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          Institute: MPI für Gravitationsphysik     Collection: Laser Interferometry & Gravitational Wave Astronomy     Display Documents



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ID: 442863.0, MPI für Gravitationsphysik / Laser Interferometry & Gravitational Wave Astronomy
A burst search for gravitational waves from binary black holes
Authors:Pankow, C.; Klimenko, S.; Mitselmakher, G.; Yakushin, I.; Vedovato, G.; Drago, M.; Mercer, R. A.; Ajith, P.
Date of Publication (YYYY-MM-DD):2009-10-21
Title of Journal:Classical and Quantum Gravity
Volume:26
Issue / Number:20
Sequence Number of Article:204004
Review Status:not specified
Audience:Not Specified
Abstract / Description:Compact binary coalescence (CBC) is one of the most promising sources of gravitational waves. These sources are usually searched for with matched filters which require accurate calculation of the GW waveforms and generation of large template banks. We present a complementary search technique based on algorithms used in un-modeled searches. Initially designed for detection of un-modeled bursts, which can span a very large set of waveform morphologies, the search algorithm presented here is constrained for targeted detection of the smaller subset of CBC signals. The constraint is based on the assumption of elliptical polarization for signals received at the detector. We expect that the algorithm is sensitive to CBC signals in a wide range of masses, mass ratios and spin parameters. In preparation for the analysis of data from the fifth LIGO-Virgo science run (S5), we performed preliminary studies of the algorithm on test data. We present the sensitivity of the search to different types of simulated binary black hole waveforms. Also, we discuss how to extend the results of the test run into a search over all of the current LIGO-Virgo data set.
External Publication Status:published
Document Type:Article
Communicated by:Karsten Danzmann
Affiliations:MPI für Gravitationsphysik/Laser Interferometry & Gravitational Wave Astronomy
Identifiers:ISI:000270514600005 [ID No:1]
ISSN:0264-9381 [ID No:2]
DOI:10.1088/0264-9381/26/20/204004
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