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dc.contributor.authorAbbott, B.en
dc.contributor.authorAbbott, R.en
dc.contributor.authorAdhikari, R.en
dc.contributor.authorAgresti, J.en
dc.contributor.authorAllen, B.en
dc.contributor.authorAllen, G.en
dc.contributor.authorAmin, R.en
dc.contributor.authorAnderson, S.en
dc.contributor.authorAnderson, W.en
dc.contributor.authorAraya, M.en
dc.contributor.authorArmandula, H.en
dc.contributor.authorAshley, M.en
dc.contributor.authorAulbert, C.en
dc.contributor.authorBabak, S.en
dc.contributor.authorBalasubramanian, R.en
dc.contributor.authorBallmer, S.en
dc.contributor.authorBarish, B.en
dc.contributor.authorBarker, C.en
dc.contributor.authorBarker, D.en
dc.contributor.authorBarton, M.en
dc.contributor.authoret al.en
dc.identifier.citationPhysical Review Letters, 2005; 95(22):221101-1-221101-6en
dc.description.abstractThe Laser Interferometer Gravitational-Wave Observatory has performed a third science run with much improved sensitivities of all three interferometers. We present an analysis of approximately 200 hours of data acquired during this run, used to search for a stochastic background of gravitational radiation. We place upper bounds on the energy density stored as gravitational radiation for three different spectral power laws. For the flat spectrum, our limit of Ω0<8.4×10-4 in the 69–156 Hz band is ∼105 times lower than the previous result in this frequency range.en
dc.description.statementofresponsibilityB. Abbott... D. J. Ottaway... et al.(LIGO Scientific Collaboration)en
dc.publisherAmerican Physical Socen
dc.rights©2005 American Physical Societyen
dc.subjectLIGO Scientific Collaborationen
dc.titleUpper limits on a stochastic background of gravitational wavesen
dc.typeJournal articleen
pubs.library.collectionPhysics publicationsen
dc.identifier.orcidOttaway, D. [0000-0001-6794-1591]en
Appears in Collections:Physics publications

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