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論文・著書情報
| タイトル |
| 和文: | |
| 英文: | XEUS: the x-ray evolving universe spectroscopy mission |
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| 著者 |
| 和文: |
Parmar, A. N.,
Hasinger, G.,
Arnaud, M.,
Barcons, X.,
Barret, D.,
Blanchard, A.,
Boehringer, H.,
Cappi, M.,
Comastri, A.,
Courvoisier, T.,
Fabian, A. C.,
Georgantopoulos, I.,
Griffiths, R.,
河合 誠之,
Koyama, K.,
Makishima, K.,
Malaguti, P.,
Mason, K. O.,
Motch, C.,
Mendez, M.,
Ohashi, T.,
Paerels, F.,
Piro, L.,
Schmitt, J.,
van der Klis, M.,
Ward, M. ..
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| 英文: |
Parmar, A. N.,
Hasinger, G.,
Arnaud, M.,
Barcons, X.,
Barret, D.,
Blanchard, A.,
Boehringer, H.,
Cappi, M.,
Comastri, A.,
Courvoisier, T.,
Fabian, A. C.,
Georgantopoulos, I.,
Griffiths, R.,
Kawai, N.,
Koyama, K.,
Makishima, K.,
Malaguti, P.,
Mason, K. O.,
Motch, C.,
Mendez, M.,
Ohashi, T.,
Paerels, F.,
Piro, L.,
Schmitt, J.,
van der Klis, M.,
Ward, M. ..
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| 言語 |
English |
| 掲載誌/書名 |
| 和文: | |
| 英文: | X-Ray and Gamma-Ray Telescopes and Instruments for Astronomy. Edited by Joachim E. Truemper, Harvey D. Tananbaum. Proceedings of the SPIE, Volume 4851, pp. 304-313 (2003). |
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巻, 号, ページ
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Vol. 4851
pp. 304-313
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| 出版年月 |
2003年3月 |
| 出版者 |
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| 会議名称 |
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| 開催地 |
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| アブストラクト |
XEUS is under study by ESA as part of the Horizon 2000+ program to utilize the International Space Station (ISS) for astronomical applications. XEUS will be a long-term x-ray observatory with an initial mirror area of 6 m2 at 1 keV that will be expanded to 30 m2 following a visit to the ISS. The 1 keV spatial resolution is expected to be 2-5" half-energy-width. XEUS will consist of separate detector and mirror spacecraft aligned by active control to provide a focal length of 50 m. A new detector spacecraft, complete with the next generation of instruments, will also be added after visiting the ISS. The limiting sensitivity will then be 4×10-18 erg cm-2s-1, around 200 times better than XMM-Newton, allowing XEUS to study the properties of the hot baryons and dark matter at high redshift. |
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