Ray-tracing simulation and in-orbit performance of the ASTRO-H hard x-ray telescope (HXT)

Autor: Satoshi Sugita, Kazunori Ishibashi, Ryo Iizuka, Tatsuro Kosaka, Yoshitomo Maeda, Yutaka Suzuki, Yoshito Haba, Hisamitsu Awaki, Housei Nagano, Masayuki Itoh, K. Uesugi, Yoshiharu Namba, Takuya Miyazawa, Hideyuki Mori, Hideyo Kunieda, Keisuke Tamura, Y. Ogasaka, Shigeo Yamauchi, Yuzuru Tawara, Ikuyuki Mitsuishi, Keiji Ogi, Manabu Ishida, Takayuki Hayashi, Takashi Okajima, Akihiro Furuzawa, Hironori Matsumoto

Publikováno v: SPIE Proceedings.

A ray-trace simulation code for the Hard X-ray Telescope (HXT) on board the Hitomi (ASTRO-H) satellite is being developed. The half power diameter and effective area simulated based on the code are consistent with ground measurements within 10%. The

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::cd4074417c9fc7caa91dde6da07a26c0
https://doi.org/10.1117/12.2232135

ASCA Observations of Luminous Infrared Galaxies: Evolution from Starburst to AGN?

Autor: Takao Nakagawa, Hajime Inoue, R. Fujimoto, Keith Arnaud, Tsuneo Kii, Ryohei Kawabe, Toshiyuki Miyazaki, Y. Ogasaka

Publikováno v: Symposium - International Astronomical Union. 186:341-344

One of the most important results of the IRAS survey is the discovery of a class of “Luminous Infrared Galaxies” (LIGs), which emit most of the energy in the infrared and are the dominant population in the local universe at luminosities above 101

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::38315511a51cc3b3ca4204f456d5f539
https://doi.org/10.1017/s0074180900112938

ASCA Sky Survey Observations and the Cosmic X-Ray Background in 2-10 KeV

Autor: H. Inoue, T. Takahashi, Y. Ueda, A. Yamashita, Y. Ishisaki, Y. Ogasaka

Publikováno v: Symposium - International Astronomical Union. 188:197-200

The X-ray background in the energy range above 2 keV is highly uniform except for an excess component along the Galactic plane. The excess along the plane is considered to be associated with our Galaxy, whereas the rest of the emission is believed to

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::7857a9ce6751da40e19a0aa35b382c4a
https://doi.org/10.1017/s0074180900114755

The NeXT Mission

Autor: Y. Ogasaka, Hiroshi Tsunemi, Kiyoshi Hayashida, H. Tajima, Kazuhisa Mitsuda, G. M. Madejski, Ryuichi Fujimoto, Shin Watanabe, Yukikatsu Terada, Kazuo Makishima, Katsuji Koyama, Motohide Kokubun, Kazuhiro Nakazawa, Takeshi Go Tsuru, K. Mori, Y. Ishisaki, Yoshihiro Ueda, Yasushi Fukazawa, N. E. White, M. Ozaki, Manabu Ishida, Robert Petre, Tadayasu Dotani, R. F. Mushotzky, Tadayuki Takahashi, Makoto Tashiro, Takaya Ohashi, Hideyo Kunieda, Noriko Y. Yamasaki, NeXT team, R. L. Kelley

Publikováno v: Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray.

The NeXT (New exploration X-ray Telescope), the new Japanese X-ray Astronomy Satellite following Suzaku, is an international X-ray mission which is currently planed for launch in 2013. NeXT is a combination of wide band X-ray spectroscopy (3 - 80 keV

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e68dc1c9ce28a231b096d32d618cb89e
https://doi.org/10.1117/12.789640

In-flight status of the X-ray observatory Suzaku

Autor: Hideaki Katagiri, Ryo Shibata, Naomi Ota, T. Mihara, Mitsuhiro Kohama, J. A. Nousek, Yukikatsu Terada, T. Furusho, T. Kotani, Kazuo Makishima, Kazutami Misaki, Tadayuki Takahashi, Motoko Suzuki, Chiho Matsumoto, A. E. Szymkowiak, D. McCammon, I. M. Harrus, Ikuya Sakurai, T. Tamagawa, Y. Uchiyama, Martin J. L. Turner, J. Hiraga, Makoto Tashiro, F. Makino, Hideyuki Mori, Naohisa Anabuki, Y. Ishisaki, N. Yamamoto, Hironori Matsumoto, Koji Mori, Günther Hasinger, Una Hwang, R. Smith, James Reeves, Shinichiro Uno, Kazutaka Yamaoka, Hitoshi Negoro, Isamu Hatsukade, Toshio Murakami, Wilton T. Sanders, John P. Hughes, Daisuke Yonetoku, Yuichiro Ezoe, Shiro Ueno, Shigeo Yamauchi, Keith C. Gendreau, Yuzuru Tawara, Lorella Angelini, Marshall W. Bautz, T. Kamae, Kazuhisa Mitsuda, Yasushi Fukazawa, Alex Markowitz, Kenzo Kinugasa, Takashi Okajima, Caroline A. Kilbourne, H. Tomida, John P. Doty, A. C. Fabian, Kai Wing Chan, Hiroshi Murakami, M. Matsuoka, A. N. Parmar, Tahir Yaqoob, J. Kotoku, Y. Tsuboi, N. Isobe, K. Hamaguchi, Atsumasa Yoshida, M. Ueno, Aya Kubota, Takayuki Tamura, K. Ebisawa, Yang Soong, Y. Urata, Richard E. Griffiths, K. Mukai, K. R. Boyce, Akihiro Furuzawa, Koji Nakazawa, Shunji Kitamoto, H. Moseley, N. E. White, Y. Ogawara, Gregory V. Brown, H. Ozawa, F. Scott Porter, Y. Ogasaka, Yasuyuki T. Tanaka, Fumiaki Nagase, M. Namiki, Ann Hornschemeier, E. Figueroa, Takayoshi Kohmura, Masayuki Itoh, R. L. Kelley, Ryuichi Fujimoto, W. D. Pence, Robert Petre, Manabu Ishida, H. Tsunemi, T. Oshima, Mikio Morii, Keisuke Tamura, Yuichi Terashima, Kiyoshi Hayashida, Patrick Henry, Takaya Ohashi, Hideyo Kunieda, P. J. Serlemitsos, Noriko Y. Yamasaki, R. F. Mushotzky, Yoshitomo Maeda, Tsunefumi Mizuno, Madoka Kawaharada, Hisamitsu Awaki, Kazuya Koyama, Emi Miyata, Koujun Yamashita, Aya Bamba, K. Matsushita, Yoh Takei, Yoshito Haba, Jun Kataoka, Shin Watanabe, K. A. Arnaud, Y. Tsujimoto, Ken'ichi Torii, M. Ozaki, N. Iyomoto, George R. Ricker, Hajime Inoue, G. M. Madejski, Takeshi Go Tsuru, Atsushi Senda, N. Kawai, Motohide Kokubun, Steven E. Kissel, Haruyoshi Katayama, Yoshihiro Ueda, Makoto Yamauchi, Hiromitsu Takahashi, Tadayasu Dotani, S. M. Kahn, Jean Cottam, S. S. Holt, Keisuke Shinozaki

Publikováno v: 2007 IEEE Nuclear Science Symposium Conference Record.

We report in-flight status of the X-ray detectors on board the Suzaku observatory, the 5th X-ray astronomy satellite of Japan launched on July 10, 2005. Suzaku is equipped with two types of instruments: one is the X-ray imaging spectrometers (XISs) a

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::26f35ff5bddd7414f8f88112e7ae4e37
https://doi.org/10.1109/nssmic.2007.4436667