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Peer-reviewed

Alignment performance of scientific instruments mounted on ASTRO-H (Hitomi).

Kosei Ishimura, M. Ishida, Taro Kawano, Ryo Iizuka, Kuniyuki Omagari, K. Abe, Kenji Minesugi, Kazunori SHOJI, Akira KITO, Takayuki Hayashi, Kazuro Matsumoto, Kiyotaka TACHIKAWA, Takayuki Yuasa, Masaaki Tsushima, Hiroyuki Kajiura, S. Ueno, M Ikeda, Osamu Maeda, Naoko Iwata, T. Sasaki, Takahiro Yumoto, Daisuke Nakayama, Yukari Ono, Jun Kurihara, Takahito AMANUMA, Yuhei HAYASAKA, Mitsuhisa Baba, Tsunefumi Mizuno, Shin Watanabe, Kazuhiro Nakazawa, Ken Goto, Atsushi Wada, Chikara Natsukari, Tadayuki Takahashi

Supēsu, Enjiniaringu, Konfarensu kōen rombunshū/Supesu, Enjiniaringu, Konfarensu koen ronbunshu · 2016

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Summary

ASTRO-H (hitomi) was an X-ray astronomy satellite in Japan which was launched on 17 Feb. 2016. To meet its science goals, four kinds of instruments and six detectors were equipped on the satellite. The focal length of two soft X-ray telescopes was 5.6 m, and that of two hard X-ray telescopes is 12m. One of the most difficult challenges for the satellite structure was to meet the alignment requirements for instruments and detectors. Through the ground tests and observation results on orbit, it was confirmed that the performance of alignment meet the requirements. In this paper, the results of on-orbit alignment performance of the instruments and obtained techniques to control the alignment are reported.

Source type
Peer-reviewed study
DOI
10.1299/jsmesec.2016.25.1a6
Catalogue ID
SNmoic29yz-0moxw3
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