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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
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
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
Appears in Collections:
7. KISTI 연구성과 > 학술지 발표논문
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