Current status of hard x-ray characterization of ASTRO-H HXT at SPring-8

被引:8
|
作者
Miyazawa, Takuya [1 ]
Furuzawa, Akihiro [1 ]
Kanou, Yasufumi [1 ]
Matsuda, Kenji [1 ]
Sakai, Michito [1 ]
Yamane, Nobuyuki [1 ]
Ishida, Yousuke [1 ]
Hara, Shinji [1 ]
Miyata, Yusuke [1 ]
Sakanobe, Karin [1 ]
Haba, Yoshito [1 ]
Matsumoto, Hironori [1 ]
Tawara, Yuzuru [1 ]
Kunieda, Hideyo [1 ]
Mori, Hideyuki [1 ]
Tamura, Keisuke [1 ]
Maeda, Yoshitomo [1 ]
Ishida, Manabu [1 ]
Awaki, Hisamitsu [1 ]
Okajima, Takashi [1 ]
Uesugi, Kentaro [1 ]
Suzuki, Yoshio [1 ]
Ishida, Naoki [1 ]
Ohtsu, Nobuhiro [1 ]
Suzuki, Akio [1 ]
Ogasaka, Yasushi [1 ]
Yamashita, Koujun [1 ]
机构
[1] Nagoya Univ, Chikusa Ku, Furo Cho, Aichi 4648602, Japan
关键词
hard x-ray telescope; multilayer optics; synchrotron facility; ASTRO-H; TELESCOPE;
D O I
10.1117/12.857421
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the current status of hard X-ray telescope developments of ASTRO-H. ASTRO-H is Japan's 6th Xray satellite mission following to Suzaku. It will be launched in 2014. The HXT onboard ASTRO-H is thin-foil, multi-nested conical optics as well as Suzaku XRT. To reflect hard X-rays efficiently, reflector surfaces are coated with depth-graded Pt/C multilayer. Reflectors are fabricated by the epoxy-replication method. Currently, we have finished the preparation of mirror production facility at Nagoya University, and started test production of reflectors for HXT. The selected 22 pairs of multilayer reflectors have been characterized at the SPring-8 beamline BL20B2.
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页数:8
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