Performance evaluation of the high-voltage CMOS active pixel sensor AstroPix for gamma-ray space telescopes
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment Volume 1068
Page 169762-
published_at 2024-08-22
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Title ( eng ) |
Performance evaluation of the high-voltage CMOS active pixel sensor AstroPix for gamma-ray space telescopes
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Creator |
Caputo Regina
Steinhebel Amanda L.
Striebig Nicolas
Jadhav Manoj
Hashizume Masaki
Kierans Carolyn
Leys Richard
Metcalfe Jessica
Negro Michela
Perić Ivan
Perkins Jeremy S.
Shin Taylor
Tajima Hiroyasu
Violette Daniel
Nakano Norito
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Source Title |
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Volume | 1068 |
Start Page | 169762 |
Abstract |
AstroPix is a novel monolithic high-voltage CMOS active pixel sensor proposed for next generation mediumenergy gamma-ray observatories like the All-sky Medium Energy Gamma-ray Observatory eXplorer (AMEGOX). For AMEGO-X AstroPix must maintain a power consumption of less than 1.5 mW / cm2 while having a pixel pitch of up to 500 μm. We developed the second and third versions of AstroPix, namely AstroPix2 and AstroPix3. AstroPix2 and AstroPix3 exhibit power consumptions of 3.4 mW ∕ cm2 and 4.1 mW ∕ cm2, respectively. While AstroPix2 has a pixel pitch of 250 μm, AstroPix3 achieves the desired size for AMEGO-X with a pixel pitch of 500 μm. Performance evaluation of a single pixel in an AstroPix2 chip revealed a dynamic range from 13.9 keV to 59.5 keV, with the energy resolution meeting the AMEGO-X target value (< 10% (FWHM) at 60 keV). We performed energy calibration on most of the pixels in an AstroPix3 chip, yielding a mean energy resolution of 6.2 keV (FWHM) at 59.5 keV, with 44.4% of the pixels satisfying the target value. The dynamic range of AstroPix3 was assessed to span from 22.2 keV to 122.1 keV. The expansion of the depletion layer aligns with expectations in both AstroPix2 and AstroPix3. Furthermore, radiation tolerance testing was conducted on AstroPix. An AstroPix2 chip was subjected to an equivalent exposure of approximately 10 Gy from a high-intensity 60Co source. The chip was fully operational after irradiation although a decrease in gain by approximately 4% was observed.
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Keywords |
High energy astrophysics
MeV gamma-ray telescope
HV-CMOS active pixel sensor
MAPS
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Descriptions |
The authors gratefully acknowledge financial support from NASA, USA (18-APRA18-0084).
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Language |
eng
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Resource Type | journal article |
Publisher |
Elsevier
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Date of Issued | 2024-08-22 |
Rights |
© 2024. This manuscript version is made available under the CC-BY-NC-ND 4.0 license https://creativecommons.org/licenses/by-nc-nd/4.0/
This is not the published version. Please cite only the published version.
この論文は出版社版ではありません。引用の際には出版社版をご確認、ご利用ください。
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Publish Type | Accepted Manuscript |
Access Rights | embargoed access |
Source Identifier |
[DOI] https://doi.org/10.1016/j.nima.2024.169762
isVersionOf
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助成機関名 |
日本学術振興会
Japan Society for the Promotion of Science
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助成機関識別子 |
[Crossref Funder] https://doi.org/10.13039/501100001691
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研究課題名 |
ガンマ線バーストにおけるTeVガンマ線放射機構の解明
Study of TeV gamma-ray emission mechanisms of Gamma-Ray Bursts
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研究課題番号 |
23K13127
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助成機関名 |
日本学術振興会
Japan Society for the Promotion of Science
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助成機関識別子 |
[Crossref Funder] https://doi.org/10.13039/501100001691
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研究課題名 |
多粒子宇宙観測技術の開発による新たな「眼」の獲得
Acquisition of new "eyes" by developing multimessenger observation technologies
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研究課題番号 |
23H04897
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Remark | The full-text file will be made open to the public on 22 August 2026 in accordance with publisher's 'Terms and Conditions for Self-Archiving' |