Sample records for redshift systems corporation

  1. Implementing a Corporate Energy Management System

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

    Implementing a Corporate Energy Management System" Steve Schultz Corporate Energy Manager 3M Presented at the U.S. Department of Energy Industrial Technologies Program June 3, 2010...

  2. 2011 IBM Corporation Computer system energy management

    E-Print Network [OSTI]

    Shi, Weisong

    level EnergyScale Microcontroller IBM Systems Director · Policy management · Power & performance© 2011 IBM Corporation Computer system energy management Charles Lefurgy 28 July 2011 #12;© 2011 IBM Corporation2 Outline A short history of server power management POWER7 EnergyScale AMESTER power

  3. System to estimate ages and redshifts for radio galaxies

    E-Print Network [OSTI]

    O. V. Verkhodanov; A. I. Kopylov; N. V. Verkhodanova; O. P. Zhelenkova; V. N. Chernenkov; Yu. N. Parijskij; N. S. Soboleva; A. V. Temirova

    2001-12-06T23:59:59.000Z

    The system allowing a user to operate with simulated curves of spectral energy distribution (SED) and to estimate ages and redshifts by photometric data at server {\\bf sed.sao.ru} is described.

  4. Corporate Law, Social Norms and Belief Systems

    E-Print Network [OSTI]

    Eisenberg, Melvin

    1999-01-01T23:59:59.000Z

    fiduciary duties, corporate governance, and takeovers (Partinvestors in corporate governance. Often, the operation ofthe ALI’s Principles of Corporate Governance provides that a

  5. Copyright 2011 Northrop Grumman Corporation Northrop Grumman Information Systems (NGIS)

    E-Print Network [OSTI]

    from unattended sensors · Space vulnerabilities and survivability · Cyber security/informationCopyright © 2011 Northrop Grumman Corporation Northrop Grumman Information Systems (NGIS Northrop Grumman Corporation Page 2 1. Overview Information Sponsor ­Northrop Grumman Information Systems

  6. RedShift Systems Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere IRaghuraji Agro Industries Pvt Ltd Jump to: navigation, searchRay County,OpenCounty, Texas:Red RiverRedShift

  7. Corporate Information Systems | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE: Alternative FuelsNovember 13, 2014Contributing Data Contributing DataCorporate Information Systems

  8. Fastcap Systems Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand JumpConceptual Model,DOEHazelPennsylvania: EnergyExolisFairway,FarmersFastcap Systems Corporation Jump

  9. Buildings and corporate strategy : towards a management system model

    E-Print Network [OSTI]

    Brana, Rodrigo

    1985-01-01T23:59:59.000Z

    This thesis focuses on buildings as a subject of attention and inquiry in a corporate setting. It attempts to draw implications for the design of a management system to deal with the special nature of buildings as a resource. ...

  10. Edenspace Systems Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand JumpConceptual Model,DOEHazel Crest, Illinois: EnergyEastport,de NantesCryogenics LLCEdenspace Systems

  11. Corporate Systems Engineering | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnualProperty EditCalifornia:PowerCER.pngRoofs and Heat Islands2007) | Open EnergyTexas:PlusSystems

  12. A Model and Simulation of Competitive Electric Power Systems Martin W. Lin, Enron Corporation, Manager Research

    E-Print Network [OSTI]

    Baldick, Ross

    A Model and Simulation of Competitive Electric Power Systems Martin W. Lin, Enron Corporation Abstract-- A framework for analyzing competitive electric power systems has been developed. A model Competitive Electric Power System Model (GCEPSM), incorporate object classes to represent basic market players

  13. The Possibility of Checking the Equivalence Principle in a Null Gravitational Redshift by a Two-Resonator Laser System

    E-Print Network [OSTI]

    R. A. Daishev; Z. G. Murzakhanov; A. F. Skochilov

    2008-01-04T23:59:59.000Z

    A scheme of an optical detector is proposed for checking Einsteins equivalence principle (EEP) in a null gravitational redshift experiment and for testing methods for calculating the length of a resonator in a weak variable gravitational field by recording the variations of the difference frequency of resonators caused by lunisolar variations of the geopotential in a double or a two-resonator laser system.

  14. PIA - Corporate Planning System (CPS) | Department of Energy

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33 111 1,613 122Commercial602 1,39732onMake YourDepartmentChartForums OutreachAMWTP2009 |Corporate

  15. Chemical Enrichment at High Redshifts: Understanding the Nature of Damped Ly$?$ Systems in Hierarchical Models

    E-Print Network [OSTI]

    P. B. Tissera; D. G. Lambas M. B. Mosconi; S. A. Cora

    2001-04-18T23:59:59.000Z

    We use cosmological hydrodynamical simulations including star formation and metal enrichment to study the evolution of the chemical properties of galaxy-like objects at high redshift in the range $0.25Hydrogen column densities with abundances and scatter comparable to those observed in damped Lyman-$\\alpha$ systems (DLAs).The unweighted mean of abundance ratios and least square linear regressions through the simulated DLAs yield intrinsic metallicity evolution for the [Zn/H] and [Fe/H], consistent with results obtained from similar analysis of available observations. Our model statistically reproduces the mild evolution detected in the metallicity of the neutral hydrogen content of the Universe, given by mass-weighted means,if observational constraints are considered (as suggested by Boiss\\'ee et al. 1998). For the $\\alpha$-elements in the simulated DLAs, we find neither enhancement nor dependence on metallicity. Our results support the hypotheses that DLAs trace a variety of galactic objects with different formation histories and that both SNI and SNII are contributing to the chemical enrichment of the gas component at least since $z \\approx 2$. This study indicates that DLAs could be understood as the building blocks that merged to form today normal galaxies within a hierarchical clustering scenario.

  16. Damped Lyman Alpha Systems at High Redshift and Models of Protogalactic Disks

    E-Print Network [OSTI]

    Prochaska, Jason X.

    of neutral gas in individual dark matter halos at high redshift. For example, neutral gas in damped Ly is well approximated by a cold dark matter model with critical density and vanishing cosmological constant and CDM normalizations. Whereas the column density distribution favors small disks with large neutral gas

  17. A Spectroscopic Redshift for the Cl0024+16 Multiple Arc System: Implications for the Central Mass Distribution

    E-Print Network [OSTI]

    Tom Broadhurst; Xiaosheng Huang; Brenda Frye; Richard Ellis

    1999-02-23T23:59:59.000Z

    We present a spectroscopic redshift of z=1.675 for the well-known multiply lensed system of arcs seen in the z=0.39 cluster Cl0024+16. In contrast to earlier work, we find that the lensed images are accurately reproduced by a projected mass distribution which traces the locations of the brightest cluster ellipticals, suggesting that the most significant minima of the cluster potential are not fully erased. The averaged mass profile is shallow and consistent with predictions of recent numerical simulations. The source redshift enables us to determine an enclosed cluster mass of M(<100kpc/h)=1.11+/-0.03 x 10^{14}M_{\\odot}/h and a mass-to-light ratio of M/L_B(<100kpc/h)=320h(M/L_B)_{\\odot}, after correction for passive stellar evolution. The arc spectrum contains many ionized absorption lines and closely resembles that of the local Wolf-Rayet galaxy NGC4217. Our lens model predicts a high magnification (~20) for each image and identifies a new pair of multiple images at a predicted redshift of z=1.3.

  18. A Damped Ly-alpha Absorption-line System in an Apparent Void at Redshift 2.38

    E-Print Network [OSTI]

    L. E. H. Godfrey; P. J. Francis

    2005-06-22T23:59:59.000Z

    We study the contents of an apparent void in the distribution of Ly-alpha emitting galaxies at redshift 2.38. We show that this void is not empty, but contains a damped Ly-alpha absorption-line system, seen in absorption against background QSO 2138-4427. Imaging does not reveal any galaxy associated with this absorption-line system, but it contains metals (Fe/H ~ -1.3), and its large velocity range (~ 180 km/s) implies a significant mass.

  19. Qtier-Rapor: Managing Spreadsheet Systems & Improving Corporate Performance, Compliance and Governance

    E-Print Network [OSTI]

    Bishop, Keith

    2008-01-01T23:59:59.000Z

    Much of what EuSpRIG discusses is concerned with the integrity of individual spreadsheets. In businesses, interlocking spreadsheets are regularly used to fill functional gaps in core administrative systems. The growth and deployment of such integrated spreadsheet SYSTEMS raises the scale of issues to a whole new level. The correct management of spreadsheet systems is necessary to ensure that the business achieves its goals of improved performance and good corporate governance, within the constraints of legislative compliance - poor management will deliver the opposite. This paper is an anatomy of the real-life issues of the commercial use of spreadsheets in business, and demonstrates how Qtier-Rapor has been used to instil best practice in the use of integrated commercial spreadsheet systems.

  20. Chemical Enrichment at High Redshifts Understanding the Nature of Damped Ly$\\alpha$ Systems in Hierarchical Models

    E-Print Network [OSTI]

    Tissera, P B; Cora, S A

    2001-01-01T23:59:59.000Z

    We use cosmological hydrodynamical simulations including star formation and metal enrichment to study the evolution of the chemical properties of galaxy-like objects at high redshift in the range $0.25Hydrogen column densities with abundances and scatter comparable to those observed in damped Lyman-$\\alpha$ systems (DLAs).The unweighted mean of abundance ratios and least square linear regressions through the simulated DLAs yield intrinsic metallicity evolution for the [Zn/H] and [Fe/H], consistent with results obtained from similar analysis of available observations. Our model statistically reproduces the mild evolution detected in the metallicity of the neutral hydrogen content of the Universe, given by mass-weighted means,if observational constraints are considered (as suggested by Boiss\\'ee et al. 1998). For the $\\alpha$-elements in the simulated DLAs, we find n...

  1. First Detection of NaI D lines in High-Redshift Damped Lyman-alpha Systems

    E-Print Network [OSTI]

    Sohei Kondo; Naoto Kobayashi; Yosuke Minowa; Takuji Tsujimoto; Christopher W. Churchill; Naruhisa Takato; Masanori Iye; Yukiko Kamata; Hiroshi Terada; Tae-Soo Pyo; Hideki Takami; Yutaka Hayano; Tomio Kanzawa; D. Saint-Jacques; Wolfgang Gaessler; Shin Oya; Ko Nedachi; Alan Tokunaga

    2006-03-12T23:59:59.000Z

    A Near-infrared (1.18-1.35 micron) high-resolution spectrum of the gravitationally-lensed QSO APM 08279+5255 was obtained with the IRCS mounted on the Subaru Telescope using the AO system. We detected strong NaI D 5891,5897 doublet absorption in high-redshift DLAs at z=1.062 and 1.181, confirming the presence of NaI, which was first reported for the rest-frame UV NaI 3303.3,3303.9 doublet by Petitjean et al. This is the first detection of NaI D absorption in a high-redshift (z>1) DLA. In addition, we detected a new NaI component in the z=1.062 DLA and four new components in the z=1.181 DLA. Using an empirical relationship between NaI and HI column density, we found that all "components" have large HI column density, so that each component is classified as DLA absorption. We also detected strong NaI D absorption associated with a MgII system at z=1.173. Because no other metal absorption lines were detected in this system at the velocity of the NaI absorption in previously reported optical spectra (observed 3.6 years ago), we interpret this NaI absorption cloud probably appeared in the line of sight toward the QSO after the optical observation. This newly found cloud is likely to be a DLA based upon its large estimated HI column density. We found that the N(NaI)/N(CaII) ratios in these DLAs are systematically smaller than those observed in the Galaxy; they are more consistent with the ratios seen in the Large Magellanic Cloud. This is consistent with dust depletion generally being smaller in lower metallicity environments. However, all five clouds of the z=1.181 system have a high N(NaI)/N(CaII) ratio, which is characteristic of cold dense gas. We tentatively suggest that the host galaxy of this system may be the most significant contributor to the gravitational-lens toward APM 08279+5255.

  2. Self evaluation and community development corporations : the utility of robust management information systems

    E-Print Network [OSTI]

    Reuter, George N. (George Nicholas)

    2014-01-01T23:59:59.000Z

    Many community development corporations are broadening their program components while seeking efficient and effective ways of measuring their impacts. Recent advances in information technology have created "cloud" database ...

  3. This study explores how the EU Emissions Trading System (EU ETS) actually works on the ground affecting corporate climate strategies.

    E-Print Network [OSTI]

    This study explores how the EU Emissions Trading System (EU ETS) actually works on the ground@bookpoint.co.uk May 2013 322 pages Hardback 978-1-4094-6078-7 £60.00 Corporate Responses to EU Emissions Trading at The Fridtjof Nansen Institute, Norway `With greenhouse gas emissions trading schemes emerging worldwide

  4. The Olympus Scandal and Corporate Governance Reform: Can Japan Find a Middle Ground between the Board Monitoring Model and Management Model

    E-Print Network [OSTI]

    Aronson, Bruce E.

    2012-01-01T23:59:59.000Z

    OLYMPUS SCANDAL AND CORPORATE GOVERNANCE REFORM: CAN JAPANScandal and Corporate Governance Issues A. Background of theunder Japan's Corporate Governance System ..

  5. Description of the system planning process at Florida Power Corporation. Task I. Report No. FC-5237-1

    SciTech Connect (OSTI)

    None

    1980-01-01T23:59:59.000Z

    One of the means of evaluating a new technology is to have it considered by a utility company, run through the system planning, and thus scrutinized by a potential user of the new technology in a manner directly drawn from the user's methods of decision making on new capacity additions. By having Florida Power Corporation (FPC), a company with real potential for the future use of ocean thermal energy conversion (OTEC), exercise its system planning methods to consider this possible source of future generating capacity, a number of highly useful results will be obtained. The overall study of the application of system planning to OTEC is being carried out in four tasks. This report covers task-1 which provides a description of the existing system and the planning process of Florida Power Corporation. (WHK)

  6. The Optical - Infrared Colors of CORALS QSOs: Searching for Dust Reddening Associated With High Redshift Damped Lyman Alpha Systems

    E-Print Network [OSTI]

    Sara L. Ellison; Patrick B. Hall; Paulina Lira

    2005-07-18T23:59:59.000Z

    The presence of dust in quasar absorbers, such as damped Lyman alpha (DLA) systems, may cause the background QSO to appear reddened. We investigate the extent of this potential reddening by comparing the optical-to-infrared (IR) colors of QSOs with and without intervening absorbers. Our QSO sample is based on the Complete Optical and Radio Absorption Line System (CORALS) survey of Ellison et al (2001). We have obtained near-simultaneous B and K band magnitudes for subset of the CORALS sample and supplemented our observations with further measurements published in the literature. To account for redshift-related color changes, the B-K colors are normalized using the Sloan Digital Sky Survey (SDSS) QSO composite. The mean normalized B-K color of the DLA sub-sample is +0.12, whereas the mean for the no-DLA sample is -0.10; both distributions have RMS scatters ~0.5. Neither a student's T-test nor a KS test indicate that there is any significant difference between the two color distributions. Based on simulations which redden the colors of QSOs with intervening DLAs, we determine a reddening limit which corresponds to E(B-V) < 0.04 (SMC-like extinction) at 99% confidence (3 sigma), assuming that E(B-V) is the same for all DLAs. Finally, we do not find any general correlation between absorber properties (such as [Fe/Zn] or neutral hydrogen column density) and B-K color. One of these two QSOs shows evidence for strong associated absorption from X-ray observations, an alternative explanation for its very red color. We conclude that the presence of intervening galaxies causes a minimal reddening of the background QSO.

  7. United Technologies Corporation: Achieving Competitive Excellence (ACE): Operating System Case Study

    E-Print Network [OSTI]

    Roth, George

    2010-11-30T23:59:59.000Z

    United Technologies Corporation (abbreviated UTC, NYSE ticker symbol UTX) is a large, industrial conglomerate that designs, manufactures, and services a broad range of products, ranging from air conditioners and elevators ...

  8. Review: Business and Environmental Policy: Corporate Interests in the American Political System, by Michael E. Kraft and Sheldon Kamieniecki (eds.)

    E-Print Network [OSTI]

    Meij, Jan-Martin

    2008-01-01T23:59:59.000Z

    Business and Environmental Policy: Corporate Interests ineds). Business and Environmental Policy: Corporate Interestsalso holds in the environmental policy-making realm and many

  9. Corporate Energy Management Process

    E-Print Network [OSTI]

    Geiger, T.

    2013-01-01T23:59:59.000Z

    . May 21-24, 2013 Corporate Energy Management Process 2 ?Brief introduction to BASF ? BASF Corporate Energy Management ? Management Support ? Goals ? Continuous Improvement ? Best Practices ? Recognition ?Summary ESL-IE-13-05-25 Proceedings...-value products ? Intelligent, sustainable system solutions ? 2012 Sales: ?72.1 Billion ? Employees: 110,000 Company overview BASF ? The Chemical Company ESL-IE-13-05-25 Proceedings of the Thrity-Fifth Industrial Energy Technology Conference New Orleans, LA...

  10. Corporate Affiliate Event Details

    E-Print Network [OSTI]

    Shahriar, Selim

    Corporation Tampa Bay Lightning Tenneco Inc. TreeHouse Foods, Inc. Attendee Profile 2013 Corporate Counsel

  11. IT Capital Planning Corporate Management Improvement Program (CMIP)

    Broader source: Energy.gov [DOE]

    The Corporate Management Improvement Program (CMIP) was initiated by the Department in recognition of the fact that corporate legacy systems that support administrative functions were nearing the...

  12. Sandia Corporation

    Office of Environmental Management (EM)

    Corporation Sandia National Laboratories P.O. Box 5800, MS 0101 Albuquerque, New Mexico 87185-0101 WEL-2012-01 Dear Dr. Hommert: The Office of Health, Safety and Security's...

  13. Corporate Governance and Taxation

    E-Print Network [OSTI]

    Dyck, Alexander

    2004-01-01T23:59:59.000Z

    Accounting and Corporate Governance,” Journal of Accounting1997) “A Survey of Corporate Governance” Journal of FinanceCorporate Governance and Taxation Mihir A. Desai* Harvard

  14. On the Export of U.S.-Style Corporate Fiduciary Duties to Other Cultures: Can A Transplant Take?

    E-Print Network [OSTI]

    Stout, Lynn A.

    2005-01-01T23:59:59.000Z

    able to evolve corporate governance patterns that resemble2002. How To Fix Corporate Governance, Business Week 69-78 (Cultural Theory of Corporate Governance Systems, Delaware

  15. Development of an Enterprise-wide Energy Information and Utility Monitoring System in a Major Hotel Chain: The Hyatt Hotels Corporation Experience

    E-Print Network [OSTI]

    Burke, B.; McBride, J.; Kimble, K.

    2003-01-01T23:59:59.000Z

    resident in the Hyatt data center is accessible to the individual hotels using a web-based system. Senior engineers with authorization can access data for all Hyatt Hotels in their regions. The corporate energy director and senior management have access...

  16. Mg II ABSORPTION SYSTEMS WITH W{sub 0} >= 0.1 A FOR A RADIO SELECTED SAMPLE OF 77 QUASI-STELLAR OBJECTS AND THEIR ASSOCIATED MAGNETIC FIELDS AT HIGH REDSHIFT

    SciTech Connect (OSTI)

    Bernet, M. L.; Miniati, F.; Lilly, S. J., E-mail: mbernet@phys.ethz.c, E-mail: fm@phys.ethz.c, E-mail: simon.lilly@phys.ethz.c [Physics Department, ETH Zurich, Wolfgang-Pauli-Strasse 27, CH-8093 Zurich (Switzerland)

    2010-03-01T23:59:59.000Z

    We present a catalog of Mg II absorption systems obtained from high-resolution Ultraviolet and Visual Echelle Spectrograph/VLT data of 77 quasi-stellar objects in the redshift range 0.6 < z < 2.0, and down to an equivalent width W{sub 0} >= 0.1 A. The statistical properties of our sample are found to be in agreement with those from the previous work in the literature. However, we point out that the previously observed increase with redshift of partial derivN/partial derivz for weak absorbers pertains exclusively to very weak absorbers with W{sub 0} < 0.1 A. Instead, partial derivN/partial derivz for absorbers with W{sub 0} in the range 0.1-0.3 A actually decreases with redshift, similar to the case of strong absorbers. We then use this catalog to extend our earlier analysis of the links between the Faraday rotation measure (RM) of the quasars and the presence of intervening Mg II absorbing systems in their spectra. In contrast to the case with strong Mg II absorption systems (W{sub 0} > 0.3 A), the weaker systems do not contribute significantly to the observed RM of the background quasars. This is possibly due to the higher impact parameters of the weak systems compared to strong ones, suggesting that the high column density magnetized material that is responsible for the Faraday rotation is located within about 50 kpc of the galaxies. Finally, we show that this result also rules out the possibility that some unexpected secondary correlation between the quasar redshift and its intrinsic RM is responsible for the association of high RM and strong intervening Mg II absorption that we have presented elsewhere, since this would have produced an equal effect for the weak absorption line systems, which exhibit a very similar distribution of quasar redshifts.

  17. 1. " The impact of personal and organizational factors on the use of decision support systems by the Jordanian corporations in

    E-Print Network [OSTI]

    of marketing managers in Jordan corporations enrolled in Amman Stock Exchange. A random sample has been in marketing decision - taking at the Jordan corporations with high level. 2- There were no significant the usage level of DSS when taking the marketing decisions. The study recommended the necessity

  18. Galaxy Redshifts: Improved Techniques

    E-Print Network [OSTI]

    A. F. Heavens

    1993-05-26T23:59:59.000Z

    This paper analyses the effects of random noise in determining errors and confidence levels for galaxy redshifts obtained by cross-correlation techniques. The main finding is that confidence levels have previously been overestimated, and errors inaccurately calculated in certain applications. New formul\\ae\\ are presented.

  19. Law and Corporate Governance

    E-Print Network [OSTI]

    Fligstein, Neil; Choo, Jennifer

    2005-01-01T23:59:59.000Z

    1997. A survey of corporate governance. J. Finan. 52(2):737-1999. Employees and Corporate Governance. Washington, DC:structural change in corporate governance. J. Law Soc. 27(

  20. On the gravitational redshift

    E-Print Network [OSTI]

    Klaus Wilhelm; Bhola N. Dwivedi

    2014-04-16T23:59:59.000Z

    The study of the gravitational redshift\\,---\\,a relative wavelength increase of $\\approx 2 \\times 10^{-6}$ was predicted for solar radiation by Einstein in 1908\\,---\\,is still an important subject in modern physics. In a dispute whether or not atom interferometry experiments can be employed for gravitational redshift measurements, two research teams have recently disagreed on the physical cause of the shift. Regardless of any discussion on the interferometer aspect\\,---\\,we find that both groups of authors miss the important point that the ratio of gravitational to the electrostatic forces is generally very small. For instance, the gravitational force acting on an electron in a hydrogen atom situated in the Sun's photosphere to the electrostatic force between the proton and the electron is approximately $3 \\times 10^{-21}$. A comparison of this ratio with the predicted and observed solar redshift indicates a discrepancy of many orders of magnitude. Here we show, with Einstein's early assumption of the frequency of spectral lines depending only on the generating ion itself as starting point, that a solution can be formulated based on a two-step process in analogy with Fermi's treatment of the Doppler effect. It provides a sequence of physical processes in line with the conservation of energy and momentum resulting in the observed shift and does not employ a geometric description. The gravitational field affects the release of the photon and not the atomic transition. The control parameter is the speed of light. The atomic emission is then contrasted with the gravitational redshift of matter-antimatter annihilation events.

  1. Power Reliability at BASF Corporation

    E-Print Network [OSTI]

    Theising, T. R.

    2011-01-01T23:59:59.000Z

    Power Reliability at BASF Corporation Thomas R. Theising Energy Systems Manager BASF Corporation ABSTRACT: Quality is defined not as what the supplier puts into the product but what the customer gets out and is willing to pay for. Power.... INTRODUCTION: BASF often identifies its? power quality by the effects it has on its ability to manufacture products. Improvements are made to remedy the power quality problems either through the elimination of the problems or through some means...

  2. Power Reliability at BASF Corporation

    E-Print Network [OSTI]

    Theising, T. R.

    2012-01-01T23:59:59.000Z

    Power Reliability at BASF Corporation Thomas R. Theising Energy Systems Manager BASF Corporation ABSTRACT: Quality is defined not as what the supplier puts into the product but what the customer gets out and is willing to pay for. Power.... INTRODUCTION: BASF often identifies its? power quality by the effects it has on its ability to manufacture products. Improvements are made to remedy the power quality problems either through the elimination of the problems or through some means...

  3. Organizational identity, organizational capabilities, and the evolution of the multinational corporation : JTech's transmission systems business in the US

    E-Print Network [OSTI]

    Voisey, Christopher John

    2007-01-01T23:59:59.000Z

    When a multinational corporation (MNC) internationalizes by establishing a new subsidiary, the subsidiary's evolution depends upon its acceptance within its host country environment, by its home country headquarters, by ...

  4. United Technologies Corporation: Internal Audit Department (IAD) Case Study: A Case Study of the UTC ACE Operating System

    E-Print Network [OSTI]

    Roth, George

    2008-08-11T23:59:59.000Z

    This study of United Technologies Corporation's Internal Audit Department (IAD) examines how stability and change are important factors in how this department functions and improves. IAD is a leader in the adoption of ...

  5. 3M's System-Wide Approach to Industrial Energy Efficiency: A Corporate and Facility Perspective

    E-Print Network [OSTI]

    Schultz, S. C.; Belk, V.; Asrael, J.

    optimized through re-sealing the roof, ducts, windows and wall openings to minimize infiltration of outside air. To continue these upgrades, a preventative maintenance system has been established for evaluation and replacement of exterior door weather...

  6. Abstract--The California Independent System Operator Corporation (CAISO) is in charge of managing the electricity

    E-Print Network [OSTI]

    McCalley, James D.

    the entire WECC network and consists of the detailed representation of the CAISO control grid and a simplified representation of the WECC (Western Electricity Coordinating Council) bulk power system. Creating

  7. Element Abundances at High Redshifts

    E-Print Network [OSTI]

    Max Pettini

    1999-02-11T23:59:59.000Z

    I review measurements of element abundances in different components of the high redshift universe, including the Lyman alpha forest, damped Lyman alpha systems, and Lyman break galaxies. Although progress is being made in all three areas, recent work has also produced some surprises and shown that established ideas about the nature of the damped Lyman alpha systems in particular may be too simplistic. Overall, our knowledge of metal abundances at high z is still very sketchy. Most significantly, there seems to be an order of magnitude shortfall in the comoving density of metals which have been measured up to now compared with those produced by the star formation activity seen in Lyman break galaxies. At least some of the missing metals are likely to be in hot gas in galactic halos and proto-clusters.

  8. Development of automatic operation system for coke oven machines at Yawata Works of Nippon Steel Corporation

    SciTech Connect (OSTI)

    Matsunaga, Masao; Uematsu, Hiroshi; Nakagawa, Yoji; Ishiharaguchi, Yuji

    1995-12-01T23:59:59.000Z

    The coke plant is a working environment involving heavy dust emissions, high heat and demanding physical labor. The labor-saving operation of the coke plant is an essential issue from the standpoints of not only improvement in working environment, but also reduction in fixed cost by enhancement of labor productivity. Under these circumstances, Nippon Steel has implemented the automation of coke oven machines. The first automatic operation system for coke oven machinery entered service at Oita Works in 1992, followed by the second system at the No. 5 coke oven battery of the coke plant at Yawata Works. The Yawata automatic operation system is characterized by the installation of coke oven machinery to push as many as 140 ovens per day within a short cycle time, such as a preliminary ascension pipe cap opening car and cycle time simulator by the manned operation of the pusher, which is advantageous from the standpoint of investment efficiency, and by the monitoring of other oven machines by the pusher. These measures helped to reduce the manpower requirement to 2 persons per shift from 4 persons per shift. The system entered commercial operation in March, 1994 and has been smoothly working with an average total automatic rate of 97%. Results from the startup to recent operation of the system are reported below.

  9. EA-1862: Oneida Seven Generation Corporation Waste-To-Energy System, Ashwaubenon, Wisconsin

    Broader source: Energy.gov [DOE]

    Oneida’s Energy Recovery Project would construct and operate a solid waste-to-electricity power plant on vacant property within the Bayport Industrial Center in the City of Green Bay, Brown County, Wisconsin. This energy recovery process would involve bringing municipal solid waste into the plant for sizing (shredding), sorting (removing recyclable material), and conveying into one of three pyrolytic gasification systems.

  10. Dust and Molecules at High Redshift

    E-Print Network [OSTI]

    F. Combes

    1998-12-23T23:59:59.000Z

    In the last years, progress has been very rapid in the domain of molecules at high redshift, and we know in better detail now the molecular and dust content in several systems beyond z=1 and up to z = 5. The first discovery in 1992 by Brown and van den Bout of CO lines at z=2.28 in a gravitationally lensed starburst galaxy, strongly stimulated searches of other systems, but these were harder than foreseen, and less than 10 other systems have been discovered in CO emission. Redshifts range between 2 and 5, the largest being BR1202-0725 at z=4.69. Most of these systems, if not all, are gravitationally amplified objects. Some have been discovered first through their dust emission, relatively easy to detect because of the negative K-correction effect. The detection of all these systems could give an answer about the debated question of the star-formation rate as a function of redshift. The maximum of star-formation rate, found around z=2 from optical studies, could shift to higher z if the most remote objects are hidden by dust. Absorption in front of quasars can also probe cold gas at high redshift, taking advantage of very high spatial (milli arcsec) and spectral (30m/s) resolutions. From the diffuse components, one can measure the cosmic black body temperature as a function of redshift. All these preliminary studies will be carried out at large scales with future millimeter instruments, and some perspectives are given.

  11. Control System Applicable Use Assessment of the Secure Computing Corporation - Secure Firewall (Sidewinder)

    SciTech Connect (OSTI)

    Hadley, Mark D.; Clements, Samuel L.

    2009-01-01T23:59:59.000Z

    Battelle’s National Security & Defense objective is, “applying unmatched expertise and unique facilities to deliver homeland security solutions. From detection and protection against weapons of mass destruction to emergency preparedness/response and protection of critical infrastructure, we are working with industry and government to integrate policy, operational, technological, and logistical parameters that will secure a safe future”. In an ongoing effort to meet this mission, engagements with industry that are intended to improve operational and technical attributes of commercial solutions that are related to national security initiatives are necessary. This necessity will ensure that capabilities for protecting critical infrastructure assets are considered by commercial entities in their development, design, and deployment lifecycles thus addressing the alignment of identified deficiencies and improvements needed to support national cyber security initiatives. The Secure Firewall (Sidewinder) appliance by Secure Computing was assessed for applicable use in critical infrastructure control system environments, such as electric power, nuclear and other facilities containing critical systems that require augmented protection from cyber threat. The testing was performed in the Pacific Northwest National Laboratory’s (PNNL) Electric Infrastructure Operations Center (EIOC). The Secure Firewall was tested in a network configuration that emulates a typical control center network and then evaluated. A number of observations and recommendations are included in this report relating to features currently included in the Secure Firewall that support critical infrastructure security needs.

  12. THE CONTENT OF CORPORATE FEDERALISM

    E-Print Network [OSTI]

    Bratton, William W.

    2004-01-01T23:59:59.000Z

    Federalism in Corporate Governance: Protecting ShareholderCollaborative Corporate Governance: Listing Standards, Stateof Care Stadanrd in Corporate Governance 75 Iowa L. Rev. 1,

  13. Our Corporate Residents...

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

    the quality and variety of the Corporate Residents who call ETTP home. From young start-ups to Fortune 500 corporations, Heritage Center's resources and assets are being fully...

  14. Essays on corporate bonds

    E-Print Network [OSTI]

    Bao, Jack (Jack C.)

    2009-01-01T23:59:59.000Z

    This thesis consists of three empirical essays on corporate bonds, examining the role of both credit risk and liquidity. In the first chapter, I test the ability of structural models of default to price corporate bonds in ...

  15. Corporate sustainability assessment methodology

    E-Print Network [OSTI]

    Pinchuk, Natallia

    2011-01-01T23:59:59.000Z

    Sustainability is a vague concept specifically in the context of a corporate world. There are numerous definitions for corporate sustainability and just as many ways of evaluating it. This work attempts to define, structure ...

  16. Yubing Wang EMC Corporation

    E-Print Network [OSTI]

    Claypool, Mark

    Yubing Wang EMC Corporation Hopkinton, MA 01748, USA wang_yubing@emc.com Mark Claypool Computer@cs.wpi.edu Zheng Zuo EMC Corporation Hopkinton, MA 01748, USA zuo_zheng@emc.com Abstract--The tremendous increase

  17. A radio Search for high redshift HI absorption

    E-Print Network [OSTI]

    Jayaram N. Chengalur; A. G. de Bruyn; R. Braun; C. L. Carilli

    1995-12-12T23:59:59.000Z

    Ground based optical observations have yielded considerable information on the statistics of damped-lyman alpha systems. In particular these systems are known to be the dominant repository of the observed neutral gas at high redshift. However, particularly at high redshift, there is the possibility that optical observations could be biased due to the exclusion of damped-lyman alpha systems that contain moderate to significant amounts of dust. Independent observational constraints on the neutral hydrogen content at high redshifts and the amount of dust in high redshift systems can be obtained from a radio search against the bright lobes of distant radio galaxies (which is less affected by the presence of dust in foreground damped-lyman alpha systems). We describe here a pilot radio survey along the line of sight to a small sample of high redshift radio galaxies, and also present some preliminary results. The survey uses a novel observing mode at the WSRT which enables one to make sensitive searches of a large redshift interval in a modest amount of telescope time.

  18. Indianapolis Public Transportation Corporation

    SciTech Connect (OSTI)

    Not Available

    2004-12-01T23:59:59.000Z

    Fact sheet describes the National Renewable Energy Laboratory's evaluation of Indianapolis Public Transportation Corporation's (IndyGo's) hybrid electric buses.

  19. Southwest Gas Corporation- Combined Heat and Power Program

    Broader source: Energy.gov [DOE]

    Southwest Gas Corporation (SWG) offers incentives to qualifying commercial and industrial facilities who install efficient Combined Heat and Power systems (CHP). CHP systems produce localized, on...

  20. Use of an Enterprise Energy Monitoring System to Support Building Commissioning and Overall Energy Efficiency by the Hyatt Hotels Corporation

    E-Print Network [OSTI]

    Burke, B.; McBride, J.; Kimble, K.

    2005-01-01T23:59:59.000Z

    in the data center is accessible to the individual hotels using a web browser. Supervisory Senior Engineers with authorization can access data for all hotels under their span of control. The corporate energy director and senior management have access... the enterprise data center and entered into the monthly web forms. Hotels without a UMS enter data manually. The web form data is submitted monthly, automatically generating on-line reports for: Energy Benchmarks with BTUs of energy and gallons of water...

  1. Galactosynthesis Predictions at High Redshift

    E-Print Network [OSTI]

    Ari Buchalter; Raul Jimenez; Marc Kamionkowski

    2001-02-02T23:59:59.000Z

    We predict the Tully-Fisher (TF) and surface-brightness--magnitude relation for disk galaxies at z=3 and discuss the origin of these scaling relations and their scatter. We show that the variation of the TF relation with redshift can be a potentially powerful discriminator of galaxy-formation models. In particular, the TF relation at high redshift might be used to break parameter degeneracies among galactosynthesis models at z=0, as well as to constrain the redshift distribution of collapsing dark-matter halos, the star-formation history and baryon fraction in the disk, and the distribution of halo spins.

  2. HOME OF THE FUTURE : SYSTEM OF THE FUTUREHOME OF THE FUTURE : SYSTEM OF THE FUTURE BRUCE BEIHOFF, WHIRLPOOL CORPORATION

    E-Print Network [OSTI]

    de Weck, Olivier L.

    SOLUTION SETS ·ENERGY ·ENVIRONMENTO ·PERFORMANCE ·COMFORT ·ADAPTABILITY ·SECURITY ·NEIGHBORHOOD ·BUILDING Whirlpool #12;New Forces Connecting the Home as System Stretch Models Further 21 Oct 2010 Rev 2 8MIT SDM to home redefined : new trade offs and opportunities.j p pp oLarge Energy, Environmental, and Performance

  3. CORPORATIONS APAC Tennessee Incorporated

    E-Print Network [OSTI]

    Dasgupta, Dipankar

    Business Resources Breast Cancer Eradication Initiative Incorporated Brother International Corporation Resources Incorporated ETI Corporation Corporate and Foundation Giving The University of Memphis is grateful Family of Companies KPMG Peat Marwick LLP Knox Music Incorporated Frank Ricks/Looney Ricks Kiss Lane

  4. Cold Gas at High Redshift

    E-Print Network [OSTI]

    Colin A. Norman; Robert Braun

    1995-12-20T23:59:59.000Z

    We discuss the current observational and theoretical issues concerning cold gas at high redshift and present simulations showing how a number of observational issues can be resolved with planned future instrumentation.

  5. PHOTOMETRIC REDSHIFTS OF SUBMILLIMETER GALAXIES

    SciTech Connect (OSTI)

    Chakrabarti, Sukanya [School of Physics and Astronomy, Rochester Institute of Technology, 84 Lomb Memorial Drive, Rochester, NY 14623 (United States); Magnelli, Benjamin; Lutz, Dieter; Berta, Stefano; Popesso, Paola [Max-Planck-Institut fuer Extraterrestrische Physik, Postfach 1312, Giessenbachstrasse 1, D-85741 Garching (Germany); McKee, Christopher F. [Physics and Astronomy Departments, UC Berkeley, Berkeley, CA 94720 (United States); Pozzi, Francesca, E-mail: chakrabarti@astro.rit.edu [Dipartimento di Astronomia, Universita degli Studi di Bologna, Via Ranzani 1, I-40127 Bologna (Italy)

    2013-08-20T23:59:59.000Z

    We use the photometric redshift method of Chakrabarti and McKee to infer photometric redshifts of submillimeter galaxies with far-IR (FIR) Herschel data obtained as part of the PACS Evolutionary Probe program. For the sample with spectroscopic redshifts, we demonstrate the validity of this method over a large range of redshifts (4 {approx}> z {approx}> 0.3) and luminosities, finding an average accuracy in (1 + z{sub phot})/(1 + z{sub spec}) of 10%. Thus, this method is more accurate than other FIR photometric redshift methods. This method is different from typical FIR photometric methods in deriving redshifts from the light-to-gas mass (L/M) ratio of infrared-bright galaxies inferred from the FIR spectral energy distribution, rather than dust temperatures. To assess the dependence of our photometric redshift method on the data in this sample, we contrast the average accuracy of our method when we use PACS data, versus SPIRE data, versus both PACS and SPIRE data. We also discuss potential selection effects that may affect the Herschel sample. Once the redshift is derived, we can determine physical properties of infrared-bright galaxies, including the temperature variation within the dust envelope, luminosity, mass, and surface density. We use data from the GOODS-S field to calculate the star formation rate density (SFRD) of submillimeter bright sources detected by AzTEC and PACS. The AzTEC-PACS sources, which have a threshold 850 {mu}m flux {approx}> 5 mJy, contribute 15% of the SFRD from all ultraluminous infrared galaxies (L{sub IR} {approx}> 10{sup 12} L{sub Sun }), and 3% of the total SFRD at z {approx} 2.

  6. Automotive Fuel Cell Corporation

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

    Automotive Fuel Cell Corporation n SNL researcher Cy Fujimoto demonstrates his new flexible hydrocarbon polymer electrolyte mem- brane, which could be a key factor in realizing a...

  7. STATEMENT OF CONSIDERATIONS REQUEST BY MARTIN MARIETTA CORPORATION...

    Broader source: Energy.gov (indexed) [DOE]

    MARTIN MARIETTA CORPORATION (MMC) FORMERLY KNOWN AS GENERAL DYNAMICS - SPACE SYSTEMS DIVISION (GD- SSD) FOR AN ADVANCE WAIVER OF DOMESTIC AND FOREIGN PATENT RIGHTS UNDER DOE...

  8. Corporate Headquarters 317 Route 104

    E-Print Network [OSTI]

    Firestone, Jeremy

    Sustainable Energy Developments, Inc. is a New York Corporation Founded April 2002 Visualization Phone: (978) 422 7744 Sustainable Energy Developments, Inc. is a New York Corporation Founded Energy Developments, Inc. is a New York Corporation Founded April 2002

  9. Corporate and Business Plan

    E-Print Network [OSTI]

    Corporate and Business Plan 2010-2011 #12;Main addresses Forest Research Alice Holt Lodge Farnham Research's Business Plan 2010-2011 ..........................12 Table Contents Table 1 - Income This Corporate and Business Plan sets out FR's aims and strategic objectives. It describes the Key Performance

  10. Corporate Information & Computing Services

    E-Print Network [OSTI]

    Martin, Stephen John

    Corporate Information & Computing Services High Performance Computing Report March 2008 Author The University of Sheffield's High Performance Computing (HPC) facility is provided by CiCS. It consists of both Graduate Students and Staff. #12;Corporate Information & Computing Services High Performance Computing

  11. Smith & Franklin Academic Publishing Corporation

    E-Print Network [OSTI]

    Tong, Liang

    Smith & Franklin Academic Publishing Corporation www.smithandfranklin.com Science, Religion | Pages 23 Smith & Franklin Academic Publishing Corporation www.smithandfranklin.com ic origin, meant

  12. Rutgers Business School Corporate Finance

    E-Print Network [OSTI]

    Lin, Xiaodong

    Rutgers Business School Corporate Finance Fall 2014 Instructor: Vikram Nanda Office: 5186 to the basic and current research questions and methods ­ theoretical and empirical ­ in corporate finance areas in corporate finance. Among these: · Tirole, Corporate Finance · Finance Handbooks such as: Jarrow

  13. Old Galaxies at High Redshift

    E-Print Network [OSTI]

    James Dunlop

    1997-05-13T23:59:59.000Z

    The most passive galaxies at high redshift are unlikely to be identified by either narrow-band emission-line searches, or by Lyman limit searches (both techniques which have been highlighted at this meeting) simply because such selection methods rely on the presence of a strong ultraviolet component. Selection on the basis of extreme radio power has also proved to yield optically active objects with the majority of high-redshift objects studied to date displaying complex elongated optical/UV morphologies, relatively blue optical-ultraviolet continuum colours, and strong emission lines. These features, coupled with the failure to detect any spectral signatures of old stars at $z > 1$, has led to the suggestion that these galaxies are being observed close to or even during a general epoch of formation. However, we have recently demonstrated that radio selection at significantly fainter (mJy) flux densities can be used to identify apparently passively evolving elliptical galaxies at high redshift. Deep Keck spectra have now been obtained for two such objects yielding absorption line redshifts $z \\simeq 1.5$; 53W091 at $z = 1.552$ (Dunlop et al. 1996) and most recently 53W069 at $z = 1.432$. The ultraviolet SEDs of these galaxies indicate minimum ages $> 3$ Gyr while, as stressed in this article, the strength of the reddenning-independent ultraviolet spectral breaks actually indicate a greater minimum age of 5 Gyr for both objects assuming solar metallicity. Since the spectra comprise the integrated light of each galaxy to radii greater than $r_e$, I argue that it is difficult to justify the adoption of significantly super-solar metallicity in interpreting these data. It thus seems hard to escape the conclusion that $\\Omega_0 5$).

  14. Equivalence Principle and Gravitational Redshift

    SciTech Connect (OSTI)

    Hohensee, Michael A.; Chu, Steven; Mueller, Holger [Department of Physics, University of California, Berkeley, California 94720 (United States); Peters, Achim [Institut fuer Physik, Humboldt-Universitaet zu Berlin, Newtonstrasse 15, 12489 Berlin (Germany)

    2011-04-15T23:59:59.000Z

    We investigate leading order deviations from general relativity that violate the Einstein equivalence principle in the gravitational standard model extension. We show that redshift experiments based on matter waves and clock comparisons are equivalent to one another. Consideration of torsion balance tests, along with matter-wave, microwave, optical, and Moessbauer clock tests, yields comprehensive limits on spin-independent Einstein equivalence principle-violating standard model extension terms at the 10{sup -6} level.

  15. The Galaxy Structure-Redshift Relationship

    E-Print Network [OSTI]

    Christopher Conselice

    2004-07-21T23:59:59.000Z

    There exists a gradual, but persistent, evolutionary effect in the galaxy population such that galaxy structure and morphology change with redshift. This galaxy structure-redshift relationship is such that an increasingly large fraction of all bright and massive galaxies at redshifts 2 < z < 3 are morphologically peculiar at wavelengths from rest-frame ultraviolet to rest-frame optical. There are however examples of morphologically selected spirals and ellipticals at all redshifts up to z ~ 3. At lower redshift, the bright galaxy population smoothly transforms into normal ellipticals and spirals. The rate of this transformation strongly depends on redshift, with the swiftest evolution occurring between 1 < z < 2. This review characterizes the galaxy structure-redshift relationship, discusses its various physical causes, and how these are revealing the mechanisms responsible for galaxy formation.

  16. Well-posedness of Einstein's Equation with Redshift Data

    E-Print Network [OSTI]

    Christopher Winfield

    2011-11-22T23:59:59.000Z

    We study the solvability of a system of ordinary differential equations derived from null geodesics of the LTB metric with data given in terms of a so-called redshift parameter. Data is introduced along these geodesics by the luminosity distance function. We check our results with luminosity distance depending on the cosmological constant and with the well-known FRW model.

  17. Statement by Harvard Corporation Committee on Shareholder Responsibility (CCSR) Regarding Stock in China Petroleum and Chemical Corporation (Sinopec Corporation)

    E-Print Network [OSTI]

    Corporation and its closely affiliated parent company, China Petrochemical Corporation (Sinopec Group listed company in which a dominant (68 percent) interest is held by China Petrochemical Corporation

  18. Redshift of photons penetrating a hot plasma

    E-Print Network [OSTI]

    Ari Brynjolfsson

    2005-10-07T23:59:59.000Z

    A new interaction, plasma redshift, is derived, which is important only when photons penetrate a hot, sparse electron plasma. The derivation of plasma redshift is based entirely on conventional axioms of physics. When photons penetrate a cold and dense plasma, they lose energy through ionization and excitation, Compton scattering on the individual electrons, and Raman scattering on the plasma frequency. But in sparse hot plasma, such as in the solar corona, the photons lose energy also in plasma redshift. The energy loss per electron in the plasma redshift is about equal to the product of the photon's energy and one half of the Compton cross-section per electron. In quiescent solar corona, this heating starts in the transition zone to the corona and is a major fraction of the coronal heating. Plasma redshift contributes also to the heating of the interstellar plasma, the galactic corona, and the intergalactic plasma. Plasma redshift explains the solar redshifts, the redshifts of the galactic corona, the cosmological redshifts, the cosmic microwave background, and the X-ray background. The plasma redshift explains the observed magnitude-redshift relation for supernovae SNe Ia without the big bang, dark matter, or dark energy. There is no cosmic time dilation. The universe is not expanding. The plasma redshift, when compared with experiments, shows that the photons' classical gravitational redshifts are reversed as the photons move from the Sun to the Earth. This is a quantum mechanical effect. As seen from the Earth, a repulsion force acts on the photons. This means that there is no need for Einstein's Lambda term. The universe is quasi-static, infinite, and everlasting.

  19. Corporate Law's Current-Owner Bias

    E-Print Network [OSTI]

    Fried, Jesse M.

    2005-01-01T23:59:59.000Z

    Owner Bias in Corporate Governance Jesse Fried * Boalt Hallmy conclusion that corporate governance arrangements choseninterventions in corporate governance through the securities

  20. Corporate Law's Current-Owner Bias

    E-Print Network [OSTI]

    Fried, Jesse M.

    2006-01-01T23:59:59.000Z

    Owner Bias in Corporate Governance Jesse Fried * Boalt Hallmy conclusion that corporate governance arrangements choseninterventions in corporate governance through the securities

  1. Corporate Governance, the Environment, and the Internet

    E-Print Network [OSTI]

    Andrew, Jane

    2003-01-01T23:59:59.000Z

    contemporary society: Corporate governance at a crossroads.R. (1997). A survey of corporate governance. The Journal ofCorporate Governance, the Environment, and the Internet Jane

  2. Lesson from Fiascos in Russian Corporate Governance

    E-Print Network [OSTI]

    Fox, Merritt; Heller, Michael

    2000-01-01T23:59:59.000Z

    Cause Corporate Governance Failures . . . . . . . . . 1.understanding of how corporate governance works. See Heller,Shareholders in Corporate Governance (1999) (mimeo on file

  3. Lesson from Fiascos in Russian Corporate Governance

    E-Print Network [OSTI]

    Fox, Merritt B.; Heller, Michael A.

    1999-01-01T23:59:59.000Z

    Cause Corporate Governance Failures . . . . . . . . . 1.understanding of how corporate governance works. See Heller,Shareholders in Corporate Governance (1999) (mimeo on file

  4. Capital Structure Implications for Corporate Governance

    E-Print Network [OSTI]

    Rajan, Nishanth

    2012-01-01T23:59:59.000Z

    A. R¨oell, 2002, “Corporate governance and control,” ECGI-Enjoying the quiet life? Corporate governance and managerialGrinstein, 2007, “Corporate governance and firm value: The

  5. Quality Assurance Corporate Board | Department of Energy

    Broader source: Energy.gov (indexed) [DOE]

    Assurance Corporate Board Quality Assurance Corporate Board The Office of Environmental Management (EM) Quality Assurance Corporate Board is an executive board that includes both...

  6. Sojitz Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnualProperty Edit with form HistoryRistmaSinosteel CorporationSocovoltaic SystemsSoitec SA

  7. The Earth Institute I Corporate Circle Spring 2011

    E-Print Network [OSTI]

    Khatiwala, Samar

    ,000 in unrestricted support, to be renewed once a year · Support the on-going sustainable development work on strategic plans, metrics, operations as relates to energy, water, sustainable food systems, etc. · Corporate #12;The Earth Institute I Corporate Circle Indicative examples Global: · PepsiCo: water & energy

  8. Constraints of Dark Energy at High Redshift

    E-Print Network [OSTI]

    Qiping Su; Rong-Gen Cai

    2014-08-24T23:59:59.000Z

    Constrains of dark energy (DE) at high redshift from current and mock future observational data are obtained. It is found that present data give poor constraints of DE even beyond redshift z=0.4, and mock future 2298 type Ia supernove data only give a little improvement of the constraints. We analyze in detail why constraints of DE decrease rapidly with the increasing of redshift. Then we try to improve the constraints of DE at high redshift. It is shown that the most efficient way is to improve the error of observations.

  9. RVSAO 2.0: Digital Redshifts and Radial Velocities

    E-Print Network [OSTI]

    Michael J. Kurtz; Douglas J. Mink

    1998-03-25T23:59:59.000Z

    RVSAO is a set of programs to obtain redshifts and radial velocities from digital spectra. RVSAO operates in the IRAF(Tody 1986, 1993) environment. The heart of the system is xcsao, which implements the cross-correlation method, and is a direct descendant of the system built by Tonry and Davis (1979). emsao uses intelligent heuristics to search for emission lines in spectra, then fits them to obtain a redshift. sumspec shifts and sums spectra to build templates for cross-correlation. linespec builds synthetic spectra given a list of spectral lines. bcvcorr corrects velocities for the motion of the earth. We discuss in detail the parameters necessary to run xcsao and emsao properly. We discuss the reliability and error associated with xcsao derived redshifts. We develop an internal error estimator, and we show how large, stable surveys can be used to develop more accurate error estimators. We develop a new methodology for building spectral templates for galaxy redshifts. We show how to obtain correlation velocities using emission line templates. Emission line correlations are substantially more efficient than the previous standard technique, automated emission line fitting. We compare the use of RVSAO with new methods, which use Singular Value Decomposition and $\\chi^2$ fitting techniques.

  10. Essays in Behavioral Corporate Finance

    E-Print Network [OSTI]

    Zheng, Hui

    2012-01-01T23:59:59.000Z

    and practice of corporate finance: evidence from the field,Journal of Applied Corporate Finance 15, 8–23. 18. Graham,governance, Journal of Finance 63, 2737–2784. 21. Hackbarth,

  11. Corporate governance and insider trading

    E-Print Network [OSTI]

    Rozanov, Konstantin A

    2008-01-01T23:59:59.000Z

    I investigate the relation between corporate governance and insider trading by corporate executives. Despite the general view that trade on non-public information adversely affects capital market participants, the impact ...

  12. Corporate governance and banking regulation

    E-Print Network [OSTI]

    Alexander, Kern

    The globalisation of banking markets has raised important issues regarding corporate governance regulation for banking institutions. This research paper addresses some of the major issues of corporate governance as it relates to banking regulation...

  13. 3M Corporation Abbott Laboratories

    E-Print Network [OSTI]

    Napier, Terrence

    . Agilent Technologies, Inc. Air Products Foundation Alaska Airlines Albemarle Corporation Alcoa Foundation Energy Group, Inc. Corning Incorporated Foundation Crayola, LLC Deloitte Foundation Delta Air Lines3M Corporation Abbott Laboratories Adage Capital Management, LP Adams Electric Cooperative, Inc

  14. Forestry Commission England Corporate Plan

    E-Print Network [OSTI]

    Forestry Commission England Corporate Plan 2011-15 This is the Corporate Plan for the Forestry Commission in England. It is one of a suite of plans including those for Forestry Commission (GB) and Forest Research. Page 1Forestry Commission England Corporate Plan 2011-15 #12;Page 2Forestry Commission England

  15. Press Release Corporate Communications

    E-Print Network [OSTI]

    Haller-Dintelmann, Robert

    Page: 1/2 Press Release Corporate Communications Karolinenplatz 5 D-64289 Darmstadt Germany Your.ch@pvw.tu- darmstadt.de Internet: http://www.tu- darmstadt.de/presse e-mail: presse@tu-darmstadt.de On Cloud Nine TU). She intends to use the funding for basic research into the programming of software that will be fit

  16. Antecedents of corporate volunteerism

    E-Print Network [OSTI]

    Henning, Jaime Blaine

    2009-05-15T23:59:59.000Z

    LIST OF FIGURES FIGURE Page 1 Hypothesized relationships between the perceived locus of causality, functional motives, and theory of planned behavior variables ....................... 41 2 Significant... engages in, independent of work, with or without the support of the employer, whereas corporate volunteerism (CV) requires some form of knowledge and support for the volunteering on the part of the employer (Graff, 2004; Lukka, 2000; Seel, 1995...

  17. Photometric Redshifts in the IRAC Shallow Survey

    SciTech Connect (OSTI)

    Brodwin, M; Brown, M; Ashby, M; Bian, C; Brand, K; Dey, A; Eisenhardt, P; Eisenstein, D; Gonzalez, A; Huang, J; Kochanek, C; McKenzie, E; Pahre, M; Smith, H; Soifer, B; Stanford, S; Stern, D; Elston, R

    2006-06-13T23:59:59.000Z

    Accurate photometric redshifts are calculated for nearly 200,000 galaxies to a 4.5 micron flux limit of {approx} 13 {micro}Jy in the 8.5 deg{sup 2} Spitzer/IRAC Shallow survey. Using a hybrid photometric redshift algorithm incorporating both neural-net and template-fitting techniques, calibrated with over 15,000 spectroscopic redshifts, a redshift accuracy of {sigma} = 0.06 (1+z) is achieved for 95% of galaxies at 0 < z < 1.5. The accuracy is {sigma} = 0.12 (1 + z) for 95% of AGN at 0 < z < 3. Redshift probability functions, central to several ongoing studies of the galaxy population, are computed for the full sample. We demonstrate that these functions accurately represent the true redshift probability density, allowing the calculation of valid confidence intervals for all objects. These probability functions have already been used to successfully identify a population of Spitzer-selected high redshift (z > 1) galaxy clusters. We present one such spectroscopically confirmed cluster at = 1.24, ISCS J1434.2+3426. Finally, we present a measurement of the 4.5 {micro}m-selected galaxy redshift distribution.

  18. Measuring Galaxy Environments with Deep Redshift Surveys

    E-Print Network [OSTI]

    Michael C. Cooper; Jeffrey A. Newman; Darren S. Madgwick; Brian F. Gerke; Renbin Yan; Marc Davis

    2005-06-21T23:59:59.000Z

    We study the applicability of several galaxy environment measures (n^th-nearest-neighbor distance, counts in an aperture, and Voronoi volume) within deep redshift surveys. Mock galaxy catalogs are employed to mimic representative photometric and spectroscopic surveys at high redshift (z ~ 1). We investigate the effects of survey edges, redshift precision, redshift-space distortions, and target selection upon each environment measure. We find that even optimistic photometric redshift errors (\\sigma_z = 0.02) smear out the line-of-sight galaxy distribution irretrievably on small scales; this significantly limits the application of photometric redshift surveys to environment studies. Edges and holes in a survey field dramatically affect the estimation of environment, with the impact of edge effects depending upon the adopted environment measure. These edge effects considerably limit the usefulness of smaller survey fields (e.g. the GOODS fields) for studies of galaxy environment. In even the poorest groups and clusters, redshift-space distortions limit the effectiveness of each environment statistic; measuring density in projection (e.g. using counts in a cylindrical aperture or a projected n^th-nearest-neighbor distance measure) significantly improves the accuracy of measures in such over-dense environments. For the DEEP2 Galaxy Redshift Survey, we conclude that among the environment estimators tested the projected n^th-nearest-neighbor distance measure provides the most accurate estimate of local galaxy density over a continuous and broad range of scales.

  19. Optical Approach to Gravitational Redshift

    E-Print Network [OSTI]

    Y. G. Yi

    2012-04-12T23:59:59.000Z

    An optical approach begins by interpreting the gravitational redshift resulting to a change in the relative velocity of light due to the medium of propagation in the gravitational field. The discussion continues by pointing out an agreement in structure between the equation for rays in geometrical optics and the geodesic equation of general relativity. From their comparison we learn that the path of rays should be given by the relation $ds^2=n^2(r)dr^2+r^2d\\theta^2$, not by $ds^2=dr^2+r^2d\\theta^2$, in a medium with spherical symmetry of refractive index $n(r)$. The development of an optical analogy suggests introducing $n^2(r)$ in place of $g_{rr}$ as an optical version of the Schwarzschild metric. In form and content, $n^2(r)$ is different from $g_{rr}$. The optical point of view replaces the general-relativity explanations in terms of time and gravitation.

  20. Chemical Enrichment at High Redshifts

    E-Print Network [OSTI]

    Snigdha Das; Pushpa Khare

    1998-08-09T23:59:59.000Z

    We have tried to understand the recent observations related to metallicity in Ly $\\alpha$ forest clouds in the framework of the two component model suggested by Chiba & Nath (1997). We find that even if the mini-halos were chemically enriched by an earlier generation of stars, to have [C/H] $\\simeq$ -2.5, the number of C IV lines with column density $>10^{12} cm^{-2}$, contributed by the mini-halos, at the redshift of 3, would be only about 10% of the total number of lines, for a chemical enrichment rate of $(1+z)^{-3}$ in the galaxies. Recently reported absence of heavy element lines associated with most of the Ly $\\alpha$ lines with H I column density between $10^{13.5} cm^{-2}$ and $10^{14} cm^{-2}$ by Lu et al (1998), if correct, gives an upper limit on [C/H]=-3.7, not only in the mini-halos, but also in the outer parts of galactic halos. This is consistent with the results of numerical simulations, according to which, the chemical elements associated with the Ly $\\alpha$ clouds are formed in situ in clouds, rather than in an earlier generation of stars. However, the mean value of $7 \\times 10^{-3}$ for the column density ratio of C IV and H I, determined by Cowie and Songaila (1998) for low Lyman alpha optical depths, implies an abundance of [C/H] =-2.5 in mini-halos as well as in most of the region in galactic halos, presumably enriched by an earlier generation of stars. The redshift and column density distribution of C IV has been shown to be in reasonable agreement with the observations.

  1. Estimating photometric redshifts with artificial neural networks

    E-Print Network [OSTI]

    Andrew E. Firth; Ofer Lahav; Rachel S. Somerville

    2002-10-21T23:59:59.000Z

    A new approach to estimating photometric redshifts - using Artificial Neural Networks (ANNs) - is investigated. Unlike the standard template-fitting photometric redshift technique, a large spectroscopically-identified training set is required but, where one is available, ANNs produce photometric redshift accuracies at least as good as and often better than the template-fitting method. The Bayesian priors on the underlying redshift distribution are automatically taken into account. Furthermore, inputs other than galaxy colours - such as morphology, angular size and surface brightness - may be easily incorporated, and their utility assessed. Different ANN architectures are tested on a semi-analytic model galaxy catalogue and the results are compared with the template-fitting method. Finally the method is tested on a sample of ~ 20000 galaxies from the Sloan Digital Sky Survey. The r.m.s. redshift error in the range z < 0.35 is ~ 0.021.

  2. The kinematic component of the cosmological redshift

    E-Print Network [OSTI]

    Micha? Chodorowski

    2011-03-08T23:59:59.000Z

    It is widely believed that the cosmological redshift is not a Doppler shift. However, Bunn & Hogg have recently pointed out that to settle properly this problem, one has to transport parallelly the velocity four-vector of a distant galaxy to the observer's position. Performing such a transport along the null geodesic of photons arriving from the galaxy, they found that the cosmological redshift is purely kinematic. Here we argue that one should rather transport the velocity four-vector along the geodesic connecting the points of intersection of the world-lines of the galaxy and the observer with the hypersurface of constant cosmic time. We find that the resulting relation between the transported velocity and the redshift of arriving photons is not given by a relativistic Doppler formula. Instead, for small redshifts it coincides with the well known non-relativistic decomposition of the redshift into a Doppler (kinematic) component and a gravitational one. We perform such a decomposition for arbitrary large redshifts and derive a formula for the kinematic component of the cosmological redshift, valid for any FLRW cosmology. In particular, in a universe with Omega_m = 0.24 and Omega_Lambda = 0.76, a quasar at a redshift 6, at the time of emission of photons reaching us today had the recession velocity v = 0.997c. This can be contrasted with v = 0.96c, had the redshift been entirely kinematic. Thus, for recession velocities of such high-redshift sources, the effect of deceleration of the early Universe clearly prevails over the effect of its relatively recent acceleration. Last but not least, we show that the so-called proper recession velocities of galaxies, commonly used in cosmology, are in fact radial components of the galaxies' four-velocity vectors. As such, they can indeed attain superluminal values, but should not be regarded as real velocities.

  3. Japanese Corporate Governance: The Hidden Problems of the Corporate Law and Their Solutions

    E-Print Network [OSTI]

    Shishido, Zenichi

    1999-01-01T23:59:59.000Z

    norm. Japanese Corporate Governance: The Hidden Problems ofsame time. Arguments on corporate governance can be dividedinto two types: corporate governance in the narrow sense and

  4. Surface brightness in plasma-redshift cosmology

    E-Print Network [OSTI]

    Ari Brynjolfsson

    2006-05-31T23:59:59.000Z

    In 2001 Lori M. Lubin and Allan Sandage, using big-bang cosmology for interpreting the data, found the surface brightness of galaxies to be inversely proportional to about the third power of (1+z), while the contemporary big-bang cosmology predicts that the surface brightness is inversely proportional to the fourth power of (1+z). In contrast, these surface brightness observations are in agreement with the predictions of the plasma-redshift cosmology. Lubin and Sandage (2001) and Barden et al. (2005), who surmised the big-bang expansion, interpreted the observations to indicate that the diameters of galaxies are inversely proportional to (1+z). In contrast, when assuming plasma-redshift cosmology, the diameters of galaxies are observed to be constant independent of redshift and any expansion. Lubin and Sandage (2001) and Barden et al. (2005), when using big-bang cosmology, observed the average absolute magnitude of galaxies to decrease with redshift; while in plasma redshift cosmology it is a constant. Lubin and Sandage and Barden et al. suggested that a coherent evolution could explain the discrepancy between the observed relations and those predicted in the big-bang cosmology. We have failed to find support for this explanation. We consider the observed relations between the redshift and the surface-brightness, the galaxy diameter, and the absolute magnitude to be robust confirmations of plasma-redshift cosmology.

  5. Mining the Sky with Redshift Surveys

    E-Print Network [OSTI]

    Marc Davis; Jeffrey Newman

    2001-04-25T23:59:59.000Z

    Since the late 1970's, redshift surveys have been vital for progress in understanding large-scale structure in the Universe. The original CfA redshift survey collected spectra of 20-30 galaxies per clear night on a 1.5 meter telescope; over a two year period the project added ~2000 new redshifts to the literature. Subsequent low-z redshift surveys have been up to an order of magnitude larger, and ongoing surveys will yield a similar improvement over the generation preceding them. Full sky redshift surveys have a special role to play as predictors of cosmological flows, and deep pencil beam surveys have provided fundamental constraints on the evolution of properties of galaxies. With the 2DF redshift survey and the SDSS survey, our knowledge of the statistical clustering of low-redshift galaxies will achieve unprecedented precision. Measurements of clustering in the distant Universe are more limited at present, but will become much better in this decade as the VLT/VIRMOS and Keck/DEIMOS projects produce results. As in so many other fields, progress in large scale structure studies, both observational and theoretical, has been made possible by improvements in technologies, especially computing. This review briefly highlights twenty years of progress in this evolving discipline and describes a few novel cosmological tests that will be attempted with the Keck/DEIMOS survey.

  6. Benchmarking Corporate Energy Management

    E-Print Network [OSTI]

    Norland, D. L.

    BENCHMARKING CORPORATE ENERGY MANAGEMENT Dr. Douglas L. Norland Director of Research and Industrial Programs Alliance to Save Energy Washington, DC ABSTRACT There is growing interest among energy managers in finding out how their company...'s energy management procedures and perfonnance compare to that of other companies. Energy management involves everything from setting goals and targets to implementing best maintenance practices. This paper, however, discusses benchmarking energy...

  7. STATEMENT OF CONSIDERATIONS REQUEST BY EATON CORPORATION FOR...

    Broader source: Energy.gov (indexed) [DOE]

    EATON CORPORATION FOR AN ADVANCE WAIVER OF PATENT RIGHTS UNDER SUBCONTRACT NO. NREL-ZCL-2-32060-01 ENTITLED "ADVANCED HEAVY HYBRID PROPULSION SYSTEMS FOR INCREASE FUEL EFFICIENCY...

  8. Redshift indicators for gamma-ray bursts

    E-Print Network [OSTI]

    J-L. Atteia

    2005-05-04T23:59:59.000Z

    The measure of the distances and luminosities of gamma-ray bursts (GRBs) led to the discovery that many GRB properties are strongly correlated with their intrinsic luminosity, leading to the construction of reliable luminosity indicators. These GRB luminosity indicators have quickly found applications, like the construction of 'pseudo-redshifts', or the measure of luminosity distances, which can be computed independently of the measure of the redshift. In this contribution I discuss various issues connected with the construction of luminosity-redshift indicators for gamma-ray bursts.

  9. Corporate Headquarters Cisco Systems, Inc.

    E-Print Network [OSTI]

    Brody, James P.

    and any other company. (0501R) OL-7762-01 Quick Reference Cisco IP Phone 7961G/7961G-GE and 7941G/7941G number DirTrfr Transfer two calls to each other EditDial Edit a number in a call log EndCall Disconnect If you want to... Then... View or dial from your call logs Press . Choose a call log. To dial, scroll

  10. Transition redshift in $f(T)$ cosmology and observational constraints

    E-Print Network [OSTI]

    Capozziello, Salvatore; Saridakis, Emmanuel N

    2015-01-01T23:59:59.000Z

    We extract constraints on the transition redshift $z_{tr}$, determining the onset of cosmic acceleration, predicted by an effective cosmographic construction, in the framework of $f(T)$ gravity. In particular, employing cosmography we obtain bounds on the viable $f(T)$ forms and their derivatives. Since this procedure is model independent, as long as the scalar curvature is fixed, we are able to determine intervals for $z_{tr}$. In this way we guarantee that the Solar-System constraints are preserved and moreover we extract bounds on the transition time and the free parameters of the scenario. We find that the transition redshifts predicted by $f(T)$ cosmology, although compatible with the standard $\\Lambda$CDM predictions, are slightly smaller. Finally, in order to obtain observational constraints on $f(T)$ cosmology, we perform a Monte Carlo fitting using supernova data, involving the most recent union 2.1 data set.

  11. SPECTROSCOPIC REDSHIFTS OF GALAXIES WITHIN THE FRONTIER FIELDS

    SciTech Connect (OSTI)

    Ebeling, Harald; Ma, Cheng-Jiun; Barrett, Elizabeth [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States)

    2014-04-01T23:59:59.000Z

    We present a catalog of 1921 spectroscopic redshifts measured in the fields of the massive galaxy clusters MACSJ0416.1–2403 (z = 0.397), MACSJ0717.5+3745 (z = 0.546), and MACSJ1149.5+2223 (z = 0.544), i.e., three of the four clusters selected by Space Telescope Science Institute as the targets of the Frontier Fields (FFs) initiative for studies of the distant Universe via gravitational lensing. Compiled in the course of the Massive Cluster Survey project (MACS) that detected the FF clusters, this catalog is provided to the community for three purposes: (1) to allow the identification of cluster members for studies of the galaxy population of these extreme systems, (2) to facilitate the removal of unlensed galaxies and thus reduce shear dilution in weak-lensing analyses, and (3) to improve the calibration of photometric redshifts based on both ground- and spacebased observations of the FF clusters.

  12. Multi-object spectroscopy of low redshift EIS clusters. III. Properties of optically selected clusters

    E-Print Network [OSTI]

    L. F. Olsen; C. Benoist; L. da Costa; L. Hansen; H. E. Jorgensen

    2005-02-25T23:59:59.000Z

    We have carried out an investigation of the properties of low redshift EIS clusters using both spectroscopy and imaging data. We present new redshifts for 738 galaxies in 21 ESO Imaging Survey (EIS) Cluster fields. We use the ``gap''-technique to search for significant overdensities in redshift space and to identify groups/clusters of galaxies corresponding to the original EIS matched filter cluster candidates. In this way we spectroscopically confirm 20 of the 21 cluster candidates with a matched-filter estimated redshift z_MF=0.2. We have now obtained spectroscopic redshifts for 34 EIS cluster candidates with z_MF=0.2 (see also Hansen et al., 2002; Olsen et al., 2003). Of those we spectroscopically confirm 32 with redshifts ranging from z=0.064 to 0.283. We find that: 1) the velocity dispersions of the systems range from sigma_v<=130km/s to sigma_v=1200km/s, typical of galaxy groups to rich clusters; 2) richnesses corresponding to Abell classes R<=1; and 3) concentration indices ranging from C=0.2 to C=1.2. From the analysis of the colours of the galaxy populations we find that 53% of the spectroscopically confirmed systems have a ``significant'' red sequence. These systems are on average richer and have higher velocity dispersions. We find that the colour of the red sequence galaxies matches passive stellar evolution predictions.

  13. Gender Diversity in Corporate Leadership

    E-Print Network [OSTI]

    McLean, Lindsey

    2011-01-01T23:59:59.000Z

    ceiling’ and attain top leadership positions has positivehierarchy. Thus, changing leadership may be a mechanism toDiversity in Corporate Leadership RECENTLY RELEASED WORKING

  14. Refining and Extending the Business Model with Information Technology: Dell Computer Corporation

    E-Print Network [OSTI]

    Kraemer, Kenneth L; Dedrick, Jason; Yamashiro, Sandra

    1999-01-01T23:59:59.000Z

    SAP implementation was dubbed the Genesis Project, and involved a 140 member staff pulled together from corporate and regional information systems

  15. THE AEROSPACE CORPORATION

    Office of Legacy Management (LM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn AprilA group currentBradleyTableSelling7 AugustAFRICAN3uj: ;;I : T' j-jE: i tCORPORATION

  16. Cosmic Streaming Field at Low Redshift

    E-Print Network [OSTI]

    Lifan Wang

    2007-05-04T23:59:59.000Z

    We study the expansion of the nearby Universe using a sample of Type Ia supernovae at redshifts below 0.08. These supernovae allow peculiar velocities to be measured at unprecedented precision. We have investigated in detail the possibility of a varying Hubble constant with redshift and found no evidence of a monopole term for the nearby Universe. A large scale streaming motion is found at an amplitude of about $340^{63}_{-71}$ km/sec, aligned in the direction of $(l_0, b_0) = (312^{\\rm o}.0^{13.5}_{-7.4}, 25^{\\rm o}.7^{8.0}_{-9.2})$, which is close to the direction of the center of Shapley supercluster of galaxies. The large scale streaming motion is best fit by a function involving a strong bipolar term. The streaming velocity field extends from the lowest redshift ($\\sim 0.007$) to beyond 0.025 and likely out to even higher redshifts. The velocity field at redshift below 0.01 can be equally well described by a dipole field or by the same bipolar streaming velocity field that reaches out to beyond $z \\sim 0.025$. We are also able to deduce a robust estimate of the random velocity component of the peculiar velocity field. Within the volume of redshift below 0.01 (weighted average redshift of $\\sim$ 0.067), this thermal component is found to be about 270 km/sec. After correcting this smooth streaming motion, we are able to significantly improve the Hubble expansion fits of these supernovae. The CMAGIC method gives a dramatic decrease of $\\chi^2$ from 90 to 63 for 69 degrees of freedom, and yields a residual scatter of only 0.12 magnitude; the maximum light method gives also a moderate improvement.

  17. LANL named 2010 top corporate volunteer organization

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

    2010 top corporate volunteer organization LANL named 2010 top corporate volunteer organization The Laboratory ranked ahead of dozens of other qualifying companies with 10,000 or...

  18. Siemens Pittsburgh, PA Novelis Corporation Atlanta, GA

    E-Print Network [OSTI]

    McGaughey, Alan

    Industrial Design ­ Shanghai, China Eaton Corporation ­ Pittsburgh, PA CMU, CTTEC ­ PittsburghSiemens ­ Pittsburgh, PA Novelis Corporation ­ Atlanta, GA Expense

  19. CMB and Molecules at High Redshift

    E-Print Network [OSTI]

    F. Combes

    1999-01-17T23:59:59.000Z

    It becomes possible now to detect cold molecules at high redshift in the millimeter domain. Since the first discovery in 1992 by Brown and van den Bout of CO lines at z=2.28 in a gravitationally lensed starburst galaxy, nearly ten objects are now known to possess large quantities of molecular gas beyond z=1 and up to z = 5, through millimeter and sub-millimeter emission lines. The continuum dust emission is the most easily detected: in the mm domain, the emission is stronger for the more redshifted objects. For the CO lines, the situation is less favorable, and the reported detections are helped by gravitational amplification. The increase of the CMB temperature T_{bg} with redshift helps the rotational line excitation (especially at high z), but not its detection. Absorption in front of quasars is a more sensitive probe of cold gas at high redshift, able to detect individual clouds of a few solar masses (instead of 10^{10} Mo for emission). From the diffuse components, one can measure the cosmic black body temperature as a function of redshift. The high column densities component allow to observe important molecules not observable from the ground, like O2, H2O and LiH for example.

  20. Detecting the Gravitational Redshift of Cluster Gas

    E-Print Network [OSTI]

    Tom Broadhurst; Evan Scannapieco

    2000-03-08T23:59:59.000Z

    We examine the gravitational redshift of radiation emitted from within the potential of a cluster. Spectral lines from the intracluster medium (ICM) are redshifted in proportion to the emission-weighted mean potential along the line of sight, amounting to approximately 50 km/s at a radius of 100 kpc/h, for a cluster dispersion of 1200 km/s. We show that the relative redshifts of different ionization states of metals in the ICM provide a unique probe of the three-dimensional matter distribution. An examination of the reported peculiar velocities of cD galaxies in well studied Abell clusters reveals they are typically redshifted by an average of $\\sim +200$ km/s. This can be achieved by gravity with the addition of a steep central potential associated with the cD galaxy. Note that in general gravitational redshifts cause a small overestimate of the recessional velocities of clusters by an average of $\\sim$ 20 km/s.

  1. Atom Interferometers and the Gravitational Redshift

    E-Print Network [OSTI]

    Supurna Sinha; Joseph Samuel

    2011-05-16T23:59:59.000Z

    From the principle of equivalence, Einstein predicted that clocks slow down in a gravitational field. Since the general theory of relativity is based on the principle of equivalence, it is essential to test this prediction accurately. Muller, Peters and Chu claim that a reinterpretation of decade old experiments with atom interferometers leads to a sensitive test of this gravitational redshift effect at the Compton frequency. Wolf et al dispute this claim and adduce arguments against it. In this article, we distill these arguments to a single fundamental objection: an atom is NOT a clock ticking at the Compton frequency. We conclude that atom interferometry experiments conducted to date do not yield such sensitive tests of the gravitational redshift. Finally, we suggest a new interferometric experiment to measure the gravitational redshift, which realises a quantum version of the classical clock "paradox".

  2. GLAST observation of high-redshift GRBs

    SciTech Connect (OSTI)

    Bissaldi, Elisabetta; Longo, Francesco; Barbiellini, Guido [Dipartimento di Fisica, Universita di Trieste, Via Valerio 2, 34100, Trieste (Italy); INFN, Sezione di Trieste, Via Valerio 2, 34100, Trieste (Italy); Calura, Francesco [INAF - Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, 34131 Trieste (Italy); Matteucci, Francesca [Dipartimento di Astronomia, Universita di Trieste, Via G. B. Tiepolo 11, 34131 Trieste (Italy); INAF - Osservatorio Astronomico di Trieste, via G.B. Tiepolo 11, 34131 Trieste (Italy); Omodei, Nicola [INFN, Sezione di Pisa, Edificio C - Polo Fibonacci, Largo B. Pontecorvo 3, 56127, Pisa (Italy)

    2007-07-12T23:59:59.000Z

    We compare predicted Type Ib/c supernova (SNIb/c) rates with the observed long-duration Gamma-Ray-Burst (GRB) rates both locally and as a function of redshift, by assuming different star formation histories in galaxies of different morphological types. Due to the high star formation in spheroids at high redshift, we predict a large number of GRBs beyond z > 7. Moreover, based on our studies and on the current LAT performance, an estimate of the detection possibility of this burst population is presented.

  3. Hubble constant from lensing in plasma-redshift cosmology, and intrinsic redshift of quasars

    E-Print Network [OSTI]

    Ari Brynjolfsson

    2004-12-02T23:59:59.000Z

    In a series of articles, we have shown that the newly discovered plasma-redshift cosmology gives a simpler, more accurate and consistent explanation of many cosmological phenomena than the big-bang cosmology. The SNe Ia observations are in better agreement with the magnitude-redshift relation predicted by the plasma redshift than that predicted by the multi-parameter big-bang cosmology. No deceleration or expansion parameters are needed. The plasma-redshift cosmology is flat and quasi-static on a large scale. The Hubble constant is no longer an expansion parameter, but is instead a measure of the average electron density along the line of sight towards an object. Perusal of the SNe Ia data and quasar data has shown that there is no time dilation. The conventional estimates of the Hubble constant from gravitational lensing observations use the big-bang cosmology for interpreting the observations. This has lead to a large spread and discordant estimates of the Hubble constant. The purpose of the present article is to show that the gravitational lensing observations are in agreement with the plasma-redshift cosmology, and to show how to evaluate the lensing observations based on the new plasma-redshift cosmology. The lensing observations also indicate that the quasars have large intrinsic redshifts.

  4. Incorporation of PCI flow measurement/control at AK Steel Corporation

    SciTech Connect (OSTI)

    Dibert, W.A.; Keaton, D. [AK Steel Corp., Ashland, KY (United States)

    1994-12-31T23:59:59.000Z

    A measurement and control system has been developed and implemented to improve the distribution of coal among the tuyere lines on AK Steel Corporation`s Amanda blast furnace at Ashland, Kentucky. This paper discusses the development and design of the system, and briefly reviews operating results achieved.

  5. High redshift Gamma-Ray Bursts

    E-Print Network [OSTI]

    Salvaterra, R

    2015-01-01T23:59:59.000Z

    Ten years of operations of the Swift satellite have allow us to collect a small sample of long Gamma-Ray Bursts (GRBs) at redshift larger than six. I will review here the present status of this research field and discuss the possible use of GRBs as a fundamental new tool to explore the early Universe, complementary to quasar and galaxy surveys.

  6. Plasma Redshift, Time Dilation, and Supernovas Ia

    E-Print Network [OSTI]

    Ari Brynjolfsson

    2004-07-20T23:59:59.000Z

    The measurements of the absolute magnitudes and redshifts of supernovas Ia show that conventional physics, which includes plasma redshift, fully explains the observed magnitude-redshift relation of the supernovas. The only parameter that is required is the Hubble constant, which in principle can be measured independently. The contemporary theory of the expansion of the universe (Big Bang) requires in addition to the Hubble constant several adjustable parameters, such as an initial explosion, the dark matter parameter, and a time adjustable dark energy parameter for explaining the supernova Ia data. The contemporary Big Bang theory also requires time dilation of distant events as an inherent premise. The contention is usually that the light curves of distant supernovas show or even prove the time dilation. In the present article, we challenge this assertion. We document and show that the previously reported data in fact indicate that there is no time dilation. The data reported by Riess et al. in the Astrophysical Journal in June 2004 confirm the plasma redshift, the absence of time dilation, dark matter, and dark energy.

  7. Corporate Jobs Tax Credit (Louisiana)

    Broader source: Energy.gov [DOE]

    Corporate Jobs Tax Credit is a one-time tax credit ranging from up to $225 for each net new permanent job created as the result of a new business start-up or the expansion of an existing one. ...

  8. The VIMOS Public Extragalactic Redshift Survey (VIPERS): Reconstruction of the redshift-space galaxy density field

    E-Print Network [OSTI]

    Granett, B R; Guzzo, L; Abbas, U; Adami, C; Arnouts, S; Bel, J; Bolzonella, M; Bottini, D; Cappi, A; Coupon, J; Cucciati, O; Davidzon, I; De Lucia, G; de la Torre, S; Fritz, A; Franzetti, P; Fumana, M; Garilli, B; Ilbert, O; Iovino, A; Krywult, J; Brun, V Le; Fèvre, O Le; Maccagni, D; Ma?ek, K; Marulli, F; McCracken, H J; Polletta, M; Pollo, A; Scodeggio, M; Tasca, L A M; Tojeiro, R; Vergani, D; Zanichelli, A; Burden, A; Di Porto, C; Marchetti, A; Marinoni, C; Mellier, Y; Moutard, T; Moscardini, L; Nichol, R C; Peacock, J A; Percival, W J; Zamorani, G

    2015-01-01T23:59:59.000Z

    Aims. Using the VIMOS Public Extragalactic Redshift Survey (VIPERS) we aim to jointly estimate the key parameters that describe the galaxy density field and its spatial correlations in redshift space. Methods. We use the Bayesian formalism to jointly reconstruct the redshift-space galaxy density field, power spectrum, galaxy bias and galaxy luminosity function given the observations and survey selection function. The high-dimensional posterior distribution is explored using the Wiener filter within a Gibbs sampler. We validate the analysis using simulated catalogues and apply it to VIPERS data taking into consideration the inhomogeneous selection function. Results. We present joint constraints on the anisotropic power spectrum as well as the bias and number density of red and blue galaxy classes in luminosity and redshift bins as well as the measurement covariances of these quantities. We find that the inferred galaxy bias and number density parameters are strongly correlated although these are only weakly co...

  9. Magnitude-Redshift Relation for SNe Ia, Time Dilation, and Plasma Redshift

    E-Print Network [OSTI]

    Ari Brynjolfsson

    2006-02-22T23:59:59.000Z

    We have previously shown that the type Ia supernovae data by Riess et al. match the prediction of the magnitude-redshift relation in the plasma-redshift cosmology. In this article, we also show that the recent SNLS data, which have a slightly narrower distribution as reported by Astier et al. in 2005, match the predictions of the plasma-redshift cosmology. The standard deviation of the SNLS-magnitude from the predicted curve is only about 0.14. The data indicate that there is no cosmic time dilation. The big-bang cosmology therefore appears false. The plasma redshift, which follows from exact evaluation of photons interaction with hot sparse electron plasma, leads to a quasi-static, infinite, and everlasting universe. It does not need big bang, dark energy, or dark matter for describing the observations. It predicts intrinsic redshifts of galaxies consistent with what is observed. The Hubble constant that best fits the SNLS data is about 63 km per sec per Mpc. This corresponds to an average electron density of about 0.0002 per cubic centimeter in intergalactic space. This density together with the plasma redshift heating to an average plasma temperature in intergalactic space of about 3 million K explains the observed isotropic cosmic microwave background (CMB) and the cosmic X-ray background.

  10. REDSHIFT CATALOG FOR SWIFT LONG GAMMA-RAY BURSTS

    SciTech Connect (OSTI)

    Xiao Limin; Schaefer, Bradley E., E-mail: lxiao1@lsu.edu [Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA 70803 (United States)

    2011-04-20T23:59:59.000Z

    We present a catalog of the redshifts for most long-duration gamma-ray bursts (GRBs) by Swift from 2004 December 20 to 2008 July 23 (258 bursts in total). All available information is collected, including spectroscopic redshifts, photometric redshift limits, and redshifts calculated from various luminosity relations. Error bars for the redshifts derived from the luminosity relations are asymmetric, with tails extended to the high-redshift end, and this effect is evaluated by looking at the 30% of Swift bursts with spectroscopic redshifts. A simulation is performed to eliminate this asymmetric effect, and the resultant redshift distribution is deconvolved. We test and confirm this simulation on the sample of bursts with known spectroscopic redshifts and then apply it to the 70% of Swift bursts that do not have spectroscopic measures. A final intrinsic redshift distribution is then made for almost all Swift bursts, and the efficiency of the spectroscopic detections is evaluated. The efficiency of spectroscopic redshifts varies from near unity at low redshift to 0.5 at z = 1, to near 0.3 at z = 4, and to 0.1 at z = 6. We also find that the fraction of GRBs with z>5 is {approx}10%, and this fraction is compared with simulations from a cosmological model.

  11. Karnataka Power Corporation Limited and National Thermal Power...

    Open Energy Info (EERE)

    Limited and National Thermal Power Corporation JV Jump to: navigation, search Name: Karnataka Power Corporation Limited and National Thermal Power Corporation JV Place: India...

  12. Culture, Law, and Finance: Cultural Dimensions of Corporate Governance Laws

    E-Print Network [OSTI]

    Licht, Amir N.; Goldschmidt, Chanan; Schwartz, Shalom H.

    2001-01-01T23:59:59.000Z

    Protection and Corporate Governance, 58 J. Fin. Econ.the legal approach to corporate governance by presenting newlegal rules of corporate governance. 5 The need to take

  13. Corporate Governance, State-Contingent Control Rights, and Financial Distress

    E-Print Network [OSTI]

    Rasmussen, Robert K.

    2004-01-01T23:59:59.000Z

    20-6:00 pm, Boalt 13 Corporate Governance, State-ContingentRobert K. Rasmussen Corporate Governance, State-ContingentTraditional accounts of corporate governance focus on how

  14. U.S. Style Corporate Governance in Korea's Largest Companies

    E-Print Network [OSTI]

    Ehrlich, Craig; Kang, Dae-Seob

    2000-01-01T23:59:59.000Z

    E.g. , D. Gordon Smith, Corporate Governance and ManagerialPrinciples of Corporate Governance, http://www.oecd.orgdaf/Bank/OECD Global Corporate Governance Forum, Washington

  15. Corporate Social Responsibility as a Conflict Between Owners

    E-Print Network [OSTI]

    Rubin, Amir

    2005-01-01T23:59:59.000Z

    Metrick, 2003, Corporate governance and equity prices,to link CSR with corporate governance. Arguably this linkexpenditure and good corporate governance mechanisms are to

  16. How Big a Problem is U.S. Corporate Governance?

    E-Print Network [OSTI]

    Kaplan, Steve

    2007-01-01T23:59:59.000Z

    suggests that poor corporate governance or managerial powertheories argue that corporate governance deteriorated in thestealing CEOs or poor corporate governance cannot possibly

  17. Choice as Regulatory Reform: The Case of Japanese Corporate Governance

    E-Print Network [OSTI]

    Milhaupt, Curtis

    2004-01-01T23:59:59.000Z

    Globalization of Corporate Governance: Convergence of Formthe idea that U.S. corporate governance was a model for AsiaWoochan Kim, Does Corporate Governance Predict Firms’ Market

  18. Nuclear Safety Enforcement Letter issued to Sandia Corporation...

    Broader source: Energy.gov (indexed) [DOE]

    Enforcement Letter issued to Sandia Corporation Nuclear Safety Enforcement Letter issued to Sandia Corporation 9222014 Enforcement Letter, Sandia Corporation, September 22, 2014...

  19. abolishes corporate income: Topics by E-print Network

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

    5, 2014 12;Corporate Affiliates Chairman: Mark Ambrose San Diego Site Executive, Raytheon 12;Corporate Affiliates Program Welcome New CAP Members 12;Corporate Affiliates...

  20. agua corporal total: Topics by E-print Network

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

    5, 2014 12;Corporate Affiliates Chairman: Mark Ambrose San Diego Site Executive, Raytheon 12;Corporate Affiliates Program Welcome New CAP Members 12;Corporate Affiliates...

  1. abolishing corporate income: Topics by E-print Network

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

    5, 2014 12;Corporate Affiliates Chairman: Mark Ambrose San Diego Site Executive, Raytheon 12;Corporate Affiliates Program Welcome New CAP Members 12;Corporate Affiliates...

  2. Steffes Corporation Smart Grid RFI: Addressing Policy and Logistical...

    Energy Savers [EERE]

    Steffes Corporation Smart Grid RFI: Addressing Policy and Logistical Challenges Steffes Corporation Smart Grid RFI: Addressing Policy and Logistical Challenges Steffes Corporation...

  3. Galaxy Bulges at Mid and High-Redshift

    E-Print Network [OSTI]

    Christopher J. Conselice

    2007-09-28T23:59:59.000Z

    Bulges are a major galaxy component in the nearby universe, and are one of the primary features that differentiates and defines galaxies. The origin of bulges can be directly probed in part by examining distant galaxies to search for high redshift bulges, and to study the properties of bulges in formation. We review the evidence for bulges at high redshift in this article, and how by studying bulges through a variety of approaches, including morphological, colour, and stellar mass selection, we can determine when and how these systems assembled. We argue that the majority of the most massive 'classical' bulges are in place by z ~ 1.5 - 2, and likely formed very early through major mergers. Other, likely lower mass, bulges form through a secular process along with their disks. Direct observations suggest that these two formation processes are occurring, as spheroids are commonly seen at z > 1, as are disks and spiral galaxies in the form of luminous diffuse objects, clump-clusters, and chain galaxies. However, bulge+disk systems are relatively rare until z ~ 1, suggesting that this structural assembly occurred relatively late.

  4. --ibm corporate responsibility report--The IBM Corporate Responsibility Report represents the information reported in various categories on IBM's Corporate Responsibility Web site.

    E-Print Network [OSTI]

    Thomas, Harvard Business School The Future of Work: an interview with Thomas Malone, MIT Sloan School Corporate Governance · Leadership · External Audits Management System · Objectives · Business Conduct Guidelines · Policies · Internal Audits · Personal Business Commitments Relationships · Business Partners

  5. Redshifts of the Long Gamma-Ray Bursts

    E-Print Network [OSTI]

    Z. Bagoly; I. Csabai; A. Meszaros; P. Meszaros; I. Horvath; L. G. Balazs; R. Vavrek

    2007-04-06T23:59:59.000Z

    The low energy spectra of some gamma-ray bursts' show excess components beside the power-law dependence. The consequences of such a feature allows to estimate the gamma photometric redshift of the long gamma-ray bursts in the BATSE Catalog. There is good correlation between the measured optical and the estimated gamma photometric redshifts. The estimated redshift values for the long bright gamma-ray bursts are up to z=4, while for the the faint long bursts - which should be up to z=20 - the redshifts cannot be determined unambiguously with this method. The redshift distribution of all the gamma-ray bursts with known optical redshift agrees quite well with the BATSE based gamma photometric redshift distribution.

  6. Chemical Elements at High and Low Redshifts

    E-Print Network [OSTI]

    Max Pettini

    2006-03-02T23:59:59.000Z

    The past few years have seen a steady progress in the determination of element abundances at high redshifts, with new and more accurate measures of metallicities in star-forming galaxies, in QSO absorbers, and in the intergalactic medium. We have also become more aware of the limitations of the tools at our disposal in such endeavours. I summarise these recent developments and--in tune with the theme of this meeting--consider the clues which chemical abundance studies offer to the links between the high redshift galaxy populations and today's galaxies. The new data are `fleshing out' the overall picture of element abundances at redshifts z = 2 - 3 which has been gradually coming into focus over the last decade. In particular, we can now account for at least 40% of the metals produced by the global star formation activity in the universe from the Big Bang to z = 2.5, and we have strong indications of where the remainder are likely to be found.

  7. Development of the SEA Corporation Powergrid{trademark} photovoltaic concentrator

    SciTech Connect (OSTI)

    Kaminar, N.; Curchod, D.; Daroczi, S.; Walpert, M.; Sahagian, J.; Pepper, J. [Photovoltaics International, LLC, Sunnyvale, CA (United States)

    1998-03-01T23:59:59.000Z

    This report covers the three phase effort to bring the SEA Corporation`s Powergrid{trademark} from the concept stage to pilot production. The three phases of this contract covered component development, prototype module development, and pilot line production. The Powergrid is a photovoltaic concentrator that generates direct current electricity directly from sunlight using a linear Fresnel lens. Analysis has shown that the Powergrid has the potential to be very low cost in volume production. Before the start of the project, only proof of concept demonstrations of the components had been completed. During the project, SEA Corporation developed a low cost extruded Fresnel lens, a low cost receiver assembly using one sun type cells, a low cost plastic module housing, a single axis tracking system and frame structure, and pilot production equipment and techniques. In addition, an 800 kW/yr pilot production rate was demonstrated and two 40 kW systems were manufactured and installed.

  8. Measurement of the gravitational redshift effect with RadioAstron satellite

    E-Print Network [OSTI]

    Birukov, A V; Litvinov, D A; Porayko, N K; Rudenko, V N

    2015-01-01T23:59:59.000Z

    RadioAstron satellite admits in principle a testing the gravitational redshift effect with an accuracy of better than $10^{-5}$. It would surpass the result of Gravity Probe A mission at least an order of magnitude. However, RadioAstron's communications and frequency transfer systems are not adapted for a direct application of the non relativistic Doppler and troposphere compensation scheme used in the Gravity Probe A experiment. This leads to degradation of the redshift test accuracy approximately to the level 0.01. We discuss the way to overcome this difficulty and present preliminary results based on data obtained during special observing sessions scheduled for testing the new techniques.

  9. Measurement of the gravitational redshift effect with RadioAstron satellite

    E-Print Network [OSTI]

    A. V. Birukov; V. L. Kauts; D. A. Litvinov; N. K. Porayko; V. N. Rudenko

    2015-06-07T23:59:59.000Z

    RadioAstron satellite admits in principle a testing the gravitational redshift effect with an accuracy of better than $10^{-5}$. It would surpass the result of Gravity Probe A mission at least an order of magnitude. However, RadioAstron's communications and frequency transfer systems are not adapted for a direct application of the non relativistic Doppler and troposphere compensation scheme used in the Gravity Probe A experiment. This leads to degradation of the redshift test accuracy approximately to the level 0.01. We discuss the way to overcome this difficulty and present preliminary results based on data obtained during special observing sessions scheduled for testing the new techniques.

  10. PROPERTIES OF LY-AND GAMMA RAY BURST SELECTED STARBURSTS AT HIGH REDSHIFTS

    E-Print Network [OSTI]

    Fynbo, Johan

    , Palle Møller6, Bjarne Thomsen3 1Niels Bohr Institute, University of Copenhagen, Denmark 2Nordic Optical (Partridge & Peebles 1967). The first detection of redshifted Ly- emis- sion from galaxies not powered counterparts of QSO ab- sorbers such as DLAs and Lyman-limit system

  11. Matching Gift Companies LEHIGH UNIVERSITY 1 3M Corporation

    E-Print Network [OSTI]

    Gilchrist, James F.

    Corporation Foundation The Eaton Charitable Fund Electroline Corporation Eli Lilly and Company FoundationMatching Gift Companies LEHIGH UNIVERSITY 1 3M Corporation Abbott Laboratories Accenture Foundation Technologies, Inc. Air Products Air Products Foundation Albemarle Corporation Alcoa Foundation Alliance Capital

  12. Corporate Headquarters Tax Credit (West Virginia)

    Broader source: Energy.gov [DOE]

    The Corporate Headquarters Tax Credit is available to companies who relocate their corporate headquarters to West Virginia and create 15 new jobs. The credit can offset up to 100% of the tax...

  13. Corporate decision analysis : an engineering approach

    E-Print Network [OSTI]

    Tang, Victor, Ph.D. Massachusetts Institute of Technology

    2006-01-01T23:59:59.000Z

    We explore corporate decisions and their solutions under uncertainty using engineering methods. Corporate decisions tend to be complex; they are interdisciplinary and defy programmable solutions. To address these challenges, ...

  14. Corporate governance : the case for Asian REITs

    E-Print Network [OSTI]

    Tan, Denise, S.M. Massachusetts Institute of Technology

    2009-01-01T23:59:59.000Z

    At the entity level, the design of sound corporate governance mechanisms is critical for REITs that are preparing to go public. At the industry level, issues of transparency and corporate governance are consequential to ...

  15. The Market for Borrowing Corporate Bonds

    E-Print Network [OSTI]

    Asquith, Paul

    This paper describes the market for borrowing corporate bonds using a comprehensive data set from a major lender. The cost of borrowing corporate bonds is comparable to the cost of borrowing stock, between 10 and 20 basis ...

  16. A CRITICAL ASSESSMENT OF PHOTOMETRIC REDSHIFT METHODS: A CANDELS INVESTIGATION

    SciTech Connect (OSTI)

    Dahlen, Tomas; Ferguson, Henry C. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Mobasher, Bahram [Department of Physics and Astronomy, University of California, Riverside, CA 92521 (United States); Faber, Sandra M.; Barro, Guillermo; Guo, Yicheng [UCO/Lick Observatory, Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States); Finkelstein, Steven L. [Department of Astronomy, The University of Texas at Austin, Austin, TX 78712 (United States); Finlator, Kristian [Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen (Denmark); Fontana, Adriano [INAF-Osservatorio Astronomico di Roma, Via Frascati 33, I-00040, Monteporzio (Italy); Gruetzbauch, Ruth [Center for Astronomy and Astrophysics, Observatorio Astronomico de Lisboa, Tapada da Ajuda, 1349-018 Lisboa (Portugal); Johnson, Seth [Department of Astronomy, University of Massachusetts, 710 North Pleasant Street, Amherst, MA 01003 (United States); Pforr, Janine; Dickinson, Mark E. [NOAO, 950 N. Cherry Avenue, Tucson, AZ 85719 (United States); Salvato, Mara; Wuyts, Stijn [Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching bei München (Germany); Wiklind, Tommy [Joint ALMA Observatory, Alonso de Cordova 3107, Vitacura, Santiago (Chile); Acquaviva, Viviana [Physics Department, CUNY NYC College of Technology, 300 Jay Street, Brooklyn, NY 11201 (United States); Huang, Jiasheng [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Huang, Kuang-Han [Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218 (United States); Newman, Jeffrey A., E-mail: dahlen@stsci.edu [Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260 (United States); and others

    2013-10-01T23:59:59.000Z

    We present results from the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS) photometric redshift methods investigation. In this investigation, the results from 11 participants, each using a different combination of photometric redshift code, template spectral energy distributions (SEDs), and priors, are used to examine the properties of photometric redshifts applied to deep fields with broadband multi-wavelength coverage. The photometry used includes U-band through mid-infrared filters and was derived using the TFIT method. Comparing the results, we find that there is no particular code or set of template SEDs that results in significantly better photometric redshifts compared to others. However, we find that codes producing the lowest scatter and outlier fraction utilize a training sample to optimize photometric redshifts by adding zero-point offsets, template adjusting, or adding extra smoothing errors. These results therefore stress the importance of the training procedure. We find a strong dependence of the photometric redshift accuracy on the signal-to-noise ratio of the photometry. On the other hand, we find a weak dependence of the photometric redshift scatter with redshift and galaxy color. We find that most photometric redshift codes quote redshift errors (e.g., 68% confidence intervals) that are too small compared to that expected from the spectroscopic control sample. We find that all codes show a statistically significant bias in the photometric redshifts. However, the bias is in all cases smaller than the scatter; the latter therefore dominates the errors. Finally, we find that combining results from multiple codes significantly decreases the photometric redshift scatter and outlier fraction. We discuss different ways of combining data to produce accurate photometric redshifts and error estimates.

  17. Corporate Real Estate and Facilities Cost Reduction IBM Corporation | December 2, 2009 Page 1 of 7

    E-Print Network [OSTI]

    Corporate Real Estate and Facilities Cost Reduction © IBM Corporation | December 2, 2009 Page 1 of 7 - Internal distribution only Corporate Real Estate and Facilities Cost Reduction Summary By moving and facilities costs by 15-20%, whilst still improving services. Successful cost reduction in corporate real

  18. Mastermind Session: Wisconsin Energy Conservation Corporation...

    Energy Savers [EERE]

    Corporation Better Buildings Neighborhood Program Peer Exchange Call: Program Sustainability Mastermind Session, featuring host Brian Driscoll, Wisconsin Energy Conservation...

  19. Essays on the Market for Corporate Control

    E-Print Network [OSTI]

    Kim, Hyunjung

    2011-02-22T23:59:59.000Z

    corporate governance play its role during this process? And why do managers often resist takeovers? The agency model this paper develops is compatible with existing theories on takeovers including neoclassical, inefficient stock market, and the free cash... .............................................................................................................. 72 IV CORPORATE GOVERNANCE DRIVEN TAKEOVERS ........................................... 82 1. The basic setting ................................................................................................. 82 2. Corporate...

  20. Internship opportunity with URS Corporation

    E-Print Network [OSTI]

    Internship opportunity with URS Corporation URS is the largest global engineering design firm of undergraduate studies to participate in an internship program with the School of Ocean & Earth Science & Technology (SOEST) at the University of Hawaii. The intent of the internship is two-fold: · To establish

  1. Hindawi Publishing Corporation Prostate Cancer

    E-Print Network [OSTI]

    Ahn, Hongshik

    Hindawi Publishing Corporation Prostate Cancer Volume 2011, Article ID 176164, 7 pages doi:10.1155/2011/176164 Clinical Study Effect of Zoledronic Acid on Bone Mineral Density in Men with Prostate Cancer Receiving cancer is well recognized. We assessed the effects of quarterly infusion of zoledronic acid on bone

  2. CORPORATE GOVERNANCE IN THE KINGDOM OF SAUDI ARABIA

    E-Print Network [OSTI]

    Al-Zaid, Ahmad Abdulaziz

    2012-12-31T23:59:59.000Z

    , Companies Act's provisions which describe the function, effect, scope and what they fall short of by themselves and/or within other rules forming the system of corporate governance in Saudi Arabia. In addition, there has been little to no treatment...

  3. Large Scale Periodicity in Redshift Distribution

    E-Print Network [OSTI]

    K. Bajan; M. Biernacka; P. Flin; W. Godlowski; V. Pervushin; A. Zorin

    2004-08-30T23:59:59.000Z

    We review the previous studies of galaxies and quasar redshifts discretisation. We present also the investigations of the large scale periodicity, detected by pencil--beam observations, which revealed 128 (1/h) Mpc period, afterwards confirmed with supercluster studies. We present the theoretical possibility of obtaining such a periodicity using a toy-model. We solved the Kepler problem, i.e. the equation of motion of a particle with null energy moving in the uniform, expanding Universe, decribed by FLRW metrics. It is possible to obtain theoretically the separation between large scale structures similar to the observed one.

  4. HI at a Redshift of Zero

    E-Print Network [OSTI]

    Christopher M. Springob

    2004-11-17T23:59:59.000Z

    While LOFAR and the SKA will enable the study of HI at the epoch of reionization for the first time, expectations for the distribution of HI at that redshift depend on our understanding of the cosmological HI mass density at the present epoch and its variation with environment. We exploit a complete optical diameter and HI flux limited sample of galaxies in the local universe to derive a robust measurement of the HIMF for masses log(M / M_{Sun}) > 7.4 which takes into account the effects of local large scale structure.

  5. ANNz: estimating photometric redshifts using artificial neural networks

    E-Print Network [OSTI]

    Adrian A. Collister; Ofer Lahav

    2004-02-27T23:59:59.000Z

    We introduce ANNz, a freely available software package for photometric redshift estimation using Artificial Neural Networks. ANNz learns the relation between photometry and redshift from an appropriate training set of galaxies for which the redshift is already known. Where a large and representative training set is available ANNz is a highly competitive tool when compared with traditional template-fitting methods. The ANNz package is demonstrated on the Sloan Digital Sky Survey Data Release 1, and for this particular data set the r.m.s. redshift error in the range 0 < z < 0.7 is 0.023. Non-ideal conditions (spectroscopic sets which are small, or which are brighter than the photometric set for which redshifts are required) are simulated and the impact on the photometric redshift accuracy assessed.

  6. Eaton Aftertreatment System (EAS) for On-Highway Diesel Engines

    Broader source: Energy.gov (indexed) [DOE]

    System (EAS) for On- Highway Diesel Engines Highway Diesel Engines Haoran Hu Eaton Corporation August 22, 2006 2004 Eaton Corporation. All rights reserved. Agenda...

  7. Redshift Limits of BL Lacertae Objects from Optical Spectroscopy

    E-Print Network [OSTI]

    J. D. Finke; J. C. Shields; M. Boettcher; S. Basu

    2007-11-13T23:59:59.000Z

    Context: BL Lacertae objects have been the targets for numerous recent multiwavelength campaigns, continuum spectral variability studies, and theoretical spectral and variability modeling. A meaningful interpretation of the results of such studies requires a reliable knowledge of the objects' redshifts; however, the redshifts for many are still unknown or uncertain. Aims: Therefore, we hope to determine or constrain the redshifts of six BL Lac objects with unknown or poorly known redshifts. Methods: Observations were made of these objects with the MDM 2.4 m Hiltner telescope. Although no spectral features were detected, and thus no redshifts could be measured, lower redshift limits were assigned to the objects based on the expected equivalent widths of absorption features in their host galaxies. Redshifts were also estimated for some objects by assuming the host galaxies are standard candles and using host galaxy apparent magnitudes taken from the literature. Results: The commonly used redshift of $z=0.102$ for 1219+285 is almost certainly wrong, while the redshifts of the other objects studied remain undetermined.

  8. Carbon and Water Resource Management for Water Distribution Systems

    E-Print Network [OSTI]

    Hendrickson, Thomas Peter

    2013-01-01T23:59:59.000Z

    Reliability Corporation Polyethylene Polyvinyl chloride Society of Environmental Toxicology and Chemistry Water Distribution System

  9. Absorption features of high redshift galactic winds

    E-Print Network [OSTI]

    A. P. M. Fangano; A. Ferrara; P. Richter

    2007-06-11T23:59:59.000Z

    The environment of high-redshift galaxies is characterized by both wind-driven outflowing gas and gravitationally infalling streams. To investigate such galaxy-IGM interplay we have generated synthetic optical absorption line spectra piercing the volume surrounding a starbursting analog of a Lyman Break Galaxy selected in a $z \\approx 3$ output from a SPH simulation, including a detailed treatment of mechanical feedback from winds. Distributions for several observable species (HI, CIII, CIV, SiII, SiIII, SiIV, OVI, OVII, and OVIII) have been derived by post-processing the simulation outputs. The hot wind material is characterized by the presence of high-ionization species such as OVI, OVII, and OVIII (the latter two observable only in X-ray bands); the colder ($Tgas clumps. However, both line profile and Pixel Optical Depth analysis of the synthetic spectra show that the intergalactic filament in which the wind-blowing galaxy is embedded produces absorption signatures that closely mimic those of the wind environment. We conclude that may be difficult to clearly identify wind-blowing galaxies and their complex gaseous environment at high redshift in optical QSO absorption-line spectra based solely on the observed ion absorption patterns.

  10. Redshift drift exploration for interacting dark energy

    E-Print Network [OSTI]

    Geng, Jia-Jia; Zhang, Jing-Fei; Zhang, Xin

    2015-01-01T23:59:59.000Z

    By detecting redshift drift in the spectra of Lyman-$\\alpha$ forest of distant quasars, Sandage-Loeb (SL) test directly measures the expansion of the universe, covering the "redshift desert" of $2 \\lesssim z \\lesssim5$. Thus this method is definitely an important supplement to the other geometric measurements and will play a crucial role in cosmological constraints. In this paper, we quantify the ability of SL test signal by a CODEX-like spectrograph for constraining interacting dark energy. Four typical interacting dark energy models are considered: (\\romannumeral1) $Q=\\gamma H\\rho_c$, (\\romannumeral2) $Q=\\gamma H\\rho_{de}$, (\\romannumeral3) $Q=\\gamma H_0\\rho_c$, and (\\romannumeral4) $Q=\\gamma H_0\\rho_{de}$. The results show that for all the considered interacting dark energy models, relative to the current joint SN+BAO+CMB+$H_0$ observations, the constraints on $\\Omega_m$ and $H_0$ would be improved by about 60\\% and 30--40\\%, while the constraints on $w$ and $\\gamma$ would be slightly improved, with a 30-y...

  11. JOHNR. SCHOTT Calspan Corporation

    E-Print Network [OSTI]

    Salvaggio, Carl

    . INTRODUCTIONAND SUMMARY cooling water discharged into a water body, the temperature value and spatial extent and the effects on aquatic organisms that are drawn through cooling systems are of particular concern. In order PHOTOGRAMMETRICENGINEERINGAND REMOTESENSI Vol. 45, No. 6, June 1979, pp. 753-761. #12;PHOTOGRAMMETRIC ENGINEERING & REMOTE

  12. Corporate Security and Conflict Outcomes 

    E-Print Network [OSTI]

    Tkach, Benjamin K

    2013-10-21T23:59:59.000Z

    militaries (Avant 2000). Existing research has shown a steady increase in the number and employment of private security firms (PSFs) over the last five decades due to expansion of global market demand for private security (Avant 2005; Dunigan 2011; Singer... prominent role in international aviation security (Abrahamsen and Williams 2011). Because PSFs are based largely on corporate profit motivations, contract fulfillment and reputation are critical for firms to secure market share. The international market...

  13. BASF Corporate Energy Management Process

    E-Print Network [OSTI]

    Geiger, T.

    2014-01-01T23:59:59.000Z

    Process 2 2 ? Brief introduction to BASF ? BASF Corporate Energy Management ? Management Support ? Goals ? Continuous Improvement ? Knowledge Sharing ? Recognition ESL-IE-14-05-30 Proceedings of the Thrity-Sixth Industrial Energy Technology Conference... • 2013 Sales: €74 Billion • Employees: 112,000 Company overview BASF – The Chemical Company 3 ESL-IE-14-05-30 Proceedings of the Thrity-Sixth Industrial Energy Technology Conference New Orleans, LA. May 20-23, 2014 Structure of BASF’s segments...

  14. Singapore's Economic Balancing Act: How a Company's Collapse Challenged the Country's New Corporate Governance Regime

    E-Print Network [OSTI]

    Roseme, Sam

    2007-01-01T23:59:59.000Z

    THE COUNTRY'S NEW CORPORATE GOVERNANCE REGIME Sam RosemeON SINGAPORE'S CORPORATE GOVERNANCE REGIME . A.CORPORATE GOVERNANCE .. B. CHINA'S

  15. Multi-object spectroscopy of low-redshift EIS clusters IV. Reliability of matched-filter results at z~0.3-0.4

    E-Print Network [OSTI]

    L. F. Grove; L. da Costa; C. Benoist

    2008-09-26T23:59:59.000Z

    abridged) In this paper we present new redshifts for 747 galaxies in 23 ESO Imaging Survey (EIS) cluster fields. We use the "gap"-technique to search for significant overdensities in redshift space for identifying groups/clusters of galaxies. In this way we spectroscopically confirm systems in 10 of the 23 cluster candidate fields with a matched-filter estimated redshift z_MF=0.3-0.4 and with spectroscopic redshifts in the range from z=0.158 to z=0.534. We find that the systems identified in the present paper span a broad range of one-dimensional velocity dispersion (175-497 km/s) and richness (12L*EIS cluster candidates with estimated redshifts z<=0.4. We have measured a total of 1954 galaxy redshifts in the range z=0.0065 to z=0.6706. Of the 58 systems we confirm 42 (~75%) with redshifts between z=0.095 and z=0.534.

  16. Extending the redshift-distance relation in Cosmological General Relativity to higher redshifts

    E-Print Network [OSTI]

    John G. Hartnett

    2007-11-22T23:59:59.000Z

    The redshift-distance modulus relation, the Hubble Diagram, derived from Cosmological General Relativity has been extended to arbitrarily large redshifts. Numerical methods were employed and a density function was found that results in a valid solution of the field equations at all redshifts. The extension has been compared to 302 type Ia supernova data as well as to 69 Gamma-ray burst data. The latter however do not not truly represent a `standard candle' as the derived distance modulii are not independent of the cosmology used. Nevertheless the analysis shows a good fit can be achieved without the need to assume the existence of dark matter. The Carmelian theory is also shown to describe a universe that is always spatially flat. This results from the underlying assumption of the energy density of a cosmological constant $\\Omega_{\\Lambda} = 1$, the result of vacuum energy. The curvature of the universe is described by a \\textit{spacevelocity} metric where the energy content of the curvature at any epoch is $\\Omega_K = \\Omega_{\\Lambda} - \\Omega = 1-\\Omega$, where $\\Omega$ is the matter density of the universe. Hence the total density is always $\\Omega_K + \\Omega = 1$

  17. Of Enterprise Principles & Corporate Groups: Does Corporate Law Reach Human Rights?

    E-Print Network [OSTI]

    Harper Ho, Virginia E.

    2013-03-01T23:59:59.000Z

    conduct by remote affiliates and business partners of vast multinational corporate organizations. Corporate law, in contrast, governs the "internal affairs" of discrete legal entities within a given jurisdiction, each protected by a limited liability...

  18. North American Electric Reliability Corporation (NERC): Reliability...

    Office of Environmental Management (EM)

    (NERC): Reliability Considerations from the Integration of Smart Grid North American Electric Reliability Corporation (NERC): Reliability Considerations from the Integration of...

  19. Panasonic Corporation Energy Company formerly Matsushita Battery...

    Open Energy Info (EERE)

    to: navigation, search Name: Panasonic Corporation Energy Company (formerly Matsushita Battery Industrial Co) Place: Moriguchi, Osaka, Japan Zip: 570-8511 Product: Producer of...

  20. Duro Corporation: Proposed Penalty (2014-CE-23009)

    Broader source: Energy.gov [DOE]

    DOE alleged in a Notice of Proposed Civil Penalty that Duro Corporation failed to certify cooking products as compliant with the applicable energy conservation standards.

  1. Resources, real options, and corporate strategy

    E-Print Network [OSTI]

    Bernardo, Antonio; Chowdhry, Bhagwan

    1998-01-01T23:59:59.000Z

    211–234 Resources, real options, and corporate strategy $D83; G30; G31 Keywords: Real options; Valuation; Corporateparticipants at the Real Options Conference at Northwestern

  2. PRELIMINARY SURVEY OF WESTINGHOUSE ELECTRIC CORPORATION EAST...

    Office of Legacy Management (LM)

    OAK RIDGE NATIONAL LABORATORY operated by UNION CARBIDE CORPORATION for the DEPARTMENT OF ENERGY as part of the Formerly Utilized Sites-- Remedial Action Program WESTINGHOUSE...

  3. Gibson Electric Membership Corporation- Energy Efficiency Rebates

    Broader source: Energy.gov [DOE]

    Gibson Electric Membership Corporation, in collaboration with the Tennessee Valley Authority, promotes energy efficient building design through its [http://www.energyright.com/ ''energy right'']...

  4. ALMA REDSHIFTS OF MILLIMETER-SELECTED GALAXIES FROM THE SPT SURVEY: THE REDSHIFT DISTRIBUTION OF DUSTY STAR-FORMING GALAXIES

    SciTech Connect (OSTI)

    Weiss, A. [Max-Planck-Institut fuer Radioastronomie, Auf dem Huegel 69, D-53121 Bonn (Germany)] [Max-Planck-Institut fuer Radioastronomie, Auf dem Huegel 69, D-53121 Bonn (Germany); De Breuck, C.; Aravena, M.; Biggs, A. D. [European Southern Observatory, Karl-Schwarzschild Strasse, D-85748 Garching bei Muenchen (Germany)] [European Southern Observatory, Karl-Schwarzschild Strasse, D-85748 Garching bei Muenchen (Germany); Marrone, D. P.; Bothwell, M. [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States)] [Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721 (United States); Vieira, J. D.; Bock, J. J. [California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125 (United States)] [California Institute of Technology, 1200 E. California Blvd., Pasadena, CA 91125 (United States); Aguirre, J. E. [University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States)] [University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Aird, K. A. [University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States)] [University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States); Ashby, M. L. N.; Bayliss, M. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)] [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Benson, B. A.; Bleem, L. E.; Carlstrom, J. E.; Chang, C. L. [Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States)] [Kavli Institute for Cosmological Physics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States); Bethermin, M. [Laboratoire AIM-Paris-Saclay, CEA/DSM/Irfu - CNRS - Universite Paris Diderot, CEA-Saclay, Orme des Merisiers, F-91191 Gif-sur-Yvette (France)] [Laboratoire AIM-Paris-Saclay, CEA/DSM/Irfu - CNRS - Universite Paris Diderot, CEA-Saclay, Orme des Merisiers, F-91191 Gif-sur-Yvette (France); Bradford, C. M. [Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States)] [Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109 (United States); Brodwin, M. [Department of Physics and Astronomy, University of Missouri, 5110 Rockhill Road, Kansas City, MO 64110 (United States)] [Department of Physics and Astronomy, University of Missouri, 5110 Rockhill Road, Kansas City, MO 64110 (United States); Chapman, S. C. [Department of Physics and Atmospheric Science, Dalhousie University, Halifax, NS B3H 3J5 Canada (Canada)] [Department of Physics and Atmospheric Science, Dalhousie University, Halifax, NS B3H 3J5 Canada (Canada); and others

    2013-04-10T23:59:59.000Z

    Using the Atacama Large Millimeter/submillimeter Array, we have conducted a blind redshift survey in the 3 mm atmospheric transmission window for 26 strongly lensed dusty star-forming galaxies (DSFGs) selected with the South Pole Telescope. The sources were selected to have S{sub 1.4{sub mm}} > 20 mJy and a dust-like spectrum and, to remove low-z sources, not have bright radio (S{sub 843{sub MHz}} < 6 mJy) or far-infrared counterparts (S{sub 100{sub {mu}m}} < 1 Jy, S{sub 60{sub {mu}m}} < 200 mJy). We robustly detect 44 line features in our survey, which we identify as redshifted emission lines of {sup 12}CO, {sup 13}CO, C I, H{sub 2}O, and H{sub 2}O{sup +}. We find one or more spectral features in 23 sources yielding a {approx}90% detection rate for this survey; in 12 of these sources we detect multiple lines, while in 11 sources we detect only a single line. For the sources with only one detected line, we break the redshift degeneracy with additional spectroscopic observations if available, or infer the most likely line identification based on photometric data. This yields secure redshifts for {approx}70% of the sample. The three sources with no lines detected are tentatively placed in the redshift desert between 1.7 < z < 2.0. The resulting mean redshift of our sample is z-bar = 3.5. This finding is in contrast to the redshift distribution of radio-identified DSFGs, which have a significantly lower mean redshift of z-bar = 2.3 and for which only 10%-15% of the population is expected to be at z > 3. We discuss the effect of gravitational lensing on the redshift distribution and compare our measured redshift distribution to that of models in the literature.

  5. OPTICAL CROSS-CORRELATION FILTERS: AN ECONOMICAL APPROACH FOR IDENTIFYING SNe Ia AND ESTIMATING THEIR REDSHIFTS

    SciTech Connect (OSTI)

    Scolnic, Daniel M.; Riess, Adam G.; Huber, Mark E. [Department of Physics and Astronomy, Johns Hopkins University, MD 21218 (United States); Rest, Armin; Stubbs, Christoper W. [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Tonry, John L. [Institute for Astronomy, University of Hawaii, Honolulu, HI 96822 (United States)

    2009-11-20T23:59:59.000Z

    Large photometric surveys of transient phenomena, such as Panoramic Survey Telescope and Rapid Response System and Large Synoptic Survey Telescope, will locate thousands to millions of Type Ia supernova (SN Ia) candidates per year, a rate prohibitive for acquiring spectroscopy to determine each candidate's type and redshift. In response, we have developed an economical approach to identifying SNe Ia and their redshifts using an uncommon type of optical filter which has multiple, discontinuous passbands on a single substrate. Observation of a supernova through a specially designed pair of these 'cross-correlation filters' measures the approximate amplitude and phase of the cross-correlation between the spectrum and a SN Ia template, a quantity typically used to determine the redshift and type of a high-redshift SN Ia. Simulating the use of these filters, we obtain a sample of SNe Ia which is approx98% pure with individual redshifts measured to sigma{sub z} = 0.01 precision. The advantages of this approach over standard broadband photometric methods are that it is insensitive to reddening, independent of the color data used for subsequent distance determinations which reduce selection or interpretation bias, and because it makes use of the spectral features its reliability is greater. A great advantage over long-slit spectroscopy comes from increased throughput, enhanced multiplexing, and reduced setup time resulting in a net gain in speed of up to approx30 times. This approach is also insensitive to host galaxy contamination. Prototype filters were built and successfully used on Magellan with LDSS-3 to characterize three SuperNova Legacy Survey candidates. We discuss how these filters can provide critical information for the upcoming photometric supernova surveys.

  6. Corporate Plan Page 1Forestry Commission England Corporate Plan 2011-15

    E-Print Network [OSTI]

    Corporate Plan 2011-15 Page 1Forestry Commission England Corporate Plan 2011-15 Welcome This is the Corporate Plan for the Forestry Commission in England. It is one of a suite of plans including those for Forestry Commission (GB) and Forest Research. This document has been optimised for on-screen reading

  7. Information GRID in the Corporate World Information GRID in the Corporate World

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    Information GRID in the Corporate World Information GRID in the Corporate World .Bogonikolos Zeus Ontology Grid) project, an EU project funded under the Information Society Technologies programme and EAI Tools is discussed. The COG (Corporate Ontology Grid) project addresses the problem of accessing

  8. Carbona Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:EzfeedflagBiomassSustainableCSL GasPermitsGreen BioEnergy LLC JumpCarbona Corporation Jump to:

  9. JYT Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual Siteof Energy 2,AUDIT REPORTEnergyFarmsPower Co LtdTN LLC Jump to:PtyJYT Corporation Jump

  10. Kirmart Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual Siteof Energy 2,AUDIT REPORTEnergyFarmsPower Co LtdTN LLCKirmart Corporation Jump to:

  11. Vairex Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:Ezfeedflag JumpID-fTri Global EnergyUtility Rate Home >Vairex Corporation Jump to:

  12. AES Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:Ezfeedflag JumpID-fTriWildcat 1 WindtheEnergySulfonate asAEE Solar Jump to:AES Corporation

  13. Powerex Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual SiteofEvaluatingGroupPerfectenergyInformation toPower and ElectricityPowerex Corporation

  14. ISE Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to: navigation, search OpenEIHesperia,IDGWP Wind Farm Jump to:ILab IncubatorISE Corporation Jump

  15. Pemery Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere I Geothermal Pwer PlantMunhall,Missouri:EnergyOssian,Parle BiscuitsPemery Corporation Jump to: navigation,

  16. Emcore Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand JumpConceptual Model,DOEHazel Crest,Energy Information ElkhornElwood,Emcore Corporation Jump to:

  17. Epco Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand JumpConceptual Model,DOEHazel Crest,EnergySerranopolisEnviroMission LtdEnvisolar JumpEpco Corporation

  18. Corporate Depreciation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand JumpConceptual Model, clickInformationNew|Core Analysis At Geysers|Cornwall,Corporate Depreciation

  19. Corporate Exemption | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand JumpConceptual Model, clickInformationNew|Core Analysis At Geysers|Cornwall,Corporate

  20. Sinosteel Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnualProperty Edit with form HistoryRistmaSinosteel Corporation Jump to: navigation, search Name:

  1. corporate | netl.doe.gov

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level:Energy: Grid Integration Redefining What'sis Taking Over OurThe Iron4 Self-Scrubbing:,, , ., ..., ,+ . :,2013constantconvertCorporate

  2. Ryokuseisha Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere IRaghuraji Agro Industries Pvt Ltd Jump to:Roscommon County,Vermont:Kentucky:Wisconsin:Ryokuseisha Corporation

  3. EXAR Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnualPropertyd8c-a9ae-f8521cbb8489 No revision| Open Jump to:(RES-AEI) | OpenEUHYFISEXAR Corporation

  4. Radio source orientation and the angular diameter-redshift relation

    SciTech Connect (OSTI)

    Onuora, L.I. (University of Nigeria, Nsukka (Nigeria))

    1991-08-01T23:59:59.000Z

    The effect of a nonrandom source orientation on the angular diameter-redshift relation was considered for the 3CR sample of Laing et al., based on the 'unified' scheme of Barthel. For an inhomogeneous sample of objects displaying milliarcsecond scale structure, it was found that there was no evidence for a systematic variation for orientation angle with redshift. However, if it was assumed that quasars are closer to the line of sight than powerful extended radio galaxies, then the observed angular size-redshift relation could be interpreted in terms of source orientation, rather than linear size evolution. 14 refs.

  5. Discrete Intrinsic Redshifts from Quasars to Normal Galaxies

    E-Print Network [OSTI]

    M. B. Bell

    2002-11-05T23:59:59.000Z

    It is pointed out that the discrete velocities found by Tifft in galaxies are harmonically related to the discrete intrinsic redshifts found in quasars. All are harmonically related to the constant 0.062 +/- 0.001, and this is the fourth independent analysis in which the redshift increment 0.062 has been shown to be significant. It is concluded that there is a quantized component in the redshift of both quasars and galaxies that has a common origin and is unlikely to be Doppler-related.

  6. Fact #870: April 27, 2015 Corporate Average Fuel Economy Progress...

    Office of Environmental Management (EM)

    Fact 870: April 27, 2015 Corporate Average Fuel Economy Progress, 1978-2014 Fact 870: April 27, 2015 Corporate Average Fuel Economy Progress, 1978-2014 The Corporate Average Fuel...

  7. Law, Politics and Markets of Corporate Governance: Institutional Investors' Influence

    E-Print Network [OSTI]

    Carniglia, Stephen Davis

    2013-01-01T23:59:59.000Z

    S. , “The State of Corporate Governance Research,” 23 R.What Matters in Corporate Governance? ,” 22 R. Fin. StudiesLegitimacy and Corporate Governance,” 32 Del. J. Corp. L.

  8. Measuring Efficiency in Corporate Law: The Role of Shareholder Primacy

    E-Print Network [OSTI]

    Fisch, Jill

    2004-01-01T23:59:59.000Z

    17 Empirical studies of corporate governance reforms such asDirectors as a Corporate Governance Mechanism: Theories andMeans and Ends of Corporate Governance, 97 N W .U. L. R EV .

  9. Preliminary Notice of Violation, Safety and Ecology Corporation...

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

    Safety and Ecology Corporation - EA-2005-03 Preliminary Notice of Violation, Safety and Ecology Corporation - EA-2005-03 June 14, 2005 Issued to Safety and Ecology Corporation...

  10. Constraining inflation with future galaxy redshift surveys

    SciTech Connect (OSTI)

    Huang, Zhiqi; Vernizzi, Filippo [CEA, Institut de Physique Théorique, 91191 Gif-sur-Yvette cédex (France); Verde, Licia, E-mail: zhiqi.huang@cea.fr, E-mail: liciaverde@icc.ub.edu, E-mail: filippo.vernizzi@cea.fr [Institute of Sciences of the Cosmos (ICCUB), University of Barcelona, Marti i Franques 1, Barcelona 08024 (Spain)

    2012-04-01T23:59:59.000Z

    With future galaxy surveys, a huge number of Fourier modes of the distribution of the large scale structures in the Universe will become available. These modes are complementary to those of the CMB and can be used to set constraints on models of the early universe, such as inflation. Using a MCMC analysis, we compare the power of the CMB with that of the combination of CMB and galaxy survey data, to constrain the power spectrum of primordial fluctuations generated during inflation. We base our analysis on the Planck satellite and a spectroscopic redshift survey with configuration parameters close to those of the Euclid mission as examples. We first consider models of slow-roll inflation, and show that the inclusion of large scale structure data improves the constraints by nearly halving the error bars on the scalar spectral index and its running. If we attempt to reconstruct the inflationary single-field potential, a similar conclusion can be reached on the parameters characterizing the potential. We then study models with features in the power spectrum. In particular, we consider ringing features produced by a break in the potential and oscillations such as in axion monodromy. Adding large scale structures improves the constraints on features by more than a factor of two. In axion monodromy we show that there are oscillations with small amplitude and frequency in momentum space that are undetected by CMB alone but can be measured by including galaxy surveys in the analysis.

  11. The Environment of Galaxies at Low Redshift

    E-Print Network [OSTI]

    Nicolas B. Cowan; Zeljko Ivezic

    2008-01-15T23:59:59.000Z

    We compare environmental effects in two analogous samples of galaxies, one from the Sloan Digital Sky Survey (SDSS) and the other from a semi-analytic model (SAM) based on the Millennium Simulation (MS), to test to what extent current SAMs of galaxy formation are reproducing environmental effects. We estimate the large-scale environment of each galaxy using a Bayesian density estimator based on distances to all ten nearest neighbors and compare broad-band photometric properties of the two samples as a function of environment. The feedbacks implemented in the semi-analytic model produce a qualitatively correct galaxy population with similar environmental dependence as that seen in SDSS galaxies. In detail, however, the colors of MS galaxies exhibit an exaggerated dependence on environment: the field contains too many blue galaxies while clusters contain too many red galaxies, compared to the SDSS sample. We also find that the MS contains a population of highly clustered, relatively faint red galaxies with velocity dispersions comparable to their Hubble flow. Such high-density galaxies, if they exist, would be overlooked in any low-redshift survey since their membership to a cluster cannot be determined due to the "Fingers of God" effect.

  12. Multi-object spectroscopy of low-redshift EIS clusters IV. Reliability of matched-filter results at z~0.3-0.4

    E-Print Network [OSTI]

    Grove, L F; Benoist, C

    2008-01-01T23:59:59.000Z

    abridged) In this paper we present new redshifts for 747 galaxies in 23 ESO Imaging Survey (EIS) cluster fields. We use the "gap"-technique to search for significant overdensities in redshift space for identifying groups/clusters of galaxies. In this way we spectroscopically confirm systems in 10 of the 23 cluster candidate fields with a matched-filter estimated redshift z_MF=0.3-0.4 and with spectroscopic redshifts in the range from z=0.158 to z=0.534. We find that the systems identified in the present paper span a broad range of one-dimensional velocity dispersion (175-497 km/s) and richness (12L*EIS clust...

  13. The Carnegie Supernova Project: The Low-Redshift Survey

    E-Print Network [OSTI]

    Mario Hamuy; Gastón Folatelli; Nidia I. Morrell; Mark M. Phillips; Nicholas B. Suntzeff; S. E. Persson; Miguel Roth; Sergio Gonzalez; Wojtek Krzeminski; Carlos Contreras; Wendy L. Freedman; D. C. Murphy; Barry F. Madore; P. Wyatt; José Maza; Alexei V. Filippenko; Weidong Li; P. A. Pinto

    2005-12-01T23:59:59.000Z

    Supernovae are essential to understanding the chemical evolution of the Universe. Type Ia supernovae also provide the most powerful observational tool currently available for studying the expansion history of the Universe and the nature of dark energy. Our basic knowledge of supernovae comes from the study of their photometric and spectroscopic properties. However, the presently available data sets of optical and near-infrared light curves of supernovae are rather small and/or heterogeneous, and employ photometric systems that are poorly characterized. Similarly, there are relatively few supernovae whose spectral evolution has been well sampled, both in wavelength and phase, with precise spectrophotometric observations. The low-redshift portion of the Carnegie Supernova Project (CSP) seeks to remedy this situation by providing photometry and spectrophotometry of a large sample of supernovae taken on telescope/filter/detector systems that are well understood and well characterized. During a five-year program which began in September 2004, we expect to obtain high-precision u'g'r'i'BVYJHKs light curves and optical spectrophotometry for about 250 supernovae of all types. In this paper we provide a detailed description of the CSP survey observing and data reduction methodology. In addition, we present preliminary photometry and spectra obtained for a few representative supernovae during the first observing campaign.

  14. Corporate Training On-Site Online Global

    E-Print Network [OSTI]

    Barrett, Jeffrey A.

    MAKE THE RIGHT MOVE Corporate Training On-Site · Online · Global IMPROVE YOUR COMPETITIVE ADVANTAGE WITH WORLD-CLASS ON-SITE AND ONLINE SOLUTIONS TAILORED TO MEET YOUR BUSINESS AND EMPLOYEE TRAINING NEEDS a competitive advantage depends on how well your staff executes. UCIrvineExtension's Corporate Training helps

  15. QUESTIONING THE RELEVANCE OF CORPORATE SOCIAL PERFORMANCE

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    on the limits of the concept of Corporate Social Performance (CSP) and its instrumentation in the form on Corporate Social Performance (CSP) and its instrumentation in the form of models for measuring form, the BSC reduces its search for balance to three essential Stakeholders: employees, customers

  16. Is Sustainability Attractive for Corporate Real Estate

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    Is Sustainability Attractive for Corporate Real Estate Decisions ? Research Center ESSEC Working Is Sustainability Attractive for Corporate Real Estate Decisions? Ingrid Nappi-Choulet Professor ESSEC BUSINESS SCHOOL Real Estate and Sustainable Development Chair nappi@essec.fr Aurélien Décamps Researcher ESSEC

  17. Corporate Political Donations: Investment or Agency?

    E-Print Network [OSTI]

    Aggarwal, Rajesh K.; Meschke, Felix; Wang, Tracy Yue

    2012-04-01T23:59:59.000Z

    are negatively correlated with returns. A $10,000 increase in donations is associated with a reduction in annual excess returns of 7.4 basis points. Worse corporate governance is associated with larger donations. Even after controlling for corporate governance...

  18. Corporate Venture Capital (CVC) Seeking Innovation and

    E-Print Network [OSTI]

    , Technology Innovation Program, National Institute of Standards and Technology #12;Corporate Venture Capital, Deputy Director Technology Innovation Program Marc G. Stanley, Director #12;ii Acknowledgments T his policymakers in the role of corporate venture capital (CVC) in technology innovation. The research included

  19. Sandia National Laboratories: ECIS-Automotive Fuel Cell Corporation...

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

    ClimateECAbout ECFacilitiesCRFECIS-Automotive Fuel Cell Corporation: Hydrocarbon Membrane Fuels the Success of Future Generation Vehicles ECIS-Automotive Fuel Cell Corporation:...

  20. Comments of New England Electric Transmission Corporation on...

    Broader source: Energy.gov (indexed) [DOE]

    out of time and comments of New England Electric Transmission Corporation, New England Hydro-Transmission Electric Company, Inc. and New England Hydro-Transmission Corporation and...

  1. EA-1727: AE Polysilicon Corporation Polysilicon Production Facility...

    Office of Environmental Management (EM)

    7: AE Polysilicon Corporation Polysilicon Production Facility in Fairless Hills, PA EA-1727: AE Polysilicon Corporation Polysilicon Production Facility in Fairless Hills, PA...

  2. New York State Electric & Gas Corporation Smart Grid Demonstration...

    Open Energy Info (EERE)

    Electric & Gas Corporation Smart Grid Demonstration Project Jump to: navigation, search Project Lead New York State Electric & Gas Corporation Country United States Headquarters...

  3. Trony Solar Corporation formerly Shenzhen Trony Science Technology...

    Open Energy Info (EERE)

    Trony Solar Corporation formerly Shenzhen Trony Science Technology Development Co Ltd Jump to: navigation, search Name: Trony Solar Corporation (formerly Shenzhen Trony Science &...

  4. EA-1631: Beacon Power Corporation Frequency Regulation Facility...

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

    1: Beacon Power Corporation Frequency Regulation Facility in Stephentown, NY EA-1631: Beacon Power Corporation Frequency Regulation Facility in Stephentown, NY February 2, 2009...

  5. Shenyang Huachuang Wind Energy Corporation HCWE aka China Creative...

    Open Energy Info (EERE)

    Shenyang Huachuang Wind Energy Corporation HCWE aka China Creative Wind Energy Co Ltd Jump to: navigation, search Name: Shenyang Huachuang Wind Energy Corporation (HCWE) (aka China...

  6. Testimonials - Partnerships in R&D - Capstone Turbine Corporation...

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

    R&D - Capstone Turbine Corporation Testimonials - Partnerships in R&D - Capstone Turbine Corporation Addthis Text Version The words Office of Energy Efficiency and Renewable Energy...

  7. Integration of the EM Corporate QA Performance Metrics With Performanc...

    Office of Environmental Management (EM)

    Integration of the EM Corporate QA Performance Metrics With Performance Analysis Process Integration of the EM Corporate QA Performance Metrics With Performance Analysis Process...

  8. Structure and kinematics of galaxy clusters I. The redshift catalogue

    E-Print Network [OSTI]

    P. Stein

    1996-01-12T23:59:59.000Z

    An extensive redshift survey has been conducted on a sample of 15 nearby (0.01 < z < 0.05) clusters of galaxies. A total number of 860 redshifts were determined by fitting of emission--lines and/or cross-correlation techniques. Of this sample, 735 galaxies are within 0.2--0.8 Mpc ($H_0$ = 50 km/s/Mpc) of the center of clusters. Approximate morphological types are available for most of the galaxies. A comparison of the present redshifts with published data allows an extensive error analysis. The agreement is excellent with the most modern data, showing a zero point error of 5 km/s and an overall consistency of the measurements and their uncertainties. We estimate our redshifts to have mean random errors around 30 km/s. A population analysis of the clusters will be given in a forthcoming paper.

  9. Photometric Redshift with Bayesian Priors on Physical Properties of Galaxies

    E-Print Network [OSTI]

    Tanaka, Masayuki

    2015-01-01T23:59:59.000Z

    We present a proof-of-concept analysis of photometric redshifts with Bayesian priors on physical properties of galaxies. This concept is particularly suited for upcoming/on-going large imaging surveys, in which only several broad-band filters are available and it is hard to break some of the degeneracies in the multi-color space. We construct model templates of galaxies using a stellar population synthesis code and apply Bayesian priors on physical properties such as stellar mass and star formation rate. These priors are a function of redshift and they effectively evolve the templates with time in an observationally motivated way. We demonstrate that the priors help reduce the degeneracy and deliver significantly improved photometric redshifts. Furthermore, we show that a template error function, which corrects for systematic flux errors in the model templates as a function of rest-frame wavelength, delivers further improvements. One great advantage of our technique is that we simultaneously measure redshifts...

  10. Temperature measurement in the Intel Efraim Rotem Mobile Platform Group, Intel corporation

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    , Intel corporation Jim Hermerding ­ Mobile platform Group, Intel corporation Cohen Aviad - Microprocessor

  11. Performance Assessment and Recommendations for Rejuvenation of a Permeable Reactive Barrier: Cotter Corporation’s Cañon City, Colorado, Uranium Mill

    Broader source: Energy.gov [DOE]

    Performance Assessment and Recommendations for Rejuvenation of a Permeable Reactive Barrier: Cotter Corporation’s Canon City, Colorado, Uranium Mill (April 2005)

  12. High redshift AGNs and HI reionisation: limits from the unresolved X-ray background

    E-Print Network [OSTI]

    Haardt, Francesco

    2015-01-01T23:59:59.000Z

    The rapidly declining population of bright quasars at z~3 appears to make an increasingly small contribution to the ionising background at the HI Lyman limit. It is then generally though that massive stars in (pre-)galactic systems may provide the additional ionising flux needed to complete HI reionisation by z>6. A galaxy dominated background, however, may require that the escape fraction of Lyman continuum radiation from high redshift galaxies is as high as 10%, a value somewhat at odds with (admittedly scarce) observational constraints. High escape fractions from dwarf galaxies have been advocated, or, alternatively, a so-far undetected (or barely detected) population of unobscured, high-redshift faint AGNs. Here we question the latter hypothesis, and show that such sources, to be consistent with the measured level of the unresolved X-ray background at z=0, can provide a fraction of the HII filling factor not larger than 13% by z=6. The fraction rises to 10%.

  13. The Hubble series: Convergence properties and redshift variables

    E-Print Network [OSTI]

    Celine Cattoen; Matt Visser

    2007-10-10T23:59:59.000Z

    In cosmography, cosmokinetics, and cosmology it is quite common to encounter physical quantities expanded as a Taylor series in the cosmological redshift z. Perhaps the most well-known exemplar of this phenomenon is the Hubble relation between distance and redshift. However, we now have considerable high-z data available, for instance we have supernova data at least back to redshift z=1.75. This opens up the theoretical question as to whether or not the Hubble series (or more generally any series expansion based on the z-redshift) actually converges for large redshift? Based on a combination of mathematical and physical reasoning, we argue that the radius of convergence of any series expansion in z is less than or equal to 1, and that z-based expansions must break down for z>1, corresponding to a universe less than half its current size. Furthermore, we shall argue on theoretical grounds for the utility of an improved parameterization y=z/(1+z). In terms of the y-redshift we again argue that the radius of convergence of any series expansion in y is less than or equal to 1, so that y-based expansions are likely to be good all the way back to the big bang y=1, but that y-based expansions must break down for y<-1, now corresponding to a universe more than twice its current size.

  14. Implementing a Corporate Energy Management System

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the.pdfBreaking of BlytheDepartment of Energy IRSJuly 2012 |Energy Technology -

  15. EcoSystem Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand JumpConceptual Model,DOEHazel Crest, Illinois: EnergyEastport, Maine:EauEcoFactor

  16. Extremely metal-poor gas at a redshift of 7

    E-Print Network [OSTI]

    Simcoe, Robert A; Cooksey, Kathy L; Kao, Melodie M; Matejek, Michael S; Burgasser, Adam J; 10.1038/nature11612

    2012-01-01T23:59:59.000Z

    In typical astrophysical environments, the abundance of heavy elements ranges from 0.001 to 2 times the solar concentration. Lower abundances have been seen in select stars in the Milky Way's halo and in two quasar absorption systems at redshift z=3. These are widely interpreted as relics from the early universe, when all gas possessed a primordial chemistry. Before now there have been no direct abundance measurements from the first Gyr after the Big Bang, when the earliest stars began synthesizing elements. Here we report observations of hydrogen and heavy element absorption in a quasar spectrum at z=7.04, when the universe was just 772 Myr old (5.6% its present age). We detect a large column of neutral hydrogen but no corresponding heavy elements, limiting the chemical abundance to less than 1/10,000 the solar level if the gas is in a gravitationally bound protogalaxy, or less than 1/1,000 solar if it is diffuse and unbound. If the absorption is truly intergalactic, it would imply that the universe was neit...

  17. Sloan Digital Sky Survey Spectroscopic Lens Search. I. Discovery of Intermediate-Redshift Star-Forming Galaxies Behind Foreground Luminous Red Galaxies

    E-Print Network [OSTI]

    Adam S. Bolton; Scott Burles; David J. Schlegel; Daniel J. Eisenstein; J. Brinkmann

    2004-03-16T23:59:59.000Z

    We present a catalog of 49 spectroscopic strong gravitational lens candidates selected from a Sloan Digital Sky Survey sample of 50996 luminous red galaxies. Potentially lensed star-forming galaxies are detected through the presence of background oxygen and hydrogen nebular emission lines in the spectra of these massive foreground galaxies. This multiline selection eliminates the ambiguity of single-line identification and provides a very promising sample of candidate galaxy-galaxy lens systems at low to intermediate redshift, with foreground redshifts ranging from 0.16 to 0.49 and background redshifts from 0.25 to 0.81. Any lenses confirmed within our sample would be important new probes of early-type galaxy mass distributions, providing complementary constraints to those obtained from currently known lensed high-redshift quasars.

  18. A Multiple Network Approach to Corporate Governance

    E-Print Network [OSTI]

    Bonacina, Fausto; Moretto, Enrico; Stefani, Silvana; Torriero, Anna

    2014-01-01T23:59:59.000Z

    In this work, we consider Corporate Governance ties among companies from a multiple network perspective. Such a structurenaturally arises from the close interrelation between the Shareholding Network and the Board of Directors network. Inorder to capture the simultaneous effects on both networks on Corporate Governance, we propose to model the Corporate Governance multiple network structure via tensor analysis. In particular, we consider the TOPHITS model, based on the PARAFAC tensor decomposition, to show that tensor techniques can be successfully applied in this context. After providing some empirical results from the Italian financial market in the univariate case, we will show that a tensor-based multiple network approach can reveal important information.

  19. Daiwa House Industry Co., Ltd. Asahi Kasei Amidas Corporation Sompo Japan Insurance Inc. Nihon Shokken Holdings Co., Ltd. Sysmex Corporation NS Solutions Corporation Fujitsu Research Institute Rakuten Inc. Nomura Research Institute, Ltd. Toray Industries,

    E-Print Network [OSTI]

    Banbara, Mutsunori

    Daiwa House Industry Co., Ltd. Asahi Kasei Amidas Corporation Sompo Japan Insurance Inc. Nihon Shokken Holdings Co., Ltd. Sysmex Corporation NS Solutions Corporation Fujitsu Research Institute Corporation Kawasaki Heavy Industries, Ltd. All Nippon Airways Co., Ltd. Lotteria Co., Ltd. Kao

  20. The redshifts of bright sub-mm sources

    E-Print Network [OSTI]

    James S. Dunlop

    2001-01-17T23:59:59.000Z

    One of the key goals in observational cosmology over the next few years will be to establish the redshift distribution of the recently-discovered sub-mm source population. In this brief review I discuss and summarize the redshift information which has been gleaned to date for the ~ 50 bright sub-mm sources which have been uncovered via the six main classes of survey performed with SCUBA on the JCMT over the last 2-3 years. Despite the biases inherent in some of these surveys, and the crudeness of the redshift information available in others, I conclude that all current information suggests that only 10-15 % of luminous sub-mm sources lie at z < 2, and that the median redshift of this population is z ~ 3. I suggest that such a high median redshift is arguably not unexpected given current theories designed to explain the correlation between black-hole mass and spheroid mass found at low redshift. In such scenarios, peak AGN emission is expected to correspond to, or even to cause termination of major star-formation activity in the host spheroid. In contrast, maximum dust emission is expected to occur roughly half-way through the star-formation process. Given that optical emission from bright quasars peaks at z = 2.5, dust-emission from massive ellipticals might be reasonably expected to peak at some point in the preceding ~ 1 Gyr, at z ~ 3. Confirmation or refutation of this picture requires significantly-improved redshift information on bright samples of SCUBA sources.

  1. Essays on consumption cycles and corporate finance

    E-Print Network [OSTI]

    Issler, Paulo Floriano

    2013-01-01T23:59:59.000Z

    In: The Journal of Finance 41.1, pp. 19–37. Flannery, Markand practice of corporate finance: evidence from the field”.Issues”. In: Journal of Finance 51.5, pp. 1809–33. Hamilton,

  2. Corporate Analysis of DOE Safety Performance

    Broader source: Energy.gov [DOE]

    The Office of Environment, Health, Safety and Security (EHSS), Office of Analysis develops analysis tools and performance dashboards, and conducts analysis of DOE safety performance corporately and on a variety of specific environment, safety and health topics.

  3. 3M's Corporate Approach to Energy Management

    E-Print Network [OSTI]

    Schultz, S. C.; Bingham, P. R.

    number of companies have recognized the benefits of developing structured approaches to improving their energy efficiency through means that are also compatible with being environmentally responsible. 3M has long been recognized as a corporate...

  4. Law as Economy: Convention, Corporation, Currency

    E-Print Network [OSTI]

    Barrett, Jeffrey A.

    1015 Law as Economy: Convention, Corporation, Currency Ritu Birla* I. Law as Economy: Nomos. Law Inside/Outside Economy of an orthodox faith in economy as universal law, that is, in the free market as the law of the universe

  5. Refundable Clean Heating Fuel Tax Credit (Corporate)

    Broader source: Energy.gov [DOE]

    The state of New York began offering a corporate income tax credit for biodiesel purchases used for residential space heating and water heating beginning in 2006. The original credit was authorized...

  6. Alternative Energy Development Incentive (Corporate) (Utah)

    Broader source: Energy.gov [DOE]

    The Alternative Energy Development Incentive (AEDI) is a post-performance non-refundable tax credit for 75% of new state tax revenues (including, state, corporate, sales and withholding taxes) over...

  7. Selecting Financing Strategies to Overcome Corporate Barriers

    E-Print Network [OSTI]

    Michaelson, M. L.

    1984-01-01T23:59:59.000Z

    , or longer than the list of presentations at this year's Industrial Energy Conservation Conference. This paper will focus on two of the many potential answers. First, the corporate decision making process in industrial firms presents many obstacles to a final...

  8. Managing preventative maintenance activities at Intel Corporation

    E-Print Network [OSTI]

    Fearing, Rebecca Cassler

    2006-01-01T23:59:59.000Z

    The work for this thesis was completed at Intel Corporation in Colorado Springs, Colorado at Fab 23, a semiconductor fabrication facility making flash memory. The project focused on evaluating and managing preventative ...

  9. Renewable Energy Production Tax Credit (Corporate)

    Broader source: Energy.gov [DOE]

    Enacted in 2002, the New Mexico Renewable Energy Production Tax Credit provides a tax credit against the corporate income tax of one cent per kilowatt-hour for companies that generate electricity...

  10. IBM Software Group Copyright IBM Corporation 2007

    E-Print Network [OSTI]

    · Componentization of existing code · Assembler programs repackaged as reusable objects · Breaks monolithic code base © Copyright IBM Corporation 2007Page 4 z/TPF fits into your Services Centric Plug and Play Strategy Transport

  11. Data augmentation for machine learning redshifts applied to SDSS galaxies

    E-Print Network [OSTI]

    Hoyle, Ben; Bonnett, Christopher; Seitz, Stella; Weller, Jochen

    2015-01-01T23:59:59.000Z

    We present analyses of data augmentation for machine learning redshift estimation. Data augmentation makes a training sample more closely resemble a test sample, if the two base samples differ, in order to improve measured statistics of the test sample. We perform two sets of analyses by selecting 800k (1.7M) SDSS DR8 (DR10) galaxies with spectroscopic redshifts. We construct a base training set by imposing an artificial r band apparent magnitude cut to select only bright galaxies and then augment this base training set by using simulations and by applying the K-correct package to artificially place training set galaxies at a higher redshift. We obtain redshift estimates for the remaining faint galaxy sample, which are not used during training. We find that data augmentation reduces the error on the recovered redshifts by 40% in both sets of analyses, when compared to the difference in error between the ideal case and the non augmented case. The outlier fraction is also reduced by at least 10% and up to 80% u...

  12. Energy Conservation in China North Industries Corporation

    E-Print Network [OSTI]

    You, W. T.; De, C. H.; Chu, J. X.; Fu, L. R.

    . In some plants which have stable steam consumption we have established small scale power and steam cogeneration. This has improved boilers' efficiencies and utilization of energy. For further reduction oil firing, we have been studying on alternative... ENERGY CONSERVATION IN CHINA NORTH INDUSTRIES CORPORATION Wang Tian You, Chen Hua De, Jing Xing Chu, Ling Rui Fu, China North Industries Corporation Beijing, People's Republic of China ABSTRACT This paper describes an overview of the energy...

  13. Corporate social responsibility (CSR) : responsibility or Innovation? : an analysis of the feedback between CSR activities and the expectations placed upon corporations

    E-Print Network [OSTI]

    Rodriguez, Adrian Xavier

    2010-01-01T23:59:59.000Z

    This thesis uses case study and interview data to present a framework for analyzing corporate behavior in order to define corporate social responsibility (CSR). It answers the question: Can corporations tie corporate social ...

  14. Radio-loud high-redshift protogalaxy canidates in Bootes

    SciTech Connect (OSTI)

    Croft, S; van Breugel, W; Brown, M J; de Vries, W; Dey, A; Eisenhardt, P; Jannuzi, B; Rottgering, H; Stanford, S A; Stern, D; Willner, S P

    2007-07-20T23:59:59.000Z

    We used the Near Infrared Camera (NIRC) on Keck I to obtain K{sub s}-band images of four candidate high-redshift radio galaxies selected using optical and radio data in the NOAO Deep Wide-Field Survey in Bootes. Our targets have 1.4 GHz radio flux densities greater than 1 mJy, but are undetected in the optical. Spectral energy distribution fitting suggests that three of these objects are at z > 3, with radio luminosities near the FR-I/FR-II break. The other has photometric redshift z{sub phot} = 1.2, but may in fact be at higher redshift. Two of the four objects exhibit diffuse morphologies in K{sub s}-band, suggesting that they are still in the process of forming.

  15. Investor Sentiment and Antitrust Law as Determinants of Corporate Ownership Structure: The great Merger Wave of 1897 to 1903

    E-Print Network [OSTI]

    Cheffins, Brian R.

    2002-01-01T23:59:59.000Z

    for Corporate Control: Corporate Governance and EconomicCurrent Trends in Corporate Governance: Going From London toon international corporate governance. This paper retrieves

  16. Investor Sentiment and Antitrust Law as Determinants of Corporate Ownership Structure: The Great Merger Wave of 1897 to 1903

    E-Print Network [OSTI]

    Cheffins, Brian

    2002-01-01T23:59:59.000Z

    for Corporate Control: Corporate Governance and EconomicCurrent Trends in Corporate Governance: Going From London toon international corporate governance. This paper retrieves

  17. CorporateTraining extension.uci.edu/corporate

    E-Print Network [OSTI]

    Stanford, Kyle

    of the system development lifecycle includ- ing procurement, definition, implementation, production, and support

  18. Nonlinear Cosmological Power Spectra in Real and Redshift--Space

    E-Print Network [OSTI]

    A. N. Taylor; A. J. S. Hamilton

    1996-04-03T23:59:59.000Z

    We present an expression for the nonlinear evolution of the cosmological power spectrum based on following Lagrangian trajectories. This is simplified using the Zel'dovich approximation to trace particle displacements, assuming Gaussian initial conditions. The model is found to exhibit the transfer of power from large to small scales expected in self- gravitating fields. We have extended this analysis into redshift-space and found a solution for the nonlinear, anisotropic redshift-space power spectrum in the limit of plane--parallel redshift distortions. The quadrupole-to- monopole ratio is calculated for the case of power-law initial spectra. We find that the shape of this ratio depends on the shape of the initial spectrum, but when scaled to linear theory depends only weakly on the redshift-space distortion parameter, $\\beta$. The point of zero-crossing of the quadrupole, $k_0$, is found to obey a scaling relation. This model is found to be in agreement with $N$-body simulations on scales down to the zero-crossing of the quadrupole, although the wavenumber at zero-crossing is underestimated. These results are applied to the quadrupole--monopole ratio found in the merged QDOT+1.2 Jy IRAS redshift survey. We have estimated that the distortion parameter is constrained to be $\\beta>0.5$ at the $95 \\%$ level. The local primordial spectral slope is not well constrained, but analysis suggests $n \\approx -2$ in the translinear regime. The zero-crossing scale of the quadrupole is $k_0=0.5 \\pm 0.1 h/Mpc$ and from this we infer the amplitude of clustering is $\\sigma_8=0.7 \\pm 0.05$. We suggest that the success of this model is due to nonlinear redshift--space effects arising from infall onto caustics and is not dominated by virialised cluster cores.

  19. Ice emission and the redshifts of submillimeter sources

    E-Print Network [OSTI]

    C. C. Dudley; M. Imanishi; P. R. Maloney

    2008-02-12T23:59:59.000Z

    Observations at submillimeter wavelengths have revealed a population of sources thought to be at relatively large redshifts. The position of the 850 $\\mu$m passband on the Rayleigh-Jeans portion of the Planck function leads to a maximum redshift estimate of $z\\sim$4.5 since sources will not retain their redshift independent brightness close to the peak of the Planck function and thus drop out of surveys. Here we review evidence that ice absorption is present in the spectra of local ultraluminous infrared galaxies which are often taken as analogs for the 850 $\\mu$m source population. We consider the implication of this absorption for ice induced spectral structure at far infrared wavelengths and present marginal astronomical evidence that amorphous ice may have a feature similar to crystalline ice near 150 $\\mu$m. Recent corroborative laboratory evidence is supportive of this conclusion. It is argued that early metal enrichment by pair instability SN may lead to a high ice content relative to refractory dust at high redshift and a fairly robust detection of ice emission in a $z=6.42$ quasar is presented. It is further shown that ice emission is needed to understand the 450 $\\mu$m sources observed in the GOODS-N field. We are thus encouraged to apply far infrared ice emission models to the available observations of HDF 850.1, the brightest submillimeter source in the {\\it Hubble Deep Field}. We suggest that a redshift as large as 13 may need to be considered for this source, nearly a factor of three above the usual top estimate. Inclusion of the possibility of far infrared ice emission in the spectral energy distributions of model sources generally broadens the range of redshifts to be considered for submillimeter sources compared to models without ice emission.

  20. The characteristic stellar mass as a function of redshift

    E-Print Network [OSTI]

    Cathie J. Clarke; Volker Bromm

    2003-05-11T23:59:59.000Z

    We present a model for the star formation process during the initial collapse of dark matter haloes at redshifts z=0-30. We derive a simple expression for the characteristic stellar mass scale during this initial burst of star formation. In our picture, this characteristic scale reflects both the minimum temperature to which the gas can cool (determined by the metallicity and the temperature of the cosmic microwave background) and the pressure of overlying baryons in the collapsing halo. This prescription reproduces both the large mass scales found in simulations of Population III star formation and the near solar values observed for star formation at low redshift.

  1. Multi-object spectroscopy of low redshift EIS clusters. II

    E-Print Network [OSTI]

    L. F. Olsen; L. Hansen; H. E. Joergensen; C. Benoist; L. da Costa; M. Scodeggio

    2003-08-01T23:59:59.000Z

    We present the results of carrying out multi-object spectroscopy in 10 EIS cluster fields. Based on the list of 345 galaxy redshifts we identify significant 3D-density enhancements. For 9 of the EIS clusters we identify significant 3D-concentrations corresponding to the originally detected cluster candidate. We find redshifts in the range 0.097<=z<=0.257 which is in good agreement with the matched filter estimate of z_MF=0.2. We estimate velocity dispersions in the range 219-1160 km/s for the confirmed clusters.

  2. Multi-object spectroscopy of low redshift EIS clusters. I

    E-Print Network [OSTI]

    L. Hansen; L. F. Olsen; H. E. Jorgensen

    2002-04-23T23:59:59.000Z

    We report the results of the first multi-object spectroscopic observations at the Danish 1.54m telescope at La Silla, Chile. Observations of five cluster candidates from the ESO Imaging Survey Cluster Candidate Catalog are described. From these observations we confirm the reality of the five clusters with measured redshifts of 0.11<=z<=0.35. We estimate velocity dispersions in the range 294-621km/s indicating rather poor clusters. This, and the measured cluster redshifts are consistent with the results of the matched filter procedure applied to produce the Cluster Candidate Catalog.

  3. Page 1Forestry Commission England Corporate Plan 2012-13 Corporate Plan

    E-Print Network [OSTI]

    Page 1Forestry Commission England Corporate Plan 2012-13 Corporate Plan 2012-13 #12;Page 2Forestry the environment and supporting a strong green economy, and the Forestry Commission is well placed to contribute toward this. The recent report from the Forestry Regulation Task Force highlighted the need to make

  4. Australian Efforts to Promote Corporate Social Responsibility: Can Disclosure Alone Suffice?

    E-Print Network [OSTI]

    von Nessen, Paul

    2009-01-01T23:59:59.000Z

    they comply with the ASX Corporate Governance Principles andAUSTRALIAN EFFORTS Corporate Governance Principles, isand Gary O'Donovan, Corporate Governance and Environmental

  5. Comparative Corporate Governance: Findings from a Workshop, March 14-15, 2008

    E-Print Network [OSTI]

    Huberty, Mark; Newsome, Akasemi; Street, Alex; Ziegler, J. Nicholas

    2008-01-01T23:59:59.000Z

    of Chicago, ‘‘Corporate Governance: History withoutComparative Corporate Governance Findings from a Workshopon Comparative Corporate Governance, March 14-15, 2008

  6. The Maximands of Corporate Governance: A Theory of Values and Cognitive Style

    E-Print Network [OSTI]

    Licht, Amir

    2004-01-01T23:59:59.000Z

    roots of American corporate governance. See Mark J. Roe, Aover the maximands of corporate governance. 4 My goal ison the maximands of corporate governance, that identifies

  7. Firm Value and Corporate Governance: How the Former Determines the Latter

    E-Print Network [OSTI]

    Hermalin, Benjamin E.

    2008-01-01T23:59:59.000Z

    The Econometrics of Corporate Governance Studies, Cambridge,Firm Value and Corporate Governance: How the FormerAbstract A model of corporate governance must explain (i)

  8. Changes in Japanese Corporate Law and Governance: Revisiting the Convergence Debate

    E-Print Network [OSTI]

    Shishido, Zenichi

    2004-01-01T23:59:59.000Z

    of Path Dependence in Corporate Governance and Ownership.Convergence in Corporate Governance and Its Implicatins.2001). Globalizing Corporate Governance: Convergence of Form

  9. Imitate or Differentiate? Evaluating the validity of corporate social responsibility ratings

    E-Print Network [OSTI]

    Chatterji, Aaron K; Levine, David I. I.

    2008-01-01T23:59:59.000Z

    and A. Metrick “Corporate Governance and Equity Prices. ”investors on corporate governance and social http://it focuses directly on corporate governance and is much more

  10. Corporate Governance from a Comparative Perspective: Specific Applications of the Duty of Loyalty in Korea

    E-Print Network [OSTI]

    Kwon, Jae Yeol

    2004-01-01T23:59:59.000Z

    transaction. Kon S. Kim, Corporate Governance in Korea, 8 J.ARTICLES CORPORATE GOVERNANCE FROM A COMPARATIVEof Care Standard in Corporate Governance, 75 IOWA L. REV. 1,

  11. The Role of Boards of Directors in Corporate Governance: A Conceptual Framework & Survey

    E-Print Network [OSTI]

    Adams, Renee; Hermalin, Benjamin E.; Weisbach, Michael S.

    2008-01-01T23:59:59.000Z

    Era of Heightened Corporate Governance,” New York UniversityThe Emergence of Corporate Governance from Wall St. to MainAnna, ed. , Corporate Governance and Firm Organization,

  12. A TYPE Ia SUPERNOVA AT REDSHIFT 1.55 IN HUBBLE SPACE TELESCOPE INFRARED OBSERVATIONS FROM CANDELS

    SciTech Connect (OSTI)

    Rodney, Steven A.; Riess, Adam G.; Jones, David O. [Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218 (United States); Dahlen, Tomas; Ferguson, Henry C.; Casertano, Stefano; Grogin, Norman A. [Space Telescope Science Institute, Baltimore, MD 21218 (United States); Strolger, Louis-Gregory [Department of Physics, Western Kentucky University, Bowling Green, KY 42101 (United States); Hjorth, Jens; Frederiksen, Teddy F. [Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen (Denmark); Weiner, Benjamin J. [Department of Astronomy, University of Arizona, Tucson, AZ 85721 (United States); Mobasher, Bahram [Department of Physics and Astronomy, University of California, Riverside, CA 92521 (United States); Challis, Peter; Kirshner, Robert P. [Harvard/Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Faber, S. M. [Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 92064 (United States); Filippenko, Alexei V. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Garnavich, Peter; Hayden, Brian [Department of Physics, University of Notre Dame, Notre Dame, IN 46556 (United States); Graur, Or [Department of Astrophysics, Tel Aviv University, 69978 Tel Aviv (Israel); Jha, Saurabh W. [Department of Physics and Astronomy, Rutgers, State University of New Jersey, Piscataway, NJ 08854 (United States); and others

    2012-02-10T23:59:59.000Z

    We report the discovery of a Type Ia supernova (SN Ia) at redshift z = 1.55 with the infrared detector of the Wide Field Camera 3 (WFC3-IR) on the Hubble Space Telescope (HST). This object was discovered in CANDELS imaging data of the Hubble Ultra Deep Field and followed as part of the CANDELS+CLASH Supernova project, comprising the SN search components from those two HST multi-cycle treasury programs. This is the highest redshift SN Ia with direct spectroscopic evidence for classification. It is also the first SN Ia at z > 1 found and followed in the infrared, providing a full light curve in rest-frame optical bands. The classification and redshift are securely defined from a combination of multi-band and multi-epoch photometry of the SN, ground-based spectroscopy of the host galaxy, and WFC3-IR grism spectroscopy of both the SN and host. This object is the first of a projected sample at z > 1.5 that will be discovered by the CANDELS and CLASH programs. The full CANDELS+CLASH SN Ia sample will enable unique tests for evolutionary effects that could arise due to differences in SN Ia progenitor systems as a function of redshift. This high-z sample will also allow measurement of the SN Ia rate out to z Almost-Equal-To 2, providing a complementary constraint on SN Ia progenitor models.

  13. Identifying high-redshift gamma-ray bursts with RATIR

    SciTech Connect (OSTI)

    Littlejohns, O. M.; Butler, N. R. [School of Earth and Space Exploration, Arizona State University, AZ 85287 (United States); Cucchiara, A. [Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Watson, A. M.; Lee, W. H.; Richer, M. G.; De Diego, J. A.; Georgiev, L.; González, J.; Román-Zúñiga, C. G. [Instituto de Astronomía, Universidad Nacional Autónoma de México, Apartado Postal 70-264, 04510 México, D. F. (Mexico); Kutyrev, A. S.; Troja, E.; Gehrels, N.; Moseley, H. [NASA, Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Klein, C. R.; Fox, O. D.; Bloom, J. S. [Astronomy Department, University of California, Berkeley, CA 94720-7450 (United States); Prochaska, J. X.; Ramirez-Ruiz, E. [Department of Astronomy and Astrophysics, UCO/Lick Observatory, University of California, 1156 High Street, Santa Cruz, CA 95064 (United States)

    2014-07-01T23:59:59.000Z

    We present a template-fitting algorithm for determining photometric redshifts, z {sub phot}, of candidate high-redshift gamma-ray bursts (GRBs). Using afterglow photometry, obtained by the Reionization and Transients InfraRed (RATIR) camera, this algorithm accounts for the intrinsic GRB afterglow spectral energy distribution, host dust extinction, and the effect of neutral hydrogen (local and cosmological) along the line of sight. We present the results obtained by this algorithm and the RATIR photometry of GRB 130606A, finding a range of best-fit solutions, 5.6 < z {sub phot} < 6.0, for models of several host dust extinction laws (none, the Milky Way, Large Magellanic Clouds, and Small Magellanic Clouds), consistent with spectroscopic measurements of the redshift of this GRB. Using simulated RATIR photometry, we find that our algorithm provides precise measures of z {sub phot} in the ranges of 4 < z {sub phot} ? 8 and 9 < z {sub phot} < 10 and can robustly determine when z {sub phot} > 4. Further testing highlights the required caution in cases of highly dust-extincted host galaxies. These tests also show that our algorithm does not erroneously find z {sub phot} < 4 when z {sub sim} > 4, thereby minimizing false negatives and allowing us to rapidly identify all potential high-redshift events.

  14. High-redshift Gamma-Ray Burst Studies with GLAST

    SciTech Connect (OSTI)

    Bissaldi, Elisabetta; Longo, Francesco; Barbiellini, Guido [Dipartimento di Fisica, Universita di Trieste, Via Valerio 2, 34100, Trieste (Italy); INFN, Sezione di Trieste, Via Valerio 2, 34100, Trieste (Italy); Calura, Francesco [INAF - Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, 34131 Trieste (Italy); Matteucci, Francesca [Dipartimento di Astronomia, Universita di Trieste, Via G. B. Tiepolo 11, 34131 Trieste (Italy); INAF - Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, 34131 Trieste (Italy)

    2007-05-01T23:59:59.000Z

    We compare predicted Type Ib/c supernova (SN) rates with the observed long-duration gamma-ray burst (GRB) rates both locally and as a function of redshift. To do that, we assume different star formation histories in galaxies of different morphological type: ellipticals, spirals and irregulars. In particular, the predicted Type Ib/c SN rate (SNRIb/c) is always higher than the GRB rate, as expected, suggesting that only a small fraction (0.1-1%) of them become GRBs. We predict a ratio between the cosmic GRB rate and the cosmic SNRIb/c in the range 10-2 - 10-3, in agreement with previous estimates. Finally, due to the high star formation in spheroids at high redshift, we predict more GRBs at high redshift than previous estimates, a prediction which awaits to be proven by future observations by GLAST. Based on our studies and on the current LAT performance, an estimate of the detection possibility of this high-redshift burst population is finally presented.

  15. The metallicities of luminous, massive field galaxies at intermediate redshifts

    E-Print Network [OSTI]

    M. Mouhcine; S. P. Bamford; A. Aragon-Salamanca; O. Nakamura

    2006-03-23T23:59:59.000Z

    We derive oxygen abundances for a sample of 40 luminous (M_{B} = 0.45. Oxygen abundances, relative to hydrogen, of the interstellar emitting gas are estimated by means of the empirically calibrated strong emission line ratio technique. The derived (12+log(O/H)) values range from 8.4 to 9.0, with a median of 8.7. Twenty of these galaxies have securely measured rotation velocities, in the range 50--244 km/s. The measured emission line equivalent widths and diagnostic ratios for the intermediate redshift galaxies cover similar ranges to those observed across a large sample of local galaxies. The estimated oxygen abundances for our luminous star-forming intermediate redshift galaxies cover the same range as their local counterparts. However, at a given galaxy luminosity, many of our galaxies have significantly lower oxygen abundances, i.e., $(12+log(O/H))~8.6$, than local galaxies with similar luminosities. Interestingly, these luminous, massive, intermediate redshift, star-forming galaxies with low oxygen abundances exhibit physical conditions, i.e., emission line equivalent width and ionization state, very similar to those of local faint and metal-poor star-forming galaxies. The oxygen abundance of the interstellar gas does not seem to correlate with the maximum rotation velocity or the emission scale length of the parent galaxy. This suggests that there is a diversity in the intrinsic properties of the massive field galaxy population at intermediate redshifts (ABRIDGED).

  16. The Wolf effect and the redshift of quasars

    SciTech Connect (OSTI)

    James, Daniel F.V.

    1998-01-23T23:59:59.000Z

    We consider a simple model, based on currently accepted models for active galactic nuclei, for a quasi-stellar object (QSO or "quasar") and examine the influence that correlation-induced spectral changes ("The Wolf Effect") may have upon the redshifts of the optical emission lines.

  17. The Age-Redshift Relation for Standard Cosmology

    E-Print Network [OSTI]

    R. C. Thomas; R. Kantowski

    2000-08-10T23:59:59.000Z

    We present compact, analytic expressions for the age-redshift relation $\\tau(z)$ for standard Friedmann-Lema\\^ \\itre-Robertson-Walker (FLRW) cosmology. The new expressions are given in terms of incomplete Legendre elliptic integrals and evaluate much faster than by direct numerical integration.

  18. Multi-parameter estimating photometric redshifts with artificial neural networks

    E-Print Network [OSTI]

    Lili Li; Yanxia Zhang; Yongheng Zhao; Dawei Yang

    2007-04-17T23:59:59.000Z

    We calculate photometric redshifts from the Sloan Digital Sky Survey Data Release 2 Galaxy Sample using artificial neural networks (ANNs). Different input patterns based on various parameters (e.g. magnitude, color index, flux information) are explored and their performances for redshift prediction are compared. For ANN technique, any parameter may be easily incorporated as input, but our results indicate that using dereddening magnitude produces photometric redshift accuracies often better than the Petrosian magnitude or model magnitude. Similarly, the model magnitude is also superior to Petrosian magnitude. In addition, ANNs also show better performance when the more effective parameters increase in the training set. Finally, the method is tested on a sample of 79, 346 galaxies from the SDSS DR2. When using 19 parameters based on the dereddening magnitude, the rms error in redshift estimation is sigma(z)=0.020184. The ANN is highly competitive tool when compared with traditional template-fitting methods where a large and representative training set is available.

  19. Probing the Intergalactic Medium with high-redshift quasars

    E-Print Network [OSTI]

    Calverley, Alexander Peter

    2011-11-08T23:59:59.000Z

    . In Chapter 4 I present the first measurements of ?_bkg at z > 5 from the proximity effect. The UVB intensity declines smoothly with redshift over 4.6 < z < 6.4, implying a smooth evolution in the mean free path of ionizing photons. This suggests...

  20. The Wolf effect and the Redshift of Quasars

    E-Print Network [OSTI]

    Daniel F. V. James

    1998-07-20T23:59:59.000Z

    We consider a simple model, based on currently accepted models for active galactic nuclei, for a quasi-stellar object (QSO or ``quasar'') and examine the influence that correlation- induced spectral changes (``The Wolf Effect'') may have upon the redshifts of the optical emission lines.

  1. EVOLUTION OF GALAXY LUMINOSITY FUNCTION USING PHOTOMETRIC REDSHIFTS

    SciTech Connect (OSTI)

    Ramos, B. H. F.; Pellegrini, P. S.; Da Costa, L. N.; Maia, M. A. G.; Ogando, R. L. C.; De Simoni, F. [Observatorio Nacional, Rua Gal. Jose Cristino 77, Rio de Janeiro, RJ 20921-400 (Brazil); Benoist, C.; Makler, M. [Laboratorio Interinstitucional de e-Astronomia-LIneA, Rua Gal. Jose Cristino 77, Rio de Janeiro, RJ 20921-400 (Brazil); Mesquita, A. A., E-mail: ramos@linea.gov.br, E-mail: pssp@linea.gov.br, E-mail: ldacosta@linea.gov.br, E-mail: maia@linea.gov.br, E-mail: ogando@linea.gov.br, E-mail: fsimoni@linea.gov.br, E-mail: benoist@oca.eu, E-mail: martin@cbpf.br, E-mail: albertoalves@on.br [Universidade Federal do Rio de Janeiro, Observatorio do Valongo, Ladeira do Pedro Antonio, 43 Rio de Janeiro, RJ 20080-090 (Brazil)

    2011-08-15T23:59:59.000Z

    We examine the impact of using photometric redshifts for studying the evolution of both the global galaxy luminosity function (LF) and that for different galaxy types. To this end, we compare the LFs obtained using photometric redshifts from the Canada-France-Hawaii Telescope Legacy Survey (CFHTLS) D1 field with those from the spectroscopic survey VIMOS VLT Deep Survey (VVDS) comprising {approx}4800 galaxies. We find that for z {<=} 2.0, in the interval of magnitudes considered by this survey, the LFs obtained using photometric and spectroscopic redshifts show a remarkable agreement. This good agreement led us to use all four Deep fields of the CFHTLS comprising {approx}386,000 galaxies to compute the LF of the combined fields and directly estimate the error in the parameters based on the field-to-field variation. We find that the characteristic absolute magnitude M* of Schechter fits fades by {approx}0.7 mag from z {approx} 1.8 to z {approx} 0.3, while the characteristic density {phi}* increases by a factor of {approx}4 in the same redshift interval. We use the galaxy classification provided by the template fitting program used to compute photometric redshifts and split the sample into galaxy types. We find that these Schechter parameters evolve differently for each galaxy type, an indication that their evolution is a combination of several effects: galaxy merging, star formation quenching, and mass assembly. All these results are compatible with those obtained by different spectroscopic surveys such as VVDS, DEEP2, and zCosmos, which reinforces the fact that photometric redshifts can be used to study galaxy evolution, at least for the redshift bins adopted so far. This is of great interest since future very large imaging surveys containing hundreds of millions of galaxies will allow us to obtain important precise measurements to constrain the evolution of the LF and to explore the dependence of this evolution on morphology and/or color helping constrain the mechanisms of galaxy evolution.

  2. UV Spectroscopy of Type Ia Supernovae at Low- and High-Redshift

    E-Print Network [OSTI]

    Nugent, Peter

    2005-01-01T23:59:59.000Z

    Spectroscopy of Type Ia Supernovae at Low- and High-RedshiftUV properties of Type Ia Supernovae. The low-redshift studyULDA Access Guide No. 6: Supernovae, The Netherlands: ESA

  3. U. S. forms uranium enrichment corporation

    SciTech Connect (OSTI)

    Seltzer, R.

    1993-07-12T23:59:59.000Z

    After almost 40 years of operation, the federal government is withdrawing from the uranium enrichment business. On July 1, the Department of Energy turned over to a new government-owned entity--the US Enrichment Corp. (USEC)--both the DOE enrichment plants at Paducah, Ky., and Portsmouth, Ohio, and domestic and international marketing of enriched uranium from them. Pushed by the inability of DOE's enrichment operations to meet foreign competition, Congress established USEC under the National Energy Policy Act of 1992, envisioning the new corporation as the first step to full privatization. With gross revenues of $1.5 billion in fiscal 1992, USEC would rank 275th on the Fortune 500 list of top US companies. USEC will lease from DOE the Paducah and Portsmouth facilities, built in the early 1950s, which use the gaseous diffusion process for uranium enrichment. USEC's stock is held by the US Treasury, to which it will pay annual dividends. Martin Marietta Energy Systems, which has operated Paducah since 1984 and Portsmouth since 1986 for DOE, will continue to operate both plants for USEC. Closing one of the two facilities will be studied, especially in light of a 40% world surplus of capacity over demand. USEC also will consider other nuclear-fuel-related ventures. USEC will produce only low-enriched uranium, not weapons-grade material. Indeed, USEC will implement a contract now being completed under which the US will purchase weapons-grade uranium from dismantled Russian nuclear weapons and convert it into low-enriched uranium for power reactor fuel.

  4. Hydra Fuel Cell Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are8COaBulkTransmissionSitingProcess.pdfGetecGtel JumpCounty, Texas: EnergyHy9 CorporationHydra Fuel Cell Corporation

  5. The Canada-France Deep Fields III: Photometric Redshift Distribution to I(AB) ~ 24

    E-Print Network [OSTI]

    M. Brodwin; S. J. Lilly; C. Porciani; H. J. McCracken; O. Le Fevre; S. Foucaud; D. Crampton; Y. Mellier

    2006-07-21T23:59:59.000Z

    We compute accurate redshift distributions to I(AB) = 24 and R(AB) = 24.5 using photometric redshifts estimated from six-band UBVRIZ photometry in the Canada-France Deep Fields-Photometric Redshift Survey (CFDF-PRS). Our photometric redshift algorithm is calibrated using hundreds of CFRS spectroscopic redshifts in the same fields. The dispersion in redshift is \\sigma/(1+z) \\la 0.04 to the CFRS depth of I(AB) = 22.5, rising to \\sigma/(1+z) \\la 0.06 at our nominal magnitude and redshift limits of I(AB) = 24 and z \\le 1.3, respectively. We describe a new method to compute N(z) that incorporates the full redshift likelihood functions in a Bayesian iterative analysis and we demonstrate in extensive Monte Carlo simulations that it is superior to distributions calculated using simple maximum likelihood redshifts. The field-to-field differences in the redshift distributions, while not unexpected theoretically, are substantial even on 30' scales. We provide I(AB) and R(AB) redshift distributions, median redshifts, and parametrized fits of our results in various magnitude ranges, accounting for both random and systematic errors in the analysis.

  6. Fact #624: May 24, 2010 Corporate Average Fuel Economy Standards...

    Energy Savers [EERE]

    4: May 24, 2010 Corporate Average Fuel Economy Standards, Model Years 2012-2016 Fact 624: May 24, 2010 Corporate Average Fuel Economy Standards, Model Years 2012-2016 The final...

  7. Fact #870: April 27, 2015 Corporate Average Fuel Economy Progress...

    Energy Savers [EERE]

    70: April 27, 2015 Corporate Average Fuel Economy Progress, 1978-2014 - Dataset Fact 870: April 27, 2015 Corporate Average Fuel Economy Progress, 1978-2014 - Dataset Excel file...

  8. Corporate Energy Management: A Survey of Large Manufacturing Companies

    E-Print Network [OSTI]

    Norland, D. L.; Lind, L.

    Corporate practices regarding energy management vary substantially from one company to another. Some companies pay close attention to energy use throughout the corporation while others pay scant attention. This paper first describes what we call...

  9. DOE and Calpine Corporation Tap Geothermal Energy from Abandoned...

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

    DOE and Calpine Corporation Tap Geothermal Energy from Abandoned Steam Wells DOE and Calpine Corporation Tap Geothermal Energy from Abandoned Steam Wells April 9, 2015 - 3:48pm...

  10. THE INTERFACE BETWEEN ENVIRONMENTAL ASSESSMENT AND CORPORATE RESPONSIBILITY: THE

    E-Print Network [OSTI]

    THE INTERFACE BETWEEN ENVIRONMENTAL ASSESSMENT AND CORPORATE RESPONSIBILITY: THE VICTOR DIAMOND Report No: 436 Title of Research Project: The Interface Between Environmental Assessment and Corporate: ___________________________________________ #12;iii ABSTRACT The environmental assessment and sustainable development literature recognizes

  11. Fitting In: Extreme Corporate Wellness and Organizational Communication

    E-Print Network [OSTI]

    James, Eric Preston

    2014-07-31T23:59:59.000Z

    In this dissertation I examine the intersection of organizational communication and what I name extreme corporate wellness. I define extreme corporate wellness as the push towards more radical fitness and workplace health promotion via the exercise...

  12. Sandia Corporate Overview - ERN SMU

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

    arrays at any number of insertion points Advanced R&D * System level performance and reliability testing * Component interoperability testing Advanced Power Electronics...

  13. X-RAY ABSORPTION OF HIGH-REDSHIFT QUASARS

    SciTech Connect (OSTI)

    Eitan, Assaf; Behar, Ehud, E-mail: sassafe@tx.technion.ac.il, E-mail: behar@physics.technion.ac.il [Physics Department, Technion, Haifa 32000 (Israel)

    2013-09-01T23:59:59.000Z

    The soft X-ray photoelectric absorption of high-z quasars has been known for two decades, but has no unambiguous astrophysical context. We construct the largest sample to date of 58 high-redshift quasars (z > 0.45) selected from the XMM-Newton archive based on a high photon count criterion (>1800). We measure the optical depth {tau} at 0.5 keV and find that 43% of the quasars show significant absorption. We aim to find which physical parameters of the quasars, e.g., redshift, radio luminosity, radio loudness, or X-ray luminosity, drive their observed absorption. We compare the absorption behavior with redshift with the pattern expected if the diffuse intergalactic medium (IGM) is responsible for the observed absorption. We also compare the absorption with a comparison sample of gamma-ray burst (GRB) X-ray afterglows. Although the z > 2 quasar opacity is consistent with diffuse IGM absorption, many intermediate-z (0.45 < z < 2) quasars are not sufficiently absorbed for this scenario, and are appreciably less absorbed than GRBs. Only 10/37 quasars at z < 2 are absorbed, and only 5/30 radio-quiet quasars are absorbed. We find a weak correlation between {tau} and z, and an even weaker correlation between {tau} and radio luminosity. These findings lead to the conclusion that although a diffuse IGM origin for the quasar absorption is unlikely, the optical depth does seem to increase with redshift, roughly as (1 + z){sup 2.2{+-}0.6}, tending to {tau} Almost-Equal-To 0.4 at high redshifts, similar to the high-z GRBs. This result can be explained by an ionized and clumpy IGM at z < 2, and a cold, diffuse IGM at higher redshift. If, conversely, the absorption occurs at the quasar, and owing to the steep L{sub x} {proportional_to}(1 + z){sup 7.1{+-}0.5} correlation in the present sample, the host column density scales as N{sub H}{proportional_to}L{sub x}{sup 0.7{+-}0.1}.

  14. Rutgers Business School Professor Simi Kedia Corporate Finance

    E-Print Network [OSTI]

    Lin, Xiaodong

    Rutgers Business School Professor Simi Kedia Corporate Finance Office: WP - 1132 26:390:572 Phone Objectives: The objective of this course is to introduce doctoral students to research in corporate finance of capital, corporation finance and the theory of investment, American Economic Review. ***S. Myers and N

  15. The metallicity and dust content of a redshift 5 gamma-ray burst host galaxy

    SciTech Connect (OSTI)

    Sparre, M.; Krühler, T.; Fynbo, J. P. U.; Watson, D. J.; De Ugarte Postigo, A.; Hjorth, J.; Malesani, D. [Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen (Denmark); Hartoog, O. E.; Kaper, L. [Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1098 XH, Amsterdam (Netherlands); Wiersema, K. [Department of Physics and Astronomy, University of Leicester, University Road, Leicester, LE1 7RH (United Kingdom); D'Elia, V. [INAF/Rome Astronomical Observatory, via Frascati 33, I-00040 Monteporzio Catone (Roma) (Italy); Zafar, T. [European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching (Germany); Afonso, P. M. J. [Physics and Astronomy Department, American River College, 4700 College Oak Drive, Sacramento, CA 95841 (United States); Covino, S. [INAF, Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 Merate (Italy); Flores, H. [Laboratoire GEPI, Observatoire de Paris, CNRS-UMR8111, Universite Paris Diderot 5 place Jules Janssen, F-92195 Meudon (France); Goldoni, P. [APC, Astroparticule et Cosmologie, Universite Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, Rue Alice Domon et Léonie Duquet, F-75205 Paris, Cedex 13 (France); Greiner, J. [Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, D-85748 Garching (Germany); Jakobsson, P. [Centre for Astrophysics and Cosmology, Science Institute, University of Iceland, Dunhagi 5, IS-107 Reykjavik (Iceland); Klose, S. [Thüringer Landessternwarte Tautenburg, Sternwarte 5, D-07778 Tautenburg (Germany); Levan, A. J., E-mail: sparre@dark-cosmology.dk [Department of Physics, University of Warwick, Coventry CV4 7AL (United Kingdom); and others

    2014-04-20T23:59:59.000Z

    Observations of the afterglows of long gamma-ray bursts (GRBs) allow the study of star-forming galaxies across most of cosmic history. Here we present observations of GRB 111008A, from which we can measure metallicity, chemical abundance patterns, dust-to-metals ratio (DTM), and extinction of the GRB host galaxy at z = 5.0. The host absorption system is a damped Ly? absorber with a very large neutral hydrogen column density of log?N(H I)/cm{sup ?2}=22.30±0.06 and a metallicity of [S/H] = –1.70 ± 0.10. It is the highest-redshift GRB with such a precise metallicity measurement. The presence of fine-structure lines confirms the z = 5.0 system as the GRB host galaxy and makes this the highest redshift where Fe II fine-structure lines have been detected. The afterglow is mildly reddened with A{sub V} = 0.11 ± 0.04 mag, and the host galaxy has a DTM that is consistent with being equal to or lower than typical values in the Local Group.

  16. CORPORATE: RECORDING Moderator: N/A

    E-Print Network [OSTI]

    US Army Corps of Engineers

    Dredging Program Regulations Webinar, Mr. Joe Wilson. CORPORATE: RECORDING May 29, 2013 Julie Marcy: Okay to the first in our Dredging Operations Technical Support or DOTS Summer Webinar Meeting Series. This series of meetings is intended to share topics of concern about the National Dredging Program. And the meetings

  17. Hindawi Publishing Corporation International Journal of Hypertension

    E-Print Network [OSTI]

    Gleeson, Joseph G.

    Hindawi Publishing Corporation International Journal of Hypertension Volume 2012, Article ID 405892 of Hypertension: The Experience of the Cardiovascular Health Program in Chilean Primary Health Care Centers. To assess the blood pressure control and cardiovascular risk factors (CVRFs) in a population of hypertensive

  18. SUMMER PLACEMENT REPORT International Corporate Leadership Programme

    E-Print Network [OSTI]

    Berzins, M.

    SUMMER PLACEMENT REPORT International Corporate Leadership Programme Name: Faisal M. Khan Year lime product suitable for flue gas treatment. 2. Methods and Results Analytical Methods Used: Research:\\Faculty-of-Engineering\\Keyworth\\Projects\\ICLP\\Private\\2007\\Case Studies\\Faisal Khan - Singleton Birch.doc #12;Business Case: The potential market

  19. DOW CORNING CORPORATION Material Safety Data Sheet

    E-Print Network [OSTI]

    Garmestani, Hamid

    -88-3 Toluene The above components are hazardous as defined in 29 CFR 1910.1200. 3. HAZARDS or water spray. Water can be used to cool fire exposed containers. Fire Fighting Measures: Self to keep fire exposed containers cool. #12;DOW CORNING CORPORATION Material Safety Data Sheet Page: 3 of 8

  20. Senior projectS corporate Sponsored

    E-Print Network [OSTI]

    Stuart, Josh

    --Professor, Computer Engineering | http://users.soe.ucsc. edu/~larrabee/Site/Professor_Tracy_Larrabee.html Charlie McSenior projectS program corporate Sponsored Partner's Day May 31, 2012 Baskin School of Engineering earning their engineering degree and fulfilling this capstone design sequence. Our students who have

  1. Hindawi Publishing Corporation Advances in Multimedia

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    Hindawi Publishing Corporation Advances in Multimedia Volume 2010, Article ID 386035, 17 pages doi:10.1155/2010/386035 Research Article MMSA: Metamodel Multimedia Software Architecture Makhlouf with heterogeneous multimedia components. It enables the description of the software architectures as a collection

  2. Hindawi Publishing Corporation Advances in Multimedia

    E-Print Network [OSTI]

    Paris-Sud XI, Université de

    Hindawi Publishing Corporation Advances in Multimedia Volume 2013, Article ID 175064, 22 pages http camera is a challenge that multimedia community is facing with the proliferation of such sensors posed to the Multimedia research community earlier. For instance, visual lifelogs can record daily

  3. Hindawi Publishing Corporation Comparative and Functional Genomics

    E-Print Network [OSTI]

    Newcastle upon Tyne, University of

    Hindawi Publishing Corporation Comparative and Functional Genomics Volume 2007, Article ID 47304, 7 pages doi:10.1155/2007/47304 Meeting Report eGenomics: Cataloguing Our Complete Genome Collection III, Michigan State University, East Lansing, MI 48824, USA 3 The Institute for Genomic Research, 9712 Medical

  4. Libraries Reference Copyright 1996 -2003 Intel Corporation

    E-Print Network [OSTI]

    Fossati, Giovanni

    Intel® Fortran Libraries Reference Copyright © 1996 - 2003 Intel Corporation All Rights Reserved PROPERTY RIGHT. Intel products are not intended for use in medical, life saving, or life sustain- ing applications. This Intel® Fortran Libraries Reference as well as the software described in it is furnished

  5. Hindawi Publishing Corporation Journal of Sensors

    E-Print Network [OSTI]

    Calgary, University of

    Hindawi Publishing Corporation Journal of Sensors Volume 2010, Article ID 967245, 10 pages doi:10 artificial magnetic perturbations introduced close to the sensor on the host platform and without additional landmarks, like mountains or stones that early men could easily recognize and remember during their travels

  6. Hindawi Publishing Corporation Advances in Artificial Intelligence

    E-Print Network [OSTI]

    Hexmoor, Henry

    Coulomb's Law Pejman Kamkarian1 and Henry Hexmoor2 1 Electrical and Computer Engineering Department, supervisors can guide people to safety. In this paper, we combine Coulomb's electrical law, graph theoryHindawi Publishing Corporation Advances in Artificial Intelligence Volume 2012, Article ID 340615

  7. Hindawi Publishing Corporation International Journal of Ecology

    E-Print Network [OSTI]

    Rieseberg, Loren

    Hindawi Publishing Corporation International Journal of Ecology Volume 2012, Article ID 939862, 17 pages doi:10.1155/2012/939862 Review Article Parallel Ecological Speciation in Plants? Katherine L speciation, known as parallel ecological speciation, is one of several forms of evidence for ecology's role

  8. URANIUM MILLING ACTIVITIES AT SEQUOYAH FUELS CORPORATION

    E-Print Network [OSTI]

    unknown authors

    Sequoyah Fuels Corporation (SFC) describes previous operations at its Gore, Oklahoma, uranium conversion facility as: (1) the recovery of uranium by concentration and purification processes; and (2) the conversion of concentrated and purified uranium ore into uranium hexafluoride (UF 6), or the reduction of depleted uranium tetrafluoride (UF 4) to UF 6. SFC contends that these

  9. Researcher at Cerner Corporation Cerner Overview

    E-Print Network [OSTI]

    Jornsten, Rebecka

    Researcher at Cerner Corporation Cerner Overview Cerner is the leading U.S. supplier of healthcare Qualifications Minimum Qualifications: · Master's degree in biostatistics, epidemiology, MIS or related field. Preferred Qualifications: · Intermediate knowledge of both traditional statistical methods and modern

  10. Hindawi Publishing Corporation Journal of Nanotechnology

    E-Print Network [OSTI]

    Wang, Yan Alexander

    Hindawi Publishing Corporation Journal of Nanotechnology Volume 2010, Article ID 801789, 42 pages a general interest in both fundamental and practical nanotechnology. Over the past 20 years, research's -orbital axis vector (POAV) #12;2 Journal of Nanotechnology (0,0) (1,0) (2,0) (3,0) (4,0) (5,0) (1,1) (2

  11. The internship in Corporate Communications at Beaumont Hospital, Royal Oak is affiliated with one of the

    E-Print Network [OSTI]

    Cinabro, David

    The internship in Corporate Communications at Beaumont Hospital, Royal Oak is affiliated with one atmosphere and Beaumont is a great place to work! Beaumont Internship 3601 W. 13 Mile Road Royal Oak, MI 48073 Rebecca Calappi internship coordinator rcalappi@beaumont.edu Intern with Beaumont Health System

  12. Renewable Energy Tax Credit (Corporate)

    Broader source: Energy.gov [DOE]

    Nebraska offers a production-based tax credit to any producer of electricity generated by wind, solar, geothermal, hydropower, fuel cells or methane gas. To qualify, a system must be placed into...

  13. Revisiting the cosmological bias due to local gravitational redshifts

    E-Print Network [OSTI]

    Huang, Zhiqi

    2015-01-01T23:59:59.000Z

    A recent article by Wojtak {\\it et al} (arXiv:1504.00178) pointed out that the local gravitational redshift, despite its smallness ($\\sim 10^{-5}$), can have a noticeable ($\\sim 1\\%$) systematic effect on our cosmological parameter measurements. The authors studied a few extended cosmological models (non-flat $\\Lambda$CDM, $w$CDM, and $w_0$-$w_a$CDM) with a mock supernova dataset. We repeat this calculation and find that the $\\sim 1\\%$ biases are due to strong degeneracy between cosmological parameters. When Cosmic Microwave Background (CMB) data are added to break the degeneracy, the biases due to local gravitational redshift are negligible ($\\lesssim 0.1 \\sigma$).

  14. Can Population III Stars at High Redshifts produce GRB's?

    E-Print Network [OSTI]

    C. Sivaram; Kenath Arun

    2010-08-24T23:59:59.000Z

    Gamma ray bursts are the most luminous physical phenomena in the universe, consisting of flashes of gamma rays that last from seconds to hours. There have been attempts to observe gamma ray bursts, for example, from population III stars of about 500 solar mass at high redshifts. Here we argue that collapse of such high mass stars does not lead to gamma ray burst as their core collapse temperatures are not sufficient to produce gamma rays, leading to GRBs.

  15. Time, Distance, Velocity, Redshift: a personal guided tour

    E-Print Network [OSTI]

    T. Kiang

    2003-08-01T23:59:59.000Z

    An attempt to answer the question 'Can we observe galaxies that recede faster than light ?' led to a re-examination of the notions of time, distance, velocity and redshift as they occur in newtonian physics, special relativity, general relativity and cosmology. A number of misconceptions were uncovered. It was found that, once freed of special relativity preconceptions, the above question is easily and unequivocally answered

  16. A faint galaxy redshift survey behind massive clusters

    SciTech Connect (OSTI)

    Frye, Brenda

    1999-12-01T23:59:59.000Z

    This thesis is concerned with the gravitational lensing effect by massive galaxy clusters. We have explored a new technique for measuring galaxy masses and for detecting high-z galaxies by their optical colors. A redshift survey has been obtained at the Keck for a magnitude limited sample of objects (I<23) behind three clusters, A1689, A2390, and A2218 within a radius of 0.5M pc. For each cluster we see both a clear trend of increasing flux and redshift towards the center. This behavior is the result of image magnifications, such that at fixed redshift one sees further down the luminosity function. The gradient of this magnification is, unlike measurements of image distortion, sensitive to the mass profile, and found to depart strongly from a pure isothermal halo. We have found that V RI color selection can be used effectively as a discriminant for finding high-z galaxies behind clusters and present five 4.1 < z < 5.1 spectra which are of very high quality due to their high mean magnification of {approximately}20, showing strong, visibly-saturated interstellar metal lines in some cases. We have also investigated the radio ring lens PKS 1830-211, locating the source and multiple images and detected molecular absorption at mm wavelengths. Broad molecular absorption of width 1/40kms is found toward the southwest component only, where surprisingly it does not reach the base of the continuum, which implies incomplete coverage of the SW component by molecular gas, despite the small projected size of the source, less than 1/8h pc at the absorption redshift.

  17. Powerful evidences for supporting the claim that gamma-ray burst redshifts are gravity-generated

    E-Print Network [OSTI]

    Fu-Gao Song

    2012-06-24T23:59:59.000Z

    At present, it is widely believed that the phenomenon of the gamma-ray burst redshift is cosmological origin. From a theoretical point of view, this redshift has either a cosmological or a cause that is related to gravity. However, the question of whether the gamma-ray burst redshift has a cosmological origin or not should be answerable in no uncertain terms because both the spectrum characteristics and the count distribution law arising from the two distinct settings are completely different. If the redshift of GRB is generated by gravity, then the afterglow spectrum will certainly contain both the gravitational redshits (containing emission and absorption feature) and Doppler absorption redshift, and hold a definite relation between the two redshifts. In this paper, we present nine direct and decisive evidences to show that the gamma-ray burst redshift is indeed generated by gravity of neutron stars in their merging process; in which, 114 GRBs' redshifts showed that the statistical count distribution law for the two kinds redshift is the same (with errors less than 1.5%), and 74 spectral line redshifts of two GRBs showed that the relation between the two kinds redshift is completely correct (with errors less than 0.0061%).

  18. Cosmographic transition redshift in $f(R)$ gravity

    E-Print Network [OSTI]

    Salvatore Capozziello; Orlando Luongo

    2014-11-10T23:59:59.000Z

    We propose a strategy to infer the transition redshift $z_{da}$, which characterizes the passage through the universe decelerated to accelerated phases, in the framework $f(R)$ gravities. To this end, we numerically reconstruct $f(z)$, i.e. the corresponding $f(R)$ function re-expressed in terms of the redshift $z$ and we show how to match $f(z)$ with cosmography. In particular, we relate $f(z)$ and its derivatives to the cosmographic coefficients, i.e. $H_0, q_0$ and $j_0$ and demonstrate that its corresponding evolution may be framed by means of an effective logarithmic dark energy term $\\Omega_X$, slightly departing from the case of a pure cosmological constant. Afterwards, we show that our model predicts viable transition redshift constraints, which agree with $\\Lambda$CDM. To do so, we compute the corresponding $z_{da}$ in terms of cosmographic outcomes and find that $z_{da}\\leq1$. Finally, we reproduce an effective $f(z)$ and show that this class of models is fairly well compatible with present-time data. To do so, we get numerical constraints employing Monte Carlo fits with the Union 2.1 supernova survey and with the Hubble measurement data set.

  19. Testing the Accuracy of Redshift Space Group Finding Algorithms

    E-Print Network [OSTI]

    James J. Frederic

    1994-09-07T23:59:59.000Z

    Using simulated redshift surveys generated from a high resolution N-body cosmological structure simulation, we study algorithms used to identify groups of galaxies in redshift space. Two algorithms are investigated; both are friends-of-friends schemes with variable linking lengths in the radial and transverse dimensions. The chief difference between the algorithms is in the redshift linking length. The algorithm proposed by Huchra \\& Geller (1982) uses a generous linking length designed to find ``fingers of god'' while that of Nolthenius \\& White (1987) uses a smaller linking length to minimize contamination by projection. We find that neither of the algorithms studied is intrinsically superior to the other; rather, the ideal algorithm as well as the ideal algorithm parameters depend on the purpose for which groups are to be studied. The Huchra/Geller algorithm misses few real groups, at the cost of including some spurious groups and members, while the Nolthenius/White algorithm misses high velocity dispersion groups and members but is less likely to include interlopers in its group assignments. In a companion paper we investigate the accuracy of virial mass estimates and clustering properties of groups identified using these algorithms.

  20. Ampulse Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnualProperty EditCalifornia: Energy Resources Jump to:Almo,Transmission Systems IncAmpulse

  1. HTS wire development at Intermagnetic General Corporation

    SciTech Connect (OSTI)

    Haldar, P. [Intermagnetics General Corp., Latham, NY (United States)

    1994-07-29T23:59:59.000Z

    The HTS wire development program at Intermagnetics General Corporation is outlined. Technical achievements in the Bi-2223, Tl-1223 and Tl-based conductor program are summarized. Long lengths of Tl-based HTS tapes with uniform transport properties have been fabricated. Multifilament samples of Tl-based HTS tapes have been fabricated for the first time. Optimization of thermomechanical processing is ongoing and weak links is still a major problem in P-I-T tapes. Future work is summarized.

  2. How to measure redshift-space distortions without sample variance

    E-Print Network [OSTI]

    Patrick McDonald; Uros Seljak

    2008-10-02T23:59:59.000Z

    We show how to use multiple tracers of large-scale density with different biases to measure the redshift-space distortion parameter beta=f/b=(dlnD/dlna)/b (where D is the growth rate and a the expansion factor), to a much better precision than one could achieve with a single tracer, to an arbitrary precision in the low noise limit. In combination with the power spectrum of the tracers this allows a much more precise measurement of the bias-free velocity divergence power spectrum, f^2 P_m - in fact, in the low noise limit f^2 P_m can be measured as well as would be possible if velocity divergence was observed directly, with rms improvement factor ~[5.2(beta^2+2 beta+2)/beta^2]^0.5 (e.g., ~10 times better than a single tracer for beta=0.4). This would allow a high precision determination of f D as a function of redshift with an error as low as 0.1%. We find up to two orders of magnitude improvement in Figure of Merit for the Dark Energy equation of state relative to Stage II, a factor of several better than other proposed Stage IV Dark Energy surveys. The ratio b_2/b_1 will be determined with an even greater precision than beta, producing, when measured as a function of scale, an exquisitely sensitive probe of the onset of non-linear bias. We also extend in more detail previous work on the use of the same technique to measure non-Gaussianity. Currently planned redshift surveys are typically designed with signal to noise of unity on scales of interest, and are not optimized for this technique. Our results suggest that this strategy may need to be revisited as there are large gains to be achieved from surveys with higher number densities of galaxies.

  3. Gravitational red-shift and deflection of slow light

    E-Print Network [OSTI]

    J. Dressel; S. G. Rajeev; J. C. Howell; A. N. Jordan

    2008-10-27T23:59:59.000Z

    We explore the nature of the classical propagation of light through media with strong frequency-dependent dispersion in the presence of a gravitational field. In the weak field limit, gravity causes a redshift of the optical frequency, which the slow-light medium converts into a spatially-varying index of refraction. This results in the bending of a light ray in the medium. We further propose experimental techniques to amplify and detect the phenomenon using weak value measurements. Independent heuristic and rigorous derivations of this effect are given.

  4. A Spectroscopic Survey of the Fields of 28 Strong Gravitational Lenses: The Redshift Catalog

    E-Print Network [OSTI]

    Momcheva, Ivelina; Cool, Richard J; Keeton, Charles R; Zabludoff, Ann I

    2015-01-01T23:59:59.000Z

    We present the spectroscopic redshift catalog from a wide-field survey of the fields of 28 galaxy-mass strong gravitational lenses. We discuss the acquisition and reduction of the survey data, collected over 40 nights of 6.5m MMT and Magellan time, employing four different multi-object spectrographs. We determine that no biases are introduced by combining datasets obtained with different instrument/spectrograph combinations. Special care is taken to determine redshift uncertainties using repeat observations. The redshift catalog consists of 9768 new and unique galaxy redshifts. 82.4% of the catalog redshifts are between z=0.1 and z=0.7, and the catalog median redshift is z=0.36. The data from this survey will be used to study the lens environments and line-of-sight structures to gain a better understanding of the effects of large scale structure on lens statistics and lens-derived parameters.

  5. FEEDBACK FROM HIGH-MASS X-RAY BINARIES ON THE HIGH-REDSHIFT INTERGALACTIC MEDIUM: MODEL SPECTRA

    SciTech Connect (OSTI)

    Power, Chris [International Centre for Radio Astronomy Research, University of Western Australia, 35 Stirling Highway, Crawley, WA 6009 (Australia)] [International Centre for Radio Astronomy Research, University of Western Australia, 35 Stirling Highway, Crawley, WA 6009 (Australia); James, Gillian; Wynn, Graham [Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH (United Kingdom)] [Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH (United Kingdom); Combet, Celine, E-mail: chris.power@icrar.org [Laboratoire de Physique Subatomique et de Cosmologie, Universite Joseph Fourier Grenoble 1/CNRS/IN2P3/INPG, 53 avenue des Martyrs, F-38026 Grenoble (France)] [Laboratoire de Physique Subatomique et de Cosmologie, Universite Joseph Fourier Grenoble 1/CNRS/IN2P3/INPG, 53 avenue des Martyrs, F-38026 Grenoble (France)

    2013-02-10T23:59:59.000Z

    Massive stars at redshifts z {approx}> 6 are predicted to have played a pivotal role in cosmological reionization as luminous sources of ultraviolet (UV) photons. However, the remnants of these massive stars could be equally important as X-ray-luminous (L{sub X} {approx} 10{sup 38} erg s{sup -1}) high-mass X-ray binaries (HMXBs). Because the absorption cross section of neutral hydrogen decreases sharply with photon energy ({sigma}{proportional_to}E {sup -3}), X-rays can escape more freely than UV photons from the star-forming regions in which they are produced, allowing HMXBs to make a potentially significant contribution to the ionizing X-ray background during reionization. In this paper, we explore the ionizing power of HMXBs at redshifts z {approx}> 6 using a Monte Carlo model for a coeval stellar population of main-sequence stars and HMXBs. Using the archetypal Galactic HMXB Cygnus X-1 as our template, we propose a composite HMXB spectral energy distribution consisting of blackbody and power-law components, whose contributions depend on the accretion state of the system. We determine the time-dependent ionizing power of a combined population of UV-luminous stars and X-ray-luminous HMXBs and deduce fitting formulae for the boost in the population's ionizing power arising from HMXBs; these fits allow for simple implementation of HMXB feedback in numerical simulations. Based on this analysis, we estimate the contribution of high-redshift HMXBs to the present-day soft X-ray background, and we show that it is a factor of {approx}100-1000 smaller than the observed limit. Finally, we discuss the implications of our results for the role of HMXBs in reionization and in high-redshift galaxy formation.

  6. Distribution function approach to redshift space distortions. Part III: halos and galaxies

    SciTech Connect (OSTI)

    Okumura, Teppei; Seljak, Uroš [Institute for the Early Universe, Ewha Womans University, Seoul 120-750, S. Korea (Korea, Republic of); Desjacques, Vincent, E-mail: teppei@ewha.ac.kr, E-mail: useljak@berkeley.edu, E-mail: dvince@physik.uzh.ch [Département de Physique Théorique and Center for Astroparticle Physics (CAP), Université de Genève, 1211 Genève (Switzerland)

    2012-11-01T23:59:59.000Z

    It was recently shown that the power spectrum in redshift space can be written as a sum of cross-power spectra between number weighted velocity moments, of which the lowest are density and momentum density. We investigate numerically the properties of these power spectra for simulated galaxies and dark matter halos and compare them to the dark matter power spectra, generalizing the concept of the bias in density-density power spectra. Because all of the quantities are number weighted this approach is well defined even for sparse systems such as massive halos. This contrasts to the previous approaches to RSD where velocity correlations have been explored, but velocity field is a poorly defined concept for sparse systems. We find that the number density weighting leads to a strong scale dependence of the bias terms for momentum density auto-correlation and cross-correlation with density. This trend becomes more significant for the more biased halos and leads to an enhancement of RSD power relative to the linear theory. Fingers-of-god effects, which in this formalism come from the correlations of the higher order moments beyond the momentum density, lead to smoothing of the power spectrum and can reduce this enhancement of power from the scale dependent bias, but are relatively small for halos with no small scale velocity dispersion. In comparison, for a more realistic galaxy sample with satellites the small scale velocity dispersion generated by satellite motions inside the halos leads to a larger power suppression on small scales, but this depends on the satellite fraction and on the details of how the satellites are distributed inside the halo. We investigate several statistics such as the two-dimensional power spectrum P(k,?), where ? is the angle between the Fourier mode and line of sight, its multipole moments, its powers of ?{sup 2}, and configuration space statistics. Overall we find that the nonlinear effects in realistic galaxy samples such as luminous red galaxies affect the redshift space clustering on very large scales: for example, the quadrupole moment is affected by 10% for k < 0.1hMpc{sup ?1}, which means that these effects need to be understood if we want to extract cosmological information from the redshift space distortions.

  7. DETERMINING THE LUMINOSITY FUNCTION OF SWIFT LONG GAMMA-RAY BURSTS WITH PSEUDO-REDSHIFTS

    SciTech Connect (OSTI)

    Tan Weiwei; Yu Yunwei [Institute of Astrophysics, Central China Normal University, Wuhan (China); Cao Xiaofeng, E-mail: yuyw@phy.ccnu.edu.cn [School of Physics, Huazhong University of Science and Technology, Wuhan (China)

    2013-07-20T23:59:59.000Z

    The determination of the luminosity function (LF) of gamma-ray bursts (GRBs) is an important role for the cosmological applications of the GRBs, which, however, is seriously hindered by some selection effects due to redshift measurements. In order to avoid these selection effects, we suggest calculating pseudo-redshifts for Swift GRBs according to the empirical L-E{sub p} relationship. Here, such a L-E{sub p} relationship is determined by reconciling the distributions of pseudo- and real redshifts of redshift-known GRBs. The values of E{sub p} taken from Butler's GRB catalog are estimated with Bayesian statistics rather than observed. Using the GRB sample with pseudo-redshifts of a relatively large number, we fit the redshift-resolved luminosity distributions of the GRBs with a broken-power-law LF. The fitting results suggest that the LF could evolve with redshift by a redshift-dependent break luminosity, e.g., L{sub b} = 1.2 Multiplication-Sign 10{sup 51}(1 + z){sup 2} erg s{sup -1}. The low- and high-luminosity indices are constrained to 0.8 and 2.0, respectively. It is found that the proportional coefficient between the GRB event rate and the star formation rate should correspondingly decrease with increasing redshifts.

  8. Progress Report on the Berkeley/Anglo-Australian Observatory High-Redshift Supernova Search

    E-Print Network [OSTI]

    Goldhaber, G.

    2008-01-01T23:59:59.000Z

    photometry curve for type Ia supernovae and the redshift vsdistributions for observed supernovae. Figure 5 from Millermain efforts related to supernovae in progress at Berkeley.

  9. THE 2dF REDSHIFT SURVEY. I. PHYSICAL ASSOCIATION AND PERIODICITY IN QUASAR FAMILIES

    SciTech Connect (OSTI)

    Fulton, C. C. [School of Physics, University of Western Australia, 35 Stirling Highway, Crawley, 6009 WA (Australia); Arp, H. C., E-mail: chris.fulton@uwa.edu.au, E-mail: arp@mpa-garching.mpg.de [Max-Planck-Institut fuer Astrophysik, Karl Schwarzschild-Str. 1, Postfach 1317, D-85741 Garching (Germany)

    2012-08-01T23:59:59.000Z

    We have tested for physical association of candidate companion quasars with putative parent galaxies by virtue of Karlsson periodicity in quasar redshifts. We examined galaxies from the 2dF Galaxy Redshift Survey (2dFGRS) and quasars from the 2dF Quasar Redshift Survey (2QZ) in the two declination strips (at declinations 0 Degree-Sign and -30 Degree-Sign ) covered by the 2QZ, first filtering out galaxies and quasars using the respective survey masks and observation qualities as described, and using only quasars with z {>=} 0.5 to avoid the redshift region of mixed galaxies and quasars. Around each galaxy, quasars are detected as physically associated with a putative parent galaxy if their respective redshifts conform to empirically derived constraints based on an ejection hypothesis. We ran Monte Carlo control trials against the pure physical associations by replacing the actual redshifts of the candidate companion quasars with quasar redshifts drawn randomly from each respective right ascension hour. The constraints are grouping of quasar redshifts and Karlsson periodicity of quasar redshifts.

  10. The Shareholder Derivative Action and Good Corporate Governance in China: Why the Excitement is Actually for Nothing

    E-Print Network [OSTI]

    Zhang, Zhong

    2011-01-01T23:59:59.000Z

    Noack & Dirk Zetzsche, Corporate Governance Reform in Ger-Protection Seriously? Corporate Governance in the UnitedDonald C. Clarke, Corporate Governance in China: An Overview

  11. "Enlightened Shareholder Value": Corporate Governance Beyond the Shareholder - Stakeholder Divide

    E-Print Network [OSTI]

    Harper Ho, Virginia E.

    2010-01-01T23:59:59.000Z

    Ho FINAL.docx Do Not Delete 11/15/2010 4:38 PM “Enlightened Shareholder Value”: Corporate Governance Beyond the Shareholder-Stakeholder Divide Virginia Harper Ho* I. INTRODUCTION... on Risk Management and Corporate Governance, Oct. 2009, for their generous comments on earlier drafts. All remaining errors are mine alone. Ho FINAL.docx Do Not Delete 11/15/2010 4:38 PM 60 The Journal of Corporation Law [Vol. 36:1 1. The Enlightened...

  12. Accessing the population of high redshift Gamma Ray Bursts

    E-Print Network [OSTI]

    Ghirlanda, G; Ghisellini, G; Mereghetti, S; Tagliaferri, G; Campana, S; Osborne, J P; O'Brien, P; Tanvir, N; Willingale, R; Amati, L; Basa, S; Bernardini, M G; Burlon, D; Covino, S; D'Avanzo, P; Frontera, F; Gotz, D; Melandri, A; Nava, L; Piro, L; Vergani, S D

    2015-01-01T23:59:59.000Z

    Gamma Ray Bursts (GRBs) are a powerful probe of the high redshift Universe. We present a tool to estimate the detection rate of high-z GRBs by a generic detector with defined energy band and sensitivity. We base this on a population model that reproduces the observed properties of GRBs detected by Swift, Fermi and CGRO in the hard X-ray and gamma-ray bands. We provide the expected cumulative distributions of the flux and fluence of simulated GRBs in different energy bands. We show that scintillator detectors, operating at relatively high energies (e.g. tens of keV to the MeV), can detect only the most luminous GRBs at high redshifts due to the link between the peak spectral energy and the luminosity (Ep-Liso) of GRBs. We show that the best strategy for catching the largest number of high-z bursts is to go softer (e.g. in the soft X-ray band) but with a very high sensitivity. For instance, an imaging soft X-ray detector operating in the 0.2-5 keV energy band reaching a sensitivity, corresponding to a fluence o...

  13. The SDSS Coadd: A Galaxy Photometric Redshift Catalog

    SciTech Connect (OSTI)

    Reis, Ribamar R.R.; /Fermilab /Rio de Janeiro Federal U.; Soares-Santos, Marcelle; /Fermilab /Inst. Geo. Astron., Havana /Sao Paulo U.; Annis, James; /Fermilab; Dodelson, Scott; /Fermilab /Chicago U. /Chicago U., KICP; Hao, Jiangang; /Fermilab; Johnston, David; /Fermilab; Kubo, Jeffrey; /Fermilab; Lin, Huan; /Fermilab; Seo, Hee-Jong; /UC, Berkeley; Simet, Melanie; /Chicago U.

    2011-11-01T23:59:59.000Z

    We present and describe a catalog of galaxy photometric redshifts (photo-z's) for the Sloan Digital Sky Survey (SDSS) Coadd Data. We use the Artificial Neural Network (ANN) technique to calculate photo-z's and the Nearest Neighbor Error (NNE) method to estimate photo-z errors for {approx} 13 million objects classified as galaxies in the coadd with r < 24.5. The photo-z and photo-z error estimators are trained and validated on a sample of {approx} 89, 000 galaxies that have SDSS photometry and spectroscopic redshifts measured by the SDSS Data Release 7 (DR7), the Canadian Network for Observational Cosmology Field Galaxy Survey (CNOC2), the Deep Extragalactic Evolutionary Probe Data Release 3(DEEP2 DR3), the SDSS-III's Baryon Oscillation Spectroscopic Survey (BOSS), the Visible imaging Multi-Object Spectrograph - Very Large Telescope Deep Survey (VVDS) and the WiggleZ Dark Energy Survey. For the best ANN methods we have tried, we find that 68% of the galaxies in the validation set have a photo-z error smaller than {sigma}{sub 68} = 0.036. After presenting our results and quality tests, we provide a short guide for users accessing the public data.

  14. The mass function of high redshift seed black holes

    E-Print Network [OSTI]

    Giuseppe Lodato; Priyamvada Natarajan

    2007-02-13T23:59:59.000Z

    In this paper we derive the mass function of seed black holes that result from the central mass concentrated via disc accretion in collapsed haloes at redshift $z\\approx 15$. Using standard arguments including stability, we show that these pre-galactic discs can assemble a significant mass concentration in the inner regions, providing fuel for the formation and initial growth of super-massive black holes. Assuming that these mass concentrations do result in central seed black holes, we determine the mass distribution of these seeds as a function of key halo properties. The seed mass distribution determined here turns out to be asymmetric and skewed to higher masses. Starting with these initial seeds, building up to $10^9$ solar masses by $z = 6$ to power the bright quasars is not a problem in the standard LCDM cosmogony. These seed black holes in gas rich environments are likely to grow into the supermassive black holes at later times via mergers and accretion. Gas accretion onto these seeds at high redshift will produce miniquasars that likely play an important role in the reionization of the Universe. Some of these seed black holes on the other hand could be wandering in galaxy haloes as a consequence of frequent mergers, powering the off-nuclear ultra-luminous X-ray sources detected in nearby galaxies.

  15. The inferred redshift distribution of the faint blue excess

    E-Print Network [OSTI]

    Driver, S P; Phillipps, S; Windhorst, R A; Driver, Simon P; Couch, Warrick J; Phillipps, Steven; Windhorst, Rogier A

    1996-01-01T23:59:59.000Z

    We infer the redshift distribution of the faint blue galaxy excess (FBE) at B=23.5 by subtracting the predicted distribution of giant/normal galaxies from the observed N(z) distribution for all types. This is possible because of the recent deep {\\it Hubble Space Telescope} (HST) WFPC2 morphological number counts which have convincingly demonstrated that little evolution of the giant population is seen to B=26.0. The mean redshift of the FBE at B=23.5 is found to be _{FBE}=0.40 +/- 0.07 with upper and lower quartiles defined by z_{0.75}=0.58 +/- 0.05 and z_{0.25}=0.28 +/- 0.05, respectively. We compare this inferred FBE N(z) distribution to the predictions from three generic faint galaxy models: dwarf dominated (no evolution), pure luminosity evolution, and evolving dwarfs. The inferred FBE N(z) distribution strongly supports a hybrid evolving dwarf--rich model wherein a large population of dwarfs present at z=0.5 has subsequently faded to obscurity. The total integrated number density of dwarfs (down to M_{B}...

  16. The inferred redshift distribution of the faint blue excess

    E-Print Network [OSTI]

    Simon P. Driver; Warrick J. Couch; Steven Phillipps; Rogier A. Windhorst

    1996-05-10T23:59:59.000Z

    We infer the redshift distribution of the faint blue galaxy excess (FBE) at B=23.5 by subtracting the predicted distribution of giant/normal galaxies from the observed N(z) distribution for all types. This is possible because of the recent deep {\\it Hubble Space Telescope} (HST) WFPC2 morphological number counts which have convincingly demonstrated that little evolution of the giant population is seen to B=26.0. The mean redshift of the FBE at B=23.5 is found to be _{FBE}=0.40 +/- 0.07 with upper and lower quartiles defined by z_{0.75}=0.58 +/- 0.05 and z_{0.25}=0.28 +/- 0.05, respectively. We compare this inferred FBE N(z) distribution to the predictions from three generic faint galaxy models: dwarf dominated (no evolution), pure luminosity evolution, and evolving dwarfs. The inferred FBE N(z) distribution strongly supports a hybrid evolving dwarf--rich model wherein a large population of dwarfs present at z=0.5 has subsequently faded to obscurity. The total integrated number density of dwarfs (down to M_{B}=-11) is estimated to be a factor of 20 times greater than that of E---Sc galaxies and the estimated fading to be 1.0 < \\Delta m < 1.4 mags. Thus, the dwarf population is estimated to be responsible for ~30% of the luminosity density locally, rising to ~57% at z=0.5.

  17. arinc research corporation: Topics by E-print Network

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

    examines how firm-level corporate expenditure represented by R&D, capital expenditure (CAPEX) and selling, general and administrative (SGA) costs responds to stock price...

  18. Corporate Clean Energy Investment Trends in Brazil, China, India...

    Open Energy Info (EERE)

    Jump to: navigation, search Name Corporate Clean Energy Investment Trends in Brazil, China, India and South Africa AgencyCompany Organization Carbon Disclosure Project...

  19. Corn Belt Energy Corporation- Residential Energy Efficiency Rebate Program

    Broader source: Energy.gov [DOE]

    Corn Belt Energy Corporation (CBEC), in association with the Wabash Valley Power Association, provides its customers with the "Power Moves" energy efficiency rebate program. Through this program,...

  20. Microsoft Word - EM QA Corporate Board Meeting Minutes - Oct...

    Office of Environmental Management (EM)

    th Environmental Management Quality Assurance Corporate Board Meeting Minutes October 27, 2014 - Nevada Site Office Page 1 of 10 Voting Board Members in Attendance: Randy Kay -...

  1. Alternative Energy Projects by Rural Electric Membership Corporations (Indiana)

    Broader source: Energy.gov [DOE]

    This legislation encourages the development of alternative energy projects using clean or renewable resources by rural electric membership corporations. The section establishes the Office of...

  2. 2008_Transition_Corporate_Overview_Book_One.pdf | Department...

    Broader source: Energy.gov (indexed) [DOE]

    2008TransitionCorporateOverviewBookOne.pdf More Documents & Publications DOE Transition Documents - 2008 DOE Organization Chart - May 2, 2014 DOE Organization Chart - October...

  3. Electric, Street Railway, and Gas Corporations (South Dakota)

    Broader source: Energy.gov [DOE]

    This legislation contains provisions pertaining to a corporation formed for the purpose of constructing, maintaining and operating a street railway or railways; generating, transmitting or...

  4. Southwest Gas Corporation- Residential and Builder Efficiency Rebate Program (Arizona)

    Broader source: Energy.gov [DOE]

    Southwest Gas Corporation (SWG) offers rebates to residential customers in Arizona who purchase and install energy efficient natural gas tankless water heaters, clothes dryers, windows, attic...

  5. Citizens Electric Corporation- Residential Energy Efficiency Rebate Program

    Broader source: Energy.gov [DOE]

    Citizens Electric Corporation offers rebates and price reductions to its residential customers for purchasing and installing energy efficient equipment. Eligible equipment and measures include a...

  6. Southwest Gas Corporation- Residential Energy Efficiency Rebate Program

    Broader source: Energy.gov [DOE]

    Southwest Gas Corporation (SWG) offers rebates to residential customers in Nevada who purchase energy efficient natural gas tankless water heaters, clothes dryers, windows and smart low-flow...

  7. EERE Partner Testimonials- Robert Gleason, Capstone Turbine Corporation

    Broader source: Energy.gov [DOE]

    Robert Gleason, Senior Vice President of Product Development for Capstone Turbine Corporation describes the benefits of a strategic partnership with the U.S. Department of Energy.

  8. azure dynamics corporation: Topics by E-print Network

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

    Coverage of Students on Medically Necessary Leave of Absence 116 Navneet Gulati Eaton Corporation, Engineering Websites Summary: autonomy to human-scale power-comparable...

  9. EERE Partner Testimonials- Darren Jamison, Capstone Turbine Corporation

    Broader source: Energy.gov [DOE]

    Darren Jamison, President and CEO of Capstone Turbine Corporation, shares his experience of partnering with the U.S. Department of Energy.

  10. Mainzer taps Gendron, Ehli to lead Power and Corporate Strategy

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

    Mainzer-taps-Gendron-Ehli-to-lead-Power-and-Corporate-Strategy Sign In About | Careers | Contact | Investors | bpa.gov Search News & Us Expand News & Us Projects & Initiatives...

  11. Preliminary Notice of Violation, Fluor Daniel Fernald Corporation...

    Broader source: Energy.gov (indexed) [DOE]

    July 29, 1997 Issued to Fluor Daniel Fernald Corporation related to Corrective Actions Implementation Deficiencies at the Fernald Environmental Management Project, (EA-97-05) On...

  12. Testimonials- Partnerships in Battery Technologies- Capstone Turbine Corporation

    Broader source: Energy.gov [DOE]

    Robert Gleason, Senior Vice President of Product Development for Capstone Turbine Corporation describes the benefits of a strategic partnership with the U.S. Department of Energy.

  13. Testimonials- Partnerships in R&D- Capstone Turbine Corporation

    Broader source: Energy.gov [DOE]

    Darren Jamison, President and CEO of Capstone Turbine Corporation, shares his experience of partnering with the U.S. Department of Energy.

  14. Microsoft Word - EM QA Corporate Board Meeting Minutes - February...

    Office of Environmental Management (EM)

    th Environmental Management Quality Assurance Corporate Board Meeting Minutes February 11, 2014 - Teleconference Page 1 of 8 Voting Board Members in Attendance: Randy Kay - Idaho...

  15. Southwest Gas Corporation- Commercial Energy Efficient Equipment Rebate Program

    Broader source: Energy.gov [DOE]

    Southwest Gas Corporation (SWG) offers rebates to commercial customers in Nevada who purchase energy efficient natural gas equipment. Eligible equipment includes clothes washers, storage water...

  16. Southwest Gas Corporation- Commercial High-Efficiency Equipment Rebate Program

    Broader source: Energy.gov [DOE]

    Southwest Gas Corporation (SWG) offers rebates to commercial customers in Arizona who purchase energy efficient natural gas equipment. Eligible equipment includes natural gas storage and tankless...

  17. Accounting for Taste: Board Member Preferences and Corporate Policy Choices

    E-Print Network [OSTI]

    Richardson, Scott

    2003-05-23T23:59:59.000Z

    This paper explores whether firms that share common directors also pursue similar corporate policies. Using a sample of 885 U.S. firms with common directors, we find ...

  18. TANGENTIAL VELOCITY OF THE DARK MATTER IN THE BULLET CLUSTER FROM PRECISE LENSED IMAGE REDSHIFTS

    SciTech Connect (OSTI)

    Molnar, Sandor M. [Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei 10617, Taiwan (China); Broadhurst, Tom [Fisika Teorikoa, Zientzia eta Teknologia Fakultatea, Euskal Herriko Unibertsitatea UPV/EHU, 644 Posta Kutxatila, E-48080 Bilbao (Spain); Umetsu, Keiichi [Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei 10617, Taiwan (China); Zitrin, Adi [Universitaet Heidelberg, Zentrum fuer Astronomie, Institut fuer Theoretische Astrophysik, Philosophenweg 12, D-69120 Heidelberg (Germany); Rephaeli, Yoel; Shimon, Meir, E-mail: sandor@phys.ntu.edu.tw [School of Physics and Astronomy, Tel Aviv University, Tel Aviv 69978 (Israel)

    2013-09-01T23:59:59.000Z

    We show that the fast-moving component of the ''Bullet Cluster'' (1E0657-56) can induce potentially resolvable redshift differences between multiply lensed images of background galaxies. This moving cluster effect, due to the tangential peculiar velocity of the lens, can be expressed as the scalar product of the lensing deflection angle with the tangential velocity of the mass components; the effect is maximal for clusters colliding in the plane of the sky with velocities boosted by their mutual gravity. The Bullet Cluster is likely to be the best candidate for the first measurement of this effect due to the large collision velocity and because the lensing deflection and the cluster fields can be calculated in advance. We derive the deflection field using multiply lensed background galaxies detected with the Hubble Space Telescope. The velocity field is modeled using self-consistent N-body/hydrodynamical simulations constrained by the observed X-ray and gravitational lensing features of this system. We predict that the triply lensed images of systems ''G'' and ''H'' straddling the critical curve of the bullet component will show the largest frequency shifts up to {approx}0.5 km s{sup -1}. These shifts are within the range of the Atacama Large Millimeter/Submillimeter Array for molecular emission, and are near the resolution limit of the new generation high-throughput optical-IR spectrographs. The detection of this effect measures the tangential motion of the subclusters directly, thereby clarifying the tension with {Lambda}CDM, which is inferred from the gas motion less directly. This method may be extended to smaller redshift differences using the Ly{alpha} forest toward QSOs lensed by more typical clusters of galaxies. More generally, the tangential component of the peculiar velocities of clusters derived by our method complements the radial component determined by the kinematic Sunyaev-Zel'dovich effect, providing a full three-dimensional description of velocities.

  19. Corporate social responsibility and its impact on the corporate decision-making process for university undergraduate research fellows

    E-Print Network [OSTI]

    Bain, Joseph E

    2013-02-22T23:59:59.000Z

    corporations can have a detrimental effect by allowing the pilfering of societal resources by greedy corporate executives. On the other hand, limited economic resources disallow the corporation to meet every demand of society without infringing on its... stakeholders are perceived to be stakeholders whom the firm depends on to operate efficiently; while, normative stakeholders possess moral claims on the firm but do not exercise a substantive influence over the firm's operations. Welcomer (2002) argues, "the...

  20. Chapter 2Chapter 2 A Complete CorporateA Complete Corporate

    E-Print Network [OSTI]

    Schubart, Christoph

    average cost of capital (WACC) Estimate expected future free cash flows (FCF)(FCF) Find value of company investors called the weightedinvestors--called the weighted average cost of capital (WACC) DES Chapter 2 13 #12;Steps in the corporate value model Determine weighted average cost of capitalDetermine weighted

  1. Developing a Corporate Water Management Strategy 

    E-Print Network [OSTI]

    Tutterow, V.

    2015-01-01T23:59:59.000Z

    stream_source_info ESL-IE-15-06-22.pdf.txt stream_content_type text/plain stream_size 21539 Content-Encoding UTF-8 stream_name ESL-IE-15-06-22.pdf.txt Content-Type text/plain; charset=UTF-8 Developing a Corporate Water... Management Strategy Vestal Tutterow Senior Technical Consultant Jackson Stubbs Senior Analyst Project Performance Company McLean, VA Eoin O’Driscoll, PhD Energy Analyst ABSTRACT Industrial facilities universally rely on water as a raw...

  2. Special features of corporation accounting in Texas

    E-Print Network [OSTI]

    Davis, Garnett Stant

    1943-01-01T23:59:59.000Z

    ') Excess of Depletion Reserve over Leasehold Costs. The analysis of changes in taxable capital consists of a combined income and surplus statement, together with any additions or deductions from capital stock that may have taken place withLn the year... Forfeited Stock To record forfeitup of stock and previous payments. 500. 00 200i00 500. 00 200. 00 300. 00 200 00 tchell v. Porter, Tex. Civ. App. , 223 S. S. 1/7. Hildebrand, Texas Corporations, Vol. 1, p. 111. Broad, Some Comments on Surplus...

  3. First Gen Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnualPropertyd8c-a9ae-f8521cbb8489 NoEuropeStrat.pdfInactive Jump to:FinnishFireballGen Corporation

  4. Corporate Culture | National Nuclear Security Administration

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625govInstrumentstdmadapInactiveVisitingContract Management Fermi Site Office (FSO)Corporate Culture | National

  5. Corporate Fellows Council | ornl.gov

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625govInstrumentstdmadapInactiveVisitingContract Management Fermi Site Office (FSO)Corporate Culture |

  6. Environmental Credit Corporation ECC | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual SiteofEvaluating A PotentialJump to:EmminolEntergy ArkansasEnvironmental Credit Corporation

  7. GainSpan Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual SiteofEvaluating A PotentialJumpGermanFifeGEXA Corp. (New Jersey)GainSpan Corporation Jump to:

  8. Corporate Operating Experience Program | Department of Energy

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33 111 1,613PortsmouthBartlesvilleAbout » Contact Us ContactPractices in IndianDebate thCorporate

  9. Wanxiang America Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere IRaghuraji Agro IndustriesTown ofNationwide Permit webpageWalthall County,Wanxiang America Corporation Jump

  10. China Technology Development Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand JumpConceptual Model, click here.TelluricPower International New Energy Holding Ltd Place:Corporation

  11. Sierra Energy Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere IRaghuraji Agro Industries Pvt LtdShawangunk, New York:SiG Solar GmbH Jump to:Sierra Energy Corporation Place:

  12. Wisconsin Energy Conservation Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:Ezfeedflag JumpID-fTriWildcat 1 Wind Project Jump to:WilsonIIaEnergy Conservation Corporation

  13. LANL named 2010 top corporate volunteer organization

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645U.S. DOE Office of Science (SC)Integrated Codes |Is Your Home as ReadyAppointedKyungmin2010 top corporate volunteer

  14. NewPage Corporation | Department of Energy

    Energy Savers [EERE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directed offOCHCO2:Introduction toManagement ofConverDynNet-ZeroNew Wave Power ProjectTomNewPage Corporation

  15. Project Resources Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to: navigation,Pillar Group BV Jump to: navigation,PowerInformationOpenProeInyoCorporation

  16. Iosil Energy Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are8COaBulkTransmissionSitingProcess.pdfGetecGtelInterias Solar Energy Jump to:IESIntervalIosil Energy Corporation Jump

  17. IST Energy Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to: navigation, search OpenEIHesperia,IDGWP Wind Farm Jump to:ILab IncubatorISE Corporation

  18. Hy9 Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are8COaBulkTransmissionSitingProcess.pdfGetecGtel JumpCounty, Texas: EnergyHy9 Corporation Jump to: navigation, search

  19. Corporate Tax Credit | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual Siteof EnergyInnovationinConcentratingEnergyCoosa Valley ElectricCornwall LightCorporate

  20. StarSolar Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere IRaghuraji Agro Industries Pvt LtdShawangunk,SoutheastSt. Francis(Redirected fromStarSolar Corporation Jump

  1. Corporate International Operations | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand JumpConceptual Model, clickInformationNew|Core Analysis At Geysers|Cornwall,CorporateInternational

  2. Covanta Holding Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand JumpConceptual Model, clickInformationNew|Core AnalysisCouncil, Idaho: EnergyCovantaIncCorporation

  3. Sumco Techxiv Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnualProperty Edit with formSoutheastern IL ElecStrategicStories HomeSumco Techxiv Corporation Jump

  4. Apollo Energy Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:Ezfeedflag JumpID-fTriWildcatAntrim County, Michigan: EnergySalient of Normal FaultCorporation

  5. ArchRock Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:Ezfeedflag JumpID-fTriWildcatAntrim County,Delhi (NCT),Arborview CapitalArchRock Corporation

  6. ClimeCo Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnualProperty EditCalifornia:PowerCER.png El CER esDatasetCityFund JumpClimeCo Corporation Jump to:

  7. BioJet Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand Jump to:EzfeedflagBiomass ConversionsSouth Carolina:EnergyPark,BioJet Corporation Jump to: navigation,

  8. Ruihao Corporation Group | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere IRaghuraji Agro Industries Pvt Ltd Jump to:Roscommon County,Vermont: Energy ResourcesRuihao Corporation Group

  9. Ruihua Construction Corporation RHC | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov YouKizildere IRaghuraji Agro Industries Pvt Ltd Jump to:Roscommon County,Vermont: Energy ResourcesRuihao Corporation

  10. Arrowhead Research Corporation | Open Energy Information

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual Siteof EnergyInnovation in Carbon Capture andsoftware andSolarResearch Corporation Place:

  11. Tax Savings as a Provision of Corporate Welfare is a State-Corporate Crime When it Becomes Socially Injurious

    E-Print Network [OSTI]

    Nery, Annebelle

    2010-01-01T23:59:59.000Z

    From their definition and further research, the theory wasTraditional Definitions of Crime Criminology Theory: Theintegrated theory of state corporate crime, definitions of

  12. Software & Services Group Developer Products Division Copyright 2011, Intel Corporation. All rights reserved.

    E-Print Network [OSTI]

    California at Berkeley, University of

    Software & Services Group Developer Products Division Copyright© 2011, Intel Corporation. All & Services Group Developer Products Division Copyright© 2011, Intel Corporation. All rights reserved. *Other Division Copyright© 2011, Intel Corporation. All rights reserved. *Other brands and names are the property

  13. Dead Hand and No Hand Pills: Precommitment Strategies in Corporate Law

    E-Print Network [OSTI]

    Bainbridge, Stephen M

    2003-01-01T23:59:59.000Z

    Decisionmaking in Corporate Governance, 55 V AND . L. R EV .Dooley, Two Models of Corporate Governance, 47 B US . L AW .resurgence of the corporate governance issues that dominated

  14. The Shareholder As Ulysses: Some Empirical Evidence on Why Investors in Public Corporations Tolerate Board Governance

    E-Print Network [OSTI]

    Stout, Lynn A.

    2003-01-01T23:59:59.000Z

    default rules of corporate governance at all, they almostThe Means and Ends of Corporate Governance, 97 N W . U. L. Rof the way modern corporate governance actually works. In

  15. Anglo-American Corporate Taxation: Tracing the Common Roots of Divergent Approaches

    E-Print Network [OSTI]

    Bank, Steven A.

    2013-01-01T23:59:59.000Z

    History and the Global Corporate Governance Revolution: Thelength structure of corporate governance, the U.K. continuedarm’s-length form of corporate governance in the U.K. was

  16. Social Impact Management Plans: Innovation in corporate and public policy

    SciTech Connect (OSTI)

    Franks, Daniel M., E-mail: d.franks@uq.edu.au [Centre for Social Responsibility in Mining, The University of Queensland, Sustainable Minerals Institute, St Lucia, Brisbane, Queensland 4072 (Australia); Vanclay, Frank, E-mail: frank.vanclay@rug.nl [Department of Cultural Geography, Faculty of Spatial Sciences, The University of Groningen, P.O. Box 800, 9700 AV Groningen (Netherlands)] [Department of Cultural Geography, Faculty of Spatial Sciences, The University of Groningen, P.O. Box 800, 9700 AV Groningen (Netherlands)

    2013-11-15T23:59:59.000Z

    Social Impact Assessment (SIA) has traditionally been practiced as a predictive study for the regulatory approval of major projects, however, in recent years the drivers and domain of focus for SIA have shifted. This paper details the emergence of Social Impact Management Plans (SIMPs) and undertakes an analysis of innovations in corporate and public policy that have put in place ongoing processes – assessment, management and monitoring – to better identify the nature and scope of the social impacts that might occur during implementation and to proactively respond to change across the lifecycle of developments. Four leading practice examples are analyzed. The International Finance Corporation (IFC) Performance Standards require the preparation of Environmental and Social Management Plans for all projects financed by the IFC identified as having significant environmental and social risks. Anglo American, a major resources company, has introduced a Socio-Economic Assessment Toolbox, which requires mine sites to undertake regular assessments and link these assessments with their internal management systems, monitoring activities and a Social Management Plan. In South Africa, Social and Labour Plans are submitted with an application for a mining or production right. In Queensland, Australia, Social Impact Management Plans were developed as part of an Environmental Impact Statement, which included assessment of social impacts. Collectively these initiatives, and others, are a practical realization of theoretical conceptions of SIA that include management and monitoring as core components of SIA. The paper concludes with an analysis of the implications for the practice of impact assessment including a summary of key criteria for the design and implementation of effective SIMPs. -- Highlights: • Social impact management plans are effective strategies to manage social issues. • They are developed in partnership with regulatory agencies, investors and community. • SIMPs link assessment to ongoing management and address social and community issues. • SIMPs clarify responsibilities in the management of impacts, opportunities and risks. • SIMPs demonstrate a shift to include management as a core component of SIA practice.

  17. Interpreting the unresolved intensity of cosmologically redshifted line radiation

    E-Print Network [OSTI]

    Switzer, Eric R; Masui, Kiyoshi W; Pen, Ue-Li; Voytek, Tabitha C

    2015-01-01T23:59:59.000Z

    Intensity mapping experiments survey the spectrum of diffuse line radiation rather than detect individual objects at high signal-to-noise. Spectral maps of unresolved atomic and molecular line radiation contain three-dimensional information about the density and environments of emitting gas, and efficiently probe cosmological volumes out to high redshift. Intensity mapping survey volumes also contain all other sources of radiation at the frequencies of interest. Continuum foregrounds are typically ~10^2-10^3 times brighter than the cosmological signal. The instrumental response to bright foregrounds will produce new spectral degrees of freedom that are not known in advance, nor necessarily spectrally smooth. The intrinsic spectra of foregrounds may also not be well-known in advance. We describe a general class of quadratic estimators to analyze data from single-dish intensity mapping experiments, and determine contaminated spectral modes from the data itself. The key attribute of foregrounds is not that they ...

  18. Weighing black holes from zero to high redshift

    E-Print Network [OSTI]

    A. Marconi; D. Axon; R. Maiolino; T. Nagao; P. Pietrini; A. Robinson; G. Torricelli

    2008-09-02T23:59:59.000Z

    The application of the virial theorem provides a tool to estimate supermassive black hole (BH) masses in large samples of active galactic nuclei (AGN) with broad emission lines at all redshifts and luminosities, if the broad line region (BLR) is gravitationally bound. In this paper we discuss the importance of radiation forces on BLR clouds arising from the deposition of momentum by ionizing photons. Such radiation forces counteract gravitational ones and, if not taken into account, BH masses can be severely underestimated. We provide virial relations corrected for the effect of radiation pressure and we discuss their physical meaning and application. If these corrections to virial masses, calibrated with low luminosity objects, are extrapolated to high luminosities then the BLRs of most quasars might be gravitationally unbound. The importance of radiation forces in high luminosity objects must be thoroughly investigated to assess the reliability of quasar BH masses.

  19. Enrichment of the High-Redshift IGM by Galactic Winds

    E-Print Network [OSTI]

    A. Aguirre; J. Schaye; L. Hernquist; D. Weinberg; N. Katz; J. Gardner

    2001-09-17T23:59:59.000Z

    This paper discusses a semi-numerical method of investigating the enrichment of the intergalactic medium by galactic winds. We find that most galaxies at z >~ 3 should be driving winds, and that (if these winds are similar to those at low-z) these winds should escape to large distances. Our calculations -- which permit exploration of a large region of model parameter space -- indicate that the wind velocity, the mass of the wind-driving galaxies, the fraction of ambient material entrained, and the available time (between wind launch and the observed redshift) all affect wind propagation significantly; other physical effects can be important but are sub-dominant. We find that under reasonable assumptions, the enrichment by 3 enrichment is compatible with the intergalactic medium's detailed metal distribution or relative quiescence.

  20. COSMIC RAYS CAN DRIVE STRONG OUTFLOWS FROM GAS-RICH HIGH-REDSHIFT DISK GALAXIES

    SciTech Connect (OSTI)

    Hanasz, M.; Kowalik, K.; Wólta?ski, D. [Centre for Astronomy, Nicolaus Copernicus University, Faculty of Physics, Astronomy and Informatics, Grudziadzka 5, PL-87100 Toru? (Poland)] [Centre for Astronomy, Nicolaus Copernicus University, Faculty of Physics, Astronomy and Informatics, Grudziadzka 5, PL-87100 Toru? (Poland); Lesch, H. [Universitäts-Sternwarte München, Scheinerstr. 1, D-81679 München (Germany)] [Universitäts-Sternwarte München, Scheinerstr. 1, D-81679 München (Germany); Naab, T. [Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85741 Garching bei München (Germany)] [Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, D-85741 Garching bei München (Germany); Gawryszczak, A., E-mail: mhanasz@astri.uni.torun.pl [Pozna? Supercomputing and Networking Centre, ul. Noskowskiego 10, PL-61-704 Pozna? (Poland)

    2013-11-10T23:59:59.000Z

    We present simulations of the magnetized interstellar medium (ISM) in models of massive star-forming (40 M {sub ?} yr{sup –1}) disk galaxies with high gas surface densities (?{sub gas} ? 100 M {sub ?} pc{sup –2}) similar to observed star-forming high-redshift disks. We assume that type II supernovae deposit 10% of their energy into the ISM as cosmic rays (CRs) and neglect the additional deposition of thermal energy or momentum. With a typical Galactic diffusion coefficient for CRs (3 × 10{sup 28} cm{sup 2} s{sup –1}), we demonstrate that this process alone can trigger the local formation of a strong low-density galactic wind maintaining vertically open field lines. Driven by the additional pressure gradient of the relativistic fluid, the wind speed can exceed 10{sup 3} km s{sup –1}, much higher than the escape velocity of the galaxy. The global mass loading, i.e., the ratio of the gas mass leaving the galactic disk in a wind to the star formation rate, becomes of order unity once the system has settled into an equilibrium. We conclude that relativistic particles accelerated in supernova remnants alone provide a natural and efficient mechanism to trigger winds similar to observed mass-loaded galactic winds in high-redshift galaxies. These winds also help in explaining the low efficiencies for the conversion of gas into stars in galaxies, as well as the early enrichment of the intergalactic medium with metals. This mechanism may be at least of similar importance to the traditionally considered momentum feedback from massive stars and thermal and kinetic feedback from supernova explosions.

  1. Aurora Organic Dairy Phase III: Corporate Sustainability Report

    E-Print Network [OSTI]

    Edwards, Paul N.

    Aurora Organic Dairy Phase III: Corporate Sustainability Report Rosemary Lapka, Neesha Modi, Lauren Start and David Weinglass Report No. CSS11-07 April 19, 2011 #12;Aurora Organic Dairy Phase III Keoleian, Professor #12;Document Description AURORA ORGANIC DAIRY PHASE III: CORPORATE SUSTAINABILITY

  2. Industrial Engineering 361 Six Sigma Making Corporations and

    E-Print Network [OSTI]

    Vardeman, Stephen B.

    Industrial Engineering 361 Six Sigma ­ Making Corporations and Stockholders... Kim Knuth Grant in the late 1980's. The term "Six Sigma" came to identify a popular form of corporate improvement://www.public.iastate.edu/~vardeman/stat531/sixsigma.pdf). Before we began research, we questioned the importance of Six Sigma and were

  3. Classifying Web content for a corporate digital library Ian Thurlow

    E-Print Network [OSTI]

    Haddadi, Hamed

    Classifying Web content for a corporate digital library Ian Thurlow BT Abstract: The integration of relevant Web content into corporate digital libraries is expected to be of significant benefit when tools. The integration of Web content into a digital library, however, raises some concerns with regard

  4. Nolij Corporation Proprietary & Confidential Information Release Notes for Nolij Web

    E-Print Network [OSTI]

    Escher, Christine

    Nolij Corporation Proprietary & Confidential Information Release Notes for Nolij Web Release 6.3.x Web Release 6.3.x Copyright © 2010 - 2011, Nolij Corporation. All rights reserved. Revised 02Release Notes for Nolij Web Release 6.3.x Introduction These release notes provide information about new

  5. Copyright 1997 by Rational Software Corporation Analysis and Design

    E-Print Network [OSTI]

    Mylopoulos, John

    Page 1 Copyright © 1997 by Rational Software Corporation Analysis and Design with UML Page 2 Copyright © 1997 by Rational Software Corporation Agenda n Benefits of Visual Modeling n History of the UML n Visual Modeling with UML n The Rational Iterative Development Process #12;Page 3 Copyright © 1997

  6. High Redshift Gamma-Ray Bursts: Observational Signatures of Superconducting Cosmic Strings?

    E-Print Network [OSTI]

    K. S. Cheng; Yun-Wei Yu; T. Harko

    2010-06-11T23:59:59.000Z

    The high-redshift gamma-ray bursts (GRBs), GRBs 080913 and 090423, challenge the conventional GRB progenitor models by their short durations, typical for short GRBs, and their high energy releases, typical for long GRBs. Meanwhile, the GRB rate inferred from high-redshift GRBs also remarkably exceeds the prediction of the collapsar model, with an ordinary star formation history. We show that all these contradictions could be eliminated naturally, if we ascribe some high-redshift GRBs to electromagnetic bursts of superconducting cosmic strings. High-redshift GRBs could become a reasonable way to test the superconducting cosmic string model, because the event rate of cosmic string bursts increases rapidly with increasing redshifts, whereas the collapsar rate decreases.

  7. Corporate governance reform in a developing country : the case of Bangladesh 

    E-Print Network [OSTI]

    Sobhan, Md. Abdus

    2014-07-02T23:59:59.000Z

    Bangladesh reformed its corporate governance by adopting Bangladesh Corporate Governance Guidelines-2006 (the BCGG-2006 hereafter) due to pressures from international financial institutions (IFIs). However, there is huge ...

  8. IS THE TAIL WAGGING THE DOG? AN EMPIRICAL ANALYSIS OF CORPORATE CARBON FOOTPRINTS AND FINANCIAL PERFORMANCE

    E-Print Network [OSTI]

    Delmas, Magali A; Nairn-Birch, Nicholas S.

    2011-01-01T23:59:59.000Z

    The importance of carbon footprint estimation boundaries.ANALYSIS OF CORPORATE CARBON FOOTPRINTS AND FINANCIALANALYSIS OF CORPORATE CARBON FOOTPRINTS AND FINANCIAL

  9. Plasma Assisted Catalysis System for NOx Reduction

    Broader source: Energy.gov (indexed) [DOE]

    2 NOXTECH NOXTECH PLASMA ASSISTED CATALYSIS SYSTEM FOR NOx REDUCTION BY NOXTECH With the Support & Cooperation of DOE Noxtech, Inc. *Delaware Corporation registered to do business...

  10. Comprehensive Renewable Energy Feasibility Study for Sealaska Corporation

    SciTech Connect (OSTI)

    Robert Lynette; John Wade: Larry Coupe

    2006-06-30T23:59:59.000Z

    The purposes of this project were: (1) to conduct a comprehensive feasibility study to determine the potential sustainability of wind and/or small hydroelectric power plants on Southeast Alaska native village lands, and (2) to provide the villages with an understanding of the requirements, costs, and benefits of developing and operating wind or small hydroelectric power plants. The program was sponsored by the Tribal Energy program, Office of Energy Efficiency and Renewable Energy, US Department of Energy. The Contractor was Sealaska Corporation, the Regional Native Corporation for Southeast Alaska that includes 12 village/urban corporations. Most villages are isolated from any central electric transmission and use diesel-electric systems for power generation, making them prime candidates for deploying renewable energy sources. Wind Energy - A database was assembled for all of the candidate sites in SE Alaska, including location, demographics, electricity supply and demand, existing and planned transmission interties with central generation, topographical maps, macro wind data, and contact personnel. Field trips were conducted at the five candidate villages that were deemed most likely to have viable wind resources. Meetings were held with local village and utility leaders and the requirements, costs, and benefits of having local renewable energy facilities were discussed. Two sites were selected for anemometry based on their needs and the probability of having viable wind resources – Yakutat and Hoonah. Anemometry was installed at both sites and at least one year of wind resource data was collected from the sites. This data was compared to long-term data from the closest weather stations. Reports were prepared by meteorologist John Wade that contains the details of the measured wind resources and energy production projections. Preliminary financial analysis of hypothetical wind power stations were prepared to gauge the economic viability of installing such facilities at each site. The average wind resources measured at Yakutat at three sites were very marginal, with an annual average of 4.0 mps (9 mph) at 60 meters above ground level. At Hoonah, the average wind resources measured on the 1,417 ft elevation ridge above the village were very low, with a six-month average of 3.9 mps (8.7 mph) at 60 meters above ground level. The wind resources at both sites were not sufficient to justify installation of wind turbines. In summary, although there are several known windy spots in SE Alaska (e.g., Skagway), we were not able to identify any isolated Native American villages that utilize diesel-electric power generation that have commercially viable wind resources. Small Hydroelectric - The study focused on the communities associated with Sealaska Corporation that use diesel-electric for electricity and have a potential for hydroelectric power generation. Most of them have had at least an assessment of hydroelectric potential, and a few have had feasibility studies of potential hydroelectric projects. Although none of the sites examined are financially viable without substantial grant funding, Hoonah, Kake, and Yakutat appear to have the best potential for new hydro facilities.

  11. The effect of a corporate name change related to a change in corporate image upon a firm's stock price

    E-Print Network [OSTI]

    DeFanti, Mark P.

    2009-06-02T23:59:59.000Z

    primary research questions. First, what is the effect of a CNC related to a change in corporate image, as opposed to a change in corporate entity (e.g., acquisition), on a firm’s stock price? Second, what is the effect of a major change versus a minor...

  12. CU-Boulder Faculty Awards Campus, School/College, and System Level

    E-Print Network [OSTI]

    Corporation Faculty Community Service Award CU System, Office of Academic Affairs https://www.cu.edu/content/chase-corporation/teaching.html February All Faculty Eaton Faculty Awards for Outstanding Achievement CU-Boulder, Center for Humanities

  13. A FAST FLARE AND DIRECT REDSHIFT CONSTRAINT IN FAR-ULTRAVIOLET SPECTRA OF THE BLAZAR S5 0716+714

    SciTech Connect (OSTI)

    Danforth, Charles W.; Nalewajko, Krzysztof; France, Kevin; Keeney, Brian A., E-mail: danforth@casa.colorado.edu [CASA, Department of Astrophysical and Planetary Sciences, University of Colorado, 389-UCB, Boulder, CO 80309 (United States)

    2013-02-10T23:59:59.000Z

    The BL Lacertae object S5 0716+714 is one of the most studied blazars on the sky due to its active variability and brightness in many bands, including very-high-energy gamma rays. We present here two serendipitous results from recent far-ultraviolet spectroscopic observations by the Cosmic Origins Spectrograph onboard the Hubble Space Telescope (HST). First, during the course of our 7.3 hr HST observations, the blazar increased in flux rapidly by {approx}40% (-0.45 mag hr{sup -1}) followed by a slower decline (+0.36 mag hr{sup -1}) to previous FUV flux levels. We model this flare using asymmetric flare templates and constrain the physical size and energetics of the emitting region. Furthermore, the spectral index of the object softens considerably during the course of the flare from {alpha}{sub {nu}} Almost-Equal-To -1.0 to {alpha}{sub {nu}} Almost-Equal-To -1.4. Second, we constrain the source redshift directly using the {approx}30 intervening absorption systems. A system at z = 0.2315 is detected in Ly{alpha}, Ly{beta}, O VI, and N V and defines the lower bound on the source redshift. No absorbers are seen in the remaining spectral coverage (0.2315 < z {sub Ly{alpha}} {approx}< 0.47) and we set a statistical upper bound of z < 0.322 (95% confidence) on the blazar. This is the first direct redshift limit for this object and is consistent with literature estimates of z = 0.31 {+-} 0.08 based on the detection of a host galaxy.

  14. Materials Analyst -Federal-Mogul Corporation -Skokie Plant The Material Analyst is responsible for procuring materials to support the manufacturing

    E-Print Network [OSTI]

    Heller, Barbara

    Materials Analyst - Federal-Mogul Corporation - Skokie Plant The Material Analyst is responsible for procuring materials to support the manufacturing function by maintaining raw material levels that ensure and utilize inventory system to analyze material requirements to ensure proper inventory levels. 2. Place

  15. A NEW POPULATION OF HIGH-REDSHIFT SHORT-DURATION GAMMA-RAY BURSTS E. Berger,1,2,3

    E-Print Network [OSTI]

    Sheppard, Scott S.

    A NEW POPULATION OF HIGH-REDSHIFT SHORT-DURATION GAMMA-RAY BURSTS E. Berger,1,2,3 D. B. Fox,4 P. A The redshift distribution of the short-duration gamma-ray bursts (GRBs) is a crucial, but currently fragmentary rays: bursts Online material: color figures 1. INTRODUCTION The redshift distribution of the short

  16. Restframe I-band Hubble diagram for type Ia supernovae up to redshift z ~; 0.5

    E-Print Network [OSTI]

    2005-01-01T23:59:59.000Z

    up to redshift z ? 0.5 ? S. Nobili 1,2 , R. Amanullah 2 , G.up to redshift z ? 0.5 Filippenko, A.V. , Richmond, M.W. ,Ia supernovae up to redshift z ? 0.5 ported by cross-cutting

  17. The Low-Redshift Lyman Alpha Forest toward PKS 0405-123

    E-Print Network [OSTI]

    G. M. Williger; S. R. Heap; R. J. Weymann; R. Dave; E. Ellingson; R. F. Carswell; T. M. Tripp; E. B. Jenkins

    2005-08-31T23:59:59.000Z

    We present STIS 7km/s resolution data of the Ly-a forest toward PKS0405-123 (z=0.574). We make two samples. The strong sample (60 systems) has column density logNHI>13.3 over 0.00213.1 at 0.020velocity from HI. The strong sample Doppler parameters show =47+-22km/s; for the weak, =44+-21km/s. Line blending and s/n effects likely inflate b. The redshift density dN/dz is consistent with previous, lower resolution results for logNHI>14.0. For 13.113.3, consistent with a numerical model. There is a void in the strong sample at 0.0320radial velocity correlations for Delta v 13.5-14.0. The strength is similar to that of the galaxy-galaxy correlation for our sample, implying that such Ly-a systems have mass log M/Msun= 11.3+1.0-0.6. Including lower column density systems in the sample shows correlations only out to Delta v <125km/s, as would be expected for smaller density perturbations. Galaxy counts and local HI column density appear correlated, peaking at ~5000km/s. We also give column densities for Galactic species. (Abridged)

  18. Paper to be presented at IEEE High Assurance Softwar Software Engineering, Nov. 1999, DC. UML--Based Analysis of Embedded Systems

    E-Print Network [OSTI]

    Cheng, Betty H.C.

    ­96­1­0298, managed by Air Force's Rome Laboratories, and Eaton Corporation. veloping and modeling embedded systems

  19. EA-1472: Commercial Demonstration fo the Low Nox Burner/Separated Over-Fire Air (LNB/SOFA) Integration System Emission Reduction Technology, Holcolm Station, Sunflower Electric Power Corporation Finnety County, Kansas

    Broader source: Energy.gov [DOE]

    The DOE has prepared an Environmental Assessment (EA), to analyze the potential impacts of the commercial application of the Low-NOx Burner/Separated Over-Fire Air (LNB/SOFA) integration system to achieve nitrogen oxide (NOx) emissions reduction at Sunflower’s Holcomb Unit No. 1 (Holcomb Station), located near Garden City, in Finney County, Kansas. The Holcomb Station would be modified in three distinct phases to demonstrate the synergistic effect of layering NOx control technologies.

  20. Wise detections of known QSOs at redshifts greater than six

    SciTech Connect (OSTI)

    Blain, Andrew W. [Physics and Astronomy, University of Leicester, 1 University Road, Leicester LE1 7RH (United Kingdom); Assef, Roberto; Stern, Daniel; Tsai, Chao-Wei; Eisenhardt, Peter [Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 (United States); Bridge, Carrie [California Institute of Technology, 249-17, Pasadena, CA 91125 (United States); Benford, Dominic [Goddard Space Flight Center, Greenbelt, MD 20771 (United States); Jarrett, Tom [Astronomy Department, University of Cape Town (South Africa); Cutri, Roc [Infrared Processing and Analysis Center, California Institute of Technology, MS100-22, Pasadena, CA 91125 (United States); Petty, Sara [Virginia Tech, Department of Physics MC 0435, 910 Drillfield Drive, Blacksburg, VA 24061 (United States); Wu, Jingwen; Wright, Edward L., E-mail: ab520@le.ac.uk [Division of Astronomy and Astrophysics, University of California, Los Angeles, Physics and Astronomy Building, 430 Portola Plaza, Los Angeles, CA 90095-1547 (United States)

    2013-12-01T23:59:59.000Z

    We present WISE All-Sky mid-infrared (IR) survey detections of 55% (17/31) of the known QSOs at z > 6 from a range of surveys: the SDSS, the CFHT-LS, FIRST, Spitzer, and UKIDSS. The WISE catalog thus provides a substantial increase in the quantity of IR data available for these sources: 17 are detected in the WISE W1 (3.4 ?m) band, 16 in W2 (4.6 ?m), 3 in W3 (12 ?m), and 0 in W4 (22 ?m). This is particularly important with Spitzer in its warm-mission phase and no faint follow-up capability at wavelengths longward of 5 ?m until the launch of James Webb Space Telescope (JWST). WISE thus provides a useful tool for understanding QSOs found in forthcoming large-area optical/IR sky surveys using PanSTARRS, SkyMapper, VISTA, DES, and LSST. The rest-UV properties of the WISE-detected and the WISE-non-detected samples differ: the detections have brighter i/z-band magnitudes and redder rest-UV colors. This suggests that a more aggressive hunt for very high redshift QSOs by combining WISE W1 and W2 data with red, observed optical colors could be effective at least for a subset of dusty candidate QSOs. Stacking the WISE images of the WISE-non-detected QSOs indicates that they are, on average, significantly fainter than the WISE-detected examples, and are thus not narrowly missing detection in the WISE catalog. The WISE catalog detection of three of our sample in the W3 band indicates that their mid-IR flux can be detected individually, although there is no stacked W3 detection of sources detected in W1 but not W3. Stacking analyses of WISE data for large active galactic nucleus samples will be a useful tool, and high-redshift QSOs of all types will be easy targets for JWST.

  1. What fraction of stars formed in infrared galaxies at high redshift?

    E-Print Network [OSTI]

    Neil Trentham

    2004-11-18T23:59:59.000Z

    Star formation happens in two types of environment: ultraviolet-bright starbursts (like 30 Doradus and HII galaxies at low redshift and Lyman-break galaxies at high redshift) and infrared-bright dust-enshrouded regions (which may be moderately star-forming like Orion in the Galaxy or extreme like the core of Arp 220). In this work I will estimate how many of the stars in the local Universe formed in each type of environment, using observations of star-forming galaxies at all redshifts at different wavelengths and of the evolution of the field galaxy population.

  2. Quantifying the Cosmic Web in the New Era of Redshift Surveys

    E-Print Network [OSTI]

    Ofer Lahav

    2004-11-03T23:59:59.000Z

    Two main strategies have been implemented in mapping the local universe: whole-sky 'shallow' surveys and 'deep' surveys over limited parts of the sky. The two approaches complement each other in studying cosmography and statistical properties of the Universe. We summarise some results on the power spectrum of fluctuations and Wiener reconstruction of the density field from the 2dF Galaxy Redshift Survey (2dFGRS) of 230,000 redshifts. We then discuss future challenges in quantifying the web of cosmic structure in the on-going redshift surveys.

  3. Galaxy sizes as a function of environment at intermediate redshift from the ESO Distant Cluster Survey

    E-Print Network [OSTI]

    Kelkar, Kshitija; Gray, Meghan E; Maltby, David; Vulcani, Benedetta; De Lucia, Gabriella; Poggianti, Bianca M; Zaritsky, Dennis

    2015-01-01T23:59:59.000Z

    In order to assess whether the environment has a significant effect on galaxy sizes, we compare the mass--size relations of cluster and field galaxies in the $0.4 1$), with early-type/passive galaxies in higher density environments growing earlier. Such dependence disappears at lower redshifts. Therefore, if the reported difference at higher-$z$ is real, the growth of field galaxies has caught up with that of cluster galaxies by $z\\sim1$. Any putative mechanism responsible for galaxy growth has to account for the existence of environmental differences at high redshift and their absence (or weakening) at lower redshifts.

  4. Nonlinear stochastic growth rates and redshift space distortions

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

    Jennings, Elise [Fermi National Accelerator Lab., Batavia, IL (United States); Jennings, David [Imperial College, London (United Kingdom)

    2015-04-09T23:59:59.000Z

    The linear growth rate is commonly defined through a simple deterministic relation between the velocity divergence and the matter overdensity in the linear regime. We introduce a formalism that extends this to a nonlinear, stochastic relation between ? – ? • ?(x,t)/aH and ?. This provides a new phenomenological approach that examines the conditional mean (???), together with the fluctuations of ? around this mean. We measure these stochastic components using N-body simulations and find they are non-negative and increase with decreasing scale from ~10% at kLT?, where fLT is the linear growth rate. This rotation increases with wavenumber, k, and we show that it can be well-described by second order Lagrangian perturbation theory (2LPT) for k LT from two point statistics in redshift space. Given that the relationship between ? and ? is stochastic and nonlinear, this will have implications for the interpretation and precision of fLT extracted using models which assume a linear, deterministic expression.

  5. Deuterium at High Redshifts: Recent Advances and Open Issues

    E-Print Network [OSTI]

    Max Pettini

    2006-01-19T23:59:59.000Z

    Among the light elements created in the Big Bang, deuterium is one of the most difficult to detect but is also the one whose abundance depends most sensitively on the density of baryons. Thus, although we still have only a few positive identifications of D at high redshifts--when the D/H ratio was close to its primordial value--they give us the most reliable determination of the baryon density, in excellent agreement with measures obtained from entirely different probes, such as the anisotropy of the cosmic microwave background temperature and the average absorption of the UV light of quasars by the intergalactic medium. In this review, I relate observations of D/H in distant gas clouds to the large body of data on the local abundance of D obtained in the last few years with the FUSE satellite. I also discuss some of the outstanding problems in light element abundances and consider future prospects for advances in this area.

  6. Cosmic Ray production of Beryllium and Boron at high redshift

    E-Print Network [OSTI]

    Emmanuel Rollinde; David Maurin; Elisabeth Vangioni; Keith A. Olive; Susumu Inoue

    2007-07-13T23:59:59.000Z

    Recently, new observations of Li6 in Pop II stars of the galactic halo have shown a surprisingly high abundance of this isotope, about a thousand times higher than its predicted primordial value. In previous papers, a cosmological model for the cosmic ray-induced production of this isotope in the IGM has been developed to explain the observed abundance at low metallicity. In this paper, given this constraint on the Li6, we calculate the non-thermal evolution with redshift of D, Be, and B in the IGM. In addition to cosmological cosmic ray interactions in the IGM, we include additional processes driven by SN explosions: neutrino spallation and a low energy component in the structures ejected by outflows to the IGM. We take into account CNO CRs impinging on the intergalactic gas. Although subdominant in the galactic disk, this process is shown to produce the bulk of Be and B in the IGM, due to the differential metal enrichment between structures (where CRs originate) and the IGM. We also consider the resulting extragalactic gamma-ray background which we find to be well below existing data. The computation is performed in the framework of hierarchical structure formation considering several star formation histories including Pop III stars. We find that D production is negligible and that a potentially detectable Be and B plateau is produced by these processes at the time of the formation of the Galaxy (z ~ 3).

  7. The Galaxy Population of Low-Redshift Abell Clusters

    E-Print Network [OSTI]

    Barkhouse, Wayne A; Lopez-Cruz, Omar

    2009-01-01T23:59:59.000Z

    We present a study of the luminosity and color properties of galaxies selected from a sample of 57 low-redshift Abell clusters. We utilize the non-parametric dwarf-to-giant ratio (DGR) and the blue galaxy fraction (fb) to investigate the clustercentric radial-dependent changes in the cluster galaxy population. Composite cluster samples are combined by scaling the counting radius by r200 to minimize radius selection bias. The separation of galaxies into a red and blue population was achieved by selecting galaxies relative to the cluster color-magnitude relation. The DGR of the red and blue galaxies is found to be independent of cluster richness (Bgc), although the DGR is larger for the blue population at all measured radii. A decrease in the DGR for the red and red+blue galaxies is detected in the cluster core region, while the blue galaxy DGR is nearly independent of radius. The fb is found not to correlate with Bgc; however, a steady decline toward the inner-cluster region is observed for the giant galaxies....

  8. The Luminosity Function of Low-Redshift Abell Galaxy Clusters

    E-Print Network [OSTI]

    Barkhouse, Wayne A; López-Cruz, Omar

    2007-01-01T23:59:59.000Z

    We present the results from a survey of 57 low-redshift Abell galaxy clusters to study the radial dependence of the luminosity function (LF). The dynamical radius of each cluster, r200, was estimated from the photometric measurement of cluster richness, Bgc. The shape of the LFs are found to correlate with radius such that the faint-end slope, alpha, is generally steeper on the cluster outskirts. The sum of two Schechter functions provides a more adequate fit to the composite LFs than a single Schechter function. LFs based on the selection of red and blue galaxies are bimodal in appearance. The red LFs are generally flat for -22 -18. The blue LFs contain a larger contribution from faint galaxies than the red LFs. The blue LFs have a rising faint-end component (alpha ~ -1.7) for M_Rc > -21, with a weaker dependence on radius than the red LFs. The dispersion of M* was determined to be 0.31 mag, which is comparable to the median measurement uncertainty of 0.38 mag. This suggests that the bright-end of the LF is...

  9. Nonlinear stochastic growth rates and redshift space distortions

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

    Jennings, Elise; Jennings, David

    2015-04-09T23:59:59.000Z

    The linear growth rate is commonly defined through a simple deterministic relation between the velocity divergence and the matter overdensity in the linear regime. We introduce a formalism that extends this to a nonlinear, stochastic relation between ? – ? • ?(x,t)/aH and ?. This provides a new phenomenological approach that examines the conditional mean (???), together with the fluctuations of ? around this mean. We measure these stochastic components using N-body simulations and find they are non-negative and increase with decreasing scale from ~10% at kmore »relation and nonlinearity are more pronounced for halos, M ? 5 x 10¹²Mh?¹, compared to the dark matter at z – 0 and 1. Nonlinear growth effects manifest themselves as a rotation of the mean (???) away from the linear theory prediction –fLT?, where fLT is the linear growth rate. This rotation increases with wavenumber, k, and we show that it can be well-described by second order Lagrangian perturbation theory (2LPT) for k LT from two point statistics in redshift space. Given that the relationship between ? and ? is stochastic and nonlinear, this will have implications for the interpretation and precision of fLT extracted using models which assume a linear, deterministic expression.« less

  10. Comment submitted by Whirlpool Corporation regarding the Energy Star Verification Testing Program

    Broader source: Energy.gov [DOE]

    This document is a comment submitted by Whirlpool Corporation regarding the Energy Star Verification Testing Program

  11. QER- Comment of GenConn Energy on behalf of UIL Holdings Corporation

    Broader source: Energy.gov [DOE]

    Provided are comments of UIL Holdings Corporation on New England Regional Infrastructure Constraints.

  12. STATEMENT OF CONSIDERATIONS REQUEST BY ABENGOA BIOENERGY CORPORATION...

    Broader source: Energy.gov (indexed) [DOE]

    ABENGOA BIOENERGY CORPORATION FOR AN ADVANCE WAIVER OF DOMESTIC AND FOREIGN PATENT RIGHTS UNDER A DOE COOPERATIVE AGREEMENT INITIALLY IDENTIFIED AS GOV WORKS NO. 04-03- CA-79759...

  13. Information Environment and the Investment Decisions of Multinational Corporations

    E-Print Network [OSTI]

    Shroff, Nemit

    This paper examines how the external information environment in which foreign subsidiaries operate affects the investment decisions of multinational corporations (MNCs). We hypothesize and find that the investment decisions ...

  14. Creating an incentive for investor intermediaries to improve corporate governance

    E-Print Network [OSTI]

    Gershkowitz, Todd M

    2006-01-01T23:59:59.000Z

    At the end of the 1980s, there was some speculation that leveraged buyouts (LBOs) would lead to the demise of the public company in favor of privately owned companies after a decade of the market for corporate control ...

  15. Corporate Governance & The UK Split Capital Investment Trust Crisis 

    E-Print Network [OSTI]

    Adams, Andrew T; Angus, Robin

    2005-01-01T23:59:59.000Z

    of corporate governance issues. This paper draws on the results of a survey of investment trust directors and other investment professionals connected with the investment trust industry to examine the lessons to be learned from the crisis. The regulatory...

  16. Board independence and corporate governance: evidence from director resignations

    E-Print Network [OSTI]

    Gupta, Manu

    2005-08-29T23:59:59.000Z

    As evident from recent changes in NYSE and Nasdaq listing requirements, board independence is considered an important constituent of firms?? corporate governance structures. However, the empirical evidence regarding the impact of board structure...

  17. Corporate governance and long-term stock returns

    E-Print Network [OSTI]

    Moorman, Theodore Clark

    2005-08-29T23:59:59.000Z

    Extant literature finds that long-term abnormal stock returns are generated by a strategy based on corporate governance index values (Gompers, Ishii, and Metrick 2003). The result is inconsistent with efficient markets and suggests that information...

  18. LEE-0153- In the Matter of Martin Petroleum Corporation

    Broader source: Energy.gov [DOE]

    On August 17, 1994, Martin Petroleum Corporation (Martin) of Ft. Lauderdale, Florida, filed an Application for Exception with the Office of Hearings and Appeals of the Department of Energy. In its...

  19. Hindawi Publishing Corporation Science and Technology of Nuclear Installations

    E-Print Network [OSTI]

    Demazière, Christophe

    Hindawi Publishing Corporation Science and Technology of Nuclear Installations Volume 2013, Article Department of Nuclear Chemistry, Chalmers University of Technology, 412 96 Gothenburg, Sweden 2 Department of Nuclear Engineering, Chalmers University of Technology, 412 96 Gothenburg, Sweden Correspondence should

  20. Uncertain Growth Cycles, Corporate Investment, and Dynamic Hedging

    E-Print Network [OSTI]

    Yonce, Adam

    2010-01-01T23:59:59.000Z

    Chowdhry. Resources, real options, and corporate strategy.not exist in standard real option models: When invest- mentIn the theory of real options, uncertainty plays a crucial

  1. Corporate budgeting In practice : driving strategic focus and performance

    E-Print Network [OSTI]

    Briggman, Chandra A. (Chandra Alisa)

    2014-01-01T23:59:59.000Z

    This paper identifies insights and methods used in practice to address two weaknesses in the traditional corporate budgeting process. One point of failure is the weak linkage between organizational strategy and budgeting ...

  2. VBZ-0028- In the Matter of Sandia Corporation

    Broader source: Energy.gov [DOE]

    This decision considers a “Motion to Dismiss” filed by the Sandia Corporation (Sandia) on August 24, 1999. In its Motion, Sandia seeks judgment on the record of Complaint filed by Dr. Jiunn Yu (Yu)...

  3. STATEMENT OF CONSIDERATIONS REQUEST BY EATON CORPORATION FOR...

    Broader source: Energy.gov (indexed) [DOE]

    EATON CORPORATION FOR AN ADVANCE WAIVER OF DOMESTIC AND FOREIGN INVENTION RIGHTS UNDER DOE COOPERATIVE AGREEMENT NO. DE-FC26-04NT42263; W(A)-04-074, CH-1252 The Petitioner, Eaton...

  4. REQUEST BY EATON CORPORATION FOR AN ADVANCE WAIVER OF DOMESTIC...

    Broader source: Energy.gov (indexed) [DOE]

    DOE CONTRACT NO. DE-AC05-840R21400; DOE WAIVER DOCKET W(A)-94-011 ORO-578 The Eaton Corporation (Eaton) has made a timely request for an advance waiver to worldwide...

  5. REQUEST BY EATON CORPORATION FOR ADVANCE WAIVER OF DOMESTIC AND...

    Broader source: Energy.gov (indexed) [DOE]

    AND OPERATING CONTRACT NO. DE-AC05-840R21400; DOE WAIVER DOCKET W(A)-93-003 0RO-548 Eaton Corporation (Eaton) has made a timely request for an advance waiver to worldwide...

  6. UNDERSTANDING POSTAL PRIVATIZATION: CORPORATIONS, UNIONS AND "THE PUBLIC INTEREST"

    E-Print Network [OSTI]

    1 UNDERSTANDING POSTAL PRIVATIZATION: CORPORATIONS, UNIONS AND "THE PUBLIC INTEREST" BY SARAH F Relations Written under the direction of Professor Adrienne Eaton and approved by ___________[Jeffrey Keefe]_____________ ____________[Dorothy Sue Cobble]____________ ____________[Adrienne Eaton]_____________ New Brunswick, New Jersey

  7. STATEMENT OF CONSIDERATIONS REQUEST BY EATON CORPORATION FOR...

    Broader source: Energy.gov (indexed) [DOE]

    FR IPL DOE CH 630 252 2779 TO RGCP-HO P.02-03 * * STATEMENT OF CONSIDERATIONS REQUEST BY EATON CORPORATION FOR AN ADVANCE WAIVER OF PATENT RIGHTS UNDER DOE COOPERATIVE AGREEMENT...

  8. Essays on banking and corporate finance in developing countries

    E-Print Network [OSTI]

    Gormley, Todd A

    2006-01-01T23:59:59.000Z

    This dissertation consists of three essays that examine banking and corporate finance in developing countries. Specifically, it explores the theoretical and empirical implications of open capital markets, foreign bank ...

  9. THREE ESSAYS ON MONITORING OF FINANCIAL REPORTING BY CORPORATE DIRECTORS

    E-Print Network [OSTI]

    Xu, Yang

    2012-08-31T23:59:59.000Z

    Recent high-profile financial scandals and increasing instances of restatements focus public attention on the role of audit committees, auditors and CFOs in maintaining the integrity and quality of corporate financial ...

  10. Corporate serial acquisitions: An empirical test of the learning hypothesis

    E-Print Network [OSTI]

    Nesterov, Yurii

    2007/23 Corporate serial acquisitions: An empirical test of the learning hypothesis Nihat Aktas: An empirical test of the learning hypothesis Nihat AKTAS1, Eric DE BODT2 and Richard ROLL3 March2007 Abstract

  11. Logistics barriers for multinational corporations doing business in China

    E-Print Network [OSTI]

    Luo, Manqin, 1976-

    2004-01-01T23:59:59.000Z

    With rapid economic growth, China attracts many multinational corporations (MNCs) as a manufacturing center with both its cheap labor cost and a huge consumer market. While doing business in China, most MNCs have faced ...

  12. Overdensities of SMGs around WISE-selected, ultra-luminous, high-redshift galaxies

    E-Print Network [OSTI]

    Jones, Suzy F

    2015-01-01T23:59:59.000Z

    Submillimetre (submm) observations of WISE-selected, dusty, luminous, high-redshift galaxies have revealed intriguing overdensities around them on arcmin scales. They could be the best signposts of overdense environments on the sky.

  13. Quantitative comparison between Type Ia supernova spectra at low and high redshifts: A case study

    E-Print Network [OSTI]

    Garavini, G.; Supernova Cosmology Project

    2008-01-01T23:59:59.000Z

    Highlight - The Physics of Supernovae, ESO/MPA/MPE Workshop,Evolution in high-redshift supernovae Fig. 8 “Ca ii H&K”SN 1991T/SN 1999aa-like supernovae. 1. Introduction Type Ia

  14. Simultaneous Estimation of Photometric Redshifts and SED Parameters: Improved Techniques and a Realistic Error Budget

    E-Print Network [OSTI]

    Acquaviva, Viviana; Gawiser, Eric

    2015-01-01T23:59:59.000Z

    We seek to improve the accuracy of joint galaxy photometric redshift estimation and spectral energy distribution (SED) fitting. By simulating different sources of uncorrected systematic errors, we demonstrate that if the uncertainties on the photometric redshifts are estimated correctly, so are those on the other SED fitting parameters, such as stellar mass, stellar age, and dust reddening. Furthermore, we find that if the redshift uncertainties are over(under)-estimated, the uncertainties in SED parameters tend to be over(under)-estimated by similar amounts. These results hold even in the presence of severe systematics and provide, for the first time, a mechanism to validate the uncertainties on these parameters via comparison with spectroscopic redshifts. We propose a new technique (annealing) to re-calibrate the joint uncertainties in the photo-z and SED fitting parameters without compromising the performance of the SED fitting + photo-z estimation. This procedure provides a consistent estimation of the mu...

  15. The SCUBA HAlf Degree Extragalactic Survey (SHADES) - IV: Radio-mm-FIR photometric redshifts

    E-Print Network [OSTI]

    Itziar Aretxaga; David H. Hughes; Kristen Coppin; Angela M. J. Mortier; Jeff Wagg; James S. Dunlop; Edward L. Chapin; Stephen A. Eales; Enrique Gaztanaga; Mark Halpern; Rob J. Ivison; Eelco van Kampen; Douglas Scott; Stephen Serjeant; Ian Smail; Thomas Babbedge; Andrew J. Benson; Scott Chapman; David L. Clements; Loretta Dunne; Simon Dye; Duncan Farrah; Matthew J. Jarvis; Robert G. Mann; Alexandra Pope; Robert Priddey; Steve Rawlings; Marc Seigar; Laura Silva; Chris Simpson; Mattia Vaccari

    2007-05-31T23:59:59.000Z

    We present the redshift distribution of the SHADES galaxy population based on the rest-frame radio-mm-FIR colours of 120 robustly detected 850um sources in the Lockman Hole East (LH) and Subaru XMM-Newton Deep Field (SXDF). The redshift distribution derived from the full SED information is shown to be narrower than that determined from the radio-submm spectral index, as more photometric bands contribute to a higher redshift accuracy. The redshift distribution of sources derived from at least two photometric bands peaks at z ~ 2.4 and has a near-Gaussian distribution, with 50 per cent (interquartile range) of sources at z=1.8-3.1. We find a statistically-significant difference between the measured redshift distributions in the two fields; the SXDF peaking at a slightly lower redshift (median z ~ 2.2) than the LH (median z ~ 2.7), which we attribute to the noise-properties of the radio observations. We demonstrate however that there could also be field-to-field variations that are consistent with the measured differences in the redshift distributions, and hence, that the incomplete area observed by SHADES with SCUBA, despite being the largest sub-mm survey to date, may still be too small to fully characterize the bright sub-mm galaxy population. Finally we present a brief comparison with the predicted, or assumed, redshift distributions of sub-mm galaxy formation and evolution models, and we derive the contribution of these SHADES sources and the general sub-mm galaxy population to the star formation-rate density at different epochs.

  16. $?$--PhotoZ: Photometric Redshifts by Inverting the Tolman Surface Brightness Test

    E-Print Network [OSTI]

    Michael J. Kurtz; Margaret J. Geller; Daniel G. Fabricant; William F. Wyatt; Ian P. Dell'Antonio

    2007-07-03T23:59:59.000Z

    Surface brightness is a fundamental observational parameter of galaxies. We show, for the first time in detail, how it can be used to obtain photometric redshifts for galaxies, the $\\mu$-PhotoZ method. We demonstrate that the Tolman surface brightness relation, $\\mu \\propto (1+z)^{-4}$, is a powerful tool for determining galaxy redshifts from photometric data. We develop a model using $\\mu$ and a color percentile (ranking) measure to demonstrate the $\\mu$-PhotoZ method. We apply our method to a set of galaxies from the SHELS survey, and demonstrate that the photometric redshift accuracy achieved using the surface brightness method alone is comparable with the best color-based methods. We show that the $\\mu$-PhotoZ method is very effective in determining the redshift for red galaxies using only two photometric bands. We discuss the properties of the small, skewed, non-gaussian component of the error distribution. We calibrate $\\mu_r, (r-i)$ from the SDSS to redshift, and tabulate the result, providing a simple, but accurate look up table to estimate the redshift of distant red galaxies.

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

    SciTech Connect (OSTI)

    Pursimo, Tapio [Nordic Optical Telescope, Apartado 474, 38700 Santa Cruz de La Palma (Spain)] [Nordic Optical Telescope, Apartado 474, 38700 Santa Cruz de La Palma (Spain); Ojha, Roopesh [NVI Inc./U. S. Naval Observatory, 3450 Massachusetts Ave NW, Washington DC (United States)] [NVI Inc./U. S. Naval Observatory, 3450 Massachusetts Ave NW, Washington DC (United States); Jauncey, David L. [CSIRO Astronomy and Space Science and Mount Stromlo Observatory, Canberra ACT 0200 (Australia)] [CSIRO Astronomy and Space Science and Mount Stromlo Observatory, Canberra ACT 0200 (Australia); Rickett, Barney J. [Department of Electrical and Computer Engineering, University of California, San Diego, La Jolla, CA 92093 (United States)] [Department of Electrical and Computer Engineering, University of California, San Diego, La Jolla, CA 92093 (United States); Dutka, Michael S. [The Catholic University of America, 620 Michigan Ave., N.E., Washington DC 20064 (United States)] [The Catholic University of America, 620 Michigan Ave., N.E., Washington DC 20064 (United States); Koay, Jun Yi; Bignall, Hayley E.; Macquart, Jean-Pierre [ICRAR, Curtin University, Bentley, WA 6845 (Australia)] [ICRAR, Curtin University, Bentley, WA 6845 (Australia); Lovell, James E. J. [School of Mathematics and Physics, University of Tasmania, TAS 7001 (Australia)] [School of Mathematics and Physics, University of Tasmania, TAS 7001 (Australia); Kedziora-Chudczer, Lucyna, E-mail: tpursimo@not.iac.es [School of Physics and Astrophysics, UNSW, Sydney NSW 2052 (Australia)] [School of Physics and Astrophysics, UNSW, Sydney NSW 2052 (Australia)

    2013-04-10T23:59:59.000Z

    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. The Environments of Low and High Luminosity Radio Galaxies at Moderate Redshifts

    E-Print Network [OSTI]

    M. W. Auger; R. H. Becker; C. D. Fassnacht

    2008-01-02T23:59:59.000Z

    In the local Universe, high-power radio galaxies live in lower density environments than low-luminosity radio galaxies. If this trend continues to higher redshifts, powerful radio galaxies would serve as efficient probes of moderate redshift groups and poor clusters. Photometric studies of radio galaxies at 0.3 environment correlation disappears at moderate redshifts, though this could be the result of foreground/background contamination affecting the photometric measures of environment. We have obtained multi-object spectroscopy of in the fields of 14 lower luminosity (L_1.4GHz 1.2x10^25 W/Hz) radio galaxies at z ~ 0.3 to spectroscopically investigate the link between the environment and the radio luminosity of radio galaxies at moderate redshifts. Our results support the photometric analyses; there does not appear to be a correlation between the luminosity of a radio galaxy and its environment at moderate redshifts. Hence, radio galaxies are not efficient signposts for group environments at moderate redshifts.

  19. Corporate governance under stress : an institutional perspective on the transformation of corporate governance in France and Germany

    E-Print Network [OSTI]

    Goyer, Michel, 1964-

    2004-01-01T23:59:59.000Z

    This work contributes to the study of comparative political economy by examining the impact of financial deregulation on corporate governance in the two main continental European economies, France and Germany. It investigates ...

  20. Radiative Feedback in Relic HII Regions at High-Redshift

    E-Print Network [OSTI]

    Andrei Mesinger; Greg L. Bryan; Zoltan Haiman

    2009-09-13T23:59:59.000Z

    UV radiation from early astrophysical sources could have a large impact on subsequent star formation in nearby protogalaxies. Here we study the radiative feedback from the first, short-lived stars using hydrodynamical simulations with transient UV backgrounds (UVBs) and persistent Lyman-Werner backgrounds (LWBs) of varying intensity. We extend our prior work in Mesinger et al. (2006), by studying a more typical region whose proto-galaxies form at lower redshifts, z~13-20, in the epoch likely preceding the bulk of reionization. We confirm our previous results that feedback in the relic HII regions resulting from such transient radiation, is itself transient. Feedback effects dwindle away after ~30% of the Hubble time, and the same critical specific intensity of J_UV~0.1 x 10^{-21} ergs/s/cm^2/Hz/sr separates positive and negative feedback regimes. Additionally, we discover a second episode of eventual positive feedback in halos which have not yet collapsed when their progenitor regions were exposed to the transient UVB. This eventual positive feedback appears in all runs, regardless of the strength of the UVB. However, this feedback regime is very sensitive to the presence of Lyman-Werner radiation, and notable effects disappear under fairly modest background intensities of J_LW>10^{-3} x 10^{-21} ergs/s/cm^2/Hz/sr. We conclude that UV radiative feedback in relic HII regions, although a complicated process, seems unlikely to have a major impact on the progress of cosmological reionization, provided that present estimates of the lifetime and luminosity of a PopIII star are accurate. More likely is that the build-up of the LWB ultimately governs the feedback strength until a persistent UV background can be established. [abridged

  1. The Luminosity Function of Low-Redshift Abell Galaxy Clusters

    E-Print Network [OSTI]

    Wayne A. Barkhouse; H. K. C. Yee; Omar López-Cruz

    2007-09-07T23:59:59.000Z

    We present the results from a survey of 57 low-redshift Abell galaxy clusters to study the radial dependence of the luminosity function (LF). The dynamical radius of each cluster, r200, was estimated from the photometric measurement of cluster richness, Bgc. The shape of the LFs are found to correlate with radius such that the faint-end slope, alpha, is generally steeper on the cluster outskirts. The sum of two Schechter functions provides a more adequate fit to the composite LFs than a single Schechter function. LFs based on the selection of red and blue galaxies are bimodal in appearance. The red LFs are generally flat for -22 -18. The blue LFs contain a larger contribution from faint galaxies than the red LFs. The blue LFs have a rising faint-end component (alpha ~ -1.7) for M_Rc > -21, with a weaker dependence on radius than the red LFs. The dispersion of M* was determined to be 0.31 mag, which is comparable to the median measurement uncertainty of 0.38 mag. This suggests that the bright-end of the LF is universal in shape at the 0.3 mag level. We find that M* is not correlated with cluster richness when using a common dynamical radius. Also, we find that M* is weakly correlated with BM-type such that later BM-type clusters have a brighter M*. A correlation between M* and radius was found for the red and blue galaxies such that M* fades towards the cluster center.

  2. Fuel-Flexible Microturbine and Gasifier System for Combined Heat...

    Energy Savers [EERE]

    Power Fuel-Flexible Microturbine and Gasifier System for Combined Heat and Power Capstone Turbine Corporation, in collaboration with the University of California-Irvine, Packer...

  3. Development on simultaneous reduction system of NOx and PM from...

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

    system of NOx and PM from a diesel engine 2003 DEER Converence Presentation: Toyota Motor Corporation 2003deerwatanabe.pdf More Documents & Publications An Improvement of...

  4. Gas informations systems as an asset, not an expense

    SciTech Connect (OSTI)

    Neill, C.

    1995-12-31T23:59:59.000Z

    The utilization of information systems in the natural gas industry is described. Opportunities for the acquisition of important business information and corporate issues are illustrated.

  5. Korea's Newly Enacted Unified Bankruptcy Act: The Role of the New Act in Facilitating (or Discouraging) the Transfer of Corporate Control

    E-Print Network [OSTI]

    Ko, Haksoo

    2007-01-01T23:59:59.000Z

    perspective of corporate governance, the decision whether toefforts to implement corporate governance reforms and otherthe weakness of the corporate governance mechanism in Korea,

  6. A CLOSE-PAIR ANALYSIS OF DAMP MERGERS AT INTERMEDIATE REDSHIFTS

    SciTech Connect (OSTI)

    Chou, Richard C. Y.; Abraham, Roberto G. [Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5S 3H4 (Canada); Bridge, Carrie R., E-mail: chou@astro.utoronto.ca, E-mail: abraham@astro.utoronto.ca, E-mail: bridge@astro.caltech.edu [Department of Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125 (United States)

    2012-12-01T23:59:59.000Z

    We have studied the kinematics of {approx}2800 candidate close-pair galaxies at 0.1 < z < 1.2 identified from the Canada-France-Hawaii Telescope Legacy Survey fields. Spectra of these systems were obtained using spectrometers on the 6.5 m Magellan and 5 m Hale telescopes. These data allow us to constrain the rate of dry mergers at intermediate redshifts and to test the 'hot halo' model for quenching of star formation. Using virial radii estimated from the correlation between dynamical and stellar masses published by Leauthaud et al., we find that around 1/5 of our candidate pairs are likely to share a common dark matter halo (our metric for close physical association). These pairs are divided into red-red, blue-red, and blue-blue systems using the rest-frame colors classification method introduced in Chou et al.. Galaxies classified as red in our sample have very low star formation rates, but they need not be totally quiescent, and hence we refer to them as 'damp', rather than 'dry', systems. After correcting for known selection effects, the fraction of blue-blue pairs is significantly greater than that of red-red and blue-red pairs. Red-red pairs are almost entirely absent from our sample, suggesting that damp mergers are rare at z {approx} 0.5. Our data support models with a short merging timescale (<0.5 Gyr) in which star formation is enhanced in the early phase of mergers, but quenched in the late phase. Hot halo models may explain this behavior, but only if virial shocks that heat gas are inefficient until major mergers are nearly complete.

  7. Autofib Redshift Survey: II -- The Evolution of the Galaxy Luminosity Function by Spectral Type

    E-Print Network [OSTI]

    Jeremy Heyl; Matthew Colless; Richard S. Ellis; Tom Broadhurst

    1996-10-04T23:59:59.000Z

    We determine the evolution of the galaxy luminosity function (LF) as a function of spectral type using the Autofib redshift survey, a compendium of over 1700 galaxy redshifts in various magnitude-limited samples spanning b_J=11.5-24.0. To carry out this analysis we have developed a cross-correlation technique which classifies faint galaxy spectra into one of six types based on local galaxy templates. Tests and simulations show that this technique yields classifications correct to within one type for more than 90% of the galaxies in our sample. We have also developed extensions of the step-wise maximum likelihood method and the STY parametric method for estimating LFs which are applicable to recovering an evolving LF from multiple samples. We find that: (i) The spectra and LF of E/S0 galaxies show no appreciable evolution out to at least z ~ 0.5. (ii) Early-type spirals show modest evolution, characterised by a gradual steepening of the faint end of their LF with redshift. (iii) Out to z ~ 0.5, the overall evolution of the galaxy population is dominated by changes seen in late-type spirals. The characteristic luminosity (L^*) of these galaxies appears to brighten with redshift and there are signs of strong density evolution (a rapid increase in \\phi^*). These effects appear to be luminosity dependent so that the LF steepens at higher redshift. These trends are accompanied by a steep increase in the median [OII] equivalent width, implying a rapid increase in the star-formation rate with redshift at fixed luminosity---a given star-formation rate is found at higher redshift in galaxies of higher luminosity. We find that these conclusions are robust with respect to spectral classification errors and the luminosity function estimator.

  8. Covanta Energy Corporation formerly Ogden Martin Systems of Hillsborou...

    Open Energy Info (EERE)

    Inc) Place: Fairfield, New Jersey Zip: 7004 Product: Owner and operator of modern waste-to-energy facilities (over 1GW). Coordinates: 47.38522, -117.171254 Show Map...

  9. For Immediate Release: June 14, 2001 MULTIDATA SYSTEMS INTERNATIONAL CORPORATION

    E-Print Network [OSTI]

    Responds to IAEA Reports on Radiological Emergency in Panama In public documents released aware of a radiological emergency in Panama. In a preliminary report issued on June 2, 2001, the IAEA reported on a radiological emergency at the National Oncology Institute of Panama. The emergency involved

  10. Optimizing Electric Motor Systems at a Corporate Campus Facility |

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the.pdfBreaking ofOilNEWResponse toOctober 2014FundsOpti-MN Impact HouseDepartmentDepartment

  11. Tax Credit for Solar Energy Systems on Residential Property (Corporate) |

    Broader source: Energy.gov (indexed) [DOE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn April 23, 2014,ZaleskiThis Decision considersTable 1: PointsGasContact

  12. Optimizing Electric Motor Systems at a Corporate Campus Facility

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn'tOrigin of Contamination in ManyDepartment ofOil'sEnergy8 * October

  13. Optimizing Electric Motor Systems at a Corporate Campus Facility |

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn'tOrigin of Contamination in ManyDepartment ofOil'sEnergy8 * OctoberDepartment of Energy

  14. Renewable Energy Systems Tax Credit (Corporate) | Department of Energy

    Broader source: Energy.gov (indexed) [DOE]

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742EnergyOn April 23, 2014, an OHASeptember 2010InJanuaryGeothermal ElectricConstruction Residential

  15. Implementing a Corporate Energy Management System | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page onYouTube YouTube Note: Since the.pdfBreaking of BlytheDepartment of Energy IRSJuly 2012 |Energy Technology

  16. Nevaro Capital Corporation Formerly VRB Power Systems | Open Energy

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are being directedAnnual SiteofEvaluatingGroup |JilinLuOpen EnergyNelsoniX Ltd JumpNepaliInformation Nevaro Capital

  17. Covanta Energy Corporation formerly Ogden Martin Systems of Hillsborough

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are beingZealand JumpConceptual Model, clickInformationNew|Core AnalysisCouncil, Idaho: EnergyCovantaInc | Open

  18. Georgia System Operations Corporation Inc. Smart Grid Project | Open Energy

    Open Energy Info (EERE)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page onYou are now leaving Energy.gov You are now leaving Energy.gov You are8COaBulkTransmissionSitingProcess.pdf Jump1946865°,Park,2005) | Open Energy(Blackwell,GeopowerInformation

  19. Implementing a Corporate Energy Management System | Department of Energy

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

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels DataDepartment of Energy Your Density Isn't YourTransport(Fact Sheet),Energy PetroleumEnergyImplementing Executive Order

  20. An Analysis of Gravitational Redshift from Rotating Body-II: The Effect of Electro and Magneto Static Field

    E-Print Network [OSTI]

    Dubey, Anuj Kumar

    2015-01-01T23:59:59.000Z

    It is well known fact that gravitational mass can alter the space time structure and gravitational redshift is its one example. Static electric or magnetic charge can also alter the space-time similar to gravitational mass. So Static electric or magnetic charge can also give rise to an effect of same kind on redshift (analogous to gravitational redshift). This can be considered as electro and magneto static redshift. Gravitational redshift has been reported by most of the authors without consideration of static electric and / or magnetic charge present on the rotating body. As a continuation of our previous work [1], in the present paper we will discuss combined gravitational and electro-magneto-static redshift for rotating by using Kerr - Newman - Kasuya metric.

  1. Red-Shift Distribution of Gamma-ray Bursts and Their Progenitors

    E-Print Network [OSTI]

    Soomin Jeong; Chang-Hwan Lee

    2007-10-08T23:59:59.000Z

    Gamma ray bursts have been divided into two classes, long-soft gamma ray burst and short-hard gamma ray burst according to the bimodal distribution in duration time. Due to the harder spectrum and the lack of afterglows of short-hard bursts in optical and radio observations, different progenitors for short-hard bursts and long-soft bursts have been suggested. Based on the X-ray afterglow observation and the cumulative red-shift distribution of short-hard bursts, Nakar et al. (2006) found that the progenitors of short-hard bursts are consistent with old populations, such as mergers of binary neutron stars. Recently, the existence of two subclasses in long-soft bursts has been suggested after considering multiple characteristics of gamma-ray bursts, including fluences and the duration time. In this work, we extended the analysis of cumulative red-shift distribution to two possible subclasses in L-GRBs. We found that two possible subclass GRBs show different red-shift distributions, especially for red-shifts z > 1. Our results indicate that the accumulative red-shift distribution can be used as a tool to constrain the progenitor characteristics of possible subclasses in L-GRBs.

  2. The Swift Gamma-Ray Burst Host Galaxy Legacy Survey - I. Sample Selection and Redshift Distribution

    E-Print Network [OSTI]

    Perley, D A; Schulze, S; Postigo, A de Ugarte; Hjorth, J; Berger, E; Cenko, S B; Chary, R; Cucchiara, A; Ellis, R; Fong, W; Fynbo, J P U; Gorosabel, J; Greiner, J; Jakobsson, P; Laskar, T; Levan, A J; Micha?owski, M J; Milvang-Jensen, B; Tanvir, N R; Thöne, C C; Wiersema, K

    2015-01-01T23:59:59.000Z

    We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey ("SHOALS"), a multi-observatory high-redshift galaxy survey targeting the largest unbiased sample of long-duration gamma-ray burst hosts yet assembled (119 in total). We describe the motivations of the survey and the development of our selection criteria, including an assessment of the impact of various observability metrics on the success rate of afterglow-based redshift measurement. We briefly outline our host-galaxy observational program, consisting of deep Spitzer/IRAC imaging of every field supplemented by similarly-deep, multi-color optical/NIR photometry, plus spectroscopy of events without pre-existing redshifts. Our optimized selection cuts combined with host-galaxy follow-up have so far enabled redshift measurements for 110 targets (92%) and placed upper limits on all but one of the remainder. About 20% of GRBs in the sample are heavily dust-obscured, and at most 2% originate from z>5.5. Using this sample we estimate the redshift-depen...

  3. IBM Global Services 2008 IBM Corporation

    E-Print Network [OSTI]

    or a supported ESXI operating system and configure basic networking. Test and verify the operation of each Blade operating system and configure basic networking. Test and verify the operation of the Blade. Implement up to three blades in BladeCenter chassis. Install a supported Microsoft operating system

  4. 2012 IBM Corporation IBM operates in 170

    E-Print Network [OSTI]

    Raja, Anita

    Smart traffic systems Smart water management Smart energy grids Smart healthcare Smart food systems cities Smart retail Making the worlds systems smarter depends on data and analytics #12;© 2012 IBM Intelligent oil field technologies Smart regions Smart weather Smart countries Smart supply chains Smart

  5. Hindawi Publishing Corporation International Journal of Photoenergy

    E-Print Network [OSTI]

    Aristomenis, Antoniadis

    , Pages 1­8 DOI 10.1155/IJP/2006/73650 Sizing Stand-Alone Photovoltaic Systems A. Balouktsis,1 T. D August 2005; Accepted 5 September 2005 A method of sizing stand-alone photovoltaic systems regarding­9]. The present study is concerned with sizing stand-alone photovoltaic systems for different locations in Greece

  6. General Doppler Shift Equation and the Possibility of Systematic Error in Calculation of Z for High Redshift Type Ia Supernovae

    E-Print Network [OSTI]

    Steven M Taylor

    2007-04-10T23:59:59.000Z

    Systematic error in calculation of z for high redshift type Ia supernovae could help explain unexpected luminosity values that indicate an accelerating rate of expansion of the universe.

  7. A corporate fitness center : an example for the reuse of the Empire Stores, Brooklyn, N.Y.

    E-Print Network [OSTI]

    Georgopulos, Diane Theodora

    1982-01-01T23:59:59.000Z

    The proliferation of over 500 fitness programs for the employees of American corporations marks a turning point for the way American corporations regard employee and corporate health. Typically, sports facilities were the ...

  8. Recovery Act: Waste Energy Project at AK Steel Corporation Middletown

    SciTech Connect (OSTI)

    Joyce, Jeffrey

    2012-06-30T23:59:59.000Z

    In 2008, Air Products and Chemicals, Inc. (“Air Products”) began development of a project to beneficially utilize waste blast furnace “topgas” generated in the course of the iron-making process at AK Steel Corporation’s Middletown, Ohio works. In early 2010, Air Products was awarded DOE Assistance Agreement DE-EE002736 to further develop and build the combined-cycle power generation facility. In June 2012, Air Products and AK Steel Corporation terminated work when it was determined that the project would not be economically viable at that time nor in the foreseeable future. The project would have achieved the FOA-0000044 Statement of Project Objectives by demonstrating, at a commercial scale, the technology to capture, treat, and convert blast furnace topgas into electric power and thermal energy.

  9. Accounting procedures under the Texas Business Corporation Act

    E-Print Network [OSTI]

    Dodson, Donald R

    1961-01-01T23:59:59.000Z

    with the definit, ion as provided in the Texas Business Corp oration Act ~ Consider for example the followingn Xo to m~s Auditlngf "Surplus ie 1 generally unZerstoo3 as tEe equity of stock- holders in corporate assets in excess of the par or stated value... in excess of stated capital/ proprietory reservea ~ and unrealised appreciation in the value. of' asseta, The Texas Business Corporation Aot, excludes an appreciation in value of 'assetS as 8 Component of surplus, Lehart and Defliese, nt ome '8 ~Au it...

  10. Comments of Space Data Corporation | Department of Energy

    Office of Environmental Management (EM)

    AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative1 First Use of Energy for All Purposes (Fuel and Nonfuel), 2002; Level: National5Sales for4,645 3,625 1,006 492 742 33 1112011AT&T, Inc.'sEnergyTexas1.Space Data Corporation Comments of Space Data Corporation

  11. Redshift evolution of the dynamical properties of massive galaxies from SDSS-III/BOSS

    E-Print Network [OSTI]

    Beifiori, Alessandra; Maraston, Claudia; Steele, Oliver; Masters, Karen L; Pforr, Janine; Saglia, Roberto P; Bender, Ralf; Tojeiro, Rita; Chen, Yan-Mei; Bolton, Adam; Brownstein, Joel R; Johansson, Jonas; Leauthaud, Alexie; Nichol, Robert C; Schneider, Donald P; Senger, Robert; Skibba, Ramin; Wake, David; Pan, Kaike; Snedden, Stephanie; Bizyaev, Dmitry; Brewington, Howard; Malanushenko, Viktor; Malanushenko, Elena; Oravetz, Daniel; Simmons, Audrey; Shelden, Alaina; Ebelke, Garrett

    2014-01-01T23:59:59.000Z

    We study the redshift evolution of the dynamical properties of ~180,000 massive galaxies from SDSS-III/BOSS combined with a local early-type galaxy sample from SDSS-II in the redshift range 0.12sigma significance. By combining our sample with high-redshift literature data we find that this evolution of the dynamical to stellar mass ratio continues beyond z~0.7 up to z>2 as Mdyn/Mstar~ (1+z)^{-0.30+/- 0.12} further strengthening the evidence for an increase of Mdyn/Mstar with cosmic time. This result is in line with recent predictions from galaxy formation simulations based on minor merger driven mass growth, in which the dark matter fraction within the half-light radius increases with cosmic time.

  12. Type Ia supernova rate at a redshift of ~ 0.1

    E-Print Network [OSTI]

    Blanc, G; Alard, C; Albert, J N; Aldering, G; Amadon, A; Andersen, J; Ansari, R; Aubourg, E; Balland, C; Bareyre, P; Beaulieu, J P; Charlot, X; Conley, A; Coutures, C; Dahlen, T; Derue, F; Fan, X; Ferlet, R; Folatelli, G; Fouqué, P; Garavini, G; Glicenstein, J F; Goldman, B; Goobar, A; Gould, A; Graff, D; Gros, M; Haïssinski, J; Hamadache, C; Hardin, D; Hook, I M; De Kat, J; Kent, S; Kim, A; Lasserre, T; Le Guillou, Laurent; Lesquoy, E; Loup, C; Magneville, C; Marquette, J B; Maurice, E; Maury, A; Milsztajn, A; Moniez, M; Mouchet, M; Newberg, H; Nobili, S; Palanque-Delabrouille, Nathalie; Perdereau, O; Prévôt, L; Rahal, Y R; Regnault, N; Rich, J; Ruiz-Lapuente, P; Spiro, M; Tisserand, P; Vidal-Madjar, A; Vigroux, L; Walton, N A; Zylberajch, S

    2004-01-01T23:59:59.000Z

    We present the type Ia rate measurement based on two EROS supernova search campaigns (in 1999 and 2000). Sixteen supernovae identified as type Ia were discovered. The measurement of the detection efficiency, using a Monte Carlo simulation, provides the type Ia supernova explosion rate at a redshift ~ 0.13. The result is $0.125^{+0.044+0.028}_{-0.034-0.028} h_{70}^2$ SNu where 1 SNu = 1 SN / $10^{10} L_{sun}^B$ / century. This value is compatible with the previous EROS measurement (Hardin et al. 2000), done with a much smaller sample, at a similar redshift. Comparison with other values at different redshifts suggests an evolution of the type Ia supernova rate.

  13. Type Ia supernova rate at a redshift of ~ 0.1

    E-Print Network [OSTI]

    G. Blanc; C. Afonso; C. Alard; J. N. Albert; G. Aldering; A. Amadon; J. Andersen; R. Ansari; E. Aubourg; C. Balland; P. Bareyre; J. P. Beaulieu; X. Charlot; A. Conley; C. Coutures; T. Dahlen; F. Derue; X. Fan; R. Ferlet; G. Folatelli; P. Fouque; G. Garavini; J. F. Glicenstein; B. Goldman; A. Goobar; A. Gould; D. Graff; M. Gros; J. Haissinski; C. Hamadache; D. Hardin; I. M. Hook; J. deKat; S. Kent; A. Kim; T. Lasserre; L. LeGuillou; E. Lesquoy; C. Loup; C. Magneville; J. B. Marquette; E. Maurice; A. Maury; A. Milsztajn; M. Moniez; M. Mouchet; H. Newberg; S. Nobili; N. Palanque-Delabrouille; O. Perdereau; L. Prevot; Y. R. Rahal; N. Regnault; J. Rich; P. Ruiz-Lapuente; M. Spiro; P. Tisserand; A. Vidal-Madjar; L. Vigroux; N. A. Walton; S. Zylberajch

    2004-05-11T23:59:59.000Z

    We present the type Ia rate measurement based on two EROS supernova search campaigns (in 1999 and 2000). Sixteen supernovae identified as type Ia were discovered. The measurement of the detection efficiency, using a Monte Carlo simulation, provides the type Ia supernova explosion rate at a redshift ~ 0.13. The result is $0.125^{+0.044+0.028}_{-0.034-0.028} h_{70}^2$ SNu where 1 SNu = 1 SN / $10^{10} L_{sun}^B$ / century. This value is compatible with the previous EROS measurement (Hardin et al. 2000), done with a much smaller sample, at a similar redshift. Comparison with other values at different redshifts suggests an evolution of the type Ia supernova rate.

  14. The environments of intermediate-redshift QSOs: 0.3 < z < 0.7

    E-Print Network [OSTI]

    R. J. Smith; B. J. Boyle; S. J. Maddox

    1999-11-22T23:59:59.000Z

    An angular correlation of low significance (2 sigma) is observed between 0.3 0.5 QSOs. After converting to an excess of galaxies physically associated with the QSO, this lack of strong correlation is shown to be consistent with the clustering of normal galaxies at the same moderate redshifts. Combined with previous observations, these results imply that the environments of radio-quiet QSOs do not undergo significant evolution with respect to the galaxy population over a wide range of redshifts (0 < z < 1.5). This is in marked contrast to the rapid increase in the richness of the environments associated with radio-loud QSOs over the same redshift range.

  15. The gravitational redshift of photons traversing a collapsing dust cloud and observable consequences

    E-Print Network [OSTI]

    Néstor Ortiz; Olivier Sarbach

    2014-11-24T23:59:59.000Z

    We analyze the frequency shift of photons propagating on an asymptotically flat spacetime describing a collapsing, spherical dust cloud. We focus on the case where the interaction of the photons with the matter can be neglected. Under fairly general assumptions on the initial data characterizing the collapse, we show that photons with zero angular momentum which travel from past to future null infinity, crossing the collapsing cloud through its center, are always redshifted with respect to stationary observers. We compute this redshift as a function of proper time of a distant stationary observer and discuss its dependency on the mass distribution of the cloud. Possible implications of this redshift effect for weak cosmic censorship and light propagation in cosmological spacetimes are also briefly discussed.

  16. The fate of high redshift massive compact galaxies in dense environments

    SciTech Connect (OSTI)

    Kaufmann, Tobias; /Zurich, ETH; Mayer, Lucio; /Zurich U.; Carollo, Marcella; /Zurich, ETH; Feldmann, Robert; /Fermilab /Chicago U., KICP

    2012-01-01T23:59:59.000Z

    Massive compact galaxies seem to be more common at high redshift than in the local universe, especially in denser environments. To investigate the fate of such massive galaxies identified at z {approx} 2 we analyse the evolution of their properties in three cosmological hydrodynamical simulations that form virialized galaxy groups of mass {approx} 10{sup 13} M{sub {circle_dot}} hosting a central massive elliptical/S0 galaxy by redshift zero. We find that at redshift {approx} 2 the population of galaxies with M{sub *} > 2 x 10{sup 10} M{sub {circle_dot}} is diverse in terms of mass, velocity dispersion, star formation and effective radius, containing both very compact and relatively extended objects. In each simulation all the compact satellite galaxies have merged into the central galaxy by redshift 0 (with the exception of one simulation where one of such satellite galaxy survives). Satellites of similar mass at z = 0 are all less compact than their high redshift counterparts. They form later than the galaxies in the z = 2 sample and enter the group potential at z < 1, when dynamical friction times are longer than the Hubble time. Also, by z = 0 the central galaxies have increased substantially their characteristic radius via a combination of in situ star formation and mergers. Hence in a group environment descendants of compact galaxies either evolve towards larger sizes or they disappear before the present time as a result of the environment in which they evolve. Since the group-sized halos that we consider are representative of dense environments in the {Lambda}CDM cosmology, we conclude that the majority of high redshift compact massive galaxies do not survive until today as a result of the environment.

  17. NCCR Trade Regulation Brown Bag Series Dr Franziska Humbert, Policy Advisor Corporate Social Responsibility, Oxfam Germany

    E-Print Network [OSTI]

    Richner, Heinz

    Social Responsibility, Oxfam Germany International Constitutionalism and Child Labour Wednesday, 23, Policy Advisor Corporate Social Responsibility, Oxfam Germany. Abstract The postdoctoral thesis builds of the Speaker Franziska Humbert is a policy advisor on corporate social responsibility at Oxfam Germany

  18. Bear Head LNG Corporation and Bear Head LNG (USA), LLC - FE Dkt...

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

    Bear Head LNG Corporation and Bear Head LNG (USA), LLC - FE Dkt. No. - 15-33-LNG Bear Head LNG Corporation and Bear Head LNG (USA), LLC - FE Dkt. No. - 15-33-LNG The Office of...

  19. Changing gear : driving corporate real estate financing decisions for the agile workplace

    E-Print Network [OSTI]

    Hardy, Trevor J. F. (Trevor John Fraser), 1977-

    2002-01-01T23:59:59.000Z

    Given the needs of corporations in the global business environment, corporate real estate investment decisions represent strategic choices that support a company's overall business strategy. This thesis clearly illustrates ...

  20. State Participation and the Corporate Value of Natural Resource Economic Rents 

    E-Print Network [OSTI]

    Kretzschmar, Gavin Lee

    2007-01-01T23:59:59.000Z

    The asset participation relationship between the state and the corporate entity is an essential determinant of corporate value in the natural resource sector. Natural resources deplete, with the result that oil reserve ...