Autor: |
Takahashi, Tadayuki, Mitsuda, Kazuhisa, Kelley, Richard, Aharonian, Felix, Akimoto, Fumie, Allen, Steve, Anabuki, Naohisa, Angelini, Lorella, Arnaud, Keith, Awaki, Hisamitsu, Bamba, Aya, Bando, Nobutaka, Bautz, Mark, Blandford, Roger, Boyce, Kevin, Brown, Greg, Chernyakova, Maria, Coppi, Paolo, Costantini, Elisa, Cottam, Jean, Crow, John, de Plaa, Jelle, de Vries, Cor, Herder, Jan-Willem den, DiPirro, Michael, Done, Chris, Dotani, Tadayasu, Ebisawa, Ken, Enoto, Teruaki, Ezoe, Yuichiro, Fabian, Andrew, Fujimoto, Ryuichi, Fukazawa, Yasushi, Funk, Stefan, Furuzawa, Akihiro, Galeazzi, Massimiliano, Gandhi, Poshak, Gendreau, Keith, Gilmore, Kirk, Haba, Yoshito, Hamaguchi, Kenji, Hatsukade, Isamu, Hayashida, Kiyoshi, Hiraga, Junko, Hirose, Kazuyuki, Hornschemeier, Ann, Hughes, John, Hwang, Una, Iizuka, Ryo, Ishibashi, Kazunori, Ishida, Manabu, Ishimura, Kosei, Ishisaki, Yoshitaka, Isobe, Naoki, Ito, Masayuki, Iwata, Naoko, Kaastra, Jelle, Kallman, Timothy, Kamae, Tuneyoshi, Katagiri, Hideaki, Kataoka, Jun, Katsuda, Satoru, Kawaharada, Madoka, Kawai, Nobuyuki, Kawasaki, Shigeo, Khangaluyan, Dmitry, Kilbourne, Caroline, Kinugasa, Kenzo, Kitamoto, Shunji, Kitayama, Tetsu, Kohmura, Takayoshi, Kokubun, Motohide, Kosaka, Tatsuro, Kotani, Taro, Koyama, Katsuji, Kubota, Aya, Kunieda, Hideyo, Laurent, Philippe, Lebrun, Francois, Limousin, Olivier, Loewenstein, Michael, Long, Knox, Madejski, Grzegorz, Maeda, Yoshitomo, Makishima, Kazuo, Markevitch, Maxim, Matsumoto, Hironori, Matsushita, Kyoko, McCammon, Dan, Miller, Jon, Mineshige, Shin, Minesugi, Kenji, Miyazawa, Takuya, Mizuno, Tsunefumi, Mori, Koji, Mori, Hideyuki, Mukai, Koji, Murakami, Hiroshi, Murakami, Toshio, Mushotzky, Richard, Nakagawa, Yujin, Nakagawa, Takao, Nakajima, Hiroshi, Nakamori, Takeshi, Nakazawa, Kazuhiro, Namba, Yoshiharu, Nomachi, Masaharu, Dell, Steve O', Ogawa, Hiroyuki, Ogawa, Mina, Ogi, Keiji, Ohashi, Takaya, Ohno, Masanori, Ohta, Masayuki, Okajima, Takashi, Ota, Naomi, Ozaki, Masanobu, Paerels, Frits, Paltani, Stéphane, Parmer, Arvind, Petre, Robert, Pohl, Martin, Porter, Scott, Ramsey, Brian, Reynolds, Christopher, Sakai, Shin-ichiro, Sambruna, Rita, Sato, Goro, Sato, Yoichi, Serlemitsos, Peter, Shida, Maki, Shimada, Takanobu, Shinozaki, Keisuke, Shirron, Peter, Smith, Randall, Sneiderman, Gary, Soong, Yang, Stawarz, Lukasz, Sugita, Hiroyuki, Szymkowiak, Andrew, Tajima, Hiroyasu, Takahashi, Hiromitsu, Takei, Yoh, Tamagawa, Toru, Tamura, Takayuki, Tamura, Keisuke, Tanaka, Takaaki, Tanaka, Yasuo, Tanaka, Yasuyuki, Tashiro, Makoto, Tawara, Yuzuru, Terada, Yukikatsu, Terashima, Yuichi, Tombesi, Francesco, Tomida, Hiroshi, Tozuka, Miyako, Tsuboi, Yoko, Tsujimoto, Masahiro, Tsunemi, Hiroshi, Tsuru, Takeshi, Uchida, Hiroyuki, Uchiyama, Yasunobu, Uchiyama, Hideki, Ueda, Yoshihiro, Uno, Shinichiro, Urry, Meg, Watanabe, Shin, White, Nicholas, Yamada, Takahiro, Yamaguchi, Hiroya, Yamaoka, Kazutaka, Yamasaki, Noriko, Yamauchi, Makoto, Yamauchi, Shigeo, Yatsu, Yoichi, Yonetoku, Daisuke, Yoshida, Atsumasa |
Rok vydání: |
2010 |
Předmět: |
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Zdroj: |
Proceedings of the SPIE, Volume 7732, pp. 77320Z-77320Z-18 (2010) |
Druh dokumentu: |
Working Paper |
DOI: |
10.1117/12.857875 |
Popis: |
The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions initiated by the Institute of Space and Astronautical Science (ISAS). ASTRO-H will investigate the physics of the high-energy universe by performing high-resolution, high-throughput spectroscopy with moderate angular resolution. ASTRO-H covers very wide energy range from 0.3 keV to 600 keV. ASTRO-H allows a combination of wide band X-ray spectroscopy (5-80 keV) provided by multilayer coating, focusing hard X-ray mirrors and hard X-ray imaging detectors, and high energy-resolution soft X-ray spectroscopy (0.3-12 keV) provided by thin-foil X-ray optics and a micro-calorimeter array. The mission will also carry an X-ray CCD camera as a focal plane detector for a soft X-ray telescope (0.4-12 keV) and a non-focusing soft gamma-ray detector (40-600 keV) . The micro-calorimeter system is developed by an international collaboration led by ISAS/JAXA and NASA. The simultaneous broad bandpass, coupled with high spectral resolution of Delta E ~7 eV provided by the micro-calorimeter will enable a wide variety of important science themes to be pursued. Comment: 18 pages, 12 figures, Proceedings of the SPIE Astronomical Instrumentation "Space Telescopes and Instrumentation 2010: Ultraviolet to Gamma Ray" |
Databáze: |
arXiv |
Externí odkaz: |
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