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2004 Class. Quantum Grav. 21 S685-S690 doi: 10.1088/0264-9381/21/5/044
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Abstract. I describe analysis of correlations in the outputs of the three LIGO interferometers from LIGO's first science run, held over 17 days in August and September of 2002, and the resulting upper limit set on a stochastic background of gravitational waves. By searching for cross-correlations between the LIGO detectors in Livingston, LA and Hanford, WA, we are able to set a 90% confidence level upper limit of h2100Ω0 < 23 ± 4.6.
PACS numbers: 04.80.Nn, 07.05.Kf, 98.70.Vc
Print publication: Issue 5 (7 March 2004)| Post to CiteUlike | | Post to Connotea | | Post to Bibsonomy |
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