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
Abstract
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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
Abstract
Open-access reader
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.
Key concepts: LIGO, Physics, Gravitational wave, Interferometry, Detector, Astronomical interferometer, Statistic, Gravitational wave background