Characterization of the LIGO detectors during their sixth science run

Abstract : In 2009-2010, the Laser Interferometer Gravitational-wave Observatory (LIGO) operated together with international partners Virgo and GEO600 as a network to search for gravitational waves of astrophysical origin. The sensitiv- ity of these detectors was limited by a combination of noise sources inherent to the instrumental design and its environment, often localized in time or frequency, that couple into the gravitational-wave readout. Here we review the performance of the LIGO instruments during this epoch, the work done to characterize the de- tectors and their data, and the effect that transient and continuous noise artefacts have on the sensitivity of LIGO to a variety of astrophysical sources.
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J. Aasi, M.-A. Bizouard, V. Brisson, F. Cavalier, M. Davier, et al.. Characterization of the LIGO detectors during their sixth science run. Classical and Quantum Gravity, IOP Publishing, 2015, 32 (11), pp.115012. ⟨10.1088/0264-9381/32/11/115012⟩. ⟨in2p3-01078464⟩

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