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1

CO2 Emissions - Maldives  

NLE Websites -- All DOE Office Websites (Extended Search)

Far East Maldives CO2 Emissions from Maldives Data graphic Data CO2 Emissions from Maldives image Per capita CO2 Emission Estimates for Maldives...

2

Maldives | OpenEI  

Open Energy Info (EERE)

Maldives Maldives Dataset Summary Description (Abstract): This document describes the development of detailed high-resolution (1 km2) wind energy resource maps for Sri Lanka and the Maldives. (Purpose): To provide information on the wind resource potential within Sri Lanka and the Maldives. Source NREL Date Released August 21st, 2006 (8 years ago) Date Updated August 21st, 2006 (8 years ago) Keywords documentation GEF GIS Maldives NREL Sri Lanka SWERA UNEP wind Data application/pdf icon Download Report (pdf, 30.1 MiB) Quality Metrics Level of Review Some Review Comment Temporal and Spatial Coverage Frequency Time Period 2006 License License Open Data Commons Public Domain Dedication and Licence (PDDL) Comment Restrictions to use (Use Constraints): This GIS data was developed by the National Renewable Energy Laboratory ("NREL"), which is operated by the Midwest Research Institute for the U.S. Department of Energy ("DOE"). The user is granted the right, without any fee or cost, to use, copy, modify, alter, enhance and distribute this data for any purpose whatsoever, provided that this entire notice appears in all copies of the data. Further, the user of this data agrees to credit NREL in any publications or software that incorporate or use the data. Access to and use of the GIS data shall further impose the following obligations on the User. The names DOE/NREL may not be used in any advertising or publicity to endorse or promote any product or commercial entity using or incorporating the GIS data unless specific written authorization is obtained from DOE/NREL. The User also understands that DOE/NREL shall not be obligated to provide updates, support, consulting, training or assistance of any kind whatsoever with regard to the use of the GIS data. THE GIS DATA IS PROVIDED "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL DOE/NREL BE LIABLE FOR ANY SPECIAL, INDIRECT OR CONSEQUENTIAL DAMAGES OR ANY DAMAGES WHATSOEVER, INCLUDING BUT NOT LIMITED TO CLAIMS ASSOCIATED WITH THE LOSS OF DATA OR PROFITS, WHICH MAY RESULT FROM AN ACTION IN CONTRACT, NEGLIGENCE OR OTHER TORTIOUS CLAIM THAT ARISES OUT OF OR IN CONNECTION WITH THE ACCESS OR USE OF THE GIS DATA. The User acknowledges that access to the GIS data is subject to U.S. Export laws and regulations and any use or transfer of the GIS data must be authorized under those regulations. The User shall not use, distribute, transfer, or transmit GIS data or any products incorporating the GIS data except in compliance with U.S. export regulations. If requested by DOE/NREL, the User agrees to sign written assurances and other export-related documentation as may be required to comply with U.S. export regulations.

3

Maldives-NREL Cooperation | Open Energy Information  

Open Energy Info (EERE)

Maldives-NREL Cooperation Maldives-NREL Cooperation Jump to: navigation, search Logo: Maldives-NREL Cooperation Name Maldives-NREL Cooperation Agency/Company /Organization National Renewable Energy Laboratory Partner U.S. Department of Energy Sector Energy Focus Area Solar, Wind Topics Resource assessment, Background analysis Resource Type Dataset, Maps, Software/modeling tools Website http://www.nrel.gov/internatio Country Maldives Southern Asia References NREL International Program[1] Abstract NREL partnered with the Maldives to develop wind and solar assessments for the country. NREL partnered with the Maldives to develop wind and solar assessments for the country. References ↑ "NREL International Program" Retrieved from "http://en.openei.org/w/index.php?title=Maldives-NREL_Cooperation&oldid=375297"

4

Maldives-Supporting the Zero Emissions Strategy | Open Energy Information  

Open Energy Info (EERE)

Maldives-Supporting the Zero Emissions Strategy Maldives-Supporting the Zero Emissions Strategy Jump to: navigation, search Name Maldives-Supporting the Zero Emissions Strategy Agency/Company /Organization German Agency for International Cooperation (GIZ) Partner Federal Ministry for the Environment, Nature Conservation and Nuclear Safety (BMU) Sector Energy Focus Area Energy Efficiency Topics Low emission development planning, Pathways analysis Program Start 2011 Program End 2013 Country Maldives Southern Asia References GTZ Schwerpunkte[1] GIZ[2] Contents 1 Overview 1.1 Costa Rica 1.2 Maldives 2 Outcomes, Lessons Learned and Good Practices 3 References Overview Costa Rica Maldives The Maldives are less the 2.5 m above sea level. Hence, the danger from climate change is crucial. At the same time the Maldives' economy,

5

Maldives: Energy Resources | Open Energy Information  

Open Energy Info (EERE)

Maldives: Energy Resources Maldives: Energy Resources Jump to: navigation, search Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"TERRAIN","zoom":5,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"390px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":3.2,"lon":73,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

6

Technical Report - Sri Lanka and the Maldives Wind Energy Resource  

Open Energy Info (EERE)

Sri Lanka and the Maldives Wind Energy Resource Assessment (Abstract):  This document describes the development of detailed high-resolution (1 km2) wind energy...

7

Wind Energy Resource Atlas of Sri Lanka and the Maldives  

DOE Green Energy (OSTI)

The Wind Energy Resource Atlas of Sri Lanka and the Maldives, produced by the National Renewable Energy Laboratory's (NREL's) wind resource group identifies the wind characteristics and distribution of the wind resource in Sri Lanka and the Maldives. The detailed wind resource maps and other information contained in the atlas facilitate the identification of prospective areas for use of wind energy technologies, both for utility-scale power generation and off-grid wind energy applications.

Elliott, D.; Schwartz, M.; Scott, G.; Haymes, S.; Heimiller, D.; George, R.

2003-08-01T23:59:59.000Z

8

Maldives-Program for Scaling Up Renewable Energy in Low Income Countries  

Open Energy Info (EERE)

Maldives-Program for Scaling Up Renewable Energy in Low Income Countries Maldives-Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Jump to: navigation, search Name Maldives-Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Agency/Company /Organization World Bank Sector Energy, Land Topics Background analysis, Finance, Implementation, Low emission development planning, Market analysis Website http://www.climatefundsupdate. Program Start 2009 Country Maldives UN Region Southern Asia References Program for Scaling Up Renewable Energy in Low Income Countries (SREP)[1] Ethiopia Specific Documents[2] Honduras Specific Documents[3] Kenya Specific Documents[4] Maldives Specific Documents[5] Mali Specific Documents[6] Nepal Specific Documents[7] Overview "The Scaling-Up Renewable Energy Program for Low Income Countries (SREP) is

9

Solar Resource Assessment for Sri Lanka and Maldives  

DOE Green Energy (OSTI)

The countries of Sri Lanka and the Maldives lie within the equatorial belt, a region where substantial solar energy resources exist throughout much of the year in adequate quantities for many applications, including solar water heating, solar electricity, and desalination. The extent of solar resources in Sri Lanka has been estimated in the past based on a study of the daily total direct sunshine hours recorded at a number of weather and agricultural stations throughout the country. These data have been applied to the well-known Angstrom relationship in order to obtain an estimate of the distribution of monthly average daily total solar resources at these stations. This study is an effort in improve on these estimates in two ways: (1) to apply a gridded cloud cover database at a 40-km resolution to produce updated monthly average daily total estimates of all solar resources (global horizontal, DNI, and diffuse) for the country, and (2) to input hourly or three-hourly cloud cover observations made at nine weather stations in Sri Lanka and two in the Maldives into a solar model that produces estimates of hourly solar radiation values of the direct normal, global, and diffuse resource covering the length of the observational period. Details and results of these studies are summarized in this report.

Renne, D.; George, R.; Marion, B.; Heimiller, D.; Gueymard, C.

2003-08-01T23:59:59.000Z

10

Technical Report - Sri Lanka and the Maldives Wind Energy Resource  

Open Energy Info (EERE)

Sri Lanka and the Maldives Wind Energy Resource Sri Lanka and the Maldives Wind Energy Resource Assessment Dataset Summary Description (Abstract): This document describes the development of detailed high-resolution (1 km2) wind energy resource maps for Sri Lanka and the Maldives. (Purpose): To provide information on the wind resource potential within Sri Lanka and the Maldives. Source NREL Date Released August 21st, 2006 (8 years ago) Date Updated August 21st, 2006 (8 years ago) Keywords documentation GEF GIS Maldives NREL Sri Lanka SWERA UNEP wind Data application/pdf icon Download Report (pdf, 30.1 MiB) Quality Metrics Level of Review Some Review Comment Temporal and Spatial Coverage Frequency Time Period 2006 License License Open Data Commons Public Domain Dedication and Licence (PDDL) Comment Restrictions to use (Use Constraints): This GIS data was developed by the National Renewable Energy Laboratory ("NREL"), which is operated by the Midwest Research Institute for the U.S. Department of Energy ("DOE"). The user is granted the right, without any fee or cost, to use, copy, modify, alter, enhance and distribute this data for any purpose whatsoever, provided that this entire notice appears in all copies of the data. Further, the user of this data agrees to credit NREL in any publications or software that incorporate or use the data. Access to and use of the GIS data shall further impose the following obligations on the User. The names DOE/NREL may not be used in any advertising or publicity to endorse or promote any product or commercial entity using or incorporating the GIS data unless specific written authorization is obtained from DOE/NREL. The User also understands that DOE/NREL shall not be obligated to provide updates, support, consulting, training or assistance of any kind whatsoever with regard to the use of the GIS data. THE GIS DATA IS PROVIDED "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL DOE/NREL BE LIABLE FOR ANY SPECIAL, INDIRECT OR CONSEQUENTIAL DAMAGES OR ANY DAMAGES WHATSOEVER, INCLUDING BUT NOT LIMITED TO CLAIMS ASSOCIATED WITH THE LOSS OF DATA OR PROFITS, WHICH MAY RESULT FROM AN ACTION IN CONTRACT, NEGLIGENCE OR OTHER TORTIOUS CLAIM THAT ARISES OUT OF OR IN CONNECTION WITH THE ACCESS OR USE OF THE GIS DATA. The User acknowledges that access to the GIS data is subject to U.S. Export laws and regulations and any use or transfer of the GIS data must be authorized under those regulations. The User shall not use, distribute, transfer, or transmit GIS data or any products incorporating the GIS data except in compliance with U.S. export regulations. If requested by DOE/NREL, the User agrees to sign written assurances and other export-related documentation as may be required to comply with U.S. export regulations.

11

Wind and Solar Resource Assessment of Sri Lanka and the Maldives (CD-ROM)  

DOE Green Energy (OSTI)

The Wind and Solar Resource Assessment of Sri Lanka and the Maldives CD contains an electronic version of Wind Energy Resource Atlas of Sri Lanka and the Maldives (NREL/TP-500-34518), Solar Resource Assessment for Sri Lanka and the Maldives (NREL/TO-710-34645), Sri Lanka Wind Farm Analysis and Site Selection Assistance (NREL/SR-500-34646), GIS Data Viewer (software and data files with a readme file), and Hourly Solar and Typical Meteorological Year Data with a readme file.

Elliott, D.; Schwartz, M.; Scott, G.; Haymes, S.; Heimiller, D.; George, R.

2003-08-01T23:59:59.000Z

12

Last resorts : a tour guide to territorial protection for the Republic of the Maldives  

E-Print Network (OSTI)

A two meter rise in sea levels projected by the end of this century threatens the sovereignty of the Maldivian nation state. While flight from the Maldives to establish a new homeland elsewhere has been proposed, the culture ...

Sleeper, Buck (Thomas Buck)

2011-01-01T23:59:59.000Z

13

M-1C.  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

M-1C. M-1C. fTZ. u.s. DEPARTl\IENT OF ENERGY EERE PROJECT MANAGEMENT CENTER NEPA DETERl\IINATION RECIPI ENT:City of Boston PROJECT TITLE: EECBG· City Of Boston (S) Page 1 01'2 STATE:MA Funding Opportunity Announc:ement Number OE-EEOOOO736/ EEC8G Proc:urementlnstrumcnt Number NEPA Control Number cm Number o Based on my review ofthc information (Onc:crning the proposed adion, as NEPA Complianc:c Offic:cr (authorizcd undcr DOE Order 45I.1A), I havc madc the following dctermination: ex, EA, EIS APPENDIX AND NUMBER: Oescription: 85.1 Actions to conserve energy, demonstrate potential energy conservation, and promote energy-efficiency that do not increase the indoor concentrations of potentially harmful substances. These actions may involve financial and technical

14

muMAG session report, Anaheim  

Science Conference Proceedings (OSTI)

µMAG Evening Session. 9th Joint MMM/Intermag Conference January 7, 2004 Anaheim, CA Bob McMichael, Session Chair Agenda: ...

2004-01-22T23:59:59.000Z

15

MagStar Technologies | Open Energy Information  

Open Energy Info (EERE)

Partnership Type Other Relationship LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now MagStar Technologies is a company located in Hopkins, MN....

16

Northern Tales: A Synthesis of MAGS Atmospheric and Hydrometeorological Research  

Science Conference Proceedings (OSTI)

The Mackenzie Global Energy and Water Cycle Experiment (GEWEX) Study (MAGS) is one of the continental-scale experiments approved specifically by GEWEX to better understand and model water and energy cycling at high latitudes. The project has gone ...

K. K. Szeto; R. E. Stewart; M. K. Yau; J. Gyakum

2007-09-01T23:59:59.000Z

17

AOCS Official Method M 1-92  

Science Conference Proceedings (OSTI)

Determination of Precision of Analytical Methods AOCS Official Method M 1-92 Methods Downloads Methods Downloads Official Methods and Recommended Practices of the AOCS (Methods) aocs applicants certified chemist chemists fats lab laboratories la

18

M1 Energy | Open Energy Information  

Open Energy Info (EERE)

M1 Energy M1 Energy Jump to: navigation, search Name M1 Energy Place Chicago, Illinois Zip 60604 Sector Renewable Energy Product M1 Energy invests in renewable energy projects either solely or in partnership. Their project scope is focused on small to medium-sized oil, gas and electricity projects. Coordinates 41.88415°, -87.632409° Loading map... {"minzoom":false,"mappingservice":"googlemaps3","type":"ROADMAP","zoom":14,"types":["ROADMAP","SATELLITE","HYBRID","TERRAIN"],"geoservice":"google","maxzoom":false,"width":"600px","height":"350px","centre":false,"title":"","label":"","icon":"","visitedicon":"","lines":[],"polygons":[],"circles":[],"rectangles":[],"copycoords":false,"static":false,"wmsoverlay":"","layers":[],"controls":["pan","zoom","type","scale","streetview"],"zoomstyle":"DEFAULT","typestyle":"DEFAULT","autoinfowindows":false,"kml":[],"gkml":[],"fusiontables":[],"resizable":false,"tilt":0,"kmlrezoom":false,"poi":true,"imageoverlays":[],"markercluster":false,"searchmarkers":"","locations":[{"text":"","title":"","link":null,"lat":41.88415,"lon":-87.632409,"alt":0,"address":"","icon":"","group":"","inlineLabel":"","visitedicon":""}]}

19

On the nonexistence of $[\\binom{2m}{m-1}, 2m, \\binom{2m-1}{m-1}]$, $m$ odd, complex orthogonal design  

E-Print Network (OSTI)

Complex orthogonal designs (CODs) are used to construct space-time block codes. COD $\\mathcal{O}_z$ with parameter $[p, n, k]$ is a $p\\times n$ matrix, where nonzero entries are filled by $\\pm z_i$ or $\\pm z^*_i$, $i = 1, 2,..., k$, such that $\\mathcal{O}^H_z \\mathcal{O}_z = (|z_1|^2+|z_2|^2+...+|z_k|^2)I_{n \\times n}$. Adams et al. in "The final case of the decoding delay problem for maximum rate complex orthogonal designs," IEEE Trans. Inf. Theory, vol. 56, no. 1, pp. 103-122, Jan. 2010, first proved the nonexistence of $[\\binom{2m}{m-1}, 2m, \\binom{2m-1}{m-1}]$, $m$ odd, COD. Combining with the previous result that decoding delay should be an integer multiple of $\\binom{2m}{m-1}$, they solved the final case $n \\equiv 2 \\pmod 4$ of the decoding delay problem for maximum rate complex orthogonal designs. In this paper, we give another proof of the nonexistence of COD with parameter $[\\binom{2m}{m-1}, 2m, \\binom{2m-1}{m-1}]$, $m$ odd. Our new proof is based on the uniqueness of $[\\binom{2m}{m-1}, 2m-1, \\binom{...

Li, Yuan

2011-01-01T23:59:59.000Z

20

PPG and MAG Team Up for Turbine Blade Research | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

PPG and MAG Team Up for Turbine Blade Research PPG and MAG Team Up for Turbine Blade Research PPG and MAG Team Up for Turbine Blade Research May 14, 2010 - 12:39pm Addthis Lindsay Gsell For more than 15 years, PPG Industries has been supplying fiberglass to the wind turbine production industry. Now, with more than $700,000 in Recovery Act funds, PPG and partner MAG Industrial Automation Systems are researching materials and processes that could result in stronger and more reliable wind blades. "Current materials need to be optimized to meet the demanding performance needs of today's largest wind blade designs," said Cheryl Richards, PPG global marketing manager in wind energy. According to Cheryl, wind turbine blades are produced by combining dry fiber glass fabrics with a strong resin to form a composite. This method is widely used in production,

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


21

Review of M-1 Plugging in Pipeline Results  

NLE Websites -- All DOE Office Websites (Extended Search)

PIPELINE PLUG PREVENTION: PIPELINE PLUG PREVENTION: Enlightenment Yielded From Initiative M-1 Testing Results Principal Investigator: Adam Poloski Presenter: Harold Adkins May 21, 2009 Outline Test purpose & design Invaluable literature information Stability map concept development Results/sedimentation observations General conclusions 2 M-1 Initiative Testing: Purpose & Design Investigate critical deposition velocity for slurries with wide range of properties to mimic large cross section of Hanford waste to be processed (WTP-RPT-175, Rev 0) Particle density (2.5 g/cc - 8 g/cc) Particle size (10 µm - 100 µm) Rheology (0, 3, 6 Pa) koalin composition Investigate influence of complex piping geometry (WTP- RPT-178, Rev 0) Investigate critical deposition velocity for a representative

22

A Novel MagPipe Pipeline transportation system using linear motor drives  

Science Conference Proceedings (OSTI)

A novel capsule pipeline transportation system using linear motor drives, called Magplane MagPipe, is under development with the intention to replace trucks and railways for hauling materials from the mine to the rail head, power plant, or processing plant with reduced operating cost and energy consumption. The initial demonstration of a MagPipe line in Inner Mongolia will be a 500-m-long double-pipe coal transport system with the design transportation capacity of 3 Mega-Mg per year. The pipeline consists of 6-m-long plastic pipe modules with an I-beam suspension system inside the pipe to carry sets of five coupled capsules. The pipe will also contain noncontinuous motor winding modules spaced at 50-m intervals. A set of Halbach-arrayed permanent magnets on the bottom of the capsules interact with the linear motor windings to provide propulsion. The motor is driven by variable frequency drives outside the pipe to control the speed. This paper briefly describes the overall MagPipe pipeline transportation system, including the preliminary conclusions of the linear synchronous motor analysis.

Fang, J.R.; Montgomery, D.B.; Roderick, L. [Magplane Technology Inc., Littleton, MA (United States)

2009-11-15T23:59:59.000Z

23

INSTALLATION MAG~NiX.ILRI DIVI8ION, CAN.fAN,CONN.  

Office of Legacy Management (LM)

INSTALLATION INSTALLATION MAG~NiX.ILRI DIVI8ION, CAN.fAN,CONN. .PERI,jD Aiq~+ 1, i950 TO: August 31, 195 .:\,.:. ,,., WORK SHEET FOR: I b WSIGNOR I. v DowChemical Go. Velasco, Texas ., Azlterprise Meetala cc Brooklyn, New York Meili $Worthin&m Hatboro, ?'a. LOT NO. '... I [ATERIAL SYnB,fJL KEASURED' NET WT. 100,007~ ( 4;020 I ! 19 ~, ANALYBIS % METAL/100 r, Noi. 23) METAL CONTENT INSTRUCTIONS: This sheet% will be Used.ln.preDarlng Haterlal Balance. 'The totals from the various ltams listed above ~111 be Inserted on the Material Balance Summary Sheet. Shipments ~111 he llated on this Work'Sheet separately With the-ConsIgnor and Consignee of each Shipment noted; Copies Of thls sheet ~111 accompany the naterlal Balance Summary Sheet at the end of the'month.

24

MAG2D: Interactive 2-1/2-dimensional magnetic modeling program (User's Guide and Documentation for Rev. 1)  

DOE Green Energy (OSTI)

MAG2D is an interactive computer program used for modeling 2-1/2-dimensional magnetic data. A forward algorithm is used to give the theoretical attraction of magnetic intensity at a station due to a perturbing body given by the initial model. The resultant model can then be adjusted for a better fit by a combination of manual adjustment, one-dimensional automatic search, and Marquardt inversion. MAG2D has an interactive data management system for data manipulation and display built around subroutines to do a forward problem, a one-dimensional direct search and an inversion. These subroutines were originally separate batch-mode programs.

Nutter, C.

1981-04-01T23:59:59.000Z

25

Spin-flip M1 giant resonance as a challenge for Skyrme forces  

E-Print Network (OSTI)

Despite a great success of the Skyrme mean-field approach in exploration of nuclear dynamics, it seems to fail in description of the spin-flip M1 giant resonance. The results for different Skyrme parameterizations are contradictory and poorly agree with experiment. In particular, there is no parameterization which simultaneously describes the one-peak gross structure of M1 strength in doubly magic nuclei and two-peak structure in heavy deformed nuclei. The reason of this mismatch could lie in an unsatisfactory treatment of spin correlations and spin-orbit interaction. We discuss the present status of the problem and possible ways of its solution. In particular, we inspect i) the interplay of the collective shift and spin-orbit splitting, ii) the isovector M1 response versus isospin-mixed responses, and iii) the role of tensor and isovector spin-orbit interaction.

V. O. Nesterenko; J. Kvasil; P. Vesely; W. Kleinig; P. -G. Reinhard; V. Yu. Ponomarev

2010-01-22T23:59:59.000Z

26

On Sojourn Times in the Finite Capacity $M/M/1$ Queue with Processor Sharing  

E-Print Network (OSTI)

We consider a processor shared $M/M/1$ queue that can accommodate at most a finite number $K$ of customers. We give an exact expression for the sojourn time distribution in the finite capacity model, in terms of a Laplace transform. We then give the tail behavior, for the limit $K\\to\\infty$, by locating the dominant singularity of the Laplace transform.

Zhen, Qiang

2009-01-01T23:59:59.000Z

27

MAG2D: Interactive 2-1/2-dimensional magnetic modeling program (User's Guide and Documentation for Rev. 1)  

SciTech Connect

MAG2D is an interactive computer program used for modeling 2-1/2-dimensional magnetic data. A forward algorithm is used to give the theoretical attraction of magnetic intensity at a station due to a perturbing body given by the initial model. The resultant model can then be adjusted for a better fit by a combination of manual adjustment, one-dimensional automatic search, and Marquardt inversion. MAG2D has an interactive data management system for data manipulation and display built around subroutines to do a forward problem, a one-dimensional direct search and an inversion. These subroutines were originally separate batch-mode programs.

Nutter, C.

1981-04-01T23:59:59.000Z

28

Enhanced oil recovery by micellar polymer flooding: M-1 project status report  

Science Conference Proceedings (OSTI)

Marathon Oil Co. has operated a large micellar-polymer project in S. Illinois. The M-1 Maraflood Project, encompasses ca 407 acres of the Main Robinson sand reservoir. The M-1 Project was developed using 5-spot patterns on 2 different spacing schemes; 248 acres were developed using 2.5-acre spacing; and 159 acres were developed using 5.0-acre spacing. The project utilizes 114 injection wells and 132 oil wells. Objectives of the project are to determine the economic feasibility of large-scale projects in waterflooded reservoirs and to compare the performance of the 2.5- and 5.0-acre patterns. Oil production increased from 150 bopd to a peak of 680 bopd. To date a total 848,000 bbl of tertiary oil have been produced. 11 references.

Hinchman, S.B.

1983-01-01T23:59:59.000Z

29

Isovector and isoscalar spin-flip M1 strengths in $^{11}$B  

E-Print Network (OSTI)

The $^{11}$B($^3$He$, t$), $^{11}$B($d, d'$), and $^{11}$B($p, p'$) reactions were measured at forward scattering angles including $0^\\circ$ to study the isovector and isoscalar spin-flip M1 strengths in $^{11}$B. The measured $^{11}$B($^3$He$, t$) cross sections were compared with the results of the distorted-wave impulse-approximation (DWIA) calculation, and the Gamow-Teller (GT) strengths for low-lying states in $^{11}$C were determined. The GT strengths were converted to the isovector spin-flip M1 strengths using the isobaric analog relations under the assumption of the isospin symmetry. The isoscalar spin-flip M1 strengths were obtained from the ($d, d'$) analysis by assuming that the shape of the collective transition form factor with the same ${\\Delta}J^\\pi$ is similar in the $^{11}$B($d, d'$) and $^{12}$C($d, d'$) reactions. The obtained isovector and isoscalar strengths were used in the DWIA calculations for the $^{11}$B($p, p'$) reaction. The DWIA calculation reasonably well explains the present $^{11}$B($p, p'$) result. However, the calculated cross section for the 8.92-MeV 3/2$^-_2$ state was significantly smaller than the experimental values. The transition strengths obtained in the shell-model calculations were found to be 20-50% larger than the experimental strengths. The transition strengths for the neutrino induced reactions were estimated by using the isovector and isoscalar spin-flip M1 strengths. The present results are quantitatively in agreement with the theoretical estimation discussing the axial isoscalar coupling in the neutrino scattering process, and are useful in the measurement of the stellar neutrinos using the neutral- and charged-current reactions on $^{11}$B.

T. Kawabata; H. Akimune; H. Fujimura; H. Fujita; Y. Fujita; M. Fujiwara; K. Hara; K. Y. Hara; K. Hatanaka; T. Ishikawa; M. Itoh; J. Kamiya; S. Kishi; M. Nakamura; K. Nakanishi; T. Noro; H. Sakaguchi; Y. Shimbara; H. Takeda; A. Tamii; S. Terashima; H. Toyokawa; M. Uchida; H. Ueno; T. Wakasa; Y. Yasuda; H. P. Yoshida; M. Yosoi

2004-06-24T23:59:59.000Z

30

Skyrme-Rpa Description of Spin-Flip M1 Giant Resonance  

E-Print Network (OSTI)

The spin-flip M1 giant resonance is explored in the framework of Random Phase Approximation on the basis of the Skyrme energy functional. A representative set of eight Skyrme parameterizations (SkT6, SkM*, SLy6, SG2, SkO, SkO', SkI4, and SV-bas) is used. Light and heavy, spherical and deformed nuclei ($^{48}$Ca, $^{158}$Gd, $^{208}$Pb, and $^{238}$U) are considered. The calculations show that spin densities play a crucial role in forming the collective shift in the spectrum. The interplay of the collective shift and spin-orbit splitting determines the quality of the description. None of the considered Skyrme parameterizations is able to describe simultaneously the M1 strength distribution in closed-shell and open-shell nuclei. It is found that the problem lies in the relative positions of proton and neutron spin-orbit splitting. Necessity to involve the tensor and isovector spin-orbit interaction is called for.

P. Vesely; J. Kvasil; V. O. Nesterenko; W. Kleinig; P. -G. Reinhard; V. Yu. Ponomarev

2009-07-06T23:59:59.000Z

31

Skyrme random-phase-approximation description of spin-flip M1 giant resonance  

SciTech Connect

The spin-flip M1 giant resonance is explored in the framework of the random-phase-approximation (RPA) on the basis of the Skyrme energy functional. A representative set of eight Skyrme parametrizations (SkT6, SkM*, SLy6, SG2, SkO, SkO', SkI4, and SV-bas) is used. Light and heavy, spherical and deformed nuclei ({sup 48}Ca, {sup 158}Gd, {sup 208}Pb, and {sup 238}U) are considered. The calculations show that spin densities play a crucial role in forming the collective shift in the spectrum. The interplay of the collective shift and spin-orbit splitting determines the quality of the description. None of the considered Skyrme parametrizations is able to describe simultaneously the M1 strength distribution in closed-shell and open-shell nuclei. It is found that the problem lies in the relative positions of proton and neutron spin-orbit splitting. This calls for a better modeling of the tensor and isovector spin-orbit interaction.

Vesely, P.; Kvasil, J. [Institute of Particle and Nuclear Physics, Charles University, CZ-18000, Praha 8 (Czech Republic); Nesterenko, V. O. [Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna, Moscow region, RU-141980 (Russian Federation); Kleinig, W. [Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna, Moscow region, RU-141980 (Russian Federation); Technische Universitaet Dresden, Inst. fuer Analysis, D-0106 Dresden (Germany); Reinhard, P.-G. [Institut fuer Theoretische Physik II, Universitaet Erlangen, D-91058 Erlangen (Germany); Ponomarev, V. Yu. [Institut fuer Kernphysik, Technische Universitaet Darmstadt, D-64289 Darmstadt (Germany)

2009-09-15T23:59:59.000Z

32

98 mag 3  

NLE Websites -- All DOE Office Websites (Extended Search)

National Laboratory 9700 S. Cass Avenue, Building 207 Argonne, IL 60439 ABSTRACT The laser beam weldability of AZ31B magnesium alloy was examined with high power CW CO 2 and...

33

mag div org chart  

NLE Websites -- All DOE Office Websites (Extended Search)

Magnet Division Magnet Division Peter Wanderer Division Head Administrative Support Diana Votruba (P/T), Ron Prwivo Division QA Rep. - Henry Hocker Building Manager - John Cintorino ES&H Coordinator- Walter Czejak Training Coordinator - Joyce Fortunato ECR - F. Craner Mechanical Engineering Mike Anerella Magnet Design, R&D, Testing Peter Wanderer Electrical Systems Piyush Joshi Technical Support R. Ceruti D. Carleton M. Hartsough D. Ince G. Jochen T. Levine D. Milidantri F. Teich T. Van Winckel Project Engineering J. Cozzolino A. Marone S. Plate J. Schmalzle __________________________________

34

ARM - VAP Product - 30smplcmask1zwang  

NLE Websites -- All DOE Office Websites (Extended Search)

Airport, Gan Island, Maldives GRW M1 Browse Data Graciosa Island, Azores, Portugal HFE M1 Browse Data Shouxian, Anhui, China PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1...

35

Customer Equilibrium and Optimal Strategies in an M/M/1 Queue with Dynamic Service Control  

E-Print Network (OSTI)

We consider the problem of customer equilibrium strategies in an M/M/1 queue under dynamic service control. The service rate switches between a low and a high value depending on system congestion. Arriving customers do not observe the system state at the moment of arrival. We show that due to service rate variation, the customer equilibrium strategy is not generally unique, and derive an upper bound on the number of possible equilibria. For the problem of social welfare optimization, we numerically analyze the relationship between the optimal arrival rate, which maximizes the overall welfare of the customers, and the equilibrium ones as a function of various parameter values. We finally derive analytic solutions for the special case where the service rate switch occurs when the queue ceases to be empty.

Dimitrakopoulos, Y

2011-01-01T23:59:59.000Z

36

The development and evaluation of a sensitive minicolumn assay for the detection of aflatoxin M1 in milk  

E-Print Network (OSTI)

The aflatoxins comprise a subgroup of mycotoxins usually produced by Aspergillus parasiticus or Aspergillus flavus. Dairy cattle which ingest aflatoxin-contaminated feed will excrete aflatoxin M1 into the milk. The presence of this metabolite in milk is a concern for humans. At the present time, the best method to prevent ingestion of contaminated milk is by detection and diversion from our food supply. A field-practical method for the chemiselective immobilization and detection of aflatoxin M1 (CSID-M1) in milk has been developed in our laboratory. In this new method, aflatoxin M1 (AfM1) is selectively adsorbed in a small glass minicolumn at the interface of a layer of packed neutral sand and a narrow band of magnesium silicate (or Florisil). AfM1, at a level of 0.5 ppb or greater in contaminated milk, can be easily detected as a band of bright blue fluorescence with this assay. Briefly, whole milk- is diluted with water and passed through a C18 Sep-Pak cartridge. AfM1 is then partitioned by polarity and eluted from the cartridge with 2.5% acetone in methylene chloride. The eluate (containing AfM1) is added to the minicolumn detector. The tube is then washed with 2% methanol in methylene chloride and viewed under longwave UV light for AfM1. The limit o detection for CSID-M1 assay was determined to be 0.2 ppb compared with 0.3 ppb AfM1 using an immunoaffinity column extraction. The CSID-M1 assay was found to accurate, exhibiting no false positives or false negatives under the experimental condition imposed in this study. Also, the CSID-M1 detectors were shown to be chemically stable requiring no refrigeration for storage up to 20 weeks. In summary, the CSID-M1 assay was shown to be rapid, practical, easy to perform, and stable, thus facilitating its use in the prescreening of milk.

Cathey, Carol Grmela

1993-01-01T23:59:59.000Z

37

On Sojourn Times in the $M/M/1$-PS Model, Conditioned on the Number of Other Users  

E-Print Network (OSTI)

We consider the $M/M/1$-PS queue with processor sharing. We study the conditional sojourn time distribution of an arriving customer, conditioned on the number of other customers present. A new formula is obtained for the conditional sojourn time distribution, using a discrete Green's function. This is shown to be equivalent to some classic results of Pollaczeck and Vaulot from 1946. Then various asymptotic limits are studied, including large time and/or large number of customers present, and heavy traffic, where the arrival rate is only slightly less than the service rate.

Zhen, Qiang

2009-01-01T23:59:59.000Z

38

An evaluation of the Robinson M-1 commercial scale demonstration of enhanced oil recovery by micellar-polymer flood  

SciTech Connect

A commercial scale micellar-polymer project was conducted in the Robinson Sand of the M-1 project in southwestern Illinois. The project utilized a crude oil sulfonate surfactant system to flood the reservoir which, at the time of the project, was in an advanced stage of waterflood depletion. Injected fluids consisted of a 0.10 pore volume crude oil sulfonate slug, a 1.05 pore volume graded mobility slug using Dow Pusher 700, and a drive water slug to depletion. Micellar injection started in 1977. By December, 1986, overall operations in the 2.5-acre pattern area were uneconomical while polymer injection was continuing in the 5.0-acre pattern area. Depletion of the 5.0-acre pattern area is forecast for 1991 or sooner. Ultimate oil recovery is estimated at 1,397,000 barrels with cumulative oil recovery at December, 1986, of 1,299,000 barrels. Although the crude oil sulfonate system successfully mobilized and produced waterflood residual oil, the project was not economic because of both lower than anticipated recovery and higher than expected operating costs. The lower than anticipated recovery is attributed to poor volumetric sweep efficiency and salinity/hardness effects. 7 refs., 54 figs., 25 tabs.

Cole, E.L.

1988-12-01T23:59:59.000Z

39

Safety Analysis Report for Packaging (SARP): Model AL-M1 nuclear packaging (DOE C of C No. USA/9507/BLF)  

Science Conference Proceedings (OSTI)

This Safety Analysis Report for Packaging (SARP) satisfies the request of the US Department of Energy for a formal safety analysis of the shipping container identified as USA/9507/BLF, also called AL-M1, configuration 5. This report makes available to all potential users the technical information and the limits pertinent to the construction and use of the shipping containers. It includes discussions of structural integrity, thermal resistance, radiation shielding and radiological safety, nuclear criticality safety, and quality control. A complete physical and technical description of the package is presented. The package consists of an inner container centered within an insulated steel drum. The configuration-5 package contains tritiated water held on sorbent material. There are two other AL-M1 packages, designated configurations 1 and 3. These use the same insulated outer drum, but licensing of these containers will not be addressed in this SARP. Design and development considerations, the tests and evaluations required to prove the ability of the container to withstand normal transportation conditions, and the sequence of four hypothetical accident conditions (free drop, puncture, thermal, and water immersion) are discussed. Tables, graphs, dimensional sketches, photographs, technical references, loading and shipping procedures, Monsanto Research Corporation-Mound experience in using the containers, and a copy of the DOE/OSD/ALO Certificate of Compliance are included.

Coleman, H.L.; Whitney, M.A.; Williams, M.A.; Alexander, B.M.; Shapiro, A.

1987-11-24T23:59:59.000Z

40

Propane ammoxidation over the Mo-V-Te-Nb-O M1 phase: Reactivity of surface cations in hydrogen abstraction steps  

Science Conference Proceedings (OSTI)

Density functional theory calculations (GGA-PBE) have been performed to investigate the adsorption of C3 (propane, isopropyl, propene, and allyl) and H species on the proposed active center present in the surface ab planes of the bulk Mo-V-Te-Nb-O M1 phase in order to better understand the roles of the different surface cations in propane ammoxidation. Modified cluster models were employed to isolate the closely spaced V=O and Te=O from each other and to vary the oxidation state of the V cation. While propane and propene adsorb with nearly zero adsorption energy, the isopropyl and allyl radicals bind strongly to V=O and Te=O with adsorption energies, {Delta}E, being {le} -1.75 eV, but appreciably more weakly on other sites, such as Mo=O, bridging oxygen (Mo-O-V and Mo-O-Mo), and empty metal apical sites ({Delta}E > -1 eV). Atomic H binds more strongly to Te = O ({Delta}E {le} -3 eV) than to all the other sites, including V = O ({Delta}E = -2.59 eV). The reduction of surface oxo groups by dissociated H and their removal as water are thermodynamically favorable except when both H atoms are bonded to the same Te=O. Consistent with the strong binding of H, Te=O is markedly more active at abstracting the methylene H from propane (E{sub a} {le} 1.01 eV) than V = O (E{sub a} = 1.70 eV on V{sup 5+} = O and 2.13 eV on V{sup 4+} = O). The higher-than-observed activity and the loose binding of Te = O moieties to the mixed metal oxide lattice of M1 raise the question of whether active Te = O groups are in fact present in the surface ab planes of the M1 phase under propane ammoxidation conditions.

Muthukumar, Kaliappan [University of Cincinnati; Yu, Junjun [University of Cincinnati; Xu, Ye [ORNL; Guliants, Vadim V. [University of Cincinnati

2011-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


41

Search for 14.4-KeV Solar Axions Emitted in the M1-Transition of Fe-57 Nuclei with CAST  

SciTech Connect

We have searched for 14.4 keV solar axions or more general axion-like particles (ALPs), that may be emitted in the M1 nuclear transition of 57Fe, by using the axion-to-photon conversion in the CERN Axion Solar Telescope (CAST) with evacuated magnet bores (Phase I). From the absence of excess of the monoenergetic X-rays when the magnet was pointing to the Sun, we set model-independent constraints on the coupling constants of pseudoscalar particles that couple to two photons and to a nucleon g{sub ay}|-1.19g{sub aN}{sup 0}+g{sub aN}{sup 3}| < 1.36 x 10{sup -16} GeV{sup -1} for ma < 0.03 eV at the 95% confidence level.

Andriamonje, S.; Aune, S.; /DAPNIA, Saclay; Autiero, D.; /CERN /Lyon, IPN; Barth, K.; /CERN; Belov, A.; /Moscow, INR; Beltran, B.; /Zaragoza U. /Queen's U., Kingston; Brauninger, H.; /Garching, Max Planck Inst., MPE; Carmona, J.M.; Cebrian, S.; /Zaragoza U.; Collar, J.I.; /Chicago U., EFI /Chicago U., KICP; Dafni, T.; /DAPNIA, Saclay /Darmstadt, Tech. Hochsch. /Zaragoza U.; Davenport, M.; /CERN; Di Lella, L.; /CERN /Pisa, Scuola Normale Superiore; Eleftheriadis, C.; /Aristotle U., Thessaloniki; Englhauser, J.; /Garching, Max Planck Inst., MPE; Fanourakis, G.; /Democritos Nucl. Res. Ctr.; Ferrer-Ribas, E.; /DAPNIA, Saclay; Fischer, H.; Franz, J.; /Freiburg U.; Friedrich, P.; /Garching, Max Planck Inst., MPE; Geralis, T.; /Democritos Nucl. Res. Ctr. /DAPNIA, Saclay /Moscow, INR /Zaragoza U. /British Columbia U. /Freiburg U. /Darmstadt, Tech. Hochsch. /DAPNIA, Saclay /Zaragoza U. /Frankfurt U. /Boskovic Inst., Zagreb /Freiburg U. /Munich, Max Planck Inst. /Boskovic Inst., Zagreb /Democritos Nucl. Res. Ctr. /Darmstadt, Tech. Hochsch. /Garching, Max Planck Inst., MPE /Boskovic Inst., Zagreb /CERN /Aristotle U., Thessaloniki /Boskovic Inst., Zagreb /Munich, Max Planck Inst. /Zaragoza U. /Chicago U., EFI /Chicago U., KICP /Stanford U., Phys. Dept. /SLAC /Zaragoza U. /CERN /DAPNIA, Saclay /CERN /Munich, Max Planck Inst. /Darmstadt, Tech. Hochsch. /Zaragoza U. /Aristotle U., Thessaloniki /Patras U. /Brookhaven /CERN /Munich, Max Planck Inst. /CERN /Chicago U., EFI /Chicago U., KICP /Zaragoza U. /Freiburg U. /CERN /CERN /Patras U.

2011-12-02T23:59:59.000Z

42

STEM HAADF Image Simulation of the Orthorhombic M1 Phase in the Mo-V-Nb-Te-O Propane Oxidation Catalyst  

Science Conference Proceedings (OSTI)

A full frozen phonon multislice simulation of high angle annular dark field scanning transmission electron microscopy (HAADF STEM) images from the M1 phase of the Mo-V-Nb-Te-O propane oxidation catalyst has been performed by using the latest structural model obtained using the Rietveld method. Simulated contrast results are compared with experimental HAADF images. Good agreement is observed at ring sites, however significant thickness dependence is noticed at the linking sites. The remaining discrepancies between the model based on Rietveld refinement and image simulations indicate that the sampling of a small volume element in HAADF STEM and averaging elemental contributions of a disordered site in a crystal slab by using the virtual crystal approximation might be problematic, especially if there is preferential Mo/V ordering near the (001) surface.

D Blom; X Li; S Mitra; T Vogt; D Buttrey

2011-12-31T23:59:59.000Z

43

NORTHEAST OREGON W I L D L I F E M 1 T I G AT I 0 N P R 0 J  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

NORTHEAST OREGON NORTHEAST OREGON W I L D L I F E M 1 T I G AT I 0 N P R 0 J E CT FINAL ENVIRONMENTAL ASSESSMENT DOE/EA-1160 DEC 1 3 1996 U S T I Northeast Oregon' Wildlife Mitigation Project Environmental Assess men t Table of Contents CHAPTER 1: PURPOSE OF AND NEED FOR ACTION 1 1 . 1.1 Underlying Need for Action 1.2 Purposes 1 CHAPTER 2: ALTERNATIVES, INCLUDING THE PROPOSED ACTION 2 2.1 Proposed Action 2 2.2 No Action 4 ENVIRONMENTAL IMPACTS OF THE PROPOSED ACTION AND ALTERNATIVES 6 CHAPTER 3: 3.1 Water Quality 7 3.2 Vegetation 8 3.3 Fish and Wildlife 9 3.4 Land Use 10 3.5 Cultural Resources 11 3.6 Air Quality 12 CHAPTER 4: PERSONS AND AGENCIES CONSULTED 13 CHAPTER 5: REFERENCES 13 Table 1: predicted Performance Summary 5 Table 1: predicted Performance Summary 5

44

Adsorption of propane, isopropyl, and hydrogen on cluster models of the M1 phase of Mo-V-Te-Nb-O mixed metal oxide catalyst  

Science Conference Proceedings (OSTI)

The Mo-V-Te-Nb-O mixed metal oxide catalyst possessing the M1 phase structure is uniquely capable of directly converting propane into acrylonitrile. However, the mechanism of this complex eight-electron transformation, which includes a series of oxidative H-abstraction and N-insertion steps, remains poorly understood. We have conducted a density functional theory study of cluster models of the proposed active and selective site for propane ammoxidation, including the adsorption of propane, isopropyl (CH{sub 3}CHCH{sub 3}), and H which are involved in the first step of this transformation, that is, the methylene C-H bond scission in propane, on these active site models. Among the surface oxygen species, the telluryl oxo (Te=O) is found to be the most nucleophilic. Whereas the adsorption of propane is weak regardless of the MO{sub x} species involved, isopropyl and H adsorption exhibits strong preference in the order of Te=O > V=O > bridging oxygens > empty Mo apical site, suggesting the importance of TeO{sub x} species for H abstraction. The adsorption energies of isopropyl and H and consequently the reaction energy of the initial dehydrogenation of propane are strongly dependent on the number of ab planes included in the cluster, which points to the need to employ multilayer cluster models to correctly capture the energetics of surface chemistry on this mixed metal oxide catalyst.

Govindasamy, Agalya [University of Cincinnati; Muthukumar, Kaliappan [University of Cincinnati; Yu, Junjun [University of Cincinnati; Xu, Ye [ORNL; Guliants, Vadim V. [University of Cincinnati

2010-01-01T23:59:59.000Z

45

µMAG: Micromagnetic Modeling Activity Group  

Science Conference Proceedings (OSTI)

... Understanding these structures is key to technologies such as information storage, spintronics, and sensors as well as to the use of magnetism to ...

2013-07-23T23:59:59.000Z

46

µMAG Standard Problem #4 results  

Science Conference Proceedings (OSTI)

... J.Miltat and A.Thiaville, IMACS 2000 World Congress Proceedings G.Albuquerque, J.Miltat and A.Thiaville, Joint MMM-Intermag Conference 2001 ...

2007-04-26T23:59:59.000Z

47

µMAG Standard Problem #4 results  

Science Conference Proceedings (OSTI)

... References: LD Buda, IL Prejbeanu, M. Demand, U. Ebels and K. Ounadjela, The 8th Joint MMM-Intermag Conference 2001 Proceedings ...

2007-04-26T23:59:59.000Z

48

The MAGS Water and Energy Budget Study  

Science Conference Proceedings (OSTI)

This study represents the first attempt at developing a comprehensive climatology of atmospheric and surface water and energy budgets for the Mackenzie River basin (MRB). Different observed, remotely sensed, (re)analyzed, and modeled datasets ...

K. K. Szeto; H. Tran; M. D. MacKay; R. Crawford; R. E. Stewart

2008-02-01T23:59:59.000Z

49

SimulMag Version 1.0  

Science Conference Proceedings (OSTI)

... AMR Anisotropic magnetoresistance GMR Giant magnetoresistance ... For a detailed description of the modeling of giant magnetoresistance see Sec. ...

1999-02-17T23:59:59.000Z

50

The influence of Asian monsoon variability on precipitation patterns over the Maldives.  

E-Print Network (OSTI)

??Asian climate varies on various spatial and temporal scales and has a wide spectrum of climatic characteristics. Climate variability, especially decadal to inter-annual scale rainfall… (more)

Zahid

2011-01-01T23:59:59.000Z

51

ARM - Instrument - mwr3c  

NLE Websites -- All DOE Office Websites (Extended Search)

MAG M1 Browse Data Los Angeles, CA to Honolulu, HI - container ship Horizon Spirit OLI M1 Browse Data Oliktok Point, Alaska PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1...

52

Climate Mag_27JUN2013_ms07022013.indd  

NLE Websites -- All DOE Office Websites (Extended Search)

CLIMATE CLIMATE AND IMPACT RESEARCH at Los Alamos National Laboratory Climate Research and National Security Los Alamos National Laboratory is truly a national security science laboratory, tackling some of the world's most challenging science and engineering issues. We are interested in the potential future impacts of climate change on global security, such as the coastal e ects of sea level rise, increased number of extreme storms, and the consequences of extensive regional tree mortality. Gaining a better understanding of the forces behind global climate change-how these forces operate, how they may a ect us, and how we might mitigate their negative impacts-brings together biologists, physicists, mathematicians, geologists, electrical engineers, computer

53

Fine coal cleaning via the micro-mag process  

SciTech Connect

A method of cleaning particulate coal which is fed with a dense medium slurry as an inlet feed to a cyclone separator. The coal particle size distribution is in the range of from about 37 microns to about 600 microns. The dense medium comprises water and ferromagnetic particles that have a relative density in the range of from about 4.0 to about 7.0. The ferromagnetic particles of the dense medium have particle sizes of less than about 15 microns and at least a majority of the particle sizes are less than about 5 microns. In the cyclone, the particulate coal and dense-medium slurry is separated into a low gravity product stream and a high gravity produce stream wherein the differential in relative density between the two streams is not greater than about 0.2. The low gravity and high gravity streams are treated to recover the ferromagnetic particles therefrom.

Klima, Mark S. (Finleyville, PA); Maronde, Carl P. (McMurray, PA); Killmeyer, Richard P. (Pittsburgh, PA)

1991-01-01T23:59:59.000Z

54

Nuclear Power Plant Fire Modeling Application Guide (NPP FIRE MAG)  

Science Conference Proceedings (OSTI)

There is a movement to introduce risk-informed and performance-based (RI/PB) analyses into fire protection engineering practice, both domestically and worldwide.  This movement exists in both the general fire protection and the nuclear power plant (NPP) fire protection communities.  The U.S. Nuclear Regulatory Commission (NRC) has used risk-informed insights as a part of its regulatory decision making since the 1990s.In 2001, the National Fire Protection Association (NFPA) ...

2012-11-30T23:59:59.000Z

55

MagSonic™ Carbothermal Technology Compared with the ...  

Science Conference Proceedings (OSTI)

Carbothermal technology is advantageous on all measures except capital intensity (where it is roughly twice the capital cost of a similarly-sized Pidgeon plant).

56

CULHAM LOCAL LIAISON COMMITTEE Meeting Reference CLLC(12)M1  

E-Print Network (OSTI)

Publication Mail: 40062527 Meet Memorial's newest female electrical apprentice 2 Discover Delores Wheeler in electrical pursuits, excelling in math and science. That led her to a nine- month industrial electrician a job here at Memorial in November 2007 as one of two industrial electrician apprentices with Facilities

57

Revised 8/24/2010 Cooper, S.M. 1  

E-Print Network (OSTI)

for Research on Adolescence, San Francisco. Kizzie, K. & Cooper, S.M. (2006). Perceived discrimination, racial

Almor, Amit

58

WWVB Radio Controlled Clocks: Recommended Practices for ...  

Science Conference Proceedings (OSTI)

... 4, British Indian Ocean Territory (Chagos), Kerguelen Island, Maldives Islands, Turkmenistan, Tajikistan, Pakistan, Uzbekistan ,Western Kazakhstan ...

2009-09-08T23:59:59.000Z

59

NIST Global Standards Information WTO TBT Inquiry Point  

Science Conference Proceedings (OSTI)

... Republic; Maldives; Nepal; Pakistan; Russia; Sri Lanka; Turkmenistan; Uzbekistan. Asia-Pacific: Australia; Brunei Darussalam; ...

60

NIST Global Standards Information Global Standards News  

Science Conference Proceedings (OSTI)

... Republic; Maldives; Nepal; Pakistan; Russia; Sri Lanka; Turkmenistan; Uzbekistan. Asia-Pacific: Australia; Brunei Darussalam; ...

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


61

NIST Global Standards Information EMC/Telecom MRAs  

Science Conference Proceedings (OSTI)

... Republic; Maldives; Nepal; Pakistan; Russia; Sri Lanka; Turkmenistan; Uzbekistan. Asia-Pacific: Australia; Brunei Darussalam; ...

62

ARM - Datastreams - aosuhsas  

NLE Websites -- All DOE Office Websites (Extended Search)

( binnum ) Locations ARM Mobile Facility MAG M1 Browse Data Los Angeles, CA to Honolulu, HI - container ship Horizon Spirit PVC S1 Browse Data Highland Center, Cape Cod MA; MAOS...

63

LANL | TT | License | MagViz - Los Alamos National Lab: National ...  

Operated by Los Alamos National Security, LLC for the U.S. Department of Energy's NNSA. Inside | © Copyright 2010-11 Los Alamos National Security, ...

64

Mag Feet : a robotic device for the inspection of steel bridge structures  

E-Print Network (OSTI)

The aging of America's steel bridges presents many challenges. Undetected cracks and corrosion can eventually lead to catastrophic failure. Due to the difficulties with inspecting existing bridges the use of mobile robots ...

Mazumdar, Anirban

2009-01-01T23:59:59.000Z

65

The causes and consequences of tax policy  

E-Print Network (OSTI)

Tax Revenue Country Bosnia and Herzegovina Maldives MoldovaTax Jordan Seychelles Bosnia and Herzegovina Macao, China

Weller, Nicholas William

2008-01-01T23:59:59.000Z

66

NIST Global Standards Information Navigation Tips  

Science Conference Proceedings (OSTI)

... The United States Central & South Asia Afghanistan Bangladesh Bhutan India Kazakhstan Kyrgyz Republic Maldives Nepal Pakistan Russia Sri ...

67

C:\MYDOCS\FBSS-M~1\HATTIE\LAYOUT94.TXT  

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

1993 Federal Buildings Supplemental Survey 1993 Federal Buildings Supplemental Survey Survey Data File Documentation Energy Information Administration August 1997 Overview of Survey Data File Documentation This document contains only the file layouts and variable codes for use with the 1993 Public Use files. For information on the FBSS and the organization and use of these files, please go to http://www/eia.doe.gov/emeu/cbecs/contents.html and click on: "1993 Micro-Data Files." Layout of Data Files A file layout is provided here for each of the 22 files. Column 1 is the variable name that is found in the files; column 2 is a brief description of the variable; column 3 is the variable position on the files.

68

M1L11OR04020102 IASCC initial Assessment Results Rev2  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

0/346 0/346 Assessment of Initial Test Conditions for Experiments to Assess Irradiation Assisted Stress Corrosion Cracking Mechanisms December 2010 Prepared by J.T. Busby and M.N. Gussev Oak Ridge National Laboratory This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsibility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Reference herein to any specific commercial product, process, or service by trade name, trademark, manufacturer, or

69

Water/Wastewater Engineering Report (Storm Sewer/Infiltration Sanitary Sewage Separation-M1 Model)  

E-Print Network (OSTI)

In some cities, the municipal sewer system collects both storm water and sanitary sewage in the same pipes. During dry weather these sewers carry all the sanitary sewage to the wastewater treatment plant for treatment. However, when rainstorms or snow melt increase the amount of runoff, the combined flow of sanitary sewage and storm water can exceed the capacity of the sewer system, which can cause serious problems like the storm water and sewage mix are discharged untreated into the river or the sewage backs up into streets and basement. Storm water treated in the sewage treatment plant also causes unnecessary energy use. Sewer systems can also have unintended ground water entering the network, which occurs because of hydraulic pressure on the buried sewer lines infiltration. Therefore, separating the storm water/infiltration and sanitary sewage reduces the possibility of sewage discharge during heavy rain periods, and saves energy.

Liu, Z.; Brumbelow, K.; Haberl, J. S.

2006-10-30T23:59:59.000Z

70

M1: Fabrication of Bulk Nanocrystalline Ni-W with Plastic ...  

Science Conference Proceedings (OSTI)

About this Abstract. Meeting, The 8th Pacific Rim International Congress on Advanced Materials and Processing. Symposium, M. Bulk Metallic Glasses, ...

71

M-1: Acid Cleaning of Titanium Based Scales Formed on Preheaters ...  

Science Conference Proceedings (OSTI)

This paper reports an acid formulation which is best suited for titanium based scales. ... Extracting Alumina from Coal Fly Ash Using Acid Sintering-Leaching ...

72

SI}M!1ARY REPORT ON SITE nnTESTIGATION AND REMOVAL ACTIVITIES  

E-Print Network (OSTI)

du.ring the removal operations on the site.. The Response, Engineering! and &!'1alytical Contractor codes') . In 1987, CSMRI contracted with Jacobs Engineering, Inc. (Jacobs) to provide a site assessment State Engineers office inspected the dam and recommended the repairs be initiated immediately to prevent

73

u.s. DEPARIMENT OF ENERGY EERE PROJECT M~'1AGEMENT ...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

energy, demonstrate potential energy conservation, and promote energy-efficiency thai do not increase the indoor concentrations of potentially harmful substances. These...

74

Correlations between charge radii, E0 transitions, and M1 strength  

E-Print Network (OSTI)

In the framework of the interacting boson model, relations are derived between nuclear charge radii, electric monopole transition rates, and summed magnetic dipole transition in even-even nuclei. The proposed correlations are tested in the rare-earth region.

Van Isacker, P

2013-01-01T23:59:59.000Z

75

Correlations between charge radii, E0 transitions, and M1 strength  

E-Print Network (OSTI)

In the framework of the interacting boson model, relations are derived between nuclear charge radii, electric monopole transition rates, and summed magnetic dipole transition in even-even nuclei. The proposed correlations are tested in the rare-earth region.

P. Van Isacker

2013-06-12T23:59:59.000Z

76

31.02.09.M1 Optional Retirement Program Page 1 of 3 UNIVERSITY RULE  

E-Print Network (OSTI)

of the employee's total compensation to the Optional Retirement Program (ORP). Percentages for both the em- ployee in ORP is allowed to withdraw onlythe contributions the employee made to the Teacher Retirement System (TRS) plus any accrued interest. Moneyrefunded byTRS to ORP participants is subject to the normal

77

M1, Material and Electronic Properties of CVD Graphene Grown on ...  

Science Conference Proceedings (OSTI)

GG6, Thermomagnetic Transport Properties of (AgxSbTex/2+1)15(GeTe)85 Thermoelectric Materials · GG7, Thermoelectric Properties of Sn-Rich Pb1?xSnx

78

Radiative Heat Transfer in a Hydrous Mantle Transition Zone Thomas, S.-M.1,2  

E-Print Network (OSTI)

, USA 3 Geophysical Laboratory, Carnegie Institution of Washington, Washington, DC 20015, USA craig spectra reveals an energy transmission "window" in the IR-VIS spectral range, as for both mineral phases-3260 [15] F.C. Marton, T.J. Shankland, D.C. Rubie and Y. Xu (2005) "Effect of variable thermal con

Bina, Craig R.

79

Feedback suppression of the internal m = 1 helical mode in a tokamak  

SciTech Connect

A stabilization system that measures the boundary of the plasma filament and controls the perturbation of the magnetic field outside the plasma is discussed. (AIP)

Mikhailovskii, A.B.

1979-03-01T23:59:59.000Z

80

Mechanics and Dynamics of the Strain-induced M1-M2 Structural ...  

Science Conference Proceedings (OSTI)

Symposium, O. Advanced Neutron and Synchrotron Studies of Materials .... Status of China Spallation Neutron Source and Perspectives of Neutron Research in ...

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


81

M1L11OR04020102 IASCC initial Assessment Results Rev2  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

of Energy Office of Nuclear Energy Light Water Reactor Sustainability Materials Aging and Degradation Pathway Prepared by OAK RIDGE NATIONAL LABORATORY Oak Ridge, Tennessee...

82

12/16/07 12:50 PMID3Mag.com -The Pulse of Podcasting Page 1 of 2http://finance.id3mag.com/id3?ChannelID=3206&GUID=3074055&Page=MediaViewer  

E-Print Network (OSTI)

, Dec 14, 2007 06:45 PM UN Climate Conference Hears How EO Can Help 06:45 PM Two New Landfill Gas-to-Energy Facilities Commence Operation In Virginia 06:45 PM Return To Europa: A Closer Look Is Possible 06:45 PM

Glaser, Rainer

83

Extension of Studies with 3M Empore TM and Selentec MAG *SEP SM Technologies for Improved Radionuclide Field Sampling  

Science Conference Proceedings (OSTI)

The Savannah River Technology Center is evaluating new field sampling methodologies to more easily determine concentrations of radionuclides in aqueous systems. One methodology studied makes use of 3M EmporeTM disks. The disks are composed of selective resins embedded in a Teflon support. The disks remove the ion of interest from aqueous solutions when the solution is passed through the disk. The disk can then be counted directly to quantify the isotope of interest. Four types of disks were studied during this work: for the extraction of technetium (two types), cesium, plutonium, and strontium. A sampler has been developed for automated, unattended, in situ use of the EmporeTM disks.

Beals, D.M. [Westinghouse Savannah River Company, AIKEN, SC (United States); Bibler, J.P.; Brooks, D.A.

1996-07-10T23:59:59.000Z

84

Supporting the Zero Emissions Strategy | Open Energy Information  

Open Energy Info (EERE)

the Zero Emissions Strategy the Zero Emissions Strategy Jump to: navigation, search Name Maldives - Supporting the Zero Emissions Strategy Agency/Company /Organization German Agency for International Cooperation (GIZ) Partner Federal Ministry for the Environment, Nature Conservation and Nuclear Safety (BMU) Sector Energy Focus Area Energy Efficiency Topics Low emission development planning, Pathways analysis Program Start 2011 Program End 2013 Country Costa Rica, Maldives Central America, Southern Asia References GTZ Schwerpunkte[1] GIZ[2] Contents 1 Overview 1.1 Costa Rica 1.2 Maldives 2 Outcomes, Lessons Learned and Good Practices 3 References Overview Costa Rica Maldives The Maldives are less the 2.5 m above sea level. Hence, the danger from climate change is crucial. At the same time the Maldives' economy,

85

ARM - AMF Data  

NLE Websites -- All DOE Office Websites (Extended Search)

2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat...

86

ARM - AMF3 Baseline Instruments  

NLE Websites -- All DOE Office Websites (Extended Search)

2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat...

87

ARM - AMF Operations  

NLE Websites -- All DOE Office Websites (Extended Search)

2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat...

88

ARM - AMF1 Baseline Instrument  

NLE Websites -- All DOE Office Websites (Extended Search)

2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat...

89

ARM Publications Database  

NLE Websites -- All DOE Office Websites (Extended Search)

Sites: ARM Instruments: Data Products: AMF - Black Forest, Germany (FKB) AMF - Cape Cod, Massachusetts (PVC) AMF - Gan Island, Maldives (GAN) AMF - Ganges Valley, India (PGH)...

90

ARM - AMF Architecture  

NLE Websites -- All DOE Office Websites (Extended Search)

2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat...

91

ARM - AMF Contacts  

NLE Websites -- All DOE Office Websites (Extended Search)

2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat...

92

ARM - AMF Science  

NLE Websites -- All DOE Office Websites (Extended Search)

2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat...

93

ARM - AMF2 Baseline Instruments  

NLE Websites -- All DOE Office Websites (Extended Search)

2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat...

94

ARM - Site Instruments  

NLE Websites -- All DOE Office Websites (Extended Search)

2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat...

95

A bioeconomic analysis of Maldivian skipjack tuna fishery .  

E-Print Network (OSTI)

??Skipjack tuna fishery in the Maldives is the most important and by far the predominant fishery in the country. This fishery is an open access… (more)

Mohamed, Solah

2007-01-01T23:59:59.000Z

96

South Asia Regional Initiative for Energy Cooperation and Development...  

Open Energy Info (EERE)

Background analysis Website http:www.usaid.govourwork Country Afghanistan, Pakistan, Bhutan, India, Sri Lanka, Bangladesh, Nepal, Maldives Southern Asia, Southern Asia,...

97

OPEN 4:30p.m. 1:00a.m. daily (except University holidays)  

E-Print Network (OSTI)

.79 Gatorade: Red, Yellow, Orange, Light Blue, Medium Blue; G2: Red, Orange, Purple, Dark Blue Canned Soda, 12 Wings and 2 Large Wedges $49.99 Three Sbarro Cheese Pizzas $37.99 Pizza and Wing Special: One Topping Pizza and 20 Wings $29.99 Specials Sbarro Pizza Made with all-natural ingredients, including dough made

Raina, Ramesh

98

A.E. K.Ris Ris -M -1 i34b Title and author(s)  

E-Print Network (OSTI)

UBHUUTINt PLOTOLtY.P.IA.AA.BB»TITLE) C C 1) XX(L> · L « MAXIMUM NUMBER OF CHANNELS OINENSIUN r(ft00) HEAL TITLE(20HULINE · 37M ·40H SUM«0. DO V01 I»VI .V.3 SUM-SUM.h

99

SampleID: 53051 Test Date: 4/17/2010 mean,std_dev,n,m1 ...  

Science Conference Proceedings (OSTI)

... 233.2,48238 231.57,3.09294762322286,5,233.2,230.49,227.77,230.49,235.91, 48241 240.5,3.92874025611264,5,238.7,242.2,241.1,245.5,235 ...

2012-10-09T23:59:59.000Z

100

Phase I A Phase I B Phase I C  

Office of Legacy Management (LM)

300 Mag-82 Mag-81 Mag-80 Mag-83 Mag-84 Mound Closure Project - Current Parcels and Buildings FILE NAME: mndbldgparcelownerc.mxd DATE: Legend Parcel - DOE Parcel - MMCIC Pond...

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


101

OSP WEEKLY FUNDING BULLETIN Volume 5, Issue 13 March 28, 2011  

E-Print Network (OSTI)

Lanka, and the Maldives) and the Youth Leadership Program with Azerbaijan Solicitation No. ECA Asia (Nepal, Sri Lanka, and the Maldives) and the Youth Leadership Program with Azerbaijan. Public, Nepal, Sri Lanka, and the United States. For the Youth Leadership Program with Azerbaijan, hereinafter

Alabama in Huntsville, University of

102

16. Zaanen, J., Osman, Y., Kruis, H. V., Nussinov, Z. & Tworzydlo, J. The geometric order of stripes and Luttinger liquids. Phil. Mag. B 81, 14851531 (2001).  

E-Print Network (OSTI)

such as the Siberian Traps (,250 million years ago) and the Karoo Igneous Province (,183 million years ago). A huge

103

GalaxyCount: a JAVA calculator of galaxy counts and variances in multiband wide-field surveys to 28 AB mag  

E-Print Network (OSTI)

We provide a consistent framework for estimating galaxy counts and variances in wide-field images for a range of photometric bands. The variances include both Poissonian noise and variations due to large scale structure. We demonstrate that our statistical theory is consistent with the counts in the deepest multiband surveys available. The statistical estimates depend on several observational parameters (e.g. seeing, signal to noise ratio), and include a sophisticated treatment of detection completeness. The JAVA calculator is freely available and offers the user the option to adopt our consistent framework or a different scheme. We also provide a summary table of statistical measures in the different bands for a range of different fields of view. Reliable estimation of the background counts has profound consequences in many areas of observational astronomy. We provide two such examples. One is from a recent study of the Sculptor galaxy NGC 300 where stellar photometry has been used to demonstrate that the outer disc extends to 10 effective radii, far beyond what was thought possible for a normal low-luminosity spiral. We confirm this finding by a reanalysis of the background counts. Secondly, we determine the luminosity function of the galaxy cluster Abell 2734, both through spectroscopically determined cluster membership, and through statistical subtraction of the background galaxies using the calculator and offset fields. We demonstrate very good agreement, suggesting that expensive spectroscopic follow-up, or off-source observations, may often be bypassed via determination of the galaxy background with GalaxyCount.

S. C. Ellis; J. Bland-Hawthorn

2006-02-27T23:59:59.000Z

104

Love this PDF? Add it to your Reading List! 4 joliprint.com/mag Pesticide kills bee colonies by turning insects into `picky  

E-Print Network (OSTI)

on the learning capacity and performance of bees We rely on a varied cocktail of pesticides to protect crops from will study the brain cells of bees in the laboratory to monitor the effects of pesticides (both single pest damage. Pesticides are also used to protect bees from mite infestation. Exposure to such chemicals

Nieh, James

105

IEEE Transactions on Magn@ticS, V O l . MAG-13, No. 1, January 1977 LOSSESINTWISTEDCOMPOSITESUPERCONDUCTORS IN A HIGHPULSEDMAGNETIC FIELD  

E-Print Network (OSTI)

gas holder with a water seal. The entrainment of liquid droplets by the gas is precluded by means values with the aid of calibrated pulsed heaters. The scatter of the measured en- ergy values relative a so varies synchronously with For the theoretical analysis of losses in twisted compos- ite

Mints, Roman G.

106

Costa Rica-Supporting the Zero Emissions Strategy of Costa Rica | Open  

Open Energy Info (EERE)

Costa Rica-Supporting the Zero Emissions Strategy of Costa Rica Costa Rica-Supporting the Zero Emissions Strategy of Costa Rica Jump to: navigation, search Name Costa Rica-Supporting the Zero Emissions Strategy Agency/Company /Organization German Agency for International Cooperation (GIZ) Partner Federal Ministry for the Environment, Nature Conservation and Nuclear Safety (BMU) Sector Energy Focus Area Energy Efficiency Topics Low emission development planning, Pathways analysis Program Start 2011 Program End 2013 Country Costa Rica Central America References GTZ Schwerpunkte[1] GIZ[2] Contents 1 Overview 1.1 Costa Rica 1.2 Maldives 2 Outcomes, Lessons Learned and Good Practices 3 References Overview Costa Rica Maldives The Maldives are less the 2.5 m above sea level. Hence, the danger from climate change is crucial. At the same time the Maldives' economy,

107

Scheuten SolarWorld Solizium GmbH | Open Energy Information  

Open Energy Info (EERE)

search Name Scheuten SolarWorld Solizium GmbH Place Maldives Sector Solar Product Joint Venture of SolarWorld AG and Scheuten Solarholding for production of solar-grade...

108

International Energy Statistics - Energy Information Administration  

U.S. Energy Information Administration (EIA)

Korea, North: NA : 0 : 0 : NA : Korea, South: 2,306 : 0 : 0 : 136,482 : Laos: NA : 0 : 0 : NA : Macau: NA : 0 : 0 : NA : Malaysia: NA : 0 : 0 : 25,632 : Maldives: NA ...

109

International Energy Statistics - Energy Information Administration  

U.S. Energy Information Administration (EIA)

Korea, North: NA : NA : NA : NA : Korea, South: 15 : 1,671 : 0 : 1,753 : Laos: NA : NA : NA : NA : Macau: NA : NA : NA : NA : Malaysia: NA : NA : NA : NA : Maldives ...

110

Decontamination of hot cells K-1, K-3, M-1, M-3, and A-1, M-Wing, Building 200: Project final report Argonne National Laboratory-East  

SciTech Connect

The purpose of this project was to remove radioactively contaminated materials and equipment from the hot cells, to decontaminate the hot cells, and to dispose of the radioactive waste. The goal was to reduce stack releases of Rn-220 and to place the hot cells in an emptied, decontaminated condition with less than 10 {micro}Sv/h (1 mrem/h) general radiation background. The following actions were needed: organize and mobilize a decontamination team; prepare decontamination plans and procedures; perform safety analyses to ensure protection of the workers, public, and environment; remotely size-reduce, package, and remove radioactive materials and equipment for waste disposal; remotely decontaminate surfaces to reduce hot cell radiation background levels to allow personnel entries using supplied air and full protective suits; disassemble and package the remaining radioactive materials and equipment using hands-on techniques; decontaminate hot cell surfaces to remove loose radioactive contaminants and to attain a less than 10 {micro}Sv/h (1 mrem/h) general background level; document and dispose of the radioactive and mixed waste; and conduct a final radiological survey.

Cheever, C.L.; Rose, R.W.

1996-09-01T23:59:59.000Z

111

M-1 N-Reactor fuel development. Excerpts from N-Reactor Department Research and Development Budget for FY-1967 and Revision of Budget for FY-1966  

SciTech Connect

The use of metallic uranium fuel elements on a large scale in a pressurized water cooled graphite moderated power reactor environment in N-Reactor not only represents an extrapolation from previous Hanford fuel technology but it represents the only production-scale application of this concept in this country or abroad. Provision of a supporting technology is and will continue to be a major activity at Hanford as only a limited amount of directly applicable R&D will be available from other sites. The major benefit to be achieved through an extensive and continuing fuel program is attainment of the full capabilities of the N-Reactor at much reduced fuel cycle costs. The current N-Reactor fuel design represents the best engineering judgment of what is required for adequate performance. While the design is intentionally conservative, some features may not fully provide the level of performance required to sustain efficient reactor operation. Results of production-scale irradiation experience and special test irradiations will provide direction to a continuing program to correct any excesses or deficiencies in the initial fuel design. Reduction of unwarranted conservatism in the design will lower fuel fabrication costs, and correction of deficiencies will lower irradiation costs through increased time operated efficiency. Costs of this program are summarized for 1965, 66, and 67. The paper describes the scope of the program, its relationship to other programs, and technical progress in FY-1965 which included improved performance of the fuel elements even with the large number of rapid shutdowns of the reactor.

1965-04-19T23:59:59.000Z

112

High Level ab initio Predictions of the Energetics of mCO2•(H2O)n (n = 1-3, m = 1-12) Clusters  

SciTech Connect

Electronic structure calculations at the correlated molecular orbital theory and density functional theory levels have been used to generate a reliable set of clustering energies for up to three water molecules in carbon dioxide clusters up to n = 12. The structures and energetics are dominated by Lewis acid-base interactions with hydrogen bonding interactions playing a lesser energetic role. The actual binding energies are somewhat larger than might be expected. The correlated molecular orbital MP2 method and density functional theory with the ?B97X exchange-correlation functional provide good results for the energetics of the clusters but the B3LYP and ?B97X-D functionals do not. Seven CO2 molecules form the first solvent shell about a single H2O with four CO2 molecules interacting with the H2O via Lewis acid-base interactions, two CO2 interacting with the H2O by hydrogen bonds, and the seventh CO2 completing the shell. The Lewis acid-base and weak hydrogen bond interactions between the water molecules and the CO2 molecules are strong enough to disrupt the trimer ring configuration for as few as seven CO2 molecules. Calculated 13C NMR chemical shifts for mCO2•(H2O)n show little change with respect to the number of H2O or CO2 molecules in the cluster. The O-H stretching frequencies do exhibit shifts that can provide information about the interactions between water and CO2 molecules.

Thanthiriwatte, Sahan; Duke, Jessica R.; Jackson, Virgil E.; Felmy, Andrew R.; Dixon, David A.

2012-10-04T23:59:59.000Z

113

State Selective Electron Capture Studies:The Contribution of M1-and E2-Transitions to the Lyman Radiation of H-like Uranium  

E-Print Network (OSTI)

Radiation of H-like Uranium Th. Sto« hlker,1;2 F. Bosch,2 R. W. Dunford,3 C. Kozhuharov,2 T. Ludziejewski,2 to decelerate highly charged ions up to bare uranium to energies which are far below the energy required for decelerated bare uranium ion are discussed and their relevance for Lamb shift investigations on high

114

60 80 100 120 Arctic Circle  

E-Print Network (OSTI)

TAJIKISTAN GEORGIA ARMENIA (INDIA) MALDIVES R U S S I A U.K. NORWAY SWEDEN FINLAND DEN. BELA. LITH. LAT. EST KH REBET SIKHOTE-ALIN' T I E N S H A N K U N L U N ZAGROSMTS. CAUCASUS MTS. KHREBET CHERSKOGO M O U N

115

60 80 100 120 Arctic Circle  

E-Print Network (OSTI)

.A.E. TURKMENISTAN UZBEKISTAN KYRGYZSTAN TAJIKISTAN GEORGIA ARMENIA (INDIA) MALDIVES R U S S I A U.K. NORWAY SWEDEN KHREBET YABLONO V Y Y KH REBET SIKHOTE-ALIN' T I E N S H A N K U N L U N ZAGROSMTS. CAUCASUS MTS. KHREBET

116

60 80 100 120 Arctic Circle  

E-Print Network (OSTI)

.A.E. TURKMENISTAN UZBEKISTAN KYRGYZSTAN TAJIKISTAN GEORGIA ARMENIA (INDIA) MALDIVES R U S S I A U.K. NORWAY SWEDEN VERKHOY ANSK KHREBET YABLONOVYY K H R EBET SIKHOTE-ALIN' T I E N S H A N K U N L U N ZAGROSMTS. CAUCASUS

117

Z. Geomorph. N.F. Suppl.-Vol.146 235-251 Berlin Stuttgart November 2006 Geologic Impacts of the 2004 Indian OceanTsunami on Indonesia,  

E-Print Network (OSTI)

of the 2004 Indian OceanTsunami on Indonesia, Sri Lanka, and the Maldives Bruce M. Richmond, Bruce E in the eastern Indian Ocean near northern Sumatra, Indonesia.The resulting tsunami was measured globally and had.1) with an epicenter located under the seafloor in the eastern Indian Ocean near northern Sumatra, Indonesia

118

CATALOG AND STATISTICAL STUDY OF X-RAY SELECTED BL LACERTAE OBJECTS  

Science Conference Proceedings (OSTI)

This paper presents a catalog of 312 X-ray selected BL Lacerate objects (XBLs), optically identified through the end of 2011. It contains the names from different surveys, equatorial coordinates, redshifts, multifrequency flux values, and luminosities for each source. In addition, the different characteristics of XBLs are statistically investigated (redshift, radio/optical/X-ray luminosities, central black hole (BH) mass, synchrotron peak frequency, broadband spectral indices, optical flux variability). Their values are collected through an extensive bibliographic and database search or calculated by us. The redshifts range from 0.031 to 0.702 with a maximum of the distribution at z = 0.223. The 1.4 GHz luminosities of XBLs log {nu}L{sub {nu}} {approx} 39-42 erg s{sup -1} while optical V and X-ray 0.1-2.4 keV bands show log {nu}L{sub {nu}} {approx} 43-46 erg s{sup -1}. The XBL hosts are elliptical galaxies with effective radii r{sub eff} = 3.2625.40 kpc and ellipticities, in = 0.040.52. Their R-band absolute magnitudes M{sub R} range from -21.11 mag to -24.86 mag with a mean value of -22.83 mag. The V - R indices of the hosts span from 0.61 to 1.52 and reveal a fourth-degree polynomial relationship with z that enables us to evaluate the redshifts of five sources whose V - R indices were determined from the observations but whose irredshifts values are either not found or not confirmed. The XBL nuclei show a wider range of 7.31 mag for M{sub R} with the highest luminosity corresponding to M{sub R} = -27.24 mag. The masses of central BHs are found in the interval log M{sub BH} = 7.39-9.30 solar masses (with distribution maximum at log M{sub BH}/M{sub Sun} = 8.30). The synchrotron peak frequencies are spread over the range log {nu}{sub peak} = 14.56-19.18 Hz with a peak of the distribution at log {nu}{sub peak} = 16.60 Hz. The broadband radio-to-optical ({alpha}{sub ro}), optical-to-X-ray ({alpha}{sub ox}), and radio-to-X-ray ({alpha}{sub rx}) spectral indices are distributed in the intervals (0.17,0.59), (0.56,1.48), and (0.41,0.75), respectively. In the optical energy range, the overall flux variability increases, on average, towards shorter wavelengths: ({Delta}m) = 1.22, 1.50, and 1.82 mag through the R, V, B bands of Johnson-Cousins system, respectively. XBLs seem be optically less variable at the intranight timescales compared to the radio-selected BL Lacs (RBLs).

Kapanadze, Bidzina Z., E-mail: bidzina_kapandaze@iliauni.edu.ge [E. Kharadze Abastumani Astrophysical Observatory at Ilia State University, 0162, Cholokashvili Avenue 3/5, Tbilisi (Georgia)

2013-02-01T23:59:59.000Z

119

Donald G. Porter  

Science Conference Proceedings (OSTI)

... Projects. The OOMMF project µMAG: Micromagnetic Modeling Activity Group Tcl/Tk Contributions Contact Information. Selected Publications. ...

2012-09-25T23:59:59.000Z

120

Program for Scaling Up Renewable Energy in Low Income Countries (SREP) |  

Open Energy Info (EERE)

Scaling Up Renewable Energy in Low Income Countries (SREP) Scaling Up Renewable Energy in Low Income Countries (SREP) Jump to: navigation, search Name Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Agency/Company /Organization World Bank Sector Energy, Land Topics Background analysis, Finance, Implementation, Low emission development planning, Market analysis Website http://www.climatefundsupdate. Program Start 2009 Country Ethiopia, Honduras, Kenya, Maldives, Mali, Nepal UN Region Southern Asia References Program for Scaling Up Renewable Energy in Low Income Countries (SREP)[1] Ethiopia Specific Documents[2] Honduras Specific Documents[3] Kenya Specific Documents[4] Maldives Specific Documents[5] Mali Specific Documents[6] Nepal Specific Documents[7] Overview "The Scaling-Up Renewable Energy Program for Low Income Countries (SREP) is

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


121

ARM - Facility News Article  

NLE Websites -- All DOE Office Websites (Extended Search)

May 20, 2011 [Facility News] May 20, 2011 [Facility News] From Snow to Sand; Mobile Facility Headed to the Maldives Bookmark and Share AMF2 operations team members pack up the 3-channel microwave radiometer at the STORMVEX valley floor site in Steamboat Springs, Colorado. AMF2 operations team members pack up the 3-channel microwave radiometer at the STORMVEX valley floor site in Steamboat Springs, Colorado. After spending six very snowy months at Steamboat Springs, Colorado, the second ARM Mobile Facility (AMF2) is switching gears and heading to the tropical climes of the Maldives in the Indian Ocean. In mid-April, the Storm Peak Lab Cloud Property Validation Experiment (STORMVEX) came to a close, ending the final chapter of the AMF2's maiden deployment. After packing up the instruments and data systems, the AMF2 team is now preparing

122

ARM - Feature Stories and Releases Article  

NLE Websites -- All DOE Office Websites (Extended Search)

, 2011 [Feature Stories and Releases] , 2011 [Feature Stories and Releases] AMIE, What You Wanna Do? Bookmark and Share Data spanning the Maldives to Papua New Guinea will help scientists analyze far-reaching tropical weather cycle This view shows a subset of the ARM Mobile Facility instruments operating at the Gan Island airport for the AMIE campaign. To see the complete collection, see the image set in Flickr. This view shows a subset of the ARM Mobile Facility instruments operating at the Gan Island airport for the AMIE campaign. To see the complete collection, see the image set in Flickr. Like the lyrics in the song from the 1970s, the ARM Mobile Facility is going to stay in the Maldives "for a while, maybe longer"-about six months, actually-in support of the ARM Madden Julian Oscillation (MJO)

123

ROCKY MOUNTAIN OILFIELD TESTING CENTER PROJECT TEST RESULTS  

NLE Websites -- All DOE Office Websites (Extended Search)

MAG-WELL DOWNHOLE MAGNETIC FLUID CONDITIONERS MAG-WELL DOWNHOLE MAGNETIC FLUID CONDITIONERS APRIL 4,1995 FC9511 / 95PT5 ROCKY MOUNTAIN OILFIELD TESTING CENTER MAG-WELL DOWNHOLE MAGNETIC FLUID CONDITIONERS PROJECT TEST RESULTES Prepared for: Industry Publication Prepared by: MICHAEL R. TYLER RMOTC Field Engineer November 28, 1995 650100/9511:jb ABSTRACT November 28, 1995 The Rocky Mountain Oilfield Testing Center (RMOTC) conducted a field test on the Mag-Well Downhole Magnetic Fluid Conditioners (MFCs), at the Naval Petroleum Reserve No. 3 (NPR- 3) located 35 miles north of Casper in Natrona County, Wyoming. Mag-Well, Inc., manufactures the MFCs, that are designed to reduce scale and paraffin buildup on the rods, tubing and downhole pump of producing oil wells. The Mag-Well magnetic tools failed to

124

Maricopa Assn. of Governments - PV and Solar Domestic Water Heating...  

Open Energy Info (EERE)

is in addition to the existing standards for residential and commercial PV systems. Local solar installers have reported that being able to refer permitting officials to these MAG...

125

monopole_s028-web.dvi  

NLE Websites -- All DOE Office Websites (Extended Search)

magnetic charge. Precision measurements of the properties of known particles have led to tight limits on the values of mag- netic charge they may possess. Using the induction...

126

Data Analysis Sheet T.3  

Science Conference Proceedings (OSTI)

... specified length? 7, orient =, 0° 90° 180° 270° other. orientation of the test structure on the chip. 8, mag N =, ×, ×, magnification. 9, ...

127

Data Analysis Sheet T.2  

Science Conference Proceedings (OSTI)

... 1, mag =, ×, magnification. 2, orient =, 0° 90° other, orientation of the test structure on the test chip. 3, align =, Yes No, alignment ensured ? ...

128

New airport liquid analysis system undergoes testing at Albuquerque...  

NLE Websites -- All DOE Office Websites (Extended Search)

sustainable energy sources, to plasma physics and new materials. Contact Nancy Ambrosiano Communications Office (505) 667-0471 Email MagViz technology from Los Alamos sorts out...

129

Donald G. Porter  

Science Conference Proceedings (OSTI)

... OOMMF; µMAG; Tcl. Selected Publications. Analytical Determination of the Landau Lifshitz Gilbert (LLG) Zero-Damping Critical Switching Field; ...

2013-06-27T23:59:59.000Z

130

X-8 14-73-72 PROCEEDINGS OF THE FOURTH PRECISE ...  

Science Conference Proceedings (OSTI)

... Fadeouts may also result from other factors, such as ionospheric storms, solar flares, mag- netic storms, and sporadic E-layer reflection. ...

2002-09-11T23:59:59.000Z

131

Materials Sustainability: Digital Resource Center - A Replacement ...  

Science Conference Proceedings (OSTI)

Jul 1, 2008 ... This presentation from the 2003 EPA Conference describes the prior art for magnesium protection and presents the MagShield system with ...

132

Magnesium Components Achieve Weight Reduction and Fuel Savings  

NLE Websites -- All DOE Office Websites (Extended Search)

cast mag- nesium can achieve consider- able weight reduction advantages over both steel and aluminum. Furthermore, this favorable weight reduction potential can enable...

133

EV Micro-Climate TM Plan  

NLE Websites -- All DOE Office Websites (Extended Search)

of Transportation EV Electric Vehicle EVSE Electric Vehicle Supply Equipment HEV Hybrid Electric Vehicle INL Idaho National Laboratory MAG Maricopa Association of Governments MSA...

134

Application to Export Electric Energy OE Docket No. EA-306-A...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Solutions: Federal Register Notice Volume 75, No. 237 - Dec. 10, 2010 Application to Export Electric Energy OE Docket No. EA-306-A MAG Energy Solutions: Federal Register Notice...

135

Atomic Data for Americium (Am)  

Science Conference Proceedings (OSTI)

... Atomic Number = 95. Atomic Weight = (243). Reference E95. Isotope, Mass, Abundance, Spin, Mag Moment, 241 Am, 241.056823, 0, 5/2, +1.61. ...

136

LANL | TT | News Archive - Los Alamos National Lab: National ...  

Biomoda Allowed Patent in Canada (Biomoda Inc.) Sounds better than light (R&D Mag.) Los Alamos National Laboratory seeks funding ideas (NM Business Weekly)

137

Instrument Schedule for SPINS  

Science Conference Proceedings (OSTI)

... [1] Andreas Kreyssig. [1] Ames Laboratory. [2] Iowa State University. [3] Helmholtz Zentrum Berlin. Magnet - 10T, dry, dilfrig insert - Mag10T<1.5. ...

138

Asian Development Outlook 2010 | Open Energy Information  

Open Energy Info (EERE)

Asian Development Outlook 2010 Asian Development Outlook 2010 Jump to: navigation, search Tool Summary LAUNCH TOOL Name: Asian Development Outlook 2010: Macroeconomic Management Beyond the Crisis Agency/Company /Organization: Asian Development Bank Sector: Energy Topics: Market analysis, Resource assessment Resource Type: Publications Website: www.adb.org/Documents/Books/ADO/2010/ado2010.pdf Country: Armenia, Azerbaijan, Georgia (country), Kazakhstan, Kyrgyzstan, Tajikistan, Turkmenistan, Uzbekistan, China, South Korea, Mongolia, Afghanistan, Bangladesh, Bhutan, India, Maldives, Pakistan, Sri Lanka, Nepal, Cambodia, Indonesia, Malaysia, Laos, Vietnam, Singapore, Thailand, Philippines, Myanmar, Fiji, Papua New Guinea, Timor-Leste UN Region: Central Asia, Eastern Asia, South-Eastern Asia

139

Rural Energy Options Analysis Training Development and Implementation at NREL  

DOE Green Energy (OSTI)

NREL has developed a rural energy options analysis training program for rural energy decision makers that provides knowledge, skills and tools for the evaluation of technologies, including renewables, for rural energy applications. Through the Department of Energy (DOE) Solar Energy Technologies Program (SETP), NREL has refined materials for the program and developed a module that offers hands-on training in the preparation of data for options analysis using HOMER, NREL's micropower optimization model. NREL has used the materials for training in Brazil, the Maldives, Mexico, and Sri Lanka.

Gilman, P.

2005-01-01T23:59:59.000Z

140

Slide23 | OSTI, US Dept of Energy, Office of Scientific and Technical  

Office of Scientific and Technical Information (OSTI)

Slide23 Slide23 Slide23 Developing Country Access Afghanistan Guatemala Nigeria Albania Guinea Pakistan Algeria Guinea-Bissau Palestinian Territories (West Bank/ Gaza) Angola Guyana Papua New Guinea Armenia Haiti Paraguay Azerbaijan Honduras Peru Bangladesh Indonesia Philippines Belize Iraq Rwanda Benin Jordan Samoa Bhutan Kenya Sao Tome and Principe Bolivia Kiribati Senegal Burkina Faso Kyrgyzstan Sierra Leone Burundi Lao People's Democratic Republic Solomon Islands Cambodia Lesotho Somalia Cameroon Liberia Sri Lanka Cape Verde Macedonia, The Former Yugoslav Republic of Swaziland Central African Republic Madagascar Tajikistan Chad Malawi Tanzania, United Republic of Colombia Maldives Thailand Comoros Mali Timor-Leste Congo Marshall Islands Togo Congo, The Democratic Republic of Mauritania Tonga

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


141

Das Mitteilungsblatt erscheint jeweils am 1. und 3. Mittwoch jeden Monats. Eigentmer, Herausgeber, Vervielfltigung und Vertrieb: Zentrale Dienste der Universitt Innsbruck,  

E-Print Network (OSTI)

bis 16 für die Studien: D �bersetzen und Dolmetschen (Deutsch, Englisch, Französisch, Italienisch für die Studien: D Deutsche Philologie BA Germanistik MA Germanistik D Sprachwissenschaft Dr für Chemie und Pharmazie Univ.-Prof. Mag. Dr. Hermann Stuppner (V: Univ.-Prof. Mag. Dr. Andreas

Breu, Ruth

142

Detection, size, measurement and structural analysis limits for the 2MASS, UKIDSS-LAS & VISTA VIKING surveys  

E-Print Network (OSTI)

The 2MASS, UKIDSS-LAS and VISTA VIKING surveys have all now observed the GAMA 9hr region in the $K_s$ band. Here we compare the detection rates, photometry, basic size measurements, and single-component GALFIT structural measurements for a sample of 37,591 galaxies. We explore the sensitivity limits where the data agree for a variety of issues including: detection, star-galaxy separation, photometric measurements, size and ellipticity measurements, and S\\'{e}rsic measurements. We find that 2MASS fails to detect at least 20% of the galaxy population within all magnitude bins, however for those that are detected we find photometry is robust ($\\pm$ 0.2 mag) to 14.7 AB mag and star-galaxy separation to 14.8 AB mag. For UKIDSS-LAS we find incompleteness starts to enter at a flux limit of 18.9 AB mag, star-galaxy separation is robust to 16.3 AB mag and structural measurements are robust to 17.7 AB mag. VISTA VIKING data is complete to approximately 20.0 AB mag and structural measurements appear robust to 18.8 AB ma...

Andrews, Stephen K; Driver, Simon P; Robotham, Aaron S G

2013-01-01T23:59:59.000Z

143

uvbyHbeta CCD Photometry of Clusters. IV. Solving the Riddle of NGC 3680  

E-Print Network (OSTI)

CCD photometry on the uvbyCaHbeta system is presented for the open cluster, NGC 3680. Restricting the data to probable cluster members using the CMD and the photometric indices alone defines a sample of 34 stars at the cluster turnoff that imply E(b-y)=0.042(0.002) or E(B-V) = 0.058(0.003), where the errors (s.e.m) refer to internal errors alone. With this reddening, [Fe/H] is derived from both m1 and hk using both b-y and Hbeta as the temperature indices. The agreement among the four approaches is excellent, leading to final value of [Fe/H] = -0.14 (0.03) for the cluster and removing the apparent discrepancy between the past uvby analyses and extensive results from the red giants for which the cause has been traced to an apparent zero-point offset in the original m1 indices. Using the homogenized and combined V, b-y data from a variety of studies transformed to B-V, the cluster CMD is compared to NGC 752, IC 4651, and the core-convective-overshoot isochrones of Girardi et al. (2002). By interpolation to the proper metallicity, it is found that the E(B-V), (m-M), and age for NGC 752, IC 4651, and NGC 3680 are (0.03, 8.30, 1.55 Gyr), (0.10, 10.20, 1.7 Gyr), and (0.06, 10.20, 1.85 Gyr), respectively. The revised age and metallicity sequence and the color distribution of the giants provide evidence for the suggestion that the giants defining the apparent clump in NGC 3680 are predominantly first-ascent giants, as indicated by their Li abundance, while the clump stars in NGC 752, 0.1 mag bluer in (B-V), are He-core-burning stars. When combined with the color distribution in IC 4651, it is suggested that over this modest age range where He-core flash becomes important, the distribution of so-called clump stars switches from being dominated by He-core burning stars to first-ascent giants in the bump phase.

B. J. Anthony-Twarog; B. A. Twarog

2003-10-31T23:59:59.000Z

144

Essays on International Finance and Trade  

E-Print Network (OSTI)

1973M 1-20 09M7 Real oil prices TOT 1973M 1-20 09M7 1973M 1-1973M 1-20 09M7 REER Real oil prices 1973M 1-20 09M7 1973M1975M 1-20 09M7 Real oil prices TOT 1975M 1-20 09M7 1975M 1-

Zeng, Li

2009-01-01T23:59:59.000Z

145

Magellan Queues end November 30  

NLE Websites -- All DOE Office Websites (Extended Search)

Magellan Queues End November 30 Magellan Queues End November 30 November 15, 2011 by Francesca Verdier (0 Comments) Schedule and Status Mon, Nov 28 westmere queue drain - 08:00 - DONE remove - 10:20 - DONE serial queue add westmere nodes - 10:40 - DONE Tue, Nov 29 mag_xlmem queue drain - 08:00 - DONE remove - 09:15 - DONE reg_xlmem queue create - 14:00 - DONE enable - 17:00 Wed, Nov 30 no queue modifications Thu, Dec 1 magellan queue drain - 08:00 - DONE remove - 09:30 - DONE mag_serial queue drain - 08:00 - DONE remove - 09:30 - DONE Overview The "magellan" and "mag_serial" batch queues will be drained and disabled at 08:00, Thursday, December 1. Any jobs left in those queues will be discarded. The "mag_xlmem" queue, which provides shared access to a single node that

146

A Precision Photometric Comparison between SDSS-II and CSP Type Ia Supernova Data  

Science Conference Proceedings (OSTI)

Consistency between Carnegie Supernova Project (CSP) and SDSS-II Supernova Survey ugri measurements has been evaluated by comparing Sloan Digital Sky Survey (SDSS) and CSP photometry for nine spectroscopically confirmed Type Ia supernova observed contemporaneously by both programs. The CSP data were transformed into the SDSS photometric system. Sources of systematic uncertainty have been identified, quantified, and shown to be at or below the 0.023 mag level in all bands. When all photometry for a given band is combined, we find average magnitude differences of equal to or less than 0.011 mag in ugri, with rms scatter ranging from 0.043 to 0.077 mag. The u-band agreement is promising, with the caveat that only four of the nine supernovae are well observed in u and these four exhibit an 0.038 mag supernova-to-supernova scatter in this filter.

Mosher, J.; /Pennsylvania U.; Sako, M.; /Pennsylvania U.; Corlies, L.; /Pennsylvania U. /Columbia U.; Folatelli, G.; /Tokyo U. /Carnegie Inst. Observ.; Frieman, J.; /Chicago U., KICP /Chicago U., Astron. Astrophys. Ctr.; Holtzman, J.; /New Mexico State U.; Jha, S.W.; /Rutgers U., Piscataway; Kessler, R.; /Chicago U., Astron. Astrophys. Ctr. /Chicago U., KICP; Marriner, J.; /Fermilab; Phillips, M.M.; /Carnegie Inst. Observ.; Stritzinger, M.; /Aarhus U. /Stockholm U., OKC /Bohr Inst. /Carnegie Inst. Observ.

2012-06-01T23:59:59.000Z

147

A PRECISION PHOTOMETRIC COMPARISON BETWEEN SDSS-II AND CSP TYPE Ia SUPERNOVA DATA  

SciTech Connect

Consistency between Carnegie Supernova Project (CSP) and SDSS-II Supernova Survey ugri measurements has been evaluated by comparing Sloan Digital Sky Survey (SDSS) and CSP photometry for nine spectroscopically confirmed Type Ia supernova observed contemporaneously by both programs. The CSP data were transformed into the SDSS photometric system. Sources of systematic uncertainty have been identified, quantified, and shown to be at or below the 0.023 mag level in all bands. When all photometry for a given band is combined, we find average magnitude differences of equal to or less than 0.011 mag in ugri, with rms scatter ranging from 0.043 to 0.077 mag. The u-band agreement is promising, with the caveat that only four of the nine supernovae are well observed in u and these four exhibit an 0.038 mag supernova-to-supernova scatter in this filter.

Mosher, J.; Sako, M.; Corlies, L. [Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA 19104 (United States); Folatelli, G. [Institute for the Physics and Mathematics of the Universe (IPMU), University of Tokyo, 5-1-5 Kashiwanoha, Kashiwa, Chiba 277-8583 (Japan); Frieman, J.; Kessler, R. [Department of Astronomy and Astrophysics, University of Chicago, 5640 South Ellis Avenue, Chicago, IL 60637 (United States); Holtzman, J. [Department of Astronomy, MSC 4500, New Mexico State University, P.O. Box 30001, Las Cruces, NM 88003 (United States); Jha, S. W. [Department of Physics and Astronomy, Rutgers, the State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ 08854 (United States); Marriner, J. [Center for Particle Astrophysics, Fermi National Accelerator Laboratory, P.O. Box 500, Batavia, IL 60510 (United States); Phillips, M. M.; Morrell, N. [Las Campanas Observatory, Carnegie Observatories, Casilla 601, La Serena (Chile); Stritzinger, M. [Oskar Klein Centre for Cosmo Particle Physics, AlbaNova University Center, 106 91 Stockholm (Sweden); Schneider, D. P., E-mail: jmosher@sas.upenn.edu [Department of Astronomy and Astrophysics, Pennsylvania State University, 525 Davey Laboratory, University Park, PA 16802 (United States)

2012-07-15T23:59:59.000Z

148

A 6.4 TESLA DIPOLE MAGNET FOR THE SSC  

E-Print Network (OSTI)

Engineering, Volume 31 A 6.4 TESLA DIPOLE MAGNET FOR THE SSCR. SCANLAN SSC-MAG A 6.4 TESLA DIPOLE MAGiET FOR THE SSC* C.increa.ing up to . 28 tesla . - The resultins systematic

Taylor, C.E.

2010-01-01T23:59:59.000Z

149

Facilities: NHMFL 14.5 Tesla Fourier Transform Ion Cyclotron Resonance Mass Spectrometer Citation: A Pseudoatomic Model of the COPII Cage Obtained from Cryo-Electron Microscopy and Mass Spectrometry,  

E-Print Network (OSTI)

Facilities: NHMFL 14.5 Tesla Fourier Transform Ion Cyclotron Resonance Mass Spectrometer Citation ultrahigh-resolution 14.5 tesla Fourier transform ion cyclotron resonance mass spectrometry. The Mag

Weston, Ken

150

THSE PRSENTE L'UNIVERSIT DU QUBEC CHICOUTIMI  

E-Print Network (OSTI)

quantifier les principaux processus de solidification magmatiques à l'oeuvre dans la genèse des basaltes de type "pipe" sous le rift du Mauna Ulu. Le mag

Paris-Sud XI, Université de

151

Skin lesions in carpet hand-weavers  

E-Print Network (OSTI)

its export development. Iran hand woven carpet Mag. 1997;10:Solaleh pub. co. Zanjan /Iran 1998 (in Persian) 5. Kutluhanscience university Yazd, Iran. mtnoorbala@gmail.com Abstract

Noorbala, MT

2008-01-01T23:59:59.000Z

152

Laboratory snags five R&D 100 awards  

NLE Websites -- All DOE Office Websites (Extended Search)

R&D 100 awards Laboratory snags five R&D 100 awards Winning Laboratory projects are MagViz, the SIMTECHE CO2 Capture Process, Lasonix, TeraOps Software Radio, and the Artificial...

153

Table-top SEM: Hitachi TM-1000  

Science Conference Proceedings (OSTI)

... use, depth of focus, auto image adjustment and speed (3 min. set-up time). Specifications / Capabilities: Mag: 20-10,000x; Accel. voltage: 15kV; Max ...

2010-10-05T23:59:59.000Z

154

Mr. James Bearzi, Chief Hazardous Waste Bureau  

NLE Websites -- All DOE Office Websites (Extended Search)

Subject: Certification by a New Mexico Registered Professional Engineer in Support of TRUPACT-III References: United States Department Of Energy letter CBFO:OESH :GTB:MAG:11-...

155

Bader-053013 - Argonne National Laboratories, Materials Sicence...  

NLE Websites -- All DOE Office Websites (Extended Search)

SPEAKER: Sam Bader Materials Science Division, Nanoscience & Technology Division TITLE: Nano-Mag - Past, Present & Future DATE: Thursday, May 30, 2013 TIME: 11:00 a.m. PLACE:...

156

Multiscale modeling of nano/micro systems by a multiscale continuum field theory  

E-Print Network (OSTI)

a multiscale the- ory for nano/micro physics. Phil Mag 85:2006) Conservation laws at nano/micro scales. J Mech MaterStresses and strains at nano/micro scales. J Mech Mater

Zeng, Xiaowei; Wang, Xianqiao; Lee, James D.; Lei, Yajie

2011-01-01T23:59:59.000Z

157

Instrument Schedule for dcs  

Science Conference Proceedings (OSTI)

... [5] david Cole. [1] Oak Ridge National Laboratory. ... [2] Oak Ridge National Laboratory. Magnet - 10T, dry, T > 1.5 K - Mag10T>1.5. Yiming Qiu. ...

158

Office of Educational Programs  

NLE Websites -- All DOE Office Websites (Extended Search)

k-6) Elementary Science Fair (Grades: 6-8) MagLev Contest (Grades: 6-8) Middle School Science Bowl and Car Challenge (Grades: 9-12) Bridge Building Contest (Grades: 9-12)...

159

MDC No. 096 Rev. D RECEIVING INSPECTION AND  

NLE Websites -- All DOE Office Websites (Extended Search)

Mechanical Visual inspection: RHIC-MAG-R-7536- 3.3.1.5 FUNCTION: APPROVAL (6) Seller's packaging. Part No., Revision letter, & Serial No. verified. Protective covers (2) are...

160

Microsoft Word - Transmittal of Final Audit Report A-13-02, SRS...  

NLE Websites -- All DOE Office Websites (Extended Search)

DSM:MAG:13-1490:UFC 2300.00 Department of Energy Carlsbad Field Office P.O. Box 3090 Carlsbad, New Mexico 88221 August 6, 2013 Mr. John E. Kieling, Chief Hazardous Waste Bureau New...

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


161

TRAINING OF LBL-SSC MODEL DIPOLE MAGNETS AT 1.8 K  

E-Print Network (OSTI)

Conditioning (Non·Quench Training) of Model SSC Dipole." ,lL, March 20-23,1989 Training of LBL-SSC Model DipoleJ SSC-MAG-231 LBL-26282 TRAINING OF LBL-SSC MODEL DIPOLE

Gilbert, W.S.

2011-01-01T23:59:59.000Z

162

RussiaLANLV3-web.indd  

National Nuclear Security Administration (NNSA)

PROBE CURRENT DATA 3 Faraday records 2 Mag Probe records 120 100 80 60 40 20 0 -20 C U R R E N T 0 50 100 150 200 250 300 Modifi ed for the Web Project Description Complementing...

163

Design, Implementation and Control of a Sparse Aperture Imaging Satellite  

E-Print Network (OSTI)

], calcium fluoride [41,51], and mag- nesium fluoride [47, 50, 53]. Their free-spectral range (FSR) may vary nitride ring fabrication and valuable technical discussion and guideline. I express my deep gratitude

164

Onsite Tours  

NLE Websites -- All DOE Office Websites (Extended Search)

science & research Onsite tour info (pdf) | Map of onsite tours (jpg) 1 Aqua Tour, Smart Grid House and Solar Power More info: Los Alamos Smart Grid 2 Yellow Tour, MagViz...

165

Magnetic mesoporous materials for removal of environmental wastes  

Science Conference Proceedings (OSTI)

We have synthesized two different magnetic mesoporous materials that can be easily separated from aqueous solutions by applying a magnetic field. Synthesized magnetic mesoporous materials, Mag-SBA-15 (magnetic ordered mesoporous silica) and Mag-OMC (magnetic ordered mesoporous carbon), have a high loading capacity of contaminants due to high surface area of the supports and high magnetic activity due to the embedded iron oxide particles. Application of surface-modified Mag-SBA-15 was investigated for the collection of mercury from water. The mercury adsorption using Mag-SBA-15 was rapid during the initial contact time and reached a steady-state condition, with an uptake of approximately 97% after 7 hours. Application of Mag-OMC for collection of organics from water, using fluorescein as an easily trackable model analyte, was explored. The fluorescein was absorbed into Mag-OMC within minutes and the fluorescent intensity of solution was completely disappeared after an hour. In another application, Mag-SBA-15 was used as a host of tyrosinase, and employed as recyclable catalytic scaffolds for tyrosinase-catalyzed biodegradation of catechol. Tyrosinase aggregates in Mag-SBA-15, prepared in a two step process of tyrosinase adsorption and crosslinking, could be used repeatedly for catechol degradation with no serious loss of enzyme activity. Considering these results of cleaning up water from toxic inorganic, organic and biochemical contaminants, magnetic mesoporous materials have a great potential to be employed for the removal of environmental contaminants and potentially for the application in large-scale wastewater treatment plants.

Kim, Byoung Chan; Lee, Jinwoo; Um, Wooyong; Kim, Jaeyun; Joo, Jin; Lee, Jin Hyung; Kwak, Ja Hun; Kim, Jae Hyun; Lee, Changha; Lee, Hongshin; Addleman, Raymond S.; Hyeon, Taeghwan; Gu, Man Bock; Kim, Jungbae

2011-09-15T23:59:59.000Z

166

Hierarchical path planning for situated agents in informed virtual geographic environments  

Science Conference Proceedings (OSTI)

Multi-Agent Geo-Simulation (MAGS) is a modelling and simulation paradigm which involves a large number of autonomous situated agents of various extents evolving in, and interacting with, an explicit description of a geographic environment called a Virtual ... Keywords: autonomous situated agents (ASA), geographic information system (GIS), hierarchical path planning (HPP), informed virtual geographic environment (IVGE), multi-agent geo-simulation (MAGS), optimisation, situated reasoning (SR)

Mehdi Mekni

2010-03-01T23:59:59.000Z

167

Ethiopia-Program for Scaling Up Renewable Energy in Low Income Countries  

Open Energy Info (EERE)

Ethiopia-Program for Scaling Up Renewable Energy in Low Income Countries Ethiopia-Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Jump to: navigation, search Name Ethiopia-Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Agency/Company /Organization World Bank Sector Energy, Land Topics Background analysis, Finance, Implementation, Low emission development planning, Market analysis Website http://www.climatefundsupdate. Program Start 2009 Country Ethiopia UN Region Southern Asia References Program for Scaling Up Renewable Energy in Low Income Countries (SREP)[1] Ethiopia Specific Documents[2] Honduras Specific Documents[3] Kenya Specific Documents[4] Maldives Specific Documents[5] Mali Specific Documents[6] Nepal Specific Documents[7] Overview "The Scaling-Up Renewable Energy Program for Low Income Countries (SREP) is

168

ARM - AMF2 Organization and Contact Information  

NLE Websites -- All DOE Office Websites (Extended Search)

Organization and Contact Information Organization and Contact Information AMF Information Science Architecture Baseline Instruments AMF1 AMF2 AMF3 Data Operations AMF Fact Sheet Images Contacts AMF Deployments Hyytiälä, Finland, 2014 Manacapuru, Brazil, 2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat Springs, Colorado, 2010 Graciosa Island, Azores, 2009-2010 Shouxian, China, 2008 Black Forest, Germany, 2007 Niamey, Niger, 2006 Point Reyes, California, 2005 AMF2 Organization and Contact Information The Argonne AMF2 Operations Office manages the operation of the second ARM mobile facility. Basic contact information, phone numbers, email, and shipping information to personnel in this office is available on this page.

169

Mobile Facility  

NLE Websites -- All DOE Office Websites (Extended Search)

Facility Facility AMF Information Science Architecture Baseline Instruments AMF1 AMF2 AMF3 Data Operations AMF Fact Sheet Images Contacts AMF Deployments Hyytiälä, Finland, 2014 Manacapuru, Brazil, 2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat Springs, Colorado, 2010 Graciosa Island, Azores, 2009-2010 Shouxian, China, 2008 Black Forest, Germany, 2007 Niamey, Niger, 2006 Point Reyes, California, 2005 Mobile Facilities Pictured here in Gan, the second mobile facility is configured in a standard layout. Pictured here in Gan, the second mobile facility is configured in a standard layout. To explore science questions beyond those addressed by ARM's fixed sites at

170

ARM - Surface Aerosol Observing System  

NLE Websites -- All DOE Office Websites (Extended Search)

FacilitiesSurface Aerosol Observing System FacilitiesSurface Aerosol Observing System AMF Information Science Architecture Baseline Instruments AMF1 AMF2 AMF3 Data Operations AMF Fact Sheet Images Contacts AMF Deployments Hyytiälä, Finland, 2014 Manacapuru, Brazil, 2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat Springs, Colorado, 2010 Graciosa Island, Azores, 2009-2010 Shouxian, China, 2008 Black Forest, Germany, 2007 Niamey, Niger, 2006 Point Reyes, California, 2005 Surface Aerosol Observing System The ARM Mobile Facility (AMF) is equipped to quantify the interaction between clouds and aerosol particles. A counter-flow virtual impactor (CVI) is used to selectively sample cloud drops. The CVI takes advantage of the

171

Asia-Pacific Regional Climate Change Adaptation Assessment | Open Energy  

Open Energy Info (EERE)

Asia-Pacific Regional Climate Change Adaptation Assessment Asia-Pacific Regional Climate Change Adaptation Assessment Jump to: navigation, search Tool Summary Name: Asia-Pacific Regional Climate Change Adaptation Assessment Agency/Company /Organization: U.S. Agency for International Development Sector: Energy Topics: Adaptation, Co-benefits assessment, Policies/deployment programs Resource Type: Publications Website: www.usaid.gov/rdma/documents/RDMA_Asia-Pacific_Climate_Change_Adaptati Country: China, Bangladesh, India, Indonesia, Laos, Marshall Islands, Federated States of Micronesia, Philippines, Thailand, Vietnam, Cambodia, Maldives, Mongolia, Nepal, Papua New Guinea, Timor-Leste, Solomon Islands, Sri Lanka, Vanuatu UN Region: Central Asia, Eastern Asia, South-Eastern Asia References: Asia-Pacific Adaptation Assessment[1]

172

ARM - Mobile Aerosol Observing System  

NLE Websites -- All DOE Office Websites (Extended Search)

FacilitiesMobile Aerosol Observing System FacilitiesMobile Aerosol Observing System AMF Information Science Architecture Baseline Instruments AMF1 AMF2 AMF3 Data Operations AMF Fact Sheet Images Contacts AMF Deployments Hyytiälä, Finland, 2014 Manacapuru, Brazil, 2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat Springs, Colorado, 2010 Graciosa Island, Azores, 2009-2010 Shouxian, China, 2008 Black Forest, Germany, 2007 Niamey, Niger, 2006 Point Reyes, California, 2005 Mobile Aerosol Observing System Intensive aerosol observations conducted on the campus of Brookhaven National Laboratory on Long Island, New York, using the ARM Mobile Aerosol Observing System. Intensive aerosol observations conducted on the campus of Brookhaven

173

Nepal-Program for Scaling Up Renewable Energy in Low Income Countries  

Open Energy Info (EERE)

Nepal-Program for Scaling Up Renewable Energy in Low Income Countries Nepal-Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Jump to: navigation, search Name Nepal-Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Agency/Company /Organization World Bank Sector Energy, Land Topics Background analysis, Finance, Implementation, Low emission development planning, Market analysis Website http://www.climatefundsupdate. Program Start 2009 Country Nepal UN Region Southern Asia References Program for Scaling Up Renewable Energy in Low Income Countries (SREP)[1] Ethiopia Specific Documents[2] Honduras Specific Documents[3] Kenya Specific Documents[4] Maldives Specific Documents[5] Mali Specific Documents[6] Nepal Specific Documents[7] Overview "The Scaling-Up Renewable Energy Program for Low Income Countries (SREP) is

174

Honduras-Program for Scaling Up Renewable Energy in Low Income Countries  

Open Energy Info (EERE)

Honduras-Program for Scaling Up Renewable Energy in Low Income Countries Honduras-Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Jump to: navigation, search Name Honduras-Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Agency/Company /Organization World Bank Sector Energy, Land Topics Background analysis, Finance, Implementation, Low emission development planning, Market analysis Website http://www.climatefundsupdate. Program Start 2009 Country Honduras UN Region Southern Asia References Program for Scaling Up Renewable Energy in Low Income Countries (SREP)[1] Ethiopia Specific Documents[2] Honduras Specific Documents[3] Kenya Specific Documents[4] Maldives Specific Documents[5] Mali Specific Documents[6] Nepal Specific Documents[7] Overview "The Scaling-Up Renewable Energy Program for Low Income Countries (SREP) is

175

ARM - AMF2 Architecture  

NLE Websites -- All DOE Office Websites (Extended Search)

Architecture Architecture AMF Information Science Architecture Baseline Instruments AMF1 AMF2 AMF3 Data Operations AMF Fact Sheet Images Contacts AMF Deployments Hyytiälä, Finland, 2014 Manacapuru, Brazil, 2014 Oliktok Point, Alaska, 2013 Los Angeles, California, to Honolulu, Hawaii, 2012 Cape Cod, Massachusetts, 2012 Gan Island, Maldives, 2011 Ganges Valley, India, 2011 Steamboat Springs, Colorado, 2010 Graciosa Island, Azores, 2009-2010 Shouxian, China, 2008 Black Forest, Germany, 2007 Niamey, Niger, 2006 Point Reyes, California, 2005 AMF2 Architecture The core AMF2 instrumentation is designed to operate out of modules; small independent climate controlled systems that house instrument computers, data loggers and other support equipment. This design feature sets the AMF2 apart in its flexibility and mobility at deployment sites.

176

Mali-Program for Scaling Up Renewable Energy in Low Income Countries (SREP)  

Open Energy Info (EERE)

Mali-Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Mali-Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Jump to: navigation, search Name Mali-Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Agency/Company /Organization World Bank Sector Energy, Land Topics Background analysis, Finance, Implementation, Low emission development planning, Market analysis Website http://www.climatefundsupdate. Program Start 2009 Country Mali UN Region Southern Asia References Program for Scaling Up Renewable Energy in Low Income Countries (SREP)[1] Ethiopia Specific Documents[2] Honduras Specific Documents[3] Kenya Specific Documents[4] Maldives Specific Documents[5] Mali Specific Documents[6] Nepal Specific Documents[7] Overview "The Scaling-Up Renewable Energy Program for Low Income Countries (SREP) is

177

Kenya-Program for Scaling Up Renewable Energy in Low Income Countries  

Open Energy Info (EERE)

Kenya-Program for Scaling Up Renewable Energy in Low Income Countries Kenya-Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Jump to: navigation, search Name Kenya-Program for Scaling Up Renewable Energy in Low Income Countries (SREP) Agency/Company /Organization World Bank Sector Energy, Land Topics Background analysis, Finance, Implementation, Low emission development planning, Market analysis Website http://www.climatefundsupdate. Program Start 2009 Country Kenya UN Region Southern Asia References Program for Scaling Up Renewable Energy in Low Income Countries (SREP)[1] Ethiopia Specific Documents[2] Honduras Specific Documents[3] Kenya Specific Documents[4] Maldives Specific Documents[5] Mali Specific Documents[6] Nepal Specific Documents[7] Overview "The Scaling-Up Renewable Energy Program for Low Income Countries (SREP) is

178

Sustainable Development Strategy for South Asia | Open Energy Information  

Open Energy Info (EERE)

Name Sustainable Development Strategy for South Asia Agency/Company /Organization AIT-UNEP Regional Resource Centre for Asia and the Pacific Sector Energy, Land Topics Implementation, Policies/deployment programs, Background analysis Resource Type Guide/manual Website http://www.rrcap.unep.org/nsds Country Afghanistan, Bangladesh, Bhutan, Nepal, Maldives, Pakistan, Sri Lanka UN Region South-Eastern Asia References AIT-UNEP RRC.AP[1] Purpose "This document is expected to provide the strategic direction for the pursuit of sustainable development in the SAS. It is important to note that this document addresses the issues at the sub-regional level, building upon national level issues and policies but particularly addressing those transcending and common to the countries in the SAS. It is expected that

179

South Asia Regional Initiative for Energy Cooperation and Development  

Open Energy Info (EERE)

Initiative for Energy Cooperation and Development Initiative for Energy Cooperation and Development (SARI/Energy) Jump to: navigation, search Logo: South Asia Regional Initiative for Energy Cooperation and Development (SARI/Energy) Name South Asia Regional Initiative for Energy Cooperation and Development (SARI/Energy) Agency/Company /Organization U.S. Agency for International Development, National Renewable Energy Laboratory Sector Energy, Land Focus Area Energy Efficiency Topics Background analysis Website http://www.usaid.gov/our_work/ Country Afghanistan, Pakistan, Bhutan, India, Sri Lanka, Bangladesh, Nepal, Maldives Southern Asia, Southern Asia, Southern Asia, Southern Asia, Southern Asia, Southern Asia, Southern Asia, Southern Asia References USAID Regional Climate Programs[1] Abstract SARI/Energy is at the center of efforts to strengthen public-private sector partnerships and regional economic cooperation. By promoting rational use of regional energy supplies, SARI/Energy contributes to energy security, reduced greenhouse gas emissions, and overall improvements in environmental quality and human health in the region.

180

Nationally Appropriate Mitigation Actions | Open Energy Information  

Open Energy Info (EERE)

Page Page Edit with form History Facebook icon Twitter icon » Nationally Appropriate Mitigation Actions Jump to: navigation, search Tool Summary LAUNCH TOOL Name: Nationally Appropriate Mitigation Actions Agency/Company /Organization: United Nations Framework Convention on Climate Change Sector: Energy, Land Focus Area: Energy Efficiency Topics: GHG inventory, Low emission development planning Resource Type: Publications, Lessons learned/best practices, Case studies/examples Website: unfccc.int/home/items/5265.php Country: Afghanistan, Antigua and Barbuda, Armenia, Benin, Bhutan, Botswana, Brazil, Cameroon, Central African Republic, China, Democratic Republic of Congo, Costa Rica, Ivory Coast, Ethiopia, Eritrea, Gabon, Georgia (country), Ghana, India, Indonesia, Israel, Jordan, Madagascar, Maldives, Marshall Islands, Mauritania, Mexico, Mongolia, Morocco, Papua New Guinea, Peru, South Korea, Moldova, San Marino, Sierra Leone, Singapore, South Africa, Republic of Macedonia, Togo, Tunisia

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


181

Reply to comment | OSTI, US Dept of Energy, Office of Scientific and  

Office of Scientific and Technical Information (OSTI)

Reply to comment Reply to comment Slide23 Submitted by gibsone on Fri, 2013-08-30 06:22 FY2011-hitson Slide23 Developing Country Access Afghanistan Guatemala Nigeria Albania Guinea Pakistan Algeria Guinea-Bissau Palestinian Territories (West Bank/ Gaza) Angola Guyana Papua New Guinea Armenia Haiti Paraguay Azerbaijan Honduras Peru Bangladesh Indonesia Philippines Belize Iraq Rwanda Benin Jordan Samoa Bhutan Kenya Sao Tome and Principe Bolivia Kiribati Senegal Burkina Faso Kyrgyzstan Sierra Leone Burundi Lao People's Democratic Republic Solomon Islands Cambodia Lesotho Somalia Cameroon Liberia Sri Lanka Cape Verde Macedonia, The Former Yugoslav Republic of Swaziland Central African Republic Madagascar Tajikistan Chad Malawi Tanzania, United Republic of Colombia Maldives Thailand Comoros Mali Timor-Leste

182

ARM - Instrument - tsi  

NLE Websites -- All DOE Office Websites (Extended Search)

ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PYE M1 Browse Data Point Reyes, CA SBS M1 Browse Data Steamboat Springs CO,...

183

ARM - Instrument - irt  

NLE Websites -- All DOE Office Websites (Extended Search)

Niger OLI M1 Browse Data Oliktok Point, Alaska PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PYE M1 Browse Data Point Reyes, CA Contact(s) Victor Morris (509) 372-6144...

184

ARM - VAP Product - qcrad1long  

NLE Websites -- All DOE Office Websites (Extended Search)

ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PYE M1 Browse Data Point Reyes, CA SBS M1 Browse Data Steamboat Springs CO,...

185

ARM - Datastreams - irt200ms  

NLE Websites -- All DOE Office Websites (Extended Search)

Australia ARM Mobile Facility GRW M1 Browse Data Graciosa Island, Azores, Portugal OLI M1 Browse Data Oliktok Point, Alaska PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1...

186

ARM - Instrument - gndrad  

NLE Websites -- All DOE Office Websites (Extended Search)

ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PYE M1 Browse Data Point Reyes, CA SBS M1 Browse Data Steamboat Springs CO,...

187

ARM - Instrument - skyrad  

NLE Websites -- All DOE Office Websites (Extended Search)

ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PYE M1 Browse Data Point Reyes, CA SBS M1 Browse Data Steamboat Springs CO,...

188

ARM - Datastreams - nfov2ch  

NLE Websites -- All DOE Office Websites (Extended Search)

Shouxian, Anhui, China PGH M1 Browse Data ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PYE M1 Browse Data Point Reyes, CA...

189

ARM - Instrument - met  

NLE Websites -- All DOE Office Websites (Extended Search)

ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PYE M1 Browse Data Point Reyes, CA SBS M1 Browse Data Steamboat Springs CO,...

190

ARM - Datastreams - vceil25k  

NLE Websites -- All DOE Office Websites (Extended Search)

ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PYE M1 Browse Data Point Reyes, CA SBS M1 Browse Data Steamboat Springs CO,...

191

ARM - Instrument - mwrp  

NLE Websites -- All DOE Office Websites (Extended Search)

Data Niamey, Niger PGH M1 Browse Data ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PYE M1 Browse Data Point Reyes, CA...

192

Image reduction pipeline for the detection of variable sources in highly crowded fields  

E-Print Network (OSTI)

We present a reduction pipeline for CCD (charge-coupled device) images which was built to search for variable sources in highly crowded fields like the M31 bulge and to handle extensive databases due to large time series. We describe all steps of the standard reduction in detail with emphasis on the realisation of per pixel error propagation: Bias correction, treatment of bad pixels, flatfielding, and filtering of cosmic rays. The problems of conservation of PSF (point spread function) and error propagation in our image alignment procedure as well as the detection algorithm for variable sources are discussed: We build difference images via image convolution with a technique called OIS (Alard & Lupton, 1998), proceed with an automatic detection of variable sources in noise dominated images and finally apply a PSF-fitting, relative photometry to the sources found. For the WeCAPP project (Riffeser et al., 2001) we achieve 3 sigma detections for variable sources with an apparent brightness of e.g. m = 24.9 mag at their minimum and a variation of dm = 2.4 mag (or m = 21.9 mag brightness minimum and a variation of dm = 0.6 mag) on a background signal of 18.1 mag/arcsec^2 based on a 500 s exposure with 1.5 arcsec seeing at a 1.2 m telescope. The complete per pixel error propagation allows us to give accurate errors for each measurement.

Claus A. Goessl; Arno Riffeser

2001-10-31T23:59:59.000Z

193

Scale-model Experiment of Magnetoplasma Sail for Future Deep Space Missions  

Science Conference Proceedings (OSTI)

When Magnetic sail (MagSail) spacecraft is operated in space, the supersonic solar wind plasma flow is blocked by an artificially produced magnetic cavity to accelerate the spacecraft in the direction leaving the Sun. To evaluate the momentum transferring process from the solar wind to the coil onboard the MagSail spacecraft, we arranged a laboratory experiment of MagSail spacecraft. Based on scaling considerations, a solenoidal coil was immersed into the plasma flow from a magnetoplasmadynamic arcjet in a quasi-steady mode of about 1 ms duration. In this setup, it is confirmed that a magnetic cavity, which is similar to that of the geomagnetic field, was formed around the coil to produce thrust in the ion Larmor scale interaction. Also, the controllability of magnetic cavity size by a plasma jet from inside the coil of MagSail is demonstrated, although the thrust characteristic of the MagSail with plasma jet, which is so called plasma sail, is to be clarified in our next step.

Funaki, Ikkoh [Japan Aerospace Exploration Agency, Sagamihara, Kanagawa, 229-8510 (Japan); Yamakawa, Hiroshi [Kyoto University, Uji, Kyoto, 611-0011 (Japan); Ueno, Kazuma; Kimura, Toshiyuki; Ayabe, Tomohiro; Horisawa, Hideyuki [Tokai University, Hiratsuka, Kanagawa, 259-1292 (Japan)

2008-04-28T23:59:59.000Z

194

On the newly discovered Canes Venatici II dSph galaxy  

E-Print Network (OSTI)

We report on the detection of variable stars in the Canes Venatici II (CVn II) dwarf spheroidal galaxy, a new satellite of the Milky Way recently discovered by the Sloan Digital Sky Survey. We also present a V, B-V color-magnitude diagram that reaches V = 25.5 mag, showing the galaxy's main sequence turn off at V = 24.5 mag and revealing several candidate blue straggler stars. Two RR Lyrae stars have been identified within the half-light radius of CVn II,a fundamental-mode variable (RRab) with period P_ab = 0.743 days, and a first-overtone (RRc) RR Lyrae star with P_c = 0.358 days. The rather long periods of these variables along with their position on the period-amplitude diagram support an Oosterhoff type II classification for CVn II. The average apparent magnitude of the RR Lyrae stars, = 21.48 +/- 0.02 mag, is used to obtain a precision distance modulus of mu_0 = 21.02 +/- 0.06 mag and a corresponding distance of 160(+4,-5} kpc, for an adopted reddening E(B-V) = 0.015 mag.

C. Greco; M. Dall'Ora; G. Clementini; V. Ripepi; L. Di Fabrizio; K. Kinemuchi; M. Marconi; I. Musella; H. A. Smith; C. T. Rodgers; C. Kuehn; T. C. Beers; M. Catelan; B. J. Pritzl

2007-12-13T23:59:59.000Z

195

The University of British Columbia Residential Environmental  

E-Print Network (OSTI)

...................................................................................15 EA M1.8: Energy Star Appliances. EA M1.8 ­ Energy Star Appliances 2 Specify and install Energy Star-labelled dishwashers

Strynadka, Natalie

196

Page not found | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

01 - 3110 of 26,777 results. 01 - 3110 of 26,777 results. Download Application to Export Electric Energy OE Docket No. EA-306-A MAG Energy Solutions, Inc. Application from MAG Energy Solutions, Inc. to export electric energy to Canada http://energy.gov/oe/downloads/application-export-electric-energy-oe-docket-no-ea-306-mag-energy-solutions-inc Download PP-366 Twin Rivers Paper Company, Inc. http://energy.gov/oe/downloads/pp-366-twin-rivers-paper-company-inc Download Application to export electric energy OE Docket No. EA-349 Bruce Power Inc http://energy.gov/oe/downloads/application-export-electric-energy-oe-docket-no-ea-349-bruce-power-inc Download PP-82-2 Vermont Electric Power Company, Inc. (VELCO) Presidential Permit authorizing Vermont Electric Power Company, Inc. (VELCO) to construct, operate and maintain electric transmission facilities

197

Page not found | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

01 - 5510 of 8,172 results. 01 - 5510 of 8,172 results. Download Application to Export Electric Energy OE Docket No. EA-306-A MAG Energy Solutions: Federal Register Notice Volume 75, No. 237- Dec. 10, 2010 Application from MAG Energy Solutions to esport electric energy to Canada. Federal Register Notice. http://energy.gov/oe/downloads/application-export-electric-energy-oe-docket-no-ea-306-mag-energy-solutions-federal Download Superconductivity Program Overview http://energy.gov/oe/downloads/superconductivity-program-overview Download High-Temperature Superconductivity Cable Demonstration Projects http://energy.gov/oe/downloads/high-temperature-superconductivity-cable-demonstration-projects Download Western Resource Adequacy: Challenges- Approaches- Metrics http://energy.gov/oe/downloads/western-resource-adequacy-challenges-approaches-metrics

198

SCP06G4  

NLE Websites -- All DOE Office Websites (Extended Search)

G4 "Shaya" G4 "Shaya" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3207.94 , 4506.01) Gaussian Fit (3207.87 , 4505.94) RA,DEC (14:29:18.743 , +34:38:37.39) Cluster Offset 80.1 arcsec Redshift 1.350 Redshift from host Cluster Redshift 1.26 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN Ia Typing based on a,b,c Discovery 1 ep = 06 (3207.99,4506.42) mag = 25.378 apsig = 5.723 Discovery 2 ep = 07 (3207.92,4505.54) mag = 24.096 apsig = 17.287 Discovery 3 ep = 09 (3207.68,4505.93) mag = 24.347 apsig = 15.220 Discovery 4 ep = 10 (3208.20,4506.16) mag = 25.087 apsig = 9.004

199

SCP06F6  

NLE Websites -- All DOE Office Websites (Extended Search)

F6 F6 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3710.64 , 2604.82) Gaussian Fit (3710.66 , 2604.78) RA,DEC (14:32:27.395 , +33:32:24.84) Cluster Offset 35.9 arcsec Redshift 1.189 Redshift from sn Cluster Redshift 1.11 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN non-Ia Typing based on a Discovery 1 ep = 05 (3710.60,2604.84) mag = 22.105 apsig = 67.928 Discovery 2 ep = 06 (3710.63,2604.76) mag = 21.583 apsig = 94.530 Discovery 3 ep = 07 (3710.63,2604.83) mag = 21.283 apsig = 109.318 Discovery 4 ep = 08 (3710.70,2604.86) mag = 21.165 apsig = 112.969

200

SCP05D15  

NLE Websites -- All DOE Office Websites (Extended Search)

D15 D15 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (1423.31 , 4300.15) Gaussian fit RA,DEC ( 2:21:47.973 , - 3:20:52.55) Cluster Offset 103.1 arcsec Redshift Unknown Redshift from Cluster Redshift 1.02 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification AGN Typing based on Discovery 1 ep = 01 (1423.55,4299.86) mag = 24.684 apsig = 8.573 Discovery 2 ep = 02 (1423.18,4300.14) mag = 23.939 apsig = 16.857 Discovery 3 ep = 03 (1423.25,4300.19) mag = 23.756 apsig = 19.811 Discovery 4 ep = 04 (1423.40,4300.13) mag = 24.619 apsig = 8.333 Discovery 5 ep = 05 (1423.17,4300.45)

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


201

Chemical abundances of metal-poor RR Lyrae stars in the Magellanic Clouds  

E-Print Network (OSTI)

We present for the first time a detailed spectroscopic study of chemical element abundances of metal-poor RR Lyrae stars in the Large and Small Magellanic Cloud (LMC and SMC). Using the MagE echelle spectrograph at the 6.5 ...

Haschke, Raoul

202

The First Systematic Study of Type Ibc Supernova Multi-color Light-curves  

E-Print Network (OSTI)

We present detailed optical photometry for 25 Type Ibc supernovae within d~150 Mpc obtained with the robotic Palomar 60-inch telescope in 2004-2007. This study represents the first uniform, systematic, and statistical sample of multi-color SNe Ibc light-curves available to date. We correct the light-curves for host galaxy extinction using a new technique based on the photometric color evolution, namely, we show that the (V-R) color of extinction-corrected SNe Ibc at t~10 days after V-band maximum is tightly distributed, (V-R)=0.26+-0.06 mag. Using this technique, we find that SNe Ibc typically suffer from significant host galaxy extinction, E(B-V)~0.4 mag. A comparison of the extinction-corrected light-curves for SNe Ib and Ic reveals that they are statistically indistinguishable, both in luminosity and decline rate. We report peak absolute magnitudes of M_R=-17.9+-0.9 mag and M_R=-18.3+-0.6 mag for SNe Ib and Ic, respectively. Focusing on the broad-lined SNe Ic, we find that they are more luminous than the n...

Drout, Maria R; Gal-Yam, A; Cenko, S B; Fox, D B; Leonard, D C; Sand, D J; Moon, D -S; Arcavi, I; Green, Y

2010-01-01T23:59:59.000Z

203

Simulating the thermochemical magmatic and tectonic evolution of Venus's mantle and lithosphere  

E-Print Network (OSTI)

mode of heat loss is magmatic heat pipe, which requires massive magmatism and produces very thick crust modes, with a viscosity profile that is Earth-like but shifted to higher values. The basalt densityW/m2 . If widespread melting occurs then a mag- matic "heat pipe" mechanism, as is commonly thought

Tackley, Paul J.

204

CENTER FOR RADIOLOGICAL RESEARCH ANNUAL REPORT 2004 RARAF -Table of Contents  

E-Print Network (OSTI)

CENTER FOR RADIOLOGICAL RESEARCH · ANNUAL REPORT 2004 RARAF - Table of Contents RARAF Staff of the stand-alone microbeam vacuum sys- tem and installation and testing of the quadrupole mag- nets. Research and scored directly, in other experiments unir- radiated cells are physically separated from the irradiated

205

Efficient in vitro TRAIL-gene delivery in drug-resistant A2780/DDP ovarian cancer cell line via magnetofection  

Science Conference Proceedings (OSTI)

Tumor necrosis factor-related apoptosis-inducing ligand (TRAIL) presents great promise as an anticancer agent for human cancer therapy. In this study, a magnetofection agent (polyMAG-l000) was evaluated for in vitro delivery of TRAIL gene towards drugresistant ...

Fang Li; Sumei Niu; Jing Sun; Huaishi Zhu; Qiujie Ba; Yi Guo; Donglu Shi

2011-01-01T23:59:59.000Z

206

Global Methodology to Integrate Innovative Models for Electric Motors in Complete Vehicle Simulators  

E-Print Network (OSTI)

. 66 (2011), No. 5878 ABBREVIATIONS EM Electric Motor FE Finite Element FEA Finite Element Analysis FEM: the Interior Magnet Synchronous Motor with V-shape mag- net, (V-IPMSM), technology used in the Toyota Prius II, the electro- magnetic parameters of the Toyota Prius II Electric Motor are estimated thanks to the presented

Paris-Sud XI, Université de

207

doi: 10.1130/GES00506.1 2010;6;211-224Geosphere  

E-Print Network (OSTI)

are common within doler- ite sill intrusions in the Karoo Basin in South Africa. The dikes are subvertical affected by mag- matic sill intrusions (i.e., volcanic basins), like the Karoo Basin in South breccias within sills in the Karoo Basin. However, the results can be applied to other sedimentary basins

Svensen, Henrik

208

Annales Geophysicae (2004) 22: 20472052 SRef-ID: 1432-0576/ag/2004-22-2047  

E-Print Network (OSTI)

when mag- netic energy that has built up in the solar atmosphere is sud- denly released (Carrington (Anastasiadis, 1999). The energy released during solar flare is used in intense local- ized heating, particle). These high-energy radiation reach the Earth's ionosphere and heat the plasma. All solar flare events selected

Paris-Sud XI, Université de

209

UNIVERSITY OF WASHINGTON'S Fifth Annual Undergraduate Research Symposium  

E-Print Network (OSTI)

are characterized by the presence of in- tracellular, single-domain magnetic inclusions, termed mag- netosomes, that serve to orient the bacteria along the earth's magnetic field lines. This may have a role in maintaining. However, magnetic enrichment procedures [100] have been used to obtain relatively purified preparations

Klavins, Eric

210

Transcranial Magnetic Stimulation in a Finger-tapping Task Separates Motor from Timing  

E-Print Network (OSTI)

Transcranial Magnetic Stimulation in a Finger- tapping Task Separates Motor from Timing Mechanisms,3 , and Elisha Moses1 Abstract & We study the interplay between motor programs and their timing in the brain by using precise pulses of transcranial mag- netic stimulation (TMS) applied to the primary motor cortex

Moses, Elisha

211

arXiv:1103.2923v1[math.OC]15Mar2011 Estimation of Saturation of Permanent-Magnet  

E-Print Network (OSTI)

arXiv:1103.2923v1[math.OC]15Mar2011 Estimation of Saturation of Permanent-Magnet Synchronous Motors a parametric model of the saturated Permanent-Magnet Synchronous Motor (PMSM) together with an estimation: Permanent magnet synchronous motor, mag- netic circuit modeling, magnetic saturation, energy-based mod

Paris-Sud XI, Université de

212

A 2.15 hr ORBITAL PERIOD FOR THE LOW-MASS X-RAY BINARY XB 1832-330 IN THE GLOBULAR CLUSTER NGC 6652  

Science Conference Proceedings (OSTI)

We present a candidate orbital period for the low-mass X-ray binary (LMXB) XB 1832-330 in the globular cluster NGC 6652 using a 6.5 hr Gemini South observation of the optical counterpart of the system. Light curves in g' and r' for two LMXBs in the cluster, sources A and B in previous literature, were extracted and analyzed for periodicity using the ISIS image subtraction package. A clear sinusoidal modulation is evident in both of A's curves, of amplitude {approx}0.11 mag in g' and {approx}0.065 mag in r', while B's curves exhibit rapid flickering, of amplitude {approx}1 mag in g' and {approx}0.5 mag in r'. A Lomb-Scargle test revealed a 2.15 hr periodic variation in the magnitude of A with a false alarm probability less than 10{sup -11}, and no significant periodicity in the light curve for B. Though it is possible that saturated stars in the vicinity of our sources partially contaminated our signal, the identification of A's binary period is nonetheless robust.

Engel, M. C.; Heinke, C. O.; Sivakoff, G. R.; Elshamouty, K. G. [Physics Department, 4-183 CCIS, University of Alberta, Edmonton, AB T6G 2E1 (Canada); Edmonds, P. D., E-mail: mcengel@ualberta.ca, E-mail: heinke@ualberta.ca [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2012-03-10T23:59:59.000Z

213

iFInstitut fr Forschungsinformation  

E-Print Network (OSTI)

in die deutsche Schwankliteratur eingegangen ist, mag dies illustrieren: Ein frisch gebackener Magister für das deutsche Mittelalter bis 1550 rechnet man mit rund 50.000 gelehrten Personen aus 70 Fakultäten akademische Deutsch- land, Band 3: Die deutschen Hochschulen in ihren Beziehungen zur Gegenwartskultur. Berlin

Greifswald, Ernst-Moritz-Arndt-Universität

214

Annales Geophysicae (2002) 20: 619628 c European Geophysical Society 2002 Geophysicae  

E-Print Network (OSTI)

that these slow flows are driven by mass and/or momentum transfer across the distant tail mag- netopause is explored. We establish that 40% of these flows could be driven by the transfer of approximately 4 The structure of the distant magnetotail plasma sheet (X

Paris-Sud XI, Université de

215

AGRICULTURAL SECTOR ANALYSIS ON GREENHOUSE GAS EMISSION MITIGATION IN THE UNITED STATES  

E-Print Network (OSTI)

AGRICULTURAL SECTOR ANALYSIS ON GREENHOUSE GAS EMISSION MITIGATION IN THE UNITED STATES: Agricultural Economics #12;AGRICULTURAL SECTOR ANALYSIS ON GREENHOUSE GAS EMISSION MITIGATION IN THE UNITED on Greenhouse Gas Emission Mitigation in the United States. (December 2000) Uwe Schneider, M.Ag., Humboldt

McCarl, Bruce A.

216

Annales Geophysicae, 23, 27852801, 2005 SRef-ID: 1432-0576/ag/2005-23-2785  

E-Print Network (OSTI)

to apogee is given, in- cluding the different whistler mode waves (hiss, chorus, lion roars) and broad the magnetosheath lion roars are right-handed and propagate close to the mag- netic field. An example of a combined substorms, to possibly determine their onset location. Keywords. Space Plasma Physics (Instruments and tech

Paris-Sud XI, Université de

217

Generated using version 3.0 of the official AMS LATEX template Spatial Decomposition of Climate Feedbacks in the Community1  

E-Print Network (OSTI)

) feedbacks (ASCF: Figure 2a) and longwave (LW) feedbacks (ALCF:193 Figure 2b) components. Each point.71) and the slope is 0.16 Wm-2 K-2 . When196 compared to ASCF, ALCF has a similar correlation, but a smaller slope. The physical197 interpretation is that ALCF has a tighter fit, but is less important for explaining the mag-198

Gettelman, Andrew

218

Philosophical Magazine, 1 September 2003 Vol. 83, No. 25, 29412953  

E-Print Network (OSTI)

by chemical dissolution of the glass in KOH which selectively extracts As only from As4S4 units (Kosek et al. 1983). The difference between our calculation and the result reported earlier (Kosek et al. 1983., 1973, Phys. Rev. B, 8, 756. Kosek, F., Chlebny, J., Cimpl, Z., and Masek, J., 1983, Phil. Mag. B, 47

Boolchand, Punit

219

JOURNAL OF LIGHTWAVE TECHNOLOGY, VOL. 28, NO. 4, FEBRUARY 15, 2010 1 Fiber-Wireless Networks and  

E-Print Network (OSTI)

by chemical dissolution of the glass in KOH which selectively extracts As only from As4S4 units (Kosek et al. 1983). The difference between our calculation and the result reported earlier (Kosek et al. 1983., 1973, Phys. Rev. B, 8, 756. Kosek, F., Chlebny, J., Cimpl, Z., and Masek, J., 1983, Phil. Mag. B, 47

Bakaul, Masuduzzaman

220

St-Onge, G., and J.S. Stoner. 2011. Paleomagnetism near the North Magnetic Pole: A unique vantage point for understanding the dynamics of the geomagnetic field and its secular  

E-Print Network (OSTI)

vantage point for understanding the dynamics of the geomagnetic field and its secular variationsOmagNeTiSm Near The NOrTh magNeTiC pOle a unique Vantage point for understanding the Dynamics of the geomagnetic Field and its Secular Variations abSTraCT. Along with the dramatic decrease in global geomagnetic field

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


221

SCP2003hubbletrans.pdf  

NLE Websites -- All DOE Office Websites (Extended Search)

1.0 0.5 0.0 0.5 1.0 mag. residual from empty cosmology 0.25,0.75 0.25, 0 1, 0 0.25,0.75 0.25, 0 1, 0 redshift z Supernova Cosmology Project Knop et al. (2003) CalanTololo & CfA...

222

Search for a T-odd, P-even Triple Correlation in Neutron Decay  

E-Print Network (OSTI)

beta and neutrino asymmetries, and the 560 µT mag- netic field,beta and neutrino asymmetries in the presence of trans- verse polarization and the 560 µT magnetic field.beta-asymmetry and neutrino-asymmetry terms leaving the D-coefficient term; however, the magnetic field

Chupp, T. E.

2013-01-01T23:59:59.000Z

223

UV-Continuum Slopes of >4000 z~4-8 Galaxies from the HUDF/XDF, HUDF09, ERS, CANDELS-South, and CANDELS-North Fields  

E-Print Network (OSTI)

We measure the UV-continuum slope beta for over 4000 high-redshift galaxies over a wide range of redshifts z~4-8 and luminosities from the HST HUDF/XDF, HUDF09-1, HUDF09-2, ERS, CANDELS-N, and CANDELS-S data sets. Our new beta results reach very faint levels at z~4 (-15.5 mag: 0.006 L*(z=3)), z~5 (-16.5 mag: 0.014L*(z=3)), and z~6 and z~7 (-17 mag: 0.025 L*(z=3)). Inconsistencies between previous studies led us to conduct a comprehensive review of systematic errors and develop a new technique for measuring beta that is robust against biases that arise from the impact of noise. We demonstrate, by object-by-object comparisons, that all previous studies, including our own and those done on the latest HUDF12 dataset, suffer from small systematic errors in beta. We find that after correcting for the systematic errors (typically d(beta) ~0.1-0.2) all beta results at z~7 from different groups are in excellent agreement. The mean beta we measure for faint (-18 mag: 0.1L*(z=3)) z~4, z~5, z~6, and z~7 galaxies is -2.03...

Bouwens, R J; Oesch, P A; Labbe, I; van Dokkum, P G; Trenti, M; Franx, M; Smit, R; Gonzalez, V; Magee, D

2013-01-01T23:59:59.000Z

224

Pulsating Variable Stars in the Coma Berenices dwarf spheroidal galaxy  

E-Print Network (OSTI)

We present B, V, I time-series photometry of the Coma Berenices dwarf spheroidal galaxy, a faint Milky Way satellite, recently discovered by the Sloan Digital Sky Survey. We have obtained V, B-V and V, V-I color-magnitude diagrams that reach V~23.0-23.2 mag showing the galaxy turnoff at V~21.7 mag, and have performed the first study of the variable star population of this new Milky Way companion. Two RR Lyrae stars (a fundamental-mode -RRab- and a first overtone -RRc- pulsator) and a short period variable with period P=0.12468 days were identified in the galaxy. The RRab star has a rather long period of P_ab=0.66971 days and is about 0.2 mag brighter than the RRc variable and other non-variable stars on the galaxy horizontal branch. In the period-amplitude diagram the RRab variable falls closer to the loci of Oosterhoff type-II systems and evolved fundamental-mode RR Lyrae stars in the Galactic globular cluster M3. The average apparent magnitude of the galaxy horizontal branch, =18.64+-0.04 mag, leads to a di...

Musella, I; Clementini, G; Dall'Ora, M; Kinemuchi, K; Di Fabrizio, L; Greco, C; Marconi, M; Smith, H; Radovich, M; Beers, T

2009-01-01T23:59:59.000Z

225

The ARAUCARIA project: Deep near-infrared survey of nearby galaxies. I. The distance to the Large Magellanic Cloud from K-band photometry of red clump stars  

E-Print Network (OSTI)

We have obtained deep imaging in the near-infrared J and K bands for 2 nearby fields in the bar of the LMC with the ESO NTT telescope, under exquisite seeing conditions. The K, J-K color-magnitude diagrams constructed from these data are of outstanding photometric quality and reveal the presence of several hundreds of red clump stars. Using the calibration of Alves for the K-band absolute magnitude of Hipparcos-observed red clump stars in the solar neigbourhood we derive a distance modulus to our observed LMC fields of 18.487 mag. Applying a correction for the tilt of the LMC bar with respect to the line of sight according to the geometrical model of van der Marel et al., the corresponding LMC barycenter distance is 18.501 mag. If we adopt a K-band population correction of -0.03 mag, as done by Alves et al. 2002, to account for the difference in age and metallicity between the solar neighborhood and LMC red clump star populations, we obtain an LMC barycenter distance modulus of 18.471 mag from our data. This is in excellent agreement with the result of Alves et al., and of another very recent study of Sarajedini et al. (2002) obtained from K-band photometry. However, we emphasize that current model predictions about the uncertainties of population corrections seem to indicate that errors up to about 0.12 mag may be possible, probably in any photometric band. Therefore, work must continue to tighten the constraints on these corrections. We also determine the mean red clump star magnitude in our LMC fields in the J band, which could be a useful alternative to the K band should future work reveal that population effect corrections for red clump stars in the J band are smaller, or more reliably determined than those for the K band.

G. Pietrzynski; W. Gieren

2002-08-07T23:59:59.000Z

226

International Energy and Climate Initiative - Energy+ | Open Energy  

Open Energy Info (EERE)

Initiative - Energy+ Initiative - Energy+ Jump to: navigation, search Name International Energy and Climate Initiative - Energy+ Agency/Company /Organization Norway Ministry of Foreign Affairs Partner Government of Kenya, Government of Bhutan, Government of Liberia, Government of Ethiopia, Government of Maldives, Government of Senegal, Government of Morocco, Government of Tanzania, Government of Nepal, Government of United Kingdom, Government of France, Government of Denmark, Government of Switzerland, Government of The Netherlands, Government of Republic of Korea, Government of Norway, World Bank, Asian Development Bank, African Development Bank, United Nations Environment Programme (UNEP), United Nations Development Programme (UNDP), United Nations Industrial Development Organization (UNIDO), International Energy Agency (IEA), Organisation for Economic Co-Operation and Development (OECD), Global Village Energy Partnership (GVEP), ECOWAS Regional Centre for Renewable Energy and Energy Efficiency (ECREEE), Latin American Energy Organization (OLADE), International Hydropower Association (IHA), World Business Council for Sustainable Development (WBCSD), United Nations Foundation (UNF), Center for Clean Air Policy (CCAP), World Wildlife Fund, Friends of the Earth Norway, Practical Action UK, World Future Council, Bellona

227

AOCS Official Method Cb 6-86  

Science Conference Proceedings (OSTI)

Aflatoxins M1 and M2 in Dairy Products AOCS Official Method Cb 6-86 Methods Analytical Chemistry Methods Downloads Methods Downloads Methods and Analyses DEFINITION This method determines aflatoxins M 1...

228

ARM - Instrument - mpl  

NLE Websites -- All DOE Office Websites (Extended Search)

ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PYE M1 Browse Data Point Reyes, CA SBS S1 Browse Data Steamboat Springs CO,...

229

ARM - Datastreams - aosccn100  

NLE Websites -- All DOE Office Websites (Extended Search)

PGH M1 Browse Data ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 SBS S2 Browse Data Steamboat Springs CO, Christie Peak...

230

ARM - Datastreams - mplpolfs  

NLE Websites -- All DOE Office Websites (Extended Search)

PGH M1 Browse Data ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 SBS S1 Browse Data Steamboat Springs CO, Thunderhead Lodge...

231

ARM - Instrument - nfov  

NLE Websites -- All DOE Office Websites (Extended Search)

ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PYE M1 Browse Data Point Reyes, CA Contact(s) Gary Hodges (303) 497-6460...

232

ARM - Instrument - ceilpblht  

NLE Websites -- All DOE Office Websites (Extended Search)

OK ARM Mobile Facility OLI M1 Browse Data Oliktok Point, Alaska PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 Contact(s) Yan Shi Developer (509) 375-6858 yan.shi@pnnl...

233

ARM - Instrument - dl  

NLE Websites -- All DOE Office Websites (Extended Search)

PGH M1 Browse Data ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 Contact(s) Rob Newsom (509) 372-6020 rob.newsom@pnnl...

234

ARM - Instrument - sasze  

NLE Websites -- All DOE Office Websites (Extended Search)

Spirit PGH M1 Browse Data ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 Contact(s) Connor Flynn (509) 375-2041 connor.flynn...

235

ARM - Instrument - aeri  

NLE Websites -- All DOE Office Websites (Extended Search)

ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PYE M1 Browse Data Point Reyes, CA Contact(s) Jonathan Gero 608-265-2335...

236

ARM - VAP Process - mplcmask  

NLE Websites -- All DOE Office Websites (Extended Search)

HFE M1 Browse Data Shouxian, Anhui, China PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 Contact(s) Chitra Sivaraman Developer (509) 375-2436 chitra.sivaraman@pnnl.go...

237

ARM - Instrument - sebs  

NLE Websites -- All DOE Office Websites (Extended Search)

East Arm, Darwin, Australia ARM Mobile Facility PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 SBS M1 Browse Data Steamboat Springs CO, Valley Site Contact(s) David Cook...

238

Design Considerations for Future RF Circuits 1 Behzad Razavi  

E-Print Network (OSTI)

be chosen high enough R VIF VDD R VRF VLO M 2 M 3 R VIF VDD R M 1 M 2 VRF LO LO VDD M 1 (a) (b) Supply

Razavi, Behzad

239

The extragalactic distance scale Key Project. III. The discovery of Cepheids and a new distance to M101 using the {ital Hubble} {ital Space} {ital Telescope}  

Science Conference Proceedings (OSTI)

We report on the discovery of 29 Cepheid variables in the galaxy M101 using the original Wide Field Camera (WFC) and the new Wide Field and Planetary Camera 2 (WFPC2) on the {ital Hubble} {ital Space} {ital Telescope}. We observed a field in M101 at 17 independent epochs in {ital V} (F555W), five epochs in {ital I} (F785LP/F814W), and one epoch in {ital B} (F439W), with a time interval baseline of 381 days. We have found Cepheids with periods ranging from 10 to 60 days. The data have been calibrated using WFPC2 observations with zero points derived from {omega} Cen, Pal 4, and NGC 2419 observations. This calibration has been verified by using the Medium Deep Survey (MDS) WFC photometric zero points, and ground-based secondary standards in {ital V} and {ital I}. The {ital V} calibrations agree to {plus_minus}0.06 mag, and the {ital I} calibrations agree to {plus_minus}0.04 mag. We have constructed {ital V} and {ital I} period-luminosity (PL) relations and have derived apparent distance moduli based on a distance modulus for the Large Magellanic Cloud (LMC) of 18.50 mag and a reddening of {ital E}({ital B}{minus}{ital V})=0.10 mag to the LMC Cepheids. Period-residual minimization was used to minimize the effects of Malmquist bias on the period-luminosity relation fitting process. Using a Galactic extinction law and the apparent {ital V} and {ital I} distance moduli, we have found a mean reddening for the M101 sample of {ital E}({ital B}{minus}{ital V})=0.03 mag and a true distance modulus to M101 of 29.34{plus_minus}0.17 mag, corresponding to a distance of 7.4{plus_minus}0.6 Mpc. The sources of error have been rigorously tracked through an error budget; systematic and random errors contribute roughly equally to the quoted error. The mean gas-phase metal abundances in the LMC and in the M101 outer field are similar so we expect metallicity effects to be minimal. (Abstract Truncated)

Kelson, D.D.; Illingworth, G.D. [UCO/Lick Observatory, University of California, Santa Cruz, California 95064 (United States); Freedman, W.F. [Carnegie Observatories, 813 Santa Barbara Street, Pasadena, California 91101 (United States); Graham, J.A. [Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road NW, Washington, District of Columbia 20015 (United States); Hill, R. [Carnegie Observatories, 813 Santa Barbara Street, Pasadena, California 91101 (United States); Madore, B.F. [NASA/IPAC Extragalactic Database, Infrared Processing and Analysis Center, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91125 (United States); Saha, A. [Space Telescope Institute, Homewood Campus, Baltimore, Maryland 21218 (United States); Stetson, P.B. [Dominion Astrophysical Observatory, National Research Council, 5071 West Saanich Road, Victoria, BC, V8X 4M6 (CANADA); Kennicutt, R.C. Jr. [Steward Observatory, University of Arizona, Tucson, Arizona 85721 (United States); Mould, J.R. [Mt. Stromlo and Siding Springs Observatories, Private Bag, Weston Creek Post Office ACT 2611 (Australia); Hughes, S.M. [Royal Greenwich Observatory, Madingley Road, Cambridge, (United Kingdom) CB3 0EZ; Ferrarese, L. [Space Telescope Institute, Homewood Campus, Baltimore, Maryland 21218 (United States)]|[Department of Physics and Astronomy, Bloomberg 501, Johns Hopkins University, 3400 North Charles Street, Baltimore, Maryland 21218 (United States); Phelps, R. [Carnegie Observatories, 813 Santa Barbara Street, Pasadena, California 91101 (United States); Turner, A. [Steward Observatory, University of Arizona, Tucson, Arizona 85721 (United States); Cook, K.H. [Lawrence Livermore National Laboratory, Mississippi L-401, P.O. Box 808, Livermore, California 94550 (United States); Ford, H. [Space Telescope Institute, Homewood Campus, Baltimore, Maryland 21218 (United States)

1996-05-01T23:59:59.000Z

240

Synthesis, Structure, and Molecular Dynamics of Gallium Complexes of Schizokinen and the Amphiphilic  

E-Print Network (OSTI)

). The activation parameters found for the two sequential steps of the proton independent pathway were Hq ) 25 ( 3 kcal M-1 , Sq ) 25 ( 7 cal M-1 K-1 and Hq ) 17.1 ( 0.2 kcal M-1 , Sq ) 0.3 ( 2.7 cal M-1 K-1 organic compounds that are produced by microorganisms in response to iron deficiency. These compounds

Groves, John T.

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


241

Time & Freq Sp Publication A  

Science Conference Proceedings (OSTI)

... Includes all observed geomagnetic storms, solar radiation storms (proton events) and Radio blackouts (class M1 and greater flares). ...

2003-04-23T23:59:59.000Z

242

EM for mixtures STA705 Spring 2006  

E-Print Network (OSTI)

, ) = Pr(cij = 1, yi, ) Pr(yi, ) = Pr(cij = 1, yi, ) k m=1 Pr(cim = 1, yi, ) = Pr(yi|cij = 1, )Pr(cij = 1|) k m=1 Pr(yi|cim = 1, )Pr(cim = 1|) = pjN(µj, 2 j )(yi) k m=1 pmN(µm, 2 m)(yi) For the maximization

Viele, Kert

243

dimensions Package — FiPy 3.0.1-dev144-g950431e ...  

Science Conference Proceedings (OSTI)

... 1 acres = 4046.8564224 m**2 1 amu = 1.6605402e-27 kg 1 Ang = 1e-10 m 1 atm = 101325.0 kg/s**2/m 1 b = 1e-28 m 1 bar = 100000.0 kg/s**2/m ...

2013-07-19T23:59:59.000Z

244

Notice of Intent To Prepare the Tank Closure and Waste Management Environmental Impact Statement for the Hanford Site, Richland, WA (DOE/EIS-0391) (2/2/06)  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

5 Federal Register 5 Federal Register / Vol. 71, No. 22 / Thursday, February 2, 2006 / Notices addressed as follows: Office of Electricity Delivery & Energy Reliability (Mail Code OE-20), U.S. Department of Energy, 1000 Independence Avenue, SW., Washington, DC 20585-0350 (FAX 202-586-5860). FOR FURTHER INFORMATION CONTACT: Ellen Russell (Program Office) 202-586- 9624 or Michael Skinker (Program Attorney) 202-586-2793. SUPPLEMENTARY INFORMATION: Exports of electricity from the United States to a foreign country are regulated and require authorization under section 202(e) of the Federal Power Act (FPA) (16 U.S.C. 824a(e)). On December 14, 2005, the Department of Energy (DOE) received an application from MAG E.S. to transmit electric energy from the United States to Canada. MAG E.S. is a Canadian

245

Definition: Magnetic Techniques | Open Energy Information  

Open Energy Info (EERE)

Magnetic Techniques Magnetic Techniques Jump to: navigation, search Dictionary.png Magnetic Techniques The magnetic method is the study of the distribution of magnetic minerals in the upper 20-30km of the earth's crust. The magnetic method may also be used to estimate the thickness of the crust or to constrain temperatures in the crust using the Curie isotherm (the temperatures at which minerals lose their strong magnetic properties), whichever is shallower.[1] References ↑ http://www.ipgp.fr/~diament/Imageries%20Gravi-Mag/Nabighian_etal_Mag.pdf http://www.cflhd.gov/resources/agm/geoApplications/SurfaceMethods/911MagneticMethods.cfm http://onlinelibrary.wiley.com/doi/10.1029/JB087iB06p04846/abstract Ret LikeLike UnlikeLike You like this.Sign Up to see what your friends like. rieved from

246

Microsoft Word - Transmittal of Final Audit Report A-13-02, SRS-CCP.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

DSM:MAG:13-1490:UFC 2300.00 DSM:MAG:13-1490:UFC 2300.00 Department of Energy Carlsbad Field Office P.O. Box 3090 Carlsbad, New Mexico 88221 August 6, 2013 Mr. John E. Kieling, Chief Hazardous Waste Bureau New Mexico Environment Department 2905 Rodeo Park Drive East, Building 1 Santa Fe, New Mexico 87505 Subject: Transmittal of the Final Audit Report for Recertification Audit A-13-02, SRS/CCP Dear Mr. Kieling: This letter transmits the Final Audit Report for Carlsbad Field Office (CBFO) Recertification Audit A-13-02 of the Savannah River Site Central Characterization Program (SRS/CCP) for processes performed to characterize and certify waste in accordance with the Waste Isolation

247

SCP06X18  

NLE Websites -- All DOE Office Websites (Extended Search)

X18 X18 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (4307.60 , 2177.60) Gaussian fit RA,DEC ( 9:10:39.319 , +54:21:25.89) Cluster Offset 64.8 arcsec Redshift Unknown Redshift from Cluster Redshift 1.10 Found with uniform selection No Lightcurve Cut 1, 2, 3 FAIL, FAIL, FAIL Classification SN ? Typing based on Discovery 1 ep = 00 (4307.60,2177.60) mag = 0.000 apsig = 0.000 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails) Spectroscopy Observations Num Date MJD Instrument

248

Maricopa Assn. of Governments - PV and Solar Domestic Water Heating  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Maricopa Assn. of Governments - PV and Solar Domestic Water Heating Maricopa Assn. of Governments - PV and Solar Domestic Water Heating Permitting Standards Maricopa Assn. of Governments - PV and Solar Domestic Water Heating Permitting Standards < Back Eligibility Commercial Construction Installer/Contractor Residential Savings Category Solar Buying & Making Electricity Heating & Cooling Water Heating Program Info State Arizona Program Type Solar/Wind Permitting Standards Provider Maricopa Association of Governments In an effort to promote uniformity, the Maricopa Association of Governments (MAG) approved standard procedures for securing necessary electrical/building permits for residential (single-family) and commercial PV systems. These procedures are a part of the MAG Building Code Standards. The standards address requirements for the solar installation, plans,

249

SCP06J50  

NLE Websites -- All DOE Office Websites (Extended Search)

0 0 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position ( 753.34 , 3967.62) Gaussian fit RA,DEC (14:34:56.673 , +35:20:31.22) Cluster Offset 127.0 arcsec Redshift Unknown Redshift from Cluster Redshift 1.37 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification star Typing based on Discovery 1 ep = 06 ( 753.34,3967.62) mag = 24.299 apsig = 6.443 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails) Spectroscopy All thumbnails Ep z850 z850 subtraction

250

Anisotropic intermediate valence in Yb2M3Ga9 (M = Rh, Ir)  

SciTech Connect

The intermediate valence compounds Yb{sub 2}M{sub 3}Ga{sub 9} (M = Rh, Ir) exhibit an anisotropic magnetic susceptibility. We report measurements of the temperature dependence of the 4f occupation number, n{sub f}(T), for Yb{sub 2}M{sub 3}Ga{sub 9} as well as the magnetic inelastic neutron scattering spectrum S{sub mag}({Delta}E) at 12 and 300 K for Yb{sub 2}Rh{sub 3}Ga{sub 9}. Both n{sub f}(T) and S{sub mag}({Delta}E) were calculated for the Anderson impurity model with crystal field terms within an approach based on the non-crossing approximation. These results corroborate the importance of crystal field effects in these materials; they also suggest that Anderson lattice effects are important to the physics of Yb{sub 2}M{sub 3}Ga{sub 9}.

Christianson, A.D.; Lawrence, J.M.; Lobos, A.M.; Aligia, A.A.; Bauer, E.D.; Moreno, N.O.; Booth, C.H.; Goremychkin, E.A.; Sarrao, J.L.; Thompson, J.D.; Batista, C.D.; Trouw, F.R.; Hehlen, M.P.

2005-04-26T23:59:59.000Z

251

Efficient One-Step Electrolytic Recycling of Low-Grade and Post-Consumer Magnesium Scrap  

SciTech Connect

Metal Oxygen Separation Technologies, Inc. (abbreviated MOxST, pronounced most) and Boston University (BU) have developed a new low-cost process for recycling post-consumer co-mingled and heavily-oxidized magnesium scrap, and discovered a new chemical mechanism for magnesium separations in the process. The new process, designated MagReGenTM, is very effective in laboratory experiments, and on scale-up promises to be the lowest-cost lowest-energy lowest-impact method for separating magnesium metal from aluminum while recovering oxidized magnesium. MagReGenTM uses as little as one-eighth as much energy as today's methods for recycling magnesium metal from comingled scrap. As such, this technology could play a vital role in recycling automotive non-ferrous metals, particularly as motor vehicle magnesium/aluminum ratios increase in order to reduce vehicle weight and increase efficiency.

Adam C. Powell, IV

2012-07-19T23:59:59.000Z

252

Reference Documents:  

NLE Websites -- All DOE Office Websites (Extended Search)

LHC D1 MAGNET ASSEMBLY LHC D1 MAGNET ASSEMBLY BAY 'E' WARM & COLD TESTING PRODUCTION TRAVELER MDC No. 744 Rev. B Sheet 2 of 17 Issued: 4/3/02 UNIT SERIAL #: D1L________ Caution: During all Hypot operations in this section, ensure that the leads for the Temperature Sensors are floating and not connected to ground. 60 902 Connect Beam Tube, Quench Protection Resistors & Iron to each other and to ground. Connect coils to each other and perform 1.5 kV Hypot between coils and ground per RHIC-MAG-R-7242 and RHIC- MAG-R-7243. The leakage current must be less than 50 µa. Leakage: µa. 70 902 Connect Beam Tube, Coils & Iron to each other and to ground. Perform 1.5Kv Hypot between each connected pair of Quench Protection Resistors and ground per RHIC-

253

SCP06T54  

NLE Websites -- All DOE Office Websites (Extended Search)

4 4 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3945.78 , 3927.16) Gaussian fit RA,DEC (15:11:01.443 , + 9:04:04.20) Cluster Offset 62.5 arcsec Redshift Unknown Redshift from Cluster Redshift 0.97 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification star Typing based on Discovery 1 ep = 02 (3945.78,3927.16) mag = 24.236 apsig = 7.196 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails) Spectroscopy All thumbnails Ep z850 z850 subtraction

254

Normal-state transport in electron-doped La2-xCexCuO4 thin films in magnetic fields up to 40 Tesla  

E-Print Network (OSTI)

Normal-state transport in electron-doped La2-xCexCuO4 thin films in magnetic fields up to 40 Tesla.17 are studied in magnetic fields up to 40 Tesla. For the whole doping region investigated, the negative, the upper critical mag- netic field Bc2 order of 100 Tesla 8 is too high to be achieved. The n-type HTSCs

Moshchalkov, Victor V.

255

EARLY PHASE OBSERVATIONS OF EXTREMELY LUMINOUS TYPE Ia SUPERNOVA 2009dc  

Science Conference Proceedings (OSTI)

We present early phase observations in optical and near-infrared wavelengths for the extremely luminous Type Ia supernova (SN Ia) 2009dc. The decline rate of the light curve is DELTAm{sub 15}(B) = 0.65 +- 0.03, which is one of the slowest among SNe Ia. The peak V-band absolute magnitude is estimated to be M{sub V} = -19.90 +- 0.15 mag if no host extinction is assumed. It reaches M{sub V} = -20.19 +- 0.19 mag if we assume the host extinction of A{sub V} = 0.29 mag. SN 2009dc belongs to the most luminous class of SNe Ia, like SNe 2003fg and 2006gz. Our JHK{sub s} -band photometry shows that this SN is also one of the most luminous SNe Ia in near-infrared wavelengths. We estimate the ejected {sup 56}Ni mass of 1.2 +- 0.3 M{sub sun} for the no host extinction case (and of 1.6 +- 0.4 M{sub sun} for the host extinction of A{sub V} = 0.29 mag). The C II lambda6580 absorption line remains visible until a week after the maximum brightness, in contrast to its early disappearance in SN 2006gz. The line velocity of Si II lambda6355 is about 8000 km s{sup -1} around the maximum, being considerably slower than that of SN 2006gz. The velocity of the C II line is similar to or slightly less than that of the Si II line around the maximum. The presence of the carbon line suggests that the thick unburned C+O layer remains after the explosion. Spectropolarimetric observations by Tanaka et al. indicate that the explosion is nearly spherical. These observational facts suggest that SN 2009dc is a super-Chandrasekhar mass SN Ia.

Yamanaka, M.; Arai, A.; Chiyonobu, S.; Fukazawa, Y.; Ikejiri, Y.; Itoh, R.; Komatsu, T.; Miyamoto, H. [Department of Physical Science, Hiroshima University, Kagamiyama 1-3-1, Higashi-Hiroshima 739-8526 (Japan); Kawabata, K. S. [Hiroshima Astrophysical Science Center, Hiroshima University, Higashi-Hiroshima, Hiroshima 739-8526 (Japan); Kinugasa, K.; Hashimoto, O.; Honda, S. [Gunma Astronomical Observatory, Takayama, Gunma 377-0702 (Japan); Tanaka, M. [Department of Astronomy, School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033 (Japan); Imada, A.; Kuroda, D. [Okayama Astrophysical Observatory, National Astronomical Observatory of Japan, Kamogata, Asakuchi-shi, Okayama 719-0232 (Japan); Maeda, K.; Nomoto, K. [Institute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwa (Japan); Kamata, Y. [National Astronomical Observatory of Japan, Osawa, Mitaka, Tokyo 181-8588 (Japan); Kawai, N. [Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551 (Japan); Konishi, K., E-mail: myamanaka@hiroshima-u.ac.j [Institute for Cosmic Ray Research, University of Tokyo, 5-1-5, Kashiwanoha, Kashiwa, Chiba, 277-8582 (Japan)

2009-12-20T23:59:59.000Z

256

Solar Physics DOI: 10.1007/----  

E-Print Network (OSTI)

Solar Physics DOI: 10.1007/·····-···-···-····-· The Observed Long and Short-Term Phase Relation c Springer ···· Abstract The observed phase relations between the weak background solar mag- netic latitudes are presented. For measurements of the solar magnetic field (SMF) the low-resolution images

Zharkova, Valentina V.

257

SCP06C1  

NLE Websites -- All DOE Office Websites (Extended Search)

C1 "Midge" C1 "Midge" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2005.65 , 3118.19) Gaussian Fit (2005.58 , 3118.16) RA,DEC (12:29:33.012 , + 1:51:36.68) Cluster Offset 21.6 arcsec Redshift 0.980 Redshift from sn Cluster Redshift 0.97 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN Ia Typing based on a,c Discovery 1 ep = 02 (2005.71,3118.26) mag = 25.048 apsig = 6.335 Discovery 2 ep = 03 (2005.51,3118.14) mag = 23.468 apsig = 22.321 Discovery 3 ep = 05 (2005.72,3118.18) mag = 23.934 apsig = 14.651 Host Distance 0.964 arcsec ( 19.28 pixels) Host z850

258

SCP05P1  

NLE Websites -- All DOE Office Websites (Extended Search)

P1 "Gabe" P1 "Gabe" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3251.01 , 4841.15) Gaussian Fit (3250.97 , 4841.17) RA,DEC ( 3:37:50.352 , -28:43:02.67) Cluster Offset 116.8 arcsec Redshift 0.926 Redshift from host Cluster Redshift 1.10 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN Ia Typing based on c Discovery 1 ep = 02 (3251.12,4841.02) mag = 24.332 apsig = 14.392 Discovery 2 ep = 03 (3250.96,4841.16) mag = 23.675 apsig = 21.986 Discovery 3 ep = 04 (3250.95,4841.26) mag = 24.552 apsig = 9.166 Host Distance 0.299 arcsec ( 5.99 pixels) Host z850

259

SCP05D0  

NLE Websites -- All DOE Office Websites (Extended Search)

D0 "Frida" D0 "Frida" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3192.48 , 3088.61) Gaussian Fit (3192.58 , 3088.70) RA,DEC ( 2:21:42.066 , - 3:21:53.13) Cluster Offset 2.9 arcsec Redshift 1.014 Redshift from host Cluster Redshift 1.02 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN Ia Typing based on a,b,c Discovery 1 ep = 02 (3192.33,3088.63) mag = 24.804 apsig = 10.200 Discovery 2 ep = 03 (3192.43,3088.79) mag = 23.966 apsig = 19.830 Discovery 3 ep = 04 (3192.68,3088.41) mag = 24.788 apsig = 8.762 Host Distance 0.602 arcsec ( 12.04 pixels) Host z850

260

SCP06H3  

NLE Websites -- All DOE Office Websites (Extended Search)

H3 "Elizabeth" H3 "Elizabeth" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3157.48 , 4278.84) Gaussian Fit (3157.45 , 4278.97) RA,DEC (14:34:28.879 , +34:27:26.61) Cluster Offset 64.1 arcsec Redshift 0.850 Redshift from host Cluster Redshift 1.24 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN Ia Typing based on a,c Discovery 1 ep = 05 (3157.58,4278.61) mag = 23.987 apsig = 17.222 Discovery 2 ep = 06 (3157.44,4278.85) mag = 23.133 apsig = 33.680 Discovery 3 ep = 08 (3157.42,4279.05) mag = 24.060 apsig = 16.362 Host Distance 0.052 arcsec ( 1.03 pixels)

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


261

SCP06Z13  

NLE Websites -- All DOE Office Websites (Extended Search)

Z13 Z13 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3134.04 , 2933.96) Gaussian fit RA,DEC (22:35:20.535 , -25:57:31.86) Cluster Offset 8.4 arcsec Redshift Unknown Redshift from Cluster Redshift 1.39 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN ? Typing based on Discovery 1 ep = 08 (3134.03,2934.00) mag = 24.288 apsig = 14.058 Discovery 2 ep = 09 (3134.04,2933.92) mag = 23.582 apsig = 24.728 Host Distance 4.686 arcsec ( 93.71 pixels) Host z850 23.82 Host i775 - z850 0.33 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 )

262

SCP06U3  

NLE Websites -- All DOE Office Websites (Extended Search)

U3 U3 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2358.05 , 3167.73) Gaussian fit RA,DEC (23:45:31.377 , -36:32:40.89) Cluster Offset 26.5 arcsec Redshift 1.534 Redshift from Cluster Redshift 1.04 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification AGN Typing based on Discovery 1 ep = 03 (2358.39,3167.66) mag = 23.911 apsig = 11.595 Discovery 2 ep = 05 (2358.33,3168.04) mag = 23.657 apsig = 15.064 Discovery 3 ep = 06 (2357.44,3167.50) mag = 23.993 apsig = 11.261 Host Distance 0.033 arcsec ( 0.67 pixels) Host z850 21.85 Host i775 - z850 0.17 Flux in a 3 pixel radius aperture, including host galaxy light.

263

SCP06F3  

NLE Websites -- All DOE Office Websites (Extended Search)

F3 F3 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3979.54 , 2334.25) Gaussian fit RA,DEC (14:32:26.319 , +33:32:11.31) Cluster Offset 51.1 arcsec Redshift Unknown Redshift from Cluster Redshift 1.11 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification AGN Typing based on Discovery 1 ep = 05 (3979.41,2334.32) mag = 24.146 apsig = 11.051 Discovery 2 ep = 06 (3979.67,2334.18) mag = 24.379 apsig = 9.147 Host Distance 0.050 arcsec ( 0.99 pixels) Host z850 22.68 Host i775 - z850 0.15 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 )

264

EXPLORING THE VARIABLE SKY WITH LINEAR. I. PHOTOMETRIC RECALIBRATION WITH THE SLOAN DIGITAL SKY SURVEY  

SciTech Connect

We describe photometric recalibration of data obtained by the asteroid survey LINEAR. Although LINEAR was designed for astrometric discovery of moving objects, the data set described here contains over 5 billion photometric measurements for about 25 million objects, mostly stars. We use Sloan Digital Sky Survey (SDSS) data from the overlapping {approx}10,000 deg{sup 2} of sky to recalibrate LINEAR photometry and achieve errors of 0.03 mag for sources not limited by photon statistics with errors of 0.2 mag at r {approx} 18. With its 200 observations per object on average, LINEAR data provide time domain information for the brightest four magnitudes of the SDSS survey. At the same time, LINEAR extends the deepest similar wide-area variability survey, the Northern Sky Variability Survey, by 3 mag. We briefly discuss the properties of about 7000 visually confirmed periodic variables, dominated by roughly equal fractions of RR Lyrae stars and eclipsing binary stars, and analyze their distribution in optical and infrared color-color diagrams. The LINEAR data set is publicly available from the SkyDOT Web site.

Sesar, Branimir [Division of Physics, Mathematics and Astronomy, Caltech, Pasadena, CA 91125 (United States); Stuart, J. Scott [Lincoln Laboratory, Massachusetts Institute of Technology, Lexington, MA 02420-9108 (United States); Ivezic, Zeljko; Morgan, Dylan P.; Becker, Andrew C. [Department of Astronomy, University of Washington, Seattle, WA 98195-1580 (United States); Wozniak, Przemyslaw [Los Alamos National Laboratory, Los Alamos, NM 87545-0001 (United States)

2011-12-15T23:59:59.000Z

265

Evolution of Dust Extinction and Supernova Cosmology  

E-Print Network (OSTI)

We have made a quantitative calculation for the systematic evolution of average extinction by interstellar dust in host galaxies of high-redshift Type Ia supernovae, by using a realistic model of photometric and chemical evolution of galaxies and supernova rate histories in various galaxy types. We find that average B band extinction at z \\sim 0.5 is typically 0.1-0.2 mag larger than present, under a natural assumption that dust optical depth is proportional to gas column density and gas metallicity. This systematic evolution causes average reddening with E(B-V) \\sim 0.025-0.05 mag with the standard extinction curve, and this is comparable with the observational uncertainty of the reddening of high-redshift supernovae. Therefore, our result does not contradict the observations showing no significant reddening in high-z supernovae. However, the difference in apparent magnitude between an open universe and a \\Lambda-dominated flat universe is only \\sim 0.2 mag at z \\sim 0.5, and hence this systematic evolution of extinction should be taken into account in a reliable measurement of cosmological parameters. Considering this uncertainty, we show that it is difficult to discriminate between an open and \\Lambda-dominated flat cosmologies from the current data.

Tomonori Totani; Chiaki Kobayashi

1999-10-04T23:59:59.000Z

266

The occultation events of the Herbig Ae/Be star V1247 Ori  

E-Print Network (OSTI)

Aims: I study new deep (DeltaV ~ 1.20-1.65 mag) occultation events of the delta Scuti, Herbig Ae/Be star V1247 Ori in the Ori OB1 b association. Methods: I use the V-band ASAS light curve of V1247 Ori, which covers the last nine years, together with photometric data in the near-ultraviolet, visible, near-, and far-infrared taken from the literature. I carry out a periodogram analysis of the "cleaned" light curve and construct the spectral energy distribution of the star. Results: The star V1247 Ori is interesting for the study of the UX Orionis phenomenon, in which Herbig Ae/Be stars are occulted by their protoplanetary discs, for three reasons: brightness (V ~ 9.85 mag), large infrared excess at 20-100 mum (F_60 ~ 10 Jy), and photometric stability out of occultation (sigma(V) ~ 0.02 mag), which may help to determine the location and spatial structure of the occulting disc clumps.

Caballero, Jose A

2010-01-01T23:59:59.000Z

267

THE BRIGHT END OF THE ULTRAVIOLET LUMINOSITY FUNCTION AT z {approx} 8: NEW CONSTRAINTS FROM CANDELS DATA IN GOODS-SOUTH  

Science Conference Proceedings (OSTI)

We present new z {approx} 8 galaxy candidates from a search over {approx}95 arcmin{sup 2} of WFC3/IR data, tripling the previous search area for bright z {approx} 8 galaxies. Our analysis uses newly acquired WFC3/IR imaging data from the CANDELS Multi-Cycle Treasury program over the GOODS-South field. These new data are combined with existing deep optical Advanced Camera for Surveys (ACS) imaging to search for relatively bright (M {sub UV} search area, we identify 16 candidate z {approx} 8 galaxies, spanning a magnitude range H {sub 160,AB} = 25.7-27.9 mag. The new data show that the UV LF is a factor {approx}1.7 lower at M {sub UV} < -19.5 mag than determined from the HUDF09 and Early Release Science (ERS) data alone. Combining this new sample with the previous candidates from the HUDF09 and ERS data allows us to perform the most accurate measurement of the z {approx} 8 UV LF yet. Schechter function fits to the combined data result in a best-fit characteristic magnitude of M {sub *}(z = 8) = -20.04 {+-} 0.46 mag. The faint-end slope is very steep, though quite uncertain, with {alpha} = -2.06 {+-} 0.32. A combination of wide-area data with additional ultra-deep imaging will be required to significantly reduce the uncertainties on these parameters in the future.

Oesch, P. A.; Illingworth, G. D.; Gonzalez, V.; Magee, D. [UCO/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States); Bouwens, R. J.; Franx, M.; Labbe, I. [Leiden Observatory, Leiden University, NL-2300 RA Leiden (Netherlands); Trenti, M. [Center for Astrophysics and Space Astronomy, University of Colorado, 389-UCB, Boulder, CO 80309 (United States); Van Dokkum, P. G. [Department of Astronomy, Yale University, New Haven, CT 06520 (United States); Carollo, C. M., E-mail: poesch@ucolick.org [Institute for Astronomy, ETH Zurich, 8092 Zurich (Switzerland)

2012-11-10T23:59:59.000Z

268

A sample of mJy radio sources at 1.4 GHz in the Lynx and Hercules fields - I. Radio imaging, multicolour photometry and spectroscopy  

E-Print Network (OSTI)

With the goal of identifying high redshift radio galaxies with FRI classification, here are presented high resolution, wide-field radio observations, near infra-red and optical imaging and multi-object spectroscopy of two fields of the Leiden-Berkeley Deep Survey. These fields, Hercules.1 and Lynx.2, contain a complete sample of 81 radio sources with S(1.4 GHz) > 0.5 mJy within 0.6 square degrees. This sample will form the basis for a study of the population and cosmic evolution of high redshift, low power, FRI radio sources which will be presented in Paper II. Currently, the host galaxy identification fraction is 86% with 11 sources remaining unidentified at a level of r > 25.2 mag (Hercules; 4 sources) or r > 24.4 mag (Lynx; 7 sources) or K > 20 mag. Spectroscopic redshifts have been determined for 49% of the sample and photometric redshift estimates are presented for the remainder of the sample.

Rigby, E E; Best, P N

2007-01-01T23:59:59.000Z

269

A sample of mJy radio sources at 1.4 GHz in the Lynx and Hercules fields - I. Radio imaging, multicolour photometry and spectroscopy  

E-Print Network (OSTI)

With the goal of identifying high redshift radio galaxies with FRI classification, here are presented high resolution, wide-field radio observations, near infra-red and optical imaging and multi-object spectroscopy of two fields of the Leiden-Berkeley Deep Survey. These fields, Hercules.1 and Lynx.2, contain a complete sample of 81 radio sources with S(1.4 GHz) > 0.5 mJy within 0.6 square degrees. This sample will form the basis for a study of the population and cosmic evolution of high redshift, low power, FRI radio sources which will be presented in Paper II. Currently, the host galaxy identification fraction is 86% with 11 sources remaining unidentified at a level of r > 25.2 mag (Hercules; 4 sources) or r > 24.4 mag (Lynx; 7 sources) or K > 20 mag. Spectroscopic redshifts have been determined for 49% of the sample and photometric redshift estimates are presented for the remainder of the sample.

E. E. Rigby; I. A. Snellen; P. N. Best

2007-06-15T23:59:59.000Z

270

ON THE DETECTABILITY OF A PREDICTED MESOLENSING EVENT ASSOCIATED WITH THE HIGH PROPER MOTION STAR VB 10  

Science Conference Proceedings (OSTI)

Extrapolation of the astrometric motion of the nearby low-mass star VB 10 indicates that sometime in late 2011 December or during the first 2-3 months of 2012, the star will make a close approach to a background point source. Based on astrometric uncertainties, we estimate a 1 in 2 chance that the distance of closest approach {rho}{sub min} will be less than 100 mas, a 1 in 5 chance that {rho}{sub min} light from the background source and an astrometric shift of 3.3 mas. The lensing signal will however be significantly diluted by the light from VB 10, which is 1.5 mag brighter than the background source in B band, 5 mag brighter in I band, and 10 mag brighter in K band, making the event undetectable in all but the bluer optical bands. However, we show that if VB 10 happens to harbor a {approx}1 M{sub J} planet on a moderately wide ( Almost-Equal-To 0.18 AU-0.84 AU) orbit, there is a chance (1% to more than 10%, depending on the distance of closest approach and orbital period and inclination) that a passage of the planet closer to the background source will result in a secondary event of higher magnification. The detection of secondary events could be made possible with a several-times-per-night multi-site monitoring campaign.

Lepine, Sebastien [Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024 (United States); DiStefano, Rosanne, E-mail: lepine@amnh.org, E-mail: rd@cfa.harvard.edu [Harvard Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2012-04-10T23:59:59.000Z

271

The Blazhko behaviour of RR Geminorum II -- long-term photometric results  

E-Print Network (OSTI)

Context. RR Gem is one of the few Blazhko RR Lyrae that has photometric observations available extended enough to study the long-term courses of its pulsation and modulation properties in detail. Aims. We investigate the pulsation and modulation properties and the relations between them in RR Gem using photometric observations from the past 70 years in order to gain further insight into the nature of the Blazhko modulation. Methods. We studied the photographic, photoelectric, and CCD light curves obtained at the Konkoly Observatory and other authors' published maxima observations. Detailed analysis of the light curves, maximum brightness, and O-C data are carried out. Results. RR Gem showed modulation most of the time it was observed. The modulation amplitude showed strong variations from the undetectable level (less than 0.04 mag in maximum brightness) to about 0.20 mag. The amplitudes of the amplitude and phase modulations showed parallel changes, thus the total 'power' of the modulation have changed during the past 70 years. Parallel changes in the pulsation and modulation periods occur with a d P_mod / d P_puls = 1.6 +/- 0.8 * 10^3 ratio. We also detected 0.05-0.1 mag changes in the mean maximum brightness and mean pulsation amplitude.

Á. Sódor; B. Szeidl; J. Jurcsik

2007-04-25T23:59:59.000Z

272

Chemical and structural analysis of the Large Magellanic Cloud using the fundamental mode RR Lyrae stars  

E-Print Network (OSTI)

We present a careful and detailed light curve analysis of publicly available $I$-band data on fundamental mode RR Lyrae (RRab) stars of the Large Magellanic Cloud (LMC) obtained by the Optical Gravitational Lensing Experiment (OGLE) phase-III project. Using the Fourier parameters of $13,095$ RRab stars, metallicities and absolute magnitudes of individual stars are obtained. The representation of stars on the $P-\\phi_{31}^{V}$ plane shows the existence of three significant metallicity groups with mean metallicities as $-1.20 \\pm 0.12$ dex, $-1.57 \\pm 0.10$ dex and $-1.89 \\pm 0.09$ dex. The corresponding absolute magnitudes of these three groups are obtained as $0.70\\pm 0.08$ mag, $0.59 \\pm 0.06$ mag and $0.49 \\pm 0.08$ mag, respectively. Distribution of these three groups as a function of vertical $|z|$ distance indicates that the formation of the LMC disk predates the formation of the inner halo. Issue of the existence of a metallicity gradient as a function of galactocentric distances has also been addressed...

Deb, Sukanta

2013-01-01T23:59:59.000Z

273

Galactic Globular and Open Clusters in the Sloan Digital Sky Survey. I. Crowded Field Photometry and Cluster Fiducial Sequences in ugriz  

E-Print Network (OSTI)

We present photometry for globular and open cluster stars observed with the Sloan Digital Sky Survey (SDSS). In order to exploit over 100 million stellar objects with r < 22.5 mag observed by SDSS, we need to understand the characteristics of stars in the SDSS ugriz filters. While star clusters provide important calibration samples for stellar colors, the regions close to globular clusters, where the fraction of field stars is smallest, are too crowded for the standard SDSS photometric pipeline to process. To complement the SDSS imaging survey, we reduce the SDSS imaging data for crowded cluster fields using the DAOPHOT/ALLFRAME suite of programs and present photometry for 17 globular clusters and 3 open clusters in a SDSS value-added catalog. Our photometry and cluster fiducial sequences are on the native SDSS 2.5-meter ugriz photometric system, and the fiducial sequences can be directly applied to the SDSS photometry without relying upon any transformations. Model photometry for red giant branch and main-sequence stars obtained by Girardi et al. cannot be matched simultaneously to fiducial sequences; their colors differ by ~0.02-0.05 mag. Good agreement (< ~0.02 mag in colors) is found with Clem et al. empirical fiducial sequences in u'g'r'i'z' when using the transformation equations in Tucker et al.

Deokkeun An; Jennifer A. Johnson; James L. Clem; Brian Yanny; Constance M. Rockosi; Heather L. Morrison; Paul Harding; James E. Gunn; Carlos Allende Prieto; Timothy C. Beers; Kyle M. Cudworth; Inese I. Ivans; Zeljko Ivezic; Young Sun Lee; Robert H. Lupton; Dmitry Bizyaev; Howard Brewington; Elena Malanushenko; Viktor Malanushenko; Dan Oravetz; Kaike Pan; Audrey Simmons; Stephanie Snedden; Shannon Watters; Donald G. York

2008-07-31T23:59:59.000Z

274

GSC 02626-00896: an RR Lyrae star with a ceasing Blazhko effect and three new variables in the field  

E-Print Network (OSTI)

By analysis of Superwasp data, Srdoc and Bernhard (2012) have shown recently that GSC 02626-00896 (18:09:30.34 + 32:45:13.52) is an RRc type variable showing indications of Blazhko effect. A night by night reanalysis of the data shows that in fact a 26 d secondary period is present in the 2004 observations. However, no trace of this can be found in the 2007 and 2008 data. CCD observations of the star on 19 nights in 2012 yielded a strictly repeating light curve with a broad maximum similar to those derived from the second and third SWASP data group. A slightly revised ephemeris Max.(HJD) = 2456069.3919(43) + 0.32272138(60) d x E could be derived. The CCD observations also revealed three short period eclipsing variables in the field of GSC 02626-00896. The 15.16 R mag. GSC2.3 star N25F001920 (18:09:24.282 +32:44:51.72) shows 0.15 and 0.1 mag. shallow eclipses with the ephemeris Max.(HJD) = 2456064.5155(13) + 0.389228(18) d x E. The 15.39 R mag. GSC 2.3 N25D013720 (18:09:41.141 +32:33:46.99) is a W UMa type sta...

Groebel, Rainer

2013-01-01T23:59:59.000Z

275

SCP06U6  

NLE Websites -- All DOE Office Websites (Extended Search)

U6 U6 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3953.57 , 3031.15) Gaussian fit RA,DEC (23:45:24.757 , -36:32:47.72) Cluster Offset 15.7 arcsec Redshift Unknown Redshift from Cluster Redshift 1.04 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification AGN Typing based on Discovery 1 ep = 05 (3953.52,3031.38) mag = 25.088 apsig = 5.758 Discovery 2 ep = 06 (3953.61,3030.91) mag = 24.616 apsig = 8.693 Host Distance 0.011 arcsec ( 0.22 pixels) Host z850 23.87 Host i775 - z850 0.15 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 )

276

Total All Countries Exports of Crude Oil and Petroleum Products by  

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

Destination: Total All Countries Afghanistan Albania Algeria Andora Angola Anguilla Antigua and Barbuda Argentina Armenia Aruba Australia Austria Azerbaijan Bahama Islands Bahrain Barbados Belarus Belgium Belize Benin Bolivia Bosnia and Herzegovina Brazil Brunei Bulgaria Burma Bermuda Cambodia Cameroon Canada Cayman Islands Chad Chile China Colombia Congo (Brazzaville) Congo (Kinshasa) Costa Rica Croatia Cyprus Czech Republic Denmark Djbouti Dominica Dominican Republic Ecuador Egypt El Salvador Equatorial Guinea Eritrea Estonia Ethiopia Fiji Finland France French Guiana French Pacific Islands Gabon Georgia, Republic of Germany Ghana Gibraltar Greece Greenland Grenada Guadeloupe Guatemala Guinea Guyana Haiti Honduras Hong Kong Hungary Iceland India Indonesia Iran Iraq Ireland Israel Italy Ivory Coast Jamaica Japan Jordon Kazakhstan Kenya Korea, South Korea, North Kyrgyzstan Kutubu Kuwait Latvia Lebanon Liberia Libya Lithuania Macau S.A.R. Macedonia Madagascar Malaysia Maldives Mali Malta Marshall Islands Mauritania Mauritius Mexico Micronesia, Federated States of Midway Islands Moldova Monaco Mongolia Montenegro Montserrat Morocco Mozambique Namibia Nepal Netherlands Netherlands/Antilles New Caledonia New Zealand Nicaragua Niger Nigeria Niue Norway Oman Pakistan Panama Papau New Guinea Paracel Islands Paraguay Peru Philippines Poland Portugal Puerto Rico Qatar Romania Russia St. Kitts and Nevis St. Lucia St. Pierre and Miquelon St. Vincent and the Grenadines Samoa San Marino Saudi Arabia Senegal Serbia and Montenegro Seychelles Sierra Leone Singapore Slovakia Slovenia Soloman Islands South Africa Spain Spratly Islands Sri Lanka Sudan Suriname Swaziland Sweden Switzerland Syria Taiwan Tanzania Thailand Tonga Togo Trinidad and Tobago Tunisia Turkey Turkmenistan Turks and Caicos Islands Uganda Ukraine United Arab Emirates United Kingdom Uruguay Uzbekistan Vanuatu Venezuela Vietnam Virgin Islands (British) Virgin Islands (U.S.) Yemen Yugoslavia Zambia Period-Unit: Monthly-Thousand Barrels Monthly-Thousand Barrels per Day Annual-Thousand Barrels Annual-Thousand Barrels per Day

277

Total Net Imports of Crude Oil and Petroleum Products into the U.S.  

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

Country: Total All Countries Persian Gulf OPEC Algeria Angola Ecuador Iran Iraq Kuwait Libya Nigeria Qatar Saudi Arabia United Arab Emirates Venezuela Non OPEC Afghanistan Albania Andora Anguilla Antigua and Barbuda Argentina Armenia Aruba Australia Austria Azerbaijan Bahamas Bahrain Bangladesh Barbados Belarus Belgium Belize Benin Bermuda Bolivia Bosnia and Herzegovina Brazil Brunei Bulgaria Burma Cambodia Cameroon Canada Cayman Islands Chad Chile China Colombia Congo (Brazzaville) Congo (Kinshasa) Cook Islands Costa Rica Croatia Cyprus Czech Republic Denmark Djbouti Dominica Dominican Republic Egypt El Salvador Equatorial Guinea Ethiopia Eritrea Estonia Fiji Finland France French Pacific Islands French Guiana Gabon Georgia, Republic of Germany Ghana Gibraltar Greece Greenland Grenada Guadeloupe Guatemala Guinea Guyana Haiti Honduras Hong Kong Hungary Iceland India Indonesia Ireland Israel Italy Ivory Coast Jamaica Japan Jordan Kazakhstan Kenya Korea, South Kutubu Kyrgyzstan Latvia Lebanon Liberia Lithuania Macau S.A.R. Macedonia Madagascar Malaysia Maldives Mali Malta Marshall Islands Mauritania Mauritius Mexico Micronesia, Federated States of Midway Islands Moldova Monaco Mongolia Montenegro Montserrat Morocco Mozambique Namibia Nepal Netherlands Netherlands Antilles New Caledonia New Zealand Nicaragua Niger Niue Norway Oman Pakistan Panama Papau New Guinea Paracel Islands Paraguay Peru Philippines Poland Portugal Puerto Rico Romania Russia St. Kitts and Nevis St. Lucia St. Pierre and Miquelon St. Vincent and the Grenadines Samoa San Marino Senegal Serbia and Montenegro Sierra Leone Singapore Slovakia Slovenia South Africa Spain Spratly Islands Sri Lanka Suriname Swaziland Sweden Switzerland Syria Taiwan Tanzania Thailand Togo Tonga Trinidad and Tobago Tunisia Turkey Turkmenistan Turks and Caicos Islands Uganda Ukraine United Kingdom Uruguay Uzbekistan Vanuatu Vietnam Virgin Islands (British) Virgin Islands (U.S.) Yemen Yugoslavia Other Non OPEC Period-Unit: Monthly-Thousand Barrels per Day Annual-Thousand Barrels per Day

278

Annex A Metrics for the Smart Grid System Report  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

of technical and businessfinancial barriers to implementing dynamic pricing in the energy sector as outlined in the remainder of this section. M.1.4.1 Technical Challenges...

279

Single machine stochastic appointment sequencing and scheduling  

E-Print Network (OSTI)

linear combination of job waiting time, machine idle time, and overtime. .... Through straightforward but lengthy analysis we found finite values for M1 and M2.

280

ESS 2012 Peer Review - Advanced Materials for Flow Batteries...  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

Cu-DEA 2 m 10 m 1 m Flow Cell Tester assembly Key Issues: * Force fluid against gravity * Avoid sharp turns * Carbon feltmembrane contact * Wettability * Membrane 8...

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


281

OIML R 111-1 (E) Edition 2004  

Science Conference Proceedings (OSTI)

... field strength H EZ A m1 vertical component of earth magnetic field ... material) driven into an internal circular groove or into the threads of the tube. ...

2013-06-21T23:59:59.000Z

282

Alumina and Bauxite  

Science Conference Proceedings (OSTI)

Jul 31, 2011 ... Kinetics of Boehmite Precipitation from Supersaturated Sodium Aluminates Solutions with Ethanol-Water Solvent · M-1: Acid Cleaning of ...

283

AGE_110526_MINATEC_MoreMoore_publish_ppt ...  

Science Conference Proceedings (OSTI)

... zM 1 101 102 103 104 105 106 107 108 109 No amplification Target or signal amplification Proteins ... Hydrogels Implantable Biofuel Cells Page 34. ...

2011-10-03T23:59:59.000Z

284

Storage Ring Parameters  

NLE Websites -- All DOE Office Websites (Extended Search)

Functions (x and x '), and 1- Beam Sizes () and Divergences (') at Photon Source Points* Beam Port Angle** degrees Device Axis m m-1 x m x ' ...

285

Multiobjective optimization for sustainable groundwater management in semiarid regions  

E-Print Network (OSTI)

2003). “A Working Water Conservation Plan. ” Upper San Pedroimplementation of water conservation projects, m = 1 . . .Basin. Among the many water conservation initiatives that

McPhee, James; Yeh, William W-G.

2004-01-01T23:59:59.000Z

286

X-ray Polarization  

Science Conference Proceedings (OSTI)

... of crystal spectrometers where the energy dispersion is polarization selective. ... by observing forbidden (M1) transitions within the ground term of ...

2010-12-07T23:59:59.000Z

287

spectroscopy  

Science Conference Proceedings (OSTI)

... of crystal spectrometers where the energy dispersion is polarization selective. ... by observing forbidden (M1) transitions within the ground term of ...

2010-12-07T23:59:59.000Z

288

Current and Future Research  

Science Conference Proceedings (OSTI)

... of crystal spectrometers where the energy dispersion is polarization selective. ... by observing forbidden (M1) transitions within the ground term of ...

289

Prym varieties of curves of genus 3 - CECM  

E-Print Network (OSTI)

Definition: Prym(D/C) is the connected component of Ker(??) containing 0. Properties: ... Consider the quadratic forms / symmetric matrices: M1. = ?. ?. ?. ?. Q1.

290

Cuttings Analysis At Coso Geothermal Area (1977) | Open Energy...  

Open Energy Info (EERE)

Unknown Notes Chip samples were collected at ten foot intervals. References Galbraith, R. M. (1 May 1978) Geological and geophysical analysis of Coso Geothermal Exploration Hole...

291

Microsoft Word - Report_Shagaliev_eng.doc  

National Nuclear Security Administration (NNSA)

Shagaliev, R.M. 1 Numerical Simulation Methods Used at VNIIEF for Multidimensional Radiation and Particle Transport Problems R.M. Shagaliev Russian Federal Nuclear Center - VNIIEF,...

292

EMC-99 Advance Mailer  

Science Conference Proceedings (OSTI)

Jun 29, 1999 ... Lincoln, NE 68588-0511 ... Technology. Lincoln Laboratory. John M. ..... 1.4 µm: Frank Heinrichsdorff1; Nikolai Zakharov2; Peter Werner2;.

293

Deuteron photodisintegration with polarized photons at astrophysical energies  

E-Print Network (OSTI)

Following precise experimental studies at the Duke Free-Electron Laser Laboratory, we discuss photodisintegration of deuterons with 100% linearly polarized photons using a model independent theoretical approach taking together $M1$ and $E1$ amplitudes simultaneously. The isoscalar $M1_s$ contribution is also taken exactly into account. From the existing experimental measurement on doubly polarized thermal neutron capture, it is seen that the isoscalar $M1_s$ contribution could be of the same order of magnitude as the experimentally measured cross sections at energies relevant to Big Bang Nucleosynthesis (BBN). Therefore appropriate measurements on deuteron photodisintegration are suggested to empirically determine the $M1_s$ contribution at astrophysical energies.

G. Ramachandran; S. P. Shilpashree

2006-06-12T23:59:59.000Z

294

SDSS Standard Star Catalog for Stripe 82: the Dawn of Industrial 1% Optical Photometry  

E-Print Network (OSTI)

We describe a standard star catalog constructed using multiple SDSS photometric observations (at least four per band, with a median of ten) in the $ugriz$ system. The catalog includes 1.01 million non-variable unresolved objects from the equatorial stripe 82 ($|\\delta_{J2000}|<$ 1.266$^\\circ$) in the RA range 20h 34m to 4h 00m, and with the corresponding $r$ band (approximately Johnson V band) magnitudes in the range 14--22. The distributions of measurements for individual sources demonstrate that the photometric pipeline correctly estimates random photometric errors, which are below 0.01 mag for stars brighter than (19.5, 20.5, 20.5, 20, 18.5) in $ugriz$, respectively (about twice as good as for individual SDSS runs). Several independent tests of the internal consistency suggest that the spatial variation of photometric zeropoints is not larger than $\\sim$0.01 mag (rms). In addition to being the largest available dataset with optical photometry internally consistent at the $\\sim$1% level, this catalog provides practical definition of the SDSS photometric system. Using this catalog, we show that photometric zeropoints for SDSS observing runs can be calibrated within nominal uncertainty of 2% even for data obtained through 1 mag thick clouds, and demonstrate the existence of He and H white dwarf sequences using photometric data alone. Based on the properties of this catalog, we conclude that upcoming large-scale optical surveys such as the Large Synoptic Survey Telescope will be capable of delivering robust 1% photometry for billions of sources.

Zeljko Ivezic; J. Allyn Smith; Gajus Miknaitis; Huan Lin; Douglas Tucker

2007-03-07T23:59:59.000Z

295

THE 2MASS REDSHIFT SURVEY-DESCRIPTION AND DATA RELEASE  

SciTech Connect

We present the results of the 2MASS Redshift Survey (2MRS), a ten-year project to map the full three-dimensional distribution of galaxies in the nearby universe. The Two Micron All Sky Survey (2MASS) was completed in 2003 and its final data products, including an extended source catalog (XSC), are available online. The 2MASS XSC contains nearly a million galaxies with K{sub s} {<=} 13.5 mag and is essentially complete and mostly unaffected by interstellar extinction and stellar confusion down to a galactic latitude of |b| = 5 Degree-Sign for bright galaxies. Near-infrared wavelengths are sensitive to the old stellar populations that dominate galaxy masses, making 2MASS an excellent starting point to study the distribution of matter in the nearby universe. We selected a sample of 44,599 2MASS galaxies with K{sub s} {<=} 11.75 mag and |b| {>=} 5 Degree-Sign ({>=}8 Degree-Sign toward the Galactic bulge) as the input catalog for our survey. We obtained spectroscopic observations for 11,000 galaxies and used previously obtained velocities for the remainder of the sample to generate a redshift catalog that is 97.6% complete to well-defined limits and covers 91% of the sky. This provides an unprecedented census of galaxy (baryonic mass) concentrations within 300 Mpc. Earlier versions of our survey have been used in a number of publications that have studied the bulk motion of the Local Group, mapped the density and peculiar velocity fields out to 50 h{sup -1} Mpc, detected galaxy groups, and estimated the values of several cosmological parameters. Additionally, we present morphological types for a nearly complete sub-sample of 20,860 galaxies with K{sub s} {<=} 11.25 mag and |b| {>=} 10 Degree-Sign .

Huchra, John P.; Berlind, Perry; Calkins, Michael; Falco, Emilio; Mink, Jessica D.; Tokarz, Susan [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Macri, Lucas M. [George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, Department of Physics and Astronomy, Texas A and M University, 4242 TAMU, College Station, TX 77843 (United States); Masters, Karen L. [Institute for Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Burnaby Road, Portsmouth, PO1 3FX (United Kingdom); Jarrett, Thomas H. [Infrared Processing and Analysis Center, California Institute of Technology, 770 S Wilson Ave., Pasadena, CA 91125 (United States); Crook, Aidan C. [Microsoft Corp., 1 Microsoft Way, Redmond, WA 98052 (United States); Cutri, Roc [SEPNet (South East Physics Network) (United Kingdom); Erdogdu, Pirin; Lahav, Ofer [Department of Physics and Astronomy, University College London, London WC1E 6BT (United Kingdom); George, Teddy [Canada-France-Hawaii Telescope, 65-1238 Mamalahoa Hwy, Kamuela, HI 96743 (United States); Hutcheson, Conrad M. [Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA 94309 (United States); Mader, Jeff [Keck Observatory, 65-1120 Mamalahoa Hwy, Kamuela, HI 96743 (United States); Martimbeau, Nathalie [Planetarium de Montreal, 1000 rue Saint-Jacques, Montreal, Quebec H3C 1G7 (Canada); Schneider, Stephen [Department of Astronomy, University of Massachusetts, Amherst, MA 01003 (United States); Skrutskie, Michael [Department of Astronomy, University of Virginia, Charlottesville, VA 22904 (United States); Westover, Michael, E-mail: lmacri@tamu.edu, E-mail: karen.masters@port.ac.uk [McKinsey and Co., 1420 Fifth Ave., Ste 3100, Seattle, WA 98101 (United States)

2012-04-01T23:59:59.000Z

296

TOWARD IDENTIFYING THE UNASSOCIATED GAMMA-RAY SOURCE 1FGL J1311.7-3429 WITH X-RAY AND OPTICAL OBSERVATIONS  

Science Conference Proceedings (OSTI)

We present deep optical and X-ray follow-up observations of the bright unassociated Fermi-LAT gamma-ray source 1FGL J1311.7-3429. The source was already known as an unidentified EGRET source (3EG J1314-3431, EGR J1314-3417), hence its nature has remained uncertain for the past two decades. For the putative counterpart, we detected a quasi-sinusoidal optical modulation of {Delta}m {approx} 2 mag with a period of {approx_equal}1.5 hr in the Rc, r', and g' bands. Moreover, we found that the amplitude of the modulation and peak intensity changed by {approx}>1 mag and {approx}0.5 mag, respectively, over our total six nights of observations from 2012 March to May. Combined with Swift UVOT data, the optical-UV spectrum is consistent with a blackbody temperature, kT {approx_equal} 1 eV and the emission volume radius R{sub bb} {approx_equal} 1.5 Multiplication-Sign 10{sup 4} d{sub kpc} km (d{sub kpc} is the distance to the source in units of 1 kpc). In contrast, deep Suzaku observations conducted in 2009 and 2011 revealed strong X-ray flares with a light curve characterized with a power spectrum density of P(f) {proportional_to} f {sup -2.0{+-}0.4}, but the folded X-ray light curves suggest an orbital modulation also in X-rays. Together with the non-detection of a radio counterpart, and significant curved spectrum and non-detection of variability in gamma-rays, the source may be the second 'radio-quiet' gamma-ray emitting millisecond pulsar candidate after 1FGL J2339.7-0531, although the origin of flaring X-ray and optical variability remains an open question.

Kataoka, J.; Takahashi, Y.; Maeda, K. [Research Institute for Science and Engineering, Waseda University, 3-4-1, Okubo, Shinjuku, Tokyo 169-8555 (Japan); Yatsu, Y.; Kawai, N. [Tokyo Institute of Technology, 2-12-1, Ohokayama, Meguro, Tokyo 152-8551 (Japan); Urata, Y.; Tsai, A. [Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan (China); Cheung, C. C. [National Research Council Research Associate, National Academy of Sciences, Washington, DC 20001 (United States); Totani, T.; Makiya, R. [Department of Astronomy, Kyoto University, Kitashirakawa, Sakyo-ku, Kyoto 606-8502 (Japan); Hanayama, H.; Miyaji, T., E-mail: kataoka.jun@waseda.jp [Ishigakijima Astronomical Observatory, National Astronomical Observatory of Japan, 1024-1 Arakawa, Ishigaki, Okinawa, 907-0024 (Japan)

2012-10-01T23:59:59.000Z

297

NGC 6811: AN INTERMEDIATE-AGE CLUSTER IN THE KEPLER FIELD  

SciTech Connect

NGC 6811 is one of the four open clusters located in the Kepler spacecraft field of view. We obtained UBVRI photometry of the cluster on six nights (four of them photometric) with the 1.08 m Hall and 1.83 m Perkins telescopes at Lowell Observatory. The mean photometric precision ranges from better than 0.01 mag in the V, B - V, V - R, and V - I indices among stars brighter than magnitude 15 to about 0.05 mag for U - B at magnitude 18. We followed a Bayesian statistical approach using the Markov Chain Monte Carlo algorithm to determine the cluster reddening, distance, age, and iron content from a maximum-likelihood fit to stellar isochrones. Using the Yale-Yonsei isochrones, we derived E(B - V) 0.066 {+-} 0.025, (m - M){sub V} = 10.13 {+-} 0.19, age = 1.06 {+-} 0.19 Gyr, and Z = 0.012 {+-} 0.004 ([Fe/H] = -0.18); with the Padova isochrones, we found E(B - V) = 0.081 {+-} 0.015, (m - M){sub V} = 10.31 {+-} 0.11, age = 0.94 {+-} 0.08 Gyr, and Z = 0.012 {+-} 0.002 ([Fe/H] = -0.20). The uncertainties include possible errors in the photometric zero points of {+-}0.01 mag, but do not include uncertainties in the models. Taking into account the differences between the two sets of models, we find the best estimate for the cluster parameters to be E(B - V) = 0.074 {+-} 0.024, (m - M){sub V} = 10.22 {+-} 0.18, age = 1.00 {+-} 0.17 Gyr, and Z = 0.012 {+-} 0.004 ([Fe/H] = -0.19).

Janes, Kenneth; Hoq, Sadia [Astronomy Department, Boston University, Boston, MA 02215 (United States); Barnes, Sydney A. [Space Science Institute, Boulder, CO 80301 (United States); Meibom, Soren [Center for Astrophysics, 60 Garden St., Cambridge, MA 02138 (United States)

2013-01-01T23:59:59.000Z

298

A CATALOG OF NEAR-IR SOURCES FOUND TO BE UNRESOLVED WITH MILLIARCSECOND RESOLUTION  

SciTech Connect

Calibration is one of the long-standing problems in optical interferometric measurements, particularly with long baselines which demand stars with angular sizes on the milliarcsecond scale and no detectable companions. While systems of calibrators have been generally established for the near-infrared in the bright source regime (K {approx}< 3 mag), modern large interferometers are sensitive to significantly fainter magnitudes. We aim to provide a list of sources found to be unresolved from direct observations with high angular resolution and dynamic range, which can be used to choose interferometric calibrators. To this purpose, we have used a large number of lunar occultations recorded with the ISAAC instrument at the Very Large Telescope to select sources found to be unresolved and without close companions. An algorithm has been used to determine the limiting angular resolution achieved for each source, taking into account a noise model built from occulted and unocculted portions of the light curves. We have obtained upper limits on the angular sizes of 556 sources, with magnitudes ranging from K{sub s} Almost-Equal-To 4 to 10, with a median of 7.2 mag. The upper limits on possible undetected companions (within Almost-Equal-To 0.''5) range from K{sub s} Almost-Equal-To 8 to 13, with a median of 11.5 mag. One-third of the sources have angular sizes {<=}1 mas, and two-thirds have sizes {<=}2 mas. This list of unresolved sources matches well the capabilities of current large interferometric facilities. We also provide available cross-identifications, magnitudes, spectral types, and other auxiliary information. A fraction of the sources are found to be potentially variable. The list covers parts of the Galactic Bulge and in particular the vicinity of the Galactic Center, where extinction is very significant and traditional lists of calibrators are often insufficient.

Richichi, A. [National Astronomical Research Institute of Thailand, 191 Siriphanich Bldg., Huay Kaew Rd., Suthep, Muang, Chiang Mai 50200 (Thailand); Fors, O. [Departament Astronomia i Meteorologia and Institut de Ciencies del Cosmos (ICC), Universitat de Barcelona (UB/IEEC), Marti i Franques 1, E-08028 Barcelona (Spain); Cusano, F. [INAF-Osservatorio Astronomico di Bologna, Via Ranzani 1, I-40127 Bologna (Italy); Moerchen, M., E-mail: andrea@narit.or.th [European Southern Observatory, Casilla 19001, Santiago 19 (Chile)

2012-12-15T23:59:59.000Z

299

An Investigation of the effect of graphite degradation on irreversible  

NLE Websites -- All DOE Office Websites (Extended Search)

An Investigation of the effect of graphite degradation on irreversible An Investigation of the effect of graphite degradation on irreversible capacity in lithium-ion cells. Title An Investigation of the effect of graphite degradation on irreversible capacity in lithium-ion cells. Publication Type Journal Article Year of Publication 2008 Authors Hardwick, Laurence J., Marek Marcinek, Leanne Beer, John B. Kerr, and Robert Kostecki Journal Electrochemical Society Volume 155 Start Page A442 Issue 6 Pagination A442-A447 Keywords chromatography, electrochemical electrodes, electrochemical impedance spectroscopy, Fourier transform spectra, graphite, infrared spectra, lithium, mass spectra, Raman spectra, scanning electron microscopy, secondary cells, sputtering, surface structure Abstract The effect of surface structural damage on graphitic anodes, commonly observed in tested Li-ion cells, was investigated. Similar surface structural disorder was artificially induced in Mag-10 synthetic graphite anodes using argon-ion sputtering. Raman microscopy, scanning electron microscopy, and Brunauer-Emmett-Teller measurements confirmed that Ar-ion sputtered Mag-10 electrodes display a similar degree of surface degradation as the anodes from tested Li-ion cells. Artificially modified Mag-10 anodes showed double the irreversible charge capacity during the first formation cycle compared to fresh unaltered anodes. Impedance spectroscopy and Fourier transform infrared spectroscopy on surface-modified graphite anodes indicated the formation of a thicker and slightly more resistive solid electrolyte interphase (SEI) layer. Gas chromatography/mass spectroscopy analysis of solvent extracts from the electrodes detected the presence of new compounds with Mw on the order of 1600gmol-1 for the surface-modified electrode with no evidence of elevated Mw species for the unmodified electrode. The structural disorder induced in the graphite during long-term cycling may be responsible for the slow and continuous SEI layer reformation, and consequently, the loss of reversible capacity due to the shift of lithium inventory in cycled Li-ion cells.

300

Fermilab | Science at Fermilab | Benefits to Society | Industry  

NLE Websites -- All DOE Office Websites (Extended Search)

Industry Industry Industry: power transmission Industry: power transmission Cables made of superconducting material can carry far more electricity than conventional cables with minimal power losses. Underground copper transmission lines or power cables are near their capacity in many densely populated areas, and superconducting cables offer an opportunity to meet continued need. Further superconducting technology advances in particle physics will help contribute to this nascent industry. Industry: transportation Magnetically levitating trains use powerful superconducting magnets to suspend and propel the train. Mag-lev trains are fast and quiet compared to wheeled mass-transit systems, potentially reaching velocities comparable to jet aircraft. The superconducting magnet technology developed for particle

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


301

Physical factors controlling the ductility of bulk metallic glasses  

SciTech Connect

In order to identify key physical factor controlling the deformation and fracture behavior of bulk metallic glasses (BMGs), we compiled and analyzed the elastic moduli and compressive ductility for BMGs. In addition, new modulus data were generated in the critical ranges in order to facilitate the analysis. We have found that the intrinsic ductility of BMGs can be correlated with the bulk-to-shear modulus ratio B/G according to Pugh's [Philos. Mag. 45, 823 (1954) ] rule. In some individual BMG systems, for example, Fe based, the relationship seems to be very clear. The physical meaning of this correlation is discussed in terms of atomic bonding and connectivity.

Liu, Y. [Central South University, China; Liu, Chain T [ORNL; Zhang, Z. [University of Tennessee, Knoxville (UTK); Keppens, V. [University of Tennessee, Knoxville (UTK)

2008-01-01T23:59:59.000Z

302

NEW OPTICAL REDDENING MAPS OF THE LARGE AND SMALL MAGELLANIC CLOUDS  

SciTech Connect

We present new reddening maps of the Small Magellanic Cloud (SMC) and Large Magellanic Cloud (LMC) based on the data of the third phase of the Optical Gravitational Lensing Experiment (OGLE III). We have used two different methods to derive optical reddening maps. We adopt a theoretical mean unreddened color for the red clump (RC) in the SMC and LMC, respectively. We subdivide the photometric data for both Clouds into subfields and calculate the difference between the observed RC position and the theoretical value for each field, which provides us with the reddening value in (V - I). Furthermore, reddening values are obtained for 13490 LMC RR Lyrae ab and 1529 SMC RR Lyrae ab stars covering the whole OGLE III region of the Magellanic Clouds (MCs). The observed colors (V - I) of the RR Lyrae stars are compared with the color from the absolute magnitudes. The absolute magnitude of each RR Lyrae star is computed using its period and metallicity derived from Fourier decomposition of its light curve. In general, we find a low and uniform reddening distribution in both MCs. The RC method indicates a mean reddening of the LMC of E(V - I) = 0.09 {+-} 0.07 mag, while for the SMC E(V - I) = 0.04 {+-} 0.06 mag is obtained. With RR Lyrae stars a median value of E(V - I) = 0.11 {+-} 0.06 mag for the LMC and E(V - I) = 0.07 {+-} 0.06 mag for the SMC is found. The LMC shows very low reddening in the bar region, whereas the reddening in the star-forming leading edge and 30 Doradus is considerably higher. In the SMC, three pronounced regions with higher reddening are visible. Two are located along the bar, while the highest reddening is found in the star-forming wing of the SMC. In general, the regions with higher reddening are in good spatial agreement with infrared reddening maps as well as with reddening estimations of other studies. The position-dependent reddening values from the RC method are available via the German Astrophysical Virtual Observatory interface.

Haschke, Raoul; Grebel, Eva K.; Duffau, Sonia, E-mail: haschke@ari.uni-heidelberg.de [Astronomisches Rechen-Institut, Zentrum fuer Astronomie der Universitaet Heidelberg, Moenchhofstrasse 12-14, D-69120 Heidelberg (Germany)

2011-05-15T23:59:59.000Z

303

A WASHINGTON PHOTOMETRIC SURVEY OF THE LARGE MAGELLANIC CLOUD FIELD STAR POPULATION  

SciTech Connect

We present photometry for an unprecedented database of some 5.5 million stars distributed throughout the Large Magellanic Cloud main body, from 21 fields covering a total area of 7.6 deg{sup 2}, obtained from Washington CT{sub 1} T{sub 2} CTIO 4 m MOSAIC data. Extensive artificial star tests over the whole mosaic image data set and the observed behavior of the photometric errors with magnitude demonstrate the accuracy of the morphology and clearly delineate the position of the main features in the color-magnitude diagrams (CMDs). The representative T{sub 1}(MS TO) mags are on average {approx}0.5 mag brighter than the T{sub 1} mags for the 100% completeness level of the respective field, allowing us to derive an accurate age estimate. We have analyzed the CMD Hess diagrams and used the peaks in star counts at the main sequence turnoff and red clump (RC) locations to age date the most dominant sub-population (or 'representative' population) in the stellar population mix. The metallicity of this representative population is estimated from the locus of the most populous red giant branch track. We use these results to derive age and metallicity estimates for all of our fields. The analyzed fields span age and metallicity ranges covering most of the galaxy's lifetime and chemical enrichment, i.e., ages and metallicities between {approx}1 and 13 Gyr and {approx}-0.2 and -1.2 dex, respectively. We show that the dispersions associated with the mean ages and metallicities represent in general a satisfactory estimate of the age/metallicity spread ({approx}1-3 Gyr/0.2-0.3 dex), although a few subfields have a slightly larger age/metallicity spread. Finally, we revisit the study of the vertical structure (VS) phenomenon, a striking feature composed of stars that extend from the bottom, bluest end of the RC to {approx}0.45 mag fainter. We confirm that the VS phenomenon is not clearly seen in most of the studied fields and suggest that its occurrence is linked to some other condition(s) in addition to the appropriate age, metallicity, and the necessary red giant star density.

Piatti, Andres E. [Instituto de Astronomia y Fisica del Espacio, CC 67, Suc. 28, 1428, Ciudad de Buenos Aires (Argentina); Geisler, Doug; Mateluna, Renee, E-mail: andres@iafe.uba.ar [Departamento de Astronomia, Universidad de Concepcion, Casilla 160-C, Concepcion (Chile)

2012-10-01T23:59:59.000Z

304

THE INFRARED LIGHT CURVE OF SN 2011fe IN M101 AND THE DISTANCE TO M101  

SciTech Connect

We present near-infrared light curves of supernova (SN) 2011fe in M101, including 34 epochs in H band starting 14 days before maximum brightness in the B band. The light curve data were obtained with the WIYN High-Resolution Infrared Camera. When the data are calibrated using templates of other Type Ia SNe, we derive an apparent H-band magnitude at the epoch of B-band maximum of 10.85 {+-} 0.04. This implies a distance modulus for M101 that ranges from 28.86 to 29.17 mag, depending on which absolute calibration for Type Ia SNe is used.

Matheson, T.; Joyce, R. R.; Allen, L. E.; Saha, A.; Silva, D. R.; Binkert, W. S.; Butler, K.; Everett, M. [National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States); Wood-Vasey, W. M. [Pittsburgh Particle Physics, Astrophysics, and Cosmology Center (PITT-PACC), University of Pittsburgh, 3941 O'Hara Street, Pittsburgh, PA 15260 (United States); Adams, J. J. [Observatories of the Carnegie Institution of Washington, 813 Santa Barbara Street, Pasadena, CA 91101 (United States); Anderson, R. E.; Beck, T. L. [Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218 (United States); Bentz, M. C. [Department of Physics and Astronomy, Georgia State University, Astronomy Offices, One Park Place South SE, Suite 700, Atlanta, GA 30303 (United States); Bershady, M. A.; Eigenbrot, A.; Gallagher, J. S. [Department of Astronomy, University of Wisconsin-Madison, 475 North Charter Street, Madison, WI 53706 (United States); Camarata, M. A. [Department of Physics, Southern Connecticut State University, 501 Crescent Street, New Haven, CT 06515 (United States); Garnavich, P. M. [Department of Physics, University of Notre Dame, Notre Dame, IN 46556 (United States); Glikman, E. [Department of Astronomy, Yale University, New Haven, CT 06511 (United States); Harbeck, D., E-mail: matheson@noao.edu [WIYN Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States); and others

2012-07-20T23:59:59.000Z

305

THE AFTERGLOW AND ENVIRONMENT OF THE SHORT GRB 111117A  

Science Conference Proceedings (OSTI)

We present multi-wavelength observations of the afterglow of the short GRB 111117A, and follow-up observations of its host galaxy. From rapid optical and radio observations, we place limits of r {approx}> 25.5 mag at {delta}t Almost-Equal-To 0.55 days and F{sub {nu}}(5.8 GHz) {approx}light curve at {delta}t {approx} 3-10 Degree-Sign (depending on the circumburst density). We conclude that Chandra observations of short GRBs are effective at determining precise positions and robust host galaxy associations in the absence of optical and radio detections.

Margutti, R.; Berger, E.; Fong, W.; Zauderer, B. A.; Soderberg, A. M.; Milisavljevic, D.; Sanders, N. [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States); Cenko, S. B. [Department of Astronomy, University of California, Berkeley, CA 94720 (United States); Greiner, J. [Max-Planck-Institut fuer Extraterrestrische Physik, D-85740 Garching (Germany); Cucchiara, A. [Department of Astronomy and Astrophysics, UCO/Lick Observatory, University of California, 1156 High Street, Santa Cruz, CA 95064 (United States); Rossi, A.; Klose, S.; Schmidl, S. [Thueringer Landessternwarte Tautenburg, Sternwarte 5, D-07778 Tautenburg (Germany)

2012-09-01T23:59:59.000Z

306

Squaring the Circle: A Mathematical Meditation on the Emptiness of Meanings Without Experience  

E-Print Network (OSTI)

this is happening will be a first step in this exploration. What comes to mind in particular is the Josephson Effect (_ [2013c]) which 13 leads to the construction of highly sensitive quantum devices to measure mag- netic fields to high precision (#16;Josephson... for growth, producing new products and new ideas that will revitalise economies and promote commerce. Nothing needs to be drastically changed or dropped, simply expanded from what we have as a starting point. My other 14 motto is: #16;use what you have now...

Vassiliadis, Vassilios S.

2013-06-19T23:59:59.000Z

307

Large Structures and Galaxy Evolution in COSMOS at z < 1.1  

E-Print Network (OSTI)

We present the first identification of large-scale structures (LSS) at z $environmental effects on galaxy evolution. The COSMOS photometric redshift catalog yields a sample of $1.5\\times10^5$ galaxies with redshift accuracy, $\\Delta z_{FWHM}/(1+z) \\leq 0.1$ at z $< 1.1$ down to I$_{AB} \\leq 25$ mag. Using this sample of galaxies, we identify 42 large-scale structures and clusters. abstract truncated for astroph 25 line limit -- see preprint

N. Scoville; H. Aussel; A. Benson; A. Blain; D. Calzetti; P. Capak; R. S. Ellis; A. El-Zant; A. Finoguenov; M. Giavalisco; L. Guzzo; G. Hasinger; J. Koda; O. Lefevre; R. Massey; H. J. McCracken; B. Mobasher; A. Renzini; J. Rhodes; M. Salvato; D. B. Sanders; S. S. Sasaki; E. Schinnerer; K. Sheth; P. L. Shopbell; Y. Taniguchi; J. E. Taylor; D. J. Thompson

2006-12-14T23:59:59.000Z

308

Clean cities: Award winning coalition -- Maricopa  

DOE Green Energy (OSTI)

The Maricopa Association of Governments (MAG) Regional Council initiated the Maricopa Clean Cities Program on June 20, 1995. Its purpose was to encourage the use of alternative fuels in the Maricopa region and to obtain recognition for the steps the region had already taken to support the use of alternative fuels. One key element to Maricopa Clean Cities' success is the strong support it receives from the Arizona legislation. The Maricopa Clean Cities stakeholders are committed to increasing the number of alternative fuel vehicles and developing the infrastructure to support those vehicles.

O'Connor, K.; Raye, M.

1999-10-25T23:59:59.000Z

309

A Real Time Tax Smoothing Based Fiscal Policy Rule  

E-Print Network (OSTI)

|djdul/ U1/ D1 Pdufhw/ W1M1 Vdujhqw dqg M1 Vhssdod +5334, _Rswlpdo wd{dwlrq zlwkrxw vwdwh frqwlqjhqw ghew%/ plphr/ Xqlyhuvlw| ri Vwdqirug1 Dohvlqd/ D1 dqg D1 Gud}hq +4<<4, _Zk| duh vwdelolvdwlrqv ghod|hgB%/ Dphulfdq Hfrqrplf Uhylhz/ ;4/ 44:3044;;1 Dohvlqd/ D...

Loukoianova, Elena; Vahey, Shaun P; Wakerly, Elizabeth C

2004-06-16T23:59:59.000Z

310

Nonlin. Processes Geophys., 15, 803813, 2008 www.nonlin-processes-geophys.net/15/803/2008/  

E-Print Network (OSTI)

are available to us for three Enercon E-40 (600 kW) wind turbines in Hungary. Two of them (M1 and M2 and timeline of the records. Heavy diamonds indicate the location of three Enercon E-40 wind turbines M1, M2

Jánosi, Imre M.

311

Transcranial magnetic stimulation and functional mri reveal cortical and subcortical interactions during stop-signal response inhibition  

Science Conference Proceedings (OSTI)

Stopping an action requires suppression of the primary motor cortex M1. Inhibitory control over M1 relies on a network including the right inferior frontal cortex rIFC and the supplementary motor complex SMC, but how these regions interact to exert inhibitory ...

Bram B. Zandbelt; Mirjam Bloemendaal; Janna Marie Hoogendam; René S. Kahn; Matthijs Vink

2013-02-01T23:59:59.000Z

312

Modelling a ratchet with cold atoms in an optical lattice C. Robilliard # , D. Lucas + , and G. Grynberg  

E-Print Network (OSTI)

of an atom with an electromagnetic field, the atom having an electronic transition from a ground state be described in terms of a # system which includes the two ground state Zeeman sublevels m = -1 and m = 1 adiabatically the excited substate and to describe all the physical processes inside the two­level subspace {m

313

Modelling a ratchet with cold atoms in an optical lattice C. Robilliard  

E-Print Network (OSTI)

of an atom with an electromagnetic field, the atom having an electronic transition from a ground state be described in terms of a system which includes the two ground state Zeeman sublevels m = -1 and m = 1 adiabatically the excited substate and to describe all the physical processes inside the two-level subspace {m

Paris-Sud XI, Université de

314

Universitatsbibliothek Heidelberg Plock 107-109 Postfach 105749  

E-Print Network (OSTI)

: Reclam 2000 LA-M 1-18253 Steht auch LSA Kunst-BM 008 Altmeister moderner Kunstgeschichte / hrsg. von Begriffs / Susanne Knaller ... (Hrsg.). - München : Fink 2006 LA-M 1-22749 Baatz, Willfried: Geschichte der - Kunstbeschreibung : Ekphrasis von der Antike bis zur Gegenwart / Gottfried Boehm ... (Hrsg.). - München : Fink

Heermann, Dieter W.

315

Newsletter Signup Form  

NLE Websites -- All DOE Office Websites (Extended Search)

EETD NEWSLETTER - MANAGE SUBSCRIPTIONS EETD NEWSLETTER - MANAGE SUBSCRIPTIONS (red fields are required) Manage subscriptions: Subscribe Unsubscribe Name E-Mail Affiliation Address Address (line 2) City State/Province Zip/Postal Code Country (please select a country) none Afghanistan Albania Algeria American Samoa Andorra Angola Anguilla Antarctica Antigua and Barbuda Argentina Armenia Aruba Australia Austria Azerbaijan Bahamas Bahrain Bangladesh Barbados Belarus Belgium Belize Benin Bermuda Bhutan Bolivia Bosnia and Herzegowina Botswana Bouvet Island Brazil British Indian Ocean Territory Brunei Darussalam Bulgaria Burkina Faso Burundi Cambodia Cameroon Canada Cape Verde Cayman Islands Central African Republic Chad Chile China Christmas Island Cocos (Keeling) Islands Colombia Comoros Congo Congo, the Democratic Republic of the Cook Islands Costa Rica Cote d'Ivoire Croatia (Hrvatska) Cuba Cyprus Czech Republic Denmark Djibouti Dominica Dominican Republic East Timor Ecuador Egypt El Salvador Equatorial Guinea Eritrea Estonia Ethiopia Falkland Islands (Malvinas) Faroe Islands Fiji Finland France France, Metropolitan French Guiana French Polynesia French Southern Territories Gabon Gambia Georgia Germany Ghana Gibraltar Greece Greenland Grenada Guadeloupe Guam Guatemala Guinea Guinea-Bissau Guyana Haiti Heard and Mc Donald Islands Holy See (Vatican City State) Honduras Hong Kong Hungary Iceland India Indonesia Iran (Islamic Republic of) Iraq Ireland Israel Italy Jamaica Japan Jordan Kazakhstan Kenya Kiribati Korea, Democratic People's Republic of Korea, Republic of Kuwait Kyrgyzstan Lao People's Democratic Republic Latvia Lebanon Lesotho Liberia Libyan Arab Jamahiriya Liechtenstein Lithuania Luxembourg Macau Macedonia, The Former Yugoslav Republic of Madagascar Malawi Malaysia Maldives Mali Malta Marshall Islands Martinique Mauritania Mauritius Mayotte Mexico Micronesia, Federated States of Moldova, Republic of Monaco Mongolia Montserrat Morocco Mozambique Myanmar Namibia Nauru Nepal Netherlands Netherlands Antilles New Caledonia New Zealand Nicaragua Niger Nigeria Niue Norfolk Island Northern Mariana Islands Norway Oman Pakistan Palau Panama Papua New Guinea Paraguay Peru Philippines Pitcairn Poland Portugal Puerto Rico Qatar Reunion Romania Russian Federation Rwanda Saint Kitts and Nevis Saint LUCIA Saint Vincent and the Grenadines Samoa San Marino Sao Tome and Principe Saudi Arabia Senegal Seychelles Sierra Leone Singapore Slovakia (Slovak Republic) Slovenia Solomon Islands Somalia South Africa South Georgia and the South Sandwich Islands Spain Sri Lanka St. Helena St. Pierre and Miquelon Sudan Suriname Svalbard and Jan Mayen Islands Swaziland Sweden Switzerland Syrian Arab Republic Taiwan, Province of China Tajikistan Tanzania, United Republic of Thailand Togo Tokelau Tonga Trinidad and Tobago Tunisia Turkey Turkmenistan Turks and Caicos Islands Tuvalu Uganda Ukraine United Arab Emirates United Kingdom United States United States Minor Outlying Islands Uruguay Uzbekistan Vanuatu Venezuela Viet Nam Virgin Islands (British) Virgin Islands (U.S.) Wallis and Futuna Islands Western Sahara Yemen Yugoslavia Zambia Zimbabwe

316

Low-energy enhancement of magnetic dipole radiation  

E-Print Network (OSTI)

Magnetic dipole strength functions have been deduced from averages of a large number of $M1$ transition strengths calculated within the shell model for the nuclides $^{90}$Zr, $^{94}$Mo, $^{95}$Mo, and $^{96}$Mo. An enhancement of $M1$ strength toward low transition energy has been found for all nuclides considered. Large $M1$ strengths appear for transitions between close-lying states with configurations including proton as well as neutron high-$j$ orbits that re-couple their spins and add up their magnetic moments coherently. The $M1$ strength function deduced from the calculated $M1$ transition strengths is compatible with the low-energy enhancement found in ($^3$He,$^3$He') and $(d,p)$ experiments. The present work presents for the first time an explanation of the experimental findings.

R. Schwengner; S. Frauendorf; A. C. Larsen

2013-10-29T23:59:59.000Z

317

SCP06T53  

NLE Websites -- All DOE Office Websites (Extended Search)

3 3 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3174.05 , 1022.53) Gaussian fit RA,DEC (15:11:04.048 , + 9:01:38.97) Cluster Offset 90.5 arcsec Redshift Unknown Redshift from Cluster Redshift 0.97 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification missub Typing based on Discovery 1 ep = 01 (3174.05,1022.53) mag = 23.418 apsig = 9.816 Host Distance 0.061 arcsec ( 1.22 pixels) Host z850 20.38 Host i775 - z850 0.32 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

318

SCP06A4  

NLE Websites -- All DOE Office Websites (Extended Search)

A4 "Aki" A4 "Aki" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2291.43 , 3499.92) Gaussian Fit (2291.29 , 3499.86) RA,DEC (22:16:01.078 , -17:37:22.09) Cluster Offset 39.3 arcsec Redshift 1.193 Redshift from host Cluster Redshift 1.46 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN Ia Typing based on c Discovery 1 ep = 04 (2291.51,3499.84) mag = 24.108 apsig = 16.573 Discovery 2 ep = 06 (2291.35,3499.99) mag = 24.586 apsig = 9.011 Host Distance 0.252 arcsec ( 5.04 pixels) Host z850 22.55 Host i775 - z850 0.97 Flux in a 3 pixel radius aperture, including host galaxy light.

319

SCP06T1  

NLE Websites -- All DOE Office Websites (Extended Search)

T1 "Jane" T1 "Jane" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2436.60 , 1675.40) Gaussian fit RA,DEC (15:11:06.494 , + 9:02:11.56) Cluster Offset 70.7 arcsec Redshift 1.112 Redshift from host Cluster Redshift 0.97 Found with uniform selection No Lightcurve Cut 1, 2, 3 FAIL, FAIL, FAIL Classification SN CC Typing based on Discovery 1 ep = 00 (2436.60,1675.40) mag = 0.000 apsig = 0.000 Host Distance 0.077 arcsec ( 1.54 pixels) Host z850 24.66 Host i775 - z850 1.02 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

320

SCP06L22  

NLE Websites -- All DOE Office Websites (Extended Search)

2 2 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3207.86 , 4163.23) Gaussian fit RA,DEC (14:33:51.544 , +33:26:45.70) Cluster Offset 54.8 arcsec Redshift 1.369 Redshift from host Cluster Redshift 1.37 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification AGN Typing based on Discovery 1 ep = 01 (3207.86,4163.23) mag = 21.727 apsig = 39.174 Host Distance 1.766 arcsec ( 35.33 pixels) Host z850 23.55 Host i775 - z850 0.61 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


321

SCP06H5  

NLE Websites -- All DOE Office Websites (Extended Search)

"Emma" "Emma" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2845.71 , 3692.41) Gaussian Fit (2845.80 , 3692.54) RA,DEC (14:34:30.139 , +34:26:57.29) Cluster Offset 41.5 arcsec Redshift 1.231 Redshift from host Cluster Redshift 1.24 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN Ia Typing based on b,c Discovery 1 ep = 06 (2845.76,3692.64) mag = 24.239 apsig = 8.507 Discovery 2 ep = 08 (2845.67,3692.18) mag = 24.436 apsig = 7.104 Host Distance 0.047 arcsec ( 0.93 pixels) Host z850 21.74 Host i775 - z850 1.06 Flux in a 3 pixel radius aperture, including host galaxy light.

322

SCP06C50  

NLE Websites -- All DOE Office Websites (Extended Search)

C50 C50 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3496.42 , 3929.39) Gaussian fit RA,DEC (12:29:28.040 , + 1:52:17.23) Cluster Offset 55.6 arcsec Redshift Unknown Redshift from Cluster Redshift 0.97 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, FAIL Classification Typing based on Discovery 1 ep = 01 (3496.42,3929.39) mag = 24.735 apsig = 5.568 Host Distance 0.027 arcsec ( 0.54 pixels) Host z850 21.96 Host i775 - z850 0.54 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

323

SCP06N51  

NLE Websites -- All DOE Office Websites (Extended Search)

1 1 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3494.54 , 3312.12) Gaussian fit RA,DEC ( 2:20:54.805 , - 3:32:57.52) Cluster Offset 16.3 arcsec Redshift Unknown Redshift from Cluster Redshift 1.03 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, FAIL Classification AGN Typing based on Discovery 1 ep = 03 (3494.54,3312.12) mag = 22.417 apsig = 19.607 Host Distance 0.009 arcsec ( 0.18 pixels) Host z850 19.97 Host i775 - z850 0.21 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

324

SCP06N50  

NLE Websites -- All DOE Office Websites (Extended Search)

0 0 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3284.65 , 2644.41) Gaussian fit RA,DEC ( 2:20:55.506 , - 3:33:30.90) Cluster Offset 20.7 arcsec Redshift Unknown Redshift from Cluster Redshift 1.03 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification AGN Typing based on Discovery 1 ep = 03 (3284.65,2644.41) mag = 21.638 apsig = 34.048 Host Distance 0.010 arcsec ( 0.20 pixels) Host z850 19.60 Host i775 - z850 0.36 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

325

SCP06D52  

NLE Websites -- All DOE Office Websites (Extended Search)

2 2 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2507.53 , 2267.30) Gaussian fit RA,DEC ( 2:21:44.353 , - 3:22:34.19) Cluster Offset 51.4 arcsec Redshift Unknown Redshift from Cluster Redshift 1.02 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification missub Typing based on Discovery 1 ep = 02 (2507.53,2267.30) mag = 24.341 apsig = 6.402 Host Distance 0.106 arcsec ( 2.13 pixels) Host z850 20.39 Host i775 - z850 0.43 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

326

SCP06L55  

NLE Websites -- All DOE Office Websites (Extended Search)

5 5 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2738.01 , 3509.00) Gaussian fit RA,DEC (14:33:53.421 , +33:26:12.99) Cluster Offset 26.6 arcsec Redshift Unknown Redshift from Cluster Redshift 1.37 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 FAIL, FAIL, PASS Classification Typing based on Discovery 1 ep = 04 (2738.01,3509.00) mag = 25.017 apsig = 7.767 Host Distance 1.945 arcsec ( 38.90 pixels) Host z850 21.79 Host i775 - z850 0.67 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

327

SCP06N54  

NLE Websites -- All DOE Office Websites (Extended Search)

4 4 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2676.44 , 4916.48) Gaussian fit RA,DEC ( 2:20:57.537 , - 3:31:37.30) Cluster Offset 96.8 arcsec Redshift Unknown Redshift from Cluster Redshift 1.03 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, FAIL Classification Typing based on Discovery 1 ep = 01 (2676.44,4916.48) mag = 25.163 apsig = 7.345 Host Distance 3.037 arcsec ( 60.74 pixels) Host z850 25.13 Host i775 - z850 0.37 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

328

SCP06D51  

NLE Websites -- All DOE Office Websites (Extended Search)

1 1 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2667.05 , 3018.33) Gaussian fit RA,DEC ( 2:21:43.820 , - 3:21:56.64) Cluster Offset 23.1 arcsec Redshift Unknown Redshift from Cluster Redshift 1.02 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification AGN Typing based on Discovery 1 ep = 08 (2667.05,3018.33) mag = 24.683 apsig = 5.465 Host Distance 0.049 arcsec ( 0.98 pixels) Host z850 20.72 Host i775 - z850 0.91 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

329

SCP06E50  

NLE Websites -- All DOE Office Websites (Extended Search)

E50 E50 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (1380.22 , 3205.29) Gaussian fit RA,DEC (14:15:18.985 , +36:12:10.22) Cluster Offset 10.9 arcsec Redshift Unknown Redshift from Cluster Redshift 1.03 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification star Typing based on Discovery 1 ep = 03 (1380.22,3205.29) mag = 24.901 apsig = 5.085 Host Distance 2.343 arcsec ( 46.87 pixels) Host z850 16.75 Host i775 - z850 -0.04 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

330

SCP06E12  

NLE Websites -- All DOE Office Websites (Extended Search)

E12 "Ashley" E12 "Ashley" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (4005.21 , 3859.81) Gaussian fit RA,DEC (14:15:08.141 , +36:12:42.94) Cluster Offset 39.5 arcsec Redshift Unknown Redshift from Cluster Redshift 1.03 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN Ia Typing based on c Discovery 1 ep = 01 (4005.18,3859.93) mag = 24.369 apsig = 11.512 Discovery 2 ep = 02 (4005.24,3859.70) mag = 24.571 apsig = 9.424 Host Distance 0.045 arcsec ( 0.89 pixels) Host z850 23.80 Host i775 - z850 0.88 Flux in a 3 pixel radius aperture, including host galaxy light.

331

SCP06N52  

NLE Websites -- All DOE Office Websites (Extended Search)

2 2 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (1083.94 , 1223.82) Gaussian fit RA,DEC ( 2:21:02.856 , - 3:34:41.93) Cluster Offset 136.0 arcsec Redshift Unknown Redshift from Cluster Redshift 1.03 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification missub Typing based on Discovery 1 ep = 04 (1083.94,1223.82) mag = 23.885 apsig = 5.341 Host Distance 0.018 arcsec ( 0.36 pixels) Host z850 19.68 Host i775 - z850 0.24 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

332

SCP06J51  

NLE Websites -- All DOE Office Websites (Extended Search)

1 1 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3378.19 , 4648.80) Gaussian fit RA,DEC (14:34:45.948 , +35:21:05.28) Cluster Offset 89.0 arcsec Redshift Unknown Redshift from Cluster Redshift 1.37 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 FAIL, PASS, PASS Classification Typing based on Discovery 1 ep = 07 (3378.19,4648.80) mag = 25.186 apsig = 7.085 Host Distance 4.026 arcsec ( 80.52 pixels) Host z850 24.93 Host i775 - z850 0.16 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

333

SCP06B3  

NLE Websites -- All DOE Office Websites (Extended Search)

B3 "Isabella" B3 "Isabella" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3157.85 , 3161.62) Gaussian fit RA,DEC (22:05:50.403 , - 1:59:13.35) Cluster Offset 16.8 arcsec Redshift 0.743 Redshift from host Cluster Redshift 1.12 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN CC Typing based on c Discovery 1 ep = 07 (3157.85,3161.62) mag = 24.835 apsig = 8.495 Host Distance 0.400 arcsec ( 8.00 pixels) Host z850 22.67 Host i775 - z850 0.09 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 )

334

SCP06X26  

NLE Websites -- All DOE Office Websites (Extended Search)

6 "Joe" 6 "Joe" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (4556.43 , 3440.25) Gaussian fit RA,DEC ( 9:10:37.890 , +54:22:29.07) Cluster Offset 66.0 arcsec Redshift 1.440 Redshift from host Cluster Redshift 1.10 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN Ia Typing based on c Discovery 1 ep = 09 (4556.43,3440.25) mag = 25.175 apsig = 6.903 Host Distance 0.048 arcsec ( 0.96 pixels) Host z850 24.16 Host i775 - z850 1.34 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

335

SCP05D55  

NLE Websites -- All DOE Office Websites (Extended Search)

D55 D55 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2656.70 , 2777.29) Gaussian fit RA,DEC ( 2:21:43.855 , - 3:22:08.70) Cluster Offset 28.1 arcsec Redshift Unknown Redshift from Cluster Redshift 1.02 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, FAIL Classification SN ? Typing based on Discovery 1 ep = 01 (2656.70,2777.29) mag = 24.903 apsig = 9.548 Host Distance 0.337 arcsec ( 6.74 pixels) Host z850 23.37 Host i775 - z850 0.41 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

336

SCP06L54  

NLE Websites -- All DOE Office Websites (Extended Search)

4 4 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3191.05 , 5371.00) Gaussian fit RA,DEC (14:33:51.611 , +33:27:46.09) Cluster Offset 115.1 arcsec Redshift Unknown Redshift from Cluster Redshift 1.37 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, FAIL Classification Typing based on Discovery 1 ep = 02 (3191.05,5371.00) mag = 25.412 apsig = 5.887 Host Distance 5.010 arcsec (100.20 pixels) Host z850 21.83 Host i775 - z850 0.36 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

337

SCP06U7  

NLE Websites -- All DOE Office Websites (Extended Search)

U7 "Ingvar" U7 "Ingvar" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (1757.69 , 3115.89) Gaussian Fit (1757.77 , 3115.80) RA,DEC (23:45:33.868 , -36:32:43.49) Cluster Offset 40.6 arcsec Redshift 0.892 Redshift from host Cluster Redshift 1.04 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN CC Typing based on c Discovery 1 ep = 06 (1757.69,3115.89) mag = 24.148 apsig = 13.282 Host Distance 0.277 arcsec ( 5.55 pixels) Host z850 22.39 Host i775 - z850 0.24 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 )

338

SCP06F8  

NLE Websites -- All DOE Office Websites (Extended Search)

F8 "Ayako" F8 "Ayako" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (4428.14 , 4323.12) Gaussian Fit (4427.94 , 4323.33) RA,DEC (14:32:24.525 , +33:33:50.75) Cluster Offset 58.4 arcsec Redshift 0.789 Redshift from host Cluster Redshift 1.11 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN CC Typing based on c Discovery 1 ep = 05 (4428.14,4323.12) mag = 24.486 apsig = 9.975 Host Distance 0.168 arcsec ( 3.37 pixels) Host z850 22.98 Host i775 - z850 0.33 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 )

339

SCP06U52  

NLE Websites -- All DOE Office Websites (Extended Search)

2 2 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2320.00 , 5133.95) Gaussian fit RA,DEC (23:45:31.535 , -36:31:02.59) Cluster Offset 110.5 arcsec Redshift Unknown Redshift from Cluster Redshift 1.04 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 FAIL, PASS, PASS Classification Typing based on Discovery 1 ep = 02 (2320.00,5133.95) mag = 24.908 apsig = 6.831 Host Distance 1.404 arcsec ( 28.07 pixels) Host z850 23.89 Host i775 - z850 0.38 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

340

SCP06C0  

NLE Websites -- All DOE Office Websites (Extended Search)

C0 "Noa" C0 "Noa" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (4211.86 , 2316.34) Gaussian Fit (4211.75 , 2316.63) RA,DEC (12:29:25.655 , + 1:50:56.58) Cluster Offset 29.6 arcsec Redshift 1.092 Redshift from host Cluster Redshift 0.97 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN Ia Typing based on b,c Discovery 1 ep = 02 (4211.86,2316.34) mag = 24.333 apsig = 11.682 Host Distance 0.572 arcsec ( 11.44 pixels) Host z850 21.48 Host i775 - z850 1.09 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 )

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


341

SCP06U4  

NLE Websites -- All DOE Office Websites (Extended Search)

U4 "Julia" U4 "Julia" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2827.42 , 3070.88) Gaussian Fit (2827.30 , 3070.96) RA,DEC (23:45:29.429 , -36:32:45.74) Cluster Offset 13.7 arcsec Redshift 1.050 Redshift from host Cluster Redshift 1.04 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN Ia Typing based on a,c Discovery 1 ep = 03 (2827.56,3070.72) mag = 23.537 apsig = 14.400 Discovery 2 ep = 05 (2827.28,3071.05) mag = 24.468 apsig = 6.610 Host Distance 0.074 arcsec ( 1.49 pixels) Host z850 21.13 Host i775 - z850 0.94 Flux in a 3 pixel radius aperture, including host galaxy light.

342

SCP06H50  

NLE Websites -- All DOE Office Websites (Extended Search)

0 0 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (1830.00 , 2398.86) Gaussian fit RA,DEC (14:34:34.245 , +34:25:52.62) Cluster Offset 89.2 arcsec Redshift Unknown Redshift from Cluster Redshift 1.24 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification missub Typing based on Discovery 1 ep = 06 (1830.00,2398.86) mag = 24.914 apsig = 5.134 Host Distance 0.208 arcsec ( 4.16 pixels) Host z850 21.15 Host i775 - z850 0.44 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

343

SCP06X27  

NLE Websites -- All DOE Office Websites (Extended Search)

7 "Olivia" 7 "Olivia" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3396.15 , 2628.90) Gaussian Fit (3395.97 , 2628.78) RA,DEC ( 9:10:44.529 , +54:21:48.51) Cluster Offset 19.4 arcsec Redshift 0.435 Redshift from host Cluster Redshift 1.10 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN CC Typing based on Discovery 1 ep = 10 (3396.14,2628.90) mag = 22.991 apsig = 23.229 Discovery 2 ep = 11 (3396.16,2628.89) mag = 22.958 apsig = 24.390 Host Distance 0.297 arcsec ( 5.95 pixels) Host z850 18.95 Host i775 - z850 0.42 Flux in a 3 pixel radius aperture, including host galaxy light.

344

SCP06T55  

NLE Websites -- All DOE Office Websites (Extended Search)

5 5 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2703.52 , 3806.34) Gaussian fit RA,DEC (15:11:05.636 , + 9:03:58.16) Cluster Offset 56.8 arcsec Redshift Unknown Redshift from Cluster Redshift 0.97 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, FAIL Classification Typing based on Discovery 1 ep = 01 (2703.52,3806.34) mag = 24.429 apsig = 6.118 Host Distance 0.073 arcsec ( 1.46 pixels) Host z850 21.86 Host i775 - z850 0.51 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

345

SCP06U2  

NLE Websites -- All DOE Office Websites (Extended Search)

U2 U2 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3319.20 , 1975.30) Gaussian fit RA,DEC (23:45:27.393 , -36:33:40.57) Cluster Offset 50.6 arcsec Redshift 0.543 Redshift from host Cluster Redshift 1.04 Found with uniform selection No Lightcurve Cut 1, 2, 3 FAIL, FAIL, FAIL Classification SN ? Typing based on Discovery 1 ep = 00 (3319.20,1975.30) mag = 0.000 apsig = 0.000 Host Distance 0.817 arcsec ( 16.34 pixels) Host z850 20.33 Host i775 - z850 0.26 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

346

SCP06N53  

NLE Websites -- All DOE Office Websites (Extended Search)

3 3 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (1152.19 , 3323.76) Gaussian fit RA,DEC ( 2:21:02.628 , - 3:32:56.93) Cluster Offset 98.2 arcsec Redshift Unknown Redshift from Cluster Redshift 1.03 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification star Typing based on Discovery 1 ep = 03 (1152.19,3323.76) mag = 23.475 apsig = 8.447 Host Distance 2.140 arcsec ( 42.80 pixels) Host z850 24.73 Host i775 - z850 -0.07 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

347

SCP06L21  

NLE Websites -- All DOE Office Websites (Extended Search)

1 1 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (1343.62 , 2133.36) Gaussian fit RA,DEC (14:33:58.990 , +33:25:04.21) Cluster Offset 69.1 arcsec Redshift Unknown Redshift from Cluster Redshift 1.37 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN CC Typing based on c Discovery 1 ep = 01 (1343.62,2133.36) mag = 24.516 apsig = 11.213 Host Distance 0.094 arcsec ( 1.87 pixels) Host z850 24.05 Host i775 - z850 0.43 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

348

SCP06M50  

NLE Websites -- All DOE Office Websites (Extended Search)

0 0 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2708.72 , 3315.71) Gaussian fit RA,DEC (16:04:25.301 , +43:04:51.86) Cluster Offset 19.3 arcsec Redshift Unknown Redshift from Cluster Redshift 0.90 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN ? Typing based on Discovery 1 ep = 04 (2708.72,3315.71) mag = 24.556 apsig = 5.661 Host Distance 0.095 arcsec ( 1.90 pixels) Host z850 21.29 Host i775 - z850 0.83 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

349

SCP06V6  

NLE Websites -- All DOE Office Websites (Extended Search)

V6 "Melys-Eve" V6 "Melys-Eve" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3047.92 , 1560.33) Gaussian Fit (3047.64 , 1560.33) RA,DEC (23:19:53.428 , + 0:37:13.36) Cluster Offset 60.1 arcsec Redshift 0.903 Redshift from host Cluster Redshift 0.90 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification AGN Typing based on a Discovery 1 ep = 05 (3047.92,1560.33) mag = 23.802 apsig = 8.567 Host Distance 0.030 arcsec ( 0.61 pixels) Host z850 20.72 Host i775 - z850 0.44 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 )

350

SCP06M51  

NLE Websites -- All DOE Office Websites (Extended Search)

1 1 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3125.95 , 3167.82) Gaussian fit RA,DEC (16:04:23.396 , +43:04:44.46) Cluster Offset 8.2 arcsec Redshift Unknown Redshift from Cluster Redshift 0.90 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, FAIL, PASS Classification Typing based on Discovery 1 ep = 05 (3125.95,3167.82) mag = 24.702 apsig = 5.555 Host Distance 0.036 arcsec ( 0.73 pixels) Host z850 22.20 Host i775 - z850 0.78 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

351

SCP06R51  

NLE Websites -- All DOE Office Websites (Extended Search)

1 1 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (4513.95 , 3460.22) Gaussian fit RA,DEC ( 2:22:59.511 , - 4:35:50.78) Cluster Offset 24.8 arcsec Redshift Unknown Redshift from Cluster Redshift 1.22 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification Typing based on Discovery 1 ep = 08 (4513.95,3460.22) mag = 25.295 apsig = 5.097 Host Distance 0.346 arcsec ( 6.92 pixels) Host z850 22.16 Host i775 - z850 0.24 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

352

SCP06N55  

NLE Websites -- All DOE Office Websites (Extended Search)

5 5 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3657.94 , 4541.00) Gaussian fit RA,DEC ( 2:20:54.259 , - 3:31:56.07) Cluster Offset 76.2 arcsec Redshift Unknown Redshift from Cluster Redshift 1.03 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, FAIL, PASS Classification Typing based on Discovery 1 ep = 04 (3657.94,4541.00) mag = 25.509 apsig = 5.201 Host Distance 2.862 arcsec ( 57.25 pixels) Host z850 24.63 Host i775 - z850 0.53 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

353

SCP06C7  

NLE Websites -- All DOE Office Websites (Extended Search)

C7 C7 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position ( 954.72 , 4214.21) Gaussian fit RA,DEC (12:29:36.517 , + 1:52:31.48) Cluster Offset 76.0 arcsec Redshift 0.610 Redshift from host Cluster Redshift 0.97 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN CC Typing based on c Discovery 1 ep = 05 ( 954.72,4214.21) mag = 24.566 apsig = 7.663 Host Distance 0.838 arcsec ( 16.76 pixels) Host z850 20.52 Host i775 - z850 0.39 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

354

SCP06I50  

NLE Websites -- All DOE Office Websites (Extended Search)

I50 I50 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2528.06 , 3674.17) Gaussian fit RA,DEC (14:32:41.267 , +34:37:26.72) Cluster Offset 62.0 arcsec Redshift Unknown Redshift from Cluster Redshift 1.34 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, FAIL Classification Typing based on Discovery 1 ep = 01 (2528.06,3674.17) mag = 24.403 apsig = 7.089 Host Distance 0.254 arcsec ( 5.07 pixels) Host z850 19.91 Host i775 - z850 0.26 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

355

SCP06Q31  

NLE Websites -- All DOE Office Websites (Extended Search)

Q31 Q31 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2103.80 , 2054.70) Gaussian fit RA,DEC ( 4:39:42.482 , -29:05:46.52) Cluster Offset 66.7 arcsec Redshift Unknown Redshift from Cluster Redshift 0.95 Found with uniform selection No Lightcurve Cut 1, 2, 3 FAIL, FAIL, FAIL Classification SN ? Typing based on Discovery 1 ep = 00 (2103.80,2054.70) mag = 0.000 apsig = 0.000 Host Distance 0.278 arcsec ( 5.57 pixels) Host z850 22.47 Host i775 - z850 0.62 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

356

SCP06F50  

NLE Websites -- All DOE Office Websites (Extended Search)

F50 F50 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3956.62 , 4430.11) Gaussian fit RA,DEC (14:32:26.411 , +33:33:56.10) Cluster Offset 57.7 arcsec Redshift Unknown Redshift from Cluster Redshift 1.11 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 FAIL, FAIL, PASS Classification Typing based on Discovery 1 ep = 05 (3956.62,4430.11) mag = 24.735 apsig = 9.255 Host Distance 2.995 arcsec ( 59.91 pixels) Host z850 25.04 Host i775 - z850 0.22 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

357

SCP06Q50  

NLE Websites -- All DOE Office Websites (Extended Search)

Q50 Q50 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3049.74 , 3007.60) Gaussian fit RA,DEC ( 4:39:38.870 , -29:04:58.82) Cluster Offset 12.6 arcsec Redshift Unknown Redshift from Cluster Redshift 0.95 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, FAIL Classification Typing based on Discovery 1 ep = 09 (3049.74,3007.60) mag = 25.191 apsig = 5.469 Host Distance 0.242 arcsec ( 4.84 pixels) Host z850 21.32 Host i775 - z850 0.48 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

358

SCP06N32  

NLE Websites -- All DOE Office Websites (Extended Search)

2 2 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (4224.23 , 1795.97) Gaussian fit RA,DEC ( 2:20:52.368 , - 3:34:13.32) Cluster Offset 76.8 arcsec Redshift Unknown Redshift from Cluster Redshift 1.03 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN CC Typing based on c Discovery 1 ep = 07 (4224.23,1795.97) mag = 24.276 apsig = 14.094 Host Distance 0.132 arcsec ( 2.64 pixels) Host z850 24.20 Host i775 - z850 0.32 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

359

A detailed census of variable stars in the globular cluster NGC 6333 (M9) from CCD differential photometry  

E-Print Network (OSTI)

We report CCD $V$ and $I$ time-series photometry of the globular cluster NGC 6333 (M9). The technique of difference image analysis has been used, which enables photometric precision better than 0.05 mag for stars brighter than $V \\sim 19.0$ mag, even in the crowded central regions of the cluster. The high photometric precision has resulted in the discovery of two new RRc stars, three eclipsing binaries, seven long-term variables and one field RRab star behind the cluster. A detailed identification chart and equatorial coordinates are given for all the variable stars in the field of our images of the cluster. Our data together with literature $V$-data obtained in 1994 and 1995 allowed us to refine considerably the periods for all RR Lyrae stars. The nature of the new variables is discussed. We argue that variable V12 is a cluster member and an Anomalous Cepheid. Secular period variations, double mode pulsations and/or the Blazhko-like modulations in some RRc variables are addressed. Through the light curve Fou...

Ferro, A Arellano; Jaimes, R Figuera; Giridhar, Sunetra; Kains, N; Kuppuswamy, K; Jørgensen, U G; Alsubai, K A; Andersen, J M; Bozza, V; Browne, P; Novati, S Calchi; Damerdji, Y; Diehl, C; Dominik, M; Dreizler, S; Elyiv, A; Giannini, E; Harpsøe, K; Hessman, F V; Hinse, T C; Hundertmark, M; Juncher, D; Kerins, E; Korhonen, H; Liebig, C; Mancini, L; Mathiasen, M; Penny, M T; Rabus, M; Rahvar, S; Ricci, D; Scarpetta, G; Skottfelt, J; Snodgrass, C; Southworth, J; Surdej, J; Tregloan-Reed, J; Vilela, C; Wertz, O

2013-01-01T23:59:59.000Z

360

Characterization of the gaseous companion {\\kappa} Andromedae b: New Keck and LBTI high-contrast observations  

E-Print Network (OSTI)

We previously reported the direct detection of a low mass companion at a projected separation of 55+-2 AU around the B9 type star {\\kappa} Andromedae. The properties of the system (mass ratio, separation) make it a benchmark for the understanding of the formation and evolution of gas giant planets and brown dwarfs on wide-orbits. We present new angular differential imaging (ADI) images of the Kappa Andromedae system at 2.146 (Ks), 3.776 (L'), 4.052 (NB 4.05) and 4.78 {\\mu}m (M') obtained with Keck/NIRC2 and LBTI/LMIRCam, as well as more accurate near-infrared photometry of the star with the MIMIR instrument. We derive a more accurate J = 15.86 +- 0.21, H = 14.95 +- 0.13, Ks = 14.32 +- 0.09 mag for {\\kappa} And b. We redetect the companion in all our high contrast observations. We confirm previous contrasts obtained at Ks and L' band. We derive NB 4.05 = 13.0 +- 0.2 and M' = 13.3 +- 0.3 mag and estimate Log10(L/Lsun) = -3.76 +- 0.06. We build the 1-5 microns spectral energy distribution of the companion and co...

Bonnefoy, M; Marleau, G -D; Schlieder, J E; Wisniewski, J; Carson, J; Covey, K R; Henning, T; Biller, B; Hinz, P; Klahr, H; Boyer, A N Marsh; Zimmerman, N; Janson, M; McElwain, M; Mordasini, C; Skemer, A; Bailey, V; Defrère, D; Thalmann, C; Skrutskie, M; Allard, F; Homeier, D; Tamura, M; Feldt, M; Cumming, A; Grady, C; Brandner, W; Kandori, R; Kuzuhara, M; Fukagawa, M; Kwon, J; Kudo, T; Hashimoto, J; Kusakabe, N; Abe, L; Brandt, T; Egner, S; Guyon, O; Hayano, Y; Hayashi, M; Hayashi, S; Hodapp, K; Ishii, M; Iye, M; Knapp, G; Matsuo, T; Mede, K; Miyama, M; Morino, J -I; Moro-Martin, A; Nishimura, T; Pyo, T; Serabyn, E; Suenaga, T; Suto, H; Suzuki, R; Takahashi,; Takami, M; Takato, N; Terada, H; Tomono, D; Turner, E; Watanabe, M; Yamada, T; Takami, H; Usuda, T

2013-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


361

Globular Cluster Distance Determinations  

E-Print Network (OSTI)

The present status of the distance scale to Galactic globular clusters is reviewed. Six distance determination techniques which are deemed to be most reliable are discussed in depth. These different techniques are used to calibrate the absolute magnitude of the RR Lyrae stars. The various calibrations fall into three groups. Main sequence fitting using Hipparcos parallaxes, theoretical HB models and the RR Lyrae in the LMC all favor a bright calibration, implying a `long' globular cluster distance scale. White dwarf fitting and the astrometric distances yield a somewhat fainter RR Lyrae calibration, while the statistical parallax solution yields faint RR Lyrae stars implying a `short' distance scale to globular clusters. Various secondary distance indicators discussed all favor the long distance scale. The `long' and `short' distance scales differ by (0.31+/-0.16) mag. Averaging together all of the different distance determinations yields Mv(RR) = (0.23+/-0.04)([Fe/H] + 1.6) + (0.56+/-0.12) mag.

Brian Chaboyer

1998-08-19T23:59:59.000Z

362

The Age of the Inner Halo Globular Cluster NGC 6652  

E-Print Network (OSTI)

HST (V,I) photometry has been obtained for the inner halo globular cluster NGC 6652. The photometry reaches approximately 4 mag below the turn-off and includes a well populated horizontal branch. This cluster is located close to the Galactic center at a galactocentric distance of approximately 2.0 kpc with a reddening of E(V-I) = 0.15 +/- 0.02 and has a metallicity of [Fe/H] approximately -0.85. Based upon Delta(V) between the point on the sub-giant branch which is 0.05 mag redder than the turn-off and the horizontal branch, NGC 6652 is 11.7 +/- 1.6 Gyr old. Using this same Delta(V), precise differential ages for 47 Tuc (a thick disk globular), M107 and NGC 1851 (both halo clusters) were obtained. NGC 6652 appears to be the same age as 47 Tuc and NGC 1851 (within +/- 1.2 Gyr), while there is a slight suggestion that M107 is older than NGC 6652 by 2.3 +/- 1.5 Gyr. As this is a less than 2-sigma result, this issue needs to be investigated further before a definitive statement regarding the relative age of M107 and NGC 6652 may be made.

Brian Chaboyer; Ata Sarajedini; Taft E. Armandroff

2000-08-28T23:59:59.000Z

363

Mound-ACT*DE*CON{sup SM} feasibility study. Phase 2: Final report  

Science Conference Proceedings (OSTI)

A portion of the abandoned Miami-Erie Canal paralleling the Greater Miami River receives the runoff and storm-water discharge from Mound Laboratory. In 1969, a low-level plutonium leak contaminated sediment as far away as 1.5 mi from the Mound site along the old canal system. An estimated one million cubic feet of sediment requires remediation. The technology being evaluated for the remediation of the low-level plutonium-238 contamination of the sediment involves two processes: washing the sediments with ACT*DE*CON{sup SM} solution to dissolve the contaminant, followed by extraction of the solution and processing with the MAG*SEP{sup SM} process to concentrate the contaminant and allow reuse of the ACT*DE*CON{sup SM} solution. The processes are being optimized for pilot-scale and field demonstration. Phase 2 of the project primarily involved identification at the laboratory scale of the optimal ACT*DE*CON{sup SM} formulation, identification of the ion-exchanger and MAG*SEP{sup SM} particles, verification of the plutonium mobility in the treated soil, and evaluation of other process parameters according to a series of tasks.

NONE

1994-12-01T23:59:59.000Z

364

Results of the ROTOR-program. I. The long-term photometric variability of classical T Tauri stars  

E-Print Network (OSTI)

We present a unique, homogeneous database of photometric measurements for Classical T Tauri stars extending up to 20 years. The database contains more than 21,000 UBVR observations of 72 CTTs. All the data were collected within the framework of the ROTOR-program at Mount Maidanak Observatory (Uzbekistan) and together they constitute the longest homogeneous, accurate record of TTS variability ever assembled. We characterize the long term photometric variations of 49 CTTs with sufficient data to allow a robust statistical analysis and propose an empirical classification scheme. Several patterns of long term photometric variability are identified. The most common pattern, exhibited by a group of 15 stars which includes T Tau itself, consists of low level variability (Delta(V)<=0.4mag) with no significant changes occurring from season to season over many years. A related subgroup of 22 stars exhibits a similar stable long term variability pattern, though with larger amplitudes (up to Delta(V)~1.6 mag). Besides these representative groups, we identify three smaller groups of 3-5 stars each which have distinctive photometric properties. The long term variability of most CTTs is fairly stable and merely reflects shorter term variability due to cold and hot surface spots. Only a small fraction of CTTs undergo significant brightness changes on the long term (months, years), which probably arise from slowly varying circumstellar extinction.

K. N. Grankin; S. Yu. Melnikov; J. Bouvier; W. Herbst; V. S. Shevchenko

2006-11-01T23:59:59.000Z

365

Upgraded Coal Interest Group. Technical progress report, January 1, 1995--March 31, 1995  

SciTech Connect

This report presents information from the coal interest group. Topics of discussion at the meeting included the current political views concerning the Department of Energy and programs contained therein. The group met on January 10 and 11, in Nashville, TN. The status of various coal upgrading technologies was also reviewed. Four new technology opportunities were given reviews, Coal/Waste pellets, Custom Coals advanced technology, CSRC sulfur removing bacteria and a Mag-Mill which is a magnetic separation done within the pulverizer. Coal Waste pellets is a technology for making pellets of coal and fiber waste from recycling plants. The incentives are low cost and low sulfur and nitrogen. Lebowitz made a field trip to the pilot unit in Canton Ohio. The Mag Mill takes advantage of the natural concentration of pyrite in the pulverizer recycle stream (due to its hardness). Special magnets are installed in the mill to remove pyrite from this stream. Custom Coals reported on an advanced two step process for removal of organic sulfur from coal. Consolidated Sulfur Reduction Co. reported on a two step microbial desulfurization process.

Weber, W. [Electric Power Research Institute, Chattanooga, TN (United States); Lebowitz, H.E. [Fossil Fuel Sciences, Palo Alto, CA (United States)

1995-08-01T23:59:59.000Z

366

and  

E-Print Network (OSTI)

We investigate the prospects for detecting dust from two body collisions during the late stages of planet formation at 1–150 AU. We develop an analytic model to describe the formation of a dusty cloud of debris and use numerical coagulation and n-body calculations to predict observable signals from these events. In a minimum mass solar nebula, collisions of 100–1000 km objects at distances of 3–5 AU or less from the parent star are observable at mid-infrared wavelengths as bright clumps or rings of dust. At 24 µm, the clumps are ? 0.1–1 mag brighter than emission from dust in the background debris disk. In edge-on systems, dusty clumps produce eclipses with depths of ? 1.0 mag that last for ? 100 orbital periods. Large-scale surveys for transits from exosolar planets, such as Kepler, can plausibly detect these eclipses and provide important constraints on the terrestrial environment for ages of ? 100–300 Myr. Subject headings: planetary systems – solar system: formation – stars: formation – circumstellar matter 1.

Scott J. Kenyon; Benjamin C. Bromley

2005-01-01T23:59:59.000Z

367

VARIABILITY AND STAR FORMATION IN LEO T, THE LOWEST LUMINOSITY STAR-FORMING GALAXY KNOWN TODAY  

SciTech Connect

We present results from the first combined study of variable stars and star formation history (SFH) of the Milky Way 'ultra-faint' dwarf (UFD) galaxy Leo T, based on F606W and F814W multi-epoch archive observations obtained with the Wide Field Planetary Camera 2 on board the Hubble Space Telescope. We have detected 14 variable stars in the galaxy. They include one fundamental-mode RR Lyrae star and 11 Anomalous Cepheids with periods shorter than 1 day, thus suggesting the occurrence of multiple star formation episodes in this UFD, of which one about 10 Gyr ago produced the RR Lyrae star. A new estimate of the distance to Leo T of 409{sup +29}{sub -27} kpc (distance modulus of 23.06 {+-} 0.15 mag) was derived from the galaxy's RR Lyrae star. Our V, V - I color-magnitude diagram (CMD) of Leo T reaches V {approx} 29 mag and shows features typical of a galaxy in transition between dwarf irregular and dwarf spheroidal types. A quantitative analysis of the SFH, based on the comparison of the observed V, V - I CMD with the expected distribution of stars for different evolutionary scenarios, confirms that Leo T has a complex SFH dominated by two enhanced periods about 1.5 and 9 Gyr ago, respectively. The distribution of stars and gas shows that the galaxy has a fairly asymmetric structure.

Clementini, Gisella; Cignoni, Michele; Ramos, Rodrigo Contreras; Federici, Luciana; Tosi, Monica [INAF, Osservatorio Astronomico di Bologna, I-40127 Bologna (Italy); Ripepi, Vincenzo; Marconi, Marcella; Musella, Ilaria, E-mail: gisella.clementini@oabo.inaf.it, E-mail: rodrigo.contreras@oabo.inaf.it, E-mail: luciana.federici@oabo.inaf.it, E-mail: monica.tosi@oabo.inaf.it, E-mail: michele.cignoni@unibo.it, E-mail: ripepi@na.astro.it, E-mail: marcella@na.astro.it, E-mail: ilaria@na.astro.it [INAF, Osservatorio Astronomico di Capodimonte, I-80131 Napoli (Italy)

2012-09-10T23:59:59.000Z

368

HUBBLE SPACE TELESCOPE PHOTOMETRY OF GLOBULAR CLUSTERS IN M81  

SciTech Connect

We perform aperture photometry and profile fitting on 419 globular cluster (GC) candidates with m{sub V} {<=} 23 mag identified in Hubble Space Telescope/Advanced Camera for Surveys BVI imaging, and estimate the effective radii of the clusters. We identify 85 previously known spectroscopically confirmed clusters, and newly identify 136 objects as good cluster candidates within the 3{sigma} color and size ranges defined by the spectroscopically confirmed clusters, yielding a total of 221 probable GCs. The luminosity function peak for the 221 probable GCs with estimated total dereddening applied is V {approx} (20.26 {+-} 0.13) mag, corresponding to a distance of {approx}3.7 {+-} 0.3 Mpc. The blue and red GC candidates, and the metal-rich and metal-poor spectroscopically confirmed clusters, respectively, are similar in half-light radius. Red confirmed clusters are about 6% larger in median half-light radius than blue confirmed clusters, and red and blue good GC candidates are nearly identical in half-light radius. The total population of confirmed and 'good' candidates shows an increase in half-light radius as a function of galactocentric distance.

Nantais, Julie B. [Departamento de Astronomia, Universidad de Concepcion Av. Esteban Iturra s/n Barrio Universitario Casilla 160-C Concepcion (Chile); Huchra, John P.; Zezas, Andreas; Gazeas, Kosmas; Strader, Jay [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2011-12-15T23:59:59.000Z

369

Reddenings of FGK supergiants and classical Cepheids from spectroscopic data  

E-Print Network (OSTI)

Accurate and homogeneous atmospheric parameters (Teff, log (g), Vt, [Fe/H]) are derived for 74 FGK non-variable supergiants from high-resolution, high signal-to-noise ratio, echelle spectra. Extremely high precision for the inferred effective temperatures (10-40 K) is achieved by using the line-depth ratio method. The new data are combined with atmospheric values for 164 classical Cepheids, observed at 675 different pulsation phases, taken from our previously published studies. The derived values are correlated with unreddened B-V colours compiled from the literature for the investigated stars in order to obtain an empirical relationship of the form: (B-V)o = 57.984 - 10.3587(log Teff)^2 + 1.67572(log Teff)^3 - 3.356(log (g)) + 0.0321(Vt) + 0.2615[Fe/H] + 0.8833((log (g))(log Teff)). The expression is used to estimate colour excesses E(B-V) for individual supergiants and classical Cepheids, with a precision of +-0.05 mag. for supergiants and Cepheids with n=1-2 spectra, reaching +-0.025 mag. for Cepheids with n>2 spectra, matching uncertainties for the most sophisticated photometric techniques. The reddening scale is also a close match to the system of space reddenings for Cepheids. The application range is for spectral types F0--K0 and luminosity classes I and II.

V. V. Kovtyukh; C. Soubiran; R. E. Luck; David G. Turner; S. I. Belik; S. M. Andrievsky; F. A. Chekhonadskikh

2008-07-13T23:59:59.000Z

370

EPIC Muon Cooling Simulations using COSY INFINITY  

SciTech Connect

Next gen­er­a­tion mag­net sys­tems need­ed for cool­ing chan­nels in both neu­tri­no fac­to­ries and muon col­lid­ers will be in­no­va­tive and com­pli­cat­ed. De­sign­ing, sim­u­lat­ing and op­ti­miz­ing these sys­tems is a chal­lenge. Using COSY IN­FIN­I­TY, a dif­fer­en­tial al­ge­bra-based code, to sim­u­late com­pli­cat­ed el­e­ments can allow the com­pu­ta­tion and cor­rec­tion of a va­ri­ety of high­er order ef­fects, such as spher­i­cal and chro­mat­ic aber­ra­tions, that are dif­fi­cult to ad­dress with other sim­u­la­tion tools. As an ex­am­ple, a he­li­cal dipole mag­net has been im­ple­ment­ed and sim­u­lat­ed, and the per­for­mance of an epicyclic para­met­ric ion­iza­tion cool­ing sys­tem for muons is stud­ied and com­pared to sim­u­la­tions made using G4Beam­line, a GEAN­T4 toolk­it.

J.A. Maloney, B. Erdelyi, A. Afanasev, R.P. Johnson, S.A. Bogacz, Y.S. Derbenev, V.S. Morozov

2011-03-01T23:59:59.000Z

371

SBF Distances to Leo and Virgo using the HST  

E-Print Network (OSTI)

We have used archive HST WFPC2 data for three elliptical galaxies (NGC 3379 in the Leo I group, and NGC 4472 and NGC 4406 in the Virgo cluster) to determine their distances using the Surface Brightness Fluctuation (SBF) method as described by Tonry and Schneider (1988). A comparison of the HST results with the SBF distance moduli of Ciardullo et al (1993) shows significant disagreement and suggests that the r.m.s. error on these ground-based distance moduli is actually as large as +-0.25 mag. The agreement is only slightly improved when we compare our results with the HST and ground-based SBF distances from Ajhar et al (1997) and Tonry et al (1997); the comparison suggests that a lower limit on the error of the HST SBF distance moduli is +-0.17 mag. Overall, these results suggest that previously quoted measurement errors may underestimate the true error in SBF distance moduli by at least a factor of 2-3.

P. W. Morris; T. Shanks

1998-02-05T23:59:59.000Z

372

The Gemini NICI Planet-Finding Campaign: The Frequency of Planets around Young Moving Group Stars  

E-Print Network (OSTI)

We report results of a direct imaging survey for giant planets around 80 members of the Beta Pic, TW Hya, Tucana-Horologium, AB Dor, and Hercules-Lyra moving groups, observed as part of the Gemini NICI Planet-Finding Campaign. For this sample, we obtained median contrasts of \\Delta H=13.9 mag at 1" in combined CH4 narrowband ADI+SDI mode and median contrasts of \\Delta H=15.1 mag at 2" in H-band ADI mode. We found numerous (>70) candidate companions in our survey images. Some of these candidates were rejected as common-proper motion companions using archival data; we reobserved with NICI all other candidates that lay within 400 AU of the star and were not in dense stellar fields. The vast majority of candidate companions were confirmed as background objects from archival observations and/or dedicated NICI campaign followup. Four co-moving companions of brown dwarf or stellar mass were discovered in this moving group sample: PZ Tel B (36+-6 MJup, 16.4+-1.0 AU, Biller et al. 2010), CD -35 2722B (31+-8 MJup, 67+-...

Biller, Beth A; Wahhaj, Zahed; Nielsen, Eric L; Hayward, Thomas L; Males, Jared R; Skemer, Andrew; Close, Laird M; Chun, Mark; Ftaclas, Christ; Clarke, Fraser; Thatte, Niranjan; Shkolnik, Evgenya L; Reid, I Neill; Hartung, Markus; Boss, Alan; Lin, Douglas; Alencar, Silvia H P; Pino, Elisabete de Gouveia Dal; Gregorio-Hetem, Jane; Toomey, Douglas

2013-01-01T23:59:59.000Z

373

Stellar Populations in the Central 0.5 pc of the Galaxy I: A New Method for Constructing Luminosity Functions and Surface-Density Profiles  

E-Print Network (OSTI)

We present new high angular resolution near-infrared spectroscopic observations of the nuclear star cluster surrounding the Milky Way's central supermassive black hole. Using the integral-field spectrograph OSIRIS on Keck II behind the laser-guide-star adaptive optics system, this spectroscopic survey enables us to separate early-type (young, 4-6 Myr) and late-type (old, >1 Gyr) stars with a completeness of 50% down to K' = 15.5 mag, which corresponds to ~10 \\msun for the early-type stars. This work increases the radial extent of reported OSIRIS/Keck measurements by more than a factor of 3 from 4" to 14" (0.16 pc to 0.56 pc), along the projected disk of young stars. For our analysis, we implement a new method of completeness correction using a combination of star-planting simulations and Bayesian inference. We assign probabilities for the spectral type of every source detected in deep imaging down to K' = 15.5 mag using information from spectra, simulations, number counts, and the distribution of stars. The i...

Do, Tuan; Ghez, Andrea M; Morris, Mark R; Yelda, Sylvana; Martinez, Gregory D; Wright, Shelley A; Matthews, Keith

2013-01-01T23:59:59.000Z

374

FOUR NEW T DWARFS IDENTIFIED IN Pan-STARRS 1 COMMISSIONING DATA  

Science Conference Proceedings (OSTI)

A complete well-defined sample of ultracool dwarfs is one of the key science programs of the Pan-STARRS 1 optical survey telescope (PS1). Here we combine PS1 commissioning data with the Two Micron All Sky Survey (2MASS) to conduct a proper motion search (0.''1-2.''0 yr{sup -1}) for nearby T dwarfs, using optical+near-IR colors to select objects for spectroscopic follow-up. The addition of sensitive far-red optical imaging from PS1 enables discovery of nearby ultracool dwarfs that cannot be identified from 2MASS data alone. We have searched 3700 deg{sup 2} of PS1 y-band (0.95-1.03 {mu}m) data to y {approx} 19.5 mag (AB) and J {approx} 16.5 mag (Vega) and discovered four previously unknown bright T dwarfs. Three of the objects (with spectral types T1.5, T2, and T3.5) have photometric distances within 25 pc and were missed by previous 2MASS searches due to more restrictive color selection criteria. The fourth object (spectral type T4.5) is more distant than 25 pc and is only a single-band detection in 2MASS. We also examine the potential for completing the census of nearby ultracool objects with the PS1 3{pi} survey.

Deacon, Niall R.; Liu, Michael C.; Magnier, Eugene A.; Bowler, Brendan P.; Burgett, W. S.; Chambers, K. C.; Flewelling, H.; Kaiser, N.; Morgan, J. S.; Sweeney, W. E.; Tonry, J. L.; Wainscoat, R. J.; Waters, C. [Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822 (United States); Goldman, Bertrand [Max Planck Institute for Astronomy, Koenigstuhl 17, D-69117 Heidelberg (Germany); Redstone, Joshua A. [Facebook, 1601 S. California Avenue, Palo Alto, CA 94304 (United States); Lupton, R. H.; Price, P. A., E-mail: ndeacon@ifa.hawaii.edu [Princeton University Observatory, 4 Ivy Lane, Peyton Hall, Princeton University, Princeton, NJ 08544 (United States)

2011-09-15T23:59:59.000Z

375

CALTECH CORE-COLLAPSE PROJECT (CCCP) OBSERVATIONS OF TYPE IIn SUPERNOVAE: TYPICAL PROPERTIES AND IMPLICATIONS FOR THEIR PROGENITOR STARS  

SciTech Connect

Type IIn supernovae (SNe IIn) are rare events, constituting only a few percent of all core-collapse SNe, and the current sample of well-observed SNe IIn is small. Here, we study the four SNe IIn observed by the Caltech Core-Collapse Project (CCCP). The CCCP SN sample is unbiased to the extent that object selection was not influenced by target SN properties. Therefore, these events are representative of the observed population of SNe IIn. We find that a narrow P-Cygni profile in the hydrogen Balmer lines appears to be a ubiquitous feature of SNe IIn. Our light curves show a relatively long rise time (>20 days) followed by a slow decline stage (0.01-0.15 mag day{sup -1}), and a typical V-band peak magnitude of M{sub V} = -18.4 {+-} 1.0 mag. We measure the progenitor star wind velocities (600-1400 km s{sup -1}) for the SNe in our sample and derive pre-explosion mass-loss rates (0.026-0.12 M{sub Sun} yr{sup -1}). We compile similar data for SNe IIn from the literature and discuss our results in the context of this larger sample. Our results indicate that typical SNe IIn arise from progenitor stars that undergo luminous-blue-variable-like mass loss shortly before they explode.

Kiewe, Michael; Gal-Yam, Avishay; Arcavi, Iair [Benoziyo Center for Astrophysics, Faculty of Physics, Weizmann Institute of Science, Rehovot 76100 (Israel); Leonard, Douglas C.; Emilio Enriquez, J. [Department of Astronomy, San Diego State University, San Diego, CA 92182 (United States); Bradley Cenko, S. [Department of Astronomy, University of California, Berkeley, CA 94720-3411 (United States); Fox, Derek B. [Department of Astronomy and Astrophysics, 525 Davey Laboratory, Pennsylvania State University, University Park, PA 16802 (United States); Moon, Dae-Sik [Department of Astronomy and Astrophysics, University of Toronto, Toronto, ON M5S 3H4 (Canada); Sand, David J.; Soderberg, Alicia M., E-mail: avishay.gal-yam@weizmann.ac.il [Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138 (United States)

2012-01-01T23:59:59.000Z

376

The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. III. RR Lyrae Stars in the Large Magellanic Cloud  

E-Print Network (OSTI)

The third part of the OGLE-III Catalog of Variable Stars comprises 24906 RR Lyr stars in the Large Magellanic Cloud (LMC). This sample consist of 17693 fundamental-mode (RRab), 4958 first-overtone (RRc), 986 double-mode (RRd) and 1269 suspected second-overtone (RRe) pulsators. 66 objects are foreground Galactic RR Lyr stars. The catalog data include basic photometric and astrometric properties of the RR Lyr stars, multi-epoch VI photometry and finding charts. We detected one new RR Lyr star with additional eclipsing variations. The spatial distribution of RR Lyr stars in the LMC is distinctly non-spherical and it is elongated in the same direction as the LMC bar. The basic statistical features of RR Lyr stars in the LMC are provided. The apparent V-band magnitudes for RRab stars have the modal value at 19.36 mag, and for overtone RR Lyr stars it is about 19.32 mag. The mean periods for RRab, RRc and RRe stars are 0.576, 0.337 and 0.270 days, respectively.

Soszynski, I; Szymanski, M K; Kubiak, M; Pietrzynski, G; Wyrzykowski, L; Szewczyk, O; Ulaczyk, K; Poleski, R

2009-01-01T23:59:59.000Z

377

A New Census of the variable star population in the Globular Cluster NGC 2419  

E-Print Network (OSTI)

We present B, V and I CCD light curves for 101 variable stars belonging to the globular cluster NGC2419, 60 of which are new discoveries, based on datasets obtained at the TNG, SUBARU and HST telescopes. The sample includes 75 RR Lyrae stars (of which 38 RRab, 36 RRc and one RRd), one Population II Cepheid, 12 SX Phoenicis variables, 2 DeltaScuti stars, 3 binary systems, 5 long-period variables, and 3 variables of uncertain classification. The pulsation properties of the RR Lyrae variables are close to those of Oosterhoff type II clusters, consistent with the low metal abundance and the cluster horizontal branch morphology,disfavoring (but not totally ruling out) an extragalactic hypotesis for the origin of NGC2419. The observed properties of RR Lyrae and SX Phoenicis stars are used to estimate the cluster reddening and distance, using a number of different methods. Our final value is mo(NGC2419)=19.71+/-0.08mag (D= 87.5+/-3.3kpc), with E(B-V)=0.08+/-0.01mag, [Fe/H]=-2.1dex in the Zinn & West metallicity ...

Di Criscienzo, M; Ripepi, V; Clementini, G; Ora, M Dall'; Marconi, M; Musella, I; Federici, L; Di Fabrizio, L

2010-01-01T23:59:59.000Z

378

Variable stars in the ultra-faint dwarf spheroidal galaxy Ursa Major I  

E-Print Network (OSTI)

We have performed the first study of the variable star population of Ursa Major I (UMa I), an ultra-faint dwarf satellite recently discovered around the Milky Way by the Sloan Digital Sky Survey. Combining time series observations in the B and V bands from four different telescopes, we have identified seven RR Lyrae stars in UMa I, of which five are fundamental-mode (RRab) and two are first-overtone pulsators (RRc). Our V, B-V color-magnitude diagram of UMa I reaches V~23 mag (at a signal-to-noise ratio of ~ 6) and shows features typical of a single old stellar population. The mean pulsation period of the RRab stars = 0.628, {\\sigma} = 0.071 days (or = 0.599, {\\sigma} = 0.032 days, if V4, the longest period and brightest variable, is discarded) and the position on the period-amplitude diagram suggest an Oosterhoff-intermediate classification for the galaxy. The RR Lyrae stars trace the galaxy horizontal branch at an average apparent magnitude of = 20.43 +/- 0.02 mag (average on 6 stars and discarding V4), ...

Garofalo, Alessia; Clementini, Gisella; Ripepi, Vincenzo; Dall'Ora, Massimo; Moretti, Maria Ida; Coppola, Giuseppina; Musella, Ilaria; Marconi, Marcella

2013-01-01T23:59:59.000Z

379

The Optical Gravitational Lensing Experiment. The OGLE-III Catalog of Variable Stars. IX. RR Lyrae Stars in the Small Magellanic Cloud  

E-Print Network (OSTI)

The ninth part of the OGLE-III Catalog of Variable Stars (OIII-CVS) comprises RR Lyrae stars in the Small Magellanic Cloud (SMC). Our sample consists of 2475 variables, of which 1933 pulsate in the fundamental mode (RRab), 175 are the first overtone pulsators (RRc), 258 oscillate simultaneously in both modes (RRd) and 109 stars are suspected second-overtone pulsators (RRe). 30 objects are Galactic RR Lyr stars seen in the foreground of the SMC. We discuss some statistical features of the sample. Period distributions show distinct differences between SMC and LMC populations of RR Lyr variables, with the SMC stars having on average longer periods. The mean periods for RRab, RRc and RRe stars are 0.596, 0.366 and 0.293 days, respectively. The mean apparent magnitudes of RRab stars are equal to 19.70 mag in the V band and 19.12 mag in the I band. Spatial distribution of RR Lyr stars shows that the halo of the SMC is roughly round in the sky, however the density map reveals two maxima near the center of the SMC. F...

Soszynski, I; Szymanski, M K; Kubiak, M; Pietrzynski, G; Wyrzykowski, L; Ulaczyk, K; Poleski, R

2010-01-01T23:59:59.000Z

380

SCP06W54  

NLE Websites -- All DOE Office Websites (Extended Search)

4 4 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3397.00 , 2513.87) Gaussian fit RA,DEC ( 8:48:59.925 , +44:51:34.44) Cluster Offset 42.1 arcsec Redshift Unknown Redshift from Cluster Redshift 1.26 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, FAIL, PASS Classification Typing based on Discovery 1 ep = 05 (3397.00,2513.87) mag = 25.508 apsig = 6.971 Host Distance 3.851 arcsec ( 77.01 pixels) Host z850 23.46 Host i775 - z850 0.44 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


381

SCP06T52  

NLE Websites -- All DOE Office Websites (Extended Search)

2 2 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2753.28 , 4422.31) Gaussian fit RA,DEC (15:11:05.468 , + 9:04:28.96) Cluster Offset 84.0 arcsec Redshift Unknown Redshift from Cluster Redshift 0.97 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification cr* Typing based on Discovery 1 ep = 04 (2753.28,4422.31) mag = 24.910 apsig = 6.778 Host Distance 0.258 arcsec ( 5.16 pixels) Host z850 22.66 Host i775 - z850 0.55 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

382

SCP06W53  

NLE Websites -- All DOE Office Websites (Extended Search)

3 3 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (3727.56 , 2382.64) Gaussian fit RA,DEC ( 8:48:58.370 , +44:51:27.87) Cluster Offset 37.6 arcsec Redshift Unknown Redshift from Cluster Redshift 1.26 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification missub Typing based on Discovery 1 ep = 09 (3727.56,2382.64) mag = 23.139 apsig = 10.777 Host Distance 0.057 arcsec ( 1.15 pixels) Host z850 19.56 Host i775 - z850 0.18 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

383

SCP05Z52  

NLE Websites -- All DOE Office Websites (Extended Search)

Z52 Z52 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (1568.28 , 3454.70) Gaussian fit RA,DEC (22:35:26.340 , -25:57:05.82) Cluster Offset 65.5 arcsec Redshift Unknown Redshift from Cluster Redshift 1.39 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, FAIL Classification SN ? Typing based on Discovery 1 ep = 01 (1568.28,3454.70) mag = 25.629 apsig = 5.619 Host Distance 4.335 arcsec ( 86.70 pixels) Host z850 24.47 Host i775 - z850 0.04 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

384

SCP06R12  

NLE Websites -- All DOE Office Websites (Extended Search)

R12 "Jennie" R12 "Jennie" See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (4343.06 , 3215.02) Gaussian Fit (4343.01 , 3214.86) RA,DEC ( 2:23:00.083 , - 4:36:03.05) Cluster Offset 13.0 arcsec Redshift 1.212 Redshift from host Cluster Redshift 1.22 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification SN Ia Typing based on b,c Discovery 1 ep = 06 (4343.06,3215.02) mag = 24.311 apsig = 12.879 Host Distance 0.185 arcsec ( 3.71 pixels) Host z850 23.03 Host i775 - z850 0.95 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 )

385

SCP06K53  

NLE Websites -- All DOE Office Websites (Extended Search)

3 3 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (2970.68 , 4784.68) Gaussian fit RA,DEC (14:38:10.453 , +34:15:44.28) Cluster Offset 95.9 arcsec Redshift Unknown Redshift from Cluster Redshift 1.41 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, FAIL, PASS Classification Typing based on Discovery 1 ep = 03 (2970.68,4784.68) mag = 25.292 apsig = 5.456 Host Distance 1.972 arcsec ( 39.45 pixels) Host z850 23.69 Host i775 - z850 0.22 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

386

SCP06G50  

NLE Websites -- All DOE Office Websites (Extended Search)

0 0 See Barbary et al. (2011) for details. Aperture photometry on this page is for diagnostic purposes only. See Suzuki et al. (2011) for photometry and cosmology analysis. Data Lightcurve Local Environment : Stacked color image Pixel Position (5271.58 , 3166.01) Gaussian fit RA,DEC (14:29:10.384 , +34:37:30.39) Cluster Offset 110.5 arcsec Redshift Unknown Redshift from Cluster Redshift 1.26 Found with uniform selection Yes Lightcurve Cut 1, 2, 3 PASS, PASS, PASS Classification missub Typing based on Discovery 1 ep = 05 (5271.58,3166.01) mag = 23.871 apsig = 6.147 Host Distance 0.107 arcsec ( 2.15 pixels) Host z850 19.85 Host i775 - z850 0.35 Flux in a 3 pixel radius aperture, including host galaxy light. Hover-over shows: MAG_AUTO z850 ( aperture i775 - z850 ) z850 Thumbnail overview (see below for all thumbnails)

387

The Extremely Red Objects Found Thus Far in the Caltech Faint Galaxy Redshift Survey  

E-Print Network (OSTI)

We discuss the very red objects found in the first field of the Caltech Faint Galaxy Redshift Survey, for which the observations and analysis are now complete. In this field, which is 15 arcmin$^2$ and at J005325+1234 there are 195 objects with $K_s < 20$ mag, of which 84% have redshifts. The sample includes 24 spectroscopically confirmed Galactic stars, 136 galaxies, three AGNs, and 32 objects without redshifts. About 10% of the sample has $(R-K) \\ge 5$ mag. Four of these objects have redshifts, with $0.78 \\le z \\le 1.23$. Three of these are based on absorption features in the mid-UV, while the lowest redshift object shows the standard features near 4000\\AA. Many of the objects still without redshifts have been observed spectroscopically, and no emission lines were seen in their spectra. We believe they are galaxies with $z \\sim 1 - 1.5$ that are red due to their age and stellar content and not to some large amount of internal reddening from dust. Among the many other results from this survey of interest here is a determination of the median extinction in the mid-UV for objects with strong emission line spectra at $z \\sim 1 - 1.3$. The result is extinction by a factor of $\\sim$2 at 2400\\AA.

Judith G. Cohen; David W. Hogg; Roger Blandford; Michael A. Pahre; Patrick L. Shopbell

1998-08-30T23:59:59.000Z

388

Discovering anomaly mediated supersymmetry at the LHC.  

E-Print Network (OSTI)

, but with AMSB one of these particles is the LSP. Since R-parity is assumed to be conserved in our analysis (unlike e.g. [21,22]) the ?˜+1 may only decay into the ?˜01 so the small mass difference ?M1 ? m(?˜+1 )?m(?˜01) (1.2) means that the lightest chargino... of the mass difference ?M1 . The mAMSB Point d’Aix, despite being ruled out, still has a number of features which are of qualitative interest (fig. 2). The light gluino means that the decays g˜ ? t˜t¯ and b˜b¯ are no longer kinematically allowed. This means...

Barr, Alan; Lester, Christopher G; Parker, Michael A; Allanach, B C; Richardson, P

389

Discovering anomaly-mediated supersymmetry at the LHC  

E-Print Network (OSTI)

, but with AMSB one of these particles is the LSP. Since R-parity is assumed to be conserved in our analysis (unlike e.g. [21,22]) the ?˜+1 may only decay into the ?˜01 so the small mass difference ?M1 ? m(?˜+1 )?m(?˜01) (1.2) means that the lightest chargino... of the mass difference ?M1 . The mAMSB Point d’Aix, despite being ruled out, still has a number of features which are of qualitative interest (fig. 2). The light gluino means that the decays g˜ ? t˜t¯ and b˜b¯ are no longer kinematically allowed. This means...

Barr, Alan; Lester, Christopher G; Parker, Michael A; Allanach, B C; Richardson, P

390

Nuclear Material Transaction Report nrc741_1  

National Nuclear Security Administration (NNSA)

XXX XXX 000031 A M 1 1 1 1 COMPANY NAME COMPANY ADDRESS CITY, STATE ZIP CODE CONTACT COMPANY NAME COMPANY ADDRESS CITY, STATE ZIP CODE CONTACT 4 1 31 20 -1405.00 -93.00 2 32 50...

391

A Generalization of Euler's Theorem on Congruencies  

E-Print Network (OSTI)

We present a theorem which generalizes the classical Euler's theorem on congruencies: if $(a,m)=1$ then $a^ \\phi(m) \\equiv 1 (mod m)$ for the case when $a$ and $m$ are not relatively primes.

Florentin Smarandache

2006-10-20T23:59:59.000Z

392

ARPA TRP turboalternator development: Quarterly Report, July--September 1995. Revision 1  

DOE Green Energy (OSTI)

This report presents information on 4 major tasks: under-armor auxiliary power unit (UAAPU) demonstration on an M1A1 tank; low-cost turbogenerator design; negligible emission catalytic combustor development; and turbogenerator demonstration on an electric bus.

NONE

1995-10-01T23:59:59.000Z

393

Fermilab Today  

NLE Websites -- All DOE Office Websites (Extended Search)

Today | Archive | Classifieds Search GO Calendar Thurs., April 26 9:00 a.m. - 1:00 p.m. TESLA Technology Collaboration meeting 1 West View schedule here. 1:00 p.m. ALCPG ILC...

394

Straightforward Microwave Mixer Measuremens  

Science Conference Proceedings (OSTI)

... instead of strips tied to ground with arrays of vias, and the curve labeled “M1 ... 1 with the load method of [8] below 50 GHz. ... The solid curves in Fig. ...

2013-04-10T23:59:59.000Z

395

Role of microRNA?155 in dendritic cells and macrophages MiR?155 directly targets PU.1 and IL13R1.  

E-Print Network (OSTI)

??In search of genes differentially expressed between M1 (pro?Th1 or pro?inflammatory) and M2 (pro?Th2 or pro?tolerogenic) macrophages, BIC (microRNA 155 hosting gene) was found up… (more)

Martinez?Nunez, Rocio Teresa

2010-01-01T23:59:59.000Z

396

ARM - VAP Process - aerinf  

NLE Websites -- All DOE Office Websites (Extended Search)

Data ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 Contact(s) Timothy Shippert Developer (509) 375-5997 timothy.shippert...

397

ARM - Instrument - cpc  

NLE Websites -- All DOE Office Websites (Extended Search)

ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PVC S1 Browse Data Highland Center, Cape Cod MA; MAOS See Also Contact(s)...

398

ARM - Instrument - psap  

NLE Websites -- All DOE Office Websites (Extended Search)

ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PVC S1 Browse Data Highland Center, Cape Cod MA; MAOS SBS S2 Browse Data...

399

ARM - Instrument - wsacr  

NLE Websites -- All DOE Office Websites (Extended Search)

Facility, Lamont, OK ARM Mobile Facility PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 Contact(s) Nitin Bharadwaj (509) 372-4267 nitin@pnnl.gov Kevin Widener (509)...

400

ARM - Datastreams - aosclap3w  

NLE Websites -- All DOE Office Websites (Extended Search)

ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 Contact(s) Yin-Nan Lee (631) 344-3294 ynlee@bnl.gov Gunnar Senum (631)...

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


401

ARM - Datastreams - 915rwpprecipcon  

NLE Websites -- All DOE Office Websites (Extended Search)

Auxiliary) SGP S07 Browse Data Supplemental 7, Lamont, OK SGP S08 Browse Data Supplemental 8, Lamont, OK ARM Mobile Facility PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1...

402

ARM - Instrument - mfr  

NLE Websites -- All DOE Office Websites (Extended Search)

SGP C1 Browse Data Central Facility, Lamont, OK ARM Mobile Facility PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 Contact(s) Gary Hodges (303) 497-6460 Gary.Hodges@noaa...

403

ARM - Instrument - nephelometer  

NLE Websites -- All DOE Office Websites (Extended Search)

ARIES Observatory, Nainital, Uttarkhand, India PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1 PVC S1 Browse Data Highland Center, Cape Cod MA; MAOS SBS S2 Browse Data...

404

ARM - Datastreams - dlusr  

NLE Websites -- All DOE Office Websites (Extended Search)

timeoffset ( time ) Locations Southern Great Plains SGP C1 Browse Data Central Facility, Lamont, OK ARM Mobile Facility PVC M1 Browse Data Highland Center, Cape Cod MA; AMF 1...

405

Tobacco Control Policy Making in North Dakota: A Tradition of Activism  

E-Print Network (OSTI)

to Mobilize North Dakota Restaurants against Federal Smokingbuildings Sm oke-free restaurant C h. 3, article 12Langdon M1):13-20. 175. Fedor L. Restaurants, Bars May Have to Quit

Welle, Jennifer R MPH; Ibrahim, Jennifer K. Ph.D.; Glantz, Stanton A. Ph.D.

2004-01-01T23:59:59.000Z

406

Mixing and the Evolution of Cloud Droplet Size Spectra in a Vigorous Continental Cumulus  

Science Conference Proceedings (OSTI)

Aircraft measurements in a vigorous, highly turbulent continental cumulus show predominantly bimodal and multiple peaked cloud droplet spectral shapes. The data are 100 m (1 s) averages. Three factors involved in the development of the cloud ...

Ilga R. Paluch; Charles A. Knight

1984-06-01T23:59:59.000Z

407

Mathematica software for numerical simulation of hurricane ...  

Science Conference Proceedings (OSTI)

... The examples are also discussed in the present manual. 1. Installing the subroutines. 1.1. ... missileType 2, a 0.0026 m 1 (sch .40 pipe) ...

2012-01-06T23:59:59.000Z

408

A Semidefinite Optimization Approach to the Steady-State Analysis ...  

E-Print Network (OSTI)

show the potential of this approach in queueing analysis. Structure ...... were run by a PC with a Intel Pentium 4 - M 1.72GHz CPX, 256 MB of RAM and Microsoft.

409

B-469 Simplified Copositive and Lagrangian Relaxations for ...  

E-Print Network (OSTI)

The standard 0-1 mixed integer linear optimization problem ..... (j = 1,2,...,m ? 1) by ?, and that the last row of the equality constraint Au + b = 0 is of the form eT u ...

410

Section J  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

M-1 Section J Appendix M Key Design, Licensing and Site Management M&O Milestone Chart Activity Planned Date Develop and Submit CD-2 (25%-30%) 082009 Submission of Construction...

411

Fundamentals of Neutron Diffraction NCNR Summer School ...  

Science Conference Proceedings (OSTI)

... Page 35. 1 M 2 M Transfer Matrix 1 2 MMM = 1 M 2 M 3 M 1 2 3 M MMM = :historically, also is called the "optical" matrix. M Aside Page 36. j M ...

2006-08-09T23:59:59.000Z

412

Technology Validation  

NLE Websites -- All DOE Office Websites (Extended Search)

10M 1.8M * FY04 request: 13.1M 15M * Key research partners - Auto manufacturers, energy companies, hydrogen suppliers, fuel cell suppliers, universities, Air Products,...

413

Wireless LAN G001 Panasonic  

E-Print Network (OSTI)

HITACHI FLORA 270W Celeron 1.50GHz 768MB 80GB 15inch 3.1kg WinXP Pro - - G034 HITACHI Prius Pentium M 1

Katsumoto, Shingo

414

Pyruvate kinase M2-specific siRNA induces apoptosis and tumor regression  

E-Print Network (OSTI)

The development of cancer-specific therapeutics has been limited because most healthy cells and cancer cells depend on common pathways. Pyruvate kinase (PK) exists in M1 (PKM1) and M2 (PKM2) isoforms. PKM2, whose expression ...

Goldberg, Michael Solomon

415

It's Elemental - Isotopes of the Element Lawrencium  

NLE Websites -- All DOE Office Websites (Extended Search)

Electron Capture No Data Available 253 0.57 seconds Alpha Decay 98.70% Spontaneous Fission 1.30% 253m 1.49 seconds Alpha Decay 92.00% Spontaneous Fission 8.00% 254 18.4...

416

gxxx005-sumtab.dvi  

NLE Websites -- All DOE Office Websites (Extended Search)

20 Page 1 GAUGE AND HIGGS BOSONS GAUGE AND HIGGS BOSONS GAUGE AND HIGGS BOSONS GAUGE AND HIGGS BOSONS NODEGXXX005 I (J PC ) 0,1(1 - - ) NODES000 Mass m < 1 10...

417

Fisica Estadistica. Relacion 4 December 2, 2009  

E-Print Network (OSTI)

´ecula consiste en dos ´atomos de hidr´ogeno de masa m = 1.66·10-24 g cada uno, separados una distancia de r 10

Johnson, Samuel

418

Fisica Estadistica. Soluciones relacion 4  

E-Print Network (OSTI)

´ecula consiste en dos ´atomos de hidr´ogeno de masa m = 1.66·10-24 g cada uno, separados una distancia de r 10

Johnson, Samuel

419

Remote Spectroscopic Sounding of Liquid Water Path in Thick Clouds...  

NLE Websites -- All DOE Office Websites (Extended Search)

restored for this particular case. For sounding of the mixed clouds, three intervals in a spectrum of solar radiation are analyzed: 0.97-1.03 m; 1.60-1.70 m; and 2.15-2.35 m...

420

Interannual Variability of the Atlantic Hadley Circulation in Boreal Summer and Its Impacts on Tropical Cyclone Activity  

Science Conference Proceedings (OSTI)

A novel method was developed to define the regional Hadley circulation (HC) in terms of the meridional streamfunction. The interannual variability of the Atlantic HC in boreal summer was examined using the EOF analysis. The leading mode (M1), ...

Gan Zhang; Zhuo Wang

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


421

Microsoft Word - 2007_jgi_final.doc  

NLE Websites -- All DOE Office Websites (Extended Search)

M.O., K. Heguri, K. Hirata, and K. Miyamoto. 2005. Production of alternatives to fuel oil from organic waste by the alkane-producing bacterium, Vibrio furnissii M1. J. Appl....

422

Microsoft Word - Appendix M_ContingencyTrees.doc  

Office of Legacy Management (LM)

M Groundwater Operable Unit Contingency Trees U.S. Department of Energy Weldon Spring Site LTS&M Plan July 2005 Doc. No. S0079000 Page M-3 Figure M-1. Validation and Statistical...

423

Section 54  

NLE Websites -- All DOE Office Websites (Extended Search)

Integrations 8 0 Antenna Type Fixed beam Cassegrain feed Scanning, offset Cassegrain parabolic dish, vertically pointing parabolic dish Antenna Diameter 10 ft. or 2 m 1.2 m...

424

ROLE OF CONSTITUENT ELEMENTS IN PROPANE OXIDATION OVER MIXED METAL OXIDES.  

E-Print Network (OSTI)

??Recently discovered multi-component Mo-V-Te-Nb-O catalysts contain so-called “M1” and “M2” phases with orthorhombic and hexagonal structures, respectively, proposed to be active and selective in propane… (more)

BHANDARI, RISHABH

2005-01-01T23:59:59.000Z

425

LS-63 T. Khoe  

NLE Websites -- All DOE Office Websites (Extended Search)

in the form (2) where G so 21ff s 1 tan s 1 '" -:2' 2a 1 (ma) 2 2 - m +1 2 - 6 a 2 To calculate the frequency spread as a function of the oscillation amplitude, we...

426

The Classification of Some Perfect Codes  

Science Conference Proceedings (OSTI)

Perfect 1-error correcting codes C in Z2n, where n=2m?1, are considered. Let ?C? denote the linear span of the words of C and let the rank of C ... Keywords: perfect codes

Sergey V. Avgustinovich; Olof Heden; Faina I. Solov’eva

2004-03-01T23:59:59.000Z

427

Microsoft Word - Shashkov_LagHyd_PE.doc  

National Nuclear Security Administration (NNSA)

Loubre R., Shashkov M. 1 A Subcell Remapping Method on Staggered Polygonal Grids for Arbitrary-Lagrangian- Eulerian Methods R.Loubre, M.Shashkov * * T-7, MS B284, Los Alamos...

428

A Modular Algorithm for Computing Polynomial GCDs over ... - CECM  

E-Print Network (OSTI)

four types of primes. ? lc-bad primes. Let m1 .... because p | den(g). In this type of example p must divide the discriminant. ...... no non-local goto facility in Magma.

429

Energy-efficient threshold circuits computing mod functions  

Science Conference Proceedings (OSTI)

We prove that the modulus function MODm of n variables can be computed by a threshold circuit C of energy e and size s = O(e(n/m)1/(e?1)) for any integer e ? ...

Akira Suzuki, Kei Uchizawa, Xiao Zhou

2011-01-01T23:59:59.000Z

430

Michigan | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

June 8, 2010 Retooling Michigan: Tanks to Turbines A company that has manufactured geared systems for the M1 Abrams tank for more than 20 years is now part of the forces working...

431

Convergent relaxations of polynomial matrix inequalities and static ...  

E-Print Network (OSTI)

Nov 15, 2004 ... Results from the theory of moments are used to detect ...... 2) Example REA3: A model of a nuclear reactor with n = 12 states, m = 1 input and.

432

Geographical extrapolation of typical hourly weather data for energy calculation in buildings  

E-Print Network (OSTI)

FOR REAL 1951 YEARS PASSIVE HOUSES DAILY LOADS FOR REAL 1951Requirements for Real Year Passive Houses DAILY LOADS FORranch house of 112 m^ (1,200 ft^), a more massive passive

Arens, Edward A; Flynn, Larry E; Nall, Daniel N; Ruberg, Kalev

1980-01-01T23:59:59.000Z

433

GRB 050408: An Atypical Gamma-Ray Burst as a Probe of an Atypical Galactic Environment  

E-Print Network (OSTI)

The bright GRB 050408 was localized by HETE-II near local midnight, enabling an impressive ground-based followup effort as well as space-based followup from Swift. The Swift data from the X-Ray Telescope (XRT) and our own optical photometry and spectrum of the afterglow provide the cornerstone for our analysis. Under the traditional assumption that the visible waveband was above the peak synchrotron frequency and below the cooling frequency, the optical photometry from 0.03 to 5.03 days show an afterglow decay corresponding to an electron energy index of p_lc = 2.05 +/- 0.04, without a jet break as suggested by others. A break is seen in the X-ray data at early times (at ~12600 sec after the GRB). The spectral slope of the optical spectrum is consistent with p_lc assuming a host-galaxy extinction of A_V = 1.18 mag. The optical-NIR broadband spectrum is also consistent with p = 2.05, but prefers A_V = 0.57 mag. The X-ray afterglow shows a break at 1.26 x 10^4 sec, which may be the result of a refreshed shock. This burst stands out in that the optical and X-ray data suggest a large H I column density of N_HI ~ 10^22 cm^-2; it is very likely a damped Lyman alpha system and so the faintness of the host galaxy (M_V > -18 mag) is noteworthy. Moreover, we detect extraordinarily strong Ti II absorption lines with a column density through the GRB host that exceeds the largest values observed for the Milky Way by an order of magnitude. Furthermore, the Ti II equivalent width is in the top 1% of Mg II absorption-selected QSOs. This suggests that the large-scale environment of GRB 050408 has significantly lower Ti depletion than the Milky Way and a large velocity width (delta v > 200 km/s).

R. J. Foley; D. A. Perley; D. Pooley; J. X. Prochaska; J. S. Bloom; W. Li; B. Cobb; H. -W. Chen; G. Aldering; C. Bailyn; C. H. Blake; E. E. Falco; P. J. Green; M. P. Kowalski; S. Perlmutter; K. Roth; K. Volk

2005-12-04T23:59:59.000Z

434

AGES AND METALLICITIES OF CLUSTER GALAXIES IN A779 USING MODIFIED STROeMGREN PHOTOMETRY  

SciTech Connect

In the quest for the formation and evolution of galaxy clusters, Rakos and co-workers introduced a spectrophotometric method using modified Stroemgren photometry, but with the considerable debate toward the project's abilities, we re-introduce the system by testing for the repeatability of the modified Stroemgren colors and compare them with the Stroemgren colors, and check for the reproducibility of the ages and metallicities (using the Principle Component Analysis (PCA) technique and the GALEV models) for the six common galaxies in all three A779 data sets. As a result, a fair agreement between two filter systems was found to produce similar colors (with a precision of 0.09 mag in (uz - vz), 0.02 mag in (bz - yz), and 0.03 mag in (vz - vz)) and the generated ages and metallicities are also similar (with an uncertainty of 0.36 Gyr and 0.04 dex from PCA and 0.44 Gyr and 0.2 dex using the GALEV models). We infer that the technique is able to relieve the age-metallicity degeneracy by separating the age effects from the metallicity effects, but it is still unable to completely eliminate it. We further extend this paper to re-study the evolution of galaxies in the low mass, dynamically poor A779 cluster (as it was not elaborately analyzed by Rakos and co-workers in their previous work) by correlating the luminosity (mass), density, and radial distance with the estimated age, metallicity, and the star formation history. Our results distinctly show the bimodality of the young, low-mass, metal-poor population with a mean age of 6.7 Gyr ({+-} 0.5 Gyr) and the old, high-mass, metal-rich galaxies with a mean age of 9 Gyr ({+-} 0.5 Gyr). The method also observes the color evolution of the blue cluster galaxies to red (Butcher-Oemler phenomenon), and the downsizing phenomenon. Our analysis shows that modified Stroemgren photometry is very well suited for studying low- and intermediate-z clusters, as it is capable of observing deeper with better spatial resolution at spectroscopic redshift limits, and the narrowband filters estimate the age and metallicity with fewer uncertainties compared to other methods that study stellar population scenarios.

Sreedhar, Yuvraj Harsha; Rakos, Karl D.; Hensler, Gerhard; Zeilinger, Werner W. [University of Vienna, Institute of Astronomy, Tuerkenschanzstrasse 17, A-1180 Vienna (Austria); Odell, Andrew P. [Department of Physics and Astronomy, Northern Arizona University, Flagstaff, AZ (United States)

2012-03-01T23:59:59.000Z

435

Chy 475--Amar Two Body Problem Given below is the classical energy expression for two atoms interacting with each other  

E-Print Network (OSTI)

interacting with each other via a potential V(r) where r is the distance between the two particles,2 2 + vz,2 2 ] + V(r) but in vector notation we might write: E = 1 2 m1 r v1 2 + 1 2 m2 r v2 2 + V(r) We'll now define the center-of-mass coordinate vector and the interparticle vector: ! r R = m1 r r1

Amar, François G.

436

Chy 475--Amar--Spring 2013 Two Body Problem Given below is the classical energy expression for two atoms interacting with each other  

E-Print Network (OSTI)

atoms interacting with each other via a potential V(r) where r is the distance between the two particles 2 + vz,2 2 ] + V(r) but in vector notation we might write: E = 1 2 m1 v1 2 + 1 2 m2 v2 2 + V(r) We'll now define the center-of-mass coordinate vector and the interparticle vector: R = m1 r1 + m2 r2 M

Amar, François G.

437

Saami Ninne Composer: Karoor Devudu Iyer  

E-Print Network (OSTI)

Sisters, TM Krishna Arohanam: S R2 M1 P N2 S Avarohanam:S N2 P D N2 P M1 R2 G2 R2 S Pallavi : Saami Ninne chalamuseya mera kaadhura O lord ("saami")! I am waiting ("koriyunnanu") for you ("ninne"). P , ,- P, M R- G R | S N , -P N S R N | Sa - - mi - - ni - | nne - - ko - - - - | S , , , , ,- N S | R G R S R M P N || Ri

Kalyanaraman, Shivkumar

438

INDIAN INSTITUTE OF TECHNOLOGY DELHI  

E-Print Network (OSTI)

in the actinide 5f states P-wave pairing in metals Organized by: B. L. Gyorffy Room D J. F. Annett (Bristol) M1D1 Realistic gap models for superconducting Sr2RuO4 M. Eschrig (Karlsruhe) M1D2 P-wave pairing correlations magnetic-dipolar-mode quantum dots Eugene Kamenetskii S1X9 Anapole moments in MS-wave ferrite disks A

Kumar, M. Jagadesh

439

Experimental observation of left polarized wave absorption near electron cyclotron resonance frequency in helicon antenna produced plasma  

SciTech Connect

Asymmetry in density peaks on either side of an m = +1 half helical antenna is observed both in terms of peak position and its magnitude with respect to magnetic field variation in a linear helicon plasma device [Barada et al., Rev. Sci. Instrum. 83, 063501 (2012)]. The plasma is produced by powering the m = +1 half helical antenna with a 2.5 kW, 13.56 MHz radio frequency source. During low magnetic field (B < 100 G) operation, plasma density peaks are observed at critical magnetic fields on either side of the antenna. However, the density peaks occurred at different critical magnetic fields on both sides of antenna. Depending upon the direction of the magnetic field, in the m = +1 propagation side, the main density peak has been observed around 30 G of magnetic field. On this side, the density peak around 5 G corresponding to electron cyclotron resonance (ECR) is not very pronounced, whereas in the m = -1 propagation side, very pronounced ECR peak has been observed around 5 G. Another prominent density peak around 12 G has also been observed in m = -1 side. However, no peak has been observed around 30 G on this m = -1 side. This asymmetry in the results on both sides is explained on the basis of polarization reversal of left hand polarized waves to right hand polarized waves and vice versa in a bounded plasma system. The density peaking phenomena are likely to be caused by obliquely propagating helicon waves at the resonance cone boundary.

Barada, Kshitish K.; Chattopadhyay, P. K.; Ghosh, J.; Kumar, Sunil; Saxena, Y. C. [Institute for Plasma Research, Bhat, Gandhinagar 382428 (India)

2013-01-15T23:59:59.000Z

440

2010-0124-NScD-Dai-SC in chalcoginide[2][1]  

NLE Websites -- All DOE Office Websites (Extended Search)

Fig. 1. Magnetic structure Fig. 1. Magnetic structure of the (a) iron chalco- genide, and (b) iron pnic- tide systems, showing exchange couplings of the Heisenburg Hamiltonian. SNS shows novel spin waves in iron chalcogenide Fe 1.05 Te Measurements conducted at the Spallation Neutron Source at ORNL have determined exchange couplings in the mag- netically ordered chalcogenide Fe1.05Te, a nonsuperconducting member of the iron-based family of superconductors. The results show the exchange pairings thought to be related to superconductivity occur in a next-nearest-neighbor ordering of atoms, rather than in nearest-neighbor order as in a previously studied iron arsenide. Researchers from the University of Tennessee, ORNL, and other institutions collaborated to study the spin waves in Fe

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While these samples are representative of the content of NLEBeta,
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We encourage you to perform a real-time search of NLEBeta
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441

Mr. James Bearzi, Chief Hazardous Waste Bureau  

NLE Websites -- All DOE Office Websites (Extended Search)

8, 2010 8, 2010 New Mexico Environment Department 2905 E. Rodeo Park Dr. Bldg . 1 Santa Fe, New Mexico 87505-6303 Subject: Certification by a New Mexico Registered Professional Engineer in Support of TRUPACT-III References: United States Department Of Energy letter CBFO:OESH :GTB:MAG:11- 0702:UFC 5487.00 from Edward Ziemianski and M. F. Sharif to James Bearzi, dated January 10, 2011, subject: Notification of Planned Change to the Permitted Facility to Support TRUPACT-III United States Department Of Energy letter CBFO:ORC:GTB:MDA:10- 1623:UFC 5487.00 from David C. Moody and M. F. Sharif to James Bearzi, dated September 16, 2010, subject: Notification of Planned Change to the Permitted Facility to Support TRUPACT-III Dear Mr. Bearzi: The purpose of this letter is to transmit to your office a New Mexico registered

442

Definition: Ground Magnetics | Open Energy Information  

Open Energy Info (EERE)

Magnetics Magnetics Jump to: navigation, search Dictionary.png Ground Magnetics The surface magnetic method is the study of the distribution of magnetic minerals in the upper 20-30km of the earth's crust, recorded at an observation point on the earth's surface.[1][2] View on Wikipedia Wikipedia Definition A magnetometer, (pronounced mag-ne-TOM-e-ter), is a measuring instrument used to measure the strength and/or direction of the magnetic field, produced either in the laboratory or existing in nature. Some countries such as the USA, Canada and Australia classify the more sensitive magnetometers as military technology, and control their distribution. The International System of Units unit of measure for the strength of a magnetic field is the Tesla. This is a very large unit of magnetic field.

443

I-Cheng Tung  

NLE Websites -- All DOE Office Websites (Extended Search)

MM-Group Home MM-Group Home MMG Advisory Committees Beamlines 4-ID-C Soft Spectroscopy 4-ID-D Hard Spectroscopy 6-ID-B,C Mag. Scattering 6-ID-D HighE Scattering 29-ID IEX - ARPES,RSXS Getting Beamtime Sector Orientation Sector 4 Orientation Sector 6 Orientation Publications (4-ID) Publications (6-ID) Contact Us APS Ring Status Current APS Schedule I-Cheng Tung Argonne National Laboratory 9700 S. Cass Ave 432/B011 Argonne, Il 60439 Phone: 630-252-7048 Fax: 630-252-7392 E-Mail: ichengtung@u.northwestern.edu Education/Experience: Research Interests: Selected Publications: "Asymmetric Orbital-Lattice Interactions in Ultrathin Correlated Oxide Films," J.Chakhalian, J.M. Rondinelli, Jian Liu, B.A. Gray, M. Kareev, E.J. Moon, N. Prasai, J.L. Cohn, M. Varela, I.C. Tung, M.J. Bedzyk, S.G. Altendorf, F.

444

Jong-Woo Kim  

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MM-Group Home MM-Group Home MMG Advisory Committees Beamlines 4-ID-C Soft Spectroscopy 4-ID-D Hard Spectroscopy 6-ID-B,C Mag. Scattering 6-ID-D HighE Scattering 29-ID IEX - ARPES,RSXS Getting Beamtime Sector Orientation Sector 4 Orientation Sector 6 Orientation Publications (4-ID) Publications (6-ID) Contact Us APS Ring Status Current APS Schedule Jong-Woo Kim Argonne National Laboratory 9700 S. Cass Ave 432/B008 Argonne, Il 60439 Phone: 252-0248 Fax: 252-7392 E-Mail: jwkim@aps.anl.gov Education/Experience: 2007 - present: Assistant Physicist, Advanced Photon Source, Argonne National Lab. 2005-2007: Postdoctoral Research Associate, APS/μ-CAT, Ames Laboratory, Argonne, IL. Ph. D. Condensed Matter Physics; Iowa State University, Ames, IA; 2005 M.S. Physics; Yongsei University, Seoul, Korea; 2000

445

 

NLE Websites -- All DOE Office Websites (Extended Search)

Curve Modeling of Superluminous Supernovae Curve Modeling of Superluminous Supernovae Takashi Moriya (IPMU) Abstract: Recent SN surveys are discovering SNe with very high luminosity (brighter than -21 mag) and they are called superluminous SNe (SLSNe). At first, I will introduce SLSNe and their observational varieties. One idea to explain the huge luminosities is the collision of dense CSM and SN ejecta. If SN ejecta is surrounded by dense CSM, the kinetic energy of SN ejecta is efficiently converted to radiation energy, making them very bright. I will show our results of numerical modeling of such collisions and their light curves. From the light curve modeling, we obtain the properties of CSM and mass loss of the progenitors of SLSNe and some constraints on the progenitors. I also shortly introduce the transient survey planned for

446

Magwind LLC | Open Energy Information  

Open Energy Info (EERE)

Magwind LLC Magwind LLC Jump to: navigation, search Name Magwind LLC Place Texas Sector Wind energy Product Inventor of the Mag-Wind vertical axis wind turbine (VAWT) for building installations. The turbines are manufactured under contract at the facilities of Vector Systems, Inc. References Magwind LLC[1] LinkedIn Connections CrunchBase Profile No CrunchBase profile. Create one now! This article is a stub. You can help OpenEI by expanding it. Magwind LLC is a company located in Texas . References ↑ "Magwind LLC" Retrieved from "http://en.openei.org/w/index.php?title=Magwind_LLC&oldid=348589" Categories: Clean Energy Organizations Companies Organizations Stubs What links here Related changes Special pages Printable version Permanent link Browse properties

447

Los Alamos, New Mexico, July 21, 2009- Los Alamos National Laboratory scientists  

NLE Websites -- All DOE Office Websites (Extended Search)

snags five R&D 100 awards snags five R&D 100 awards July 21, 2009 "Oscars of Invention" recognize greatest innovations of 2009 Los Alamos, New Mexico, July 21, 2009- Los Alamos National Laboratory scientists won five of R&D Magazine's 2009 R&D 100 Awards. Recognized as the "Oscars of Invention" by the Chicago Tribune, these awards honor the top 100 proven technological advances of the past year. Winning Laboratory projects are MagViz, the SIMTECHE CO2 Capture Process, Lasonix, TeraOps Software Radio, and the Artificial Retina Project."The Department of Energy's national laboratories are incubators of innovation, and I'm proud they are being recognized once again for their remarkable work," said Energy Secretary Steven Chu. "The cutting-edge

448

Andreas Krassnigg  

NLE Websites -- All DOE Office Websites (Extended Search)

Current address: Institute for Theoretical Physics Current address: Institute for Theoretical Physics University of Zagreb Bijenicka c. 32, P.P. 331 HR-10002 Zagreb, Croatia phone: +385 (1) 4605586 fax: +385 (1) 4680336 e-mail: akrassnigg@oberon.phy.hr more detailed web page: http://physik.uni-graz.at/~ank/ Biographical sketch 1998 Mag.rer.nat., Karl-Franzens-Universität Graz, Austria 1998 Participant of CERN Summer Student Programme, Geneva, Switzerland 2002 Dr. rer. nat. (Ph.D.) sub auspiciis praesidentis rei publicae, Karl-Franzens-Universität Graz, Austria 2002 Awarded the Prize in appreciation of excellent studies for the best graduates of the academic year 2001/2002 of the Austrian federal ministry of education. 2002 Postdoc, Institut für Theoretische Physik, Karl-Franzens-Universität Graz, Austria

449

ARM - Evaluation Product - KAZR and MWACR Ship Motion Corrections  

NLE Websites -- All DOE Office Websites (Extended Search)

ProductsKAZR and MWACR Ship Motion Corrections ProductsKAZR and MWACR Ship Motion Corrections Comments? We would love to hear from you! Send us a note below or call us at 1-888-ARM-DATA. Send Evaluation Product : KAZR and MWACR Ship Motion Corrections 2012.09.22 - 2013.01.08 Site(s) MAG General Description The second ARM mobile facility has been configured to take advantage of ship-board deployments. At issue is how the motion at sea during these deployments affects the vertically-pointing cloud radars. Two radars of this type - the Ka-band ARM Zenith Radar (KAZR) and the Marine W-band ARM Cloud Radar (MWACR) - are instruments used in ARM's first ship-based field campaign. Each of these radars requires post-processing to account for the ship's motion across the open ocean. The primary adjustments that must be

450

News | U.S. DOE Office of Science (SC)  

Office of Science (SC) Website

News News News Featured Articles Science Headlines Presentations & Testimony News Archives Contact Information Office of Science U.S. Department of Energy 1000 Independence Ave., SW Washington, DC 20585 P: (202) 586-5430 Nano Mag Flux Lines BNL Color-enhanced image of magnetic flux lines around individual nickel nanodots. Brookhaven National Laboratory Print Text Size: A A A Subscribe FeedbackShare Page The Office of Science has several vehicles to update the public on the latest scientific outcomes of funded projects. The content is available as In the News articles, In Focus articles, and presentations and testimony. Featured Articles Brookhaven Lab scientists (from left) Kumudu Mudiyanselage, Ashleigh Baber, Fang Xu, and Dario Stacchiola. 01.08.14FROM THE LABS

451

Energy Blog | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

4, 2010 4, 2010 Sensible Solar Fueling Energy Revolution in Georgia Secretary Chu describes a second industrial revolution, building America's clean energy economy. May 14, 2010 Club's Chairman Leading by Example Why the Sierra Club Oregon Chairman is helping his organization live up to its legacy. May 14, 2010 PPG and MAG Team Up for Turbine Blade Research Two companies work together to move forward in the industry, researching materials and processes that could lead to stronger, more reliable wind blades. May 14, 2010 Carports with Solar Panels do Double Duty for Navy Since 2007, China Lake has been building carports that don't just deflect heat - they also absorb it and turn it into electricity using a series of photovoltaic solar panels lining the tops of the carports.

452

Doug Robinson  

NLE Websites -- All DOE Office Websites (Extended Search)

MM-Group Home MM-Group Home MMG Advisory Committees Beamlines 4-ID-C Soft Spectroscopy 4-ID-D Hard Spectroscopy 6-ID-B,C Mag. Scattering 6-ID-D HighE Scattering 29-ID IEX - ARPES,RSXS Getting Beamtime Sector Orientation Sector 4 Orientation Sector 6 Orientation Publications (4-ID) Publications (6-ID) Contact Us APS Ring Status Current APS Schedule Doug Robinson Argonne National Laboratory 9700 S. Cass Ave 432/B007 Argonne, Il 60439 Phone: 252-0247 Fax: 252-7392 E-Mail: drobinsn@aps.anl.gov Education/Experience: 2009 - present: Physicist, Argonne National Lab. 1997 -2009: Beamline Scientist, APS/μ-CAT, Ames Laboratory, Argonne, IL. 1988-1997: Staff Scientist, Microelectronics Research Center, Iowa State University, Ames, IA Ph.D. Condensed Matter Physics, University of Illinois, Urbana,

453

It's Elemental - The Element Magnesium  

NLE Websites -- All DOE Office Websites (Extended Search)

Sodium Sodium Previous Element (Sodium) The Periodic Table of Elements Next Element (Aluminum) Aluminum The Element Magnesium [Click for Isotope Data] 12 Mg Magnesium 24.3050 Atomic Number: 12 Atomic Weight: 24.3050 Melting Point: 923 K (650°C or 1202°F) Boiling Point: 1363 K (1090°C or 1994°F) Density: 1.74 grams per cubic centimeter Phase at Room Temperature: Solid Element Classification: Metal Period Number: 3 Group Number: 2 Group Name: Alkaline Earth Metal What's in a name? For Magnesia, a district in the region of Thessaly, Greece. Say what? Magnesium is pronounced as mag-NEE-zhi-em. History and Uses: Although it is the eighth most abundant element in the universe and the seventh most abundant element in the earth's crust, magnesium is never found free in nature. Magnesium was first isolated by Sir Humphry Davy, an

454

Energy Blog | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

4, 2010 4, 2010 PPG and MAG Team Up for Turbine Blade Research Two companies work together to move forward in the industry, researching materials and processes that could lead to stronger, more reliable wind blades. May 14, 2010 Carports with Solar Panels do Double Duty for Navy Since 2007, China Lake has been building carports that don't just deflect heat - they also absorb it and turn it into electricity using a series of photovoltaic solar panels lining the tops of the carports. May 14, 2010 The massive offshore oil spill in Santa Barbara in 1969 galvanized the environmental movement, locally and perhaps nationally. | Photo courtesy Bob Duncan Oil spill still motivates Santa Barbara to be green The massive offshore oil spill in Santa Barbara in 1969 galvanized the

455

New Beam Delivery System Optics: BDS9901 Peter Tenenbaum LCC-Note-0020  

NLE Websites -- All DOE Office Websites (Extended Search)

Beam Beam Delivery System Optics: BDS9901 Peter Tenenbaum LCC-Note-0020 14-July-1999 Abstract We describe in detail the optics and XSIF decks for the NLC Beam Delivery System in its present version, BDS9901. 1 Introduction In this Note, we describe the present optics design of the NLC Beam Delivery System, which has been somewhat revised for 1999. Most important optical changes include: * Organization of BPMs into quad-style (BPMQ), BPMs in feedback loops (BPMFB), BPMs which provide sub-train/multibunch information (BPMMB), and BPMs used to measure beam-beam deflections (BPMIP) * Addition of a number of small quad, skew-quad, sextupole, and skew-sextupole tuning mag- nets * Addition of actuators for the feedbacks * A 6-quadrupole final telescope, which allows all of the linear degrees of freedom to be opti- mized * Replacement of the low-energy final quads Q1A and Q1B with a single

456

Minnesota's 5th congressional district: Energy Resources | Open Energy  

Open Energy Info (EERE)

Policy Organizations in Minnesota's 5th congressional district Policy Organizations in Minnesota's 5th congressional district Windustry Registered Energy Companies in Minnesota's 5th congressional district Advanced Bioenergy LLC Best Buy Best Power International LLC Bison Renewable Energy LLC Clear Wind Renewable Power Delphi Financial Corporation Deltak LLC Despatch Industries EcoSystem Corporation Emerald Renewable Energy FC3 Group FreEner-g Freener g Genmar Holdings Inc Great Plains Institute Honor the Earth International Green Power IGP MagStar Technologies NRG Thermal LLC National Wind National Wind Assessments formerly Romuld Wind Consulting Natural Resource Group Navitas Energy Inc Project Resources Corporation Ryan Companies U.S. Sunnyside Technologies Inc Superior Process Technology Inc Target The Center for Energy and the Environment

457

11.05_haskel_ions.qxp  

NLE Websites -- All DOE Office Websites (Extended Search)

Western Western Hemisphere's most powerful x-rays at the APS, the researchers were able to see new details of rare-earth ions, a critical component of permanent magnets. This knowledge will enable manufacturers to manipulate the rare-earth ion atomic structure for optimization of future magnets. Modern permanent magnets-chief amongst them neodymium-iron-boron-exhibit a large and persistent magnetization after a magnetizing field is removed. This is largely due to the presence of rare-earth ions in their structure (Neodynium), which add magnetic stability by way of the interaction between their anisotropic atomic orbitals and surrounding charges on neighboring atoms. This in turn determines a preferred orientation of the mag- netic moments relative to the material's crys-

458

Sector 6 Research Highlights  

NLE Websites -- All DOE Office Websites (Extended Search)

MM-Group Home MM-Group Home MMG Advisory Committees Beamlines 4-ID-C Soft Spectroscopy 4-ID-D Hard Spectroscopy 6-ID-B,C Mag. Scattering 6-ID-D HighE Scattering 29-ID IEX - ARPES,RSXS Getting Beamtime Sector Orientation Sector 4 Orientation Sector 6 Orientation Publications (4-ID) Publications (6-ID) Contact Us APS Ring Status Current APS Schedule Highlights of research on Sector 6 Teasing Out the Nature of Structural Instabilities in Ceramic Compounds Teasing Out the Nature of Structural Instabilities in Ceramic Compounds March 12, 2013 Researchers have used beamlines 6-ID-B at the APS and XmAS at the ESRF to probe the structure of the rare-earth magnetic material europium titanate. In a magnetic field, the optical properties of this system change quite dramatically, presenting hope of a strong magneto-electric material for potential use in new memory, processing, and sensor devices.

459

1  

NLE Websites -- All DOE Office Websites (Extended Search)

Advance in bottle scanning could Advance in bottle scanning could enhance airport security and benefit passengers November 25, 2013 Video shows new MRI - X-ray technology at work LOS ALAMOS, N.M., Nov. 25, 2013-Los Alamos scientists have advanced a Magnetic Resonance Imaging (MRI) technology that may provide a breakthrough for screening liquids at airport security. They've added low-power X-ray data to the mix, and as a result have unlocked a new detection technology. Funded in part by the Department of Homeland Security's Science and Technology Directorate, the new system is named MagRay. The goal is to quickly and accurately distinguish between liquids that visually appear identical. For example, what appears to be a bottle of white wine could potentially - 2 - be nitromethane, a liquid that could be used to make an explosive. Both are clear

460

1  

NLE Websites -- All DOE Office Websites (Extended Search)

Security demo at Sunport October 13 Security demo at Sunport October 13 October 8, 2010 Prototype liquid scanning system demonstrated for media, public LOS ALAMOS, New Mexico, October 8, 2010-A potential next-generation liquid- and gel-scanning system for airport travelers will be demonstrated at the Albuquerque International Sunport for the public, media, and U.S. Department of Homeland Security officials on Wednesday, October 13 at 11:00 a.m. Los Alamos National Laboratory's MagViz (Magnetic Vision) Bottled Liquid Scanner (BLS) will be displayed, employing ultra-low-field nuclear magnetic resonance technology for the checkpoint detection of liquid explosives. Time: 11:00 a.m. Wednesday, October 13, 2010 Location: Press Room, ticketing level, then moving to security access portal, departure

Note: This page contains sample records for the topic "maldives mag m1" from the National Library of EnergyBeta (NLEBeta).
While these samples are representative of the content of NLEBeta,
they are not comprehensive nor are they the most current set.
We encourage you to perform a real-time search of NLEBeta
to obtain the most current and comprehensive results.


461

Jessica McChesney  

NLE Websites -- All DOE Office Websites (Extended Search)

MM-Group Home MM-Group Home MMG Advisory Committees Beamlines 4-ID-C Soft Spectroscopy 4-ID-D Hard Spectroscopy 6-ID-B,C Mag. Scattering 6-ID-D HighE Scattering 29-ID IEX - ARPES,RSXS Getting Beamtime Sector Orientation Sector 4 Orientation Sector 6 Orientation Publications (4-ID) Publications (6-ID) Contact Us APS Ring Status Current APS Schedule Jessica McChesney Argonne National Laboratory 9700 S. Cass Ave 437/D003 Argonne, IL 60439 Phone: 252-7107 Fax: 252-7392 E-Mail: jmcchesn@aps.anl.gov Education/Experience: 2011 - present: Assistant Physicist, X-ray Science Division, Argonne National Laboratory. 2013 - present: Adjunct Assistant Professor, EECS, Northwestern University. 2007-2008: Postdoctoral Research Scholar, Advanced Light Source, Lawrence Berkeley National Laboratory and Fritz Haber Institute - Max

462

Recovery Act | Department of Energy  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

May 14, 2010 May 14, 2010 PPG and MAG Team Up for Turbine Blade Research Two companies work together to move forward in the industry, researching materials and processes that could lead to stronger, more reliable wind blades. May 14, 2010 Energy Corps Takes Root in Montana, Seeks to Make America Greener For the last 17 years, AmeriCorps members have pledged to uphold their duties as public servants, vowing to "get things done for America-to make our people safer, smarter and healthier." But a new type of volunteering in Montana is adding one more thing to that list: making America greener. May 14, 2010 Recovery Act Funding Hundreds of Jobs in California Solar Power, Inc. of Roseville, Calif., does almost everything in solar photovoltaics - from manufacturing and testing to home solar panel

463

Document  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

37 Federal Register 37 Federal Register / Vol. 73, No. 96 / Friday, May 16, 2008 / Notices DATE AND TIME: Tuesday, May 20, 2008, 4 p.m.-5:30 p.m. PLACE : Corporation for National and Community Service; 8th Floor; 1201 New York Avenue, NW., Washington, DC 20525. STATUS: Open. MATTERS TO BE CONSIDERED: I. Chair's Opening Comments II. Consideration of Previous Meetings Minutes III. CEO Report IV. Committee Reports * MAG Committee * Program Committee * Strategic Partnerships Committee V. Impact of AmeriCorps Week and the Longitudinal Study Presentation by Millicent Williams, Executive Director, Serve DC and Sally Prouty, President and CEO of The Corps Network VI. Public Comments Accomodations: Anyone who needs an interpreter or other accommodation should notify the Corporation's contact

464

A Candidate Substellar Companion to CoD -33 7795 (TWA 5)  

E-Print Network (OSTI)

We present the discovery of a candidate substellar object in a survey of young stars in the solar vicinity using the sensitivity and spatial resolution afforded by the NICMOS coronagraph on the Hubble Space Telescope. The H=12.1 mag object was discovered approximately 2 arcsec from the TW Hydrae Association member CoD -33 7795 (TWA 5), and the photometry implies a spectral type M8-M8.5, with a temperature of approximately 2600K. We estimate that the probability of a chance alignment with a background objectof this nature is < 2 X 10^(-5), and therefore postulate the object (TWA 5B) is physically associated at a projected separation of 100 AU. Given the likely youth of the primary (~ 10 Myr), current brown dwarf cooling models predict a mass of approximately 20 Jupiter masses for TWA 5B.

Lowrance, P J; Becklin, E E; Zuckerman, B; Schneider, G; Webb, R A; Hines, D C; Kirkpatrick, J D; Körner, D W; Low, F; Meier, R; Rieke, M J; Smith, B A; Terrile, R J; Thompson, R I

1999-01-01T23:59:59.000Z

465

A Candidate Substellar Companion to CoD -33 7795 (TWA 5)  

E-Print Network (OSTI)

We present the discovery of a candidate substellar object in a survey of young stars in the solar vicinity using the sensitivity and spatial resolution afforded by the NICMOS coronagraph on the Hubble Space Telescope. The H=12.1 mag object was discovered approximately 2 arcsec from the TW Hydrae Association member CoD -33 7795 (TWA 5), and the photometry implies a spectral type M8-M8.5, with a temperature of approximately 2600K. We estimate that the probability of a chance alignment with a background objectof this nature is < 2 X 10^(-5), and therefore postulate the object (TWA 5B) is physically associated at a projected separation of 100 AU. Given the likely youth of the primary (~ 10 Myr), current brown dwarf cooling models predict a mass of approximately 20 Jupiter masses for TWA 5B.

P. J. Lowrance; C. McCarthy; E. E. Becklin; B. Zuckerman; G. Schneider; R. A. Webb; D. C. Hines; J. D. Kirkpatrick; D. W. Koerner; F. Low; R. Meier; M. Rieke; B. A. Smith; R. J. Terrile; R. I. Thompson

1998-12-09T23:59:59.000Z

466

High-latitude F supergiant IRAS 18095 + 2704 - a proto-planetary nebula  

Science Conference Proceedings (OSTI)

The paper reports the discovery of a new high-latitude F supergiant, IRAS 18095 + 2704, which shows a large excess in the far-infrared. Ground-based observations have identified it as a V = 10.4 mag F3 Ib star which displays light and velocity variability. Comparison with the post-asymptotic giant branch (AGB) evolution model of Volk and Kwok suggests that it is an excellent candidate for a protoplanetary nebula. Model fitting of the spectrum of 18095 + 2704 from 0.35 to 100 microns suggests that it evolved from the AGB approximately 265 yr ago and had a mass-loss rate of 0.00003 solar mass/yr at the end of the AGB. 31 references.

Hrivnak, B.J.; Kwok, S.; Volk, K.M.

1988-08-01T23:59:59.000Z

467

Radio maps around five spiral and peculiar galaxies  

SciTech Connect

Areas of from 1 to 2 degrees square around five spiral and peculiar galaxies of apparent brightness between 10.3 and 12.7 mag have been mapped at a wavelength of 13 cm. In this small sample of observations it is found thai, on the average, about two, counting the galaxy itself, radio sources of flux strength between 0.1 and 0.4 f.u. are physically associated with each spiral. This result supports the conclusion of De Jong that satellite radio sources are associated with spiral galaxies. If these preliminary results are indicative, then the radio sources associated with spiral galaxies differ from three classically associated with elliptical galaxies by being (1) intrinsically weaker and (2) not as accurately aligned as pairs across the central galaxy. (auth)

Arp, H.

1973-08-01T23:59:59.000Z

468

Occultations of HIP and UCAC2 stars downto 15m by large TNO in 2004-2014  

E-Print Network (OSTI)

Occultations of stars brighter than 15m by largest TNOs are predicted. Search was performed using the following catalogues: Hipparcos; Tycho2 with coordinates of 2838666 stars taken from UCAC2 (Herald, 2003); UCAC2 (Zacharias et al., 2003) with 16356096 stars between 12.00 and 14.99 mag to the north from -45 declination. Predictions were made for 17 largest numbered transneptunian asteroids, recently discovered 2004 DW and 4 known binary Kuiper Belt objects. 64 events occuring at solar elongation of 30 deg and more are selected, including exceptionally rare occultation of 6.5m star by double (66652) 1999 RZ253 on 2007 October 4th. Observations of these events by all available means are extremely important since they can provide unique information about the size of TNOs and improve their orbits dramatically.

Denis Denissenko

2004-02-28T23:59:59.000Z

469

The 1998 November 14 Occultation of GSC 0622-00345 by Saturn. I. Techniques for Ground-Based Stellar Occultations  

E-Print Network (OSTI)

On 1998 November 14, Saturn and its rings occulted the star GSC 0622-00345. We observed atmospheric immersion with NSFCAM at the National Aeronautics and Space Administration's Infrared Telescope Facility on Mauna Kea, Hawaii. Immersion occurred at 55.5\\circ S planetocentric latitude. A 2.3 {\\mu}m, methane-band filter suppressed reflected sunlight. Atmospheric emersion and ring data were not successfully obtained. We describe our observation, light-curve production, and timing techniques, including improvements in aperture positioning, removal of telluric scintillation effects, and timing. Many of these techniques are known within the occultation community, but have not been described in the reviewed literature. We present a light curve whose signal-to-noise ratio per scale height is 267, among the best ground-based signals yet achieved, despite a disadvantage of up to 8 mag in the stellar flux compared to prior work.

Harrington, Joseph; 10.1088/0004-637X/716/1/398

2010-01-01T23:59:59.000Z

470

A DOZEN NEW GALAXIES CAUGHT IN THE ACT: GAS STRIPPING AND EXTENDED EMISSION LINE REGIONS IN THE COMA CLUSTER  

Science Conference Proceedings (OSTI)

We present images of extended H{alpha} clouds associated with 14 member galaxies in the Coma cluster obtained from deep narrowband imaging observations with the Suprime-Cam at the Subaru Telescope. The parent galaxies of the extended H{alpha} clouds are distributed farther than 0.2 Mpc from the peak of the X-ray emission of the cluster. Most of the galaxies are bluer than g - r {approx} 0.5 and they account for 57% of the blue (g - r < 0.5) bright (r < 17.8 mag) galaxies in the central region of the Coma cluster. They reside near the red- and blueshifted edges of the radial velocity distribution of Coma cluster member galaxies. Our findings suggest that most of the parent galaxies were recently captured by the Coma cluster potential and are now infalling toward the cluster center with their disk gas being stripped off and producing the observed H{alpha} clouds.

Yagi, Masafumi; Komiyama, Yutaka; Kashikawa, Nobunari [Optical and Infrared Astronomy Division, National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo 181-8588 (Japan); Yoshida, Michitoshi [Hiroshima Astrophysical Science Center, Hiroshima University, 1-3-1, Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526 (Japan); Furusawa, Hisanori [Astronomy Data Center, National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo 181-8588 (Japan); Okamura, Sadanori [Department of Astronomy, School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033 (Japan); Graham, Alister W. [Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, Victoria 3122 (Australia); Miller, Neal A. [Department of Astronomy, University of Maryland, College Park, MD 20742-2421 (United States); Carter, David [Astronomical Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Warf, Birkenhead CH41 1LD (United Kingdom); Mobasher, Bahram [Department of Physics and Astronomy, University of California, Riverside, CA 92521 (United States); Jogee, Shardha, E-mail: YAGI.Masafumi@nao.ac.j [Department of Astronomy, University of Texas at Austin, 1 University Station C1400, Austin, TX 78712 (United States)

2010-12-15T23:59:59.000Z

471

ABSOLUTE PROPERTIES OF THE ECLIPSING BINARY STAR V335 SERPENTIS  

SciTech Connect

V335 Ser is now known to be an eccentric double-lined A1+A3 binary star with fairly deep (0.5 mag) partial eclipses. Previous studies of the system are improved with 7456 differential photometric observations from the URSA WebScope and 5666 from the NFO WebScope, and 67 high-resolution spectroscopic observations from the Tennessee State University 2 m automatic spectroscopic telescope. From dates of minima, the apsidal period is about 880 years. Accurate (better than 2%) masses and radii are determined from analysis of the two new light curves and the radial velocity curve. Theoretical models match the absolute properties of the stars at an age of about 380 Myr, though the age agreement for the two components is poor. Tidal theory correctly confirms that the orbit should still be eccentric, but we find that standard tidal theory is unable to match the observed asynchronous rotation rates of the components' surface layers.

Lacy, Claud H. Sandberg [Physics Department, University of Arkansas, Fayetteville, AR 72701 (United States); Fekel, Francis C. [Center of Excellence in Information Systems, Tennessee State University, Nashville, TN 37209 (United States); Claret, Antonio, E-mail: clacy@uark.edu, E-mail: fekel@evans.tsuniv.edu, E-mail: claret@iaa.es [Instituto de Astrofisica de Andalucia, CSIC, Apdo. Postal 3004, E-18080 Granada (Spain)

2012-08-15T23:59:59.000Z

472

DISCOVERY OF A WOLF-RAYET STAR THROUGH DETECTION OF ITS PHOTOMETRIC VARIABILITY  

SciTech Connect

We report the serendipitous discovery of a heavily reddened Wolf-Rayet star that we name WR 142b. While photometrically monitoring a cataclysmic variable, we detected weak variability in a nearby field star. Low-resolution spectroscopy revealed a strong emission line at 7100 A, suggesting an unusual object and prompting further study. A spectrum taken with the Hobby-Eberly Telescope confirms strong He II emission and an N IV 7112 A line consistent with a nitrogen-rich Wolf-Rayet star of spectral class WN6. Analysis of the He II line strengths reveals no detectable hydrogen in WR 142b. A blue-sensitive spectrum obtained with the Large Binocular Telescope shows no evidence for a hot companion star. The continuum shape and emission line ratios imply a reddening of E(B - V) = 2.2-2.6 mag. We estimate that the distance to WR 142b is 1.4 {+-} 0.3 kpc.

Littlefield, Colin [Law School, University of Notre Dame, Notre Dame, IN 46556 (United States); Garnavich, Peter; McClelland, Colin; Rettig, Terrence [Physics Department, University of Notre Dame, Notre Dame, IN 46556 (United States); Marion, G. H. [Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138 (United States); Vinko, Jozsef [Department of Optics, University of Szeged (Hungary); Wheeler, J. Craig [Astronomy Department, University of Texas, Austin, TX 78712 (United States)

2012-06-15T23:59:59.000Z

473

The orbital and superhump periods of the deeply eclipsing dwarf nova PU UMa  

E-Print Network (OSTI)

We report unfiltered photometry during superoutbursts of PU UMa in 2009 and 2012. The amplitude was 4.5 magnitudes above mean quiescence and lasted at least 9 to 10 days. Superhumps were present with a peak-to-peak amplitude of up to ~0.3 mag, thereby confirming it to be a member of the SU UMa family of dwarf novae. The mean superhump period during the later part of the 2012 outburst was Psh = 0.08076(40) d. Analysis of the eclipse times of minimum, supplemented with data from other researchers, revealed an orbital period of Porb = 0.077880551(17) d. The superhump period excess was epsilon = 0.037(5). During the 2012 outburst, which was the better observed of the two, the FWHM eclipse duration gradually declined from 9.5 to 5 min. The eclipse depth was up to 1.7 magnitudes.

Shears, Jeremy; Littlefield, Colin; Miller, Ian; Morelle, Etienne; Pickard, Roger; Pietz, Jochen; Sabo, Richard

2012-01-01T23:59:59.000Z

474

A 500 PARSEC HALO SURROUNDING THE GALACTIC GLOBULAR NGC 1851  

SciTech Connect

Using imaging that shows 4 mag of main-sequence stars, we have discovered that the Galactic globular cluster NGC 1851 is surrounded by a halo that is visible from the tidal radius of 700 arcsec (41 pc) to more than 4500 arcsec (>250 pc). This halo is symmetric and falls in density as a power law of r {sup -1.24}. It contains approximately 0.1% of the dynamical mass of NGC 1851. There is no evidence for tidal tails. Current models of globular cluster evolution do not explain this feature, although simulations of tidal influences on dwarf spheroidal galaxies qualitatively mimic these results. Given the state of published models, it is not possible to decide between creation of this halo from either isolated cluster evaporation or from tidal or disk shocking, or from destruction of a dwarf galaxy in which this object may have once been embedded.

Olszewski, Edward W. [Steward Observatory, University of Arizona, Tucson, AZ (United States); Saha, Abhijit; Knezek, Patricia [National Optical Astronomy Observatory, Tucson, AZ (United States); Subramaniam, Annapurni [Indian Institute of Astrophysics, Bangalore (India); De Boer, Thomas [Kapteyn Astronomical Institute, University of Groningen (Netherlands); Seitzer, Patrick [Department of Astronomy, University of Michigan, Ann Arbor, MI (United States)], E-mail: eolszewski@as.arizona.edu

2009-12-15T23:59:59.000Z

475

Integration of MHD load models with circuit representations the Z generator.  

SciTech Connect

MHD models of imploding loads fielded on the Z accelerator are typically driven by reduced or simplified circuit representations of the generator. The performance of many of the imploding loads is critically dependent on the current and power delivered to them, so may be strongly influenced by the generators response to their implosion. Current losses diagnosed in the transmission lines approaching the load are further known to limit the energy delivery, while exhibiting some load dependence. Through comparing the convolute performance of a wide variety of short pulse Z loads we parameterize a convolute loss resistance applicable between different experiments. We incorporate this, and other current loss terms into a transmission line representation of the Z vacuum section. We then apply this model to study the current delivery to a wide variety of wire array and MagLif style liner loads.

Jennings, Christopher A.; Ampleford, David J.; Jones, Brent Manley; McBride, Ryan D.; Bailey, James E.; Jones, Michael C.; Gomez, Matthew Robert.; Cuneo, Michael Edward; Nakhleh, Charles; Stygar, William A.; Savage, Mark Edward; Wagoner, Timothy C.; Moore, James K.

2013-03-01T23:59:59.000Z

476

All Sky Cameras for the characterization of the Cherenkov Telescope Array candidate sites  

E-Print Network (OSTI)

The All Sky Camera (ASC) was developed as a universal device for the monitoring of the night sky quality. Eight ASCs are already installed and measure night sky parameters at eight of the candidate sites of the Cherenkov Telescope Array (CTA) gamma-ray observatory. The ACS system consists of an astronomical CCD camera, a fish eye lens, a control computer and associated electronics. The measurement is carried out during astronomical night. The images are automatically taken every 5 minutes and automatically processed using the control computer of the device. The analysis results are the cloud fraction (the percentage of the sky covered by clouds) and night sky brightness (in mag/arcsec$^{2}$)

Mandát, Dušan; Ebr, Jan; Hrabovský, Miroslav; Prouza, Michael; Bulik, Tomasz; Allekotte, Ingomar

2013-01-01T23:59:59.000Z

477

Andromeda X, A New Dwarf Spheroidal Satellite of M31: Photometry  

E-Print Network (OSTI)

We report the discovery of Andromeda X, a new dwarf spheroidal satellite of M31, based on stellar photometry from the Sloan Digital Sky Survey (SDSS). Using follow-up imaging data we have estimated its distance and other physical properties. We find that Andromeda X has a dereddened central surface brightness of mu_V,0 ~ 26.7 mag arcsec^-2 and a total apparent magnitude of V_tot ~ 16.1, which at the derived distance modulus, (m - M)_0 ~ 24.12 - 24.34, yields an absolute magnitude of M_V ~ -8.1 +/- 0.5; these values are quite comparable to those of Andromeda IX, a previously-discovered low luminosity M31 satellite. The discoveries of Andromeda IX and Andromeda X suggest that such extremely faint satellites may be plentiful in the Local Group.

Daniel B. Zucker; Alexei Y. Kniazev; David Martinez-Delgado; Eric F. Bell; Hans-Walter Rix; Eva K. Grebel; Jon A. Holtzman; Rene A. M. Walterbos; Constance M. Rockosi; Donald G. York; J. C. Barentine; Howard Brewington; J. Brinkmann; Michael Harvanek; S. J. Kleinman; Jurek Krzesinski; Dan Long; Eric H. Neilsen, Jr.; Atsuko Nitta; Stephanie A. Snedden

2006-01-26T23:59:59.000Z

478

Andromeda IX: A New Dwarf Spheroidal Satellite of M31  

E-Print Network (OSTI)

We report the discovery of a new dwarf spheroidal satellite of M31, Andromeda IX, based on resolved stellar photometry from the Sloan Digital Sky Survey (SDSS). Using both SDSS and public archival data we have estimated its distance and other physical properties, and compared these to the properties of a previously known dwarf spheroidal companion, Andromeda V, also observed by SDSS. Andromeda IX is the lowest surface brightness galaxy found to date (mu_{V} ~ 26.8 mag arcsec^-2), and at the distance we estimate from the position of the tip of Andromeda IX's red giant branch, (m - M)_{0} ~ 24.5 (805 kpc), Andromeda IX would also be the faintest galaxy known (M_{V} ~ -8.3).

Daniel B. Zucker; Alexei Y. Kniazev; Eric F. Bell; David Martinez-Delgado; Eva K. Grebel; Hans-Walter Rix; Constance M. Rockosi; Jon A. Holtzman; Rene A. M. Walterbos; James Annis; Donald G. York; Zeljko Ivezic; J. Brinkmann; Howard Brewington; Michael Harvanek; Greg Hennessy; S. J. Kleinman; Jurek Krzesinski; Dan Long; Peter R. Newman; Atsuko Nitta; Stephanie A. Snedden

2004-04-14T23:59:59.000Z

479

Andromeda X, A New Dwarf Spheroidal Satellite of M31: Photometry  

E-Print Network (OSTI)

We report the discovery of Andromeda X, a new dwarf spheroidal satellite of M31, based on stellar photometry from the Sloan Digital Sky Survey (SDSS). Using follow-up imaging data we have estimated its distance and other physical properties. We find that Andromeda X has a dereddened central surface brightness of mu_V,0 ~ 26.7 mag arcsec^-2 and a total apparent magnitude of V_tot ~ 16.1, which at the derived distance modulus, (m - M)_0 ~ 24.12 - 24.34, yields an absolute magnitude of M_V ~ -8.1 +/- 0.5; these values are quite comparable to those of Andromeda IX, a previously-discovered low luminosity M31 satellite. The discoveries of Andromeda IX and Andromeda X suggest that such extremely faint satellites may be plentiful in the Local Group.

Zucker, D B; Martínez-Delgado, D; Bell, E F; Rix, H W; Grebel, E K; Holtzman, J A; Walterbos, R A M; Rockosi, C M; York, D G; Barentine, J C; Brewington, H; Brinkmann, J; Harvanek, M; Kleinman, S J; Krzesínski, J; Long, D; Neilsen, E H; Nitta, A; Snedden, S A; Zucker, Daniel B.; Kniazev, Alexei Y.; Martinez-Delgado, David; Bell, Eric F.; Rix, Hans-Walter; Grebel, Eva K.; Holtzman, Jon A.; Walterbos, Rene A. M.; Rockosi, Constance M.; York, Donald G.; Brewington, Howard; Harvanek, Michael; Krzesinski, Jurek; Long, Dan; Neilsen, Eric H.; Nitta, Atsuko; Snedden, Stephanie A.

2006-01-01T23:59:59.000Z

480

Andromeda IX: A New Dwarf Spheroidal Satellite of M31  

E-Print Network (OSTI)

We report the discovery of a new dwarf spheroidal satellite of M31, Andromeda IX, based on resolved stellar photometry from the Sloan Digital Sky Survey (SDSS). Using both SDSS and public archival data we have estimated its distance and other physical properties, and compared these to the properties of a previously known dwarf spheroidal companion, Andromeda V, also observed by SDSS. Andromeda IX is the lowest surface brightness galaxy found to date (mu_{V} ~ 26.8 mag arcsec^-2), and at the distance we estimate from the position of the tip of Andromeda IX's red giant branch, (m - M)_{0} ~ 24.5 (805 kpc), Andromeda IX would also be the faintest galaxy known (M_{V} ~ -8.3).

Zucker, D B; Bell, E F; Martínez-Delgado, D; Grebel, E K; Rix, H W; Rockosi, C M; Holtzman, J A; Walterbos, R A M; Annis, J; York, D G; Ivezic, Z; Brinkmann, J; Brewington, H; Harvanek, M; Hennessy, G; Kleinman, S J; Krzesínski, J; Long, D; Newman, P R; Nitta, A; Snedden, S A; Zucker, Daniel B.; Kniazev, Alexei Y.; Bell, Eric F.; Martinez-Delgado, David; Grebel, Eva K.; Rix, Hans-Walter; Rockosi, Constance M.; Holtzman, Jon A.; Walterbos, Rene A. M.; Annis, James; York, Donald G.; Ivezic, Zeljko; Brewington, Howard; Harvanek, Michael; Hennessy, Greg; Krzesinski, Jurek; Long, Dan; Newman, Peter R.; Nitta, Atsuko; Snedden, Stephanie A.

2004-01-01T23:59:59.000Z

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481

A New Milky Way Dwarf Satellite in Canes Venatici  

E-Print Network (OSTI)

In this Letter, we announce the discovery of a new dwarf satellite of the Milky Way, located in the constellation Canes Venatici. It was found as a stellar overdensity in the North Galactic Cap using Sloan Digital Sky Survey Data Release 5 (SDSS DR5). The satellite's color-magnitude diagram shows a well-defined red giant branch, as well as a horizontal branch. As judged from the tip of the red giant branch, it lies at a distance of ~220 kpc. Based on the SDSS data, we estimate an absolute magnitude of Mv ~ -7.9, a central surface brightness of mu_0,V ~ 28 mag arcsecond^-2, and a half-light radius of \\~ 8.5' (~ 550 pc at the measured distance). The outer regions of Canes Venatici appear extended and distorted. The discovery of such a faint galaxy in proximity to the Milky Way strongly suggests that more such objects remain to be found.

D. B. Zucker; V. Belokurov; N. W. Evans; M. I. Wilkinson; M. J. Irwin; T. Sivarani; S. Hodgkin; D. M. Bramich; J. M. Irwin; G. Gilmore; B. Willman; S. Vidrih; M. Fellhauer; P. C. Hewett; T. C. Beers; E. F. Bell; E. K. Grebel; D. P. Schneider; H. J. Newberg; R. F. G. Wyse; C. M. Rockosi; B. Yanny; R. Lupton; J. A. Smith; J. C. Barentine; H. Brewington; J. Brinkmann; M. Harvanek; S. J. Kleinman; J. Krzesinski; D. Long; A. Nitta; S. A. Snedden

2006-04-17T23:59:59.000Z

482

A New Milky Way Dwarf Satellite in Canes Venatici  

E-Print Network (OSTI)

In this Letter, we announce the discovery of a new dwarf satellite of the Milky Way, located in the constellation Canes Venatici. It was found as a stellar overdensity in the North Galactic Cap using Sloan Digital Sky Survey Data Release 5 (SDSS DR5). The satellite's color-magnitude diagram shows a well-defined red giant branch, as well as a horizontal branch. As judged from the tip of the red giant branch, it lies at a distance of ~220 kpc. Based on the SDSS data, we estimate an absolute magnitude of Mv ~ -7.9, a central surface brightness of mu_0,V ~ 28 mag arcsecond^-2, and a half-light radius of \\~ 8.5' (~ 550 pc at the measured distance). The outer regions of Canes Venatici appear extended and distorted. The discovery of such a faint galaxy in proximity to the Milky Way strongly suggests that more such objects remain to be found.

Zucker, D B; Evans, N W; Wilkinson, M I; Irwin, M J; Sivarani, T; Hodgkin, S; Bramich, D M; Irwin, J M; Gilmore, G; Willman, B; Vidrih, S; Fellhauer, M; Hewett, P C; Beers, T C; Bell, E F; Grebel, E K; Schneider, D P; Newberg, H J; Wyse, R F G; Rockosi, C M; Yanny, B; Lupton, R; Smith, J A; Barentine, J C; Brewington, H; Brinkmann, J; Harvanek, M; Kleinman, S J; Krzesínski, J; Long, D; Nitta, A; Snedden, S A

2006-01-01T23:59:59.000Z

483

B0850+054: a new gravitational lens system from CLASS  

E-Print Network (OSTI)

We report the discovery of a new gravitational lens system from the CLASS survey. Radio observations with the VLA, the WSRT and MERLIN show that the radio source B0850+054 is comprised of two compact components with identical spectra, a separation of 0.7 arcsec and a flux density ratio of 6:1. VLBA observations at 5 GHz reveal structures that are consistent with the gravitational lens hypothesis. The brighter of the two images is resolved into a linear string of at least six sub-components whilst the weaker image is radially stretched towards the lens galaxy. UKIRT K-band imaging detects an 18.7 mag extended object, but the resolution of the observations is not sufficient to resolve the lensed images and the lens galaxy. Mass modelling has not been possible with the present data and the acquisition of high-resolution optical data is a priority for this system.

A. D. Biggs; D. Rusin; I. W. A. Browne; A. G. de Bruyn; N. J. Jackson; L. V. E. Koopmans; J. P. McKean; S. T. Myers; R. D. Blandford; K. -H. Chae; C. D. Fassnacht; M. A. Norbury; T. J. Pearson; P. M. Phillips; A. C. S. Readhead

2002-10-23T23:59:59.000Z

484

A first-overtone RR Lyrae star with cyclic period changes  

E-Print Network (OSTI)

A detailed light curve analysis is presented for a first-overtone RR Lyrae star, MACHO* J050918.712-695015.31, based on MACHO and OGLE-III observations. As a foreground object of the Large Magellanic Cloud, it gives an extraordinary opportunity to study an almost continuous, 12-year long dataset of a relatively bright (V~15.0 mag) RRc star with rapid period change. Cyclic period modulation is suggested by the O-C method, where the cycle length is about 8 years. With the available unique dataset, we could draw strong limits on other light curve changes that may be associated to the period modulation. We could exclude both multiple periodicity and amplitude modulation unambiguously. Any theoretical model should reproduce the observed lack of photometric modulations. Simple arguments are also given for possible hydromagnetic effects.

A. Derekas; L. L. Kiss; A. Udalski; T. R. Bedding; K. Szatmary

2004-07-20T23:59:59.000Z

485

Multiperiodic Galactic field RR Lyrae stars in the ASAS catalog  

E-Print Network (OSTI)

The All Sky Automated Survey (ASAS) monitors bright stars (8 mag RRc stars exhibit the Blazhko effect. We observe a deficiency of RRab Blazhko variables with main pulsation periods greater than 0.65 days. The Blazhko periods of RRc stars exhibit a strongly bimodal distribution. During our study we discovered the Blazhko effect with multiple periods in object ASAS 050747-3351.9 = SU Col. Blazhko periods of 89.3 d and 65.8 d and a candidate of 29.5 d were identified with periodogram peaks near the first three harmonics of the main pulsation. These observations may inspire new models of the Blazhko effect, which has eluded a consistent theory since its discovery about one hundred years...

Szczygiel, D M

2007-01-01T23:59:59.000Z

486

Media Center - TTRDC in the News  

NLE Websites -- All DOE Office Websites (Extended Search)

0 Press Coverage 0 Press Coverage December 22, 2010 -- DOE Energy Blog Interview with Pat Davis of DOE's Vehicle Technologies Program; discussion of electric vehicles December 17, 2010 -- The Green Optimistic Thermoelectric properties of lead chalcogenides and their application to combustion engines. December 14, 2010 -- Wired Autopia Aymeric Rousseau blogs about Autonomie. December 10, 2010 -- R&D Mag Will Elias is quoted on Argonne's battery research. November 24, 2010 -- New York Times Preparing Students to Roll Off the Campus and Into Big Automotive Jobs November 19, 2010 -- Chicago Tribune Illinois Tollway and Argonne Announce Three-Year Partnership to Work on Green Projects October 27, 2010 -- FavStocks Argonne partner BASF breaks ground on North American Li-ion cathode plant.

487

2011 Annual Workforce Analysis and Staffing Plan Report - Carlsbad  

Energy.gov (U.S. Department of Energy (DOE)) Indexed Site

United States Government United States Government Department of Energy memorandum Carlsbad Field Office Carlsbad, New Mexico 88221 DATE: REPLY TO ATTN OF: SUBJECT: January 19, 2012 CBFO:OOM:GTB:MAG:12-1801 :UFC 3410.00 CBFO Annual Workforce Analysis and Staffing Plan ro: Karen L. Boardman, Chairperson, Federal Technical Capability Panel (HS-70) The Carlsbad Field Office (CBFO) has updated the CBFO Annual Workforce Analysis and Staffing Plan as of December 31, 2011. The attachment to this Memorandum provides the updated CBFO Workforce Analysis and Staffing information on the Federal Technical Capability Program Workforce Staffing and Analysis Report template. If you have questions, please contact Mr. George T. Basabilvazo, CBFO Federal Technical Capability Panel Agent, at (575) 234-7488.

488

Caltech Faint Galaxy Redshift Survey VII: Data Analysis Techniques and Redshifts in the Field J0053+1234  

E-Print Network (OSTI)

We present the techniques used to determine redshifts and to characterize the spectra of objects in the Caltech Faint Galaxy Redshift Survey in terms of spectral classes and redshift quality classes. These are then applied to spectra from an investigation of a complete sample of objects with $K_s<20$ mag in a 2 by 7.3 arcmin^2 field at J005325+1234. Redshifts were successfully obtained for 163 of the 195 objects in the sample; these redshifts lie in the range [0.173, 1.44] and have a median of 0.58 (excluding 24 Galactic stars). The sample includes two broad lined AGNs and one QSO.

Judith G. Cohen; David W. Hogg; Michael A. Pahre; Roger Blandford; Patrick L. Shopbell; Kevin Richberg

1998-09-05T23:59:59.000Z

489

PETSc Bibliography  

NLE Websites -- All DOE Office Websites (Extended Search)

and Publications that make use of PETSc and Publications that make use of PETSc Nano-simulations A graphical extension for the Windows version of the Parallel Finite Element Micromagnetics Package (MagParExt), Tomasz Blachowicz and Bartlomiej Baron, 2008. BibTeX Field induced vortex dynamics in magnetic Ni nanotriangles, R. Y. Jaafar, A Asenjo, O Chubykalo-Fesenko, M Vazquez, E M Gonzalez, and J L Vicent, Nanotechnology, 19, 2008. BibTeX Micromagnetic Simulation of Magnetic Particles with Surface Anisotropy, Lin Yuan, Jianjun Jiang, Gang Du, Zhongyou Wang, and Huahui He, Journal of the Magnetics Society of Japan, 32, 50-53, 2008. BibTeX Magnetic strip patterns induced by focused ion beam irradiation, D. Makarov, S. Tibus, C. T. Rettner, T. Thomson, B. D. Terris, T. Schrefl, and M. Albrecht, J. Appl. Phys., 103, 2008. BibTeX

490

A multiwavlength study of PSR B0628-28: The first overluminous rotation-powered pulsar?  

E-Print Network (OSTI)

The ROSAT source RX J0630.8-2834 was suggested by positional coincidence to be the X-ray counterpart of the old field pulsar PSR B0628-28. This association, however, was regarded to be unlikely based on the computed energetics of the putative X-ray counterpart. In this paper we report on multiwavelength observations of PSR B0628-28 made with the ESO/NTT observatory in La Silla, the Jodrell Bank radio observatory and XMM-Newton. Although the optical observations do not detect any counterpart of RX J0630.8-2834 down to a limiting magnitude of V=26.1 mag and B=26.3 mag, XMM-Newton observations finally confirmed it to be the pulsar's X-ray counterpart by detecting X-ray pulses with the radio pulsar's spin-period. The X-ray pulse profile is characterized by a single broad peak with a second smaller peak leading the main pulse component by ~144 degree. The fraction of pulsed photons is (38 +- 7)% with no strong energy dependence in the XMM-Newton bandpass. The pulsar's X-ray spectrum is well described by a single component power law with photon index 2.63^{+0.23}_{-0.15}, indicating that the pulsar's X radiation is dominated by non-thermal emission processes. A low level contribution of thermal emission from residual cooling or from heated polar caps, cannot be excluded. The pulsar's spin-down to X-ray energy conversion efficiency is obtained to be ~16% for the radio dispersion measure inferred pulsar distance. If confirmed, PSR B0628-28 would be the first X-ray overluminous rotation-powered pulsar identified among all ~1400 radio pulsars known today.

Werner Becker; Axel Jessner; Michael Kramer; Vincenzo Testa; Clemens Howaldt

2005-05-24T23:59:59.000Z

491

VERY LARGE TELESCOPE/X-SHOOTER SPECTROSCOPY OF THE CANDIDATE BLACK HOLE X-RAY BINARY MAXI J1659-152 IN OUTBURST  

SciTech Connect

We present the optical to near-infrared spectrum of MAXI J1659-152 during the onset of its 2010 X-ray outburst. The spectrum was obtained with X-shooter on the ESO Very Large Telescope early in the outburst simultaneous with high-quality observations at both shorter and longer wavelengths. At the time of the observations, the source was in the low-hard state. The X-shooter spectrum includes many broad ({approx}2000 km s{sup -1}), double-peaked emission profiles of H, He I, and He II, characteristic signatures of a low-mass X-ray binary during outburst. We detect no spectral signatures of the low-mass companion star. The strength of the diffuse interstellar bands results in a lower limit to the total interstellar extinction of A{sub V} {approx_equal} 0.4 mag. Using the neutral hydrogen column density obtained from the X-ray spectrum we estimate A{sub V} {approx_equal} 1 mag. The radial velocity structure of the interstellar Na I D and Ca II H and K lines results in a lower limit to the distance of {approx}4 {+-} 1 kpc, consistent with previous estimates. With this distance and A{sub V} , the dereddened spectral energy distribution represents a flat disk spectrum. The two 10 minute X-shooter spectra show significant variability in the red wing of the emission-line profiles, indicating a global change in the density structure of the disk, though on a timescale much shorter than the typical viscous timescale of the disk.

Kaur, Ramanpreet; Kaper, Lex; Ellerbroek, Lucas E.; Russell, David M.; Altamirano, Diego; Wijnands, Rudy; Yang Yijung; Van der Horst, Alexander; Van der Klis, Michiel [Astronomical Institute 'Anton Pannekoek', University of Amsterdam, Science Park 904, 1098 XH Amsterdam (Netherlands); D'Avanzo, Paolo [INAF, Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate (Italy); De Ugarte Postigo, Antonio; Fynbo, Johan P. U. [Dark Cosmology Centre, Niels Bohr Institute, Juliane Maries Vej 30, Copenhagen 2100 (Denmark); Flores, Hector [GEPI, Paris Observatory, CNRS, University of Paris-Diderot, 5 Place Jules Janssen, 92195 Meudon (France); Goldoni, Paolo [Laboratoire Astroparticule et Cosmologie, 10 rue A. Domon et L. Duquet, 75205 Paris Cedex 13 (France); Thoene, Christina C. [IAA-CSIC, Glorieta de la Astronomia s/n, 18008 Granada (Spain); Kouveliotou, Chryssa [Space Science Office, VP62, NASA/Marshall Space Flight Center, Huntsville, AL 35812 (United States); Wiersema, Klaas [Department of Physics and Astronomy, University of Leicester, University Road, Leicester LE1 7RH (United Kingdom); Kuulkers, Erik, E-mail: r.kaur@uva.nl [European Space Agency, European Space Astronomy Centre, P.O. Box 78, 28691 Villanueva de la Canada, Madrid (Spain)

2012-02-20T23:59:59.000Z

492

Light and Motion in SDSS Stripe 82: The Catalogues  

E-Print Network (OSTI)

We present a new public archive of light-motion curves in Sloan Digital Sky Survey (SDSS) Stripe 82, covering 99 deg in right ascension from RA = 20.7 h to 3.3 h and spanning 2.52 deg in declination from Dec = -1.26 to 1.26 deg, for a total sky area of ~249 sq deg. Stripe 82 has been repeatedly monitored in the u, g, r, i and z bands over a seven-year baseline. Objects are cross-matched between runs, taking into account the effects of any proper motion. The resulting catalogue contains almost 4 million light-motion curves of stellar objects and galaxies. The photometry are recalibrated to correct for varying photometric zeropoints, achieving ~20 mmag and ~30 mmag root-mean-square (RMS) accuracy down to 18 mag in the g, r, i and z bands for point sources and extended sources, respectively. The astrometry are recalibrated to correct for inherent systematic errors in the SDSS astrometric solutions, achieving ~32 mas and ~35 mas RMS accuracy down to 18 mag for point sources and extended sources, respectively. For each light-motion curve, 229 photometric and astrometric quantities are derived and stored in a higher-level catalogue. On the photometric side, these include mean exponential and PSF magnitudes along with uncertainties, RMS scatter, chi^2 per degree of freedom, various magnitude distribution percentiles, object type (stellar or galaxy), and eclipse, Stetson and Vidrih variability indices. On the astrometric side, these quantities include mean positions, proper motions as well as their uncertainties and chi^2 per degree of freedom. The here presented light-motion curve catalogue is complete down to r~21.5 and is at present the deepest large-area photometric and astrometric variability catalogue available.

D. M. Bramich; S. Vidrih; L. Wyrzykowski; J. A. Munn; H. Lin; N. W. Evans; M. C. Smith; V. Belokurov; G. Gilmore; D. B. Zucker; P. C. Hewett; L. L. Watkins; D. C. Faria; M. Fellhauer; G. Miknaitis; D. Bizyaev; Z. Ivezic; D. P. Schneider; S. A. Snedden; E. Malanushenko; V. Malanushenko; K. Pan

2008-01-31T23:59:59.000Z

493

LUMINOUS AND HIGH STELLAR MASS CANDIDATE GALAXIES AT z Almost-Equal-To 8 DISCOVERED IN THE COSMIC ASSEMBLY NEAR-INFRARED DEEP EXTRAGALACTIC LEGACY SURVEY  

SciTech Connect

One key goal of the Hubble Space Telescope Cosmic Assembly Near-Infrared Deep Extragalactic Legacy Survey is to track galaxy evolution back to z Almost-Equal-To 8. Its two-tiered ''wide and deep'' strategy bridges significant gaps in existing near-infrared surveys. Here we report on z Almost-Equal-To 8 galaxy candidates selected as F105W-band dropouts in one of its deep fields, which covers 50.1 arcmin{sup 2} to 4 ks depth in each of three near-infrared bands in the Great Observatories Origins Deep Survey southern field. Two of our candidates have J < 26.2 mag, and are >1 mag brighter than any previously known F105W-dropouts. We derive constraints on the bright end of the rest-frame ultraviolet luminosity function of galaxies at z Almost-Equal-To 8, and show that the number density of such very bright objects is higher than expected from the previous Schechter luminosity function estimates at this redshift. Another two candidates are securely detected in Spitzer Infrared Array Camera images, which are the first such individual detections at z Almost-Equal-To 8. Their derived stellar masses are on the order of a few Multiplication-Sign 10{sup 9} M{sub Sun }, from which we obtain the first measurement of the high-mass end of the galaxy stellar mass function at z Almost-Equal-To 8. The high number density of very luminous and very massive galaxies at z Almost-Equal-To 8, if real, could imply a large stellar-to-halo mass ratio and an efficient conversion of baryons to stars at such an early time.

Yan Haojing [Department of Physics and Astronomy, University of Missouri, Columbia, MO 65211 (United States); Finkelstein, Steven L. [Department of Astronomy, University of Texas at Austin, Austin, TX 78712 (United States); Huang, Kuang-Han [Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218 (United States); Ryan, Russell E.; Ferguson, Henry C.; Koekemoer, Anton M.; Grogin, Norman A. [Space Telescope Science Institute, Baltimore, MD 21218 (United States); Dickinson, Mark [National Optical Astronomy Observatory, Tucson, AZ 85719 (United States); Newman, Jeffrey A. [Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA 15260 (United States); Somerville, Rachel S. [Physics and Astronomy Department, Rutgers University, Piscataway, NJ 08854 (United States); Dave, Romeel [Astronomy Department, University of Arizona, Tucson, AZ 85721 (United States); Faber, S. M. [University of California Observatories/Lick Observatory, University of California, Santa Cruz, CA 95064 (United States); Papovich, Casey [George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy, and Department of Physics and Astronomy, Texas A and M University, College Station, TX 77843-4242 (United States); Guo Yicheng; Giavalisco, Mauro [Department of Astronomy, University of Massachusetts, Amherst, MA 01003 (United States); Lee, Kyoung-soo [Department of Physics, Purdue University, West Lafayette, IN 47907 (United States); Reddy, Naveen; Siana, Brian D. [Department of Physics and Astronomy, University of California, Riverside, CA 92521 (United States); Cooray, Asantha R. [Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States); Hathi, Nimish P. [Observatories of the Carnegie Institution for Science, Pasadena, CA 91101 (United States); and others

2012-12-20T23:59:59.000Z

494

THE NEXT GENERATION VIRGO CLUSTER SURVEY (NGVS). I. INTRODUCTION TO THE SURVEY  

SciTech Connect

The Next Generation Virgo Cluster Survey (NGVS) is a program that uses the 1 deg{sup 2} MegaCam instrument on the Canada-France-Hawaii Telescope to carry out a comprehensive optical imaging survey of the Virgo cluster, from its core to its virial radius-covering a total area of 104 deg{sup 2}-in the u*griz bandpasses. Thanks to a dedicated data acquisition strategy and processing pipeline, the NGVS reaches a point-source depth of g Almost-Equal-To 25.9 mag (10{sigma}) and a surface brightness limit of {mu}{sub g} {approx} 29 mag arcsec{sup -2} (2{sigma} above the mean sky level), thus superseding all previous optical studies of this benchmark galaxy cluster. In this paper, we give an overview of the technical aspects of the survey, such as areal coverage, field placement, choice of filters, limiting magnitudes, observing strategies, data processing and calibration pipelines, survey timeline, and data products. We also describe the primary scientific topics of the NGVS, which include: the galaxy luminosity and mass functions; the color-magnitude relation; galaxy scaling relations; compact stellar systems; galactic nuclei; the extragalactic distance scale; the large-scale environment of the cluster and its relationship to the Local Supercluster; diffuse light and the intracluster medium; galaxy interactions and evolutionary processes; and extragalactic star clusters. In addition, we describe a number of ancillary programs dealing with 'foreground' and 'background' science topics, including the study of high-inclination trans-Neptunian objects; the structure of the Galactic halo in the direction of the Virgo Overdensity and Sagittarius Stream; the measurement of cosmic shear, galaxy-galaxy, and cluster lensing; and the identification of distant galaxy clusters, and strong-lensing events.

Ferrarese, Laura; Cote, Patrick; Gwyn, S. D. J.; MacArthur, Lauren A.; McConnachie, Alan W.; Blakeslee, John P. [Herzberg Institute of Astrophysics, National Research Council of Canada, Victoria, BC, V9E 2E7 (Canada); Cuillandre, Jean-Charles [Canada-France-Hawaii Telescope Corporation, Kamuela, HI 96743 (United States); Peng, Eric W. [Department of Astronomy, Peking University, Beijing 100871 (China); Duc, Pierre-Alain [AIM Paris Saclay, CNRS/INSU, CEA/Irfu, Universite Paris Diderot, Orme des Merisiers, F-91191 Gif sur Yvette cedex (France); Boselli, A. [Laboratoire d'Astrophysique de Marseille, UMR 6110 CNRS, 38 rue F. Joliot-Curie, F-13388 Marseille (France); Mei, Simona [GEPI, Observatoire de Paris, CNRS, 5 Place Jules Jannssen, F-92195 Meudon (France); Erben, Thomas [Argelander-Institut fuer Astronomie, University of Bonn, Auf dem Huegel 71, D-53121 Bonn (Germany); Durrell, Patrick R. [Department of Physics and Astronomy, Youngstown State University, Youngstown, OH (United States); Christopher Mihos, J. [Department of Astronomy, Case Western Reserve University, Cleveland, OH (United States); Jordan, Andres; Puzia, Thomas H. [Departamento de Astronomia y Astrofisica, Pontificia Universidad Catolica de Chile, 7820436 Macul, Santiago (Chile); Lancon, Ariane [Observatoire Astronomique, Universite de Strasbourg and CNRS UMR 7550, 11 rue de l'Universite, F-67000 Strasbourg (France); Emsellem, Eric [Universite de Lyon 1, CRAL, Observatoire de Lyon, 9 av. Charles Andre, F-69230 Saint-Genis Laval (France); CNRS, UMR 5574, ENS de Lyon (France); Balogh, Michael L. [Department of Physics and Astronomy, University of Waterloo, Waterloo, Ontario, N2L 3G1 (Canada); Van Waerbeke, Ludovic [Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, B.C., V6T 1Z1 (Canada); and others

2012-05-01T23:59:59.000Z

495

Spectrum and proper motion of a brown dwarf companion of the T Tauri star CoD-33 7795  

E-Print Network (OSTI)

We present optical and infrared spectra as well as the proper motion of an H=12 mag object 2" off the ~5 mag brighter spectroscopic binary star CoD-33 7795 (=TWA-5), a member of the TW Hya association of T Tauri stars at ~55 pc. It was suggested as companion candidate by Lowrance et al. (1999) and Webb et al. (1999), but neither a spectrum nor the proper motion of the faint object were available before. Our spectra taken with FORS2 and ISAAC at the ESO-VLT reveal that the companion candidate has spectral type M8.5 to M9. It shows strong H-alpha emission and weak Na I absorption, both indicative of a young age. The faint object is clearly detected and resolved in our optical and infrared images, with a FWHM of 0.18" in the FORS2 image. The faint object's proper motion, based on two year epoch difference, is consistent with the proper motion of CoD-33 7795 by 5 Gaussian sigma significance. From three different theoretical pre-main sequence models, we estimate the companion mass to be between ~15 and 40 M_jup, assuming the distance and age of the primary. A slight offset between the VLT and HST images with an epoch difference of two years can be interpreted as orbital motion. The probability for chance alignment of such a late-type object that close to CoD-33 7795 with the correct proper motion is below 7e-9. Hence, the faint object is physically associated with CoD-33 7795, the 4th brown dwarf companion around a normal star confirmed by both spectrum and proper motion, the first around a pre-main sequence star.

R. Neuhaeuser; E. W. Guenther; M. G. Petr; W. Brandner; N. Huelamo; J. Alves

2000-07-20T23:59:59.000Z

496

THE OUTER DISKS OF EARLY-TYPE GALAXIES. II. SURFACE-BRIGHTNESS PROFILES OF UNBARRED GALAXIES AND TRENDS WITH HUBBLE TYPE  

Science Conference Proceedings (OSTI)

We present azimuthally averaged radial profiles of R-band surface brightness for a complete sample of 47 early-type, unbarred galaxies, as a complement to our previous study of early-type barred galaxies. Following very careful sky subtraction, the profiles can typically be determined down to brightness levels well below 27 mag arcsec{sup -2} and in the best cases below 28 mag arcsec{sup -2}. We classified the profiles according to the scheme used previously for the barred sample: Type I profiles are single unbroken exponential radial declines in brightness; Type II profiles ('truncations') have an inner shallow slope (usually exponential) which changes at a well-defined break radius to a steeper exponential; and Type III profiles ('antitruncations') have an inner exponential that is steeper, giving way to a shallower outer (usually exponential) decline. By combining these profiles with previous studies, we can make the first clear statements about the trends of outer-disk-profile types along the Hubble sequence (including both barred and unbarred galaxies), and their global frequencies. We find that Type I profiles are most frequent in early-type disks, decreasing from one-third of all S0-Sa disks to barely 10% of the latest-type spirals. Conversely, Type II profiles (truncations) increase in frequency with Hubble type, from only {approx}25% of S0 galaxies to {approx}80% of Sd-Sm spirals. Overall, the fractions of Type I, II, and III profiles for all disk galaxies (Hubble types S0-Sm) are 21%, 50%, and 38%, respectively; this includes galaxies ({approx}8% of the total) with composite Type II+III profiles (counted twice). Finally, we note the presence of bars in 10 galaxies previously classified (optically) as 'unbarred'. This suggests that {approx}20% of optically unbarred galaxies are actually barred; the bars in such cases can be weak, obscured by dust, or so large as to be mistaken for the main disk of the galaxy.

Gutierrez, Leonel [Universidad Nacional Autonoma de Mexico, Instituto de Astronomia, Ensenada, B. C. (Mexico); Erwin, Peter [Max-Planck-Insitut fuer extraterrestrische Physik, 85748 Garching (Germany); Aladro, Rebeca; Beckman, John E., E-mail: leonel@astrosen.unam.mx, E-mail: r.aladro@ucl.ac.uk, E-mail: jeb@iac.es, E-mail: erwin@mpe.mpg.de [Instituto de Astrofisica de Canarias, Tenerife (Spain)

2011-11-15T23:59:59.000Z

497

A CCD Imaging Search for Wide Metal-Poor Binaries  

E-Print Network (OSTI)

We explored the regions within a radius of 25 arcsec around 473 nearby, low-metallicity G- to M-type stars using (VR)I optical filters and small-aperture telescopes. About 10% of the sample was searched up to angular separations of 90 arcsec. We applied photometric and astrometric techniques to detect true physical companions to the targets. The great majority of the sample stars was drawn from the Carney-Latham surveys; their metallicities range from roughly solar to [Fe/H]=-3.5 dex. Our I-band photometric survey detected objects that are between 0 and 5 mag fainter (completeness) than the target stars; the maximum dynamical range of our exploration is 9 mag. We also investigated the literature and inspected images from the Digitized Sky Surveys to complete our search. By combining photometric and proper motion measurements, we retrieved 29 previously known companions, and identified 13 new proper motion companions. Near-infrared 2MASS photometry is provided for the great majority of them. Low-resolution optical spectroscopy (386-1000 nm) was obtained for eight of the new companion stars. These spectroscopic data confirm them as cool, late-type, metal-depleted dwarfs, with spectral classes from esdK7 to sdM3. After comparison with low-metallicity evolutionary models, we estimate the masses of the proper motion companion stars to be in the range 0.5-0.1 Msol. They are orbiting their primary stars at projected separations between ~32 and ~57000 AU. These orbital sizes are very similar to those of solar-metallicity stars of the same spectral types. Our results indicate that about 15% of the metal-poor stars have stellar companions at large orbits, which is in agreement with the binary fraction observed among main sequence G- to M-type stars and T Tauri stars.

M. R. Zapatero Osorio; E. L. Martin

2004-02-12T23:59:59.000Z

498

RECURRENT PERIHELION ACTIVITY IN (3200) PHAETHON  

SciTech Connect

We present a study of planet-crossing asteroid (3200) Phaethon at three successive perihelia in 2009, 2010, and 2012, using the NASA STEREO spacecraft. Phaethon is clearly detected in 2009 and 2012, but not in 2010. In both former years, Phaethon brightened unexpectedly by {approx}1 mag at large phase angles, inconsistent with the {approx}1 mag of steady fading expected from a discrete, macroscopic body over the same phase angle range. With a perihelion distance of 0.14 AU and surface temperatures up to {approx}1000 K, a thermal origin of this anomalous brightening is strongly suspected. However, simple thermal emission from Phaethon is too weak, by a factor >10{sup 3}, to explain the brightening. Nor can ice survive on this body, ruling out comet-like sublimation. Our preferred explanation is that brightening occurs as a result of dust produced and ejected from Phaethon, perhaps by thermal fracture and/or thermal decomposition of surface minerals when near perihelion. A contribution from prompt emission by oxygen released by desiccation of surface minerals cannot be excluded. We infer an ejected mass of order 4 Multiplication-Sign 10{sup 8} a{sub mm} kg per outburst, where a{sub mm} is the mean dust radius in millimeters. For plausible dust radii, this mass is small compared to the estimated mass of Phaethon ({approx}2 Multiplication-Sign 10{sup 14} kg) and to the mass of the Geminid stream (10{sup 12}-10{sup 13} kg) with which Phaethon is dynamically associated. Perihelion mass-loss events like those observed in 2009 and 2012 contribute to, but do not necessarily account for the Geminids stream mass.

Li Jing; Jewitt, David, E-mail: jli@igpp.ucla.edu [Department of Earth and Space Sciences, University of California at Los Angeles, Los Angeles, CA (United States)

2013-06-15T23:59:59.000Z