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Proceedings Paper

Recent progress in the ground calibration of the ASTRO-H Hard X-ray telescope (HXT-2)
Author(s): Hideyuki Mori; Yuji Kuroda; Takuya Miyazawa; Hisamitsu Awaki; Yasunori Babazaki; Akihiro Furuzawa; Tatsuya Hibino; Ryo Iizuka; Kazunori Ishibashi; Toshihiro Iwase; Hideyo Kunieda; Daichi Kurihara; Hironori Matsumoto; Yusuke Miyata; Shigetaka Saji; Satoshi Sugita; Yoshio Suzuki; Sasagu Tachibana; Keisuke Tamura; Yuzuru Tawara; Kentaro Uesugi
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Paper Abstract

The 6th Japanese X-ray satellite, ASTRO-H, equips two Hard X-ray Telescopes (HXTs) to perform imaging spectroscopy up to 70 keV. The 2nd flight module (HXT-2) had been completed in July, 2013. After some environmental tests were passed, the X-ray performance of the HXT-2 was measured at the SPring-8 BL20B2, 3rd generation synchrotron facility. The angular resolution defined with a Half Power Diameter (HPD) was 1:′9 at 30 keV and 1:′8 at 50 keV. This small energy dependence is considered to be caused by the difference in image quality of each foil; the inner mirror shells have better quality than outer ones. The effective area was found to be 178 cm2 at 30 keV and 82 cm2 at 50 keV, both of which exceed the requirement. Furthermore, the detailed energy dependence of the effective area was examined for a limited aperture in the 30{70 keV band with a pitch of 1 keV. We also measured the off-axis dependence of the effective area at 50 keV, and then determined the optical axis. The field of view of the HXT-2 was found to be 5:′6 (FWHM of the vignetting function), consistent with the simulation. In this paper, we also report the detailed analysis of the ground calibration data, which will be used for image reconstruction by a ray-tracing simulator.

Paper Details

Date Published: 24 July 2014
PDF: 10 pages
Proc. SPIE 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 914457 (24 July 2014); doi: 10.1117/12.2055656
Show Author Affiliations
Hideyuki Mori, Nagoya Univ. (Japan)
Yuji Kuroda, Nagoya Univ. (Japan)
Takuya Miyazawa, Nagoya Univ. (Japan)
Hisamitsu Awaki, Ehime Univ. (Japan)
Yasunori Babazaki, Nagoya Univ. (Japan)
Akihiro Furuzawa, Nagoya Univ. (Japan)
Tatsuya Hibino, Nagoya Univ. (Japan)
Ryo Iizuka, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (Japan)
Kazunori Ishibashi, Nagoya Univ. (Japan)
Toshihiro Iwase, Nagoya Univ. (Japan)
Hideyo Kunieda, Nagoya Univ. (Japan)
Daichi Kurihara, Ehime Univ. (Japan)
Hironori Matsumoto, Nagoya Univ. (Japan)
Yusuke Miyata, Nagoya Univ. (Japan)
Shigetaka Saji, Nagoya Univ. (Japan)
Satoshi Sugita, Ehime Univ. (Japan)
Yoshio Suzuki, Japan Synchrotron Radiation Research Institute (Japan)
Sasagu Tachibana, Nagoya Univ. (Japan)
Keisuke Tamura, Nagoya Univ. (Japan)
Yuzuru Tawara, Nagoya Univ. (Japan)
Kentaro Uesugi, Japan Synchrotron Radiation Research Institute (Japan)


Published in SPIE Proceedings Vol. 9144:
Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray
Tadayuki Takahashi; Jan-Willem A. den Herder; Mark Bautz, Editor(s)

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