Search for gravitational waves from binary black hole inspirals in LIGO data
dc.contributor.author | Abbott, B | |
dc.contributor.author | Abbott, Robert | |
dc.contributor.author | Adhikari, R | |
dc.contributor.author | Ageev, A | |
dc.contributor.author | Agresti, A | |
dc.contributor.author | Ajith, P | |
dc.contributor.author | Cusack, B J | |
dc.contributor.author | McClelland, David | |
dc.contributor.author | Scott, Susan M | |
dc.contributor.author | Searle, Antony | |
dc.contributor.author | Allen, B | |
dc.contributor.author | Allen, J | |
dc.contributor.author | Wette, Karl | |
dc.contributor.author | Amin, R | |
dc.contributor.author | Anderson, S B | |
dc.contributor.author | Heurs, M | |
dc.contributor.author | Hough, J | |
dc.date.accessioned | 2015-12-07T22:41:37Z | |
dc.date.issued | 2006 | |
dc.date.updated | 2015-12-07T11:03:33Z | |
dc.description.abstract | We 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.issn | 0556-2821 | |
dc.identifier.uri | http://hdl.handle.net/1885/24402 | |
dc.publisher | American Physical Society | |
dc.source | Physical Review D | |
dc.title | Search for gravitational waves from binary black hole inspirals in LIGO data | |
dc.type | Journal article | |
local.bibliographicCitation.lastpage | 17 | |
local.bibliographicCitation.startpage | 1 | |
local.contributor.affiliation | Abbott, B, LIGO - California Institute of Technology | |
local.contributor.affiliation | Abbott, Robert, LIGO - California Institute of Technology | |
local.contributor.affiliation | Adhikari, R, Massachusetts Institute of Technology | |
local.contributor.affiliation | Ageev, A, Syracuse University | |
local.contributor.affiliation | Agresti, A, LIGO - California Institute of Technology | |
local.contributor.affiliation | Ajith, P, Max Planck Institute for Gravitational Physics | |
local.contributor.affiliation | Cusack, B J, College of Physical and Mathematical Sciences, ANU | |
local.contributor.affiliation | McClelland, David, College of Physical and Mathematical Sciences, ANU | |
local.contributor.affiliation | Scott, Susan M, College of Physical and Mathematical Sciences, ANU | |
local.contributor.affiliation | Searle, Antony, College of Physical and Mathematical Sciences, ANU | |
local.contributor.affiliation | Allen, B, University of Wisconsin-Milwaukee | |
local.contributor.affiliation | Allen, J, LIGO Massachusetts Institute of Technology | |
local.contributor.affiliation | Wette, Karl, College of Physical and Mathematical Sciences, ANU | |
local.contributor.affiliation | Amin, R, University of Florida | |
local.contributor.affiliation | Anderson, S B, LIGO - California Institute of Technology | |
local.contributor.affiliation | Heurs, M, University of Hannover | |
local.contributor.affiliation | Hough, J, University of Glasgow | |
local.contributor.authoruid | Cusack, B J, u4022214 | |
local.contributor.authoruid | McClelland, David, u8802403 | |
local.contributor.authoruid | Scott, Susan M, u8911327 | |
local.contributor.authoruid | Searle, Antony, u9719170 | |
local.contributor.authoruid | Wette, Karl, u4090078 | |
local.description.embargo | 2037-12-31 | |
local.description.notes | Imported from ARIES | |
local.identifier.absfor | 029904 - Synchrotrons; Accelerators; Instruments and Techniques | |
local.identifier.absfor | 020110 - Stellar Astronomy and Planetary Systems | |
local.identifier.ariespublication | u4103646xPUB32 | |
local.identifier.citationvolume | 73 | |
local.identifier.doi | 10.1103/PhysRevD.73.062001 | |
local.identifier.scopusID | 2-s2.0-33644829976 | |
local.type.status | Published Version |
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