First search for gravitational waves from inspiraling compact binaries using'TAMA300 data

Hideyuki Tagoshi; Nobuyuki Kanda; Takahiro Tanaka; Daisuke Tatsumi; Souichi Telada; Masaki Ando; Koji Arai; Akito Araya; Hideki Asada; Mark A. Barton; Masa Katsu Fujimoto; Mitsuhiro Fukushima; Toshifumi Futamase; Gerhard Heinzel; Ge N.Ichi Horikoshi; Hideki Ishizuka; Norihiko Kamikubota; Keita Kawabe; Seiji Kawamura; Nobuki Kawashima; Yasufumi Kojima; Yoshihide Kozai; Kazuaki Kuroda; Namio Matsuda; Sumihiro Matsumura; Satoshi Miki; Norikatsu Mio; Osamu Miyakawa; Shoken Miyama; Shinji Miyoki; Eiichi Mizuno; Shigenori Moriwaki; Mitsuru Musha; Shigeo Nagano; Ke N.Ichi Nakagawa; Takashi Nakamura; Ken Ichi Nakao; Kenji Numata; Yujiro Ogawa; Masatake Ohashi; Naoko Ohishi; Akira Okutomi; Ken Ichi Oohara; Shigemi Otsuka; Yoshio Saito; Misao Sasaki; Shuichi Sato; Atsushi Sekiya; Masaru Shibata; Kazumichi Shirakata; Kentaro Somiya; Toshikazu Suzuki; Ryutaro Takahashi; Akiteru Takamori; Shinsuke Taniguchi; Kuniharu Tochikubo; Takayuki Tomaru; Kimio Tsubono; Nobuhiro Tsuda; Takashi Uchiyama; Akitoshi Ueda; Ken Ichi Ueda; Kozo Ueda; Koichi Waseda; Yuko Watanabe; Hiromi Yakura; Kazuhiro Yamamoto; Toshitaka Yamazaki

doi:10.1103/PhysRevD.63.062001

First search for gravitational waves from inspiraling compact binaries using'TAMA300 data

Hideyuki Tagoshi, Nobuyuki Kanda, Takahiro Tanaka, Daisuke Tatsumi, Souichi Telada, Masaki Ando, Koji Arai, Akito Araya, Hideki Asada, Mark A. Barton, Masa Katsu Fujimoto, Mitsuhiro Fukushima, Toshifumi Futamase, Gerhard Heinzel, Ge N.Ichi Horikoshi, Hideki Ishizuka, Norihiko Kamikubota, Keita Kawabe, Seiji Kawamura, Nobuki KawashimaYasufumi Kojima, Yoshihide Kozai, Kazuaki Kuroda, Namio Matsuda, Sumihiro Matsumura, Satoshi Miki, Norikatsu Mio, Osamu Miyakawa, Shoken Miyama, Shinji Miyoki, Eiichi Mizuno, Shigenori Moriwaki, Mitsuru Musha, Shigeo Nagano, Ke N.Ichi Nakagawa, Takashi Nakamura, Ken Ichi Nakao, Kenji Numata, Yujiro Ogawa, Masatake Ohashi, Naoko Ohishi, Akira Okutomi, Ken Ichi Oohara, Shigemi Otsuka, Yoshio Saito, Misao Sasaki, Shuichi Sato, Atsushi Sekiya, Masaru Shibata, Kazumichi Shirakata, Kentaro Somiya, Toshikazu Suzuki, Ryutaro Takahashi, Akiteru Takamori, Shinsuke Taniguchi, Kuniharu Tochikubo, Takayuki Tomaru, Kimio Tsubono, Nobuhiro Tsuda, Takashi Uchiyama, Akitoshi Ueda, Ken Ichi Ueda, Kozo Ueda, Koichi Waseda, Yuko Watanabe, Hiromi Yakura, Kazuhiro Yamamoto, Toshitaka Yamazaki

Research output: Contribution to journal › Article › peer-review

88 Citations (Scopus)

Abstract

We analyzed 6 hours of data from the TAMA300 detector by matched filtering, searching for gravitational waves from inspiraling compact binaries. We incorporated a two-step hierarchical search strategy in matched filtering. We obtained an upper limit of 0.59/hpur (C.L.=90%) on the event rate of inspirais of compact binaries with a mass between 0.3A/O and 10A/Q and with a signal-to-noise ratio greater than 7.2. The distance of 1.4A/G(0.5A/o) binaries which produce the signal-to-noise ratio 7.2 was estimated to be 6.2 kpc (2.9 kpc) when the position of the MVIIXV in (he 4y und the inclination angle of the binaries were optimal.

Original language	English
Article number	062001
Journal	Physical Review D
Volume	63
Issue number	6
DOIs	https://doi.org/10.1103/PhysRevD.63.062001
Publication status	Published - 2001
Externally published	Yes

ASJC Scopus subject areas

Physics and Astronomy (miscellaneous)

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10.1103/PhysRevD.63.062001

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Tagoshi, H., Kanda, N., Tanaka, T., Tatsumi, D., Telada, S., Ando, M., Arai, K., Araya, A., Asada, H., Barton, M. A., Fujimoto, M. K., Fukushima, M., Futamase, T., Heinzel, G., Horikoshi, G. N. I., Ishizuka, H., Kamikubota, N., Kawabe, K., Kawamura, S., ... Yamazaki, T. (2001). First search for gravitational waves from inspiraling compact binaries using'TAMA300 data. Physical Review D, 63(6), [062001]. https://doi.org/10.1103/PhysRevD.63.062001

First search for gravitational waves from inspiraling compact binaries using'TAMA300 data. / Tagoshi, Hideyuki; Kanda, Nobuyuki; Tanaka, Takahiro; Tatsumi, Daisuke; Telada, Souichi; Ando, Masaki; Arai, Koji; Araya, Akito; Asada, Hideki; Barton, Mark A.; Fujimoto, Masa Katsu; Fukushima, Mitsuhiro; Futamase, Toshifumi; Heinzel, Gerhard; Horikoshi, Ge N.Ichi; Ishizuka, Hideki; Kamikubota, Norihiko; Kawabe, Keita; Kawamura, Seiji; Kawashima, Nobuki; Kojima, Yasufumi; Kozai, Yoshihide; Kuroda, Kazuaki; Matsuda, Namio; Matsumura, Sumihiro; Miki, Satoshi; Mio, Norikatsu; Miyakawa, Osamu; Miyama, Shoken; Miyoki, Shinji; Mizuno, Eiichi; Moriwaki, Shigenori; Musha, Mitsuru; Nagano, Shigeo; Nakagawa, Ke N.Ichi; Nakamura, Takashi; Nakao, Ken Ichi; Numata, Kenji; Ogawa, Yujiro; Ohashi, Masatake; Ohishi, Naoko; Okutomi, Akira; Oohara, Ken Ichi; Otsuka, Shigemi; Saito, Yoshio; Sasaki, Misao; Sato, Shuichi; Sekiya, Atsushi; Shibata, Masaru; Shirakata, Kazumichi; Somiya, Kentaro; Suzuki, Toshikazu; Takahashi, Ryutaro; Takamori, Akiteru; Taniguchi, Shinsuke; Tochikubo, Kuniharu; Tomaru, Takayuki; Tsubono, Kimio; Tsuda, Nobuhiro; Uchiyama, Takashi; Ueda, Akitoshi; Ueda, Ken Ichi; Ueda, Kozo; Waseda, Koichi; Watanabe, Yuko; Yakura, Hiromi; Yamamoto, Kazuhiro; Yamazaki, Toshitaka.

In: Physical Review D, Vol. 63, No. 6, 062001, 2001.

Research output: Contribution to journal › Article › peer-review

Tagoshi, H, Kanda, N, Tanaka, T, Tatsumi, D, Telada, S, Ando, M, Arai, K, Araya, A, Asada, H, Barton, MA, Fujimoto, MK, Fukushima, M, Futamase, T, Heinzel, G, Horikoshi, GNI, Ishizuka, H, Kamikubota, N, Kawabe, K, Kawamura, S, Kawashima, N, Kojima, Y, Kozai, Y, Kuroda, K, Matsuda, N, Matsumura, S, Miki, S, Mio, N, Miyakawa, O, Miyama, S, Miyoki, S, Mizuno, E, Moriwaki, S, Musha, M, Nagano, S, Nakagawa, KNI, Nakamura, T, Nakao, KI, Numata, K, Ogawa, Y, Ohashi, M, Ohishi, N, Okutomi, A, Oohara, KI, Otsuka, S, Saito, Y, Sasaki, M, Sato, S, Sekiya, A, Shibata, M, Shirakata, K, Somiya, K, Suzuki, T, Takahashi, R, Takamori, A, Taniguchi, S, Tochikubo, K, Tomaru, T, Tsubono, K, Tsuda, N, Uchiyama, T, Ueda, A, Ueda, KI, Ueda, K, Waseda, K, Watanabe, Y, Yakura, H, Yamamoto, K & Yamazaki, T 2001, 'First search for gravitational waves from inspiraling compact binaries using'TAMA300 data', Physical Review D, vol. 63, no. 6, 062001. https://doi.org/10.1103/PhysRevD.63.062001

Tagoshi, Hideyuki ; Kanda, Nobuyuki ; Tanaka, Takahiro ; Tatsumi, Daisuke ; Telada, Souichi ; Ando, Masaki ; Arai, Koji ; Araya, Akito ; Asada, Hideki ; Barton, Mark A. ; Fujimoto, Masa Katsu ; Fukushima, Mitsuhiro ; Futamase, Toshifumi ; Heinzel, Gerhard ; Horikoshi, Ge N.Ichi ; Ishizuka, Hideki ; Kamikubota, Norihiko ; Kawabe, Keita ; Kawamura, Seiji ; Kawashima, Nobuki ; Kojima, Yasufumi ; Kozai, Yoshihide ; Kuroda, Kazuaki ; Matsuda, Namio ; Matsumura, Sumihiro ; Miki, Satoshi ; Mio, Norikatsu ; Miyakawa, Osamu ; Miyama, Shoken ; Miyoki, Shinji ; Mizuno, Eiichi ; Moriwaki, Shigenori ; Musha, Mitsuru ; Nagano, Shigeo ; Nakagawa, Ke N.Ichi ; Nakamura, Takashi ; Nakao, Ken Ichi ; Numata, Kenji ; Ogawa, Yujiro ; Ohashi, Masatake ; Ohishi, Naoko ; Okutomi, Akira ; Oohara, Ken Ichi ; Otsuka, Shigemi ; Saito, Yoshio ; Sasaki, Misao ; Sato, Shuichi ; Sekiya, Atsushi ; Shibata, Masaru ; Shirakata, Kazumichi ; Somiya, Kentaro ; Suzuki, Toshikazu ; Takahashi, Ryutaro ; Takamori, Akiteru ; Taniguchi, Shinsuke ; Tochikubo, Kuniharu ; Tomaru, Takayuki ; Tsubono, Kimio ; Tsuda, Nobuhiro ; Uchiyama, Takashi ; Ueda, Akitoshi ; Ueda, Ken Ichi ; Ueda, Kozo ; Waseda, Koichi ; Watanabe, Yuko ; Yakura, Hiromi ; Yamamoto, Kazuhiro ; Yamazaki, Toshitaka. / First search for gravitational waves from inspiraling compact binaries using'TAMA300 data. In: Physical Review D. 2001 ; Vol. 63, No. 6.

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title = "First search for gravitational waves from inspiraling compact binaries using'TAMA300 data",

abstract = "We analyzed 6 hours of data from the TAMA300 detector by matched filtering, searching for gravitational waves from inspiraling compact binaries. We incorporated a two-step hierarchical search strategy in matched filtering. We obtained an upper limit of 0.59/hpur (C.L.=90%) on the event rate of inspirais of compact binaries with a mass between 0.3A/O and 10A/Q and with a signal-to-noise ratio greater than 7.2. The distance of 1.4A/G(0.5A/o) binaries which produce the signal-to-noise ratio 7.2 was estimated to be 6.2 kpc (2.9 kpc) when the position of the MVIIXV in (he 4y und the inclination angle of the binaries were optimal.",

author = "Hideyuki Tagoshi and Nobuyuki Kanda and Takahiro Tanaka and Daisuke Tatsumi and Souichi Telada and Masaki Ando and Koji Arai and Akito Araya and Hideki Asada and Barton, {Mark A.} and Fujimoto, {Masa Katsu} and Mitsuhiro Fukushima and Toshifumi Futamase and Gerhard Heinzel and Horikoshi, {Ge N.Ichi} and Hideki Ishizuka and Norihiko Kamikubota and Keita Kawabe and Seiji Kawamura and Nobuki Kawashima and Yasufumi Kojima and Yoshihide Kozai and Kazuaki Kuroda and Namio Matsuda and Sumihiro Matsumura and Satoshi Miki and Norikatsu Mio and Osamu Miyakawa and Shoken Miyama and Shinji Miyoki and Eiichi Mizuno and Shigenori Moriwaki and Mitsuru Musha and Shigeo Nagano and Nakagawa, {Ke N.Ichi} and Takashi Nakamura and Nakao, {Ken Ichi} and Kenji Numata and Yujiro Ogawa and Masatake Ohashi and Naoko Ohishi and Akira Okutomi and Oohara, {Ken Ichi} and Shigemi Otsuka and Yoshio Saito and Misao Sasaki and Shuichi Sato and Atsushi Sekiya and Masaru Shibata and Kazumichi Shirakata and Kentaro Somiya and Toshikazu Suzuki and Ryutaro Takahashi and Akiteru Takamori and Shinsuke Taniguchi and Kuniharu Tochikubo and Takayuki Tomaru and Kimio Tsubono and Nobuhiro Tsuda and Takashi Uchiyama and Akitoshi Ueda and Ueda, {Ken Ichi} and Kozo Ueda and Koichi Waseda and Yuko Watanabe and Hiromi Yakura and Kazuhiro Yamamoto and Toshitaka Yamazaki",

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AU - Ando, Masaki

AU - Arai, Koji

AU - Araya, Akito

AU - Asada, Hideki

AU - Barton, Mark A.

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AB - We analyzed 6 hours of data from the TAMA300 detector by matched filtering, searching for gravitational waves from inspiraling compact binaries. We incorporated a two-step hierarchical search strategy in matched filtering. We obtained an upper limit of 0.59/hpur (C.L.=90%) on the event rate of inspirais of compact binaries with a mass between 0.3A/O and 10A/Q and with a signal-to-noise ratio greater than 7.2. The distance of 1.4A/G(0.5A/o) binaries which produce the signal-to-noise ratio 7.2 was estimated to be 6.2 kpc (2.9 kpc) when the position of the MVIIXV in (he 4y und the inclination angle of the binaries were optimal.

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First search for gravitational waves from inspiraling compact binaries using'TAMA300 data

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