Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/101401
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dc.contributor.author | Abbott, B.P. | - |
dc.contributor.author | Abbott, R. | - |
dc.contributor.author | Abbott, T.D. | - |
dc.contributor.author | Abernathy, M.R. | - |
dc.contributor.author | Acernese, F. | - |
dc.contributor.author | Ackley, K. | - |
dc.contributor.author | Adams, C. | - |
dc.contributor.author | Adams, T. | - |
dc.contributor.author | Addesso, P. | - |
dc.contributor.author | Adhikari, R.X. | - |
dc.contributor.author | Adya, V.B. | - |
dc.contributor.author | Affeldt, C. | - |
dc.contributor.author | Agathos, M. | - |
dc.contributor.author | Agatsuma, K. | - |
dc.contributor.author | Aggarwal, N. | - |
dc.contributor.author | Aguiar, O.D. | - |
dc.contributor.author | Aiello, L. | - |
dc.contributor.author | Ain, A. | - |
dc.contributor.author | Ajith, P. | - |
dc.contributor.author | Allen, B. | - |
dc.contributor.author | et al. | - |
dc.date.issued | 2016 | - |
dc.identifier.citation | Physical Review D: Particles, Fields, Gravitation and Cosmology, 2016; 94(4):042002-1-042002-14 | - |
dc.identifier.issn | 1550-7998 | - |
dc.identifier.issn | 1550-2368 | - |
dc.identifier.uri | http://hdl.handle.net/2440/101401 | - |
dc.description | Published 15 August 2016 | - |
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. | - |
dc.description.statementofresponsibility | B. P. Abbott ... W. Kim ... E. J. King ... J. Munch ... D. J. Ottaway ... P. J. Veitch ... et al. (LIGO Scientific Collaboration and Virgo Collaboration) | - |
dc.language.iso | en | - |
dc.publisher | American Physical Society | - |
dc.rights | © 2016 American Physical Society | - |
dc.source.uri | http://dx.doi.org/10.1103/physrevd.94.042002 | - |
dc.title | Comprehensive all-sky search for periodic gravitational waves in the sixth science run LIGO data | - |
dc.type | Journal article | - |
dc.identifier.doi | 10.1103/PhysRevD.94.042002 | - |
pubs.publication-status | Published | - |
Appears in Collections: | Aurora harvest 7 IPAS publications |
Files in This Item:
File | Description | Size | Format | |
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hdl_101401.pdf | Published version | 959.16 kB | Adobe PDF | View/Open |
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