Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/100638
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Type: Journal article
Title: Characterization of the LIGO detectors during their sixth science run
Author: Aasi, J.
Abadie, J.
Abbott, B.
Abbott, R.
Abbott, T.
Abernathy, M.
Accadia, T.
Acernese, F.
Adams, C.
Adams, T.
Adhikari, R.
Affeldt, C.
Agathos, M.
Aggarwal, N.
Aguiar, O.
Ajith, P.
Allen, B.
Allocca, A.
Ceron, E.
Amariutei, D.
et al.
Citation: Classical and Quantum Gravity, 2015; 32(11):115012-1-115012-30
Publisher: IOP Publishing
Issue Date: 2015
ISSN: 0264-9381
1361-6382
Statement of
Responsibility: 
J Aasi ... David J Hosken ... W Kim ... Eleanor J King ... Jesper Munch ... David J Ottaway ... Peter J Veitch ... et al.
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 (GWs) of astrophysical origin. The sensitivity 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 GW readout. Here we review the performance of the LIGO instruments during this epoch, the work done to characterize the detectors and their data, and the effect that transient and continuous noise artefacts have on the sensitivity of LIGO to a variety of astrophysical sources.
Keywords: LIGO; gravitational waves; detector characterization
Rights: © 2015 IOP Publishing Ltd.
RMID: 0030030565
DOI: 10.1088/0264-9381/32/11/115012
Appears in Collections:Physics publications

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