Seiji Kawamura et al 2006 Class. Quantum Grav. 23 S125 doi:10.1088/0264-9381/23/8/S17
Seiji Kawamura1, Takashi Nakamura2, Masaki Ando3, Naoki Seto4, Kimio Tsubono3, Kenji Numata5, Ryuichi Takahashi1, Shigeo Nagano6, Takehiko Ishikawa7, Mitsuru Musha8, Ken-ichi Ueda8, Takashi Sato9, Mizuhiko Hosokawa6, Kazuhiro Agatsuma3, Tomotada Akutsu3, Koh-suke Aoyanagi10, Koji Arai1, Akito Araya11, Hideki Asada12, Yoichi Aso3, Takeshi Chiba13, Toshikazu Ebisuzaki14, Yoshiharu Eriguchi15, Masa-Katsu Fujimoto1, Mitsuhiro Fukushima1, Toshifumi Futamase16, Katsuhiko Ganzu2, Tomohiro Harada2, Tatsuaki Hashimoto17, Kazuhiro Hayama1, Wataru Hikida18, Yoshiaki Himemoto3, Hisashi Hirabayashi17, Takashi Hiramatsu3, Kiyotomo Ichiki1, Takeshi Ikegami19, Kaiki T Inoue20, Kunihito Ioka2, Koji Ishidoshiro3, Yousuke Itoh21, Shogo Kamagasako3, Nobuyuki Kanda22, Nobuki Kawashima20, Hiroyuki Kirihara3, Kenta Kiuchi10, Shiho Kobayashi23, Kazunori Kohri24, Yasufumi Kojima25, Keiko Kokeyama26, Yoshihide Kozai27, Hideaki Kudoh3, Hiroo Kunimori28, Kazuaki Kuroda29, Kei-ichi Maeda10, Hideo Matsuhara17, Yasushi Mino4, Osamu Miyakawa4, Shinji Miyoki29, Hiromi Mizusawa30, Toshiyuki Morisawa2, Shinji Mukohyama3, Isao Naito31, Noriyasu Nakagawa3, Kouji Nakamura31, Hiroyuki Nakano22, Kenichi Nakao22, Atsushi Nishizawa32, Yoshito Niwa32, Choetsu Nozawa30, Masatake Ohashi29, Naoko Ohishi1, Masashi Ohkawa9, Akira Okutomi3, Kenichi Oohara30, Norichika Sago33, Motoyuki Saijo34, Masaaki Sakagami32, Shihori Sakata26, Misao Sasaki18, Shuichi Sato1, Masaru Shibata15, Hisaaki Shinkai35, Kentaro Somiya36, Hajime Sotani10, Naoshi Sugiyama1, Hideyuki Tagoshi33, Tadayuki Takahashi17, Hirotaka Takahashi36, Ryutaro Takahashi1, Tadashi Takano17, Takahiro Tanaka2, Keisuke Taniguchi37, Atsushi Taruya3, Hiroyuki Tashiro2, Masao Tokunari3, Shinji Tsujikawa3, Yoshiki Tsunesada38, Kazuhiro Yamamoto29, Toshitaka Yamazaki1, Jun'ichi Yokoyama3, Chul-Moon Yoo22, Shijun Yoshida10 and Taizoh Yoshino39
Show affiliationsDECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. It aims at detecting various kinds of gravitational waves between 1 mHz and 100 Hz frequently enough to open a new window of observation for gravitational wave astronomy. The pre-conceptual design of DECIGO consists of three drag-free satellites, 1000 km apart from each other, whose relative displacements are measured by a Fabry–Perot Michelson interferometer. We plan to launch DECIGO in 2024 after a long and intense development phase, including two pathfinder missions for verification of required technologies.
Issue 8 (21 April 2006)
Received 3 October 2005, in final form 9 December 2005
Published 28 March 2006
Seiji Kawamura et al 2006 Class. Quantum Grav. 23 S125
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