dc.identifier.uri |
http://dx.doi.org/10.15488/2119 |
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dc.identifier.uri |
http://www.repo.uni-hannover.de/handle/123456789/2144 |
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dc.contributor.author |
Abbott, B.P.
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dc.contributor.author |
Allen, Bruce
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dc.contributor.author |
Aufmuth, Peter
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dc.contributor.author |
Bisht, A.
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dc.contributor.author |
Danzmann, Karsten
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dc.contributor.author |
Denker, T.
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dc.contributor.author |
Heurs, M.
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dc.contributor.author |
Kaufer, S.
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dc.contributor.author |
Krueger, C.
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dc.contributor.author |
Lough, J.D.
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dc.contributor.author |
Lück, Harald
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dc.contributor.author |
Sawadsky, A.
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dc.contributor.author |
Schütte, D.
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dc.contributor.author |
Steinmeyer, D.
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dc.contributor.author |
Vahlbruch, H.
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dc.contributor.author |
Willke, Benno
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dc.contributor.author |
Wimmer, M.H.
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dc.contributor.author |
Wittel, H.
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dc.contributor.author |
et al.
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dc.contributor.author |
LIGO Scientific Collaboration
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dc.contributor.author |
Virgo Collaboration
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dc.date.accessioned |
2017-10-26T07:04:21Z |
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dc.date.available |
2017-10-26T07:04:21Z |
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dc.date.issued |
2016 |
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dc.identifier.citation |
Abbott, B.P.; Abbott, R.; Abbott, T.D.; Abernathy, M.R.; Acernese, F. et al: Comprehensive all-sky search for periodic gravitational waves in the sixth science run LIGO data. In: Physical Review D 94 (2016), Nr. 4, No. 42002. DOI: https://doi.org/10.1103/PhysRevD.94.042002 |
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dc.description.abstract |
We report on a comprehensive all-sky search for periodic gravitational waves in the frequency band 100–1500 Hz and with a frequency time derivative in the range of [−1.18,+1.00]×10−8 Hz/s. Such a signal could be produced by a nearby spinning and slightly nonaxisymmetric isolated neutron star in our galaxy. This search uses the data from the initial LIGO sixth science run and covers a larger parameter space with respect to any past search. A Loosely Coherent detection pipeline was applied to follow up weak outliers in both Gaussian (95% recovery rate) and non-Gaussian (75% recovery rate) bands. No gravitational wave signals were observed, and upper limits were placed on their strength. Our smallest upper limit on worst-case (linearly polarized) strain amplitude h0 is 9.7×10−25 near 169 Hz, while at the high end of our frequency range we achieve a worst-case upper limit of 5.5×10−24. Both cases refer to all sky locations and entire range of frequency derivative values. © 2016 The American Physical Society |
eng |
dc.language.iso |
eng |
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dc.publisher |
College Park, MD : American Physical Society |
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dc.relation.ispartofseries |
Physical Review D 94 (2016), Nr. 4 |
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dc.rights |
Es gilt deutsches Urheberrecht. Das Dokument darf zum eigenen Gebrauch kostenfrei genutzt, aber nicht im Internet bereitgestellt oder an Außenstehende weitergegeben werden. |
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dc.subject |
Gravitational waves |
eng |
dc.subject |
Gravitational wave detectors |
eng |
dc.subject |
Gravitationswelle |
ger |
dc.subject.ddc |
530 | Physik
|
ger |
dc.title |
Comprehensive all-sky search for periodic gravitational waves in the sixth science run LIGO data |
eng |
dc.type |
Article |
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dc.type |
Text |
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dc.relation.issn |
2470-0010 |
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dc.relation.doi |
https://doi.org/10.1103/PhysRevD.94.042002 |
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dc.bibliographicCitation.issue |
4 |
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dc.bibliographicCitation.volume |
94 |
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dc.bibliographicCitation.firstPage |
42002 |
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dc.description.version |
publishedVersion |
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tib.accessRights |
frei zug�nglich |
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