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An upper limit on the stochastic gravitational-wave background of cosmological origin

Research output: Contribution to journal › Article › Research › peer review

Authors

  • The LIGO Scientific Collaboration

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Original languageEnglish
Pages (from-to)990-994
JournalNATURE
Volume460
Issue number7258
Publication statusPublished - 20 Aug 2009

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An upper limit on the stochastic gravitational-wave background of cosmological origin. / The LIGO Scientific Collaboration.
In: NATURE, Vol. 460, No. 7258, 20.08.2009, p. 990-994.

Research output: Contribution to journal › Article › Research › peer review

The LIGO Scientific Collaboration. An upper limit on the stochastic gravitational-wave background of cosmological origin. NATURE. 2009 Aug 20;460(7258):990-994. doi: 10.1038/nature08278
The LIGO Scientific Collaboration. / An upper limit on the stochastic gravitational-wave background of cosmological origin. In: NATURE. 2009 ; Vol. 460, No. 7258. pp. 990-994.
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@article{cdab4849830b4decba4c4a3f65ced1ea,
title = "An upper limit on the stochastic gravitational-wave background of cosmological origin",
author = "{The LIGO Scientific Collaboration} and Abbott, {B. P.} and R. Abbott and F. Acernese and R. Adhikari and P. Ajith and B. Allen and G. Allen and M. Alshourbagy and Amin, {R. S.} and Anderson, {S. B.} and Anderson, {W. G.} and F. Antonucci and S. Aoudia and Arain, {M. A.} and M. Araya and H. Armandula and P. Armor and Arun, {K. G.} and Y. Aso and S. Aston and P. Astone and P. Aufmuth and C. Aulbert and S. Babak and P. Baker and G. Ballardin and S. Ballmer and C. Barker and D. Barker and F. Barone and B. Barr and P. Barriga and L. Barsotti and M. Barsuglia and Barton, {M. A.} and Danilishin, {S. L.} and K. Danzmann and M. Hewitson and F. Kawazoe and H. Vahlbruch and B. Willke and L. Zhang",
note = "Funding information: Acknowledgement We acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max Planck Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. We also acknowledge the support of the research by these agencies and by the Australian Research Council, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educacion y Ciencia, the Conselleria d{\textquoteright}Economia Hisenda i Innovacio of the Govern de les Illes Balears, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.",
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TY - JOUR

T1 - An upper limit on the stochastic gravitational-wave background of cosmological origin

AU - The LIGO Scientific Collaboration

AU - Abbott, B. P.

AU - Abbott, R.

AU - Acernese, F.

AU - Adhikari, R.

AU - Ajith, P.

AU - Allen, B.

AU - Allen, G.

AU - Alshourbagy, M.

AU - Amin, R. S.

AU - Anderson, S. B.

AU - Anderson, W. G.

AU - Antonucci, F.

AU - Aoudia, S.

AU - Arain, M. A.

AU - Araya, M.

AU - Armandula, H.

AU - Armor, P.

AU - Arun, K. G.

AU - Aso, Y.

AU - Aston, S.

AU - Astone, P.

AU - Aufmuth, P.

AU - Aulbert, C.

AU - Babak, S.

AU - Baker, P.

AU - Ballardin, G.

AU - Ballmer, S.

AU - Barker, C.

AU - Barker, D.

AU - Barone, F.

AU - Barr, B.

AU - Barriga, P.

AU - Barsotti, L.

AU - Barsuglia, M.

AU - Barton, M. A.

AU - Danilishin, S. L.

AU - Danzmann, K.

AU - Hewitson, M.

AU - Kawazoe, F.

AU - Vahlbruch, H.

AU - Willke, B.

AU - Zhang, L.

N1 - Funding information: Acknowledgement We acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max Planck Society, and the State of Niedersachsen/Germany for support of the construction and operation of the GEO600 detector, and the Italian Istituto Nazionale di Fisica Nucleare and the French Centre National de la Recherche Scientifique for the construction and operation of the Virgo detector. We also acknowledge the support of the research by these agencies and by the Australian Research Council, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educacion y Ciencia, the Conselleria d’Economia Hisenda i Innovacio of the Govern de les Illes Balears, the Royal Society, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P. Sloan Foundation.

PY - 2009/8/20

Y1 - 2009/8/20

U2 - 10.1038/nature08278

DO - 10.1038/nature08278

M3 - Article

VL - 460

SP - 990

EP - 994

JO - NATURE

JF - NATURE

SN - 0028-0836

IS - 7258

ER -