| Autor: |
M. A. Barton, Toshifumi Futamase, Tatsuru Yoshida, Fumihiko Usui, Shinsuke Taniguchi, Ryuichi Fujita, Y. Tsunesada, Toshikazu Suzuki, Hisa-aki Shinkai, Kuniharu Tochikubo, Norikatsu Mio, Kazuhiro Yamamoto, C. T. Taylor, Keiko Kokeyama, Mayu Katsuki, Shinji Miyoki, Shihori Sakata, T. Akutsu, Hiromi Mizusawa, Ken-ichi Nakao, Seiji Kawamura, Kouichi Sato, Taketoshi Kasai, Kazuaki Kuroda, Akitoshi Ueda, Y. Aso, Takaharu Kaneyama, Shigeo Nagano, Naoki Seto, Yuko Watanabe, Misao Sasaki, Tomotada Akutsu, Namio Matsuda, Nobuaki Sato, Yoshihide Kozai, Hideyuki Tagoshi, Akiteru Takamori, Osamu Miyakawa, Kunihiko Kasahara, Takashi Kuwabara, Yoshikazu Karasawa, Nobuyuki Kanda, Youhei Sato, P. T. Beyersdorf, Takashi Nakamura, Yukiyoshi Iida, Shigenori Moriwaki, Yuriko Yanagi, Kenji Soida, Shigemi Otsuka, Zong Hong Zhu, Takayuki Tomaru, Masa Katsu Fujimoto, Takakazu Shintomi, Hideaki Hayakawa, Ken-ichi Ueda, Aya Sekido, Norihiko Kamikubota, Masatake Ohashi, Hiroyuki Nakano, Yusaku Hamuro, Hidetsugu Seki, Fumiko Kawazoe, Yoshitaka Nagayama, Tatsuo Yoda, Toshitaka Yamazaki, Naoko Ohishi, Toru Tanji, Norichika Sago, Hideo Iguchi, Ryutaro Takahashi, Takashi Uchiyama, Kunihito Ioka, Hiromi Yakura, Tomiyoshi Haruyama, Kohei Takeno, Mari Kawamura, Hirotaka Takahashi, Keisuke Taniguchi, Koji Arai, Akira Okutomi, Hideaki Kudoh, Mitsuhiro Fukushima, Hideki Ishitsuka, Hideki Asada, Daisuke Tatsumi, Masaru Shibata, Takahiro Tanaka, Gen'ichi Horikoshi, Jun'ichi Yokoyama, Yasufumi Kojima, Yujiro Ogawa, K. Kawabe, Shuzo Takemoto, Kimio Tsubono, Yoshio Saito, Gerhard Heinzel, Koichi Waseda, Souichi Telada, Kazuhiro Kondo, Masao Tokunari, Ken'ichi Nakagawa, Kazuhiro Hayama, Youhei Fujiki, Nobuki Kawashima, Kazuyuki Miura, Nobuhiro Tsuda, Shuichi Sato, Kentaro Somiya, Shoken M. Miyama, Kenji Numata, Masaki Ando, Akira Yamamoto, Yuhiko Nishi, Mitsuru Musha, Akito Araya, K. Oohara |
| Jazyk: |
angličtina |
| Rok vydání: |
2006 |
| Předmět: |
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| Zdroj: |
Physical Review D. 74:122002-122002-8 |
| Popis: |
We 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.
Comment: 8 pages, 4 Postscript figures, uses revtex4.sty The author list was corrected |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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