POWER CO","STRAITS",0,"NAT GAS",4254,"0M",1294,,95,95,0,0,0,20,371,0,33,801,0,0,0,0,0,427,0,0,0,0,0,0,0,201,2828,0,203,2283,0,10,340,0,0,0,0,0,0,0,1718,1,50658,"NG","GT" 34,26,1,4,9,21,80,"CONSUMERS POWER CO","THETFORD",0,"NAT GAS",4254,"0M",1294,,95,95,-73,0,0,51,3065,0,-47,1801,0,-81,0,0,-11,1761,0,1724,48143,0,3577,74211,0,8176,149686,0,359,8949,0,103,2718,0,99,1204,0,-193,371,0,1719,1,50658,"NG","GT" 34,26,1,2,2,21,81,"CONSUMERS POWER CO","WEADOCK",0,"LIGHT OIL",4254,"0M",1294,,95,95,0,0,0,43,71,0,206,349,0,0,0,0,0,0,0,32,55,0,418,680,0,532,903,0,187,305,0,128,198,0,422,716,0,0,0,0,1720,1,50658,"FO2","ST" 34,26,1,2,6,21,81,"CONSUMERS POWER CO","WEADOCK",0,"BIT COAL",4254,"0M",1294,,95,95,192310,85708,45814,188975,83651,56497,190706,85006,57355,187037,83678,61516,177334,80278,58828,184095,83971,65159,155632,70970,60725,137329,63894,42030,160634,72475,36751,171924,77864,49121,139453,63086,78970,91065,41232,72440,1720,1,50658,"BIT","ST" 34,26,1,4,9,21,81,"CONSUMERS POWER CO","WEADOCK",0,"NAT GAS",4254,"0M",1294,,95,95,1,12,0,16,289,0,3,117,0,0,0,0,0,0,0,7,73,0,6,58,0,5,49,0,44,404,0,8,72,0,0,0,0,0,0,0,1720,1,50658,"NG","GT" 34,26,1,2,2,21,84,"CONSUMERS POWER CO","WHITING",0,"LIGHT OIL",4254,"0M",1294,,95,95,67,114,0,17,29,0,23,38,0,43,74,0,40,69,0,63,110,0,122,217,0,60,107,0,40,69,0,81,138,0,152,260,0,71,122,0,1723,1,50658,"FO2","ST" 34,26,1,2,6,21,84,"CONSUMERS POWER CO","WHITING",0,"BIT COAL",4254,"0M",1294,,95,95,187062,77616,89934,185094,74786,71016,195982,81145,69534,189147,74635,99630,151777,65376,105918,176546,69938,98910,159910,67506,87345,170468,72736,86560,153306,62762,86674,136600,57354,115439,140799,58953,146166,157205,64361,118168,1723,1,50658,"BIT","ST" 34,26,1,4,2,21,84,"CONSUMERS POWER CO","WHITING",0,"LIGHT OIL",4254,"0M",1294,,95,95,0,0,3383,0,0,3383,0,0,3383,0,0,3383,0,0,3383,13,41,3341,40,165,3176,586,1651,1525,5,60,3025,0,0,3037,0,0,3037,13,28,3009,1723,1,50658,"FO2","GT" 34,26,1,2,1,30,2,"DETROIT EDISON CO (THE)","FERMI 2",0,"NUCLEAR",5109,"0M",1294,,,95,57145,0,0,-2291,0,0,191112,0,0,332959,0,0,429952,0,0,318206,0,0,641286,0,0,646514,0,0,632787,0,0,629384,0,0,621966,0,0,597155,0,0,1729,1,50782,"UR","ST" 34,26,1,2,2,30,5,"DETROIT EDISON CO (THE)","HARBOR BECH",0,"LIGHT OIL",5109,"0M",1294,,,95,438,1013,575,399,920,291,337,838,431,226,616,443,208,409,330,272,533,404,256,504,456,402,782,347,137,284,368,256,520,468,392,891,512,324,728,420,1731,1,50782,"FO2","ST" 34,26,1,2,6,30,5,"DETROIT EDISON CO (THE)","HARBOR BECH",0,"BIT COAL",5109,"0M",1294,,,95,19026,9916,30527,16932,9323,21204,13176,7346,13858,2917,1770,26559,11229,4899,21660,24213,10667,10993,14172,6321,18792,27860,12241,19588,7804,3632,16168,5468,2542,33328,18662,9888,37691,11914,6187,42217,1731,1,50782,"BIT","ST" 34,26,1,3,2,30,5,"DETROIT EDISON CO (THE)","HARBOR BECH",0,"LIGHT OIL",5109,"0M",1294,,,95,0,0,0,-6,7,0,1,2,0,-9,2,0,-7,8,0,-8,5,0,10,38,0,215,410,0,-7,4,0,-10,0,0,-9,2,0,-4,5,0,1731,1,50782,"FO2","IC" 34,26,1,2,2,30,10,"DETROIT EDISON CO (THE)","BEACON",0,"LIGHT OIL",5109,"0M",1294,,,95,0,0,5557,0,0,6175,0,0,6175,0,0,6175,0,0,6175,0,0,6175,0,0,6175,0,0,6175,0,0,6175,0,0,6175,0,0,6175,0,0,6175,1724,1,50782,"FO2","ST" 34,26,1,2,6,30,10,"DETROIT EDISON CO (THE)","BEACON",0,"BIT COAL",5109,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1724,1,50782,"BIT","ST" 34,26,1,2,9,30,10,"DETROIT EDISON CO (THE)","BEACON",0,"NAT GAS",5109,"0M",1294,,,95,7417,215941,0,6530,166317,0,7378,568420,0,6367,460210,0,159,197560,0,-948,134770,0,-213,186220,0,133,234260,0,-472,176150,0,2357,308180,0,7138,508130,0,9005,660050,0,1724,1,50782,"NG","ST" 34,26,1,2,2,30,30,"DETROIT EDISON CO (THE)","CONNERS CRK",0,"LIGHT OIL",5109,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1726,1,50782,"FO2","ST" 34,26,1,2,6,30,30,"DETROIT EDISON CO (THE)","CONNERS CRK",0,"BIT COAL",5109,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1726,1,50782,"BIT","ST" 34,26,1,2,9,30,30,"DETROIT EDISON CO (THE)","CONNERS CRK",0,"NAT GAS",5109,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1726,1,50782,"NG","ST" 34,26,1,3,2,30,30,"DETROIT EDISON CO (THE)","CONNERS CRK",0,"LIGHT OIL",5109,"0M",1294,,,95,-19,10,403,-10,35,368,-17,0,368,-7,30,339,-12,1,338,-11,0,338,3,19,320,272,571,293,4,24,270,-18,0,270,-7,17,327,-18,1,327,1726,1,50782,"FO2","IC" 34,26,1,4,2,30,36,"DETROIT EDISON CO (THE)","HANCOCK",0,"LIGHT OIL",5109,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1730,1,50782,"FO2","GT" 34,26,1,4,9,30,36,"DETROIT EDISON CO (THE)","HANCOCK",0,"NAT GAS",5109,"0M",1294,,,95,75,1708,0,88,2028,0,-39,0,0,75,1898,0,83,2205,0,1939,35032,0,831,16862,0,4390,52333,0,-32,0,0,63,13854,0,113,1716,0,13,727,0,1730,1,50782,"NG","GT" 34,26,1,4,2,30,37,"DETROIT EDISON CO (THE)","ENRCO FERMI",0,"LIGHT OIL",5109,"0M",1294,,,95,-23,67,9592,56,437,9156,-6,95,9061,3,40,9021,46,201,8820,22,73,8747,153,611,8157,2354,5359,6937,191,530,6407,25,406,6813,-7,117,6696,7,155,6541,1729,1,50782,"FO2","GT" 34,26,1,2,6,30,40,"DETROIT EDISON CO (THE)","MARYSVILLE",0,"BIT COAL",5109,"0M",1294,,,95,3451,2200,43168,1939,1836,41332,409,1040,40292,674,1100,39192,84,409,38783,2426,2025,36758,3997,2730,34028,24162,13503,20607,-821,0,20689,1187,1161,28911,77,1281,27712,1498,1298,26498,1732,1,50782,"BIT","ST" 34,26,1,2,9,30,40,"DETROIT EDISON CO (THE)","MARYSVILLE",0,"NAT GAS",5109,"0M",1294,,,95,758,11483,0,601,14357,0,109,6809,0,104,4289,0,18,2144,0,313,6731,0,407,7237,0,958,13528,0,-821,0,0,0,12,0,16,6473,0,766,16219,0,1732,1,50782,"NG","ST" 34,26,1,2,3,30,41,"DETROIT EDISON CO (THE)","RIVER ROUGE",0,"HEAVY OIL",5109,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1740,1,50782,"FO6","ST" 34,26,1,2,6,30,41,"DETROIT EDISON CO (THE)","RIVER ROUGE",0,"BIT COAL",5109,"0M",1294,,,95,219134,93352,55641,159139,73272,70516,175906,83846,66525,288407,131567,61779,267048,129044,38352,279504,129178,23957,147366,70111,56314,275336,132806,20939,244758,114254,49404,262473,127544,3398,311969,149413,952,289268,136099,23606,1740,1,50782,"BIT","ST" 34,26,1,2,9,30,41,"DETROIT EDISON CO (THE)","RIVER ROUGE",0,"N&BF GAS",5109,"0M",1294,,,95,13490,1142053,0,14328,1002326,0,27337,1536596,0,24705,1839986,0,27750,1701771,0,26423,2082983,0,18771,1535930,0,35058,2287285,0,27144,2100264,0,28968,1856118,0,25198,1941541,0,33781,2350884,0,1740,1,50782,"NG","ST" 34,26,1,3,2,30,41,"DETROIT EDISON CO (THE)","RIVER ROUGE",0,"LIGHT OIL",5109,"0M",1294,,,95,-64,0,605,-7,10,595,-39,17,579,-34,0,579,-17,26,552,-25,14,538,19,67,471,444,902,433,1,70,648,-12,14,633,-30,19,614,-47,0,614,1740,1,50782,"FO2","IC" 34,26,1,2,2,30,42,"DETROIT EDISON CO (THE)","ST CLAIR",0,"LIGHT OIL",5109,"0M",1294,,,95,708,1282,34227,1068,2121,32093,3247,6007,21655,5314,10052,11849,6361,11768,6584,7708,14388,5004,650,1226,3459,1539,2748,8759,0,0,36637,1336,2409,49346,2815,5029,26266,1015,1855,17641,1743,1,50782,"FO2","ST" 34,26,1,2,3,30,42,"DETROIT EDISON CO (THE)","ST CLAIR",0,"HEAVY OIL",5109,"0M",1294,,,95,67,115,41140,472,857,40929,201,356,40849,2072,3718,37736,1534,2609,35989,1725,3066,36174,1324,2443,34132,3965,6895,28662,605,1053,29986,0,0,30968,0,0,26726,0,0,26726,1743,1,50782,"FO6","ST" 34,26,1,2,6,30,42,"DETROIT EDISON CO (THE)","ST CLAIR",0,"BIT COAL",5109,"0M",1294,,,95,527154,296526,1904789,579915,330143,1298971,632525,361281,910345,483802,281107,948523,421431,243485,1140644,540448,305320,1495864,747171,415802,1708026,687564,368710,1805574,643125,334613,2160088,580105,305454,2328721,615025,322461,2497621,727329,387191,2536457,1743,1,50782,"BIT","ST" 34,26,1,2,9,30,42,"DETROIT EDISON CO (THE)","ST CLAIR",0,"NAT GAS",5109,"0M",1294,,,95,300,3042,0,495,5533,0,1182,12305,0,2642,28255,0,933,9784,0,595,6301,0,407,4362,0,801,8135,0,440,4467,0,1095,11359,0,723,7386,0,821,8584,0,1743,1,50782,"NG","ST" 34,26,1,3,2,30,42,"DETROIT EDISON CO (THE)","ST CLAIR",0,"LIGHT OIL",5109,"0M",1294,,,95,-21,0,0,6,12,0,-10,0,0,-6,8,0,0,0,0,-7,0,0,16,41,0,267,476,0,-7,0,0,-6,5,0,-10,0,0,-10,0,0,1743,1,50782,"FO2","IC" 34,26,1,4,2,30,42,"DETROIT EDISON CO (THE)","ST CLAIR",0,"LIGHT OIL",5109,"0M",1294,,,95,0,0,0,0,0,0,0,0,0,-20,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,0,1743,1,50782,"FO2","GT" 34,26,1,4,9,30,42,"DETROIT EDISON CO (THE)","ST CLAIR",0,"NAT GAS",5109,"0M",1294,,,95,-15,0,0,19,222,0,0,0,0,-42,25,0,16,175,0,-11,0,0,18,346,0,-7,0,0,14,423,0,-10,0,0,-1,11,0,-3,54,0,1743,1,50782,"NG","GT" 34,26,1,2,2,30,45,"DETROIT EDISON CO (THE)","TRENTON CNL",0,"LIGHT OIL",5109,"0M",1294,,,95,2117,5567,8586,1135,2059,8309,1543,2836,11784,1101,1955,9830,427,776,11295,1378,2621,9024,1071,2007,11104,2983,5339,10903,715,1328,11816,1060,1978,12599,597,1093,11507,590,1046,12738,1745,1,50782,"FO2","ST" 34,26,1,2,6,30,45,"DETROIT EDISON CO (THE)","TRENTON CNL",0,"BIT COAL",5109,"0M",1294,,,95,73007,53010,125588,323088,144439,89756,284495,135448,125363,339095,164391,64193,278956,138759,81062,334708,166852,92923,344600,175834,77241,387486,184117,48162,328365,176710,67462,355401,186425,60433,331742,165511,87568,334941,167769,110839,1745,1,50782,"BIT","ST" 34,26,1,4,2,30,47,"DETROIT EDISON CO (THE)","NORTHEAST",0,"LIGHT OIL",5109,"0M",1294,,,95,-29,0,2051,-9,47,2004,-31,0,2004,9,63,1940,10,85,1855,610,1799,2214,83,729,2195,1190,3965,1920,-117,0,1920,-17,238,2156,14,127,2030,-35,0,2029,1734,1,50782,"FO2","GT" 34,26,1,4,9,30,47,"DETROIT EDISON CO (THE)","NORTHEAST",0,"NAT GAS",5109,"0M",1294,,,95,-49,274,0,3,1924,0,-15,871,0,5,475,0,-70,0,0,236,15908,0,291,28798,0,1942,30986,0,-58,0,0,1,1017,0,-88,44,0,53,1442,0,1734,1,50782,"NG","GT" 34,26,1,2,2,30,48,"DETROIT EDISON CO (THE)","MONROE",0,"LIGHT OIL",5109,"0M",1294,,,95,2386,3835,8777,2169,3558,10202,1658,2697,9630,1424,2341,9860,7134,12079,8987,1592,2699,8841,1898,3281,9073,5386,9424,7517,3930,5748,10052,1222,2050,9934,11813,19875,7429,12821,21265,9414,1733,1,50782,"FO2","ST" 34,26,1,2,6,30,48,"DETROIT EDISON CO (THE)","MONROE",0,"BIT COAL",5109,"0M",1294,,,95,2055700,868846,1154764,1856029,799581,917721,1821777,792041,931826,1409911,611222,1269078,1619971,729115,1538754,2012769,908040,1475012,1970161,908523,1280247