Results of the search for inspiraling compact star binaries from TAMA300's observation in 2000–2004
Physical Review D Volume 74
Page 122002-1-122002-8
published_at 2006-12-21
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Title ( eng ) |
Results of the search for inspiraling compact star binaries from TAMA300's observation in 2000–2004
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Creator |
TAMA Collaboration
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Source Title |
Physical Review D
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Volume | 74 |
Start Page | 122002-1 |
End Page | 122002-8 |
Abstract |
We analyze the data of the TAMA300 detector to search for gravitational waves from inspiraling compact star binaries with masses of the component stars in the range 1M⊙–3M⊙. In this analysis, 2705 hours of data, taken during the years 2000–2004, are used for the event search. We combine the results of different observation runs, and obtain a single upper limit on the rate of the coalescence of compact binaries in our Galaxy of 20 per year at a 90% confidence level. In this upper limit, the effects of various systematic errors such as the uncertainty of the background estimation and the calibration of the detector's sensitivity are included.
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Keywords |
binary stars
gravitational wave detectors
stellar mass
Galaxy
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Language |
eng
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Resource Type | journal article |
Publisher |
American Physical Society
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Date of Issued | 2006-12-21 |
Rights |
Copyright (c) 2006 The American Physical Society.
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Publish Type | Version of Record |
Access Rights | open access |
Source Identifier |
[ISSN] 1550-7998
[DOI] 10.1103/PhysRevD.74.122002
[NCID] AA00773624
[DOI] http://dx.doi.org/10.1103/PhysRevD.74.122002
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