M Tashiro, T Kamae, K Makishima, T Takahashi, T Murakami, Y Fukazawa, M Kokubun, K Nakazawa, M Nomachi, A Yoshida, Y Ezoe, N Isobe, N Iyomoto, J Kataoka, J Kotoku, M Kouda, S Kubo, A Kubota, Y Matsumoto, T Mizuno, GM Madejski, Y Okada, N Ota, H Ozawa, G Sato, M Sugiho, M Sugizaki, Takahashi, I, H Takahashi, T Tamura, C Tanihata, Y Terada, Y Uchiyama, S Watanabe, K Yamaoka, D Yonetoku
IEEE TRANSACTIONS ON NUCLEAR SCIENCE, 49(4) 1893-1897, Aug, 2002
This paper summarizes the design and performance of the hard X-ray detector constructed for the ASTRO-E satellite. The detector utilizes the GSO/BGO well-type phoswich counters in a compound-eye configuration to achieve an extremely low background level of a few x 10(-5) counts s(-1) cm(-2)keV(-1) [1]. The GSO scintillators installed in the BGO active shield wells are sensitive to 30-600 keV photons, while the 2-mm-thick silicon PIN diodes, placed in front of each GSO crystal, cover the 10-60 keV energy band with a spectral resolution of similar to3.5-keV full-width at half-maximum. The design goals, of both low background and high energy resolution, in the hard X-ray bands were verified through the preflight calibration experiments.