Details
Original language | English |
---|---|
Article number | 122002 |
Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |
Volume | 74 |
Issue number | 12 |
Publication status | Published - 21 Dec 2006 |
Externally published | Yes |
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 subject areas
- Physics and Astronomy(all)
- Nuclear and High Energy Physics
- Physics and Astronomy(all)
- Physics and Astronomy (miscellaneous)
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In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 74, No. 12, 122002, 21.12.2006.
Research output: Contribution to journal › Article › Research › peer review
}
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.
UR - http://www.scopus.com/inward/record.url?scp=33845733152&partnerID=8YFLogxK
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
M1 - 122002
ER -