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공공누리This item is licensed Korea Open Government License

Title
Characterization of the LIGO detectors during their sixth science run
Author(s)
LIGO Scientific Collaboration and Virgo Collaboration강궁원김정리장행진
Publication Year
2015-05-13
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
Keyword
LIGO detectors; Sixth science run
Journal Title
Classical and Quantum Gravity
Citation Volume
32
ISSN
0264-9381
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7. KISTI 연구성과 > 학술지 발표논문
URI
https://repository.kisti.re.kr/handle/10580/14439
http://www.ndsl.kr/ndsl/search/detail/article/articleSearchResultDetail.do?cn=NART76639207
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