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Performance verification of next-generation Si CMOS soft X-ray detector for space applications.

Authors :
Ogino, Naoki
Arimoto, Makoto
Sawano, Tatsuya
Yonetoku, Daisuke
Yu, Pang
Watanabe, Shota
Hiraga, Junko S.
Yuhi, Daito
Hatori, Satoshi
Kume, Kyo
Hasegawa, Takashi
Source :
Nuclear Instruments & Methods in Physics Research Section A. Jan2021, Vol. 987, pN.PAG-N.PAG. 1p.
Publication Year :
2021

Abstract

All-sky surveys of X-ray transient objects in the soft X-ray band are essential for observing high-redshift events to probe unexplored physical conditions in the early universe and discovering mysterious electromagnetic counterparts of gravitational-wave sources. HiZ-GUNDAM is a future satellite mission that intends to perform a wide-field survey in the soft X-ray band (0.4–4 keV). The HiZ-GUNDAM X-ray detector has Si pixel sensors that require fine positioning accuracy (e.g. tens of micrometers), high detection efficiency, a large detection area (tens of cm 2) and, a relatively high frame rate of ∼ 10 frames per second that can be achieved by a back-illuminated Si CMOS image sensor. One of the most promising candidates is GSENSE6060BSI with 6144 × 6144 pixels fabricated by Gpixel Inc. In this paper, for the initial performance test, we used a smaller-sized CMOS sensor, GSENSE400BSI-TVISB, which is similar to GSENSE6060BSI in terms of pixel characteristics, such as pixel size, epilayer thickness, and resistivity, except for the number of pixels (2048 × 2048). We conducted a detailed study on the spectroscopic performance of GSENSE400BSI-TVISB in the soft X-ray band and its radiation tolerance for space applications. For the spectroscopic performance, low-energy X-ray lines such as Al-K α (1.5 keV), Mn-K α (5.9 keV), and Mn-K β (6.5 keV) were clearly detected. Furthermore, using the obtained X-ray events, we estimated > 50% detection efficiency in the 0.4–4 keV band, corresponding to a ∼ 10- μ m Si thickness of the detectable layer. We also performed radiation tolerance tests against gamma rays from 60Co, 100-MeV protons and 5.5-MeV alpha rays (5–30 krad, corresponding to 6–30 year operation in orbit). After the irradiation tests, we observed that GSENSE400BSI-TVISB has strong radiation tolerance for our purpose: the lower detectable energy of ∼ 0.4 keV can be obtained if the CMOS is operated with an exposure of 0.1 s at − 20 °C. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
01689002
Volume :
987
Database :
Academic Search Index
Journal :
Nuclear Instruments & Methods in Physics Research Section A
Publication Type :
Academic Journal
Accession number :
147342030
Full Text :
https://doi.org/10.1016/j.nima.2020.164843