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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
조희석
dc.date.accessioned
2019-08-28T07:42:08Z
dc.date.available
2019-08-28T07:42:08Z
dc.date.issued
2017-04-07
dc.identifier.issn
0004-637X
dc.identifier.uri
https://repository.kisti.re.kr/handle/10580/14677
dc.identifier.uri
http://www.ndsl.kr/ndsl/search/detail/article/articleSearchResultDetail.do?cn=NART78519830
dc.description.abstract
We present the result of searches for gravitational waves from 200 pulsars using data from the first observing run ofthe Advanced LIGO detectors. We find no significant evidence for a gravitational-wave signal from any of thesepulsars, but we are able to set the most constraining upper limits yet on their gravitational-wave amplitudes andellipticities. For eight of these pulsars, our upper limits give bounds that are improvements over the indirect spindownlimit values. For another 32, we are within a factor of 10 of the spin-down limit, and it is likely that some ofthese will be reachable in future runs of the advanced detector. Taken as a whole, these new results improve onprevious limits by more than a factor of two.
dc.language
eng
dc.relation.ispartofseries
ASTROPHYSICAL JOURNAL
dc.title
First Search for Gravitational Waves from Known Pulsars with Advanced LIGO
dc.citation.volume
839
dc.subject.keyword
gravitational waves – pulsars
dc.subject.keyword
general
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