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論文・著書情報
| タイトル |
| 和文: | |
| 英文: | Wide band X-ray Imager (WXI) and Soft Gamma-ray Detector (SGD) for the NeXT Mission |
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| 著者 |
| 和文: |
Takahashi, T.,
Awaki, A.,
Dotani, T.,
Fukazawa, Y.,
Hayashida, K.,
Kamae, T.,
片岡 淳,
河合 誠之,
Kitamoto, S.,
Kohmura, T.,
Kokubun, M.,
Koyama, K.,
Makishima, K.,
Matsumoto, H.,
Miyata, E.,
Murakami, T.,
Nakazawa, K.,
Nomachi, M.,
Ozaki, M.,
Tajima, H.,
Tashiro, M.,
Tamagawa, T.,
Terada, Y.,
Tsunemi, H.,
Tsuru, T.,
Yamaoka, K.,
Yonetoku, D.,
Yoshida, A. ..
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| 英文: |
Takahashi, T.,
Awaki, A.,
Dotani, T.,
Fukazawa, Y.,
Hayashida, K.,
Kamae, T.,
Kataoka, J.,
Kawai, N.,
Kitamoto, S.,
Kohmura, T.,
Kokubun, M.,
Koyama, K.,
Makishima, K.,
Matsumoto, H.,
Miyata, E.,
Murakami, T.,
Nakazawa, K.,
Nomachi, M.,
Ozaki, M.,
Tajima, H.,
Tashiro, M.,
Tamagawa, T.,
Terada, Y.,
Tsunemi, H.,
Tsuru, T.,
Yamaoka, K.,
Yonetoku, D.,
Yoshida, A. ..
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| 言語 |
English |
| 掲載誌/書名 |
| 和文: | |
| 英文: | UV and Gamma-Ray Space Telescope Systems. Edited by Hasinger, Günther; Turner, Martin J. L. Proceedings of the SPIE, Volume 5488, pp. 549-560 (2004). |
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巻, 号, ページ
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Vol. 5488
pp. 549-560
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| 出版年月 |
2004年10月 |
| 出版者 |
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| 会議名称 |
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| 開催地 |
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| DOI |
https://doi.org/10.1117/12.551500 |
| アブストラクト |
The NeXT mission has been proposed to study high-energy non-thermal phenomena in the universe. The high-energy response of the super mirror will enable us to perform the first sensitive imaging observations up to 80 keV. The focal plane detector, which combines a fully depleted X-ray CCD and a pixelated CdTe detector, will provide spectra and images in the wide energy range from 0.5 keV to 80 keV. In the soft gamma-ray band upto ~1 MeV, a narrow field-of-view Compton gamma-ray telescope utilizing several tens of layers of thin Si or CdTe detector will provide precise spectra with much higher sensitivity than present instruments. The continuum sensitivity will reach several x 10-8 photons/s/keV/cm2 in the hard X-ray region and a few x 10-7 photons/s/keV/cm2 in the soft gamma-ray region. |
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