| Item type |
会議発表論文 / Conference Paper(1) |
| 公開日 |
2015-03-26 |
| タイトル |
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|
タイトル |
The Hard X-ray Modulation Telescope (HXMT) mission |
|
言語 |
en |
| 言語 |
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|
言語 |
eng |
| キーワード |
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言語 |
en |
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主題Scheme |
Other |
|
主題 |
HXMT : LE, ME, HE |
| 資源タイプ |
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|
資源タイプ識別子 |
http://purl.org/coar/resource_type/c_5794 |
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資源タイプ |
conference paper |
| 著者 |
Lu, FangJun
Zhang, Shu
Wu, BoBing
Chen, Yong
Cao, XueLei
Zhang, Zhi
Deng, JingKang
Zhang, ShuangNan
Li, TiPei
|
| 著者所属（英） |
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|
en |
|
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Key Laboratory for Particle Astrophysics, Institute of High Energy Physics |
| 著者所属（英） |
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en |
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Key Laboratory for Particle Astrophysics, Institute of High Energy Physics |
| 著者所属（英） |
|
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|
en |
|
|
Key Laboratory for Particle Astrophysics, Institute of High Energy Physics |
| 著者所属（英） |
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|
en |
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Key Laboratory for Particle Astrophysics, Institute of High Energy Physics |
| 著者所属（英） |
|
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|
en |
|
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Key Laboratory for Particle Astrophysics, Institute of High Energy Physics |
| 著者所属（英） |
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|
en |
|
|
Center for Astrophysics, Tsinghua University |
| 著者所属（英） |
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en |
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Center for Astrophysics, Tsinghua University |
| 著者所属（英） |
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en |
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Center for Astrophysics, Tsinghua University |
| 著者所属（英） |
|
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en |
|
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Key Laboratory for Particle Astrophysics, Institute of High Energy Physics |
| 出版者 |
|
|
出版者 |
宇宙航空研究開発機構 |
| 出版者（英） |
|
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出版者 |
Japan Aerospace Exploration Agency (JAXA) |
| 書誌情報 |
宇宙航空研究開発機構特別資料
en : JAXA Special Publication: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop
巻 JAXA-SP-08-014E,
p. 368-372,
発行日 2009-02-27
|
| 会議概要（会議名, 開催地, 会期, 主催者等）（英） |
|
|
内容記述タイプ |
Other |
|
内容記述 |
Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008) |
| 抄録（英） |
|
|
内容記述タイプ |
Other |
|
内容記述 |
HXMT is an X-ray astronomy satellite consisting of three slat-collimated instruments, the High Energy X-ray Instrument (HE), the Medium Energy X-ray Instrument (ME), and the Low Energy X-ray Instrument (LE). HE is sensitive in 20 - 250 keV. It contains 18 individual cylindrical NaI(Tl)/CsI(Na) phoswich modules, each with an area of 283.5 sq cm and a field of view (FOV) of 5.7 deg x 1.1 deg (FWHM) each. ME is sensitive in 5 - 30 keV. It contains 3 individual Si-PIN detector arrays with an FOV of 5.7 deg x 1.1 deg each, and the total collection area is 952 sq cm. LE uses the Swept Charge Device as the detector which is sensitive in 1 - 15 keV. LE also contains 3 individual detector arrays each with two kinds of FOVs, 5.7 deg x 1.1 deg and 5.7 deg x 2.2 deg, so as to study the cosmic X-ray background in this energy band. The total collecting area of LE is 384 sq cm. HXMT will perform a broad band (1 - 250 keV) X-ray all-sky imaging survey with both high sensitivity and high spatial resolution, as well as making pointed observations of X-ray sources to study their broadband spectroscopic and multi-wavelength temporal properties in details. The 3-sigma continuum sensitivity of HXMT is about 0.5 mCrab (@100 keV, 10(exp 5) s). HXMT was proposed in 1994 and is scheduled to be launched around 2010. The designed lifetime of HXMT is 4 years. |
| 内容記述（英） |
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内容記述タイプ |
Other |
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内容記述 |
Physical characteristics: Original contains color illustrations |
| ISSN |
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収録物識別子タイプ |
ISSN |
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収録物識別子 |
1349-113X |
| 書誌レコードID |
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収録物識別子タイプ |
NCID |
|
収録物識別子 |
AA11984031 |
| 資料番号 |
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内容記述タイプ |
Other |
|
内容記述 |
資料番号: AA0064306070 |
| レポート番号 |
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|
内容記述タイプ |
Other |
|
内容記述 |
レポート番号: JAXA-SP-08-014E |
64306070.pdf (770.9 kB)
