The High-Resolution X-ray Microcalorimeter Spectrometer System for the SXS on ASTRO-H

被引：27

作者：

Mitsuda, Kazuhisa ^{[1
]}

Kelley, Richard L. ^{[7
]}

Boyce, Kevin R. ^{[7
]}

Brown, Gregory V. ^{[10
]}

Costantini, Elisa ^{[11
]}

DiPirro, Michael J. ^{[7
]}

Ezoe, Yuichiro ^{[3
]}

Fujimoto, Ryuichi ^{[4
]}

Gendreau, Keith C. ^{[7
]}

den Herder, Jan-Willem ^{[11
]}

Hoshino, Akio ^{[4
]}

Ishisaki, Yoshitaka ^{[3
]}

Kilbourne, Caroline A.

Kitamoto, Shunji

McCammon, Dan ^{[8
]}

Murakami, Masahide

Murakami, Hiroshi

Ogawa, Mina ^{[1
]}

Ohashi, Takaya

Okamoto, Atsushi ^{[2
]}

Paltani, Stephane ^{[12
]}

Pohl, Martin ^{[12
]}

Porter, F. Scott ^{[7
]}

Sato, Yoichi

Shinozaki, Keisuke ^{[2
]}

Shirron, Peter J.

Sneiderman, Gary A.

Sugita, Hiroyuki ^{[2
]}

Szymkowiak, Andrew ^{[9
]}

Takei, Yoh ^{[1
]}

Tamagawa, Toru ^{[6
]}

Tashiro, Makoto ^{[5
]}

Terada, Yukikatsu ^{[5
]}

Tsujimoto, Masahiro ^{[1
]}

de Vries, Cor ^{[11
]}

Yamaguchi, Hiroya ^{[6
]}

Yamasaki, Noriko Y. ^{[1
]}

机构：

[1] JAXA, Inst Space & Astronaut Sci, Sagamihara, Kanagawa, Japan

[2] JAXA, Aerosp Res & Dev Directorate, Tsukuba, Ibaraki, Japan

[3] Tokyo Metropolitan Univ, Hachioji, Tokyo, Japan

[4] Kanazawa Univ, Kanazawa, Ishikawa, Japan

[5] Saitama Univ, Saitama, Japan

[6] Riken, Wako, Saitama, Japan

[7] NASA Goddard, Greenbelt, MD USA

[8] Univ Wisconsin, Madison, WI USA

[9] Yale Univ, New Haven, CT USA

[10] Lawrence Livermore Natl Lab, Livermore, CA USA

[11] SRON Netherlands Inst Space Res, Utrecht, Netherlands

[12] Univ Geneva, Geneva, Switzerland

来源：

SPACE TELESCOPES AND INSTRUMENTATION 2010: ULTRAVIOLET TO GAMMA RAY | 2010年 / 7732卷

关键词：

X-ray astronomy; Soft X-ray; High resolution X-ray Spectroscopy;

D O I：

10.1117/12.856778

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present the science and an overview of the Soft X-ray Spectrometer onboard the ASTRO-H mission with emphasis on the detector system. The SXS consists of X-ray focusing mirrors and a microcalorimeter array and is developed by international collaboration lead by JAXA and NASA with European participation. The detector is a 6 x 6 format microcalorimeter array operated at a cryogenic temperature of 50 mK and covers a 3' x 3' filed of view of the X-ray telescope of 5.6 m focal length. We expect an energy resolution better than 7 eV (FWHM, requirement) with a goal of 4 eV. The effective area of the instrument will be 225 cm(2) at 7 keV; by a factor of about two larger than that of the X-ray microcalorimeter on board Suzaku. One of the main scientific objectives of the SXS is to investigate turbulent and/or macroscopic motions of hot gas in clusters of galaxies.

引用

页数：10

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