抄録
The Hitomi (ASTRO-H) mission is the sixth Japanese X-ray astronomy satellite developed by a large international collaboration, including Japan, USA, Canada, and Europe. The mission aimed to provide the highest energy resolution ever achieved at E > 2 keV, using a microcalorimeter instrument, and to cover a wide energy range spanning four decades in energy from soft X-rays to gamma-rays. After a successful launch on 2016 February 17, the spacecraft lost its function on 2016 March 26, but the commissioning phase for about a month provided valuable information on the on-board instruments and the spacecraft system, including astrophysical results obtained from first light observations. The paper describes the Hitomi (ASTRO-H) mission, its capabilities, the initial operation, and the instruments/spacecraft performances confirmed during the commissioning operations for about a month.
| 本文言語 | English |
|---|---|
| ホスト出版物のタイトル | Space Telescopes and Instrumentation 2016 |
| ホスト出版物のサブタイトル | Ultraviolet to Gamma Ray |
| 編集者 | Marshall Bautz, Tadayuki Takahashi, Jan-Willem A. den Herder |
| 出版社 | SPIE |
| ISBN（電子版） | 9781510601895 |
| DOI | |
| 出版ステータス | Published - 2016 |
| イベント | Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray - Edinburgh, United Kingdom 継続期間: 2016 6月 26 → 2016 7月 1 |
出版物シリーズ
| 名前 | Proceedings of SPIE - The International Society for Optical Engineering |
|---|---|
| 巻 | 9905 |
| ISSN（印刷版） | 0277-786X |
| ISSN（電子版） | 1996-756X |
Other
| Other | Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray |
|---|---|
| 国/地域 | United Kingdom |
| City | Edinburgh |
| Period | 16/6/26 → 16/7/1 |
ASJC Scopus subject areas
- 電子材料、光学材料、および磁性材料
- 凝縮系物理学
- コンピュータ サイエンスの応用
- 応用数学
- 電子工学および電気工学
フィンガープリント
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Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray. ed. / Marshall Bautz; Tadayuki Takahashi; Jan-Willem A. den Herder. SPIE, 2016. 99050U (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9905).
研究成果: Conference contribution
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TY - GEN
T1 - The ASTRO-H (Hitomi) X-ray astronomy satellite
AU - Takahashi, Tadayuki
AU - Kokubun, Motohide
AU - Mitsuda, Kazuhisa
AU - Kelley, Richard
AU - Ohashi, Takaya
AU - Aharonian, Felix
AU - Akamatsu, Hiroki
AU - Akimoto, Fumie
AU - Allen, Steve
AU - Anabuki, Naohisa
AU - Angelini, Lorella
AU - Arnaud, Keith
AU - Asai, Makoto
AU - Audard, Marc
AU - Awaki, Hisamitsu
AU - Axelsson, Magnus
AU - Azzarello, Philipp
AU - Baluta, Chris
AU - Bamba, Aya
AU - Bando, Nobutaka
AU - Bautz, Marshall
AU - Bialas, Thomas
AU - Blandford, Roger
AU - Boyce, Kevin
AU - Brenneman, Laura
AU - Brown, Greg
AU - Bulbul, Esra
AU - Cackett, Edward
AU - Canavan, Edgar
AU - Chernyakova, Maria
AU - Chiao, Meng
AU - Coppi, Paolo
AU - Costantini, Elisa
AU - De Plaa, Jelle
AU - Den Herder, Jan Willem
AU - DiPirro, Michael
AU - Done, Chris
AU - Dotani, Tadayasu
AU - Doty, John
AU - Ebisawa, Ken
AU - Eckart, Megan
AU - Enoto, Teruaki
AU - Ezoe, Yuichiro
AU - Fabian, Andrew
AU - Ferrigno, Carlo
AU - Foster, Adam
AU - Fujimoto, Ryuichi
AU - Fukazawa, Yasushi
AU - Furuzawa, Akihiro
AU - Galeazzi, Massimiliano
AU - Gallo, Luigi
AU - Gandhi, Poshak
AU - Gilmore, Kirk
AU - Giustini, Margherita
AU - Goldwurm, Andrea
AU - Gu, Liyi
AU - Guainazzi, Matteo
AU - Haas, Daniel
AU - Haba, Yoshito
AU - Hagino, Kouichi
AU - Hamaguchi, Kenji
AU - Harayama, Atsushi
AU - Harrus, Ilana
AU - Hatsukade, Isamu
AU - Hayashi, Takayuki
AU - Hayashi, Katsuhiro
AU - Hayashida, Kiyoshi
AU - Hiraga, Junko
AU - Hirose, Kazuyuki
AU - Hornschemeier, Ann
AU - Hoshino, Akio
AU - Hughes, John
AU - Ichinohe, Yuto
AU - Iizuka, Ryo
AU - Inoue, Yoshiyuki
AU - Inoue, Hajime
AU - Ishibashi, Kazunori
AU - Ishida, Manabu
AU - Ishikawa, Kumi
AU - Ishimura, Kosei
AU - Ishisaki, Yoshitaka
AU - Itoh, Masayuki
AU - Iwata, Naoko
AU - Iyomoto, Naoko
AU - Jewell, Chris
AU - Kaastra, Jelle
AU - Kallman, Timothy
AU - Kamae, Tuneyoshi
AU - Kara, Erin
AU - Kataoka, Jun
AU - Katsuda, Satoru
AU - Katsuta, Junichiro
AU - Kawaharada, Madoka
AU - Kawai, Nobuyuki
AU - Kawano, Taro
AU - Kawasaki, Shigeo
AU - Khangulyan, Dmitry
AU - Kilbourne, Caroline
AU - Kimball, Mark
AU - King, Ashley
AU - Kitaguchi, Takao
AU - Kitamoto, Shunji
AU - Kitayama, Tetsu
AU - Kohmura, Takayoshi
AU - Kosaka, Tatsuro
AU - Koujelev, Alex
AU - Koyama, Katsuji
AU - Koyama, Shu
AU - Kretschmar, Peter
AU - Krimm, Hans
AU - Kubota, Aya
AU - Kunieda, Hideyo
AU - Laurent, Philippe
AU - Lebrun, François
AU - Lee, Shiu Hang
AU - Leutenegger, Maurice
AU - Limousin, Olivier
AU - Loewenstein, Michael
AU - Long, Knox
AU - Lumb, David
AU - Madejski, Grzegorz
AU - Maeda, Yoshitomo
AU - Maier, Daniel
AU - Makishima, Kazuo
AU - Markevitch, Maxim
AU - Masters, Candace
AU - Matsumoto, Hironori
AU - Matsushita, Kyoko
AU - McCammon, Dan
AU - Mcguinness, Daniel
AU - McNamara, Brian
AU - Mehdipour, Missagh
AU - Miko, Joseph
AU - Miller, Jon
AU - Miller, Eric
AU - Mineshige, Shin
AU - Minesugi, Kenji
AU - Mitsuishi, Ikuyuki
AU - Miyazawa, Takuya
AU - Mizuno, Tsunefumi
AU - Mori, Koji
AU - Mori, Hideyuki
AU - Moroso, Franco
AU - Moseley, Harvey
AU - Muench, Theodore
AU - Mukai, Koji
AU - Murakami, Hiroshi
AU - Murakami, Toshio
AU - Mushotzky, Richard
AU - Nagano, Housei
AU - Nagino, Ryo
AU - Nakagawa, Takao
AU - Nakajima, Hiroshi
AU - Nakamori, Takeshi
AU - Nakano, Toshio
AU - Nakashima, Shinya
AU - Nakazawa, Kazuhiro
AU - Namba, Yoshiharu
AU - Natsukari, Chikara
AU - Nishioka, Yusuke
AU - Nobukawa, Masayoshi
AU - Nobukawa, Kumiko
AU - Noda, Hirofumi
AU - Nomachi, Masaharu
AU - O'Dell, Steve
AU - Odaka, Hirokazu
AU - Ogawa, Hiroyuki
AU - Ogawa, Mina
AU - Ogi, Keiji
AU - Ohno, Masanori
AU - Ohta, Masayuki
AU - Okajima, Takashi
AU - Okamoto, Atsushi
AU - Okazaki, Tsuyoshi
AU - Ota, Naomi
AU - Ozaki, Masanobu
AU - Paerels, Frederik
AU - Paltani, Stéphane
AU - Parmar, Arvind
AU - Petre, Robert
AU - Pinto, Ciro
AU - Pohl, Martin
AU - Pontius, James
AU - Porter, F. Scott
AU - Pottschmidt, Katja
AU - Ramsey, Brian
AU - Reynolds, Christopher
AU - Russell, Helen
AU - Safi-Harb, Samar
AU - Saito, Shinya
AU - Sakai, Shin Ichiro
AU - Sakai, Kazuhiro
AU - Sameshima, Hiroaki
AU - Sasaki, Toru
AU - Sato, Goro
AU - Sato, Yoichi
AU - Sato, Kosuke
AU - Sato, Rie
AU - Sawada, Makoto
AU - Schartel, Norbert
AU - Serlemitsos, Peter
AU - Seta, Hiromi
AU - Shibano, Yasuko
AU - Shida, Maki
AU - Shidatsu, Megumi
AU - Shimada, Takanobu
AU - Shinozaki, Keisuke
AU - Shirron, Peter
AU - Simionescu, Aurora
AU - Simmons, Cynthia
AU - Smith, Randall
AU - Sneiderman, Gary
AU - Soong, Yang
AU - Stawarz, Łukasz
AU - Sugawara, Yasuharu
AU - Sugita, Hiroyuki
AU - Sugita, Satoshi
AU - Szymkowiak, Andrew
AU - Tajima, Hiroyasu
AU - Takahashi, Hiromitsu
AU - Takeda, Shin'ichiro
AU - Takei, Yoh
AU - Tamagawa, Toru
AU - Tamura, Takayuki
AU - Tamura, Keisuke
AU - Tanaka, Takaaki
AU - Tanaka, Yasuo
AU - Tanaka, Yasuyuki
AU - Tashiro, Makoto
AU - Tawara, Yuzuru
AU - Terada, Yukikatsu
AU - Terashima, Yuichi
AU - Tombesi, Francesco
AU - Tomida, Hiroshi
AU - Tsuboi, Yohko
AU - Tsujimoto, Masahiro
AU - Tsunemi, Hiroshi
AU - Tsuru, Takeshi
AU - Uchida, Hiroyuki
AU - Uchiyama, Yasunobu
AU - Uchiyama, Hideki
AU - Ueda, Yoshihiro
AU - Ueda, Shutaro
AU - Ueno, Shiro
AU - Uno, Shin'ichiro
AU - Urry, Meg
AU - Ursino, Eugenio
AU - De Vries, Cor
AU - Wada, Atsushi
AU - Watanabe, Shin
AU - Watanabe, Tomomi
AU - Werner, Norbert
AU - Wik, Daniel
AU - Wilkins, Dan
AU - Williams, Brian
AU - Yamada, Takahiro
AU - Yamada, Shinya
AU - Yamaguchi, Hiroya
AU - Yamaoka, Kazutaka
AU - Yamasaki, Noriko
AU - Yamauchi, Makoto
AU - Yamauchi, Shigeo
AU - Yaqoob, Tahir
AU - Yatsu, Yoichi
AU - Yonetoku, Daisuke
AU - Yoshida, Atsumasa
AU - Yuasa, Takayuki
AU - Zhuravleva, Irina
AU - Zoghbi, Abderahmen
N1 - Funding Information: We acknowledge all the JAXA members who have contributed to the ASTRO-H (Hitomi) project. All U.S. members gratefully acknowledge support through the NASA Science Mission Directorate. Stanford and SLAC members acknowledge support via DoE contract to SLAC National Accelerator Laboratory DE-AC3- 76SF00515 and NASA grant NNX15AM19G. Part of this work was performed under the auspices of the U.S. DoE by LLNL under Contract DE-AC52-07NA27344 and also supported by NASA grants to LLNL. Support from the European Space Agency is gratefully acknowledged. French members acknowledge support from CNES, the Centre National d'Etudes Spatiales. SRON is supported by NWO, the Netherlands Organization for Scientific Research. Swiss team acknowledges support of the Swiss Secretariat for Education, Research and Innovation SERI and ESA's PRODEX programme. The Canadian Space Agency is acknowledged for the support of Canadian members. We acknowledge support from JSPS/MEXT KAKENHI grant numbers 15H02070, 15K05107, 23340071, 26109506, 24103002, 25400236, 25800119, 25400237, 25287042, 24540229, 25105516, 23540280, 25400235, 25247028, 26800095, 25400231, 25247028, 26220703, 24105007, 23340055, 15H00773, 23000004 15H02090, 15K17610, 15H05438, 15H00785, and 24540232. H. Akamatsu acknowledges support of NWO via Veni grant. M. Axelsson acknowledges JSPS International Research Fellowship. C. Done acknowledges STFC funding under grant ST/L00075X/1. P. Gandhi acknowledges JAXA International Top Young Fellowship and UK Science and Technology Funding Council (STFC) grant ST/J003697/2. H. Russell acknowledges support from ERC Advanced Grant Feedback 340442. We thank contributions by many companies, including in particular, NEC, Mitsubishi Heavy Industries, Sumitomo Heavy Industries, and Japan Aviation Electronics Industry. We thank the support from the JSPS Core-to-Core Program. Publisher Copyright: © 2016 SPIE.
PY - 2016
Y1 - 2016
N2 - The Hitomi (ASTRO-H) mission is the sixth Japanese X-ray astronomy satellite developed by a large international collaboration, including Japan, USA, Canada, and Europe. The mission aimed to provide the highest energy resolution ever achieved at E > 2 keV, using a microcalorimeter instrument, and to cover a wide energy range spanning four decades in energy from soft X-rays to gamma-rays. After a successful launch on 2016 February 17, the spacecraft lost its function on 2016 March 26, but the commissioning phase for about a month provided valuable information on the on-board instruments and the spacecraft system, including astrophysical results obtained from first light observations. The paper describes the Hitomi (ASTRO-H) mission, its capabilities, the initial operation, and the instruments/spacecraft performances confirmed during the commissioning operations for about a month.
AB - The Hitomi (ASTRO-H) mission is the sixth Japanese X-ray astronomy satellite developed by a large international collaboration, including Japan, USA, Canada, and Europe. The mission aimed to provide the highest energy resolution ever achieved at E > 2 keV, using a microcalorimeter instrument, and to cover a wide energy range spanning four decades in energy from soft X-rays to gamma-rays. After a successful launch on 2016 February 17, the spacecraft lost its function on 2016 March 26, but the commissioning phase for about a month provided valuable information on the on-board instruments and the spacecraft system, including astrophysical results obtained from first light observations. The paper describes the Hitomi (ASTRO-H) mission, its capabilities, the initial operation, and the instruments/spacecraft performances confirmed during the commissioning operations for about a month.
KW - Gamma-ray
KW - Gamma-ray Astronomy
KW - Hard X-ray
KW - X-ray
KW - X-ray Astronomy
KW - microcalorimeter
UR - http://www.scopus.com/inward/record.url?scp=85003550769&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85003550769&partnerID=8YFLogxK
U2 - 10.1117/12.2232379
DO - 10.1117/12.2232379
M3 - Conference contribution
AN - SCOPUS:85003550769
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - Space Telescopes and Instrumentation 2016
A2 - Bautz, Marshall
A2 - Takahashi, Tadayuki
A2 - den Herder, Jan-Willem A.
PB - SPIE
T2 - Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
Y2 - 26 June 2016 through 1 July 2016
ER -