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

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

2008-01-22

arxiv.org/abs/0801.3429v1

J.Phys.Conf.Ser.122:012032,2008

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Proceedings paper from the 7th Edoardo Amaldi Conference on Gravitational Waves, held in Sydney, Australia from 8-14 July 2007

Scientific paper

10.1088/1742-6596/122/1/012032

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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