抄録
DIOS (Diffuse Intergalactic Oxygen Surveyor) is a small scientific satellite with a main aim for the search of warm-hot intergalactic medium using redshifted OVII and OVIII lines. The instrument will consist of a 4-stage X-ray telescope and an array of TES microcalorimeters with 256 pixels, cooled with mechanical coolers. Hardware development of DIOS and the expected results are described. Survey observations over about 5°×5°area will reveal new filamentary structures. DIOS will be proposed to the 3rd mission in JAXA's small satellite series in 2011, aiming for launch around 2016 if it will be selected.
本文言語 | English |
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ホスト出版物のタイトル | Space Telescopes and Instrumentation 2010 |
ホスト出版物のサブタイトル | Ultraviolet to Gamma Ray |
DOI | |
出版ステータス | Published - 2010 |
外部発表 | はい |
イベント | Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray - San Diego, CA, United States 継続期間: 28-06-2010 → 02-07-2010 |
出版物シリーズ
名前 | Proceedings of SPIE - The International Society for Optical Engineering |
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巻 | 7732 |
ISSN(印刷版) | 0277-786X |
Other
Other | Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray |
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国/地域 | United States |
City | San Diego, CA |
Period | 28-06-10 → 02-07-10 |
All Science Journal Classification (ASJC) codes
- 電子材料、光学材料、および磁性材料
- 凝縮系物理学
- コンピュータ サイエンスの応用
- 応用数学
- 電子工学および電気工学