The ASTRO-H Mission
The ASTRO-H Mission
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DOI：
10.1117/12.857875
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发表时间：
2009-03
期刊：
影响因子：
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通讯作者：
Tadayuki Takahashi;K. Mitsuda;R. Kelley;F. Aharonian;F. Akimoto;S. Allen;N. Anabuki;L. Angelini;K. Arnaud;H. Awaki;A. Bamba;N. Bando;M. Bautz;R. Blandford;K. Boyce;G. Brown;M. Chernyakova;P. Coppi;E. Costantini;J. Cottam;J. Crow;J. Plaa;C. D. Vries;J. Herder;M. Dipirro;C. Done;T. Dotani;K. Ebisawa;T. Enoto;Y. Ezoe;A. Fabian;R. Fujimoto;Y. Fukazawa;S. Funk;A. Furuzawa;M. Galeazzi;P. Gandhi;K. Gendreau;K. Gilmore;Y. Haba;K. Hamaguchi;I. Hatsukade;K. Hayashida;J. Hiraga;K. Hirose;A. Hornschemeier;J. Hughes;U. Hwang;R. Iizuka;K. Ishibashi;M. Ishida;K. Ishimura;Y. Ishisaki;N. Isobe;Masayuki Ito;N. Iwata;J. Kaastra;T. Kallman;T. Kamae;H. Katagiri;J. Kataoka;S. Katsuda;M. Kawaharada;N. Kawai;S. Kawasaki;Dmitry Khangaluyan;C. Kilbourne;K. Kinugasa;S. Kitamoto;T. Kitayama;T. Kohmura;M. Kokubun;T. Kosaka;T. Kotani;K. Koyama;A. Kubota;H. Kunieda;P. Laurent;F. Lebrun;O. Limousin;M. Loewenstein;K. Long;G. Madejski;Y. Maeda;K. Makishima;M. Markevitch;H. Matsumoto;K. Matsushita;D. McCammon;Jonathan M. Miller;S. Mineshige;K. Minesugi;T. Miyazawa;T. Mizuno;K. Mori;H. Mori;K. Mukai;H. Murakami;T. Murakami;R. Mushotzky;Y. Nakagawa;T. Nakagawa;H. Nakajima;T. Nakamori;K. Nakazawa;Y. Namba;M. Nomachi;S. O. Dell;H. Ogawa;M. Ogawa;K. Ogi;T. Ohashi;M. Ohno;M. Ohta;T. Okajima;N. Ota;M. Ozaki;F. Paerels;S. Paltani;Arvind Parmer;R. Petre;M. Pohl;Scott Porter;B. Ramsey;C. Reynolds;S. Sakai;R. Sambruna;G. Sato;Yoichi Sato;P. Serlemitsos;M. Shida;T. Shimada;K. Shinozaki;P. Shirron;Randall K. Smith;G. Sneiderman;Y. Soong;L. Stawarz;H. Sugita;A. Szymkowiak;H. Tajima;H. Takahashi;Y. Takei;T. Tamagawa;T. Tamura;K. Tamura;Takaaki Tanaka;Yasuo Tanaka;Yasuyuki T. Tanaka;M. Tashiro;Y. Tawara;Y. Terada;Y. Terashima;F. Tombesi;H. Tomida;Miyako Tozuka;Y. Tsuboi;M. Tsujimoto;H. Tsunemi;T. Tsuru;H. Uchida;Y. Uchiyama;H. Uchiyama;Y. Ueda;S. Uno;M. Urry;S. Watanabe;N. White;Takahiro Yamada;H. Yamaguchi;K. Yamaoka;N. Yamasaki;M. Yamauchi;S. Yamauchi;Y. Yatsu;D. Yonetoku;A. Yoshida
中科院分区：
文献类型：
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作者：
Tadayuki Takahashi;K. Mitsuda;R. Kelley;F. Aharonian;F. Akimoto;S. Allen;N. Anabuki;L. Angelini;K. Arnaud;H. Awaki;A. Bamba;N. Bando;M. Bautz;R. Blandford;K. Boyce;G. Brown;M. Chernyakova;P. Coppi;E. Costantini;J. Cottam;J. Crow;J. Plaa;C. D. Vries;J. Herder;M. Dipirro;C. Done;T. Dotani;K. Ebisawa;T. Enoto;Y. Ezoe;A. Fabian;R. Fujimoto;Y. Fukazawa;S. Funk;A. Furuzawa;M. Galeazzi;P. Gandhi;K. Gendreau;K. Gilmore;Y. Haba;K. Hamaguchi;I. Hatsukade;K. Hayashida;J. Hiraga;K. Hirose;A. Hornschemeier;J. Hughes;U. Hwang;R. Iizuka;K. Ishibashi;M. Ishida;K. Ishimura;Y. Ishisaki;N. Isobe;Masayuki Ito;N. Iwata;J. Kaastra;T. Kallman;T. Kamae;H. Katagiri;J. Kataoka;S. Katsuda;M. Kawaharada;N. Kawai;S. Kawasaki;Dmitry Khangaluyan;C. Kilbourne;K. Kinugasa;S. Kitamoto;T. Kitayama;T. Kohmura;M. Kokubun;T. Kosaka;T. Kotani;K. Koyama;A. Kubota;H. Kunieda;P. Laurent;F. Lebrun;O. Limousin;M. Loewenstein;K. Long;G. Madejski;Y. Maeda;K. Makishima;M. Markevitch;H. Matsumoto;K. Matsushita;D. McCammon;Jonathan M. Miller;S. Mineshige;K. Minesugi;T. Miyazawa;T. Mizuno;K. Mori;H. Mori;K. Mukai;H. Murakami;T. Murakami;R. Mushotzky;Y. Nakagawa;T. Nakagawa;H. Nakajima;T. Nakamori;K. Nakazawa;Y. Namba;M. Nomachi;S. O. Dell;H. Ogawa;M. Ogawa;K. Ogi;T. Ohashi;M. Ohno;M. Ohta;T. Okajima;N. Ota;M. Ozaki;F. Paerels;S. Paltani;Arvind Parmer;R. Petre;M. Pohl;Scott Porter;B. Ramsey;C. Reynolds;S. Sakai;R. Sambruna;G. Sato;Yoichi Sato;P. Serlemitsos;M. Shida;T. Shimada;K. Shinozaki;P. Shirron;Randall K. Smith;G. Sneiderman;Y. Soong;L. Stawarz;H. Sugita;A. Szymkowiak;H. Tajima;H. Takahashi;Y. Takei;T. Tamagawa;T. Tamura;K. Tamura;Takaaki Tanaka;Yasuo Tanaka;Yasuyuki T. Tanaka;M. Tashiro;Y. Tawara;Y. Terada;Y. Terashima;F. Tombesi;H. Tomida;Miyako Tozuka;Y. Tsuboi;M. Tsujimoto;H. Tsunemi;T. Tsuru;H. Uchida;Y. Uchiyama;H. Uchiyama;Y. Ueda;S. Uno;M. Urry;S. Watanabe;N. White;Takahiro Yamada;H. Yamaguchi;K. Yamaoka;N. Yamasaki;M. Yamauchi;S. Yamauchi;Y. Yatsu;D. Yonetoku;A. Yoshida
日本宇宙航空研究开发机构/美国航天局联合ASTRO-H使命是空间和宇航科学研究所发起的一系列非常成功的X射线飞行任务中的第六次。ASTRO-H将通过进行具有中等角分辨率的高分辨率、高通量光谱学研究高能宇宙的物理学。ASTRO-H涵盖了从0.3 keV到600 keV的非常宽的能量范围。ASTRO-H可以将多层涂层、聚焦硬X射线镜和硬X射线成像探测器提供的宽带X射线光谱（5-80 keV）与薄箔X射线光学器件和微量热计阵列提供的高能量分辨率软X射线光谱（0.3-12 keV）相结合。该使命还将携带一台X射线CCD照相机，作为软X射线望远镜（0.4-12千电子伏）的焦平面探测器和一台非聚焦软伽马射线探测器（40-600千电子伏）。微量热计系统是由ISAS/JAXA和NASA领导的国际合作开发的。同时的宽带通，加上高光谱分辨率的ΔE ~7 eV提供的微量热计将使各种重要的科学主题被追求。
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.