DECIGO pathfinder

M. Ando; S. Kawamura; 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. Koima; 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; M. 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:10.1088/1742-6596/120/3/032005

DECIGO pathfinder

M. Ando^*, S. Kawamura, 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. Koima, 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, M. 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

^*Corresponding author for this work

Research output: Contribution to journal › Conference article › peer-review

8 Citations (Scopus)

Abstract

DECIGO pathfinder (DPF) is a milestone satellite mission for DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) which is a future space gravitational wave antenna. DECIGO is expected to provide us fruitful insights into the universe, in particular about dark energy, a formation mechanism of supermassive black holes, and the inflation of the universe. Since DECIGO will be an extremely large mission which will formed by three drag-free spacecraft with 1000m separation, it is significant to gain the technical feasibility of DECIGO before its planned launch in 2024. Thus, we are planning to launch two milestone missions: DPF and pre-DECIGO. The conceptual design and current status of the first milestone mission, DPF, are reviewed in this article.

Original language	English
Article number	032005
Journal	Journal of Physics: Conference Series
Volume	120
Issue number	Part 3
DOIs	https://doi.org/10.1088/1742-6596/120/3/032005
Publication status	Published - 2008 Jan 1
Externally published	Yes
Event	10th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2007 - Sendai , Japan Duration: 2007 Sept 11 → 2007 Sept 15

ASJC Scopus subject areas

Physics and Astronomy(all)

Access to Document

10.1088/1742-6596/120/3/032005

Cite this

Ando, M., Kawamura, S., 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). DECIGO pathfinder. Journal of Physics: Conference Series, 120(Part 3), [032005]. https://doi.org/10.1088/1742-6596/120/3/032005

Ando, M, Kawamura, S, 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, Koima, 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, MY, 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, 'DECIGO pathfinder', Journal of Physics: Conference Series, vol. 120, no. Part 3, 032005. https://doi.org/10.1088/1742-6596/120/3/032005

@article{ae597d9d82c44643bd0b43e2926d0015,

title = "DECIGO pathfinder",

abstract = "DECIGO pathfinder (DPF) is a milestone satellite mission for DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) which is a future space gravitational wave antenna. DECIGO is expected to provide us fruitful insights into the universe, in particular about dark energy, a formation mechanism of supermassive black holes, and the inflation of the universe. Since DECIGO will be an extremely large mission which will formed by three drag-free spacecraft with 1000m separation, it is significant to gain the technical feasibility of DECIGO before its planned launch in 2024. Thus, we are planning to launch two milestone missions: DPF and pre-DECIGO. The conceptual design and current status of the first milestone mission, DPF, are reviewed in this article.",

author = "M. Ando and S. Kawamura 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. Koima 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 Morimoto, {M. Y.} 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",

note = "Funding Information: This research was partially supported by the Ministry of Education, Science, Sports and Culture, Grant-in-Aid for Scientific Research, and by the Japan Aerospace Exploration Agency. Publisher Copyright: {\textcopyright} 2008 IOP Publishing Ltd.; 10th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2007 ; Conference date: 11-09-2007 Through 15-09-2007",

year = "2008",

month = jan,

day = "1",

doi = "10.1088/1742-6596/120/3/032005",

language = "English",

volume = "120",

journal = "Journal of Physics: Conference Series",

issn = "1742-6588",

publisher = "IOP Publishing Ltd.",

number = "Part 3",

}

TY - JOUR

T1 - DECIGO pathfinder

AU - Ando, M.

AU - Kawamura, S.

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 - Koima, 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, M. 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.

N1 - Funding Information: This research was partially supported by the Ministry of Education, Science, Sports and Culture, Grant-in-Aid for Scientific Research, and by the Japan Aerospace Exploration Agency. Publisher Copyright: © 2008 IOP Publishing Ltd.

PY - 2008/1/1

Y1 - 2008/1/1

N2 - DECIGO pathfinder (DPF) is a milestone satellite mission for DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) which is a future space gravitational wave antenna. DECIGO is expected to provide us fruitful insights into the universe, in particular about dark energy, a formation mechanism of supermassive black holes, and the inflation of the universe. Since DECIGO will be an extremely large mission which will formed by three drag-free spacecraft with 1000m separation, it is significant to gain the technical feasibility of DECIGO before its planned launch in 2024. Thus, we are planning to launch two milestone missions: DPF and pre-DECIGO. The conceptual design and current status of the first milestone mission, DPF, are reviewed in this article.

AB - DECIGO pathfinder (DPF) is a milestone satellite mission for DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) which is a future space gravitational wave antenna. DECIGO is expected to provide us fruitful insights into the universe, in particular about dark energy, a formation mechanism of supermassive black holes, and the inflation of the universe. Since DECIGO will be an extremely large mission which will formed by three drag-free spacecraft with 1000m separation, it is significant to gain the technical feasibility of DECIGO before its planned launch in 2024. Thus, we are planning to launch two milestone missions: DPF and pre-DECIGO. The conceptual design and current status of the first milestone mission, DPF, are reviewed in this article.

UR - http://www.scopus.com/inward/record.url?scp=85069485248&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85069485248&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/120/3/032005

DO - 10.1088/1742-6596/120/3/032005

M3 - Conference article

AN - SCOPUS:85069485248

SN - 1742-6588

VL - 120

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

IS - Part 3

M1 - 032005

T2 - 10th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2007

Y2 - 11 September 2007 through 15 September 2007

ER -

DECIGO pathfinder

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