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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
배상욱
dc.date.accessioned
2019-08-28T07:42:10Z
dc.date.available
2019-08-28T07:42:10Z
dc.date.issued
2017-10-06
dc.identifier.issn
0031-9007
dc.identifier.uri
https://repository.kisti.re.kr/handle/10580/14691
dc.identifier.uri
http://www.ndsl.kr/ndsl/search/detail/article/articleSearchResultDetail.do?cn=NART90629900
dc.description.abstract
On August 14, 2017 at 10∶30:43 UTC, the Advanced Virgo detector and the two Advanced LIGOdetectors coherently observed a transient gravitational-wave signal produced by the coalescence of twostellar mass black holes, with a false-alarm rate of ≲1 in 27 000 years. The signal was observed with athree-detector network matched-filter signal-to-noise ratio of 18. The inferred masses of the initial blackholes are 30.5þ5.7−3.0M⊙ and 25:3þ2.8−4.2M⊙ (at the 90% credible level). The luminosity distance of the source is540þ130−210 Mpc, corresponding to a redshift of z ¼ 0.11þ0.03−0.04 . A network of three detectors improves the skylocalization of the source, reducing the area of the 90% credible region from 1160 deg2 using only the twoLIGO detectors to 60 deg2 using all three detectors. For the first time, we can test the nature ofgravitational-wave polarizations from the antenna response of the LIGO-Virgo network, thus enabling anew class of phenomenological tests of gravity.
dc.language
eng
dc.relation.ispartofseries
Physical Review Letters
dc.title
GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
dc.citation.startPage
141101
dc.citation.volume
119
dc.subject.keyword
GW170814
dc.subject.keyword
Gravitational Waves
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