Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/101289
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Type: Journal article
Title: Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914
Author: Abbott, B.
Abbott, R.
Abbott, T.
Abernathy, M.
Acernese, F.
Ackley, K.
Adamo, M.
Adams, C.
Adams, T.
Addesso, P.
Adhikari, R.
Adya, V.
Affeldt, C.
Agathos, M.
Agatsuma, K.
Aggarwal, N.
Aguiar, O.
Aiello, L.
Ain, A.
Ajith, P.
et al.
Citation: Classical and Quantum Gravity, 2016; 33(13):134001-1-134001-34
Publisher: IOP Publishing
Issue Date: 2016
ISSN: 0264-9381
1361-6382
Statement of
Responsibility: 
B.P. Abbott … S.E. Hollitt … D.J. Hosken … E.J. King … J. Munch … D.J. Ottaway … P.J. Veitch … et al. (LIGO Scientific Collaboration and Virgo Collaboration)
Abstract: On 14 September 2015, a gravitational wave signal from a coalescing black hole binary system was observed by the Advanced LIGO detectors. This paper describes the transient noise backgrounds used to determine the significance of the event (designated GW150914) and presents the results of investigations into potential correlated or uncorrelated sources of transient noise in the detectors around the time of the event. The detectors were operating nominally at the time of GW150914. We have ruled out environmental influences and non-Gaussian instrument noise at either LIGO detector as the cause of the observed gravitational wave signal.
Keywords: Gravitational waves; detector characterization; GW150914
Rights: © 2016 IOP Publishing Ltd
RMID: 0030050516
DOI: 10.1088/0264-9381/33/13/134001
Appears in Collections:Physics publications

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