Abstract
The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions initiated by the Institute of Space and Astronautical Science (ISAS). ASTRO-H will investigate the physics of the high-energy universe by performing high-resolution, high-throughput spectroscopy with moderate angular resolution. ASTRO-H covers very wide energy range from 0.3 keV to 600 keV. ASTRO-H allows a combination of wide band X-ray spectroscopy (5-80 keV) provided by multilayer coating, focusing hard X-ray mirrors and hard X-ray imaging detectors, and high energy-resolution soft X-ray spectroscopy (0.3-12 keV) provided by thin-foil X-ray optics and a micro-calorimeter array. The mission will also carry an X-ray CCD camera as a focal plane detector for a soft X-ray telescope (0.4-12 keV) and a non-focusing soft gamma-ray detector (40-600 keV). The micro-calorimeter system is developed by an international collaboration led by ISAS/JAXA and NASA. The simultaneous broad bandpass, coupled with high spectral resolution of ΔE ~7 eV provided by the micro-calorimeter will enable a wide variety of important science themes to be pursued.
| Original language | English |
|---|---|
| Title of host publication | Space Telescopes and Instrumentation 2010 |
| Subtitle of host publication | Ultraviolet to Gamma Ray |
| Publisher | SPIE |
| ISBN (Print) | 9780819482228 |
| DOIs | |
| Publication status | Published - 2010 |
Publication series
| Name | Proceedings of SPIE - The International Society for Optical Engineering |
|---|---|
| Volume | 7732 |
| ISSN (Print) | 0277-786X |
Keywords
- Gamma-ray
- Gamma-ray astronomy
- Hard X-ray
- Micro-calorimete
- X-ray
- X-ray astronomy
ASJC Scopus subject areas
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics
- Computer Science Applications
- Applied Mathematics
- Electrical and Electronic Engineering
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The ASTRO-H mission. / Takahashi, Tadayuki; Mitsuda, Kazuhisa; Kelley, Richard; Aharonian, Felix; Akimoto, Fumie; Allen, Steve; Anabuki, Naohisa; Angelini, Lorella; Arnaud, Keith; Awaki, Hisamitsu; Bamba, Aya; Bando, Nobutaka; Bautz, Mark; Blandford, Roger; Boyce, Kevin; Brown, Greg; Chernyakova, Maria; Coppi, Paolo; Costantini, Elisa; Cottam, Jean; Crow, John; De Plaa, Jelle; De Vries, Cor; Den Herder, Jan Willem; DiPirro, Michael; Done, Chris; Dotani, Tadayasu; Ebisawa, Ken; Enoto, Teruaki; Ezoe, Yuichiro; Fabian, Andrew; Fujimoto, Ryuichi; Fukazawa, Yasushi; Funk, Stefan; Furuzawa, Akihiro; Galeazzi, Massimiliano; Gandhi, Poshak; Gendreau, Keith; Gilmore, Kirk; Haba, Yoshito; Hamaguchi, Kenji; Hatsukade, Isamu; Hayashida, Kiyoshi; Hiraga, Junko; Hirose, Kazuyuki; Hornschemeier, Ann; Hughes, John; Hwang, Una; Iizuka, Ryo; Ishibashi, Kazunori; Ishida, Manabu; Ishimura, Kosei; Ishisaki, Yoshitaka; Isobe, Naoki; Ito, Masayuki; Iwata, Naoko; Kaastra, Jelle; Kallman, Timothy; Kamae, Tuneyoshi; Katagiri, Hideaki; Kataoka, Jun; Katsuda, Satoru; Kawaharada, Madoka; Kawai, Nobuyuki; Kawasaki, Shigeo; Khangaluyan, Dmitry; Kilbourne, Caroline; Kinugasa, Kenzo; Kitamoto, Shunji; Kitayama, Tetsu; Kohmura, Takayoshi; Kokubun, Motohide; Kosaka, Tatsuro; Kotani, Taro; Koyama, Katsuji; Kubota, Aya; Kunieda, Hideyo; Laurent, Philippe; Lebrun, François; Limousin, Olivier; Loewenstein, Michael; Long, Knox; Madejski, Grzegorz; Maeda, Yoshitomo; Makishima, Kazuo; Markevitch, Maxim; Matsumoto, Hironori; Matsushita, Kyoko; McCammon, Dan; Miller, Jon; Mineshige, Shin; Minesugi, Kenji; Miyazawa, Takuya; Mizuno, Tsunefumi; Mori, Koji; Mori, Hideyuki; Mukai, Koji; Murakami, Hiroshi; Murakami, Toshio; Mushotzky, Richard; Nakagawa, Yujin; Nakagawa, Takao; Nakajima, Hiroshi; Nakamori, Takeshi; Nakazawa, Kazuhiro; Namba, Yoshiharu; Nomachi, Masaharu; O'Dell, Steve; Ogawa, Hiroyuki; Ogawa, Mina; Ogi, Keiji; Ohashi, Takaya; Ohno, Masanori; Ohta, Masayuki; Okajima, Takashi; Ota, Naomi; Ozaki, Masanobu; Paerels, Frits; Paltani, Stéphane; Parmer, Arvind; Petre, Robert; Pohl, Martin; Porter, Scott; Ramsey, Brian; Reynolds, Christopher; Sakai, Shin Ichiro; Sambruna, Rita; Sato, Goro; Sato, Yoichi; Serlemitsos, Peter; Shida, Maki; Shimada, Takanobu; Shinozaki, Keisuke; Shirron, Peter; Smith, Randall; Sneiderman, Gary; Soong, Yang; Stawarz, Lukasz; Sugita, Hiroyuki; Szymkowiak, Andrew; Tajima, Hiroyasu; Takahashi, Hiromitsu; Takei, Yoh; Tamagawa, Toru; Tamura, Takayuki; Tamura, Keisuke; Tanaka, Takaaki; Tanaka, Yasuo; Tanaka, Yasuyuki; Tashiro, Makoto; Tawara, Yuzuru; Terada, Yukikatsu; Terashima, Yuichi; Tombesi, Francesco; Tomida, Hiroshi; Tozuka, Miyako; Tsuboi, Yoko; Tsujimoto, Masahiro; Tsunemi, Hiroshi; Tsuru, Takeshi; Uchida, Hiroyuki; Uchiyama, Yasunobu; Uchiyama, Hideki; Ueda, Yoshihiro; Uno, Shinichiro; Urry, Meg; Watanabe, Shin; White, Nicholas; Yamada, Takahiro; Yamaguchi, Hiroya; Yamaoka, Kazutaka; Yamasaki, Noriko; Yamauchi, Makoto; Yamauchi, Shigeo; Yatsu, Yoichi; Yonetoku, Daisuke; Yoshida, Atsumasa.
Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray. SPIE, 2010. 77320Z (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7732).Research output: Chapter in Book/Report/Conference proceeding › Conference contribution
}
TY - GEN
T1 - The ASTRO-H mission
AU - Takahashi, Tadayuki
AU - Mitsuda, Kazuhisa
AU - Kelley, Richard
AU - Aharonian, Felix
AU - Akimoto, Fumie
AU - Allen, Steve
AU - Anabuki, Naohisa
AU - Angelini, Lorella
AU - Arnaud, Keith
AU - Awaki, Hisamitsu
AU - Bamba, Aya
AU - Bando, Nobutaka
AU - Bautz, Mark
AU - Blandford, Roger
AU - Boyce, Kevin
AU - Brown, Greg
AU - Chernyakova, Maria
AU - Coppi, Paolo
AU - Costantini, Elisa
AU - Cottam, Jean
AU - Crow, John
AU - De Plaa, Jelle
AU - De Vries, Cor
AU - Den Herder, Jan Willem
AU - DiPirro, Michael
AU - Done, Chris
AU - Dotani, Tadayasu
AU - Ebisawa, Ken
AU - Enoto, Teruaki
AU - Ezoe, Yuichiro
AU - Fabian, Andrew
AU - Fujimoto, Ryuichi
AU - Fukazawa, Yasushi
AU - Funk, Stefan
AU - Furuzawa, Akihiro
AU - Galeazzi, Massimiliano
AU - Gandhi, Poshak
AU - Gendreau, Keith
AU - Gilmore, Kirk
AU - Haba, Yoshito
AU - Hamaguchi, Kenji
AU - Hatsukade, Isamu
AU - Hayashida, Kiyoshi
AU - Hiraga, Junko
AU - Hirose, Kazuyuki
AU - Hornschemeier, Ann
AU - Hughes, John
AU - Hwang, Una
AU - Iizuka, Ryo
AU - Ishibashi, Kazunori
AU - Ishida, Manabu
AU - Ishimura, Kosei
AU - Ishisaki, Yoshitaka
AU - Isobe, Naoki
AU - Ito, Masayuki
AU - Iwata, Naoko
AU - Kaastra, Jelle
AU - Kallman, Timothy
AU - Kamae, Tuneyoshi
AU - Katagiri, Hideaki
AU - Kataoka, Jun
AU - Katsuda, Satoru
AU - Kawaharada, Madoka
AU - Kawai, Nobuyuki
AU - Kawasaki, Shigeo
AU - Khangaluyan, Dmitry
AU - Kilbourne, Caroline
AU - Kinugasa, Kenzo
AU - Kitamoto, Shunji
AU - Kitayama, Tetsu
AU - Kohmura, Takayoshi
AU - Kokubun, Motohide
AU - Kosaka, Tatsuro
AU - Kotani, Taro
AU - Koyama, Katsuji
AU - Kubota, Aya
AU - Kunieda, Hideyo
AU - Laurent, Philippe
AU - Lebrun, François
AU - Limousin, Olivier
AU - Loewenstein, Michael
AU - Long, Knox
AU - Madejski, Grzegorz
AU - Maeda, Yoshitomo
AU - Makishima, Kazuo
AU - Markevitch, Maxim
AU - Matsumoto, Hironori
AU - Matsushita, Kyoko
AU - McCammon, Dan
AU - Miller, Jon
AU - Mineshige, Shin
AU - Minesugi, Kenji
AU - Miyazawa, Takuya
AU - Mizuno, Tsunefumi
AU - Mori, Koji
AU - Mori, Hideyuki
AU - Mukai, Koji
AU - Murakami, Hiroshi
AU - Murakami, Toshio
AU - Mushotzky, Richard
AU - Nakagawa, Yujin
AU - Nakagawa, Takao
AU - Nakajima, Hiroshi
AU - Nakamori, Takeshi
AU - Nakazawa, Kazuhiro
AU - Namba, Yoshiharu
AU - Nomachi, Masaharu
AU - O'Dell, Steve
AU - Ogawa, Hiroyuki
AU - Ogawa, Mina
AU - Ogi, Keiji
AU - Ohashi, Takaya
AU - Ohno, Masanori
AU - Ohta, Masayuki
AU - Okajima, Takashi
AU - Ota, Naomi
AU - Ozaki, Masanobu
AU - Paerels, Frits
AU - Paltani, Stéphane
AU - Parmer, Arvind
AU - Petre, Robert
AU - Pohl, Martin
AU - Porter, Scott
AU - Ramsey, Brian
AU - Reynolds, Christopher
AU - Sakai, Shin Ichiro
AU - Sambruna, Rita
AU - Sato, Goro
AU - Sato, Yoichi
AU - Serlemitsos, Peter
AU - Shida, Maki
AU - Shimada, Takanobu
AU - Shinozaki, Keisuke
AU - Shirron, Peter
AU - Smith, Randall
AU - Sneiderman, Gary
AU - Soong, Yang
AU - Stawarz, Lukasz
AU - Sugita, Hiroyuki
AU - Szymkowiak, Andrew
AU - Tajima, Hiroyasu
AU - Takahashi, Hiromitsu
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 - Tozuka, Miyako
AU - Tsuboi, Yoko
AU - Tsujimoto, Masahiro
AU - Tsunemi, Hiroshi
AU - Tsuru, Takeshi
AU - Uchida, Hiroyuki
AU - Uchiyama, Yasunobu
AU - Uchiyama, Hideki
AU - Ueda, Yoshihiro
AU - Uno, Shinichiro
AU - Urry, Meg
AU - Watanabe, Shin
AU - White, Nicholas
AU - Yamada, Takahiro
AU - Yamaguchi, Hiroya
AU - Yamaoka, Kazutaka
AU - Yamasaki, Noriko
AU - Yamauchi, Makoto
AU - Yamauchi, Shigeo
AU - Yatsu, Yoichi
AU - Yonetoku, Daisuke
AU - Yoshida, Atsumasa
N1 - Publisher Copyright: © 2010 SPIE.
PY - 2010
Y1 - 2010
N2 - The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions initiated by the Institute of Space and Astronautical Science (ISAS). ASTRO-H will investigate the physics of the high-energy universe by performing high-resolution, high-throughput spectroscopy with moderate angular resolution. ASTRO-H covers very wide energy range from 0.3 keV to 600 keV. ASTRO-H allows a combination of wide band X-ray spectroscopy (5-80 keV) provided by multilayer coating, focusing hard X-ray mirrors and hard X-ray imaging detectors, and high energy-resolution soft X-ray spectroscopy (0.3-12 keV) provided by thin-foil X-ray optics and a micro-calorimeter array. The mission will also carry an X-ray CCD camera as a focal plane detector for a soft X-ray telescope (0.4-12 keV) and a non-focusing soft gamma-ray detector (40-600 keV). The micro-calorimeter system is developed by an international collaboration led by ISAS/JAXA and NASA. The simultaneous broad bandpass, coupled with high spectral resolution of ΔE ~7 eV provided by the micro-calorimeter will enable a wide variety of important science themes to be pursued.
AB - The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions initiated by the Institute of Space and Astronautical Science (ISAS). ASTRO-H will investigate the physics of the high-energy universe by performing high-resolution, high-throughput spectroscopy with moderate angular resolution. ASTRO-H covers very wide energy range from 0.3 keV to 600 keV. ASTRO-H allows a combination of wide band X-ray spectroscopy (5-80 keV) provided by multilayer coating, focusing hard X-ray mirrors and hard X-ray imaging detectors, and high energy-resolution soft X-ray spectroscopy (0.3-12 keV) provided by thin-foil X-ray optics and a micro-calorimeter array. The mission will also carry an X-ray CCD camera as a focal plane detector for a soft X-ray telescope (0.4-12 keV) and a non-focusing soft gamma-ray detector (40-600 keV). The micro-calorimeter system is developed by an international collaboration led by ISAS/JAXA and NASA. The simultaneous broad bandpass, coupled with high spectral resolution of ΔE ~7 eV provided by the micro-calorimeter will enable a wide variety of important science themes to be pursued.
KW - Gamma-ray
KW - Gamma-ray astronomy
KW - Hard X-ray
KW - Micro-calorimete
KW - X-ray
KW - X-ray astronomy
UR - http://www.scopus.com/inward/record.url?scp=77957866968&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=77957866968&partnerID=8YFLogxK
U2 - 10.1117/12.857875
DO - 10.1117/12.857875
M3 - Conference contribution
AN - SCOPUS:77957866968
SN - 9780819482228
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - Space Telescopes and Instrumentation 2010
PB - SPIE
ER -