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공공누리This item is licensed Korea Open Government License

dc.contributor.author
LIGO Scientific Collaboration and Virgo Collaboration
dc.contributor.author
강궁원
dc.contributor.author
김정리
dc.contributor.author
장행진
dc.date.accessioned
2019-08-28T07:41:45Z
dc.date.available
2019-08-28T07:41:45Z
dc.date.issued
2015-05-13
dc.identifier.issn
0264-9381
dc.identifier.uri
https://repository.kisti.re.kr/handle/10580/14439
dc.identifier.uri
http://www.ndsl.kr/ndsl/search/detail/article/articleSearchResultDetail.do?cn=NART76639207
dc.description.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
dc.language
eng
dc.relation.ispartofseries
Classical and Quantum Gravity
dc.title
Characterization of the LIGO detectors during their sixth science run
dc.citation.number
11
dc.citation.volume
32
dc.subject.keyword
LIGO detectors
dc.subject.keyword
Sixth science run
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