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공공누리This item is licensed Korea Open Government License

dc.contributor.author
ANTARES Collaboration, IceCube Collaboration, 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
2017-06-12
dc.identifier.issn
2470-0010
dc.identifier.uri
https://repository.kisti.re.kr/handle/10580/14695
dc.identifier.uri
http://www.ndsl.kr/ndsl/search/detail/article/articleSearchResultDetail.do?cn=NART78526987
dc.description.abstract
The Advanced LIGO observatories detected gravitational waves from two binary black hole mergersduring their first observation run (O1). We present a high-energy neutrino follow-up search for the secondgravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012.We find twoand four neutrino candidates detected by IceCube, and one and zero detected by ANTARES, within +-500 saround the respective gravitational wave signals, consistent with the expected background rate. None ofthese neutrino candidates are found to be directionally coincident with GW151226 or LVT151012.We usenondetection to constrain isotropic-equivalent high-energy neutrino emission from GW151226, adoptingthe GW event’s 3D localization, to less than 2 × 1051–2 × 10^54 erg.
dc.language
eng
dc.relation.ispartofseries
Physical Review D
dc.title
Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube
dc.citation.startPage
022005
dc.citation.volume
96
dc.subject.keyword
neutrinos
dc.subject.keyword
gravitational wave
dc.subject.keyword
GW151226
dc.subject.keyword
LVT151012
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