Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/77506
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dc.contributor.authorAasi, J.en
dc.contributor.authorMunch, J.en
dc.contributor.authorOttaway, D.en
dc.contributor.authorVeitch, P.en
dc.date.issued2013en
dc.identifier.citationPhysical Review. D. Particles, Fields, Gravitation and Cosmology, 2013; 87(2):1-15en
dc.identifier.issn1550-7998en
dc.identifier.issn1550-2368en
dc.identifier.urihttp://hdl.handle.net/2440/77506-
dc.description.abstractWe report a search for gravitational waves from the inspiral, merger and ringdown of binary black holes (BBH) with total mass between 25 and 100 solar masses, in data taken at the LIGO and Virgo observatories between July 7, 2009 and October 20, 2010. The maximum sensitive distance of the detectors over this period for a (20,20)M⊙ coalescence was 300 Mpc. No gravitational wave signals were found. We thus report upper limits on the astrophysical coalescence rates of BBH as a function of the component masses for nonspinning components, and also evaluate the dependence of the search sensitivity on component spins aligned with the orbital angular momentum. We find an upper limit at 90% confidence on the coalescence rate of BBH with nonspinning components of mass between 19 and 28M⊙ of 3.3×10⁻⁷ mergers Mpc⁻³yr⁻¹.en
dc.description.statementofresponsibilityAasi, J...Munch, Jesper...Ottaway, David John...Veitch, Peter John... et al. (LIGO Scientific Collaboration and Virgo Collaboration)en
dc.language.isoenen
dc.publisherAmerican Physical Socen
dc.rights© 2013 American Physical Societyen
dc.titleSearch for gravitational waves from binary black hole inspiral, merger, and ringdown in LIGO-Virgo data from 2009-2010en
dc.typeJournal articleen
dc.identifier.rmid0020124690en
dc.identifier.doi10.1103/PhysRevD.87.022002en
dc.identifier.pubid21712-
pubs.library.collectionIPAS publicationsen
pubs.verification-statusVerifieden
pubs.publication-statusPublisheden
dc.identifier.orcidOttaway, D. [0000-0001-6794-1591]en
dc.identifier.orcidVeitch, P. [0000-0002-2597-435X]en
Appears in Collections:IPAS publications
Environment Institute publications

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