2002Classical and Quantum GravityOpen access

Progress on stochastic background search codes for LIGO

J. T. Whelan, W. G. Anderson, Martha Casquette, M. C. Díaz, I. S. Heng, M. McHugh, Joseph D. Romano, C. Torres, Rosa Trejo, A. 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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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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Available 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.

Key concepts: LIGO, Physics, Gravitational wave, Interferometry, Detector, Astronomical interferometer, Statistic, Gravitational wave background

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