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2002 Class. Quantum Grav. 19 1521-1527 doi: 10.1088/0264-9381/19/7/339
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Abstract. One of the types of signals for which the LIGO interferometric gravitational wave detectors will search is a stochastic background of gravitational radiation. We review the technique of searching for a background using the optimally filtered cross-correlation statistic, and describe the state of plans to perform such cross-correlations between the two LIGO interferometers as well as between LIGO and other gravitational-wave detectors, in particular the preparation of software to perform such data analysis.
PACS numbers: 0430, 0480N, 9780V
Print publication: Issue 7 (7 April 2002)| Post to CiteUlike | | Post to Connotea | | Post to Bibsonomy |
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