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arXiv · 0801.3429

Searching for stochastic gravitational-wave background with the co-located LIGO interferometers

Abstract

This paper presents techniques developed by the LIGO Scientific Collaboration to search for the stochastic gravitational-wave background using the co-located pair of LIGO interferometers at Hanford, WA. We use correlations between interferometers and environment monitoring instruments, as well as time-shifts between two interferometers (described here for the first time) to identify correlated noise from non-gravitational sources. We veto particularly noisy frequency bands and assess the level of residual non-gravitational coupling that exists in the surviving data.

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BibTeXRIS

Nickolas V Fotopoulos. 2008-01-22. Searching for stochastic gravitational-wave background with the co-located LIGO interferometers. https://doi.org/10.1088/1742-6596%2F122%2F1%2F012032

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