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공공누리This item is licensed Korea Open Government License

dc.contributor.author
B.P. Abbott et al.
dc.contributor.author
강궁원
dc.contributor.author
조희석
dc.date.accessioned
2019-08-28T07:42:18Z
dc.date.available
2019-08-28T07:42:18Z
dc.date.issued
2018-02-14
dc.identifier.issn
0264-9381
dc.identifier.uri
https://repository.kisti.re.kr/handle/10580/14782
dc.identifier.uri
http://www.ndsl.kr/ndsl/search/detail/article/articleSearchResultDetail.do?cn=NART90655926
dc.description.abstract
We present the results of a search for long-duration gravitational wave transients in the data of the LIGO Hanford and LIGO Livingston second generation detectors
between $ \newcommand{\OOneStart}{{\rm 12 ~September ~2015}} \newcommand{\OOneStartShort}{{\rm September ~2015}} \OOneStartShort$ and
$ \newcommand{\OOneStop}{{\rm 19~ January ~2016}} \newcommand{\OOneStopShort}{{\rm January~ 2016}} \OOneStopShort$ , with a total observational
time of $ \newcommand{\OOneLivetime}{{\rm 49~d}} \OOneLivetime$ . The search targets gravitational wave transients of 10–500 s duration in a frequency band
of 24–2048 Hz, with minimal assumptions about the signal waveform, polarization, source direction, or time of occurrence. No significant events were observed. As a
result we set 90% confidence upper limits on the rate of long-duration gravitational wave transients for different types of gravitational wave signals. We also show that
the search is sensitive to sources in the Galaxy emitting at least  
~10−8 $ \newcommand{\msuncd}{{\rm M_{\odot} c^2}} \newcommand{\msun}{{\rm M_{\odot}}} {\msuncd}$ in gravitational waves.
dc.language
eng
dc.relation.ispartofseries
Classical and Quantum Gravity
dc.title
All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run
dc.citation.number
6
dc.citation.startPage
065009
dc.citation.volume
35
dc.subject.keyword
Gravitational wave
dc.subject.keyword
LIGO O1
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7. KISTI 연구성과 > 학술지 발표논문
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