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Note: This page contains sample records for the topic "redshift systems corporation" 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.


1

Solar Energy Systems Tax Credit (Corporate) (Iowa)  

Broader source: Energy.gov [DOE]

Iowa offers a 15% corporate tax credit for solar energy systems. The credit is based on the federal tax credits for solar; a taxpayer may claim 50% of the value of the [http://dsireusa.org...

2

Photometric Redshift Determination with the BATC Multicolor System  

E-Print Network [OSTI]

In this paper, we present the methodology of photometric redshift determination with the BATC 15-color system by using hyperz program. Both simulated galaxies and real galaxies with known redshifts were used to estimate the accuracy of redshifts inferred from the multicolor photometry. From the test with simulated galaxies, the uncertainty in the inferred redshifts is about $0.02\\sim0.03$ for a given range of photometric uncertainty of $0.05 \\sim 0.10$. The results with the 27 real galaxies are in good agreement with the simulated ones. The advantage of using BATC intermediate-band system to derive redshift is clear through the comparison with the UBVRI broad-band system. The accuracy in redshift determination with BATC system is mainly affected by the selection of filters and the photometric uncertainties in the observation. When we take the limiting magnitudes of the 15 filters into account, we find that redshift can be determined with good accuracy for galaxies with redshifts less than 0.5, using only filt...

Xia, L; Ma, J; Wu, H; Sun, W H; Jiang, Z; Xue, S; Chen, J; Chen, W; Xia, Lifang; Zhou, Xu; Ma, Jun; Wu, Hong; Sun, Wei-Hsin; Jiang, Zhaoji; Xue, Suijian; Chen, Jiansheng; Chen, Wenping

2002-01-01T23:59:59.000Z

3

System to estimate ages and redshifts for radio galaxies  

E-Print Network [OSTI]

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

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

2001-12-06T23:59:59.000Z

4

Corporate Law, Social Norms and Belief Systems  

E-Print Network [OSTI]

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

Eisenberg, Melvin

1999-01-01T23:59:59.000Z

5

QSO Metal Absorption Systems at High Redshift Toru Misawa1  

E-Print Network [OSTI]

QSO Metal Absorption Systems at High Redshift Toru Misawa1 , Nobunari Kashikawa2 , Youichi Ohyama2 Abstract. Quasar absorption systems give us useful information about very faint objects that we cannot detect directly. For example, metal absorption systems are generally provided by star formation

Iye, Masanori

6

RedShift Systems Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to: navigation, search RAPIDColoradosourceRausWyoming: EnergyElec Assn Jump to:RedShift

7

THE EVOLUTION OF LYMAN LIMIT ABSORPTION SYSTEMS TO REDSHIFT SIX  

SciTech Connect (OSTI)

We have measured the redshift evolution of the density of Lyman limit systems (LLSs) in the intergalactic medium over the redshift range 0 < z < 6. We have used two new quasar samples to (1) improve coverage at z {approx} 1, with GALEX grism spectrograph observations of 50 quasars with 0.8 < z{sub em} < 1.3, and (2) extend coverage to z {approx} 6, with Keck ESI spectra of 25 quasars with 4.17 < z{sub em} < 5.99. Using these samples together with published data, we find that the number density of LLS per unit redshift, n(z), can be well fit by a simple evolution of the form n(z) = n{sub 3.5}[(1 + z)/4.5]{sup {gamma}} with n{sub 3.5} = 2.80 {+-} 0.33 and {gamma} = 1.94{sup +0.36}{sub -0.32} for the entire range 0 < z < 6. We have also reanalyzed the evolution of damped Ly{alpha} systems (DLAs) in the redshift range 4 < z < 5 using our high-redshift quasar sample. We find a total of 17 DLAs and sub-DLAs, which we have analyzed in combination with published data. The DLAs with log H{sub I} column density > 20.3 show the same redshift evolution as the LLS. When combined with previous results, our DLA sample is also consistent with a constant {Omega}{sub DLA} = 9 x 10{sup -4} from z = 2 to z = 5. We have used the LLS number density evolution to compute the evolution in the mean free path (mfp) of ionizing photons. We find a smooth evolution to z {approx} 6, very similar in shape to that of Madau et al. but about a factor of two higher. Recent theoretical models roughly match to the z < 6 data but diverge from the measured power law at z>6 in different ways, cautioning against extrapolating the fit to the mfp outside the measured redshift range.

Songaila, Antoinette; Cowie, Lennox L. [W. M. Keck Observatory, which is jointly operated by the California Institute of Technology, University of California, and National Aeronautics and Space Administration. (United States)

2010-10-01T23:59:59.000Z

8

Hindawi Publishing Corporation EURASIP Journal on Embedded Systems  

E-Print Network [OSTI]

Hindawi Publishing Corporation EURASIP Journal on Embedded Systems Volume 2009, Article ID 175043 Yassin El-Hillali,1 and Atika Rivenq-Menhaj1 1 Universit´e de Valenciennes et du Hainaut-Cambr´esis, ISTV

Boyer, Edmond

9

Buildings and corporate strategy : towards a management system model  

E-Print Network [OSTI]

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

Brana, Rodrigo

1985-01-01T23:59:59.000Z

10

Hindawi Publishing Corporation EURASIP Journal on Bioinformatics and Systems Biology  

E-Print Network [OSTI]

--from a system's biological point of view--could be understood as organized in interacting networks at allHindawi Publishing Corporation EURASIP Journal on Bioinformatics and Systems Biology Volume 2009 and Biometry, Research Institute for the Biology of Farm Animals (FBN), Wilhelm-Stahl Allee 2, D 18196

11

Fastcap Systems Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump37.California: Energy Resources44795°, -83.3763218°Farnham,Fastcap Systems

12

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

E-Print Network [OSTI]

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

Baldick, Ross

13

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

E-Print Network [OSTI]

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

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

2001-04-18T23:59:59.000Z

14

Tax Credit for Solar Energy Systems on Residential Property (Corporate)  

Broader source: Energy.gov [DOE]

'''''Note: HB 705 of 2013 made several significant changes to this tax credit. Among other changes, wind energy systems are no longer eligible, there is now an expiration date for the credit, and...

15

Hindawi Publishing Corporation EURASIP Journal on Embedded Systems  

E-Print Network [OSTI]

that sup- port abstraction and automation. Low-level energy estimation methods take into account many circuit density and performance, the management of power consumption in system-on-chip (SoC) is becoming a better tradeoff between accuracy and speed. This paper presents a consumption estimation approach

Paris-Sud XI, Université de

16

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

E-Print Network [OSTI]

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

Tom Broadhurst; Xiaosheng Huang; Brenda Frye; Richard Ellis

1999-02-23T23:59:59.000Z

17

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

E-Print Network [OSTI]

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

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

2005-06-22T23:59:59.000Z

18

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

E-Print Network [OSTI]

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

Bishop, Keith

2008-01-01T23:59:59.000Z

19

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

E-Print Network [OSTI]

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

Tissera, P B; Cora, S A

2001-01-01T23:59:59.000Z

20

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

E-Print Network [OSTI]

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

Reuter, George N. (George Nicholas)

2014-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "redshift systems corporation" 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

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

E-Print Network [OSTI]

This study explores how the EU Emissions Trading System (EU ETS) actually works on the ground@bookpoint.co.uk May 2013 322 pages Hardback 978-1-4094-6078-7 ÂŁ60.00 Corporate Responses to EU Emissions Trading at The Fridtjof Nansen Institute, Norway `With greenhouse gas emissions trading schemes emerging worldwide

22

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

E-Print Network [OSTI]

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

Aronson, Bruce E.

2012-01-01T23:59:59.000Z

23

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

E-Print Network [OSTI]

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

Roth, George

2010-11-30T23:59:59.000Z

24

An analysis of structure and process of corporate alliance development using system architecture frameworks  

E-Print Network [OSTI]

A strategic alliance has been one of the core methods for expanding the business of many corporations in terms of geographic presence, business domain, and technological scope. The strategic alliance includes many different ...

Kim, Gwang Gyu

2007-01-01T23:59:59.000Z

25

Optimal multihump filter for photometric redshifts  

E-Print Network [OSTI]

We propose a novel type filter for multicolor imaging to improve on the photometric redshift estimation of galaxies. An extra filter - specific to a certain photometric system - may be utilized with high efficiency. We present a case study of the Hubble Space Telescope's Advanced Camera for Surveys and show that one extra exposure could cut down the mean square error on photometric redshifts by 34% over the z<1.3 redshift range.

Tamas Budavari; Alexander S. Szalay; Istvan Csabai; Andrew J. Connolly; Zlatan Tsvetanov

2001-06-05T23:59:59.000Z

26

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

E-Print Network [OSTI]

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

Meij, Jan-Martin

2008-01-01T23:59:59.000Z

27

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

E-Print Network [OSTI]

Hyatt Hotels Corporation is currently implementing an enterprise-wide Energy Information and Utility Monitoring System (UMS). New Horizon Technologies and eComponents Technology have teamed to provide an integrated solution that will ultimately...

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

2003-01-01T23:59:59.000Z

28

Corporate Energy Management Process  

E-Print Network [OSTI]

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

Geiger, T.

2013-01-01T23:59:59.000Z

29

Sandia Corporation  

Office of Environmental Management (EM)

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

30

IT Capital Planning Corporate Management Improvement Program (CMIP)  

Broader source: Energy.gov [DOE]

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

31

Corporate Governance and Taxation  

E-Print Network [OSTI]

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

Dyck, Alexander

2004-01-01T23:59:59.000Z

32

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

E-Print Network [OSTI]

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

Stout, Lynn A.

2005-01-01T23:59:59.000Z

33

The Farm and Ranch Corporation.  

E-Print Network [OSTI]

rooc - ~ TA245.7 1873 0.1302 The Texas A&M University System Texas Agricultural Extension Service 8-1302 Director Daniel C. Pfannstiel College Station, Texas 77843 The Farm and Ranch Corporation Farm and Ranch Busin 0 nization... in Texas CONTENTS Alternative Forms of Business Organization. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .. 3 Closely Held Farm Corporations. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . .. 4...

Brints, Norman; Sartin, Marvin

1980-01-01T23:59:59.000Z

34

Corporate and personal responsibility  

SciTech Connect (OSTI)

Socioeconomic aspects of global climate change are discussed in this paper. Behavioral dimensions are discussed, with a focus on individual and collective value systems. It is suggested that traditional values are not adequate for addressing the climate change issue. Social aspects of the corporate role in climatic change are also briefly discussed.

Jemieson, D. [Univ. of Colorado, Boulder, CO (United States)

1992-12-31T23:59:59.000Z

35

Redshift and Energy Conservation  

E-Print Network [OSTI]

It has always been considered a serious error to treat the cosmological redshift as a Doppler velocity effect rather than the result of space expansion. It is demonstrated here that in practical terms this is not the case, and that the apparent distance - redshift relation derived from a Doppler interpretation is reasonably consistent with supernova data (though not as good as the standard model with dark energy). The normal Doppler effect is examined in detail and shown to conserve energy as expected. Because of the equivalence between the general relativistic space expansion paradigm and the Doppler effect (as demonstrated) the long-standing problem of energy loss associated with the expansion of the Universe is treated in a similar manner to the normal well-behaved Doppler effect. The mechanism by which energy is conserved with the normal Doppler shift is applied to the cosmological redshift and the energy violation disappears. However, an additional luminosity-dependent recession factor is introduced. The effect on astronomical objects is examined and it is found to add only a small additional redshift to a body generating power by nuclear means but can be very large for objects powered by gravity. A possible connection to the claimed anomalous redshift of quasars is considered.

Alasdair Macleod

2004-08-06T23:59:59.000Z

36

Introduction to Exide Corporations`s high temperature metals recovery system  

SciTech Connect (OSTI)

Environmental strategies concerning the processing and ultimate fate of wastes and byproducts are of ever increasing importance to the public and business sectors in the world today. Recycling materials and reusing energy from wastes and byproducts results in a reduction of environmental impacts and the cost of disposal. These are the key steps in reaching the ultimate goal of waste minimization. In response to these needs, Exide Corporation, in its vision to develop waste minimization programs, has developed the Exide High Temperature Metals Recovery (EHTMR) process. This process can treat a variety of wastes and byproducts where metals contents are an issue, recover the metal values for reuse, and produce a metals-depleted slag that can be marketable under the most stringent proposed EPA regulations for leachability of contaminants. The central feature of the EHTMR process is the exposure of treated materials to a transferred arc plasma generated in an electric furnace. The process achieves a reduction in costs and liability by recovering portions of a waste that can be recycled or reclaimed and produces a slag that has beneficial use to society.

Rozelle, P.L.; Baranski, J.P.; Bitler, J.A. [Exide Corp., Reading, PA (United States)

1995-12-31T23:59:59.000Z

37

Power Reliability at BASF Corporation  

E-Print Network [OSTI]

Power Reliability at BASF Corporation Thomas R. Theising Energy Systems Manager BASF Corporation ABSTRACT: Quality is defined not as what the supplier puts into the product but what the customer gets out and is willing to pay for. Power... of overcoming these problems. The approach of addressing the reliability of its utility systems is common within BASF. This paper will address one of BASF?s approaches to addressing Power Reliability. PROBLEM RECOGNITION: The first issue to address...

Theising, T. R.

2011-01-01T23:59:59.000Z

38

Power Reliability at BASF Corporation  

E-Print Network [OSTI]

Power Reliability at BASF Corporation Thomas R. Theising Energy Systems Manager BASF Corporation ABSTRACT: Quality is defined not as what the supplier puts into the product but what the customer gets out and is willing to pay for. Power... of overcoming these problems. The approach of addressing the reliability of its utility systems is common within BASF. This paper will address one of BASF?s approaches to addressing Power Reliability. PROBLEM RECOGNITION: The first issue to address...

Theising, T. R.

2012-01-01T23:59:59.000Z

39

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

E-Print Network [OSTI]

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

40

Corporate Profitability and Corporate Longevity  

E-Print Network [OSTI]

49 2 4 6 2.9 Energy Program E 20 32.6 8 1.7 4 8 4 (2.3) F 5 8.1 4 2.4 6 12 (2) (36) G 10 16.3 8 49 6 12 2 (1.1) H 10 16.3 4 0.9 2 4 2 (1.1) With Malar Energy Program E F G H 20 5 10 10 20.0 5.0 10.0 10.0 8 4 8 4 8.0 4...CORPORATE PROFITABILITY AND CORPORATE LONGEVITY Joel S. Gilbert, P.E. Mechanical Technology Incorporated Latham, New York ABSTRACT Many firms have discovered in the last few represents 9 to 12% of the cost of their goods 10 years...

Gilbert, J. S.

1983-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "redshift systems corporation" 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

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

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

and winter and summer forecasts; monitors the bulk power systems; and educates, trains, and certifies industry personnel. North American Electric Reliability Corporation...

42

Galaxy Redshifts: Improved Techniques  

E-Print Network [OSTI]

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

A. F. Heavens

1993-05-26T23:59:59.000Z

43

Law and Corporate Governance  

E-Print Network [OSTI]

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

Fligstein, Neil; Choo, Jennifer

2005-01-01T23:59:59.000Z

44

Industrial Analytics Corporation  

SciTech Connect (OSTI)

The lost foam casting process is sensitive to the properties of the EPS patterns used for the casting operation. In this project Industrial Analytics Corporation (IAC) has developed a new low voltage x-ray instrument for x-ray radiography of very low mass EPS patterns. IAC has also developed a transmitted visible light method for characterizing the properties of EPS patterns. The systems developed are also applicable to other low density materials including graphite foams.

Industrial Analytics Corporation

2004-01-30T23:59:59.000Z

45

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

E-Print Network [OSTI]

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

Voisey, Christopher John

2007-01-01T23:59:59.000Z

46

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

E-Print Network [OSTI]

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

Roth, George

2008-08-11T23:59:59.000Z

47

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

E-Print Network [OSTI]

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

McCalley, James D.

48

On the gravitational redshift  

E-Print Network [OSTI]

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

Klaus Wilhelm; Bhola N. Dwivedi

2014-04-16T23:59:59.000Z

49

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

SciTech Connect (OSTI)

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

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

1995-12-01T23:59:59.000Z

50

FIRST DETECTION OF THE [O III] 88 {mu}m LINE AT HIGH REDSHIFTS: CHARACTERIZING THE STARBURST AND NARROW-LINE REGIONS IN EXTREME LUMINOSITY SYSTEMS  

SciTech Connect (OSTI)

We have made the first detections of the 88 {mu}m [O III] line from galaxies in the early universe, detecting the line from the lensed active galactic nucleus (AGN)/starburst composite systems APM 08279+5255 at z = 3.911 and SMM J02399-0136 at z = 2.8076. The line is exceptionally bright from both systems, with apparent (lensed) luminosities {approx}10{sup 11} L {sub sun}. For APM 08279, the [O III] line flux can be modeled in a star formation paradigm, with the stellar radiation field dominated by stars with effective temperatures, T {sub eff} > 36,000 K, similar to the starburst found in M82. The model implies {approx}35% of the total far-IR luminosity of the system is generated by the starburst, with the remainder arising from dust heated by the AGN. The 88 {mu}m line can also be generated in the narrow-line region of the AGN if gas densities are around a few 1000 cm{sup -3}. For SMM J02399, the [O III] line likely arises from H II regions formed by hot (T {sub eff} > 40,000 K) young stars in a massive starburst that dominates the far-IR luminosity of the system. The present work demonstrates the utility of the [O III] line for characterizing starbursts and AGN within galaxies in the early universe. These are the first detections of this astrophysically important line from galaxies beyond a redshift of 0.05.

Ferkinhoff, C.; Hailey-Dunsheath, S.; Nikola, T.; Parshley, S. C.; Stacey, G. J. [Department of Astronomy, Cornell University, Ithaca, NY 14853 (United States); Benford, D. J.; Staguhn, J. G., E-mail: cferkinh@astro.cornell.ed, E-mail: steve@mpe.mpg.d [Observational Cosmology Laboratory (Code 665), NASA Goddard Space Flight Center, Greenbelt, MD 20771 (United States)

2010-05-01T23:59:59.000Z

51

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

Broader source: Energy.gov [DOE]

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

52

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

E-Print Network [OSTI]

system that would reduce energy consumption of an electrical power company in Tokyo. Employees of Sumitomo 3M Limited developed a way of using 3MTM Fluorinert? Liquid as a cooling medium to make slush ice during the night for use in cooling...

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

53

Element Abundances at High Redshifts  

E-Print Network [OSTI]

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

Max Pettini

1999-02-11T23:59:59.000Z

54

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

SciTech Connect (OSTI)

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

Hadley, Mark D.; Clements, Samuel L.

2009-01-01T23:59:59.000Z

55

Dust and Molecules at High Redshift  

E-Print Network [OSTI]

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

F. Combes

1998-12-23T23:59:59.000Z

56

THE CONTENT OF CORPORATE FEDERALISM  

E-Print Network [OSTI]

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

Bratton, William W.

2004-01-01T23:59:59.000Z

57

Corporate Board Meeting Minutes  

Office of Environmental Management (EM)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "of Energy Power Systems EngineeringDepartmentSmart GridThird Quarter OverallDepartmentSpaceDebateCorporate

58

Corporate sustainability assessment methodology  

E-Print Network [OSTI]

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

Pinchuk, Natallia

2011-01-01T23:59:59.000Z

59

Yubing Wang EMC Corporation  

E-Print Network [OSTI]

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

Claypool, Mark

60

Our Corporate Residents...  

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

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

Note: This page contains sample records for the topic "redshift systems corporation" 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

Corporate/Foundation Relations CORPORATE AND FOUNDATION RELATIONS The Offices of Corporate and  

E-Print Network [OSTI]

Corporate/Foundation Relations - 1 - CORPORATE AND FOUNDATION RELATIONS The Offices of Corporate and Foundation Relations (CR, FR) are responsible for coordinating with OSP on applications to key University development and institutional advancement prospects. Applying to Foundations or Corporations. Faculty

Mather, Patrick T.

62

Southwest Gas Corporation- Combined Heat and Power Program  

Broader source: Energy.gov [DOE]

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

63

Galactosynthesis Predictions at High Redshift  

E-Print Network [OSTI]

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

Ari Buchalter; Raul Jimenez; Marc Kamionkowski

2001-02-02T23:59:59.000Z

64

Limited Liability Companies and Corporate Business Structures  

E-Print Network [OSTI]

This publication describes limited liability companies and corporate forms of business organization, including S-Corporations and C-Corporations....

Thompson, Bill; Polk, Wade; Hayenga, Wayne

2009-01-07T23:59:59.000Z

65

PHOTOMETRIC REDSHIFTS OF SUBMILLIMETER GALAXIES  

SciTech Connect (OSTI)

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

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

2013-08-20T23:59:59.000Z

66

Corporate Headquarters 317 Route 104  

E-Print Network [OSTI]

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

Firestone, Jeremy

67

Corporate Information & Computing Services  

E-Print Network [OSTI]

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

Martin, Stephen John

68

Corporate and Business Plan  

E-Print Network [OSTI]

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

69

Smith & Franklin Academic Publishing Corporation  

E-Print Network [OSTI]

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

Tong, Liang

70

Rutgers Business School Corporate Finance  

E-Print Network [OSTI]

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

Lin, Xiaodong

71

Corporate Operating Experience Program  

Broader source: Energy.gov [DOE]

The DOE Corporate Operating Experience Program helps to prevent the recurrence of significant adverse events/trends by sharing performance information, lessons learned and good practices across the DOE complex.

72

Old Galaxies at High Redshift  

E-Print Network [OSTI]

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

James Dunlop

1997-05-13T23:59:59.000Z

73

The Galaxy Structure-Redshift Relationship  

E-Print Network [OSTI]

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

Christopher Conselice

2004-07-21T23:59:59.000Z

74

Quality Assurance Corporate Board | Department of Energy  

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

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

75

Corporate Law's Current-Owner Bias  

E-Print Network [OSTI]

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

Fried, Jesse M.

2005-01-01T23:59:59.000Z

76

Corporate Law's Current-Owner Bias  

E-Print Network [OSTI]

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

Fried, Jesse M.

2006-01-01T23:59:59.000Z

77

Corporate Governance, the Environment, and the Internet  

E-Print Network [OSTI]

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

Andrew, Jane

2003-01-01T23:59:59.000Z

78

Lesson from Fiascos in Russian Corporate Governance  

E-Print Network [OSTI]

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

Fox, Merritt; Heller, Michael

2000-01-01T23:59:59.000Z

79

Lesson from Fiascos in Russian Corporate Governance  

E-Print Network [OSTI]

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

Fox, Merritt B.; Heller, Michael A.

1999-01-01T23:59:59.000Z

80

Capital Structure Implications for Corporate Governance  

E-Print Network [OSTI]

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

Rajan, Nishanth

2012-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "redshift systems corporation" 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

HIGH-REDSHIFT METALS. II. PROBING REIONIZATION GALAXIES WITH LOW-IONIZATION ABSORPTION LINES AT REDSHIFT SIX  

SciTech Connect (OSTI)

We present a survey for low-ionization metal absorption line systems toward 17 QSOs at redshifts z{sub em} = 5.8-6.4. Nine of our objects were observed at high resolution with either Keck/HIRES or Magellan/MIKE, and the remainder at moderate resolution with Keck/ESI. The survey spans 5.3 < z{sub abs} < 6.4 and has a path length interval {Delta}X = 39.5 or {Delta}z = 8.0. In total we detect ten systems, five of which are new discoveries. The line-of-sight number density, l(X) = 0.25{sup +0.21}{sub -0.13} (95% confidence), is consistent with the combined number density at z {approx} 3 of damped Ly{alpha} systems (DLAs) and sub-DLAs, which comprise the main population of low-ionization systems at lower redshifts. This apparent lack of evolution may occur because low-ionization systems are hosted by lower-mass halos at higher redshifts, or because the mean cross section of low-ionization gas at a given halo mass increases with redshift due to the higher densities and lower ionizing background. The roughly constant number density notably contrasts with the sharp decline at z > 5.3 in the number density of highly ionized systems traced by C IV. The low-ionization systems at z {approx} 6 span a similar range of velocity widths as lower-redshift sub-DLAs but have significantly weaker lines at a given width. This may imply that the mass-metallicity relation of the host galaxies evolves toward lower metallicities at higher redshifts. These systems lack strong Si IV and C IV, which are common among lower-redshift DLAs and sub-DLAs. This is consistent, however, with a similar decrease in the metallicity of the low- and high-ionization phases, and does not necessarily indicate a lack of nearby, highly ionized gas. The high number density of low-ionization systems at z {approx} 6 suggests that we may be detecting galaxies below the current limits of i-dropout and Ly{alpha} emission galaxy surveys. These systems may therefore be the first direct probes of the 'typical' galaxies responsible for hydrogen reionization.

Becker, George D.; Calverley, Alexander P. [Kavli Institute for Cosmology and Institute of Astronomy, Madingley Road, Cambridge, CB3 0HA (United Kingdom); Sargent, Wallace L. W. [Palomar Observatory, California Institute of Technology, Pasadena, CA 91125 (United States); Rauch, Michael, E-mail: gdb@ast.cam.ac.uk, E-mail: acalver@ast.cam.ac.uk, E-mail: wws@astro.caltech.edu, E-mail: mr@obs.carnegiescience.edu [Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101 (United States)

2011-07-10T23:59:59.000Z

82

Atomic and Molecular Absorption at High Redshift  

E-Print Network [OSTI]

Strong constraints on possible variations in fundamental constants can be derived from HI 21-cm and molecular rotational absorption lines observed towards quasars. With the aim of forming a statistical sample of constraints we have begun a program of systematic searches for such absorption systems. Here we describe molecular rotational searches in 25 damped Lyman-alpha systems where, in many cases, we set optical depth limits an order of magnitude better than that required to detect the 4 known redshifted millimeter-wave absorbers. We also discuss the contributory factors in the detectability of HI 21-cm absorption, focusing on possible biases (e.g.low covering factors) in the currently known sample of absorbers and non-detections.

S. J. Curran; J. K. Webb; M. T. Murphy; Y. M. Pihlström

2004-05-14T23:59:59.000Z

83

Amphenol Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address: 160 East 300Algoil JumpAltergy SystemsAmericanAmphenol Corporation Jump to: navigation,

84

Redshift of photons penetrating a hot plasma  

E-Print Network [OSTI]

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

Ari Brynjolfsson

2005-10-07T23:59:59.000Z

85

The Earth Institute I Corporate Circle Spring 2011  

E-Print Network [OSTI]

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

Khatiwala, Samar

86

A New Loss Control Management System; Assimilating Loss Control Methodology in Reducing the Overall Quality Losses in XYZ Chemical Corporation  

E-Print Network [OSTI]

that has occurred in recent past. While the quality management system that is in place at XYZ monitors and improves the overall quality of the products, it does not capture the quality losses as it should. Quality losses occur due to human error...

Shaikh, Sameer

2011-05-20T23:59:59.000Z

87

Corporate governance and insider trading  

E-Print Network [OSTI]

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

Rozanov, Konstantin A

2008-01-01T23:59:59.000Z

88

Corporate governance and banking regulation  

E-Print Network [OSTI]

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

Alexander, Kern

89

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

E-Print Network [OSTI]

is in the process of implementing an enterprise-wide automated Energy Information and Utility Monitoring System (UMS). New Horizon Technologies and eComponents Technology have teamed to provide an integrated solution that will ultimately include all... (UMS) installed, energy and water consumption data along with local weather data are automatically summarized in the web reports. Hotels without the UMS enter monthly utility and weather data manually at the website. The hotels also enter certain...

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

2005-01-01T23:59:59.000Z

90

North American Electric Reliability Corporation Interconnections...  

Office of Environmental Management (EM)

North American Electric Reliability Corporation Interconnections North American Electric Reliability Corporation Interconnections Map of the North American Electric Reliability...

91

Forestry Commission England Corporate Plan  

E-Print Network [OSTI]

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

92

Press Release Corporate Communications  

E-Print Network [OSTI]

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

Haller-Dintelmann, Robert

93

CORPORATIONS APAC Tennessee Incorporated  

E-Print Network [OSTI]

Services Deal Cooper Holton PLLC Design Details A.C.A.P. - The Care Foundation Devault Interactive Deweese of Jacksonville Inc. FedEx Corporation First South Financial Credit Union First Tennessee Bank First Tennessee and Music Publishing LLC Macmillan Subscription Services Magnolia Processing Inc Mr. Chris Marable Marsh

Dasgupta, Dipankar

94

Constraints of Dark Energy at High Redshift  

E-Print Network [OSTI]

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

Qiping Su; Rong-Gen Cai

2014-08-24T23:59:59.000Z

95

RVSAO 2.0: Digital Redshifts and Radial Velocities  

E-Print Network [OSTI]

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

Michael J. Kurtz; Douglas J. Mink

1998-03-25T23:59:59.000Z

96

Measuring Galaxy Environments with Deep Redshift Surveys  

E-Print Network [OSTI]

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

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

2005-06-21T23:59:59.000Z

97

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

E-Print Network [OSTI]

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

Shishido, Zenichi

1999-01-01T23:59:59.000Z

98

Optical Approach to Gravitational Redshift  

E-Print Network [OSTI]

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

Y. G. Yi

2012-04-12T23:59:59.000Z

99

Benchmarking Corporate Energy Management  

E-Print Network [OSTI]

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

Norland, D. L.

100

Corporate Headquarters Cisco Systems, Inc.  

E-Print Network [OSTI]

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

Brody, James P.

Note: This page contains sample records for the topic "redshift systems corporation" 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

Aeronautics Test Program (ATP) Corporate Management of Aeronautical Facilities  

E-Print Network [OSTI]

Aeronautics Test Program (ATP) Corporate Management of Aeronautical Facilities 44th AIAA Aerospace Propulsion Systems Lab. 3 & 4 · Glenn 10x10 Supersonic Tunnel ATP provides 60%- 75% of fixed costs #12

102

Surface brightness in plasma-redshift cosmology  

E-Print Network [OSTI]

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

Ari Brynjolfsson

2006-05-31T23:59:59.000Z

103

Redshift indicators for gamma-ray bursts  

E-Print Network [OSTI]

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

J-L. Atteia

2005-05-04T23:59:59.000Z

104

Observed Cosmological Redshifts Support Contracting Accelerating Universe  

E-Print Network [OSTI]

The main argument that Universe is currently expanding is observed redshift increase by distance. However, this conclusion may not be correct, because cosmological redshift depends only on the scaling factors, the change in the size of the universe during the time of light propagation and is not related to the speed of observer or speed of the object emitting the light. An observer in expanding universe will measure the same redshift as observer in contracting universe with the same scaling. This was not taken into account in analysing the SN Ia data related to the universe acceleration. Possibility that universe may contract, but that the observed light is cosmologically redshifted allows for completely different set of cosmological parameters $\\Omega_M, \\Omega_{\\Lambda}$, including the solution $\\Omega_M=1, \\Omega_{\\Lambda}=0$. The contracting and in the same time accelerating universe explains observed deceleration and acceleration in SN Ia data, but also gives significantly larger value for the age of the universe, $t_0 = 24$ Gyr. This allows to reconsider classical cosmological models with $\\Lambda =0$. The contracting stage also may explain the observed association of high redshifted quasars to low redshifted galaxies.

Branislav Vlahovic

2012-07-02T23:59:59.000Z

105

Radio Observations of High Redshift Radio Galaxies  

E-Print Network [OSTI]

We review some aspects of radio continuum polarimetric imaging of high redshift radio galaxies. The correlation between extreme values of Faraday rotation observed toward radio emitting structures in nearby radio galaxies, and X-ray emitting cluster atmospheres, is presented as a method for targeting objects at high redshift for deep X-ray searches. We present an X-ray detection of the extreme rotation measure radio galaxy PKS 1138-262 at z = 2.156, and we argue that the X-ray emission is from a cluster atmosphere with a luminosity of 1.7x10^{44} h^{-2} ergs sec^{-1}. We also present results on the correlation between size and redshift for a sample of ultra-luminous radio galaxies between 0 < z < 4.3. Source sizes decrease systematically with redshift, suggesting either denser environments, or younger sources, at high redshift. An alternative explanation is significant inverse Compton losses off the microwave background at high redshift.

C. L. Carilli; H. J. A. Rottgering; G. K. Miley L. Pentericci; D. E. Harris

1998-02-18T23:59:59.000Z

106

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

E-Print Network [OSTI]

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

Capozziello, Salvatore; Saridakis, Emmanuel N

2015-01-01T23:59:59.000Z

107

Corporate and Foundation Proposal Checklist  

E-Print Network [OSTI]

Corporate and Foundation Proposal Checklist For additional information or assistance, please contact the MSU Foundation Office of Corporate and Foundation Relations at 994-2522 MSU Mission Statement MSU Foundation Mission Statement Needs Statement States the need using hard-core statistics

Dyer, Bill

108

A survey for redshifted molecular and atomic absorption lines I  

E-Print Network [OSTI]

We are currently undertaking a large survey for redshifted atomic and molecular absorption ... only one clear and one tentative detection were obtained: HI absorption at z = 0.097 in PKS 1555-140 and OH absorption at z =0.126 in PKS 2300-189, respectively... In order to determine why no clear molecular absorption was detected in any of the 13 sources searched, we investigate the properties of the five redshifted systems currently known to exhibit OH absorption. In four of these, molecules were first detected via millimetre-wave transitions and the flat radio spectra indicate compact background continuum sources, which may suggest a high degree of coverage of the background source by the molecular clouds in the absorber. Furthermore, for these systems we find a relationship between the molecular line strength and red optical--near infrared (V-K) colours, thus supporting the notion that the reddening of these sources is due to dust, which provides an environment conducive to the formation of molecules. Upon comparison with the V-K colours of our sample, this relationship suggests that, presuming the reddening occurs at the host galaxy redshift at least in some of the targets, many of our observations still fall short of the sensitivityrequired to detect OH absorption, although a confirmation of the ``detection'' of OH in 2300-189 could contravene this.

S. J. Curran; M. T. Whiting; M. T. Murphy; J. K. Webb; S. N. Longmore; Y. M. Pihlstroem; R. Athreya; C. Blake

2006-07-26T23:59:59.000Z

109

High redshift star-forming galaxies in absorption and emission  

E-Print Network [OSTI]

-forming galaxies in the redshift range 1 emission filling of absorption lines which has implications...

Quider, Anna Marie

2011-07-12T23:59:59.000Z

110

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

E-Print Network [OSTI]

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

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

2005-02-25T23:59:59.000Z

111

Siemens Pittsburgh, PA Novelis Corporation Atlanta, GA  

E-Print Network [OSTI]

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

McGaughey, Alan

112

Cosmic Streaming Field at Low Redshift  

E-Print Network [OSTI]

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

Lifan Wang

2007-05-04T23:59:59.000Z

113

CMB and Molecules at High Redshift  

E-Print Network [OSTI]

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

F. Combes

1999-01-17T23:59:59.000Z

114

Atom Interferometers and the Gravitational Redshift  

E-Print Network [OSTI]

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

Supurna Sinha; Joseph Samuel

2011-05-16T23:59:59.000Z

115

THE PRISM MULTI-OBJECT SURVEY (PRIMUS). II. DATA REDUCTION AND REDSHIFT FITTING  

SciTech Connect (OSTI)

The PRIsm MUlti-object Survey (PRIMUS) is a spectroscopic galaxy redshift survey to z {approx} 1 completed with a low-dispersion prism and slitmasks allowing for simultaneous observations of {approx}2500 objects over 0.18 deg{sup 2}. The final PRIMUS catalog includes {approx}130,000 robust redshifts over 9.1 deg{sup 2}. In this paper, we summarize the PRIMUS observational strategy and present the data reduction details used to measure redshifts, redshift precision, and survey completeness. The survey motivation, observational techniques, fields, target selection, slitmask design, and observations are presented in Coil et al. Comparisons to existing higher-resolution spectroscopic measurements show a typical precision of {sigma}{sub z}/(1 + z) = 0.005. PRIMUS, both in area and number of redshifts, is the largest faint galaxy redshift survey completed to date and is allowing for precise measurements of the relationship between active galactic nuclei and their hosts, the effects of environment on galaxy evolution, and the build up of galactic systems over the latter half of cosmic history.

Cool, Richard J. [MMT Observatory, Tucson, AZ 85721 (United States); Moustakas, John [Department of Physics, Siena College, 515 Loudon Rd., Loudonville, NY 12211 (United States); Blanton, Michael R.; Hogg, David W. [Center for Cosmology and Particle Physics, Department of Physics, New York University, 4 Washington Place, New York, NY 10003 (United States); Burles, Scott M. [D.E. Shaw and Co. L.P, 20400 Stevens Creek Blvd., Suite 850, Cupertino, CA 95014 (United States); Coil, Alison L.; Aird, James; Mendez, Alexander J. [Department of Physics, Center for Astrophysics and Space Sciences, University of California, 9500 Gilman Dr., La Jolla, San Diego, CA 92093 (United States); Eisenstein, Daniel J. [Harvard-Smithsonian Center for Astrophysics, 60 Garden St, MS 20, Cambridge, MA 02138 (United States); Wong, Kenneth C. [Steward Observatory, The University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721 (United States); Zhu, Guangtun [Center for Astrophysical Sciences, Department of Physics and Astronomy, Johns Hopkins University, 3400 North Charles Street, Baltimore, MD 21218 (United States); Bernstein, Rebecca A. [Department of Astronomy and Astrophysics, UCA/Lick Observatory, University of California, 1156 High Street, Santa Cruz, CA 95064 (United States); Bolton, Adam S. [Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112 (United States)

2013-04-20T23:59:59.000Z

116

Hindawi Publishing Corporation PPAR Research  

E-Print Network [OSTI]

Hindawi Publishing Corporation PPAR Research Volume 2006, Article ID 27489, Pages 1­9 DOI 10 these two phenotypes and makes them inseparable [2, 3]. According to the shared precursor hypoth- esis

Abraham, Nader G.

117

Corporate Jobs Tax Credit (Louisiana)  

Broader source: Energy.gov [DOE]

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

118

Sustainable Building Tax Credit (Corporate)  

Broader source: Energy.gov [DOE]

SB 463, enacted in April 2007, established a personal tax credit and a corporate tax credit for sustainable buildings in New Mexico. The tax credits apply to both commercial and residential...

119

Incorporation of PCI flow measurement/control at AK Steel Corporation  

SciTech Connect (OSTI)

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

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

1994-12-31T23:59:59.000Z

120

Tax aspects of collapsible corporations  

E-Print Network [OSTI]

TAX ASPECTS OF COLLAPSIBLE CORPORATIONS A Thesis By HERMAN AUGUST LEHMANN Submitted to the Graduate School of the Agricultural and 14 echanical College of Texas in partial fulfillment of the requirements for the degree of MASTER OF BUSINESS... his sincere appreciation for the guidance and assistance rendered by Professor Thomas Vi'. Leland in the preparation of this thesis. TABLE OF CONTENTS Chapter Page I. INTRODUCTION II. PROBLEMS RELATING TO COLLAPSIBLE CORPORATIONS Definition...

Lehmann, Herman August

2012-06-07T23:59:59.000Z

Note: This page contains sample records for the topic "redshift systems corporation" 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

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

E-Print Network [OSTI]

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

Ari Brynjolfsson

2004-12-02T23:59:59.000Z

122

Plasma Redshift, Time Dilation, and Supernovas Ia  

E-Print Network [OSTI]

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

Ari Brynjolfsson

2004-07-20T23:59:59.000Z

123

High redshift Gamma-Ray Bursts  

E-Print Network [OSTI]

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

Salvaterra, R

2015-01-01T23:59:59.000Z

124

abolishes corporate income: Topics by E-print Network  

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

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

125

abolishing corporate income: Topics by E-print Network  

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

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

126

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

E-Print Network [OSTI]

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

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

2001-01-01T23:59:59.000Z

127

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

E-Print Network [OSTI]

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

Rasmussen, Robert K.

2004-01-01T23:59:59.000Z

128

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

E-Print Network [OSTI]

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

Ehrlich, Craig; Kang, Dae-Seob

2000-01-01T23:59:59.000Z

129

Corporate Social Responsibility as a Conflict Between Owners  

E-Print Network [OSTI]

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

Rubin, Amir

2005-01-01T23:59:59.000Z

130

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

E-Print Network [OSTI]

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

Kaplan, Steve

2007-01-01T23:59:59.000Z

131

Choice as Regulatory Reform: The Case of Japanese Corporate Governance  

E-Print Network [OSTI]

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

Milhaupt, Curtis

2004-01-01T23:59:59.000Z

132

Nuclear Safety Enforcement Letter issued to Sandia Corporation...  

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

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

133

Karnataka Power Corporation Limited and National Thermal Power...  

Open Energy Info (EERE)

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

134

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

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

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

135

The 2dF Galaxy Redshift Survey: Spectra and redshifts  

E-Print Network [OSTI]

The 2dF Galaxy Redshift Survey (2dFGRS) is designed to measure redshifts for approximately 250000 galaxies. This paper describes the survey design, the spectroscopic observations, the redshift measurements and the survey database. The 2dFGRS uses the 2dF multi-fibre spectrograph on the Anglo-Australian Telescope, which is capable of observing 400 objects simultaneously over a 2-degree diameter field. The source catalogue for the survey is a revised and extended version of the APM galaxy catalogue, and the targets are galaxies with extinction-corrected magnitudes brighter than b_J=19.45. The main survey regions are two declination strips, one in the southern Galactic hemisphere spanning 80deg x 15deg around the SGP, and the other in the northern Galactic hemisphere spanning 75deg x 10deg along the celestial equator; in addition, there are 99 fields spread over the southern Galactic cap. The survey covers 2000 sq.deg and has a median depth of z=0.11. Adaptive tiling is used to give a highly uniform sampling rate of 93% over the whole survey region. Redshifts are measured from spectra covering 3600A-8000A at a two-pixel resolution of 9.0A and a median S/N of 13 per pixel. All redshift identifications are visually checked and assigned a quality parameter Q in the range 1-5; Q>=3 redshifts are 98.4% reliable and have an rms uncertainty of 85 km/s. The overall redshift completeness for Q>=3 redshifts is 91.8%, but this varies with magnitude from 99% for the brightest galaxies to 90% for objects at the survey limit. The 2dFGRS database is available on the WWW at http://www.mso.anu.edu.au/2dFGRS

Matthew Colless; G. B. Dalton; S. J. Maddox; W. J. Sutherland; P. Norberg; S. Cole; J. Bland-Hawthorn; T. J. Bridges; R. D. Cannon; C. A. Collins; W. J Couch; N. G. J. Cross; K. Deeley; R. DePropris; S. P. Driver; G. Efstathiou; R. S. Ellis; C. S. Frenk; K. Glazebrook; C. A. Jackson; O. Lahav; I. J. Lewis; S. L. Lumsden; D. S. Madgwick; J. A. Peacock; B. A. Peterson; I. A. Price; M. Seaborne; K. Taylor

2001-12-10T23:59:59.000Z

136

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

E-Print Network [OSTI]

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

Ari Brynjolfsson

2006-02-22T23:59:59.000Z

137

REDSHIFT CATALOG FOR SWIFT LONG GAMMA-RAY BURSTS  

SciTech Connect (OSTI)

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

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

2011-04-20T23:59:59.000Z

138

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

E-Print Network [OSTI]

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

139

Development of the SEA Corporation Powergrid{trademark} photovoltaic concentrator  

SciTech Connect (OSTI)

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

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

1998-03-01T23:59:59.000Z

140

Galaxy Bulges at Mid and High-Redshift  

E-Print Network [OSTI]

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

Christopher J. Conselice

2007-09-28T23:59:59.000Z

Note: This page contains sample records for the topic "redshift systems corporation" 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

POPULATION III STARS AND REMNANTS IN HIGH-REDSHIFT GALAXIES  

SciTech Connect (OSTI)

Recent simulations of Population III star formation have suggested that some fraction form in binary systems, in addition to having a characteristic mass of tens of solar masses. The deaths of metal-free stars result in the initial chemical enrichment of the universe and the production of the first stellar-mass black holes. Here we present a cosmological adaptive mesh refinement simulation of an overdense region that forms a few 10{sup 9} M{sub Sun} dark matter halos and over 13,000 Population III stars by redshift 15. We find that most halos do not form Population III stars until they reach M{sub vir} {approx} 10{sup 7} M{sub Sun} because this biased region is quickly enriched from both Population III and galaxies, which also produce high levels of ultraviolet radiation that suppress H{sub 2} formation. Nevertheless, Population III stars continue to form, albeit in more massive halos, at a rate of {approx}10{sup -4} M{sub Sun} yr{sup -1} Mpc{sup -3} at redshift 15. The most massive starless halo has a mass of 7 Multiplication-Sign 10{sup 7} M{sub Sun }, which could host massive black hole formation through the direct gaseous collapse scenario. We show that the multiplicity of the Population III remnants grows with halo mass above 10{sup 8} M{sub Sun }, culminating in 50 remnants located in 10{sup 9} M{sub Sun} halos on average. This has implications that high-mass X-ray binaries and intermediate-mass black holes that originate from metal-free stars may be abundant in high-redshift galaxies.

Xu Hao; Norman, Michael L. [Center for Astrophysics and Space Sciences, University of California, San Diego, 9500 Gilman Drive, La Jolla, CA 92093 (United States); Wise, John H., E-mail: hxu@ucsd.edu, E-mail: mlnorman@ucsd.edu, E-mail: jwise@gatech.edu [Center for Relativistic Astrophysics, School of Physics, Georgia Institute of Technology, 837 State Street, Atlanta, GA 30332 (United States)

2013-08-20T23:59:59.000Z

142

Matching Gift Companies LEHIGH UNIVERSITY 1 3M Corporation  

E-Print Network [OSTI]

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

Gilchrist, James F.

143

The Market for Borrowing Corporate Bonds  

E-Print Network [OSTI]

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

Asquith, Paul

144

Corporate governance : the case for Asian REITs  

E-Print Network [OSTI]

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

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

2009-01-01T23:59:59.000Z

145

Corporate Headquarters Tax Credit (West Virginia)  

Broader source: Energy.gov [DOE]

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

146

CORPORATE SUSTAINABILITY, STRATEGY AND ACCOUNTING CONTROLS: AN  

E-Print Network [OSTI]

PRACTICES Nathalie CRUTZEN, Dr, Assistant Professor, Accenture Chair in Sustainable Strategy, HEC support the implementation of a sustainability strategy in practice. With reference to Malmi and Brown 1 CORPORATE SUSTAINABILITY, STRATEGY AND ACCOUNTING CONTROLS: AN EXPLORATION OF CORPORATE

Boyer, Edmond

147

Corporate decision analysis : an engineering approach  

E-Print Network [OSTI]

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

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

2006-01-01T23:59:59.000Z

148

Redshift Distortions as a Probe of Gravity  

E-Print Network [OSTI]

Redshift distortion measurements from galaxy surveys include sensitivity to the gravitational growth index distinguishing other theories from Einstein gravity. This gravitational sensitivity is substantially free from uncertainty in the effective equation of state of the cosmic expansion history. We also illustrate the bias in the traditional application to matter density determination using f=Omega_m(a)^{0.6}, and how to avoid it.

Eric V. Linder

2007-09-07T23:59:59.000Z

149

Redshifts of the Long Gamma-Ray Bursts  

E-Print Network [OSTI]

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

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

2007-04-06T23:59:59.000Z

150

Chemical Elements at High and Low Redshifts  

E-Print Network [OSTI]

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

Max Pettini

2006-03-02T23:59:59.000Z

151

Corporate Productivity and I/S Investment  

E-Print Network [OSTI]

EG&G Inc. Enron Corp. Entergy Corporation Equitable LifeDuke Power Co. Enron Corp. Entergy Servies Florida Power &

Kraemer, Kenneth L.; Dunkle, Debbie

1997-01-01T23:59:59.000Z

152

Energy Conservation in China North Industries Corporation  

E-Print Network [OSTI]

ENERGY CONSERVATION IN CHINA NORTH INDUSTRIES CORPORATION Wang Tian You, Chen Hua De, Jing Xing Chu, Ling Rui Fu, China North Industries Corporation Beijing, People's Republic of China ABSTRACT This paper describes an overview of the energy... conservation in China North Industries Corporation. It shows how the corporation improves energy effi ciencies and how it changes constitution of fuel-- converting oil consumption to coal. Energy management organization, energy balance in plants...

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

153

Essays on the Market for Corporate Control  

E-Print Network [OSTI]

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

Kim, Hyunjung

2011-02-22T23:59:59.000Z

154

IBM Research Zurich 2010 IBM Corporation  

E-Print Network [OSTI]

&D Budget>6 B $ #12;ETH PolyVortrag 2010 Jana Koehler5 IBM Research ­ Zurich © 2010 IBM Corporation IBM - Zurich #12;ETH PolyVortrag 2010 Jana Koehler8 IBM Research ­ Zurich © 2010 IBM Corporation Math;ETH PolyVortrag 2010 Jana Koehler9 IBM Research ­ Zurich © 2010 IBM Corporation Selected Projects #12

155

Corporate Partners with industry to  

E-Print Network [OSTI]

, and a place to search for solutions. Corporate Partner Induct SARL, a French company, sponsored several that meet your company's needs. UCR's College of Engineering ­ Center for Environmental Research'sorcenter'sAdvisoryCouncil · Namedgraduatefellowshipinareaofspecialinterest · Directconnectiontodepartment'sorcenter'sChairorDirector · Company

156

Corporate Security and Conflict Outcomes  

E-Print Network [OSTI]

..................................................................................................... 75 Competition in Security Contracting and Conflict Outcomes .................................. 80 Research Design ....................................................................................................... 88 Dependent Variable... ................................... 16 Table 2 Contracted Service Total by Corporate Structure ............................................... 42 Table 3 The Effects of Public and Individual Firms Operating in Iraq (Part A) .............. 54 Table 4 The Effects of Public...

Tkach, Benjamin K

2013-10-21T23:59:59.000Z

157

Hindawi Publishing Corporation Prostate Cancer  

E-Print Network [OSTI]

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

Ahn, Hongshik

158

Internship opportunity with URS Corporation  

E-Print Network [OSTI]

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

159

CORPORATE GOVERNANCE IN THE KINGDOM OF SAUDI ARABIA  

E-Print Network [OSTI]

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

Al-Zaid, Ahmad Abdulaziz

2012-12-31T23:59:59.000Z

160

JOHNR. SCHOTT Calspan Corporation  

E-Print Network [OSTI]

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

Salvaggio, Carl

Note: This page contains sample records for the topic "redshift systems corporation" 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

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

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

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

162

HI at a Redshift of Zero  

E-Print Network [OSTI]

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

Christopher M. Springob

2004-11-17T23:59:59.000Z

163

DOE Corporate Overview - 2012  

Office of Environmental Management (EM)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "of Energy Power Systems EngineeringDepartmentSmartDepartment of1 Ingrid A.C.ofCommentsCompletesU.S.

164

Carbon and Water Resource Management for Water Distribution Systems  

E-Print Network [OSTI]

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

Hendrickson, Thomas Peter

2013-01-01T23:59:59.000Z

165

BASF Corporate Energy Management Process  

E-Print Network [OSTI]

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

Geiger, T.

2014-01-01T23:59:59.000Z

166

Ampulse Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentrating SolarElectricEnergyCT Biomass Facility Jump to: navigation,Amherst,Ampulse Corporation

167

Ryokuseisha Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to: navigation, searchVirginiaRoosevelt GardensUK-basedRutherford isRyokuseisha Corporation

168

Itochu Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to:46 - 429 Throttled (botOpen Energy2005) | OpenIssaquenaItochu Corporation Jump to:

169

Redshift Limits of BL Lacertae Objects from Optical Spectroscopy  

E-Print Network [OSTI]

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

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

2007-11-13T23:59:59.000Z

170

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

E-Print Network [OSTI]

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

Roseme, Sam

2007-01-01T23:59:59.000Z

171

Redshift drift exploration for interacting dark energy  

E-Print Network [OSTI]

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

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

2015-01-01T23:59:59.000Z

172

Absorption features of high redshift galactic winds  

E-Print Network [OSTI]

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

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

2007-06-11T23:59:59.000Z

173

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

E-Print Network [OSTI]

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

Harper Ho, Virginia E.

2013-03-01T23:59:59.000Z

174

Corporations LEHIGH UNIVERSITY 1 Aesculap, Inc.  

E-Print Network [OSTI]

Corporations LEHIGH UNIVERSITY 1 Aesculap, Inc. Air Products Air Products Foundation Arcelor Smarter Fuel, Inc. Sodexo Stryker Orthopaedics Stupp Bros., Inc. Sugarbush Products, Inc. TD Bank Thomson

Napier, Terrence

175

Comments of North American Electric Reliability Corporation ...  

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

North American Electric Reliability Corporation (NERC) to DOE Smart Grid RFI: Addressing Policy and Logistical Challenges Comments of North American Electric Reliability...

176

Resources, real options, and corporate strategy  

E-Print Network [OSTI]

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

Bernardo, Antonio; Chowdhry, Bhagwan

1998-01-01T23:59:59.000Z

177

Hindawi Publishing Corporation Advances in Bioinformatics  

E-Print Network [OSTI]

Hindawi Publishing Corporation Advances in Bioinformatics Volume 2012, Article ID 582765, 12 pages- esis generation--all of these tasks require processing and summarizing large amounts of individual

Gent, Universiteit

178

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

Broader source: Energy.gov [DOE]

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

179

Gibson Electric Membership Corporation- Energy Efficiency Rebates  

Broader source: Energy.gov [DOE]

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

180

Angular Size-Redshift: Experiment and Calculation  

E-Print Network [OSTI]

In this paper the next attempt is made to clarify the nature of the Euclidean behavior of the boundary in the angular size-redshift cosmological test. It is shown experimentally that this can be explained by the selection determined by anisotropic morphology and anisotropic radiation of extended radio sources. A catalogue of extended radio sources with minimal flux densities of about 0.01 Jy at 1.4 GHz was compiled for conducting the test. Without the assumption of their size evolution, the agreement between the experiment and calculation was obtained both in the Lambda CDM model (Omega_m=0.27 , Omega_v=0.73.) and the Friedman model (Omega = 0.1 ).

Amirkhanyan, V R

2015-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "redshift systems corporation" 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

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

E-Print Network [OSTI]

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

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

2008-09-26T23:59:59.000Z

182

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

E-Print Network [OSTI]

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

183

Information GRID in the Corporate World Information GRID in the Corporate World  

E-Print Network [OSTI]

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

Paris-Sud XI, Université de

184

The Redshift Distribution of Flat-Spectrum Radio Sources  

E-Print Network [OSTI]

The redshift distribution of flat-spectrum radio sources with 5 GHz flux densities S>5 mJy is a key component in using current radio lens surveys to probe the cosmological model. We have constructed the first flat-spectrum radio sample in the flux density range 3-20 mJy. Our new sample has 33 sources; we have determined the redshifts of 14 of these (42% complete). The low mean redshift, ~0.75, of our faintest sample needs to be confirmed by further observations to improve the sample completeness. We also increased the redshift completeness of several surveys of brighter flat-spectrum sources. While the mean redshift, ~1.1 of flat-spectrum samples fainter than 1 Jy is nearly constant, the fraction of the sources identifiable as quasars steadily drops from ~80% to ~10% as the flux density of the sources decreases.

J. A. Munoz; E. E. Falco; C. S. Kochanek; J. Lehar; E. Mediavilla

2003-05-20T23:59:59.000Z

185

Earl Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump37. It is classified asThis article is a stub. You can helpEarl Corporation

186

Vairex Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address: 160 East 300 South Place: Salt Lake City, Utah Zip:Scale Solar IncVairex Corporation Jump

187

Sipex Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revisionEnvReviewNonInvasiveExplorationUT-g Grant ofRichardtonManagement, 2009) | Open EnergySCRSipex Corporation

188

Hygrogenics Corporation | Department of Energy  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE:Year in3.pdfEnergy Health andof EnergyHydrogen-Powered BusesHygrogenics Corporation

189

EXAR Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revision has beenFfe2fb55-352f-473b-a2dd-50ae8b27f0a6 No revision hasESE Alcohol Jump to:EXAR Corporation Jump to:

190

Tyntek Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to:Seadov Pty LtdSteen,LtdInformationTulsa,TuscarawasFallon | OpenTyntek Corporation Jump

191

Emcore Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump37. It is classifiedProject) | OpenTexas:CountyElyria, Ohio:Emcore Corporation

192

Etrion Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump37. It isInformationexplains a4 ClimateEtrion Corporation Jump to:

193

ISE Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revision hasInformation Earth's Heat Jump to:PhotonHolyName HousingIIIDrive LtdINDEX JumpISE Corporation Jump

194

IXYS Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revision hasInformation Earth's Heat Jump to:PhotonHolyName HousingIIIDrive LtdINDEX JumpISEIXYS Corporation

195

Kanematsu Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revision hasInformation Earth's Heat JumpInc Place: EdenOverviewKanematsu Corporation Jump to: navigation,

196

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

E-Print Network [OSTI]

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

Carniglia, Stephen Davis

2013-01-01T23:59:59.000Z

197

Measuring Efficiency in Corporate Law: The Role of Shareholder Primacy  

E-Print Network [OSTI]

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

Fisch, Jill

2004-01-01T23:59:59.000Z

198

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

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

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

199

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

SciTech Connect (OSTI)

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

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

2013-04-10T23:59:59.000Z

200

NEC Corporation Volkswagen Group of America  

E-Print Network [OSTI]

Dentsu-Aegis Network Ltd. Digital Garage Hisense Co. Ltd. Jaguar Land Rover LG Electronics, Inc Alexander W. Dreyfoos, Jr. Informatix, Inc. The LEGO Group Dorothy Lemelson LG Electronics, Inc. Master. Panasonic Corporation RECRUIT Samsung Electronics Co., Ltd. SingTel TCL Multimedia Toshiba Corporation

Note: This page contains sample records for the topic "redshift systems corporation" 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

Corporate Political Donations: Investment or Agency?  

E-Print Network [OSTI]

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

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

2012-04-01T23:59:59.000Z

202

Is Sustainability Attractive for Corporate Real Estate  

E-Print Network [OSTI]

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

Paris-Sud XI, Université de

203

QUESTIONING THE RELEVANCE OF CORPORATE SOCIAL PERFORMANCE  

E-Print Network [OSTI]

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

Paris-Sud XI, Université de

204

Corporate Training On-Site Online Global  

E-Print Network [OSTI]

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

Barrett, Jeffrey A.

205

Trony Solar Corporation formerly Shenzhen Trony Science Technology...  

Open Energy Info (EERE)

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

206

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

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

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

207

Comments of New England Electric Transmission Corporation on...  

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

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

208

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

Open Energy Info (EERE)

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

209

E-Print Network 3.0 - applications international corporation...  

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

3 Matching Gift Companies LEHIGH UNIVERSITY 1 3M Corporation Summary: -Plough Foundation Science Applications International Corporation (SAIC) Scripps Howard Foundation...

210

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

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

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

211

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

Office of Environmental Management (EM)

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

212

Corporate Human Resources Information Services (CHIRS) PIA, Office...  

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

Corporate Human Resources Information Services (CHIRS) PIA, Office of Human Capitol Management Corporate Human Resources Information Services (CHIRS) PIA, Office of Human Capitol...

213

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

E-Print Network [OSTI]

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

Paris-Sud XI, Université de

214

Discrete Intrinsic Redshifts from Quasars to Normal Galaxies  

E-Print Network [OSTI]

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

M. B. Bell

2002-11-05T23:59:59.000Z

215

The 2dF Galaxy Redshift Survey: the local E+A galaxy population  

E-Print Network [OSTI]

We select a sample of low-redshift (z ~ 0.1) E+A galaxies from the 2dF Galaxy Redshift Survey (2dFGRS). The spectra of these objects are defined by strong hydrogen Balmer absorption lines (H-delta, H-gamma, H-beta) combined with a lack of [OII] 3727A emission, together implying a recently-truncated burst of star formation. The E+A spectrum is thus a signpost to galaxies in the process of evolution. We quantify the local environments, clustering properties and luminosity function of the E+A galaxies. We find that the environments are consistent with the ensemble of 2dFGRS galaxies: low-redshift E+A systems are located predominantly in the field, existing as isolated objects or in poor groups. However, the luminosity distribution of galaxies selected using three Balmer absorption lines H-delta-gamma-beta appears more typical of ellipticals. Indeed, morphologically these galaxies are preferentially spheroidal (E/S0) systems. In a small but significant number we find evidence for recent major mergers, such as tidal tails. We infer that major mergers are one important formation mechanism for E+A galaxies, as suggested by previous studies. At low redshift the merger probability is high in the field and low in clusters, thus these recently-formed spheroidal systems do not follow the usual morphology-density relation for ellipticals. Regarding the selection of E+A galaxies: we find that basing the Balmer-line criterion solely on H-delta absorption leads to a significant sub-population of disk systems with detectable H-alpha emission. In these objects the [OII] emission is presumably either obscured by dust or present with a low signal-to-noise ratio, whilst the (H-gamma, H-beta) absorption features are subject to emission-filling.

Chris Blake; Michael Pracy; Warrick Couch; Kenji Bekki; Ian Lewis; Karl Glazebrook; Ivan Baldry; Carlton Baugh; Joss Bland-Hawthorn; Terry Bridges; Russell Cannon; Shaun Cole; Matthew Colless; Chris Collins; Gavin Dalton; Roberto De Propris; Simon Driver; George Efstathiou; Richard Ellis; Carlos Frenk; Carole Jackson; Ofer Lahav; Stuart Lumsden; Steve Maddox; Darren Madgwick; Peder Norberg; John Peacock; Bruce Peterson; Will Sutherland; Keith Taylor

2004-08-29T23:59:59.000Z

216

The Environment of Galaxies at Low Redshift  

E-Print Network [OSTI]

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

Nicolas B. Cowan; Zeljko Ivezic

2008-01-15T23:59:59.000Z

217

Corporate Information Systems | Department of Energy  

Energy Savers [EERE]

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious RankCombustion |Energy UsageAUDITVehiclesTankless orAChief MedicalDepartmentWorkingCooking Up

218

EcoSystem Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump37. It is classified asThisEcoGrid EU (Smart Grid Project)

219

Implementing a Corporate Energy Management System  

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

Results Worldwide Prevented the generation of 2.9 billion pounds of pollutants since 1975 with more than 7,400 3P projects. Cut volatile organic air emissions...

220

Corporate Systems Engineering | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentratingRenewable Solutions LLC Jump to:Information NewAdvisors Jump2007)

Note: This page contains sample records for the topic "redshift systems corporation" 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

Implementing a Corporate Energy Management System  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE:YearRound-UpHeatMulti-Dimensionalthe U.S. Department-2023Department of

222

Edenspace Systems Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump37. It is classified asThisEcoGrid EU (SmartEcovation IncNewEden, NewEdenspace

223

The Carnegie Supernova Project: The Low-Redshift Survey  

E-Print Network [OSTI]

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

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

2005-12-01T23:59:59.000Z

224

Neutral chlorine and molecular hydrogen at high redshift  

E-Print Network [OSTI]

Chlorine and molecular hydrogen are known to be tightly linked together in the cold phase of the local interstellar medium through rapid chemical reactions. We present here the first systematic study of this relation at high redshifts using H$_2$-bearing damped Ly$\\alpha$ systems (DLAs) detected along quasar lines of sight. Using high-resolution spectroscopic data from VLT/UVES and Keck/HIRES, we report the detection of Cl$\\,$I in 9 DLAs (including 5 new detections) out of 18 high-$z$ DLAs with $N($H$_2) \\ge 10^{17.3}\\,$cm$^{-2}$ (including a new H$_2$ detection at $z=3.09145$ towards J$\\,$2100$-$0641) and present upper limits for the remaining 9 systems. We find a $\\sim$5$\\,\\sigma$ correlation between $N$(Cl$\\,$I) and $N$(H$_2$) with only $\\sim$0.2$\\,$dex dispersion over the range 18.1$\\,<\\,$log$\\,N$(H$_2$)$\\,<\\,$20.1, thus probing column densities 10 times lower those seen towards nearby stars, roughly following the relation $N$(Cl$\\,$I$) \\approx 1.5\\times10^{-6} \\times N($H$_2)$. This relation betwee...

Balashev, S A; Klimenko, V V; Petitjean, P; Srianand, R; Ledoux, C; Ivanchik, A V; Varshalovich, D A

2015-01-01T23:59:59.000Z

225

Structure and kinematics of galaxy clusters I. The redshift catalogue  

E-Print Network [OSTI]

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

P. Stein

1996-01-12T23:59:59.000Z

226

A Multiple Network Approach to Corporate Governance  

E-Print Network [OSTI]

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

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

2014-01-01T23:59:59.000Z

227

The Hubble series: Convergence properties and redshift variables  

E-Print Network [OSTI]

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

Celine Cattoen; Matt Visser

2007-10-10T23:59:59.000Z

228

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

E-Print Network [OSTI]

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

Haardt, Francesco

2015-01-01T23:59:59.000Z

229

CORPORATE GOVERNANCE AND MANAGEMENT EARNINGS FORECAST  

E-Print Network [OSTI]

1 CORPORATE GOVERNANCE AND MANAGEMENT EARNINGS FORECAST QUALITY: EVIDENCE FROM FRENCH IPOS Anis attributes, ownership retained, auditor quality, and underwriter reputation and management earnings forecast quality measured by management earnings forecast accuracy and bias. Using 117 French IPOs, we find

Paris-Sud XI, Université de

230

Managing preventative maintenance activities at Intel Corporation  

E-Print Network [OSTI]

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

Fearing, Rebecca Cassler

2006-01-01T23:59:59.000Z

231

Selecting Financing Strategies to Overcome Corporate Barriers  

E-Print Network [OSTI]

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

Michaelson, M. L.

1984-01-01T23:59:59.000Z

232

Corporate Analysis of DOE Safety Performance  

Broader source: Energy.gov [DOE]

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

233

Renewable Energy Production Tax Credit (Corporate)  

Broader source: Energy.gov [DOE]

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

234

Bio-Heating Oil Tax Credit (Corporate)  

Broader source: Energy.gov [DOE]

Maryland allows individuals and corporations to take an income tax credit of $0.03/gallon for purchases of biodiesel used for space heating or water heating. The maximum credit is $500 per year. It...

235

3M's Corporate Approach to Energy Management  

E-Print Network [OSTI]

recognized as a corporate environmental management leader and continues to demonstrate such leadership via the company's participation in EPA's Climate Wise and its own internal programs such as Pollution Prevention Pays (3P). Pamela R. Bingham...

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

236

Law as Economy: Convention, Corporation, Currency  

E-Print Network [OSTI]

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

Barrett, Jeffrey A.

237

CORPORATE AND STRATEGIC PLANNING Faculty planning workbook  

E-Print Network [OSTI]

.............................................................................33 Staffing & workforce planningCORPORATE AND STRATEGIC PLANNING Faculty planning workbook Humanities, Law & Social Studies Outcomes from 2008/09 Confirmation of progress during 2009/10 Faculty planning for 2010/11 ­ 2012/13 #12

238

Alternative Energy Development Incentive (Corporate) (Utah)  

Broader source: Energy.gov [DOE]

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

239

Extremely metal-poor gas at a redshift of 7  

E-Print Network [OSTI]

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

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

2012-01-01T23:59:59.000Z

240

The redshifts of bright sub-mm sources  

E-Print Network [OSTI]

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

James S. Dunlop

2001-01-17T23:59:59.000Z

Note: This page contains sample records for the topic "redshift systems corporation" 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

CorporateTraining extension.uci.edu/corporate  

E-Print Network [OSTI]

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

Stanford, Kyle

242

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

E-Print Network [OSTI]

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

Cheffins, Brian R.

2002-01-01T23:59:59.000Z

243

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

E-Print Network [OSTI]

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

Cheffins, Brian

2002-01-01T23:59:59.000Z

244

Data augmentation for machine learning redshifts applied to SDSS galaxies  

E-Print Network [OSTI]

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

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

2015-01-01T23:59:59.000Z

245

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

E-Print Network [OSTI]

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

246

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

E-Print Network [OSTI]

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

von Nessen, Paul

2009-01-01T23:59:59.000Z

247

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

E-Print Network [OSTI]

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

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

2008-01-01T23:59:59.000Z

248

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

E-Print Network [OSTI]

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

Licht, Amir

2004-01-01T23:59:59.000Z

249

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

E-Print Network [OSTI]

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

Hermalin, Benjamin E.

2008-01-01T23:59:59.000Z

250

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

E-Print Network [OSTI]

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

Shishido, Zenichi

2004-01-01T23:59:59.000Z

251

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

E-Print Network [OSTI]

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

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

2008-01-01T23:59:59.000Z

252

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

E-Print Network [OSTI]

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

Kwon, Jae Yeol

2004-01-01T23:59:59.000Z

253

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

E-Print Network [OSTI]

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

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

2008-01-01T23:59:59.000Z

254

Radio-loud high-redshift protogalaxy candidates in Bootes  

E-Print Network [OSTI]

We used the Near Infrared Camera on Keck I to obtain Ks-band images of four candidate high-redshift radio galaxies selected using optical and radio data in the NOAO Deep Wide-Field Survey in Bootes. Our targets have 1.4 GHz radio flux densities greater than 1 mJy, but are undetected in the optical to fainter than 24 Vega mag. Spectral energy distribution fitting suggests that three of these objects are at z > 3, with radio luminosities near the FR-I / FR-II break. The other has photometric redshift 1.2, but may in fact be at higher redshift. Two of the four objects exhibit diffuse morphologies in Ks -band, suggesting that they are still in the process of forming.

Steve Croft; Wil van Breugel; Michael J. I. Brown; Wim de Vries; Arjun Dey; Peter Eisenhardt; Buell Jannuzi; Huub Röttgering; S. A. Stanford; Daniel Stern; S. P. Willner

2008-03-04T23:59:59.000Z

255

Ice emission and the redshifts of submillimeter sources  

E-Print Network [OSTI]

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

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

2008-02-12T23:59:59.000Z

256

The characteristic stellar mass as a function of redshift  

E-Print Network [OSTI]

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

Cathie J. Clarke; Volker Bromm

2003-05-11T23:59:59.000Z

257

Multi-object spectroscopy of low redshift EIS clusters. II  

E-Print Network [OSTI]

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

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

2003-08-01T23:59:59.000Z

258

Multi-object spectroscopy of low redshift EIS clusters. I  

E-Print Network [OSTI]

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

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

2002-04-23T23:59:59.000Z

259

Corporate Analysis of DOE Safety Performance | Department of Energy  

Office of Environmental Management (EM)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "of Energy Power Systems EngineeringDepartmentSmart GridThird Quarter OverallDepartmentSpaceDebateCorporate

260

Tax consequences of separating corporate businesses  

E-Print Network [OSTI]

Lips ARY g ~ggpgF ep &Ex' TAX CONSEQUENCES OP SEPARATING CORPORATE BUSINESSES A Thesis Gordon D. Zuber Submitted to the Graduate School of the Agricultural and lNechanical College of Texas in partial fulfillment of the requirements... for the Degree of MASTER OP BUSINESS ADl/iliVISTRAT ION August 1958 Ma)or Subject: Accounting TAX CONSEQUENCES OP SEPARATING CORPORATE BUSINESSES A Thesis Gordon D. Zuber Approved as to style and content by: Chairman of the Committee ead. o the Divas...

Zuber, Gordon Dewey

2012-06-07T23:59:59.000Z

Note: This page contains sample records for the topic "redshift systems corporation" 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

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

SciTech Connect (OSTI)

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

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

2012-02-10T23:59:59.000Z

262

Corporations LEHIGH UNIVERSITY 1 The Accenture Foundation, Inc.  

E-Print Network [OSTI]

Corporations LEHIGH UNIVERSITY 1 The Accenture Foundation, Inc. Air Products Air Products Foundation ArcelorMittal Atofina Chemicals Foundation B. Braun Medical, Inc. (BD) Becton, Dickinson Foundation, Inc. IBM Corporation Insaco, Inc. Just Born, Inc. Lutron Electronics Company, Inc. Lutron

Gilchrist, James F.

263

Corporate Energy Management: A Survey of Large Manufacturing Companies  

E-Print Network [OSTI]

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

Norland, D. L.; Lind, L.

264

Corporate Gray Military Officer Job Fair | Department of Energy  

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

Corporate Gray Military Officer Job Fair Corporate Gray Military Officer Job Fair September 11, 2014 8:00AM to 1:30PM EDT Location: 6715 Commerce Street, Springfield, VA 22150 POC:...

265

The Wolf effect and the redshift of quasars  

SciTech Connect (OSTI)

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

James, Daniel F.V.

1998-01-23T23:59:59.000Z

266

The Star Formation Rate-Density Relationship at Redshift Three  

E-Print Network [OSTI]

We study the star formation rate (SFR) as a function of environment for UV selected Lyman break galaxies (LBGs) at redshift three. From deep UBVI KPNO 4-m/MOSAIC images, covering a total of 0.90 deg^2, we select 334 LBGs in slices 100 Mpc (co-moving) deep spanning the redshift range 2.9projected density to the 5th nearest neighbor. These mock catalogs have a redshift depth of 100 Mpc, similar to our slice width. The large area of the MOSAIC images, 40x40 Mpc (co-moving) per field, allows us to measure the SFR from the dust-corrected UV continuum as a function of $\\Sigma_5$. In contrast to low-redshift galaxies, we find that the SFR (or UV luminosity) of LBGs at z=3 shows no detectable dependence on environment over 2 orders of magnitude in density. To test the significance of our result, we use Monte Carlo simulations (from the mock catalogs) and the same projected density estimators we applied to our data. We find that we can reject the steep z=0 SFR-density at the 5-$\\sigma$ level. We conclude that the SFR-density at z=3 must be at least 3.6 times flatter than it is locally, i.e. the SFR of LBGs is significantly less dependent on environment than the SFR of local star-forming galaxies. We find that the rest-frame UV colors are also independent of environment.

Nicolas Bouche; James D. Lowenthal

2005-03-04T23:59:59.000Z

267

The Age-Redshift Relation for Standard Cosmology  

E-Print Network [OSTI]

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

R. C. Thomas; R. Kantowski

2000-08-10T23:59:59.000Z

268

The Wolf effect and the Redshift of Quasars  

E-Print Network [OSTI]

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

Daniel F. V. James

1998-07-20T23:59:59.000Z

269

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

E-Print Network [OSTI]

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

Nugent, Peter

2005-01-01T23:59:59.000Z

270

Rutgers Business School Professor Simi Kedia Corporate Finance  

E-Print Network [OSTI]

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

Lin, Xiaodong

271

2011 Corporate Headquarters: An Analysis of Immediate Communities  

E-Print Network [OSTI]

While the Bay Area’s history has shaped today’s culture, there is little written about how corporations affect their immediate communities. This thesis focuses on the largest corporations in the Bay Area to determine if these corporations have any...

Conti, Serena Nicole

2013-04-25T23:59:59.000Z

272

Hindawi Publishing Corporation Comparative and Functional Genomics  

E-Print Network [OSTI]

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

Newcastle upon Tyne, University of

273

Hindawi Publishing Corporation Advances in Civil Engineering  

E-Print Network [OSTI]

Hindawi Publishing Corporation Advances in Civil Engineering Volume 2009, Article ID 353960, 10 and Josep Dolz3 1 Instituto de Ingenier´ia, UNAM, Ciudad Universitaria, Edificio 5, Cub. 403, 04510 M´exico, DF, Mexico 2 Facultad de Ingenier´ia, UNAM, Ciudad Universitaria, 04510 M´exico, DF, Mexico 3

Fernandez, Thomas

274

Senior projectS corporate Sponsored  

E-Print Network [OSTI]

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

Stuart, Josh

275

Hindawi Publishing Corporation International Journal of Hypertension  

E-Print Network [OSTI]

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

Gleeson, Joseph G.

276

Hindawi Publishing Corporation Journal of Nanotechnology  

E-Print Network [OSTI]

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

Wang, Yan Alexander

277

Researcher at Cerner Corporation Cerner Overview  

E-Print Network [OSTI]

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

Jornsten, Rebecka

278

A generalized simulation model for corporate planning  

E-Print Network [OSTI]

, Head of the Department of Industrial Engineering, at Texas ASM University, a" quoted by Hilton (24): "It /corporate pianning7 should serve as the roadmap of tomorrow. We see it as an azzalysis of all the activities that influ- ence ozr business...

Viswanathan, Krishnan

2012-06-07T23:59:59.000Z

279

Hindawi Publishing Corporation International Journal of Ecology  

E-Print Network [OSTI]

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

Rieseberg, Loren

280

URANIUM MILLING ACTIVITIES AT SEQUOYAH FUELS CORPORATION  

E-Print Network [OSTI]

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

unknown authors

Note: This page contains sample records for the topic "redshift systems corporation" 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

UNIVERSITY OF KENTUCKY AND AFFILIATED CORPORATIONS  

E-Print Network [OSTI]

UNIVERSITY OF KENTUCKY AND AFFILIATED CORPORATIONS ENDOWMENT INVESTMENT POLICY Amended January 30, 2014 University of Kentucky University of Kentucky Research Foundation The Fund for Advancement of Education and Research in the UK Medical Center University of Kentucky Mining Engineering Foundation, Inc

Hayes, Jane E.

282

Renewable Energy Tax Credit (Corporate)  

Broader source: Energy.gov [DOE]

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

283

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

E-Print Network [OSTI]

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

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

2006-07-21T23:59:59.000Z

284

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

E-Print Network [OSTI]

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

Cinabro, David

285

X-RAY ABSORPTION OF HIGH-REDSHIFT QUASARS  

SciTech Connect (OSTI)

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

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

2013-09-01T23:59:59.000Z

286

Exponential cosmological redshift in a linearly expanding universe  

E-Print Network [OSTI]

The first principles analysis of the radiation by an arbitrary source in a flat Friedmann-Robertson-Walker space-time is presented. The obtained analytical solution explicitly shows that the cosmological redshift is not of kinematic origin and that the source and the observer may be regarded as being at rest with respect to eachother at all times. At the same time the effect of the time-variation of the metric on the propagation of light appears to be underestimated in the standard cosmology. The cosmological redshift caused by the linear time-variation of the metric turns out to be an exponential rather than linear function of the well-defined spatial distance and the apparent brightness of the source contains an even stronger exponential decay factor.

Neil V. Budko

2009-07-03T23:59:59.000Z

287

Exponential cosmological redshift in a linearly expanding universe  

E-Print Network [OSTI]

Analytical solution of the Maxwell equations in a flat expanding Friedmann-Robertson-Walker space-time is presented. The solution is valid for arbitrary sources and for expansion rates described by positive functions of time. The near-, intermediate-, and far-field terms are explicitly identified. It is shown that the cosmological redshift introduced by a linearly expanding space-time is an exponential function of the distance factor.

Budko, Neil V

2009-01-01T23:59:59.000Z

288

A faint galaxy redshift survey behind massive clusters  

SciTech Connect (OSTI)

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

Frye, Brenda

1999-12-01T23:59:59.000Z

289

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

E-Print Network [OSTI]

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

C. Sivaram; Kenath Arun

2010-08-24T23:59:59.000Z

290

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

E-Print Network [OSTI]

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

T. Kiang

2003-08-01T23:59:59.000Z

291

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

E-Print Network [OSTI]

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

Fu-Gao Song

2012-06-24T23:59:59.000Z

292

Measuring redshift-space distortions with future SKA surveys  

E-Print Network [OSTI]

The peculiar motion of galaxies can be a particularly sensitive probe of gravitational collapse. As such, it can be used to measure the dynamics of dark matter and dark energy as well the nature of the gravitational laws at play on cosmological scales. Peculiar motions manifest themselves as an overall anisotropy in the measured clustering signal as a function of the angle to the line-of-sight, known as redshift-space distortion (RSD). Limiting factors in this measurement include our ability to model non-linear galaxy motions on small scales and the complexities of galaxy bias. The anisotropy in the measured clustering pattern in redshift-space is also driven by the unknown distance factors at the redshift in question, the Alcock-Paczynski distortion. This weakens growth rate measurements, but permits an extra geometric probe of the Hubble expansion rate. In this chapter we will briefly describe the scientific background to the RSD technique, and forecast the potential of the SKA phase 1 and the SKA2 to measure the growth rate using both galaxy catalogues and intensity mapping, assessing their competitiveness with current and future optical galaxy surveys.

Alvise Raccanelli; Philip Bull; Stefano Camera; David Bacon; Chris Blake; Olivier Dore; Pedro Ferreira; Roy Maartens; Mario Santos; Matteo Viel; Gong-bo Zhao

2015-01-15T23:59:59.000Z

293

Measuring redshift-space distortions with future SKA surveys  

E-Print Network [OSTI]

The peculiar motion of galaxies can be a particularly sensitive probe of gravitational collapse. As such, it can be used to measure the dynamics of dark matter and dark energy as well the nature of the gravitational laws at play on cosmological scales. Peculiar motions manifest themselves as an overall anisotropy in the measured clustering signal as a function of the angle to the line-of-sight, known as redshift-space distortion (RSD). Limiting factors in this measurement include our ability to model non-linear galaxy motions on small scales and the complexities of galaxy bias. The anisotropy in the measured clustering pattern in redshift-space is also driven by the unknown distance factors at the redshift in question, the Alcock-Paczynski distortion. This weakens growth rate measurements, but permits an extra geometric probe of the Hubble expansion rate. In this chapter we will briefly describe the scientific background to the RSD technique, and forecast the potential of the SKA phase 1 and the SKA2 to measu...

Raccanelli, Alvise; Camera, Stefano; Bacon, David; Blake, Chris; Dore, Olivier; Ferreira, Pedro; Maartens, Roy; Santos, Mario; Viel, Matteo; Zhao, Gong-bo

2015-01-01T23:59:59.000Z

294

Testing the Accuracy of Redshift Space Group Finding Algorithms  

E-Print Network [OSTI]

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

James J. Frederic

1994-09-07T23:59:59.000Z

295

People's Electric Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentrating Solar Powerstories onFocusOski Energy LLCPascoag UtilityPennsylvaniaPeopleCorporation

296

Jackson Purchase Energy Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentrating Solar Powerstories on climate compatibleInformation offApproachEnergy Corporation

297

Meridian Biorefining Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentrating Solar Powerstories on climateJunoMedanosElectric CoMeridian Biorefining Corporation

298

NanoPV Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to:46 -Energieprojekte3Informationof Energy Calculator29NanoPV Corporation Jump to:

299

Nanomaterials Discovery Corporation NDC | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to:46 -Energieprojekte3Informationof Energy Calculator29NanoPV Corporation

300

Cosmos Energy Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentratingRenewable Solutions LLC Jump to:Information NewAdvisorsCosmos Energy Corporation

Note: This page contains sample records for the topic "redshift systems corporation" 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

Miami Power Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to:46 -Energieprojekte GmbH Jump to: navigation,MetalysisMi GmbHMiami Power Corporation

302

PPP Equipment Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy ResourcesLoading map...(UtilityCounty,Orleans County,PPP Equipment Corporation Jump to: navigation,

303

Powder River Energy Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy ResourcesLoadingPenobscot County, Maine:Plug Power IncPowder River Energy Corporation Place: Sundance,

304

GainSpan Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentrating Solar Power Basics (TheEtelligenceGainSpan Corporation Jump to: navigation, search

305

Gateway Energy Services Corporation (Pennsylvania) | Open Energy  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentrating Solar Power Basics (TheEtelligenceGainSpan Corporation JumpGarkane Energy

306

Gateway Energy Services Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentrating Solar Power Basics (TheEtelligenceGainSpan Corporation JumpGarkane EnergyGateway

307

Catamount Resources Corporation CRC | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of Inspector GeneralDepartmentAUDIT REPORT Americium/CuriumSunways JVGroup India Jump to:Corporation CRC Jump

308

Outsourcing Ownership, Operation and Management of Industrial Facility Power Plants for the Purpose of Reducing Future Risk and Capital Requirements of the Corporation  

E-Print Network [OSTI]

For many industrial corporations, the availability of funds for maintaining and modernizing Central Utility systems is becoming more and more difficult to obtain. Total return on investments in facility infrastructure generally does not tend to meet...

Sebesta, J. J.; Schubbe, T.

309

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

E-Print Network [OSTI]

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

Harper Ho, Virginia E.

2010-01-01T23:59:59.000Z

310

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

E-Print Network [OSTI]

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

Zhang, Zhong

2011-01-01T23:59:59.000Z

311

Alternative Energy Projects by Rural Electric Membership Corporations (Indiana)  

Broader source: Energy.gov [DOE]

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

312

2008_Transition_Corporate_Overview_Book_One.pdf | Department...  

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

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

313

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

Open Energy Info (EERE)

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

314

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

Broader source: Energy.gov [DOE]

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

315

azure dynamics corporation: Topics by E-print Network  

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

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

316

Corn Belt Energy Corporation- Residential Energy Efficiency Rebate Program  

Broader source: Energy.gov [DOE]

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

317

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

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

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

318

Accounting for Taste: Board Member Preferences and Corporate Policy Choices  

E-Print Network [OSTI]

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

Richardson, Scott

2003-05-23T23:59:59.000Z

319

EERE Partner Testimonials- Robert Gleason, Capstone Turbine Corporation  

Broader source: Energy.gov [DOE]

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

320

EERE Partner Testimonials- Darren Jamison, Capstone Turbine Corporation  

Broader source: Energy.gov [DOE]

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

Note: This page contains sample records for the topic "redshift systems corporation" 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

Southwest Gas Corporation- Commercial Energy Efficient Equipment Rebate Program  

Broader source: Energy.gov [DOE]

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

322

Southwest Gas Corporation- Commercial High-Efficiency Equipment Rebate Program  

Broader source: Energy.gov [DOE]

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

323

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

Broader source: Energy.gov [DOE]

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

324

Gravitational red-shift and deflection of slow light  

E-Print Network [OSTI]

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

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

2008-10-27T23:59:59.000Z

325

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

E-Print Network [OSTI]

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

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

2015-01-01T23:59:59.000Z

326

Search for Redshifted 2.2 MeV Neutron Capture Line From A0535+262 in Outburst  

E-Print Network [OSTI]

The Be/X-ray binary system A0535+262 underwent a giant outburst in May-June 2005, followed by a dimmer outburst in August-September 2005. This increased intensity provided an opportunity to search for redshifted neutron-capture lines from the surface of the neutron star. If discovered, such lines would constrain the neutron star equation of state, providing the motivation of this search. The spectrometer (SPI) on board the INTEGRAL satellite observed the dimmer outburst and provided the data for this research. We have not detected a line with enough significance, with the width-dependent upper limits on the broadened and redshifted neutron capture line in the range of (2 - 11) x 10^(-4) photons cm^(-2) s^(-1). To our knowledge, these are the strongest upper limits on the redshifted 2.2 MeV emission from an accreting neutron star. Our analysis of the transparency of the neutron star surface for 2.2 MeV photons shows that photons have a small but finite chance of leaving the atmosphere unscattered, which diminishes the possibility of detection.

Sirin Caliskan; Emrah Kalemci; Matthew G. Baring; Steven E. Boggs; Peter Kretschmar

2008-12-15T23:59:59.000Z

327

Chapter 2Chapter 2 A Complete CorporateA Complete Corporate  

E-Print Network [OSTI]

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

Schubart, Christoph

328

Corporate Fellows Council | ornl.gov  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May JunDatastreamsmmcrcalgovInstrumentsruc DocumentationP-Series to User GroupInformationE-GovNatural Gas Usage FormCorporate Fellows

329

Lithium Technology Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revision hasInformation Earth's Heat JumpInc Place:KeystoneSolarList ofPassiveMachineBalance JumpCorporation

330

Corporate International Operations | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address: 160Benin:EnergyWisconsin:2003) |Cordova Electric Coop, IncKilauea Name: Corporate

331

Diversified Energy Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump to:52c8ff988c1Dering Harbor,DiscountDiversified Energy Corporation Jump to:

332

Workplace Charging Challenge Partner: Sears Holdings Corporation |  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "ofEarlyEnergyDepartment ofDepartment of EnergyofDepartment of Energy Sears Holdings Corporation

333

Applied Films Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address: 160 East 300AlgoilEnergy Information the Army Permit:Films Corporation Jump to:

334

HydroChina Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of Inspector GeneralDepartmentAUDIT REPORTOpen EnergyBoard"Starting a new pageHuadeHydroChina Corporation

335

Schering Plough Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revisionEnvReviewNonInvasiveExplorationUT-g Grant ofRichardton AbbeyA Jump to:Schering Plough Corporation Jump to:

336

Sound Geothermal Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to:Seadov Pty Ltd Jump to:InformationSolergyAddison,Souderton,Geothermal Corporation Jump

337

Vu1 Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address: 160 East 300 South Place: Salt Lake City,Division of OilGuyane Jump to:Vu1 Corporation

338

Jupiter Oxygen Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to:46 - 429 Throttled (botOpen6 Climate ZoneJeromeCounty isJupiter Oxygen Corporation

339

Verenium Corporation (Massachusetts) | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of InspectorConcentrating SolarElectric Coop,Save Energy NowNew HampshireValero RefiningCorporation

340

Bhoruka Power Corporation Ltd | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Office of Inspector GeneralDepartmentAUDIT REPORT Americium/CuriumSunways JV Jump to:Bhoruka Power Corporation Ltd Jump

Note: This page contains sample records for the topic "redshift systems corporation" 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

StarSolar Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to:Seadov Pty Ltd JumpGTZHolland,0162112°,St.Stanly County, NorthStarSolar Corporation Jump

342

SunPower Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to:Seadov Pty LtdSteen, Minnesota:36052°, -97.6114217°SunEnergy Power CorpSunOneCorporation

343

Technology Ventures Corporation TVC | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia:FAQ < RAPID Jump to:Seadov Pty LtdSteen,Ltd Jump to:Taos County, NewTechnologiekontor BremerhavenCorporation

344

Empire Natural Gas Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump37. It is classifiedProject) |Emeryville,Empire Natural Gas Corporation Place:

345

EnerVault Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address:011-DNA Jump37. It is classifiedProject)EnerVault Corporation Jump to: navigation, search

346

IST Energy Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 No revision hasInformation Earth's Heat Jump to:PhotonHolyName HousingIIIDrive LtdINDEX JumpISE CorporationIST

347

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

E-Print Network [OSTI]

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

Goldhaber, G.

2008-01-01T23:59:59.000Z

348

A WFC3 Grism Emission Line Redshift Catalog in the GOODS-South Field  

E-Print Network [OSTI]

We combine HST/WFC3 imaging and G141 grism observations from the CANDELS and 3D-HST surveys to produce a catalog of grism spectroscopic redshifts for galaxies in the CANDELS/GOODS-South field. The WFC3/G141 grism spectra cover a wavelength range of 1.1 0.6. The resulting spectra are visually inspected to identify emission lines and redshifts are determined using cross-correlation with empirical spectral templates. To establish the accuracy of our redshifts, we compare our results against high-quality spectroscopic redshifts from the literature. Using a sample of 411 control galaxies, this analysis yields a precision of sigma_NMAD=0.0028 for the grism-derived redshifts, which is consistent with the accuracy reported by the 3D-HST team. Our final catalog covers an area of 153 square arcmin and contains 1019 redshifts for galaxies in GOODS-S. Roughly 60% (608/1019) of these redshifts are for galaxies with no previously published spectroscopic redshift. These new redshifts span a range of 0.677 1.5. In addition, ...

Morris, Aaron M; Trump, Jonathan R; Weiner, Benjamin J; Hathi, Nimish P; Barro, Guillermo; Dahlen, Tomas; Faber, Sandra M; Finkelstein, Steven L; Fontana, Adriano; Ferguson, Henry C; Grogin, Norman A; Grützbauch, Ruth; Guo, Yicheng; Hsu, Li-Ting; Koekemoer, Anton M; Koo, David C; Mobasher, Bahram; Pforr, Janine; Salvato, Mara; Wiklind, Tommy; Wuyts, Stijn

2015-01-01T23:59:59.000Z

349

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

SciTech Connect (OSTI)

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

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

2013-07-20T23:59:59.000Z

350

The inferred redshift distribution of the faint blue excess  

E-Print Network [OSTI]

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

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

1996-01-01T23:59:59.000Z

351

The inferred redshift distribution of the faint blue excess  

E-Print Network [OSTI]

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

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

1996-05-10T23:59:59.000Z

352

The SDSS Coadd: A Galaxy Photometric Redshift Catalog  

SciTech Connect (OSTI)

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

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

2011-11-01T23:59:59.000Z

353

Accessing the population of high redshift Gamma Ray Bursts  

E-Print Network [OSTI]

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

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

2015-01-01T23:59:59.000Z

354

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

E-Print Network [OSTI]

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

Bainbridge, Stephen M

2003-01-01T23:59:59.000Z

355

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

E-Print Network [OSTI]

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

Stout, Lynn A.

2003-01-01T23:59:59.000Z

356

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

E-Print Network [OSTI]

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

Bank, Steven A.

2013-01-01T23:59:59.000Z

357

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

E-Print Network [OSTI]

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

California at Berkeley, University of

358

Social Impact Management Plans: Innovation in corporate and public policy  

SciTech Connect (OSTI)

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

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

2013-11-15T23:59:59.000Z

359

Copyright 1997 by Rational Software Corporation Analysis and Design  

E-Print Network [OSTI]

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

Mylopoulos, John

360

Industrial Engineering 361 Six Sigma Making Corporations and  

E-Print Network [OSTI]

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

Vardeman, Stephen B.

Note: This page contains sample records for the topic "redshift systems corporation" 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

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

E-Print Network [OSTI]

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

Sobhan, Md. Abdus

2014-07-02T23:59:59.000Z

362

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

E-Print Network [OSTI]

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

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

2011-01-01T23:59:59.000Z

363

Fuel-Flexible Microturbine and Gasifier System for Combined Heat...  

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

Flexible Microturbine and Gasifier System for Combined Heat and Power Fuel-Flexible Microturbine and Gasifier System for Combined Heat and Power Capstone Turbine Corporation, in...

364

Comprehensive Renewable Energy Feasibility Study for Sealaska Corporation  

SciTech Connect (OSTI)

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

Robert Lynette; John Wade: Larry Coupe

2006-06-30T23:59:59.000Z

365

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

E-Print Network [OSTI]

change to the corporate name during a CNC related to a change in corporate image? Third, what is the effect of a non-brand name altering CNC versus a brand name altering CNC on a firm’s stock price? This dissertation makes its primary contribution...

DeFanti, Mark P.

2009-06-02T23:59:59.000Z

366

Main Sequence Masses and Radii from Gravitational Redshifts  

E-Print Network [OSTI]

Modern instrumentation makes it possible to measure the mass to radius ratio for main sequence stars in open clusters from gravitational redshifts. For stars where independent information is available for either the mass or the radius, this application of general relativity directly determines the other quantity. Applicable examples are: 1) measuring the radii of solar metallicity main sequence stars for which the mass - luminosity relation is well known, 2) measuring the radii for stars where model atmospheres can be used to determine the surface gravity (the mass to radius squared ratio), 3) refining the mass - radius relation for main sequence stars, and 4) measuring the change in radius as stars evolve off the main sequence and up the giant branch.

Ted von Hippel

1995-12-02T23:59:59.000Z

367

Weighing black holes from zero to high redshift  

E-Print Network [OSTI]

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

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

2008-09-02T23:59:59.000Z

368

Distance-redshift relations in an anisotropic cosmological model  

SciTech Connect (OSTI)

In this paper we study an anisotropic model generated from a particular Bianchi type-III metric, which is a generalization of Gödel's metric and an exact solution of Einstein's field equations. We analyse type Ia supernova data, namely the SDSS sample calibrated with the MLCS2k2 fitter, and we verify in which ranges of distances and redshifts the anisotropy could be observed. We also consider, in a joint analysis, the position of the first peak in the CMB anisotropy spectrum, as well as current observational constraints on the Hubble constant. We conclude that a small anisotropy is permitted by the data, and that more accurate measurements of supernova distances above z = 2 might indicate the existence of such anisotropy in the universe.

Menezes, R. S. Jr. [Instituto Federal da Bahia, Salvador, BA (Brazil); Pigozzo, C.; Carneiro, S., E-mail: rsmjr@ifba.edu.br, E-mail: cpigozzo@ufba.br, E-mail: saulo.carneiro.ufba@gmail.com [Instituto de Física, Universidade Federal da Bahia, Salvador, Bahia (Brazil)

2013-03-01T23:59:59.000Z

369

A Group of Galaxies at Redshift 2.38  

E-Print Network [OSTI]

We report the discovery of a group of galaxies at redshift 2.38. We imaged about 10% of a claimed supercluster of QSO absorption-lines at z=2.38 (Francis & Hewett 1993). In this small field (2 arcmin radius) we detect two Ly-alpha emitting galaxies. The discovery of two such galaxies in our tiny field supports Francis & Hewett's interpretation of the absorption-line supercluster as a high redshift "Great Wall". One of the Ly-alpha galaxies lies 22 arcsec from a background QSO, and may be associated with a multi-component Ly-alpha absorption complex seen in the QSO spectrum. This galaxy has an extended (50kpc) lumpy Ly-alpha morphology, surrounding a compact IR-bright nucleus. The nucleus shows a pronounced break in its optical-UV colors at about 4000 A (rest-frame), consistent with a stellar population of mass about 7E11 solar masses, an age of more than 500 Myr, and little on-going star-formation. C IV emission is detected, suggesting that a concealed AGN is present. Extended H-alpha emission is also detected; the ratio of Ly-alpha flux to H-alpha is abnormally low (about 0.7), probable evidence for extended dust. This galaxy is surrounded by a number of very red (B-K>5) objects, some of which have colors suggesting that they too are at z=2.38. We hypothesize that this galaxy, its neighbors and a surrounding lumpy gas cloud may be a giant elliptical galaxy in the act of bottom-up formation.

Paul Francis; Bruce Woodgate; Steve Warren; Palle Moller; Marg Mazzolini; Andy Bunker; James Lowenthal; Ted Williams; Takeo Minezaki; Yukiyasu Kobayashi; Yuzuru Yoshii

1995-11-10T23:59:59.000Z

370

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

SciTech Connect (OSTI)

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

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

2013-11-10T23:59:59.000Z

371

The Apm Galaxy Survey IV: Redshifts of Rich Clusters of Galaxies  

E-Print Network [OSTI]

We present redshifts for a sample of 229 clusters selected from the APM Galaxy Survey, 189 of which are new redshift determinations. Non-cluster galaxy redshifts have been rejected from this sample using a likelihood ratio test based on the projected and apparent magnitude distributions of the cluster fields. We test this technique using cluster fields in which redshifts have been measured for more than 10 galaxies. Our redshift sample is nearly complete and has been used in previous papers to study the three dimensional distribution of rich clusters of galaxies. 157 of the clusters in our sample are listed in the Abell catalogue or supplement, and the remainder are new cluster identifications.

G. B. Dalton; G. Efstathiou; S. J. Maddox; W. J. Sutherland

1993-11-16T23:59:59.000Z

372

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

E-Print Network [OSTI]

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

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

2010-06-11T23:59:59.000Z

373

Black hole mass estimates and emission line properties of a sample of redshift Z > 6:5 quasars  

E-Print Network [OSTI]

-ionization lines (e.g., C iv) because the latter can present high-velocity offsets with respect to the source systemic redshift (?v & 1000 km s?1, corresponding to ?z ? 0.02 at z ? 6, see, e.g., Richards et al. 2002, 2011; Shang et al. 2007, and references therein... that the abundance of nitrogen (N) relative to carbon, oxygen, and helium (C, O, and He) can be used as a crude marker of the degree of chemical enrichment of the BLR (e.g., Hamann et al. 2002). This is due to the fact that N is a second generation element, i...

De Rosa, Gisella; Venemans, Bram P.; Decarli, Roberto; Gennaro, Mario; Simcoe, Robert A.; Dietrich, Matthias; Peterson, Bradley M.; Walter, Fabian; Frank, Stephan; McMahon, Richard G.; Hewett, Paul C.; Mortlock, Daniel J.; Simpson, Chris

2014-07-09T23:59:59.000Z

374

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

E-Print Network [OSTI]

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

375

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

Broader source: Energy.gov [DOE]

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

376

A Red-Shifted, Fast-Relaxing Azobenzene Photoswitch for Visible Light Control of an Ionotropic Glutamate Receptor  

E-Print Network [OSTI]

A Red-Shifted, Fast-Relaxing Azobenzene Photoswitch for Visible Light Control of an Ionotropic cores with a red-shifted cis-to-trans isomerization have been previously described, they have not yet ligand (PTL) approach. We report the synthesis and characterization of a red-shifted PTL, L-MAG0460

Trauner, Dirk

377

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

E-Print Network [OSTI]

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

Sheppard, Scott S.

378

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

E-Print Network [OSTI]

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

Cheng, Betty H.C.

379

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

Broader source: Energy.gov [DOE]

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

380

Uncertain Growth Cycles, Corporate Investment, and Dynamic Hedging  

E-Print Network [OSTI]

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

Yonce, Adam

2010-01-01T23:59:59.000Z

Note: This page contains sample records for the topic "redshift systems corporation" 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

Essays on banking and corporate finance in developing countries  

E-Print Network [OSTI]

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

Gormley, Todd A

2006-01-01T23:59:59.000Z

382

THREE ESSAYS ON MONITORING OF FINANCIAL REPORTING BY CORPORATE DIRECTORS  

E-Print Network [OSTI]

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

Xu, Yang

2012-08-31T23:59:59.000Z

383

Corporate budgeting In practice : driving strategic focus and performance  

E-Print Network [OSTI]

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

Briggman, Chandra A. (Chandra Alisa)

2014-01-01T23:59:59.000Z

384

Creating an incentive for investor intermediaries to improve corporate governance  

E-Print Network [OSTI]

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

Gershkowitz, Todd M

2006-01-01T23:59:59.000Z

385

Corporate Governance & The UK Split Capital Investment Trust Crisis   

E-Print Network [OSTI]

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

Adams, Andrew T; Angus, Robin

2005-01-01T23:59:59.000Z

386

Board independence and corporate governance: evidence from director resignations  

E-Print Network [OSTI]

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

Gupta, Manu

2005-08-29T23:59:59.000Z

387

Corporate governance and long-term stock returns  

E-Print Network [OSTI]

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

Moorman, Theodore Clark

2005-08-29T23:59:59.000Z

388

STATEMENT OF CONSIDERATIONS REQUEST BY PARKER HANNIFIN CORPORATION...  

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

HANNIFIN CORPORATION FOR AN ADVANCE WAIVER OF PATENT RIGHTS TO INVENTIONS MADE UNDER COOPERATIVE AGREEMENT NO. DE-FC26-06NT42648; W(A)-06-033, CH-1391 As set out in the...

389

STATEMENT OF CONSIDERATIONS REQUEST BY GENERAL MOTORS CORPORATION...  

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

ADVANCE WAIVER OF DOMESTIC AND FOREIGN INVENTION RIGHTS UNDER DOE COOPERATIVE AGREEMENT NO. DE-FC26-04NT42278; W(A)-04-070, CH-1248 The Petitioner, General Motors Corporation (GM)...

390

How Well Do Social Ratings Actually Measure Corporate Social Responsibility?*  

E-Print Network [OSTI]

environmental strengths, in contrast, do not accurately predict pollution levels or compliance violations. Levine Haas School of Business University of California at Berkeley 545 Student Services Building #1900 Responsibility? Abstract: Ratings of corporations' environmental activities and capabilities influence billions

Sadoulet, Elisabeth

391

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

E-Print Network [OSTI]

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

392

Introduction: White-Collar and Corporate Crime in Asia  

E-Print Network [OSTI]

International Handbook of White-Collar and Corporate Crime.Japanese social structure and white collar crime: recruitG. (2007). Black Mist and White Collars: Economic Crime in

Pontell, Henry N.; Geis, Gilbert

2010-01-01T23:59:59.000Z

393

Corporate serial acquisitions: An empirical test of the learning hypothesis  

E-Print Network [OSTI]

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

Nesterov, Yurii

394

Fitting In: Extreme Corporate Wellness and Organizational Communication  

E-Print Network [OSTI]

, and (3) corporeal ethics. First, organizational culture, including espoused values and shared levels of assumptions, took on certain changes because of an emphasis on extreme fitness. Employee participation in CrossFit led to strict notions of strength...

James, Eric Preston

2014-07-31T23:59:59.000Z

395

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

E-Print Network [OSTI]

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

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

2015-01-01T23:59:59.000Z

396

Quantifying the Cosmic Web in the New Era of Redshift Surveys  

E-Print Network [OSTI]

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

Ofer Lahav

2004-11-03T23:59:59.000Z

397

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

E-Print Network [OSTI]

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

Neil Trentham

2004-11-18T23:59:59.000Z

398

Deuterium at High Redshifts: Recent Advances and Open Issues  

E-Print Network [OSTI]

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

Max Pettini

2006-01-19T23:59:59.000Z

399

Corporate governance under stress : an institutional perspective on the transformation of corporate governance in France and Germany  

E-Print Network [OSTI]

This work contributes to the study of comparative political economy by examining the impact of financial deregulation on corporate governance in the two main continental European economies, France and Germany. It investigates ...

Goyer, Michel, 1964-

2004-01-01T23:59:59.000Z

400

Preliminary survey report, Didier Taylor Refractories Corporation Plant, Newtown, Ohio  

SciTech Connect (OSTI)

An on-site visit was made to the Didier Taylor Refractories Corporation located in Newtown, Ohio for the purpose of evaluating control methods instituted to protect workers from hazardous conditions. Raw materials were received at this location in bags and canisters. The bags were opened in an area with dual-pull exhaust ventilation from two sides. Several St. Regis single spout packers with local exhaust systems were also used at this facility. All exhaust ducts connected to a large Kirk and Blum dry-bag collector located adjacent to the building. Some molding and casting work was done at this facility, but no particularly significant health hazard controls were noted for the process. The product line included bricks, patches, ramming mixes, cements, castables, plastics, and miscellaneous items. Plaster of paris and thermo setting plastics were used as mold materials. Slip mixes involved a wide range of chemical compounds. Plans were made to conduct a walk-through preliminary-type survey of the location at a later date. An in-depth assessment of portions of the facility and operations may be decided upon at that time.

Mahon, R.D.

1981-10-20T23:59:59.000Z

Note: This page contains sample records for the topic "redshift systems corporation" 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

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

E-Print Network [OSTI]

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

Garavini, G.; Supernova Cosmology Project

2008-01-01T23:59:59.000Z

402

Comment on "The Cosmic Time in Terms of the Redshift", by Carmeli et al  

E-Print Network [OSTI]

The time-redshift relation of Carmeli et al. differs from that of the standard flat LambdaCDM model by more than 500 million years for 1 < z < 4.5.

Alan Macdonald

2006-06-08T23:59:59.000Z

403

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

E-Print Network [OSTI]

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

Acquaviva, Viviana; Gawiser, Eric

2015-01-01T23:59:59.000Z

404

Probing the epoch of reionization with redshifted 21 cm HI emission  

E-Print Network [OSTI]

Emission and absorption features in the spectrum of the diffuse radio background below 200 MHz due to the 21 cm hyperfine transition line of neutral hydrogen gas in the high redshift intergalactic medium offer a new and ...

Bowman, Judd D. (Judd David)

2007-01-01T23:59:59.000Z

405

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

E-Print Network [OSTI]

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

Jones, Suzy F

2015-01-01T23:59:59.000Z

406

The Environments of Low and High Luminosity Radio Galaxies at Moderate Redshifts  

E-Print Network [OSTI]

In the local Universe, high-power radio galaxies live in lower density environments than low-luminosity radio galaxies. If this trend continues to higher redshifts, powerful radio galaxies would serve as efficient probes of moderate redshift groups and poor clusters. Photometric studies of radio galaxies at 0.3 environment correlation disappears at moderate redshifts, though this could be the result of foreground/background contamination affecting the photometric measures of environment. We have obtained multi-object spectroscopy of in the fields of 14 lower luminosity (L_1.4GHz 1.2x10^25 W/Hz) radio galaxies at z ~ 0.3 to spectroscopically investigate the link between the environment and the radio luminosity of radio galaxies at moderate redshifts. Our results support the photometric analyses; there does not appear to be a correlation between the luminosity of a radio galaxy and its environment at moderate redshifts. Hence, radio galaxies are not efficient signposts for group environments at moderate redshifts.

M. W. Auger; R. H. Becker; C. D. Fassnacht

2008-01-02T23:59:59.000Z

407

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

E-Print Network [OSTI]

Surface brightness is a fundamental observational parameter of galaxies. We show, for the first time in detail, how it can be used to obtain photometric redshifts for galaxies, the $\\mu$-PhotoZ method. We demonstrate that the Tolman surface brightness relation, $\\mu \\propto (1+z)^{-4}$, is a powerful tool for determining galaxy redshifts from photometric data. We develop a model using $\\mu$ and a color percentile (ranking) measure to demonstrate the $\\mu$-PhotoZ method. We apply our method to a set of galaxies from the SHELS survey, and demonstrate that the photometric redshift accuracy achieved using the surface brightness method alone is comparable with the best color-based methods. We show that the $\\mu$-PhotoZ method is very effective in determining the redshift for red galaxies using only two photometric bands. We discuss the properties of the small, skewed, non-gaussian component of the error distribution. We calibrate $\\mu_r, (r-i)$ from the SDSS to redshift, and tabulate the result, providing a simple, but accurate look up table to estimate the redshift of distant red galaxies.

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

2007-07-03T23:59:59.000Z

408

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

SciTech Connect (OSTI)

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

Pursimo, Tapio [Nordic Optical Telescope, Apartado 474, 38700 Santa Cruz de La Palma (Spain)] [Nordic Optical Telescope, Apartado 474, 38700 Santa Cruz de La Palma (Spain); Ojha, Roopesh [NVI Inc./U. S. Naval Observatory, 3450 Massachusetts Ave NW, Washington DC (United States)] [NVI Inc./U. S. Naval Observatory, 3450 Massachusetts Ave NW, Washington DC (United States); Jauncey, David L. [CSIRO Astronomy and Space Science and Mount Stromlo Observatory, Canberra ACT 0200 (Australia)] [CSIRO Astronomy and Space Science and Mount Stromlo Observatory, Canberra ACT 0200 (Australia); Rickett, Barney J. [Department of Electrical and Computer Engineering, University of California, San Diego, La Jolla, CA 92093 (United States)] [Department of Electrical and Computer Engineering, University of California, San Diego, La Jolla, CA 92093 (United States); Dutka, Michael S. [The Catholic University of America, 620 Michigan Ave., N.E., Washington DC 20064 (United States)] [The Catholic University of America, 620 Michigan Ave., N.E., Washington DC 20064 (United States); Koay, Jun Yi; Bignall, Hayley E.; Macquart, Jean-Pierre [ICRAR, Curtin University, Bentley, WA 6845 (Australia)] [ICRAR, Curtin University, Bentley, WA 6845 (Australia); Lovell, James E. J. [School of Mathematics and Physics, University of Tasmania, TAS 7001 (Australia)] [School of Mathematics and Physics, University of Tasmania, TAS 7001 (Australia); Kedziora-Chudczer, Lucyna, E-mail: tpursimo@not.iac.es [School of Physics and Astrophysics, UNSW, Sydney NSW 2052 (Australia)] [School of Physics and Astrophysics, UNSW, Sydney NSW 2052 (Australia)

2013-04-10T23:59:59.000Z

409

Radiative Feedback in Relic HII Regions at High-Redshift  

E-Print Network [OSTI]

UV radiation from early astrophysical sources could have a large impact on subsequent star formation in nearby protogalaxies. Here we study the radiative feedback from the first, short-lived stars using hydrodynamical simulations with transient UV backgrounds (UVBs) and persistent Lyman-Werner backgrounds (LWBs) of varying intensity. We extend our prior work in Mesinger et al. (2006), by studying a more typical region whose proto-galaxies form at lower redshifts, z~13-20, in the epoch likely preceding the bulk of reionization. We confirm our previous results that feedback in the relic HII regions resulting from such transient radiation, is itself transient. Feedback effects dwindle away after ~30% of the Hubble time, and the same critical specific intensity of J_UV~0.1 x 10^{-21} ergs/s/cm^2/Hz/sr separates positive and negative feedback regimes. Additionally, we discover a second episode of eventual positive feedback in halos which have not yet collapsed when their progenitor regions were exposed to the transient UVB. This eventual positive feedback appears in all runs, regardless of the strength of the UVB. However, this feedback regime is very sensitive to the presence of Lyman-Werner radiation, and notable effects disappear under fairly modest background intensities of J_LW>10^{-3} x 10^{-21} ergs/s/cm^2/Hz/sr. We conclude that UV radiative feedback in relic HII regions, although a complicated process, seems unlikely to have a major impact on the progress of cosmological reionization, provided that present estimates of the lifetime and luminosity of a PopIII star are accurate. More likely is that the build-up of the LWB ultimately governs the feedback strength until a persistent UV background can be established. [abridged

Andrei Mesinger; Greg L. Bryan; Zoltan Haiman

2009-09-13T23:59:59.000Z

410

Korea's Newly Enacted Unified Bankruptcy Act: The Role of the New Act in Facilitating (or Discouraging) the Transfer of Corporate Control  

E-Print Network [OSTI]

perspective of corporate governance, the decision whether toefforts to implement corporate governance reforms and otherthe weakness of the corporate governance mechanism in Korea,

Ko, Haksoo

2007-01-01T23:59:59.000Z

411

The Kast Ground Based UV Spectral Survey of 79 QSOs at Redshift 2 for Lyman Alpha Forest and Metal Absorption  

E-Print Network [OSTI]

We present a moderate resolution (~1.15 Angstroms/pixel) survey of 79 quasars obtained using the Kast spectrograph on the Shane 3m telescope at Lick observatory. The spectra span the wavelength range of 3175-5880 Angstroms, and have typical signal to noise of 6-20 in the regions of the spectra showing Lyman alpha forest absorption. The quasars have a mean emission redshift of z=2.17, and nearly all cover the entire Lyman alpha forest between Lyman alpha and Lyman beta. Although the quasars were selected to avoid BAL, two quasars in the survey are BAL, one of which is a new discovery. We list the HI and metal ions observed in a total of 140 absorption systems. We also identify 526 emission lines, and list their observed wavelengths, along with new redshifts of the quasars. We determine the rest wavelengths of 3 emission lines or line blends in the forest to be 1070.95 +/- 1.00, 1123.13 +/- 0.51, and 1175.88 +/- 0.30 Angstroms.

Tytler, D; Suzuki, N; Kirkman, D; Lubin, D; Orin, A; Tytler, David; Meara, John M. O'; Suzuki, Nao; Kirkman, David; Lubin, Dan; Orin, Adam

2004-01-01T23:59:59.000Z

412

The Kast Ground Based UV Spectral Survey of 79 QSOs at Redshift 2 for Lyman Alpha Forest and Metal Absorption  

E-Print Network [OSTI]

We present a moderate resolution (~1.15 Angstroms/pixel) survey of 79 quasars obtained using the Kast spectrograph on the Shane 3m telescope at Lick observatory. The spectra span the wavelength range of 3175-5880 Angstroms, and have typical signal to noise of 6-20 in the regions of the spectra showing Lyman alpha forest absorption. The quasars have a mean emission redshift of z=2.17, and nearly all cover the entire Lyman alpha forest between Lyman alpha and Lyman beta. Although the quasars were selected to avoid BAL, two quasars in the survey are BAL, one of which is a new discovery. We list the HI and metal ions observed in a total of 140 absorption systems. We also identify 526 emission lines, and list their observed wavelengths, along with new redshifts of the quasars. We determine the rest wavelengths of 3 emission lines or line blends in the forest to be 1070.95 +/- 1.00, 1123.13 +/- 0.51, and 1175.88 +/- 0.30 Angstroms.

David Tytler; John M. O'Meara; Nao Suzuki; David Kirkman; Dan Lubin; Adam Orin

2004-05-04T23:59:59.000Z

413

Hindawi Publishing Corporation EURASIP Journal on Embedded Systems  

E-Print Network [OSTI]

, 17 pages doi:10.1155/2009/758480 Research Article Time-Predictable Computer Architecture Martin solutions for a time-predictable computer architecture. The proposed architecture is evaluated Standard computer architecture is driven by the following paradigm: Make the common case fast

414

Covanta Energy Corporation formerly Ogden Martin Systems of Hillsborou...  

Open Energy Info (EERE)

Inc) Place: Fairfield, New Jersey Zip: 7004 Product: Owner and operator of modern waste-to-energy facilities (over 1GW). Coordinates: 47.38522, -117.171254 Show Map...

415

Implementing a Corporate Energy Management System | Department of Energy  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "ofEarly Career Scientists'Montana.ProgramJulietipDepartment of Energy

416

Covanta Energy Corporation formerly Ogden Martin Systems of Hillsborough  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address: 160Benin:EnergyWisconsin:2003) |Cordova Electric633211°,of ForestBabylon EnergyInc |

417

Optimizing Electric Motor Systems at a Corporate Campus Facility  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious RankCombustion | Department ofT ib l L d F SSales LLCDiesel Enginesthe U.S. -- An2008 |

418

Optimizing Electric Motor Systems at a Corporate Campus Facility |  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home Page on Delicious Rank EERE:Year in3.pdfEnergyDepartment ofOil's Impact on Our National-

419

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

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear Security Administration the1 - September 2006 The 2002OpticsPeriodical: Volume 5,PET Imaging:Department

420

Georgia System Operations Corporation Inc. Smart Grid Project | Open Energy  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data CenterFranconia, Virginia: Energy Resources Jump to: navigation, searchGeauga County, Ohio:Information4348438°Information

Note: This page contains sample records for the topic "redshift systems corporation" 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

DOE and Industry Showcase New Control Systems Security Technologies...  

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

to design a secure, networked control systems architecture. The project is led by Siemens Corporate Research in partnership with Rutgers University, Siemens Energy, and the...

422

Gas informations systems as an asset, not an expense  

SciTech Connect (OSTI)

The utilization of information systems in the natural gas industry is described. Opportunities for the acquisition of important business information and corporate issues are illustrated.

Neill, C.

1995-12-31T23:59:59.000Z

423

Machine learning techniques for astrophysical modelling and photometric redshift estimation of quasars in optical sky surveys  

E-Print Network [OSTI]

Machine learning techniques are utilised in several areas of astrophysical research today. This dissertation addresses the application of ML techniques to two classes of problems in astrophysics, namely, the analysis of individual astronomical phenomena over time and the automated, simultaneous analysis of thousands of objects in large optical sky surveys. Specifically investigated are (1) techniques to approximate the precise orbits of the satellites of Jupiter and Saturn given Earth-based observations as well as (2) techniques to quickly estimate the distances of quasars observed in the Sloan Digital Sky Survey. Learning methods considered include genetic algorithms, particle swarm optimisation, artificial neural networks, and radial basis function networks. The first part of this dissertation demonstrates that GAs and PSO can both be efficiently used to model functions that are highly non-linear in several dimensions. It is subsequently demonstrated in the second part that ANNs and RBFNs can be used as effective predictors of spectroscopic redshift given accurate photometry, especially in combination with other learning-based approaches described in the literature. Careful application of these and other ML techniques to problems in astronomy and astrophysics will contribute to a better understanding of stellar evolution, binary star systems, cosmology, and the large-scale structure of the universe.

N. Daniel Kumar

2008-11-04T23:59:59.000Z

424

An Intermediate-band imaging survey for high-redshift Lyman Alpha Emitters: The Mahoroba-11  

E-Print Network [OSTI]

We present results of our intermediate-band optical imaging survey for high-$z$ Ly$\\alpha$ emitters (LAEs) using the prime focus camera, Suprime-Cam, on the 8.2m Subaru Telescope. In our survey, we use eleven filters; four broad-band filters ($B$, $R_{\\rm c}$, $i^\\prime$, and $z^\\prime$) and seven intermediate-band filters covering from 500 nm to 720 nm; we call this imaging program as the Mahoroba-11. The seven intermediate-band filters are selected from the IA filter series that is the Suprime-Cam intermediate-band filter system whose spectral resolution is $R = 23$. Our survey has been made in a $34^\\prime \\times 27^\\prime$ sky area in the Subaru XMM Newton Deep Survey field. We have found 409 IA-excess objects that provide us a large photometric sample of strong emission-line objects. Applying the photometric redshift method to this sample, we obtained a new sample of 198 LAE candidates at $3 42.67$ between $z \\sim 3$ and 5.

Yamada, S F; Sumiya, R; Umeda, K; Shioya, Y; Ajiki, M; Nagao, T; Murayama, T; Taniguchi, Y; Yamada, Sanae F.; Sasaki, Shunji S.; Sumiya, Ryoko; Umeda, Kazuyoshi; Shioya, Yasuhiro; Ajiki, Masaru; Nagao, Tohru; Murayama, Takashi; Taniguchi, Yoshiaki

2005-01-01T23:59:59.000Z

425

A CLOSE-PAIR ANALYSIS OF DAMP MERGERS AT INTERMEDIATE REDSHIFTS  

SciTech Connect (OSTI)

We have studied the kinematics of {approx}2800 candidate close-pair galaxies at 0.1 < z < 1.2 identified from the Canada-France-Hawaii Telescope Legacy Survey fields. Spectra of these systems were obtained using spectrometers on the 6.5 m Magellan and 5 m Hale telescopes. These data allow us to constrain the rate of dry mergers at intermediate redshifts and to test the 'hot halo' model for quenching of star formation. Using virial radii estimated from the correlation between dynamical and stellar masses published by Leauthaud et al., we find that around 1/5 of our candidate pairs are likely to share a common dark matter halo (our metric for close physical association). These pairs are divided into red-red, blue-red, and blue-blue systems using the rest-frame colors classification method introduced in Chou et al.. Galaxies classified as red in our sample have very low star formation rates, but they need not be totally quiescent, and hence we refer to them as 'damp', rather than 'dry', systems. After correcting for known selection effects, the fraction of blue-blue pairs is significantly greater than that of red-red and blue-red pairs. Red-red pairs are almost entirely absent from our sample, suggesting that damp mergers are rare at z {approx} 0.5. Our data support models with a short merging timescale (<0.5 Gyr) in which star formation is enhanced in the early phase of mergers, but quenched in the late phase. Hot halo models may explain this behavior, but only if virial shocks that heat gas are inefficient until major mergers are nearly complete.

Chou, Richard C. Y.; Abraham, Roberto G. [Department of Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5S 3H4 (Canada); Bridge, Carrie R., E-mail: chou@astro.utoronto.ca, E-mail: abraham@astro.utoronto.ca, E-mail: bridge@astro.caltech.edu [Department of Astronomy, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA 91125 (United States)

2012-12-01T23:59:59.000Z

426

2012 IBM Corporation IBM operates in 170  

E-Print Network [OSTI]

Smart traffic systems Smart water management Smart energy grids Smart healthcare Smart food systems cities Smart retail Making the worlds systems smarter depends on data and analytics #12;© 2012 IBM Intelligent oil field technologies Smart regions Smart weather Smart countries Smart supply chains Smart

Raja, Anita

427

Hindawi Publishing Corporation International Journal of Photoenergy  

E-Print Network [OSTI]

, Pages 1­8 DOI 10.1155/IJP/2006/73650 Sizing Stand-Alone Photovoltaic Systems A. Balouktsis,1 T. D August 2005; Accepted 5 September 2005 A method of sizing stand-alone photovoltaic systems regarding­9]. The present study is concerned with sizing stand-alone photovoltaic systems for different locations in Greece

Aristomenis, Antoniadis

428

Recovery Act: Waste Energy Project at AK Steel Corporation Middletown  

SciTech Connect (OSTI)

In 2008, Air Products and Chemicals, Inc. (“Air Products”) began development of a project to beneficially utilize waste blast furnace “topgas” generated in the course of the iron-making process at AK Steel Corporation’s Middletown, Ohio works. In early 2010, Air Products was awarded DOE Assistance Agreement DE-EE002736 to further develop and build the combined-cycle power generation facility. In June 2012, Air Products and AK Steel Corporation terminated work when it was determined that the project would not be economically viable at that time nor in the foreseeable future. The project would have achieved the FOA-0000044 Statement of Project Objectives by demonstrating, at a commercial scale, the technology to capture, treat, and convert blast furnace topgas into electric power and thermal energy.

Joyce, Jeffrey

2012-06-30T23:59:59.000Z

429

A corporate fitness center : an example for the reuse of the Empire Stores, Brooklyn, N.Y.  

E-Print Network [OSTI]

The proliferation of over 500 fitness programs for the employees of American corporations marks a turning point for the way American corporations regard employee and corporate health. Typically, sports facilities were the ...

Georgopulos, Diane Theodora

1982-01-01T23:59:59.000Z

430

Accounting procedures under the Texas Business Corporation Act  

E-Print Network [OSTI]

Cuesion 0 ~ ~ ~ ~ ~ 0 ~ 0 4 8 8 ~ 8 I, Accounting for Stook Sulsoriptions and Issue of Capital Stook . . . ~ ~ & l XX y Surplus Qsl DivM and a s ~ e s a ~ ~ e ~ ~ i7 XIII' Trasaurg Stoa& ~ ~ o ~ s s e ~ ~ ~ ~ ~ a 52 XV. Dissolution of a Corporation... of the corporation with- out par value that, have been issued except such part of the consideration actually received therefor as msy have been allocated to capital surplus in a mannex' presented by law and any other amounts that have been txanskerred to stated...

Dodson, Donald R

1961-01-01T23:59:59.000Z

431

An Analysis of Gravitational Redshift from Rotating Body-II: The Effect of Electro and Magneto Static Field  

E-Print Network [OSTI]

It is well known fact that gravitational mass can alter the space time structure and gravitational redshift is its one example. Static electric or magnetic charge can also alter the space-time similar to gravitational mass. So Static electric or magnetic charge can also give rise to an effect of same kind on redshift (analogous to gravitational redshift). This can be considered as electro and magneto static redshift. Gravitational redshift has been reported by most of the authors without consideration of static electric and / or magnetic charge present on the rotating body. As a continuation of our previous work [1], in the present paper we will discuss combined gravitational and electro-magneto-static redshift for rotating by using Kerr - Newman - Kasuya metric.

Dubey, Anuj Kumar

2015-01-01T23:59:59.000Z

432

An exploration of corporate entrepreneurship : venturing signatures and their underlying dynamics  

E-Print Network [OSTI]

The primary goal of this work is to broadly explore the factors influencing corporate entrepreneurship and to examine how its many elements can be linked together. A broad reading of the published literature on corporate ...

Furst, Michael R

2005-01-01T23:59:59.000Z

433

NCCR Trade Regulation Brown Bag Series Dr Franziska Humbert, Policy Advisor Corporate Social Responsibility, Oxfam Germany  

E-Print Network [OSTI]

Social Responsibility, Oxfam Germany International Constitutionalism and Child Labour Wednesday, 23, Policy Advisor Corporate Social Responsibility, Oxfam Germany. Abstract The postdoctoral thesis builds of the Speaker Franziska Humbert is a policy advisor on corporate social responsibility at Oxfam Germany

Richner, Heinz

434

E-business and organizational partnerships in Corporate Real Estate: a case study  

E-Print Network [OSTI]

E-business is transforming the business landscape and changing the roles and methods of Corporate Real Estate. In a Corporate Real Estate department in a large firm, a new and innovative strategy is used to manage their facilities - organizational...

Xia, Ge

2012-06-07T23:59:59.000Z

435

Corporate bankruptcy : assessment, analysis and prediction of financial distress, insolvency, and failure  

E-Print Network [OSTI]

This paper is divided into three sections that address the various elements of understanding, predicting and analyzing corporate failure and bankruptcy. Part I covers the definitions of corporate failure, explains the ...

Danilov, Konstantin A

2014-01-01T23:59:59.000Z

436

State Participation and the Corporate Value of Natural Resource Economic Rents   

E-Print Network [OSTI]

The asset participation relationship between the state and the corporate entity is an essential determinant of corporate value in the natural resource sector. Natural resources deplete, with the result that oil reserve ...

Kretzschmar, Gavin Lee

2007-01-01T23:59:59.000Z

437

Bear Head LNG Corporation and Bear Head LNG (USA), LLC - FE Dkt...  

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

Bear Head LNG Corporation and Bear Head LNG (USA), LLC - FE Dkt. No. - 15-33-LNG Bear Head LNG Corporation and Bear Head LNG (USA), LLC - FE Dkt. No. - 15-33-LNG The Office of...

438

Changing gear : driving corporate real estate financing decisions for the agile workplace  

E-Print Network [OSTI]

Given the needs of corporations in the global business environment, corporate real estate investment decisions represent strategic choices that support a company's overall business strategy. This thesis clearly illustrates ...

Hardy, Trevor J. F. (Trevor John Fraser), 1977-

2002-01-01T23:59:59.000Z

439

What are matching gifts? Many corporations match their employees' charitable contributions. Your support for The  

E-Print Network [OSTI]

Mobil FAMM LLC Firestone/Bridgestone Tire First Data Corporation FMC Foundation Freeport McMoran, Inc Co. Georgia Gulf Corporation Goodyear Corp. Graybar Electric Co. Great Lakes Carbon Corp. Grinnell

Azevedo, Ricardo

440

Beacon Power Corporation Business Case Review  

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

in part by the Energy Storage Systems Program of the U.S. Department Of Energy (DOEESS) through Sandia National Laboratories (SNL). 2 Outline * Introduction * Principles of...

Note: This page contains sample records for the topic "redshift systems corporation" 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.


441

Renewable Energy Production Tax Credit (Corporate)  

Broader source: Energy.gov [DOE]

'''''Note: this tax credit is only available for systems installed on or after December 31, 2010, and before January 1, 2021.'''''

442

Red-Shift Distribution of Gamma-ray Bursts and Their Progenitors  

E-Print Network [OSTI]

Gamma ray bursts have been divided into two classes, long-soft gamma ray burst and short-hard gamma ray burst according to the bimodal distribution in duration time. Due to the harder spectrum and the lack of afterglows of short-hard bursts in optical and radio observations, different progenitors for short-hard bursts and long-soft bursts have been suggested. Based on the X-ray afterglow observation and the cumulative red-shift distribution of short-hard bursts, Nakar et al. (2006) found that the progenitors of short-hard bursts are consistent with old populations, such as mergers of binary neutron stars. Recently, the existence of two subclasses in long-soft bursts has been suggested after considering multiple characteristics of gamma-ray bursts, including fluences and the duration time. In this work, we extended the analysis of cumulative red-shift distribution to two possible subclasses in L-GRBs. We found that two possible subclass GRBs show different red-shift distributions, especially for red-shifts z > 1. Our results indicate that the accumulative red-shift distribution can be used as a tool to constrain the progenitor characteristics of possible subclasses in L-GRBs.

Soomin Jeong; Chang-Hwan Lee

2007-10-08T23:59:59.000Z

443

The Swift Gamma-Ray Burst Host Galaxy Legacy Survey - I. Sample Selection and Redshift Distribution  

E-Print Network [OSTI]

We introduce the Swift Gamma-Ray Burst Host Galaxy Legacy Survey ("SHOALS"), a multi-observatory high-redshift galaxy survey targeting the largest unbiased sample of long-duration gamma-ray burst hosts yet assembled (119 in total). We describe the motivations of the survey and the development of our selection criteria, including an assessment of the impact of various observability metrics on the success rate of afterglow-based redshift measurement. We briefly outline our host-galaxy observational program, consisting of deep Spitzer/IRAC imaging of every field supplemented by similarly-deep, multi-color optical/NIR photometry, plus spectroscopy of events without pre-existing redshifts. Our optimized selection cuts combined with host-galaxy follow-up have so far enabled redshift measurements for 110 targets (92%) and placed upper limits on all but one of the remainder. About 20% of GRBs in the sample are heavily dust-obscured, and at most 2% originate from z>5.5. Using this sample we estimate the redshift-depen...

Perley, D A; Schulze, S; Postigo, A de Ugarte; Hjorth, J; Berger, E; Cenko, S B; Chary, R; Cucchiara, A; Ellis, R; Fong, W; Fynbo, J P U; Gorosabel, J; Greiner, J; Jakobsson, P; Laskar, T; Levan, A J; Micha?owski, M J; Milvang-Jensen, B; Tanvir, N R; Thöne, C C; Wiersema, K

2015-01-01T23:59:59.000Z

444

Comment submitted by BSH Home Appliances Corporation regarding the Energy Star Verification Testing Program  

Broader source: Energy.gov [DOE]

This document is a comment submitted by BSH Home Appliances Corporation regarding the Energy Star Verification Testing Program

445

Comment submitted by CertainTeed Corporation regarding the Energy Star Verification Testing Program  

Broader source: Energy.gov [DOE]

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

446

Comment submitted by A. O. Smith Corporation regarding the Energy Star Verification Testing Program  

Broader source: Energy.gov [DOE]

This document is a comment submitted by A. O. Smith Corporation regarding the Energy Star Verification Testing Program

447

2009 IBM Corporation IBM Academic Initiative  

E-Print Network [OSTI]

-sensitive, adaptive information seeking tools. Green and Beyond: Optimizing data center infrastructures for energy, organization, city, nation, natural system and man-made system is becoming interconnected, instrumented Academic Initiative: Building skills for a smarter planet Global market forces are impacting us all Access

448

The Earth Institute I Corporate Circle The latest information, tools and networks to achieve sustainability  

E-Print Network [OSTI]

The Earth Institute I Corporate Circle Fall 2009 The latest information, tools and networks to achieve sustainability #12;The Earth Institute I Corporate Circle STRATEGIC OPPORTUNITIES GOAL Engage and allow for flexibility in the nature and extent of engagement. The Earth Institute I Corporate Circle #12

449

Do corporate political strategies differ from one country to The case of France and Britain  

E-Print Network [OSTI]

Do corporate political strategies differ from one country to the next ? The case of France in particular to determine if corporate political actions differ from one country to the next. To answer. Then, variance analysis is used to modelize corporate political strategies in both countries. Keywords

Boyer, Edmond

450

TECHNICAL REPORT SCR-01-TR-703 c Siemens Corporate Research 2001  

E-Print Network [OSTI]

TECHNICAL REPORT SCR-01-TR-703 c Siemens Corporate Research 2001 A Spectral Power Factorization Radu Balan and Justinian Rosca radu.balan,justinian.rosca@scr.siemens.com Siemens Corporate Research) #12;c Siemens Corporate Research 2001 2 and therefore the sum has the spectral power: Rx(z) = G2 1 P1

Maryland at College Park, University of

451

2012 Eaton Corporation. All rights reserved. This is a photographic template your  

E-Print Network [OSTI]

© 2012 Eaton Corporation. All rights reserved. This is a photographic template ­ your photograph (dominiquelallement@eaton.com) #12;2© 2012 Eaton Corporation. All rights reserved. Green Days January 2012 Power Management in virtual server environment Agenda · Eaton Corporation · Power Management Software suite · Power

Lefèvre, Laurent

452

is seeking partnerships with private and corporate donors  

E-Print Network [OSTI]

mineral resources is the keystone to the global minerals industry. As existing mines are depleted of metallic mineral resources. Programs encouraging reduction in use, re-use and recycling are able to offset#12;is seeking partnerships with private and corporate donors to strengthen capacity in mineral

453

Hindawi Publishing Corporation International Journal of Plant Genomics  

E-Print Network [OSTI]

Hindawi Publishing Corporation International Journal of Plant Genomics Volume 2008, Article ID 412875, 7 pages doi:10.1155/2008/412875 Research Article TreeGenes: A Forest Tree Genome Database Jill L are to (1) provide a comprehensive resource for forest tree genomics data to facilitate gene discovery

California at Santa Cruz, University of

454

Hindawi Publishing Corporation International Journal of Biomedical Imaging  

E-Print Network [OSTI]

Hindawi Publishing Corporation International Journal of Biomedical Imaging Volume 2006, Article ID, functional, cel- lular, and molecular imaging. The overall goal of the Inter- national Journal of Biomedical the current imaging journals handle. In addition, there are new imag- ing areas that are not specifically

Virginia Tech

455

Aeronautics Test Program (ATP) Corporate Management of Aeronautical  

E-Print Network [OSTI]

Aeronautics Test Program (ATP) Corporate Management of Aeronautical Facilities Blair Gloss Program Director (Blair.B.Gloss@nasa.gov) #12;Outline · Review ATP · Accomplishments - FY'2006 · Plans · Summary Supersonic Tunnel #12;FY 2006 Accomplishments · ATP Office Staffed · Investments ­Maintained competitive

456

Corporations LEHIGH UNIVERSITY 1 4Charity Foundation, Inc.  

E-Print Network [OSTI]

Corporations LEHIGH UNIVERSITY 1 4Charity Foundation, Inc. Abbott Davidson Weiss & Company ABM Janitorial Services - Mid Atlantic, Inc. Above The Rest Answering Service Accenture Foundation, Inc. Advanced Dermatology, Mohs & Laser Surgery Center Aesculap, Inc. Air Products Air Products Foundation Alaric Compliance

Gilchrist, James F.

457

2011 SunPower Corporation 2012 SunPower  

E-Print Network [OSTI]

materials, components, and solar panels, as well as the price paid for such items and third parties and Challenges July 5, 2012 Gabriela Bunea #12;© 2012 SunPower Corporation OUTLINE § SunPower overview § Solar demand growth in the solar industry, and projected bookings and pipelines, (e) utility project

Ingrand, François

458

ORCHARD BEE NESTING MATERIALS ACE PAPER TUBE CORPORATION  

E-Print Network [OSTI]

ORCHARD BEE NESTING MATERIALS ACE PAPER TUBE CORPORATION Nesting Tubes 4918 Denison Ave., Cleveland, Ohio 44102 Tel: 216-961-0250 Mason Bees and Nesting Supplies 21323 232nd St. SE, Monroe, Washington 98272-8982 Fax: 206-820-8037 E-mail: easugden@msn.com MAXTEK Nest Blocks Chuck McSween Tel: 425

459

Company Website AES Corporation, The http://www.aes.com  

E-Print Network [OSTI]

Gas http://www.eqt.com/ ExxonMobil http://www.exxonmobil.com Exelon Corporation http://www.fpl.com/ #12;GE Energy http://www.ge-energy.com/about/index.jsp Gulf Oil Limited Partnership http://www.horizonengineering.com/ Indian Mills Pump & Tank Company http://www.impumptank.com Integrys Energy Group, Inc. http

McGaughey, Alan

460

"Practicing Statistics in Corporate R&D" William A. Brenneman  

E-Print Network [OSTI]

to efficiently produce new and improved products. Statisticians play a central role in helping the product team quickly identify areas for improvement and optimization. Many of the problems faced in industry can"Practicing Statistics in Corporate R&D" William A. Brenneman The Procter & Gamble Company

Wang, Lily

Note: This page contains sample records for the topic "redshift systems corporation" 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

Driving down corporate carbon emissions through sustainable property management  

E-Print Network [OSTI]

Driving down corporate carbon emissions through sustainable property management Challenge Many organisations are facing increasing cost challenges and pressure to reduce their carbon dioxide (CO2) emissions consideration is the carbon dioxide emissions per square metre of floor space. While an important metric

462

Is the Time a Dimension of an Alien Universe? (this hypothesis gives an additional redshift)  

E-Print Network [OSTI]

On the base of the hypothesis about a nature of the time as a dimension of alien Universe relation between alteration of time with coordinates $\\frac{\\partial t}{\\partial x}$ and time {t} offered: $ \\frac{\\partial t} {\\partial x} = H_{t} t$ . This relation is an analogy of the Habble law in the time space. The consequence of it is additional redshift $Z_{DT}$ depending on differences $\\tau$ of times existence of the objects with redshift that are compared ($t_{0}$ is the time existence of more old object): $Z_{DT}=\\frac{1+\\frac{\\tau}{t_{0}}}{\\sqrt{1-(\\frac{\\tau}{t_{0}}})^{2}}-1$. The redshift of Arp galaxies may be explained if this relation is used and this explanation doe's not contradict Arp hypothesis about supernova explosions. Discussion a possibilities of experimental verification of the hypothesis is considered.

L. Ya. Kobelev

2000-05-25T23:59:59.000Z

463

Redshifts of Emission Line Objects in the Hubble Ultra Deep Field  

E-Print Network [OSTI]

We present redshifts for 115 emission line objects in the Hubble Ultra Deep Field (HUDF) identified through the GRism ACS Program for Extragalactic Science (GRAPES) project using the slitless grism spectroscopy mode of the ACS Camera on the Hubble Space Telescope (HST). The sample was selected by an emission line search on all extracted 1-dimensional GRAPES spectra. We identify the emission lines using line wavelength ratios where multiple lines are detected in the grism wavelength range (5800A 25 mag). Such emission lines would likely remain undiscovered without our deep survey. The emission line objects fall into 3 categories: 1) Most are low to moderate redshift galaxies (0 star forming galaxies with strong HII regions; 2) 9 are high redshift (4 < z < 7) Lyman-alpha emitters; and 3) at least 3 are candidate AGNs.

Chun Xu; Norbert Pirzkal; Sangeeta Malhotra; James E. Rhoads; Bahram Mobasher; Emanuele Daddi; Caryl Gronwall; Nimish P. Hathi; Nino Panagia; Henry C. Ferguson; Anton M. Koekemoer; Martin Kuemmel; Leonidas A. Moustakas; Anna Pasquali; Sperello di Serego Alighieri; Joel Vernet; Jeremy R. Walsh; Rogier Windhorst; Haojing Yan

2007-01-30T23:59:59.000Z

464

The environments of intermediate-redshift QSOs: 0.3 < z < 0.7  

E-Print Network [OSTI]

An angular correlation of low significance (2 sigma) is observed between 0.3 0.5 QSOs. After converting to an excess of galaxies physically associated with the QSO, this lack of strong correlation is shown to be consistent with the clustering of normal galaxies at the same moderate redshifts. Combined with previous observations, these results imply that the environments of radio-quiet QSOs do not undergo significant evolution with respect to the galaxy population over a wide range of redshifts (0 < z < 1.5). This is in marked contrast to the rapid increase in the richness of the environments associated with radio-loud QSOs over the same redshift range.

R. J. Smith; B. J. Boyle; S. J. Maddox

1999-11-22T23:59:59.000Z

465

Type Ia supernova rate at a redshift of ~ 0.1  

E-Print Network [OSTI]

We present the type Ia rate measurement based on two EROS supernova search campaigns (in 1999 and 2000). Sixteen supernovae identified as type Ia were discovered. The measurement of the detection efficiency, using a Monte Carlo simulation, provides the type Ia supernova explosion rate at a redshift ~ 0.13. The result is $0.125^{+0.044+0.028}_{-0.034-0.028} h_{70}^2$ SNu where 1 SNu = 1 SN / $10^{10} L_{sun}^B$ / century. This value is compatible with the previous EROS measurement (Hardin et al. 2000), done with a much smaller sample, at a similar redshift. Comparison with other values at different redshifts suggests an evolution of the type Ia supernova rate.

Blanc, G; Alard, C; Albert, J N; Aldering, G; Amadon, A; Andersen, J; Ansari, R; Aubourg, E; Balland, C; Bareyre, P; Beaulieu, J P; Charlot, X; Conley, A; Coutures, C; Dahlen, T; Derue, F; Fan, X; Ferlet, R; Folatelli, G; Fouqué, P; Garavini, G; Glicenstein, J F; Goldman, B; Goobar, A; Gould, A; Graff, D; Gros, M; Haďssinski, J; Hamadache, C; Hardin, D; Hook, I M; De Kat, J; Kent, S; Kim, A; Lasserre, T; Le Guillou, Laurent; Lesquoy, E; Loup, C; Magneville, C; Marquette, J B; Maurice, E; Maury, A; Milsztajn, A; Moniez, M; Mouchet, M; Newberg, H; Nobili, S; Palanque-Delabrouille, Nathalie; Perdereau, O; Prévôt, L; Rahal, Y R; Regnault, N; Rich, J; Ruiz-Lapuente, P; Spiro, M; Tisserand, P; Vidal-Madjar, A; Vigroux, L; Walton, N A; Zylberajch, S

2004-01-01T23:59:59.000Z

466

Type Ia supernova rate at a redshift of ~ 0.1  

E-Print Network [OSTI]

We present the type Ia rate measurement based on two EROS supernova search campaigns (in 1999 and 2000). Sixteen supernovae identified as type Ia were discovered. The measurement of the detection efficiency, using a Monte Carlo simulation, provides the type Ia supernova explosion rate at a redshift ~ 0.13. The result is $0.125^{+0.044+0.028}_{-0.034-0.028} h_{70}^2$ SNu where 1 SNu = 1 SN / $10^{10} L_{sun}^B$ / century. This value is compatible with the previous EROS measurement (Hardin et al. 2000), done with a much smaller sample, at a similar redshift. Comparison with other values at different redshifts suggests an evolution of the type Ia supernova rate.

G. Blanc; C. Afonso; C. Alard; J. N. Albert; G. Aldering; A. Amadon; J. Andersen; R. Ansari; E. Aubourg; C. Balland; P. Bareyre; J. P. Beaulieu; X. Charlot; A. Conley; C. Coutures; T. Dahlen; F. Derue; X. Fan; R. Ferlet; G. Folatelli; P. Fouque; G. Garavini; J. F. Glicenstein; B. Goldman; A. Goobar; A. Gould; D. Graff; M. Gros; J. Haissinski; C. Hamadache; D. Hardin; I. M. Hook; J. deKat; S. Kent; A. Kim; T. Lasserre; L. LeGuillou; E. Lesquoy; C. Loup; C. Magneville; J. B. Marquette; E. Maurice; A. Maury; A. Milsztajn; M. Moniez; M. Mouchet; H. Newberg; S. Nobili; N. Palanque-Delabrouille; O. Perdereau; L. Prevot; Y. R. Rahal; N. Regnault; J. Rich; P. Ruiz-Lapuente; M. Spiro; P. Tisserand; A. Vidal-Madjar; L. Vigroux; N. A. Walton; S. Zylberajch

2004-05-11T23:59:59.000Z

467

Formula for red-shift of light signals coming from distant galaxies  

E-Print Network [OSTI]

Relying on the obtained results in Rev.[1](physics/0505035), we derive the formula relating the red-shift of light signals coming from distant galaxies to the distance of these galaxies from us and the time of detecting of these light signals. The red-shift coefficient, instead of the Hubble parameter, is introduced. It varies with time and positive at all times. Its nowadays value equals the Hubble parameter. It increases forever as time is running from the past to the future. The derived formula enables us to estimate the nowadays increasing rate of the red-shift coefficient, which is nothing but the nowadays value of the "acceleration of the expansion of the Universe".

Jian-Miin Liu

2005-05-04T23:59:59.000Z

468

Submillimetre sources in rich cluster fields - source counts, redshift estimates, and cooling flow limits  

E-Print Network [OSTI]

Recent submillimetre surveys have revealed a population of dusty, high redshift sources of great cosmological significance for understanding dust-enshrouded star formation in distant galaxies, and for determining the origin of the far-IR background. In this paper, we analyze nine rich cluster fields mapped at 850 and 450 microns with the SCUBA array on the James Clerk Maxwell telescope. Lensing models of the clusters are developed in order to derive accurate source counts for our sample. VLA maps of the same clusters are used to help constrain the redshift distribution of our SCUBA detections. Implications for high redshift galaxies and for the far-IR background are discussed. We also provide limits on distributed dust produced by cooling flows in these clusters.

Scott C. Chapman; Douglas Scott; Colin Borys; Gregory G. Fahlman

2000-09-05T23:59:59.000Z

469

The gravitational redshift of photons traversing a collapsing dust cloud and observable consequences  

E-Print Network [OSTI]

We analyze the frequency shift of photons propagating on an asymptotically flat spacetime describing a collapsing, spherical dust cloud. We focus on the case where the interaction of the photons with the matter can be neglected. Under fairly general assumptions on the initial data characterizing the collapse, we show that photons with zero angular momentum which travel from past to future null infinity, crossing the collapsing cloud through its center, are always redshifted with respect to stationary observers. We compute this redshift as a function of proper time of a distant stationary observer and discuss its dependency on the mass distribution of the cloud. Possible implications of this redshift effect for weak cosmic censorship and light propagation in cosmological spacetimes are also briefly discussed.

Néstor Ortiz; Olivier Sarbach

2014-11-24T23:59:59.000Z

470

Redshift evolution of the dynamical properties of massive galaxies from SDSS-III/BOSS  

E-Print Network [OSTI]

We study the redshift evolution of the dynamical properties of ~180,000 massive galaxies from SDSS-III/BOSS combined with a local early-type galaxy sample from SDSS-II in the redshift range 0.12sigma significance. By combining our sample with high-redshift literature data we find that this evolution of the dynamical to stellar mass ratio continues beyond z~0.7 up to z>2 as Mdyn/Mstar~ (1+z)^{-0.30+/- 0.12} further strengthening the evidence for an increase of Mdyn/Mstar with cosmic time. This result is in line with recent predictions from galaxy formation simulations based on minor merger driven mass growth, in which the dark matter fraction within the half-light radius increases with cosmic time.

Beifiori, Alessandra; Maraston, Claudia; Steele, Oliver; Masters, Karen L; Pforr, Janine; Saglia, Roberto P; Bender, Ralf; Tojeiro, Rita; Chen, Yan-Mei; Bolton, Adam; Brownstein, Joel R; Johansson, Jonas; Leauthaud, Alexie; Nichol, Robert C; Schneider, Donald P; Senger, Robert; Skibba, Ramin; Wake, David; Pan, Kaike; Snedden, Stephanie; Bizyaev, Dmitry; Brewington, Howard; Malanushenko, Viktor; Malanushenko, Elena; Oravetz, Daniel; Simmons, Audrey; Shelden, Alaina; Ebelke, Garrett

2014-01-01T23:59:59.000Z

471

Thermal Energy Corporation Combined Heat and Power Project  

SciTech Connect (OSTI)

To meet the planned heating and cooling load growth at the Texas Medical Center (TMC), Thermal Energy Corporation (TECO) implemented Phase 1 of a Master Plan to install an additional 32,000 tons of chilled water capacity, a 75,000 ton-hour (8.8 million gallon) Thermal Energy Storage (TES) tank, and a 48 MW Combined Heat and Power (CHP) system. The Department of Energy selected TMC for a $10 million grant award as part of the Financial Assistance Funding Opportunity Announcement, U.S. Department of Energy National Energy Technology, Recovery Act: Deployment of Combined Heat and Power (CHP) Systems, District Energy Systems, Waste Energy Recovery Systems, and Efficiency Industrial Equipment Funding Opportunity Number: DE-FOA-0000044 to support the installation of a new 48 MW CHP system at the TMC located just outside downtown Houston. As the largest medical center in the world, TMC is home to many of the nationâ??s best hospitals, physicians, researchers, educational institutions, and health care providers. TMC provides care to approximately six million patients each year, and medical instruction to over 71,000 students. A medical center the size of TMC has enormous electricity and thermal energy demands to help it carry out its mission. Reliable, high-quality steam and chilled water are of utmost importance to the operations of its many facilities. For example, advanced medical equipment, laboratories, laundry facilities, space heating and cooling all rely on the generation of heat and power. As result of this project TECO provides this mission critical heating and cooling to TMC utilizing a system that is both energy-efficient and reliable since it provides the capability to run on power independent of the already strained regional electric grid. This allows the medical center to focus on its primary mission â?? providing top quality medical care and instruction â?? without worrying about excessive energy costs or the loss of heating and cooling due to the risk of power outages. TECOâ??s operation is the largest Chilled Water District Energy System in the United States. The company used DOEâ??s funding to help install a new high efficiency CHP system consisting of a Combustion Turbine and a Heat Recovery Steam Generator. This CHP installation was just part of a larger project undertaken by TECO to ensure that it can continue to meet TMCâ??s growing needs. The complete efficiency overhaul that TECO undertook supported more than 1,000 direct and indirect jobs in manufacturing, engineering, and construction, with approximately 400 of those being jobs directly associated with construction of the combined heat and power plant. This showcase industrial scale CHP project, serving a critical component of the nationâ??s healthcare infrastructure, directly and immediately supported the energy efficiency and job creation goals established by ARRA and DOE. It also provided an unsurpassed model of a district energy CHP application that can be replicated within other energy intensive applications in the industrial, institutional and commercial sectors.

E. Bruce Turner; Tim Brown; Ed Mardiat

2011-12-31T23:59:59.000Z

472

The fate of high redshift massive compact galaxies in dense environments  

SciTech Connect (OSTI)

Massive compact galaxies seem to be more common at high redshift than in the local universe, especially in denser environments. To investigate the fate of such massive galaxies identified at z {approx} 2 we analyse the evolution of their properties in three cosmological hydrodynamical simulations that form virialized galaxy groups of mass {approx} 10{sup 13} M{sub {circle_dot}} hosting a central massive elliptical/S0 galaxy by redshift zero. We find that at redshift {approx} 2 the population of galaxies with M{sub *} > 2 x 10{sup 10} M{sub {circle_dot}} is diverse in terms of mass, velocity dispersion, star formation and effective radius, containing both very compact and relatively extended objects. In each simulation all the compact satellite galaxies have merged into the central galaxy by redshift 0 (with the exception of one simulation where one of such satellite galaxy survives). Satellites of similar mass at z = 0 are all less compact than their high redshift counterparts. They form later than the galaxies in the z = 2 sample and enter the group potential at z < 1, when dynamical friction times are longer than the Hubble time. Also, by z = 0 the central galaxies have increased substantially their characteristic radius via a combination of in situ star formation and mergers. Hence in a group environment descendants of compact galaxies either evolve towards larger sizes or they disappear before the present time as a result of the environment in which they evolve. Since the group-sized halos that we consider are representative of dense environments in the {Lambda}CDM cosmology, we conclude that the majority of high redshift compact massive galaxies do not survive until today as a result of the environment.

Kaufmann, Tobias; /Zurich, ETH; Mayer, Lucio; /Zurich U.; Carollo, Marcella; /Zurich, ETH; Feldmann, Robert; /Fermilab /Chicago U., KICP

2012-01-01T23:59:59.000Z

473

Solar and Wind Energy Credit (Corporate)  

Broader source: Energy.gov [DOE]

Note: The Hawaii Department of Taxation issued temporary administrative rules in November 2012 for photovoltaic systems installed on or after January 1, 2013. A formal rulemaking is underway. See "...

474

Systems Signals The newsletter of the Institute for Systems Research  

E-Print Network [OSTI]

project, Operational Meth- ods in Semiconductor Manufacturing: Integrating Product Dynamics and Process and Product Systems Division and the Semiconductor Research Corporation's Factory Sciences Division. Its's inside Bridge Baron........... 3 CATS ........................2 NSF survey .............7 Faculty news

Shapiro, Benjamin

475

RENEWABLES RESEARCH Boiler Burner Energy System Technology  

E-Print Network [OSTI]

RENEWABLES RESEARCH Boiler Burner Energy System Technology (BBEST) for Firetube Boilers PIER Renewables Research September 2010 The Issue Researchers at Altex Technologies Corporation in Sunnyvale, industrial combined heat and power (CHP) boiler burner energy system technology ("BBEST"). Their research

476

MASSIVE CLUMPS IN LOCAL GALAXIES: COMPARISONS WITH HIGH-REDSHIFT CLUMPS  

SciTech Connect (OSTI)

Local UV-bright galaxies in the Kiso survey include clumpy systems with kiloparsec-size star complexes that resemble clumpy young galaxies in surveys at high redshift. We compare clump masses and underlying disks in several dozen galaxies from each of these surveys to the star complexes and disks of normal spirals. Photometry and spectroscopy for the Kiso and spiral sample come from the Sloan Digital Sky Survey. We find that the largest Kiso clumpy galaxies resemble Ultra Deep Field (UDF) clumpies in terms of the star formation rates, clump masses, and clump surface densities. Clump masses and surface densities in normal spirals are smaller. If the clump masses are proportional to the turbulent Jeans mass in the interstellar medium, then for the most luminous galaxies in the sequence of normal:Kiso:UDF, the turbulent speeds and surface densities increase in the proportions 1.0:4.7:5.0 and 1.0:4.0:5.1, respectively, for fixed restframe B-band absolute magnitude. For the least luminous galaxies in the overlapping magnitude range, the turbulent speed and surface density trends are 1.0:2.7:7.4 and 1.0:1.4:3.0, respectively. We also find that while all three types have radially decreasing disk intensities when measured with ellipse-fit azimuthal averages, the average profiles are more irregular for UDF clumpies (which are viewed in their restframe UV) than for Kiso galaxies (viewed at g-band), and major axis intensity scans are even more irregular for the UDF than Kiso galaxies. Local clumpy galaxies in the Kiso survey appear to be intermediate between UDF clumpies and normal spirals.

Elmegreen, Bruce G. [IBM Research Division, T. J. Watson Research Center, Yorktown Hts., NY 10598 (United States); Elmegreen, Debra Meloy; Dewberry, J.; Putko, J.; Teich, Y.; Popinchalk, M. [Vassar College, Dept. of Physics and Astronomy, Poughkeepsie, NY 12604 (United States); Sanchez Almeida, J.; Munoz-Tunon, C. [Instituto de Astrof'sica de Canarias, C/via Lactea, s/n, E-38205, La Laguna, Tenerife (Spain)

2013-09-01T23:59:59.000Z

477

American Superconductor Corporation | Open Energy Information  

Open Energy Info (EERE)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE: Alternative Fuels Data Center Home Page on Google Bookmark EERE: Alternative Fuels Data Center Home5b9fcbce19 NoPublic Utilities Address: 160 East 300Algoil JumpAltergy SystemsAmerican Energy SystemsElectric Inc

478

Oracle and Corporate Citizenship Paul Salinger  

E-Print Network [OSTI]

­ Eastern Europe Oracle OpenWorld Asia 1 Event China Oracle OpenWorld Latin America 1 Event Brazil Federal practices · Environment Management System as part of ISO 14001 · Oracle U.K. uses 100% renewable power ­ Australia/New Zealand OBI 11g Launch 15 Events ­ Western Europe 1 Event ­ North America Oracle Day 11 Events

Loudon, Catherine

479

Probing the Intergalactic Medium with high-redshift quasars  

E-Print Network [OSTI]

(?bkg) . . . . . . . . . . . . . . . . . . . . . . . 77 4.4 Calculated log(?bkg) for each of the quasar sightlines . . . . . . . . . . . . . . . . . . . . 81 5.1 Summary of the effect of Lyman limit systems . . . . . . . . . . . . . . . . . . . . . . . . 99 6.1 The list of quasars included...

Calverley, Alexander Peter

2011-11-08T23:59:59.000Z

480

TOWARD DETECTING THE 2175 A DUST FEATURE ASSOCIATED WITH STRONG HIGH-REDSHIFT Mg II ABSORPTION LINES  

SciTech Connect (OSTI)

We report detections of 39 2175 A dust extinction bump candidates associated with strong Mg II absorption lines at z{approx} 1-1.8 on quasar spectra in Sloan Digital Sky Survey (SDSS) DR3. These strong Mg II absorption line systems are detected among 2951 strong Mg II absorbers with a rest equivalent width W{sub r} {lambda}2796> 1.0 A at 1.0 < z < 1.86, which is part of a full sample of 7421 strong Mg II absorbers compiled by Prochter et al. The redshift range of the absorbers is chosen to allow the 2175 A extinction features to be completely covered within the SDSS spectrograph operation wavelength range. An upper limit of the background quasar emission redshift at z = 2.1 is set to prevent the Ly{alpha} forest lines from contaminating the sensitive spectral region for the 2175 A bump measurements. The FM90 parameterization is applied to model the optical/UV extinction curve in the rest frame of Mg II absorbers of the 2175 A bump candidates. The simulation technique developed by Jiang et al. is used to derive the statistical significance of the candidate 2175 A bumps. A total of 12 absorbers are detected with 2175 A bumps at a 5{sigma} level of statistical significance, 10 are detected at a 4{sigma} level, and 17 are detected at a 3{sigma} level. Most of the candidate bumps in this work are similar to the relatively weak 2175 A bumps observed in the Large Magellanic Cloud LMC2 supershell rather than the strong ones observed in the Milky Way. This sample has greatly increased the total number of 2175 A extinction bumps measured on SDSS quasar spectra. Follow-up observations may rule out some of the possible false detections and reveal the physical and chemical natures of 2175 A quasar absorbers.

Jiang Peng; Zhou Hongyan; Wang Junxian; Wang Tinggui [Key Laboratory for Research in Galaxies and Cosmology, University of Science and Technology of China, Chinese Academy of Sciences, Hefei, Anhui 230026 (China); Ge Jian, E-mail: jpaty@mail.ustc.edu.cn [Astronomy Department, University of Florida, 211 Bryant Space Science Center, P.O. Box 112055, Gainesville, FL 32611 (United States)

2011-05-10T23:59:59.000Z

Note: This page contains sample records for the topic "redshift systems corporation" 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.


481

The 2dF Galaxy Redshift Survey: The environmental dependence of galaxy star formation rates near clusters  

E-Print Network [OSTI]

We have measured the equivalent width of the H-alpha emission line for 11006 galaxies brighter than M_b=-19 (LCDM) at 0.05Redshift Survey (2dF), in the fields of seventeen known galaxy clusters. The limited redshift range ensures that our results are insensitive to aperture bias, and to residuals from night sky emission lines. We use these measurements to trace mustar, the star formation rate normalized to Lstar, as a function of distance from the cluster centre, and local projected galaxy density. We find that the distribution of mustar steadily skews toward larger values with increasing distance from the cluster centre, converging to the field distribution at distances greater than ~3 times the virial radius. A correlation between star formation rate and local projected density is also found, which is independent of cluster velocity dispersion and disappears at projected densities below ~1 galaxy (brighter than M_b=-19) per Mpc^2. This characteristic scale corresponds approximately to the mean density at the cluster virial radius. The same correlation holds for galaxies more than two virial radii from the cluster centre. We conclude that environmental influences on galaxy properties are not restricted to cluster cores, but are effective in all groups where the density exceeds this critical value. The present day abundance of such systems, and the strong evolution of this abundance, makes it likely that hierarchical growth of structure plays a significant role in decreasing the global average star formation rate. Finally, the low star formation rates well beyond the virialised cluster rule out severe physical processes, such as ram pressure stripping of disk gas, as being completely responsible for the variations in galaxy properties with environment.

Ian Lewis; Michael Balogh; Roberto De Propris; Warrick Couch; Richard Bower; Alison Offer; Joss Bland-Hawthorn; Ivan Baldry; Carlton Baugh; Terry Bridges; Russell Cannon; Shaun Cole; Matthew Colless; Chris Collins; Nicholas Cross; Gavin Dalton; Simon Driver; George Efstathiou; Richard Ellis; Carlos Frenk; Karl Glazebrook; Edward Hawkins; Carole Jackson; Ofer Lahav; Stuart Lumsden; Steve Maddox; Darren Madgwick; Peder Norberg; John Peacock; Will Percival; Bruce Peterson; Will Sutherland; Keith Taylor

2002-03-21T23:59:59.000Z

482

Fractal analysis of the galaxy distribution in the redshift range 0.45 < z < 5.0  

E-Print Network [OSTI]

Evidence is presented that the galaxy distribution can be described as a fractal system in the redshift range of the FDF galaxy survey. The fractal dimension $D$ was derived using the FDF galaxy volume number densities in the spatially homogeneous standard cosmological model with $\\Omega_{m_0}=0.3$, $\\Omega_{\\Lambda_0}=0.7$ and $H_0=70 \\; \\mbox{km} \\; {\\mbox{s}}^{-1} \\; {\\mbox{Mpc}}^{-1}$. The ratio between the differential and integral number densities $\\gamma$ and $\\gamma^\\ast$ obtained from the red and blue FDF galaxies provides a direct method to estimate $D$, implying that $\\gamma$ and $\\gamma^\\ast$ vary as power-laws with the cosmological distances. The luminosity distance $d_{\\scriptscriptstyle L}$, galaxy area distance $d_{\\scriptscriptstyle G}$ and redshift distance $d_z$ were plotted against their respective number densities to calculate $D$ by linear fitting. It was found that the FDF galaxy distribution is characterized by two single fractal dimensions at successive distance ranges. Two straight lines were fitted to the data, whose slopes change at $z \\approx 1.3$ or $z \\approx 1.9$ depending on the chosen cosmological distance. The average fractal dimension calculated using $\\gamma^\\ast$ changes from $\\langle D \\rangle=1.4^{\\scriptscriptstyle +0.7}_{\\scriptscriptstyle -0.6}$ to $\\langle D \\rangle=0.5^{\\scriptscriptstyle +1.2}_{\\scriptscriptstyle -0.4}$ for all galaxies, and $D$ decreases as $z$ increases. Small values of $D$ at high $z$ mean that in the past galaxies were distributed much more sparsely and the large-scale galaxy structure was then possibly dominated by voids. Results of Iribarrem et al. (2014, arXiv:1401.6572) indicating similar fractal features with $\\langle D \\rangle =0.6 \\pm 0.1$ in the far-infrared sources of the Herschel/PACS evolutionary probe (PEP) at $1.5 \\lesssim z \\lesssim 3.2$ are also mentioned.

G. Conde-Saavedra; A. Iribarrem; Marcelo B. Ribeiro

2014-09-18T23:59:59.000Z

483

Corporate competition: A self-organized network  

E-Print Network [OSTI]

A substantial number of studies have extended the work on universal properties in physical systems to complex networks in social, biological, and technological systems. In this paper, we present a complex networks perspective on interfirm organizational networks by mapping, analyzing and modeling the spatial structure of a large interfirm competition network across a variety of sectors and industries within the United States. We propose two micro-dynamic models that are able to reproduce empirically observed characteristics of competition networks as a natural outcome of a minimal set of general mechanisms governing the formation of competition networks. Both models, which utilize different approaches yet apply common principles to network formation give comparable results. There is an asymmetry between companies that are considered competitors, and companies that consider others as their competitors. All companies only consider a small number of other companies as competitors; however, there are a few compan...

Braha, Dan; Bar-Yam, Yaneer

2011-01-01T23:59:59.000Z

484

I. Apples to apples $A^2$: photometric redshift predictions for next-generation surveys  

E-Print Network [OSTI]

This is the first of a series of papers where we compare the expected performance of two of the largest stage IV next-generation surveys in the optical and infrared (LSST and Euclid), with a particular focus on cluster surveys. In this first paper, we introduce the mock catalogues we have utilized in this work, an N-body simulation+semi-analytical cone with a posterior modification with PhotReal, a technique which modifies the original photometry to make it more realistic by using an empirical library of spectral templates. We have confirmed the reliability of the mock catalogue by comparing the obtained color-magnitude relation, the luminosity and mass function and the angular correlation function with those of real data. We also analyze the behavior of the expected photometric redshifts for each different survey, in terms of photometric redshift resolution, photometric redshift bias and fraction of outliers. In addition, we discuss the benefits of using the BPZ \\emph{odds} photometric redshift quality param...

Ascaso, Begońa; Benítez, Narciso

2015-01-01T23:59:59.000Z

485

Photon and neutrino redshift in the field of braneworld compact stars  

SciTech Connect (OSTI)

We study gravitational redshift of photons and neutrinos radiated by the braneworld neutron or quark stars that are considered in the framework of the simple model of the internal spacetime with uniform distribution of energy density, and the external spacetime described by the Reissner-Nordström geometry characterized by the braneworld ''tidal'' charge b. For negative tidal charges, the external spacetime is of the black-hole type, while for positive tidal charges, the external spacetime can be of both black-hole and naked-singularity type. We consider also extremely compact stars allowing existence of trapped null geodesics in their interior. We assume radiation of photons from the surface at radius R, neutrinos from the whole compact star interior, and their motion along radial null geodesics of the spacetime. In dependency on the compact stars parameters b and R, the photon surface redshift is related to the range of the neutrino internal redshift and the signatures of the tidal charge and possible existence of extremely compact stars are discussed. When both surface (photon) and internal (neutrino) redshift are given by observations, both compact star parameters R and b can be determined in the framework of our simple model.

Hladík, Jan; Stuchlík, Zden?k, E-mail: jan.hladik@fpf.slu.cz, E-mail: zdenek.stuchlik@fpf.slu.cz [Institute of Physics, Faculty of Philosophy and Science, Silesian University in Opava, Bezrucovo nám. 13, CZ-746 01 Opava (Czech Republic)

2011-07-01T23:59:59.000Z

486

The 160 Square Degree ROSAT Survey: the Revised Catalog of 201 Clusters with Spectroscopic Redshifts  

E-Print Network [OSTI]

We present the revised catalog of galaxy clusters detected as extended X-ray sources in the 160 Square Degree ROSAT Survey, including spectroscopic redshifts and X-ray luminosities for 200 of the 201 members. The median redshift is z~0.25 and the median X-ray luminosity is 4.2e+43 erg/s/h50^2 (0.5-2.0 keV). This is the largest high-redshift sample of X-ray selected clusters published to date. There are 73 objects at z>0.3 and 22 objects at z>0.5 drawn from a statistically complete flux-limited survey with a median object flux of 1.4d-13 erg/cm^2/s. We describe the optical follow-up of these clusters with an emphasis on our spectroscopy which has yielded 155 cluster redshifts, 110 of which are presented here for the first time. These measurements combined with 45 from the literature and other sources provide near-complete spectroscopic coverage for our survey. We discuss the final optical identifications for the extended X-ray sources in the survey region and compare our results to similar X-ray cluster search...

Mullis, C R; Quintana, H; Vikhlinin, A; Henry, J P; Gioia, I M; Hornstrup, A; Forman, W; Jones, C

2003-01-01T23:59:59.000Z

487

Studying large-scale structure with the 2dF Galaxy Redshift Survey  

E-Print Network [OSTI]

The 2dF Galaxy Redshift Survey is the first to observe more than 100,000 redshifts. This allows precise measurements of many of the key statistics of galaxy clustering, in particular redshift-space distortions and the large-scale power spectrum. This paper presents the current 2dFGRS results in these areas. Redshift-space distortions are detected with a high degree of significance, confirming the detailed Kaiser distortion from large-scale infall velocities, and measuring the distortion parameter beta equiv Omega_m^{0.6}/b = 0.43 +- 0.07. The power spectrum is measured to 0.02 h Mpc^{-1}, and is well fitted by a CDM model with Omega_m h = 0.20 +- 0.03 and a baryon fraction of 0.15 +- 0.07. A joint analysis with CMB data requires Omega_m = 0.29 +- 0.05, assuming scalar fluctuations, but no priors on other parameters. Two methods are used to determine the large-scale bias parameter: an internal bispectrum analysis yields b = 1.04 +- 0.11, in very good agreement with the b = 1.10 +- 0.08 obtained from a joint 2dFGRS+CMB analysis, again assuming scalar fluctuations. These figures refer to galaxies of approximate luminosity 2L^*; luminosity dependence of clustering is detected at high significance, and is well described by b/b^* = 0.85 + 0.15(L/L^*).

J. A. Peacock; M. Colless; I. Baldry; C. Baugh; J. Bland-Hawthorn; T. J. Bridges; R. Cannon; S. Cole; C. A. Collins; W. Couch; G. B. Dalton; R. De Propris; S. P. Driver; G. Efstathiou; R. S. Ellis; C. S. Frenk; K. Glazebrook; C. A. Jackson; O. Lahav; I. J. Lewis; S. Lumsden; S. J. Maddox; D. Madgwick; P. Norberg; W. Percival; B. A. Peterson; W. J. Sutherland; K. Taylor

2002-05-28T23:59:59.000Z

488

Beacon Power Corporation NREL Industry Growth Forum  

E-Print Network [OSTI]

with General Electric · Awarded "Engineer of the Year" @ GE · B.S. and M.S. degrees in M.E. from MIT · 65;7 From Flywheel to 20 MW Plant 7 #12;88 Base Business Model · Build, own/co-own and operate merchant (outright or co-investment) · Sell regulation systems outside the U.S. with strategic partners · Sell other

489

Supernova rates from the Southern inTermediate Redshift ESO Supernova Search (STRESS)  

E-Print Network [OSTI]

To measure the supernova (SN) rates at intermediate redshift we performed the Southern inTermediate Redshift ESO Supernova Search (STRESS). Unlike most of the current high redshift SN searches, this survey was specifically designed to estimate the rate for both type Ia and core collapse (CC) SNe. We counted the SNe discovered in a selected galaxy sample measuring SN rate per unit blue band luminosity. Our analysis is based on a sample of ~43000 galaxies and on 25 spectroscopically confirmed SNe plus 64 selected SN candidates. Our approach is aimed at obtaining a direct comparison of the high redshift and local rates and at investigating the dependence of the rates on specific galaxy properties, most notably their colour. The type Ia SN rate, at mean redshift z=0.3, amounts to 0.22^{+0.10+0.16}_{-0.08 -0.14} h_{70}^2 SNu, while the CC SN rate, at z=0.21, is 0.82^{+0.31 +0.30}_{-0.24 -0.26} h_{70}^2 SNu. The quoted errors are the statistical and systematic uncertainties. With respect to local value, the CC SN rate at z=0.2 is higher by a factor of ~2 already at redshift, whereas the type Ia SN rate remains almost constant. This implies that a significant fraction of SN Ia progenitors has a lifetime longer than 2-3 Gyr. We also measured the SN rates in the red and blue galaxies and found that the SN Ia rate seems to be constant in galaxies of different colour, whereas the CC SN rate seems to peak in blue galaxies, as in the local Universe. SN rates per unit volume were found to be consistent with other measurements showing a steeper evolution with redshift for CC SNe with respect to SNe Ia. Finally we have exploited the link between star formation (SF) and SN rates to predict the evolutionary behaviour of the SN rates and compare it with the path indicated by observations.

M. T. Botticella; M. Riello; E. Cappellaro; S. Benetti; G. Altavilla; A. Pastorello; M. Turatto; L. Greggio; F. Patat; S. Valenti; L. Zampieri; A. Harutyunyan; G. Pignata; S. Taubenberger

2007-10-19T23:59:59.000Z

490

DISCOVERING BRIGHT QUASARS AT INTERMEDIATE REDSHIFTS BASED ON OPTICAL/NEAR-INFRARED COLORS  

SciTech Connect (OSTI)

The identification of quasars at intermediate redshifts (2.2 < z < 3.5) has been inefficient in most previous quasar surveys since the optical colors of quasars are similar to those of stars. The near-IR K-band excess technique has been suggested to overcome this difficulty. Our recent study also proposed to use optical/near-IR colors for selecting z < 4 quasars. To verify the effectiveness of this method, we selected a list of 105 unidentified bright targets with i ? 18.5 from the quasar candidates of SDSS DR6 with both SDSS ugriz optical and UKIDSS YJHK near-IR photometric data, which satisfy our proposed Y – K/g – z criterion and have photometric redshifts between 2.2 and 3.5 estimated from the nine-band SDSS-UKIDSS data. We observed 43 targets with the BFOSC instrument on the 2.16 m optical telescope at Xinglong station of the National Astronomical Observatory of China in the spring of 2012. We spectroscopically identified 36 targets as quasars with redshifts between 2.1 and 3.4. The high success rate of discovering these quasars in the SDSS spectroscopic surveyed area further demonstrates the robustness of both the Y – K/g – z selection criterion and the photometric redshift estimation technique. We also used the above criterion to investigate the possible stellar contamination rate among the quasar candidates of SDSS DR6, and found that the rate is much higher when selecting 3 < z < 3.5 quasar candidates than when selecting lower redshift candidates (z < 2.2). The significant improvement in the photometric redshift estimation when using the nine-band SDSS-UKIDSS data over the five-band SDSS data is demonstrated and a catalog of 7727 unidentified quasar candidates in SDSS DR6 selected with optical/near-IR colors and having photometric redshifts between 2.2 and 3.5 is provided. We also tested the Y – K/g – z selection criterion with the recently released SDSS-III/DR9 quasar catalog and found that 96.2% of 17,999 DR9 quasars with UKIDSS Y- and K-band data satisfy our criterion. With some available samples of red quasars and type II quasars, we find that 88% and 96.5% of these objects can be selected by the Y – K/g – z criterion, respectively, which supports our claim that using the Y – K/g – z criterion efficiently selects both unobscured and obscured quasars. We discuss the implications of our results on the ongoing and upcoming large optical and near-IR sky surveys.

Wu, Xue-Bing; Zuo, Wenwen; Yang, Jinyi; Yang, Qian; Wang, Feige, E-mail: wuxb@pku.edu.cn [Department of Astronomy, Peking University, Beijing 100871 (China)

2013-10-01T23:59:59.000Z

491

New No-Cost ANTFARM Tool Maps Control System Networks to Help...  

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

Corporation's Critical Infrastructure Protection (NERC CIP) standards. New No-Cost ANTFARM Tool Maps Control System Networks to Help Implement Cyber Security Standards...

492

AGN Environments in the Sloan Digital Sky Survey I: Dependence on Type, Redshift, and Luminosity  

E-Print Network [OSTI]

We explore how the local environment is related to the redshift, type, and luminosity of active galactic nuclei (AGN). Recent simulations and observations are converging on the view that the extreme luminosity of quasars is fueled in major mergers of gas-rich galaxies. In such a picture, quasars are expected to be located in regions with a higher density of galaxies on small scales where mergers are more likely to take place. However, in this picture, the activity observed in low-luminosity AGN is due to secular processes that are less dependent on the local galaxy density. To test this hypothesis, we compare the local photometric galaxy density on kiloparsec scales around spectroscopic Type I and Type II quasars to the local density around lower luminosity spectroscopic Type I and Type II AGN. To minimize projection effects and evolution in the photometric galaxy sample we use to characterize AGN environments, we place our random control sample at the same redshift as our AGN and impose a narrow redshift window around both the AGN and control targets. We find that higher luminosity AGN have more overdense environments compared to lower luminosity AGN on all scales out to our $2\\Mpchseventy$ limit. Additionally, in the range $0.3\\leqslant z\\leqslant 0.6$, Type II quasars have similarly overdense environments to those of bright Type I quasars on all scales out to our $2\\Mpchseventy$ limit, while the environment of dimmer Type I quasars appears to be less overdense than the environment of Type II quasars. We see increased overdensity for Type II AGN compared to Type I AGN on scales out to our limit of $2\\Mpchseventy$ in overlapping redshift ranges. We also detect marginal evidence for evolution in the number of galaxies within $2\\Mpchseventy$ of a quasar with redshift.

Natalie E. Strand; Robert J. Brunner; Adam D. Myers

2008-07-24T23:59:59.000Z

493

The DEEP2 Galaxy Redshift Survey: The Voronoi-Delaunay Method Catalog of Galaxy Groups  

SciTech Connect (OSTI)

We use the first 25% of the DEEP2 Galaxy Redshift Survey spectroscopic data to identify groups and clusters of galaxies in redshift space. The data set contains 8370 galaxies with confirmed redshifts in the range 0.7 {<=} z {<=} 1.4, over one square degree on the sky. Groups are identified using an algorithm (the Voronoi-Delaunay Method) that has been shown to accurately reproduce the statistics of groups in simulated DEEP2-like samples. We optimize this algorithm for the DEEP2 survey by applying it to realistic mock galaxy catalogs and assessing the results using a stringent set of criteria for measuring group-finding success, which we develop and describe in detail here. We find in particular that the group-finder can successfully identify {approx}78% of real groups and that {approx}79% of the galaxies that are true members of groups can be identified as such. Conversely, we estimate that {approx}55% of the groups we find can be definitively identified with real groups and that {approx}46% of the galaxies we place into groups are interloper field galaxies. Most importantly, we find that it is possible to measure the distribution of groups in redshift and velocity dispersion, n({sigma}, z), to an accuracy limited by cosmic variance, for dispersions greater than 350 km s{sup -1}. We anticipate that such measurements will allow strong constraints to be placed on the equation of state of the dark energy in the future. Finally, we present the first DEEP2 group catalog, which assigns 32% of the galaxies to 899 distinct groups with two or more members, 153 of which have velocity dispersions above 350 km s{sup -1}. We provide locations, redshifts and properties for this high-dispersion subsample. This catalog represents the largest sample to date of spectroscopically detected groups at z {approx} 1.

Gerke, Brian F.; /UC, Berkeley; Newman, Jeffrey A.; /LBNL, NSD; Davis, Marc; /UC, Berkeley /UC, Berkeley, Astron.Dept.; Marinoni, Christian; /Brera Observ.; Yan, Renbin; Coil, Alison L.; Conroy, Charlie; Cooper, Michael C.; /UC, Berkeley, Astron.Dept.; Faber, S.M.; /Lick Observ.; Finkbeiner, Douglas P.; /Princeton U. Observ.; Guhathakurta, Puragra; /Lick Observ.; Kaiser, Nick; /Hawaii U.; Koo, David C.; Phillips, Andrew C.; /Lick Observ.; Weiner, Benjamin J.; /Maryland U.

2012-02-14T23:59:59.000Z

494

CLUSTER LENSING PROFILES DERIVED FROM A REDSHIFT ENHANCEMENT OF MAGNIFIED BOSS-SURVEY GALAXIES  

SciTech Connect (OSTI)

We report the first detection of a redshift-depth enhancement of background galaxies magnified by foreground clusters. Using 300,000 BOSS survey galaxies with accurate spectroscopic redshifts, we measure their mean redshift depth behind four large samples of optically selected clusters from the Sloan Digital Sky Survey (SDSS) surveys, totaling 5000-15,000 clusters. A clear trend of increasing mean redshift toward the cluster centers is found, averaged over each of the four cluster samples. In addition, we find similar but noisier behavior for an independent X-ray sample of 158 clusters lying in the foreground of the current BOSS sky area. By adopting the mass-richness relationships appropriate for each survey, we compare our results with theoretical predictions for each of the four SDSS cluster catalogs. The radial form of this redshift enhancement is well fitted by a richness-to-mass weighted composite Navarro-Frenk-White profile with an effective mass ranging between M{sub 200} {approx} 1.4-1.8 Multiplication-Sign 10{sup 14} M{sub Sun} for the optically detected cluster samples, and M{sub 200} {approx} 5.0 Multiplication-Sign 10{sup 14} M{sub Sun} for the X-ray sample. This lensing detection helps to establish the credibility of these SDSS cluster surveys, and provides a normalization for their respective mass-richness relations. In the context of the upcoming bigBOSS, Subaru Prime Focus Spectrograph, and EUCLID-NISP spectroscopic surveys, this method represents an independent means of deriving the masses of cluster samples for examining the cosmological evolution, and provides a relatively clean consistency check of weak-lensing measurements, free from the systematic limitations of shear calibration.

Coupon, Jean; Umetsu, Keiichi [Institute of Astronomy and Astrophysics, Academia Sinica, P.O. Box 23-141, Taipei 10617, Taiwan (China); Broadhurst, Tom, E-mail: coupon@asiaa.sinica.edu.tw [Department of Theoretical Physics, University of Basque Country UPV/EHU, P.O. Box 644, E-48080 Bilbao (Spain)

2013-07-20T23:59:59.000Z

495

Corporate Operating Experience Program | Department of Energy  

Office of Environmental Management (EM)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "of Energy Power Systems EngineeringDepartmentSmart GridThird Quarter

496

EM Corporate Performance Metrics, Complex Level  

Office of Environmental Management (EM)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "of Energy Power SystemsResources DOE ZeroThreeEnergyDepartment0: DOE512: Alaska EM| DepartmentComplex

497

EM Corporate Performance Metrics, Site Level  

Office of Environmental Management (EM)

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "of Energy Power SystemsResources DOE ZeroThreeEnergyDepartment0: DOE512: Alaska EM|

498

TrakLok Corporation | Department of Energy  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr May Jun Jul(Summary) "ofEarlyEnergyDepartment of EnergyProgram2-26 Date: March 2, 2012 To:EnergyA vacantpumping system7AC

499

Sandia National Laboratories: New Jersey Transit Corporation  

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

AFDC Printable Version Share this resource Send a link to EERE: Alternative Fuels Data Center Home Page to someone by E-mail Share EERE: Alternative Fuels Data Center Home Page on Facebook Tweet about EERE: Alternative Fuels Data Center Home Page on Twitter Bookmark EERE:1 First Use of Energy for All Purposes (Fuel and Nonfuel),Feet) Year Jan Feb Mar Apr MayAtmosphericNuclear Security Administration the1 -theErik Spoerke SSLSMolten-Salt Storage SystemAir ForceBoard of PublicTransit

500

The Corporate Headquarters for Alabama Power Company  

E-Print Network [OSTI]

of the "product", and also helps to delay require ments for future generating capacity. Therefore, cooling for the complex will be provided by a state of-the-art refrigeration plant and ice storage system which is capable of producing and storing one and a... 16-18, 1987 I Typical Peak Demand Breakdown Commercial Building LIGHTING (39.4%) AIR HANDLING (10.8%) / COOLING AUX (5.2%) Figure 1 DESIGN APPROACH Specific objectives established by Alabama Power for the project include: - Reduce peak...

Reardon, J. G.; Penuel, K. M.