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공공누리This item is licensed Korea Open Government License

dc.contributor.author
JAasi
dc.contributor.author
강궁원
dc.contributor.author
김정리
dc.contributor.author
장행진
dc.date.accessioned
2019-08-28T07:41:33Z
dc.date.available
2019-08-28T07:41:33Z
dc.date.issued
2014-04-03
dc.identifier.issn
0264-9381
dc.identifier.uri
https://repository.kisti.re.kr/handle/10580/14307
dc.identifier.uri
http://www.ndsl.kr/ndsl/search/detail/article/articleSearchResultDetail.do?cn=NART70834652
dc.description.abstract
We report on an all-sky search for periodic gravitational waves in the frequency range 50–1000 Hz with the first derivative of frequency in the range −8.9 × 10−10 Hz s−1 to zero in two years of data collected during LIGO's fifth science run. Our results employ a Hough transform technique, introducing a χ2 test and analysis of coincidences between the signal levels in years 1 and 2 of observations that offers a significant improvement in the product of strain sensitivity with compute cycles per data sample compared to previously published searches. Since our search yields no surviving candidates, we present results taking the form of frequency dependent, 95% confidence upper limits on the strain amplitude h0. The most stringent upper limit from year 1 is 1.0 × 10−24 in the 158.00–158.25 Hz band. In year 2, the most stringent upper limit is 8.9 × 10−25 in the 146.50–146.75 Hz band. This improved detection pipeline, which is computationally efficient by at least two orders of magnitude better than our flagship Einstein@Home search, will be important for 'quick-look' searches in the Advanced LIGO and Virgo detector era.
dc.language
eng
dc.relation.ispartofseries
Classical and Quantum Gravity
dc.title
Application of a Hough search for continuous gravitational waves on data from the fifth LIGO science run
dc.subject.keyword
Hough search
dc.subject.keyword
Continuous GW
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7. KISTI 연구성과 > 학술지 발표논문
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