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M ay 2 01 8 In-Orbit Performance and Calibration of the Hard X-ray Imager ( HXI ) onboard Hitomi ( ASTRO-H )

Kouichi Hagino,Kazuhiro Nakazawa,Goro Sato,Motohide Kokubun,Teruaki Enoto,Yasushi Fukazawa,Katsuhiro Hayashi,Jun Kataoka,Junichiro Katsuta,Shogo B. Kobayashi,Philippe Laurent,Francois Lebrun,Olivier Limousin,Daniel Maier,Kazuo Makishima, Taketo Mimura,Katsuma Miyake,Tsunefumi Mizuno,Kunishiro Mori,Hiroaki Murakami,Takeshi Nakamori,Toshio Nakano,Hirofumi Noda,Hirokazu Odaka,Masanori Ohno,Masayuki Ohta,Shinya Saito,Rie Sato,Hiroyasu Tajima,Hiromitsu Takahashi,Tadayuki Takahashi,Shin’ichiro Takeda,Takaaki Tanaka,Yukikatsu Terada,Hideki Uchiyama,Yasunobu Uchiyama,Shin Watanabe,Kazutaka Yamaoka,Yoichi Yatsu,Takayuki Yuasa

semanticscholar（2018）

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Abstract
The Hard X-ray Imager (HXI) onboard Hitomi (ASTRO-H) is an imaging spectrometer covering hard Xray energies of 5–80 keV. Combined with the hard X-ray telescope, it enables imaging spectroscopy with an angular resolution of 1.7 half-power diameter, in a field of view of 9 × 9. The main imager is composed of 4 layers of
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