Search for gravitational waves from binary black hole inspirals in LIGO data

dc.contributor.authorAbbott, B
dc.contributor.authorAbbott, Robert
dc.contributor.authorAdhikari, R
dc.contributor.authorAgeev, A
dc.contributor.authorAgresti, A
dc.contributor.authorAjith, P
dc.contributor.authorCusack, B J
dc.contributor.authorMcClelland, David
dc.contributor.authorScott, Susan M
dc.contributor.authorSearle, Antony
dc.contributor.authorAllen, B
dc.contributor.authorAllen, J
dc.contributor.authorWette, Karl
dc.contributor.authorAmin, R
dc.contributor.authorAnderson, S B
dc.contributor.authorHeurs, M
dc.contributor.authorHough, J
dc.date.accessioned2015-12-07T22:41:37Z
dc.date.issued2006
dc.date.updated2015-12-07T11:03:33Z
dc.description.abstractWe report on a search for gravitational waves from binary black hole inspirals in the data from the second science run of the LIGO interferometers. The search focused on binary systems with component masses between 3 and 20M. Optimally oriented binaries with distances up to 1 Mpc could be detected with efficiency of at least 90%. We found no events that could be identified as gravitational waves in the 385.6 hours of data that we searched.
dc.identifier.issn0556-2821
dc.identifier.urihttp://hdl.handle.net/1885/24402
dc.publisherAmerican Physical Society
dc.sourcePhysical Review D
dc.titleSearch for gravitational waves from binary black hole inspirals in LIGO data
dc.typeJournal article
local.bibliographicCitation.lastpage17
local.bibliographicCitation.startpage1
local.contributor.affiliationAbbott, B, LIGO - California Institute of Technology
local.contributor.affiliationAbbott, Robert, LIGO - California Institute of Technology
local.contributor.affiliationAdhikari, R, Massachusetts Institute of Technology
local.contributor.affiliationAgeev, A, Syracuse University
local.contributor.affiliationAgresti, A, LIGO - California Institute of Technology
local.contributor.affiliationAjith, P, Max Planck Institute for Gravitational Physics
local.contributor.affiliationCusack, B J, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationMcClelland, David, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationScott, Susan M, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSearle, Antony, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationAllen, B, University of Wisconsin-Milwaukee
local.contributor.affiliationAllen, J, LIGO Massachusetts Institute of Technology
local.contributor.affiliationWette, Karl, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationAmin, R, University of Florida
local.contributor.affiliationAnderson, S B, LIGO - California Institute of Technology
local.contributor.affiliationHeurs, M, University of Hannover
local.contributor.affiliationHough, J, University of Glasgow
local.contributor.authoruidCusack, B J, u4022214
local.contributor.authoruidMcClelland, David, u8802403
local.contributor.authoruidScott, Susan M, u8911327
local.contributor.authoruidSearle, Antony, u9719170
local.contributor.authoruidWette, Karl, u4090078
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor029904 - Synchrotrons; Accelerators; Instruments and Techniques
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4103646xPUB32
local.identifier.citationvolume73
local.identifier.doi10.1103/PhysRevD.73.062001
local.identifier.scopusID2-s2.0-33644829976
local.type.statusPublished Version

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