A Silicon-on-Insulator-Based Dual-Gain Charge-Sensitive Pixel Detector for Low-Noise X-ray Imaging for Future Astronomical Satellite Missions

被引:5
|
作者
Shrestha, Sumeet [1 ]
Kawahito, Shoji [1 ]
Kamehama, Hiroki [2 ]
Nakanishi, Syunta [1 ]
Yasutomi, Keita [1 ]
Kagawa, Keiichiro [1 ]
Teranishi, Nobukazu [1 ]
Takeda, Ayaki [3 ]
Tsuru, Takeshi Go [4 ]
Kurachi, Ikuo [5 ]
Arai, Yasuo [5 ]
机构
[1] Shizuoka Univ, Elect Res Inst, Hamamatsu, Shizuoka 4328011, Japan
[2] Okinawa Coll, Natl Inst Technol, Informat & Commun Syst Engn, Nago, Okinawa 9052171, Japan
[3] Univ Miyazaki, Dept Appl Phys & Elect Engn, Miyazaki 8892192, Japan
[4] Kyoto Univ, Dept Phys, Kyoto 6068502, Japan
[5] High Energy Accelerator Res Org, Tsukuba, Ibaraki 3050801, Japan
基金
日本学术振兴会;
关键词
active pixel sensor; charge sensitive amplifier; dual gain; high energy astrophysics; SOI pixel; spectroscopic performance; X-ray detector; TECHNOLOGY;
D O I
10.3390/s18061789
中图分类号
O65 [分析化学];
学科分类号
070302 ; 081704 ;
摘要
In this paper, we report on the development of a monolithic active pixel sensor for X-ray imaging using 0.2 mu m fully depleted silicon-on-insulator (SOI)-based technology to support next generation astronomical satellite missions. Detail regarding low-noise dual-gain SOI based pixels with a charge sensitive amplifier and pinned depleted diode sensor structure is presented. The proposed multi-well sensor structure underneath the fully-depleted SOI allows the design of a detector with low node capacitance and high charge collection efficiency. Configurations for achieving very high charge-to-voltage conversion gain of 52 mu V/e(-) and 187 mu V/e(-) are demonstrated. Furthermore, in-pixel dual gain selection is used for low-noise and wide dynamic range X-ray energy detection. A technique to improve the noise performance by removing correlated system noise leads to an improvement in the spectroscopic performance of the measured X-ray energy. Taken together, the implemented chip has low dark current (44.8 pA/cm(2) at -30 degrees C), improved noise performance (8.5 e(-) rms for high gain and 11.7 e(-) rms for low gain), and better energy resolution of 2.89% (171 eV FWHM) at 5.9 keV using Fe-55 and 1.67% (234 eV FWHM) at 13.95 keV using Am-241.
引用
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页数:19
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