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Astrophysics > Instrumentation and Methods for Astrophysics

arXiv:2507.21618 (astro-ph)
[Submitted on 29 Jul 2025]

Title:Evaluation of gamma-ray response of the AstroPix4 HV-CMOS active pixel sensor

Authors:Yusuke Suda, Regina Caputo, Daniel Violette, Grant Sommer, Nicolas Striebig, Manoj Jadhav, Yasushi Fukazawa, Carolyn Kierans, Richard Leys, Jessica Metcalfe, Norito Nakano, Ivan Perić, Jeremy S. Perkins, Hiroyasu Tajima
View a PDF of the paper titled Evaluation of gamma-ray response of the AstroPix4 HV-CMOS active pixel sensor, by Yusuke Suda and 13 other authors
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Abstract:AstroPix is a novel high-voltage CMOS active pixel sensor being developed for a next generation gamma-ray space telescope, AMEGO-X. To meet AMEGO-X instrument requirements, AstroPix must achieve full depletion of its $500~\rm{\mu m}$ thick, $500~\rm{\mu m}$-pitch pixels. It must be sensitive to gamma rays in the range of $25-700$ keV, with the energy resolution at 122 keV of $<10$%. Furthermore, given the space-based nature of AMEGO-X, the power consumption of AstroPix needs to be lower than $1.5~\rm{mW/{cm}^2}$. We report the gamma-ray response of the latest version of AstroPix, AstroPix4. The chip contains $16\times 13$ array of $500~\rm{\mu m}$-pitch pixels. The power consumption is estimated to be about $2~\rm{mW/{cm}^2}$, which is approximately half the power of the previous AstroPix version. The input capacitance is reduced, allowing for the detection of the 14 keV photopeak from $\rm{^{57}Co}$ and a moderate energy resolution of 14% at 122 keV. The dynamic range is estimated to be in the range from 14 keV to $\sim250$ keV. We found that the sensor depletion layer expands as expected and the measured depletion depth is approximately $90~\rm{\mu m}$ when biased at $-240$ V.
Comments: 4 pages, 7 figures, accepted for publication in Nucl. Instrum. Methods A
Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM)
Cite as: arXiv:2507.21618 [astro-ph.IM]
  (or arXiv:2507.21618v1 [astro-ph.IM] for this version)
  https://doi.org/10.48550/arXiv.2507.21618
arXiv-issued DOI via DataCite
Related DOI: https://doi.org/10.1016/j.nima.2025.170839
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From: Yusuke Suda [view email]
[v1] Tue, 29 Jul 2025 09:16:50 UTC (1,024 KB)
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