Performance evaluation of the high-voltage CMOS active pixel sensor AstroPix for gamma-ray space telescopes

Yusuke Suda, Regina Caputo, Amanda L. Steinhebel, Nicolas Striebig, Manoj Jadhav, Yasushi Fukazawa, Masaki Hashizume, Carolyn Kierans, Richard Leys, Jessica Metcalfe, Michela Negro, Ivan Perić, Jeremy S. Perkins, Taylor Shin, Hiroyasu Tajima, Daniel Violette, Norito Nakano

Research output: Contribution to journalReview articlepeer-review

1 Scopus citations

Abstract

AstroPix is a novel monolithic high-voltage CMOS active pixel sensor proposed for next generation medium-energy gamma-ray observatories like the All-sky Medium Energy Gamma-ray Observatory eXplorer (AMEGO-X). For AMEGO-X AstroPix must maintain a power consumption of less than 1.5mW/cm2 while having a pixel pitch of up to 500μm. We developed the second and third versions of AstroPix, namely AstroPix2 and AstroPix3. AstroPix2 and AstroPix3 exhibit power consumptions of 3.4mW/cm2 and 4.1mW/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.

Funding

The authors gratefully acknowledge financial support from NASA ( 18-APRA18-0084 ). This work was supported by JSPS KAKENHI Grant Numbers JP23K13127 and JP23H04897 . We would like to thank staff in the radiation facility of the School of Engineering, Hiroshima University, for granting us access to their high-intensity facility. The authors would like to thank the anonymous journal referees for their feedback, which helped to improve the quality of this paper.

Keywords

  • HV-CMOS active pixel sensor
  • High energy astrophysics
  • MAPS
  • MeV gamma-ray telescope

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