Results of the search for inspiraling compact star binaries from TAMA300's observation in 2000-2004

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dc.creatorTAMA Collaboration
dc.creatorAkutsu, T.
dc.date2006-10-12
dc.date2006-10-16
dc.date.accessioned2026-07-07T10:24:34Z
dc.date.available2026-07-07T10:24:34Z
dc.descriptionWe analyze the data of TAMA300 detector to search for gravitational waves from inspiraling compact star binaries with masses of the component stars in the range 1-3Msolar. 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 obtained 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 effect of various systematic errors such like the uncertainty of the background estimation and the calibration of the detector's sensitivity are included.
dc.description8 pages, 4 Postscript figures, uses revtex4.sty The author list was corrected
dc.identifierhttps://arxiv.org/abs/gr-qc/0610064
dc.identifierhttp://arxiv.org/abs/gr-qc/0610064
dc.identifierPhys.Rev.D74:122002,2006
dc.identifierdoi:10.1103/PhysRevD.74.122002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/176233
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.titleResults of the search for inspiraling compact star binaries from TAMA300's observation in 2000-2004
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