抄録
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 highenergy universe via a suite of four instruments, covering a very wide energy range, from 0.3 keV to 600 keV. These instruments include a high-resolution, high-Throughput spectrometer sensitive over 0.3-12 keV with high spectral resolution of ?E 5 7 eV, enabled by a micro-calorimeter array located in the focal plane of thin-foil X-ray optics; hard X-ray imaging spectrometers covering 5-80 keV, located in the focal plane of multilayer-coated, focusing hard X-ray mirrors; a wide-field imaging spectrometer sensitive over 0.4-12 keV, with an X-ray CCD camera in the focal plane of a soft X-ray telescope; and a non-focusing Compton-camera type soft gamma-ray detector, sensitive in the 40-600 keV band. The simultaneous broad bandpass, coupled with high spectral resolution, will enable the pursuit of a wide variety of important science themes.
本文言語 | 英語 |
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ホスト出版物のタイトル | Space Telescopes and Instrumentation 2012 |
ホスト出版物のサブタイトル | Ultraviolet to Gamma Ray |
DOI | |
出版ステータス | 出版済み - 2012 |
外部発表 | はい |
イベント | Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray - Amsterdam, オランダ 継続期間: 7月 1 2012 → 7月 6 2012 |
出版物シリーズ
名前 | Proceedings of SPIE - The International Society for Optical Engineering |
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巻 | 8443 |
ISSN(印刷版) | 0277-786X |
その他
その他 | Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray |
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国/地域 | オランダ |
City | Amsterdam |
Period | 7/1/12 → 7/6/12 |
!!!All Science Journal Classification (ASJC) codes
- 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
「The ASTRO-H X-ray observatory」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。引用スタイル
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The ASTRO-H X-ray observatory. / Takahashi, Tadayuki; Mitsuda, Kazuhisa; Kelley, Richard その他.
Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray. 2012. 84431Z (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 8443).研究成果: 書籍/レポート タイプへの寄稿 › 会議への寄与
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TY - GEN
T1 - The ASTRO-H X-ray observatory
AU - Takahashi, Tadayuki
AU - Mitsuda, Kazuhisa
AU - Kelley, Richard
AU - Aarts, Henri
AU - Aharonian, Felix
AU - Akamatsu, Hiroki
AU - Akimotoe, Fumie
AU - Allen, Steve
AU - Anabuki, Naohisa
AU - Angelini, Lorella
AU - Arnaud, Keith
AU - Asai, Makoto
AU - Audard, Marc
AU - Awaki, Hisamitsu
AU - Azzarello, Philipp
AU - Baluta, Chris
AU - Bamba, Aya
AU - Bando, Nobutaka
AU - Bautz, Mark
AU - Blandford, Roger
AU - Boyce, Kevin
AU - Brown, Greg
AU - Cackett, Ed
AU - Chernyakova, Maria
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 - Funk, Stefan
AU - Furuzawa, Akihiro
AU - Galeazzi, Massimiliano
AU - Gallo, Luigi
AU - Gandhi, Poshak
AU - Gendreau, Keith
AU - Gilmore, Kirk
AU - Haas, Daniel
AU - Haba, Yoshito
AU - Hamaguchi, Kenji
AU - Hatsukade, Isamu
AU - Hayashi, Takayuki
AU - Hayashida, Kiyoshi
AU - Hiraga, Junko
AU - Hirose, Kazuyuki
AU - Hornschemeier, Ann
AU - Hoshino, Akio
AU - Hughes, John
AU - Hwang, Una
AU - Iizuka, Ryo
AU - Inoue, Yoshiyuki
AU - Ishibashi, Kazunori
AU - Ishida, Manabu
AU - Ishimura, Kosei
AU - Ishisaki, Yoshitaka
AU - Ito, Masayuki
AU - Iwat, Naoko
AU - Iyomoto, Naoko
AU - Kaastr, Jelle
AU - Kallman, Timothy
AU - Kamae, Tuneyoshi
AU - Kataoka, Jun
AU - Katsuda, Satoru
AU - Kawahara, Hajime
AU - Kawaharada, Madoka
AU - Kawai, Nobuyuki
AU - Kawasaki, Shigeo
AU - Khangaluyan, Dmitry
AU - Kilbourne, Caroline
AU - Kimura, Masashi
AU - Kinugasaa, Kenzo
AU - Kitamoto, Shunji
AU - Kitayama, Tetsu
AU - Kohmura, Takayoshi
AU - Kokubun, Motohide
AU - Kosaka, Tatsuro
AU - Koujelev, Alex
AU - Koyama, Katsuji
AU - Krimm, Hans
AU - Kubota, Aya
AU - Kunieda, Hideyo
AU - LaMass, Stephanie
AU - Laurent, Philippe
AU - Lebrun, Francois
AU - Leutenegger, Maurice
AU - Limousin, Olivier
AU - Loewenstein, Michael
AU - Long, Knox
AU - Lumb, David
AU - Madejski, Grzegorz
AU - Maedaa, Yoshitomo
AU - Makishima, Kazuo
AU - Marchand, Genevieve
AU - Markevitch, Maxim
AU - Matsumoto, Hironori
AU - Matsushita, Kyoko
AU - McCammona, Dan
AU - McNamara, Brian
AU - Miller, Jon
AU - Miller, Eric
AU - Mineshige, Shin
AU - Minesugi, Kenji
AU - Mitsuishi, Ikuyuki
AU - Miyazaw, Takuya
AU - Mizuno, Tsunefumi
AU - Mori, Hideyuki
AU - Mori, Koji
AU - Mukai, Koji
AU - Murakami, Toshio
AU - Murakami, Hiroshi
AU - Mushotzky, Richard
AU - Nagano, Housei
AU - Nagino, Ryo
AU - Nakagaw, Takao
AU - Nakajim, Hiroshi
AU - Nakamori, Takeshi
AU - Nakazaw, Kazuhiro
AU - Namba, Yoshiharu
AU - Natsukari, Chikara
AU - Nishiok, Yusuke
AU - Nobukawa, Masayoshi
AU - Nomachi, Masaharu
AU - O'Dell, Steve
AU - Odak, Hirokazu
AU - Ogaw, Hiroyuki
AU - Ogaw, Mina
AU - Ogi, Keiji
AU - Ohashi, Takaya
AU - Ohno, Masanori
AU - Ohta, Masayuki
AU - Okajima, Takashi
AU - Okamotoa, Atsushi
AU - Okazaki, Tsuyoshi
AU - Ota, Naomi
AU - Ozaki, Masanobu
AU - Paerelsb, Frits
AU - Paltanii, Stephane
AU - Parmar, Arvind
AU - Petre, Robert
AU - Pohl, Martin
AU - Porter, F. Scott
AU - Ramsey, Brian
AU - Reis, Rubens
AU - Reynolds, Christopher
AU - Russell, Helen
AU - Sa-Harb, Samar
AU - Sakai, Shin Ichiro
AU - Sameshima, Hiroaki
AU - Sanders, Jeremy
AU - Sato, Goro
AU - Sato, Rie
AU - Sato, Yoichi
AU - Sato, Kosuke
AU - Sawada, Makoto
AU - Serlemitsos, Peter
AU - Seta, Hiromi
AU - Shibano, Yasuko
AU - Shida, Maki
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, Lukasz
AU - Sugawara, Yasuharu
AU - Sugita, Hiroyuki
AU - Sugit, Satoshi
AU - Szymkowiak, Andrew
AU - Tajim, 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 - Tashiro, Makoto
AU - Tawara, Yuzuru
AU - Terada, Yukikatsu
AU - Terashima, Yuichi
AU - Tombesi, Francesco
AU - Tomida, Hiroshi
AU - Tsuboi, Yoko
AU - Tsujimoto, Masahiro
AU - Tsunemi, Hiroshi
AU - Tsuru, Takeshi
AU - Uchida, Hiroyuki
AU - Uchiyam, Yasunobu
AU - Uchiyam, Hideki
AU - Ueda, Yoshihiro
AU - Ueno, Shiro
AU - Unobe, Shinichiro
AU - Urry, Meg
AU - Ursino, Eugenio
AU - De Vries, Cor
AU - Wada, Atsushi
AU - Watanabe, Shin
AU - Werner, Norbert
AU - White, Nicholas
AU - Yamada, Takahiro
AU - Yamada, Shinya
AU - Yamaguchi, Hiroya
AU - Yamasaki, Noriko
AU - Yamauchi, Shigeo
AU - Yamauchi, Makoto
AU - Yatsuag, Yoichi
AU - Yonetok, Daisuke
AU - Yoshida, Atsumasa
AU - Yuasa, Takayuki
PY - 2012
Y1 - 2012
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 highenergy universe via a suite of four instruments, covering a very wide energy range, from 0.3 keV to 600 keV. These instruments include a high-resolution, high-Throughput spectrometer sensitive over 0.3-12 keV with high spectral resolution of ?E 5 7 eV, enabled by a micro-calorimeter array located in the focal plane of thin-foil X-ray optics; hard X-ray imaging spectrometers covering 5-80 keV, located in the focal plane of multilayer-coated, focusing hard X-ray mirrors; a wide-field imaging spectrometer sensitive over 0.4-12 keV, with an X-ray CCD camera in the focal plane of a soft X-ray telescope; and a non-focusing Compton-camera type soft gamma-ray detector, sensitive in the 40-600 keV band. The simultaneous broad bandpass, coupled with high spectral resolution, will enable the pursuit of a wide variety of important science themes.
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 highenergy universe via a suite of four instruments, covering a very wide energy range, from 0.3 keV to 600 keV. These instruments include a high-resolution, high-Throughput spectrometer sensitive over 0.3-12 keV with high spectral resolution of ?E 5 7 eV, enabled by a micro-calorimeter array located in the focal plane of thin-foil X-ray optics; hard X-ray imaging spectrometers covering 5-80 keV, located in the focal plane of multilayer-coated, focusing hard X-ray mirrors; a wide-field imaging spectrometer sensitive over 0.4-12 keV, with an X-ray CCD camera in the focal plane of a soft X-ray telescope; and a non-focusing Compton-camera type soft gamma-ray detector, sensitive in the 40-600 keV band. The simultaneous broad bandpass, coupled with high spectral resolution, will enable the pursuit of a wide variety of important science themes.
UR - http://www.scopus.com/inward/record.url?scp=84871726495&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84871726495&partnerID=8YFLogxK
U2 - 10.1117/12.926190
DO - 10.1117/12.926190
M3 - Conference contribution
AN - SCOPUS:84871726495
SN - 9780819491442
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - Space Telescopes and Instrumentation 2012
T2 - Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray
Y2 - 1 July 2012 through 6 July 2012
ER -