Development of a 32-channel ASIC for an X-ray APD detector onboard the ISS

被引:2
|
作者
Arimoto, Makoto [1 ,2 ]
Harita, Shohei [2 ]
Sugita, Satoshi [2 ]
Yatsu, Yoichi [2 ]
Kawai, Nobuyuki [2 ]
Ikeda, Hirokazu [3 ]
Tomida, Hiroshi [3 ]
Isobe, Naoki [3 ]
Ueno, Shiro [4 ]
Mihara, Tatehiro [5 ]
Serino, Motoko [5 ]
Kohmura, Takayoshi [6 ]
Sakamoto, Takanori [7 ]
Yoshida, Atsumasa [7 ]
Tsunemi, Hiroshi [8 ]
Hatori, Satoshi [9 ]
Kume, Kyo [9 ]
Hasegawa, Takashi [9 ]
机构
[1] Waseda Univ, Res Inst Sci & Engn, Shinjuku Ku, 3-4-1 Ohkubo, Tokyo 1698555, Japan
[2] Tokyo Inst Technol, Meguro Ku, 2-12-1 Ookayama, Tokyo 1528550, Japan
[3] ISAS, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2298510, Japan
[4] Japan Aerosp Explorat Agcy JAXA, ISAS, ISS Sci Project Off, 2-1-1 Sengen, Tsukuba, Ibaraki 3058505, Japan
[5] RIKEN, MAXI Team, 2-1 Hirosawa, Wako, Saitama 3510198, Japan
[6] Tokyo Univ Sci, Dept Phys, 2641 Yamazaki, Noda, Chiba 2788510, Japan
[7] Aoyama Gakuin Univ, Dept Phys & Math, Coll Sci & Engn, Chuo Ku, 5-10-1 Fuchinobe, Sagamihara, Kanagawa 2525258, Japan
[8] Osaka Univ, Dept Earth & Space Sci, 1-1 Machikaneyama Cho, Toyonaka, Osaka 5600043, Japan
[9] Wakasa Wan Energy Res Ctr, 64-52-1 Nagatani, Tsuruga, Fukui 9140192, Japan
关键词
ASIC; Low-noise; X-rays; APD; Radiation tolerance;
D O I
10.1016/j.nima.2017.09.003
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
We report on the design and performance of a mixed-signal application specific integrated circuit (ASIC) dedicated to avalanche photodiodes (APDs) in order to detect hard X-ray emissions in a wide energy band onboard the International Space Station. To realize wide-band detection from 20 keV to 1 MeV, we use Ce:GAGG scintillators, each coupled to an APD, with low-noise front-end electronics capable of achieving a minimum energy detection threshold of 20 keV. The developed ASIC has the ability to read out 32-channel APD signals using 0.35 mu m CMOS technology, and an analog amplifier at the input stage is designed to suppress the capacitive noise primarily arising from the large detector capacitance of the APDs. The ASIC achieves a performance of 2099 e(-) + 1.5 e(-) /pF at root mean square (RMS) with a wide 300 fC dynamic range. Coupling a reverse-type APD with a Ce:GAGG scintillator, we obtain an energy resolution of 6.7% (FWHM) at 662 keV and a minimum detectable energy of 20 keV at room temperature (20 degrees C). Furthermore, we examine the radiation tolerance for space applications by using a 90 MeV proton beam, confirming that the ASIC is free of single-event effects and can operate properly without serious degradation in analog and digital processing. (C) 2017 Elsevier B.V. All rights reserved.
引用
收藏
页码:138 / 147
页数:10
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