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

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Authors

  • TAMA Collaboration

External Research Organisations

  • University of Tokyo
  • National Astronomical Observatory of Japan (NAOJ)
  • Hirosaki University
  • Niigata University
  • Osaka University
  • Tohoku University
  • High Energy Accelerator Research Organization (KEK)
  • University of Texas at Brownsville
  • Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
  • Tokyo Institute of Technology
  • Pennsylvania State University
  • Osaka City University
  • National Science Foundation (NSF)
  • Kyoto University
  • Kindai University
  • Ochanomizu University
  • Hiroshima University
  • Tokyo Denki University
  • Miyagi University of Education
  • California Institute of Caltech (Caltech)
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Details

Original languageEnglish
Article number122002
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume74
Issue number12
Publication statusPublished - 21 Dec 2006
Externally publishedYes

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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Cite this

Results of the search for inspiraling compact star binaries from TAMA300's observation in 2000-2004. / TAMA Collaboration.
In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 74, No. 12, 122002, 21.12.2006.

Research output: Contribution to journalArticleResearchpeer review

TAMA Collaboration. Results of the search for inspiraling compact star binaries from TAMA300's observation in 2000-2004. Physical Review D - Particles, Fields, Gravitation and Cosmology. 2006 Dec 21;74(12):122002. doi: 10.48550/arXiv.gr-qc/0610064, 10.1103/PhysRevD.74.122002
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title = "Results of the search for inspiraling compact star binaries from TAMA300's observation in 2000-2004",
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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AU - TAMA Collaboration

AU - Akutsu, Tomomi

AU - Akutsu, Tomotada

AU - Ando, Masaki

AU - Arai, Koji

AU - Araya, Akito

AU - Asada, Hideki

AU - Aso, Youichi

AU - Barton, Mark A.

AU - Beyersdorf, Peter

AU - Fujiki, Youhei

AU - Fujimoto, Masa Katsu

AU - Fujita, Ryuichi

AU - Fukushima, Mitsuhiro

AU - Futamase, Toshifumi

AU - Hamuro, Yusaku

AU - Haruyama, Tomiyoshi

AU - Hayakawa, Hideaki

AU - Hayama, Kazuhiro

AU - Heinzel, Gerhard

AU - Horikoshi, Gen'ichi

AU - Iguchi, Hideo

AU - Iida, Yukiyoshi

AU - Ioka, Kunihito

AU - Ishitsuka, Hideki

AU - Kamikubota, Norihiko

AU - Kanda, Nobuyuki

AU - Kaneyama, Takaharu

AU - Karasawa, Yoshikazu

AU - Kasahara, Kunihiko

AU - Kasai, Taketoshi

AU - Katsuki, Mayu

AU - Kawabe, Keita

AU - Kawamura, Mari

AU - Kawamura, Seiji

AU - Kawashima, Nobuki

AU - Kawazoe, Fumiko

AU - Kojima, Yasufumi

AU - Kokeyama, Keiko

AU - Kondo, Kazuhiro

AU - Kozai, Yoshihide

AU - Kudoh, Hideaki

AU - Kuroda, Kazuaki

AU - Kuwabara, Takashi

AU - Matsuda, Namio

AU - Mio, Norikatsu

AU - Miura, Kazuyuki

AU - Miyakawa, Osamu

AU - Miyama, Shoken

AU - Miyoki, Shinji

AU - Yamamoto, Kazuhiro

PY - 2006/12/21

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N2 - 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.

AB - 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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U2 - 10.48550/arXiv.gr-qc/0610064

DO - 10.48550/arXiv.gr-qc/0610064

M3 - Article

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JO - Physical Review D - Particles, Fields, Gravitation and Cosmology

JF - Physical Review D - Particles, Fields, Gravitation and Cosmology

SN - 1550-7998

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