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Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/58064
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dc.contributor.authorHosken, D.-
dc.contributor.authorMunch, J.-
dc.contributor.authorOttaway, D.-
dc.contributor.authorVeitch, P.-
dc.date.issued2009-
dc.identifier.citationPhysical Review D: Particles, Fields, Gravitation and Cosmology, 2009; 80(10):102002-1-102002-14-
dc.identifier.issn1550-7998-
dc.identifier.issn1550-2368-
dc.identifier.urihttp://hdl.handle.net/2440/58064-
dc.description.abstractWe present an all-sky search for gravitational waves in the frequency range 1 to 6 kHz during the first calendar year of LIGO's fifth science run. This is the first untriggered LIGO burst analysis to be conducted above 3 kHz. We discuss the unique properties of interferometric data in this regime. 161.3 days of triple-coincident data were analyzed. No gravitational events above threshold were observed and a frequentist upper limit of 5.4 events per year on the rate of strong gravitational wave bursts was placed at a 90% confidence level. Implications for specific theoretical models of gravitational wave emission are also discussed.-
dc.description.statementofresponsibilityB. Abbott... D. J. Hosken... J. Munch... D. J. Ottaway... P. J. Veitch...et al. (LIGO Scientific Collaboration)-
dc.language.isoen-
dc.publisherAmerican Physical Soc-
dc.rights© 2009 The American Physical Society-
dc.source.urihttp://dx.doi.org/10.1103/physrevd.80.102002-
dc.subjectGeneral Relativity and Quantum Cosmology (gr-qc)-
dc.titleSearch for high frequency gravitational-wave bursts in the first calendar year of LIGO's fifth science run-
dc.typeJournal article-
dc.identifier.doi10.1103/PhysRevD.80.102002-
pubs.publication-statusPublished-
dc.identifier.orcidOttaway, D. [0000-0001-6794-1591]-
dc.identifier.orcidVeitch, P. [0000-0002-2597-435X]-
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