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Proceedings Paper

Development of an x-ray telescope with a large effective area for the iron K line band
Author(s): Hironori Matsumoto; Sasagu Tachibana; Shun Yoshikawa; Keisuke Tamura; Hideyuki Mori; Kojun Yamashita; Ikuyuki Mitsuishi; Yuzuru Tawara; Hideyo Kunieda
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Paper Abstract

X-ray micro-calorimeters such as the Soft X-ray Spectrometer on board ASTRO-H will enable precise spectroscopy of iron K lines. To exploit the full power of the high-energy resolution, X-ray telescopes with a large effective area around 6 keV are essentially important. We designed a Wolter-I X-ray telescope with Ir/C multi- layer mirrors to enhance the effective area at around 6 keV by the principle of Bragg reflection. We assumed a diameter of 110 cm and a focal length of 110 cm for our telescope. Our simulation suggests that the effective area averaged in the 5.7{7.7 keV band could be 2000 cm2.

Paper Details

Date Published: 4 September 2015
PDF: 8 pages
Proc. SPIE 9603, Optics for EUV, X-Ray, and Gamma-Ray Astronomy VII, 96030F (4 September 2015); doi: 10.1117/12.2190591
Show Author Affiliations
Hironori Matsumoto, Nagoya Univ. (Japan)
Sasagu Tachibana, Nagoya Univ. (Japan)
Shun Yoshikawa, Nagoya Univ. (Japan)
Keisuke Tamura, Nagoya Univ. (Japan)
Hideyuki Mori, NASA Goddard Space Flight Ctr. (United States)
Kojun Yamashita, Nagoya Univ. (Japan)
Ikuyuki Mitsuishi, Nagoya Univ. (Japan)
Yuzuru Tawara, Nagoya Univ. (Japan)
Hideyo Kunieda, Nagoya Univ. (Japan)

Published in SPIE Proceedings Vol. 9603:
Optics for EUV, X-Ray, and Gamma-Ray Astronomy VII
Stephen L. O'Dell; Giovanni Pareschi, Editor(s)

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