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Progress on stochastic background search codes for LIGO

John T. Whelan·Warren G. Anderson·Martha Casquette·Mario C. Diaz·Ik Siong Heng·Martin McHugh·Joseph D. Romano·Charlie W. Torres Jr.·Rosa M. Trejo·Alberto Vecchio
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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.

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John T. Whelan, Warren G. Anderson, Martha Casquette, Mario C. Diaz, Ik Siong Heng, Martin McHugh, Joseph D. Romano, Charlie W. Torres Jr., Rosa M. Trejo, Alberto Vecchio. 2001-10-02. Progress on stochastic background search codes for LIGO. https://doi.org/10.1088/0264-9381%2F19%2F7%2F339

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