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Conference Paper

Prospects for Stochastic Background Searches Using Virgo and LSC Interferometers

MPS-Authors
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Robinson,  Emma L.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Whelan,  John T.
Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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cqg7_19_s26.pdf
(Publisher version), 228KB

0704.2983v2.pdf
(Preprint), 233KB

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Citation

Cella, G., Colacino, C. N., Cuoco, E., Di Virgilio, A., Regimbau, T., Robinson, E. L., et al. (2007). Prospects for Stochastic Background Searches Using Virgo and LSC Interferometers. Classical and Quantum Gravity, 24(19 Sp. Iss. Sp. Iss. SI), S639-S648.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0013-47B1-9
Abstract
We consider the question of cross-correlation measurements using Virgo and the LSC Interferometers (LIGO Livingston, LIGO Hanford, and GEO600) to search for a stochastic gravitational-wave background. We find that inclusion of Virgo into the network will substantially improve the sensitivity to correlations above 200 Hz if all detectors are operating at their design sensitivity. This is illustrated using a simulated isotropic stochastic background signal, generated with an astrophysically-motivated spectrum, injected into 24 hours of simulated noise for the LIGO and Virgo interferometers.