The Japanese space gravitational wave antenna - DECIGO

S. Kawamura; M. Ando; T. Nakamura; K. Tsubono; T. Tanaka; I. Funaki; N. Seto; K. Numata; S. Sato; K. Ioka; N. Kanda; T. Takashima; K. Agatsuma; T. Akutsu; T. Akutsu; K. S. Aoyanagi; K. Arai; Y. Arase; A. Araya; H. Asada; Y. Aso; T. Chiba; T. Ebisuzaki; M. Enoki; Y. Eriguchi; M. K. Fujimoto; R. Fujita; M. Fukushima; T. Futamase; K. Ganzu; T. Harada; T. Hashimoto; K. Hayama; W. Hikida; Y. Himemoto; H. Hirabayashi; T. Hiramatsu; F. L. Hong; H. Horisawa; M. Hosokawa; K. Ichiki; T. Ikegami; K. T. Inoue; K. Ishidoshiro; H. Ishihara; T. Ishikawa; H. Ishizaki; H. Ito; Y. Itoh; S. Kamagasako; N. Kawashima; F. Kawazoe; H. Kirihara; N. Kishimoto; K. Kiuchi; S. Kobayashi; K. Kohri; H. Koizumi; Y. Kojima; K. Kokeyama; W. Kokuyama; K. Kotake; Y. Kozai; H. Kudoh; H. Kunimori; H. Kuninaka; K. Kuroda; K. I. Maeda; H. Matsuhara; Y. Mino; O. Miyakawa; S. Miyoki; Y. Morimoto; T. Morioka; T. Morisawa; S. Moriwaki; S. Mukohyama; M. Musha; S. Nagano; I. Naito; N. Nakagawa; K. Nakamura; H. Nakano; K. Nakao; S. Nakasuka; Y. Nakayama; E. Nishida; K. Nishiyama; A. Nishizawa; Y. Niwa; M. Ohashi; N. Ohishi; M. Ohkawa; A. Okutomi; K. Onozato; K. Oohara; N. Sago; M. Saijo; M. Sakagami; S. I. Sakai; S. Sakata; M. Sasaki; T. Sato; M. Shibata; H. Shinkai; K. Somiya; H. Sotani; N. Sugiyama; Y. Suwa; H. Tagoshi; K. Takahashi; K. Takahashi; T. Takahashi; H. Takahashi; R. Takahashi; R. Takahashi; A. Takamori; T. Takano; K. Taniguchi; A. Taruya; H. Tashiro; M. Tokuda; M. Tokunari; M. Toyoshima; S. Tsujikawa; Y. Tsunesada; K. I. Ueda; M. Utashima; H. Yamakawa; K. Yamamoto; T. Yamazaki; J. Yokoyama; C. M. Yoo; S. Yoshida; T. Yoshino

doi:10.1088/1742-6596/122/1/012006

The Japanese space gravitational wave antenna - DECIGO

S. Kawamura^*, M. Ando, T. Nakamura, K. Tsubono, T. Tanaka, I. Funaki, N. Seto, K. Numata, S. Sato, K. Ioka, N. Kanda, T. Takashima, K. Agatsuma, T. Akutsu, T. Akutsu, K. S. Aoyanagi, K. Arai, Y. Arase, A. Araya, H. AsadaY. Aso, T. Chiba, T. Ebisuzaki, M. Enoki, Y. Eriguchi, M. K. Fujimoto, R. Fujita, M. Fukushima, T. Futamase, K. Ganzu, T. Harada, T. Hashimoto, K. Hayama, W. Hikida, Y. Himemoto, H. Hirabayashi, T. Hiramatsu, F. L. Hong, H. Horisawa, M. Hosokawa, K. Ichiki, T. Ikegami, K. T. Inoue, K. Ishidoshiro, H. Ishihara, T. Ishikawa, H. Ishizaki, H. Ito, Y. Itoh, S. Kamagasako, N. Kawashima, F. Kawazoe, H. Kirihara, N. Kishimoto, K. Kiuchi, S. Kobayashi, K. Kohri, H. Koizumi, Y. Kojima, K. Kokeyama, W. Kokuyama, K. Kotake, Y. Kozai, H. Kudoh, H. Kunimori, H. Kuninaka, K. Kuroda, K. I. Maeda, H. Matsuhara, Y. Mino, O. Miyakawa, S. Miyoki, Y. Morimoto, T. Morioka, T. Morisawa, S. Moriwaki, S. Mukohyama, M. Musha, S. Nagano, I. Naito, N. Nakagawa, K. Nakamura, H. Nakano, K. Nakao, S. Nakasuka, Y. Nakayama, E. Nishida, K. Nishiyama, A. Nishizawa, Y. Niwa, M. Ohashi, N. Ohishi, M. Ohkawa, A. Okutomi, K. Onozato, K. Oohara, N. Sago, M. Saijo, M. Sakagami, S. I. Sakai, S. Sakata, M. Sasaki, T. Sato, M. Shibata, H. Shinkai, K. Somiya, H. Sotani, N. Sugiyama, Y. Suwa, H. Tagoshi, K. Takahashi, K. Takahashi, T. Takahashi, H. Takahashi, R. Takahashi, R. Takahashi, A. Takamori, T. Takano, K. Taniguchi, A. Taruya, H. Tashiro, M. Tokuda, M. Tokunari, M. Toyoshima, S. Tsujikawa, Y. Tsunesada, K. I. Ueda, M. Utashima, H. Yamakawa, K. Yamamoto, T. Yamazaki, J. Yokoyama, C. M. Yoo, S. Yoshida, T. Yoshino

^*この研究の対応する著者

研究成果: Article › 査読

51 被引用数 (Scopus)

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DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. The goal of DECIGO is to detect gravitational waves from various kinds of sources mainly between 0.1 Hz and 10 Hz and thus to open a new window of observation for gravitational wave astronomy. DECIGO will consist of three drag-free spacecraft, 1000 km apart from each other, whose relative displacements are measured by a Fabry - Perot Michelson interferometer. We plan to launch DECIGO pathfinder first to demonstrate the technologies required to realize DECIGO and, if possible, to detect gravitational waves from our galaxy or nearby galaxies.

本文言語	English
論文番号	012006
ジャーナル	Journal of Physics: Conference Series
巻	122
DOI	https://doi.org/10.1088/1742-6596/122/1/012006
出版ステータス	Published - 2008
外部発表	はい

ASJC Scopus subject areas

物理学および天文学（全般）

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10.1088/1742-6596/122/1/012006

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引用スタイル

Kawamura, S., Ando, M., Nakamura, T., Tsubono, K., Tanaka, T., Funaki, I., Seto, N., Numata, K., Sato, S., Ioka, K., Kanda, N., Takashima, T., Agatsuma, K., Akutsu, T., Akutsu, T., Aoyanagi, K. S., Arai, K., Arase, Y., Araya, A., ... Yoshino, T. (2008). The Japanese space gravitational wave antenna - DECIGO. Journal of Physics: Conference Series, 122, Article 012006. https://doi.org/10.1088/1742-6596/122/1/012006

Kawamura, S, Ando, M, Nakamura, T, Tsubono, K, Tanaka, T, Funaki, I, Seto, N, Numata, K, Sato, S, Ioka, K, Kanda, N, Takashima, T, Agatsuma, K, Akutsu, T, Akutsu, T, Aoyanagi, KS, Arai, K, Arase, Y, Araya, A, Asada, H, Aso, Y, Chiba, T, Ebisuzaki, T, Enoki, M, Eriguchi, Y, Fujimoto, MK, Fujita, R, Fukushima, M, Futamase, T, Ganzu, K, Harada, T, Hashimoto, T, Hayama, K, Hikida, W, Himemoto, Y, Hirabayashi, H, Hiramatsu, T, Hong, FL, Horisawa, H, Hosokawa, M, Ichiki, K, Ikegami, T, Inoue, KT, Ishidoshiro, K, Ishihara, H, Ishikawa, T, Ishizaki, H, Ito, H, Itoh, Y, Kamagasako, S, Kawashima, N, Kawazoe, F, Kirihara, H, Kishimoto, N, Kiuchi, K, Kobayashi, S, Kohri, K, Koizumi, H, Kojima, Y, Kokeyama, K, Kokuyama, W, Kotake, K, Kozai, Y, Kudoh, H, Kunimori, H, Kuninaka, H, Kuroda, K, Maeda, KI, Matsuhara, H, Mino, Y, Miyakawa, O, Miyoki, S, Morimoto, Y, Morioka, T, Morisawa, T, Moriwaki, S, Mukohyama, S, Musha, M, Nagano, S, Naito, I, Nakagawa, N, Nakamura, K, Nakano, H, Nakao, K, Nakasuka, S, Nakayama, Y, Nishida, E, Nishiyama, K, Nishizawa, A, Niwa, Y, Ohashi, M, Ohishi, N, Ohkawa, M, Okutomi, A, Onozato, K, Oohara, K, Sago, N, Saijo, M, Sakagami, M, Sakai, SI, Sakata, S, Sasaki, M, Sato, T, Shibata, M, Shinkai, H, Somiya, K, Sotani, H, Sugiyama, N, Suwa, Y, Tagoshi, H, Takahashi, K, Takahashi, K, Takahashi, T, Takahashi, H, Takahashi, R, Takahashi, R, Takamori, A, Takano, T, Taniguchi, K, Taruya, A, Tashiro, H, Tokuda, M, Tokunari, M, Toyoshima, M, Tsujikawa, S, Tsunesada, Y, Ueda, KI, Utashima, M, Yamakawa, H, Yamamoto, K, Yamazaki, T, Yokoyama, J, Yoo, CM, Yoshida, S & Yoshino, T 2008, 'The Japanese space gravitational wave antenna - DECIGO', Journal of Physics: Conference Series, vol. 122, 012006. https://doi.org/10.1088/1742-6596/122/1/012006

@article{c4976abf675e4224a960047b3f2d761d,

title = "The Japanese space gravitational wave antenna - DECIGO",

abstract = "DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. The goal of DECIGO is to detect gravitational waves from various kinds of sources mainly between 0.1 Hz and 10 Hz and thus to open a new window of observation for gravitational wave astronomy. DECIGO will consist of three drag-free spacecraft, 1000 km apart from each other, whose relative displacements are measured by a Fabry - Perot Michelson interferometer. We plan to launch DECIGO pathfinder first to demonstrate the technologies required to realize DECIGO and, if possible, to detect gravitational waves from our galaxy or nearby galaxies.",

author = "S. Kawamura and M. Ando and T. Nakamura and K. Tsubono and T. Tanaka and I. Funaki and N. Seto and K. Numata and S. Sato and K. Ioka and N. Kanda and T. Takashima and K. Agatsuma and T. Akutsu and T. Akutsu and Aoyanagi, {K. S.} and K. Arai and Y. Arase and A. Araya and H. Asada and Y. Aso and T. Chiba and T. Ebisuzaki and M. Enoki and Y. Eriguchi and Fujimoto, {M. K.} and R. Fujita and M. Fukushima and T. Futamase and K. Ganzu and T. Harada and T. Hashimoto and K. Hayama and W. Hikida and Y. Himemoto and H. Hirabayashi and T. Hiramatsu and Hong, {F. L.} and H. Horisawa and M. Hosokawa and K. Ichiki and T. Ikegami and Inoue, {K. T.} and K. Ishidoshiro and H. Ishihara and T. Ishikawa and H. Ishizaki and H. Ito and Y. Itoh and S. Kamagasako and N. Kawashima and F. Kawazoe and H. Kirihara and N. Kishimoto and K. Kiuchi and S. Kobayashi and K. Kohri and H. Koizumi and Y. Kojima and K. Kokeyama and W. Kokuyama and K. Kotake and Y. Kozai and H. Kudoh and H. Kunimori and H. Kuninaka and K. Kuroda and Maeda, {K. I.} and H. Matsuhara and Y. Mino and O. Miyakawa and S. Miyoki and Y. Morimoto and T. Morioka and T. Morisawa and S. Moriwaki and S. Mukohyama and M. Musha and S. Nagano and I. Naito and N. Nakagawa and K. Nakamura and H. Nakano and K. Nakao and S. Nakasuka and Y. Nakayama and E. Nishida and K. Nishiyama and A. Nishizawa and Y. Niwa and M. Ohashi and N. Ohishi and M. Ohkawa and A. Okutomi and K. Onozato and K. Oohara and N. Sago and M. Saijo and M. Sakagami and Sakai, {S. I.} and S. Sakata and M. Sasaki and T. Sato and M. Shibata and H. Shinkai and K. Somiya and H. Sotani and N. Sugiyama and Y. Suwa and H. Tagoshi and K. Takahashi and K. Takahashi and T. Takahashi and H. Takahashi and R. Takahashi and R. Takahashi and A. Takamori and T. Takano and K. Taniguchi and A. Taruya and H. Tashiro and M. Tokuda and M. Tokunari and M. Toyoshima and S. Tsujikawa and Y. Tsunesada and Ueda, {K. I.} and M. Utashima and H. Yamakawa and K. Yamamoto and T. Yamazaki and J. Yokoyama and Yoo, {C. M.} and S. Yoshida and T. Yoshino",

year = "2008",

doi = "10.1088/1742-6596/122/1/012006",

language = "English",

volume = "122",

journal = "Journal of Physics: Conference Series",

issn = "1742-6588",

publisher = "IOP Publishing Ltd.",

}

TY - JOUR

T1 - The Japanese space gravitational wave antenna - DECIGO

AU - Kawamura, S.

AU - Ando, M.

AU - Nakamura, T.

AU - Tsubono, K.

AU - Tanaka, T.

AU - Funaki, I.

AU - Seto, N.

AU - Numata, K.

AU - Sato, S.

AU - Ioka, K.

AU - Kanda, N.

AU - Takashima, T.

AU - Agatsuma, K.

AU - Akutsu, T.

AU - Aoyanagi, K. S.

AU - Arai, K.

AU - Arase, Y.

AU - Araya, A.

AU - Asada, H.

AU - Aso, Y.

AU - Chiba, T.

AU - Ebisuzaki, T.

AU - Enoki, M.

AU - Eriguchi, Y.

AU - Fujimoto, M. K.

AU - Fujita, R.

AU - Fukushima, M.

AU - Futamase, T.

AU - Ganzu, K.

AU - Harada, T.

AU - Hashimoto, T.

AU - Hayama, K.

AU - Hikida, W.

AU - Himemoto, Y.

AU - Hirabayashi, H.

AU - Hiramatsu, T.

AU - Hong, F. L.

AU - Horisawa, H.

AU - Hosokawa, M.

AU - Ichiki, K.

AU - Ikegami, T.

AU - Inoue, K. T.

AU - Ishidoshiro, K.

AU - Ishihara, H.

AU - Ishikawa, T.

AU - Ishizaki, H.

AU - Ito, H.

AU - Itoh, Y.

AU - Kamagasako, S.

AU - Kawashima, N.

AU - Kawazoe, F.

AU - Kirihara, H.

AU - Kishimoto, N.

AU - Kiuchi, K.

AU - Kobayashi, S.

AU - Kohri, K.

AU - Koizumi, H.

AU - Kojima, Y.

AU - Kokeyama, K.

AU - Kokuyama, W.

AU - Kotake, K.

AU - Kozai, Y.

AU - Kudoh, H.

AU - Kunimori, H.

AU - Kuninaka, H.

AU - Kuroda, K.

AU - Maeda, K. I.

AU - Matsuhara, H.

AU - Mino, Y.

AU - Miyakawa, O.

AU - Miyoki, S.

AU - Morimoto, Y.

AU - Morioka, T.

AU - Morisawa, T.

AU - Moriwaki, S.

AU - Mukohyama, S.

AU - Musha, M.

AU - Nagano, S.

AU - Naito, I.

AU - Nakagawa, N.

AU - Nakamura, K.

AU - Nakano, H.

AU - Nakao, K.

AU - Nakasuka, S.

AU - Nakayama, Y.

AU - Nishida, E.

AU - Nishiyama, K.

AU - Nishizawa, A.

AU - Niwa, Y.

AU - Ohashi, M.

AU - Ohishi, N.

AU - Ohkawa, M.

AU - Okutomi, A.

AU - Onozato, K.

AU - Oohara, K.

AU - Sago, N.

AU - Saijo, M.

AU - Sakagami, M.

AU - Sakai, S. I.

AU - Sakata, S.

AU - Sasaki, M.

AU - Sato, T.

AU - Shibata, M.

AU - Shinkai, H.

AU - Somiya, K.

AU - Sotani, H.

AU - Sugiyama, N.

AU - Suwa, Y.

AU - Tagoshi, H.

AU - Takahashi, K.

AU - Takahashi, T.

AU - Takahashi, H.

AU - Takahashi, R.

AU - Takamori, A.

AU - Takano, T.

AU - Taniguchi, K.

AU - Taruya, A.

AU - Tashiro, H.

AU - Tokuda, M.

AU - Tokunari, M.

AU - Toyoshima, M.

AU - Tsujikawa, S.

AU - Tsunesada, Y.

AU - Ueda, K. I.

AU - Utashima, M.

AU - Yamakawa, H.

AU - Yamamoto, K.

AU - Yamazaki, T.

AU - Yokoyama, J.

AU - Yoo, C. M.

AU - Yoshida, S.

AU - Yoshino, T.

PY - 2008

Y1 - 2008

N2 - DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. The goal of DECIGO is to detect gravitational waves from various kinds of sources mainly between 0.1 Hz and 10 Hz and thus to open a new window of observation for gravitational wave astronomy. DECIGO will consist of three drag-free spacecraft, 1000 km apart from each other, whose relative displacements are measured by a Fabry - Perot Michelson interferometer. We plan to launch DECIGO pathfinder first to demonstrate the technologies required to realize DECIGO and, if possible, to detect gravitational waves from our galaxy or nearby galaxies.

AB - DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. The goal of DECIGO is to detect gravitational waves from various kinds of sources mainly between 0.1 Hz and 10 Hz and thus to open a new window of observation for gravitational wave astronomy. DECIGO will consist of three drag-free spacecraft, 1000 km apart from each other, whose relative displacements are measured by a Fabry - Perot Michelson interferometer. We plan to launch DECIGO pathfinder first to demonstrate the technologies required to realize DECIGO and, if possible, to detect gravitational waves from our galaxy or nearby galaxies.

UR - http://www.scopus.com/inward/record.url?scp=65649117704&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=65649117704&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/122/1/012006

DO - 10.1088/1742-6596/122/1/012006

M3 - Article

AN - SCOPUS:65649117704

SN - 1742-6588

VL - 122

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

M1 - 012006

ER -

The Japanese space gravitational wave antenna - DECIGO

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