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

dc.contributor.authorAbbott, B. P.
dc.contributor.authorDavies, G. S.
dc.contributor.authorLIGO Scientific Collaboration and Virgo Collaboration
dc.date.accessioned2017-04-06T10:19:24Z
dc.date.available2017-04-06T10:19:24Z
dc.date.issued2016-06
dc.description.abstractOn 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.en_UK
dc.identifier.citationAbbott, BP., et al., (LIGO Scientific Collaboration and Virgo Collaboration). (2016) Characterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914. Classical and Quantum Gravity, Volume 33, Issue 13, July 2016, Article number 134001en_UK
dc.identifier.urihttp://dspace.lib.cranfield.ac.uk/handle/1826/11737
dc.identifier.urihttp://dx.doi.org/10.1088/0264-9381/33/13/134001
dc.publisherInstitute of Physicsen_UK
dc.rightsAttribution 3.0
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/
dc.titleCharacterization of transient noise in Advanced LIGO relevant to gravitational wave signal GW150914en_UK
dc.typeArticleen_UK

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