Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914

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dc.identifier.uri http://dx.doi.org/10.15488/2383
dc.identifier.uri http://www.repo.uni-hannover.de/handle/123456789/2409
dc.contributor.author Abbott, B.P.
dc.contributor.author Abbott, R.
dc.contributor.author Abbott, T.D.
dc.contributor.author Abernathy, M.R.
dc.contributor.author Acernese, F.
dc.contributor.author et al.
dc.contributor.author LIGO Scientific Collaboration
dc.contributor.author Virgo Collaboration
dc.date.accessioned 2017-11-24T08:14:38Z
dc.date.available 2017-11-24T08:14:38Z
dc.date.issued 2016
dc.identifier.citation Abbott, B.P.; Abbott, R.; Abbott, T.D.; Abernathy, M.R.; Acernese, F.; et al. (LIGO Scientific Collaboration and Virgo Collaboration): Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914. In: Classical and Quantum Gravity 33 (2016), 134001. DOI: https://doi.org/10.1088/0264-9381/33/13/134001
dc.description.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. eng
dc.language.iso eng
dc.publisher Bristol : IOP Publishing Ltd.
dc.relation.ispartofseries Classical and Quantum Gravity 33 (2016)
dc.rights CC BY 3.0 Unported
dc.rights.uri https://creativecommons.org/licenses/by/3.0/
dc.subject transient noise eng
dc.subject Advanced LIGO eng
dc.subject gravitational wave eng
dc.subject GW150914 eng
dc.subject Gravitationswelle ger
dc.subject.ddc 530 | Physik ger
dc.title Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914 eng
dc.type Article
dc.type Text
dc.relation.doi https://doi.org/10.1088/0264-9381/33/13/134001
dc.bibliographicCitation.volume 33
dc.bibliographicCitation.firstPage 134001
dc.description.version publishedVersion
tib.accessRights frei zug�nglich


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