Zobrazeno 1 - 10
of 127
pro vyhledávání: '"J. Hiraga"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Aya Bamba, Tadayasu Dotani, K. Mori, Yukikatsu Terada, H. Matsumoto, S. Kimura, Takahisa Fujinaga, Hideki Uchiyama, Masanobu Ozaki, G. Pühlhofer, K. Matsuta, J. Hiraga
Publikováno v:
Proceedings of the International Symposium “Nanoscience and Quantum Physics 2012” (nanoPHYS’12).
T. Fujinaga1,2, K. Mori3, A. Bamba4 S. Kimura3, T. Dotani2,1,5, M. Ozaki2, K. Matsuta5,2, G. Puhlhofer6, H. Uchiyama7, J. S. Hiraga7, H. Matsumoto8 and Y. Terada9 1 Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8550, Japan 2 In
Autor:
Hiroshi Murakami, Masaki Sasano, Koji Nakazawa, Kazuo Makishima, Teruaki Enoto, J. Hiraga, Soki Sakurai, Toshio Nakano
Publikováno v:
Physical Review Letters. 112
Magnetars are a special type of neutron stars, considered to have extreme dipole magnetic fields reaching ~1e+11 T. The magnetar 4U 0142+61, one of prototypes of this class, was studied in broadband X-rays (0.5-70 keV) with the Suzaku observatory. In
Autor:
Kenta Kaneko, Tadayasu Dotani, M. Ozaki, Kiyoshi Hayashida, Takayoshi Kohmura, Tatsuo Watanabe, H. Tsunemi, Hiroshi Nakajima, K. Matsuta, Takahisa Fujinaga, Astro-H Team, Koji Mori, Shunji Kitamoto, Takeshi Go Tsuru, J. Hiraga, Shoma Ikeda, Naohisa Anabuki, Hiroshi Murakami, Shutaro Ueda, Kohei Kawai
Publikováno v:
AIP Conference Proceedings.
We have newly developed the back-illuminated (BI)-CCD which has an Optical Blocking Layer (OBL) directly coating its X-ray illumination surface with Aluminum-Polyimide-Aluminum instead of Optical Blocking Filter (OBF). OBL is composed of a thin polyi
Autor:
M. Ozaki, Takahisa Fujinaga, Takayoshi Kohmura, H. Tsunemi, K. Matsuta, J. Hiraga, Kohei Kawai, Tadayasu Dotani, Naohisa Anabuki, Kiyoshi Hayashida, Koji Mori, Takeshi Go Tsuru, Hiroshi Murakami, Shoma Ikeda, Astro-H Team, Hiroshi Nakajima, Tatsuo Watanabe, Shutaro Ueda, Shunji Kitamoto, Kenta Kaneko
Publikováno v:
AIP Conference Proceedings.
We have developed the back-illuminated X-ray CCD camera (BI-CCD) to observe Xray in space. The X-ray CCD has a sensitivity not only for in X-ray but also in both Optical and UV light, X-ray CCD has to equip a filter to cut off optical light as well a
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
Autor:
Toshio Nakano, Hideki Uchiyama, Teruaki Enoto, J. Hiraga, Hiroaki Murakami, Hidehiro Kaneda, Kazuo Makishima
Publikováno v:
Publications of the Astronomical Society of Japan. 67:9-9
Ages of the magnetar 1E 2259+586 and the associated supernova remnant CTB~109 were studied. Analyzing the Suzaku data of CTB~109, its age was estimated to be $\sim$14~kyr, which is much shorter than the measured characteristic age of 1E 2259+586, 230
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.