Abstract
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 February 17, 2016, the spacecraft lost its function on March 26, 2016, but the commissioning phase for about a month provided valuable information on the onboard 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.
| Original language | English |
|---|---|
| Article number | 021402 |
| Journal | Journal of Astronomical Telescopes, Instruments, and Systems |
| Volume | 4 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 01-04-2018 |
| Externally published | Yes |
All Science Journal Classification (ASJC) codes
- Electronic, Optical and Magnetic Materials
- Control and Systems Engineering
- Instrumentation
- Astronomy and Astrophysics
- Mechanical Engineering
- Space and Planetary Science
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In: Journal of Astronomical Telescopes, Instruments, and Systems, Vol. 4, No. 2, 021402, 01.04.2018.
Research output: Contribution to journal › Review article › peer-review
TY - JOUR
T1 - HITOMI (ASTRO-H) X-ray astronomy satellite
AU - Takahashi, Tadayuki
AU - Kokubun, Motohide
AU - Mitsuda, Kazuhisa
AU - Kelley, Richard L.
AU - Ohashi, Takaya
AU - Aharonian, Felix
AU - Akamatsu, Hiroki
AU - Akimoto, Fumie
AU - Allen, Steven W.
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 W.
AU - Bialas, Thomas
AU - Blandford, Roger
AU - Boyce, Kevin
AU - Brenneman, Laura W.
AU - Brown, Gregory V.
AU - Bulbul, Esra
AU - Cackett, Edward M.
AU - Canavan, Edgar
AU - Chernyakova, Maria
AU - Chiao, Meng P.
AU - Coppi, Paolo S.
AU - Costantini, Elisa
AU - O' Dell, Steve
AU - DiPirro, Michael
AU - Done, Chris
AU - Dotani, Tadayasu
AU - Doty, John
AU - Ebisawa, Ken
AU - Eckart, Megan E.
AU - Enoto, Teruaki
AU - Ezoe, Yuichiro
AU - Fabian, Andrew C.
AU - Ferrigno, Carlo
AU - Foster, Adam R.
AU - Fujimoto, Ryuichi
AU - Fukazawa, Yasushi
AU - Funk, Stefan
AU - Furuzawa, Akihiro
AU - Galeazzi, Massimiliano
AU - Gallo, Luigi C.
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 - Harrus, Ilana M.
AU - Hatsukade, Isamu
AU - Hayashi, Takayuki
AU - Hayashi, Katsuhiro
AU - Hayashida, Kiyoshi
AU - Den Herder, Jan Willem
AU - Hiraga, Junko S.
AU - Hirose, Kazuyuki
AU - Hornschemeier, Ann
AU - Hoshino, Akio
AU - Hughes, John P.
AU - Ichinohe, Yuto
AU - Iizuka, Ryo
AU - Inoue, Hajime
AU - Inoue, Yoshiyuki
AU - Ishibashi, Kazunori
AU - Ishida, Manabu
AU - Ishikawa, Kumi
AU - Ishimura, Kosei
AU - Ishisaki, Yoshitaka
AU - Itoh, Masayuki
AU - Iwai, Masachika
AU - Iwata, Naoko
AU - Iyomoto, Naoko
AU - Jewell, Chris
AU - Kaastra, Jelle
AU - Kallman, Tim
AU - Kamae, Tsuneyoshi
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 A.
AU - Kimball, Mark
AU - King, Ashley
AU - Kitaguchi, Takao
AU - Kitamoto, Shunji
AU - Kitayama, Tetsu
AU - Kohmura, Takayoshi
AU - Konami, Saori
AU - Kosaka, Tatsuro
AU - Koujelev, Alex
AU - Koyama, Katsuji
AU - Koyama, Shu
AU - Kretschmar, Peter
AU - Krimm, Hans A.
AU - Kubota, Aya
AU - Kunieda, Hideyo
AU - Laurent, Philippe
AU - Lee, Shiu Hang
AU - Leutenegger, Maurice A.
AU - Limousin, Olivier
AU - Loewenstein, Michael
AU - Long, Knox S.
AU - Lumb, David
AU - Madejski, Greg
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 R.
AU - Mehdipour, Missagh
AU - Miko, Joseph
AU - Miller, Eric D.
AU - Miller, Jon M.
AU - Mineshige, Shin
AU - Minesugi, Kenji
AU - Mitsuishi, Ikuyuki
AU - Miyazawa, Takuya
AU - Mizuno, Tsunefumi
AU - Mori, Hideyuki
AU - Mori, Koji
AU - Moroso, Franco
AU - Moseley, Harvey
AU - Muench, Theodore
AU - Mukai, Koji
AU - Murakami, Hiroshi
AU - Murakami, Toshio
AU - Mushotzky, Richard F.
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, Kumiko K.
AU - Nobukawa, Masayoshi
AU - Noda, Hirofumi
AU - Nomachi, Masaharu
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, Frits
AU - Paltani, Stéphane
AU - Parmar, Arvind
AU - Petre, Robert
AU - Pinto, Ciro
AU - De Plaa, Jelle
AU - Pohl, Martin
AU - Pontius, James
AU - Porter, Frederick S.
AU - Pottschmidt, Katja
AU - Ramsey, Brian
AU - Reynolds, Christopher
AU - Russell, Helen
AU - Safi-Harb, Samar
AU - Saito, Shinya
AU - Sakai, Kazuhiro
AU - Sakai, Shin Ichiro
AU - Sameshima, Hiroaki
AU - Sasaki, Toru
AU - Sato, Goro
AU - Sato, Kosuke
AU - Sato, Rie
AU - Sato, Yoichi
AU - Sawada, Makoto
AU - Schartel, Norbert
AU - Serlemitsos, Peter J.
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 K.
AU - Sneiderman, Gary
AU - Soong, Yang
AU - Stawarz, Łukasz
AU - Sugawara, Yasuharu
AU - Sugita, Satoshi
AU - Sugita, Hiroyuki
AU - Szymkowiak, Andrew
AU - Tajima, Hiroyasu
AU - Takahashi, Hiromitsu
AU - Shin'ichiro, Takeda
AU - Takei, Yoh
AU - Tamagawa, Toru
AU - Tamura, Takayuki
AU - Tamura, Keisuke
AU - Tanaka, Takaaki
AU - Tanaka, Yasuo
AU - Tanaka, Yasuyuki T.
AU - Tashiro, Makoto S.
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 Go
AU - Uchida, Hiroyuki
AU - Uchiyama, Hideki
AU - Uchiyama, Yasunobu
AU - Ueda, Shutaro
AU - Ueda, Yoshihiro
AU - Ueno, Shiro
AU - Shin'ichiro, Uno
AU - Megan Urry, C.
AU - Ursino, Eugenio
AU - De Vries, Cor P.
AU - Wada, Atsushi
AU - Watanabe, Shin
AU - Watanabe, Tomomi
AU - Werner, Norbert
AU - Wik, Daniel R.
AU - Wilkins, Dan R.
AU - Williams, Brian J.
AU - Yamada, Shinya
AU - Yamada, Takahiro
AU - Yamaguchi, Hiroya
AU - Yamaoka, Kazutaka
AU - Yamasaki, Noriko Y.
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 - Publisher Copyright: © The Authors.
PY - 2018/4/1
Y1 - 2018/4/1
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 February 17, 2016, the spacecraft lost its function on March 26, 2016, but the commissioning phase for about a month provided valuable information on the onboard 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 February 17, 2016, the spacecraft lost its function on March 26, 2016, but the commissioning phase for about a month provided valuable information on the onboard 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 - Microcalorimeter
KW - X-ray
KW - X-ray astronomy
UR - https://www.scopus.com/pages/publications/85062992860
UR - https://www.scopus.com/pages/publications/85062992860#tab=citedBy
U2 - 10.1117/1.JATIS.4.2.021402
DO - 10.1117/1.JATIS.4.2.021402
M3 - Review article
AN - SCOPUS:85062992860
SN - 2329-4124
VL - 4
JO - Journal of Astronomical Telescopes, Instruments, and Systems
JF - Journal of Astronomical Telescopes, Instruments, and Systems
IS - 2
M1 - 021402
ER -