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

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-Review

Autoren

  • TAMA Collaboration

Externe Organisationen

  • University of Tokyo (UTokyo)
  • 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-Institut für Gravitationsphysik (Albert-Einstein-Institut)
  • Tokyo Institute of Technology
  • Pennsylvania State University
  • Osaka City University
  • National Science Foundation (NSF)
  • Kyoto University
  • Kinki-Universität
  • Ochanomizu University
  • Hiroshima University
  • Tokyo Denki University
  • Miyagi University of Education
  • California Institute of Technology (Caltech)
Forschungs-netzwerk anzeigen

Details

OriginalspracheEnglisch
Aufsatznummer122002
FachzeitschriftPhysical Review D - Particles, Fields, Gravitation and Cosmology
Jahrgang74
Ausgabenummer12
PublikationsstatusVeröffentlicht - 21 Dez. 2006
Extern publiziertJa

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.

ASJC Scopus Sachgebiete

Zitieren

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, Jahrgang 74, Nr. 12, 122002, 21.12.2006.

Publikation: Beitrag in FachzeitschriftArtikelForschungPeer-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 Dez 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.",
author = "{TAMA Collaboration} and Tomomi Akutsu and Tomotada Akutsu and Masaki Ando and Koji Arai and Akito Araya and Hideki Asada and Youichi Aso and Barton, {Mark A.} and Peter Beyersdorf and Youhei Fujiki and Fujimoto, {Masa Katsu} and Ryuichi Fujita and Mitsuhiro Fukushima and Toshifumi Futamase and Yusaku Hamuro and Tomiyoshi Haruyama and Hideaki Hayakawa and Kazuhiro Hayama and Gerhard Heinzel and Gen'ichi Horikoshi and Hideo Iguchi and Yukiyoshi Iida and Kunihito Ioka and Hideki Ishitsuka and Norihiko Kamikubota and Nobuyuki Kanda and Takaharu Kaneyama and Yoshikazu Karasawa and Kunihiko Kasahara and Taketoshi Kasai and Mayu Katsuki and Keita Kawabe and Mari Kawamura and Seiji Kawamura and Nobuki Kawashima and Fumiko Kawazoe and Yasufumi Kojima and Keiko Kokeyama and Kazuhiro Kondo and Yoshihide Kozai and Hideaki Kudoh and Kazuaki Kuroda and Takashi Kuwabara and Namio Matsuda and Norikatsu Mio and Kazuyuki Miura and Osamu Miyakawa and Shoken Miyama and Shinji Miyoki and Kazuhiro Yamamoto",
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Download

TY - JOUR

T1 - Results of the search for inspiraling compact star binaries from TAMA300's observation in 2000-2004

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

Y1 - 2006/12/21

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

AN - SCOPUS:33845733152

VL - 74

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

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

SN - 1550-7998

IS - 12

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ER -