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Proceedings Paper

Ultra high throughput four-reflection x-ray telescope for high resolution spectroscopy
Author(s): Yuzuru Tawara; Ikuyuki Mitsuishi; Yasunori Babazaki; Ren Nakamichi; Ayako Bandai
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Paper Abstract

The first application of four-times reflection X-ray optics is planned for the DIOS mission, in which very soft X-ray observation is expected. On the other hand, effective area of the telescope for higher X-ray energy (E < 10 keV) including iron K emission lines has been so far limited to about 1000 cm2 for assumed several meter focal length. However, if we introduce four-reflection optics to this energy range, we can get several times large effective area for single telescope with same several meter focal length. To prove this possibility, we performed ray tracing simulation for four-reflection telescope with 6 m focal length and found that effective area of 3100 cm2 at 6 keV can be obtained for single telescope. In this paper, we will discuss about other telescope performances, mechanical properties and application to fine spectroscopic mission using X-ray micro-calorimeter.

Paper Details

Date Published: 4 September 2015
PDF: 7 pages
Proc. SPIE 9603, Optics for EUV, X-Ray, and Gamma-Ray Astronomy VII, 96030D (4 September 2015); doi: 10.1117/12.2187922
Show Author Affiliations
Yuzuru Tawara, Nagoya Univ. (Japan)
Ikuyuki Mitsuishi, Nagoya Univ. (Japan)
Yasunori Babazaki, Nagoya Univ. (Japan)
Ren Nakamichi, Nagoya Univ. (Japan)
Ayako Bandai, 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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