Paper 13093-293
Development of a novel HV-CMOS active pixel sensor AstroPix for gamma-ray space telescopes
On demand | Presenting live 19 June 2024
Abstract
AMEGO-X is one of the proposed MeV gamma-ray missions and its gamma-ray detector consists of silicon trackers and calorimeters. In order to efficiently detect MeV photons and to have precise Compton reconstruction, the silicon sensors must be fully depleted and have a good positional resolution (~500 um) with a good energy resolution. On top of that, the power consumption of the silicon detector must be low (< 1.5 mW/cm2). We have been developing AstroPix, an HV-CMOS active pixel sensor, to fulfill such requirements. Our latest AstroPix (ver.3) is the first full reticle chip designed to meet the requirements for both pixel pitches and power consumption. We report basic characterization of AstroPix-v3 such as I-V, noise, energy calibration/resolutions, dynamic range, and indirect depletion depth measurements using gamma-ray sources. We also present the status of a 2×2 array of AstroPix, Quad-chip, which is the smallest component of the silicon tracker.
Presenter
Yusuke Suda
Hiroshima Univ. (Japan)
Dr. Yusuke Suda is a high energy astrophysicist. He received his doctorate degree in experimental particle physics from the University of Tokyo. He joined the experimental astroparticle physics group at the Max Planck Institute for Physics as a postdoc, working on TeV gamma-ray telescopes. He continues his work at Hiroshima University as an assistant professor.