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Proceedings Paper

Development of a four-stage x-ray telescope for DIOS mission
Author(s): Yuzuru Tawara; Machiko Sakashita; Akihiro Furuzawa; Yasushi Ogasaka; Ryo Shibata; Keisuke Tamura; Takuya Miyazawa; Rika Takahashi; Kenta Shimoda; Chiaki Sakai
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Paper Abstract

The DIOS, Diffuse Intergalactic Oxygen Surveyor mission, is planned to observe diffuse soft X-rays, which might originate from warm-hot intergalactic medium as a target of missing baryon and as a probe of dark matter. To observe very weak diffuse soft X-rays, the FXT, four-stage X- ray telescope, is specially designed to have wide field of view and large effective area for the small satellite DIOS. It is confirmed that FXT meets basic requirements of the DIOS mission based on the ray tracing analysis. Al-foil based epoxy replication method is applied to the fabrication of element mirror of the FXT. Several tens of foil mirrors were fabricated and measured their performance. Mirror material combination was also reviewed from the view point of line observation other than oxygen.

Paper Details

Date Published: 8 September 2005
PDF: 5 pages
Proc. SPIE 5900, Optics for EUV, X-Ray, and Gamma-Ray Astronomy II, 59000J (8 September 2005); doi: 10.1117/12.615844
Show Author Affiliations
Yuzuru Tawara, Nagoya Univ. (Japan)
Machiko Sakashita, Nagoya Univ. (Japan)
Akihiro Furuzawa, Nagoya Univ. (Japan)
Yasushi Ogasaka, Nagoya Univ. (Japan)
Ryo Shibata, Nagoya Univ. (Japan)
Keisuke Tamura, Nagoya Univ. (Japan)
Takuya Miyazawa, Nagoya Univ. (Japan)
Rika Takahashi, Nagoya Univ. (Japan)
Kenta Shimoda, Nagoya Univ. (Japan)
Chiaki Sakai, Nagoya Univ. (Japan)


Published in SPIE Proceedings Vol. 5900:
Optics for EUV, X-Ray, and Gamma-Ray Astronomy II
Oberto Citterio; Stephen L. O'Dell, Editor(s)

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