14–24 Jul 2025
CICG - International Conference Centre - Geneva, Switzerland
Europe/Zurich timezone

Develoepment of the AstroPix HV-CMOS active pixel sensor for AMEGO-X

Not scheduled
20m
Level -1 & 0

Level -1 & 0

Poster Gamma-Ray Astrophysics PO-2

Speaker

Yasushi Fukazawa

Description

AMEGO-X is planned as a satellite to explore all-sky medium energy gamma-ray observation. MeV gamma-ray observation is important for multi-messenger astronomy. AMEGO-X detector is based on the Si-stacked Compton camera and currently developped AstroPix is considered as Si sensors.
AstroPix is a novel high-voltage CMOS active pixel sensor. AstroPix has to be 0.5 mm thick and active full depletion. Also the energy resolution must be $<10\%$ (FWHM) at 122 keV and the pixel pitch should be 0.5x0.5 mm2. Furthermore, the power consumption must be <1.5 mW/cm2. AstroPix has been developed to incrementally upgrade the chip design towards fulfilling the requirements for AMEGO-X and so far 4 version designs have been fabricated. The third version of AstroPix reached the target pixel pitch with a mean energy resolution of 6.2 keV (FWHM) at 59.5 keV. The latest version 4 is now evaluated in terms of such as I-V curve, noise performance, energy calibration/resolution, dynamic range, and depletion depth. We report the current status of AstroPix testing.

Author

Co-authors

Yusuke Suda (Hiroshima University) Regina Caputo (NASA Goddard Space Flight Center) Daniel Violette (NASA/GSFC, ORAU) Nicolas Striebig (KIT - Karlsruhe Institute of Technology (DE)) Dr Manoj Jadhav Carolyn Kierans (NASA Goddard Space Flight Center) Richard Leys (KIT - Karlsruhe Institute of Technology (DE)) Jessica Metcalfe (Argonne National Laboratory (US)) Mr Norito Nakano Ivan Peric (KIT - Karlsruhe Institute of Technology (DE)) Jeremy Perkins Hiroyasu Tajima (Nagoya University)

Presentation materials