Abstract
For the proposed space based gamma-ray observatory All-sky Medium-Energy Gamma-ray Observatory eXplorer (AMEGO-X), a silicon tracker based on a novel High Voltage-CMOS (HV-CMOS) sensor called AstroPix, is currently being developed. Preliminary measurements with the first full reticle prototype AstroPix3 show that the power target of 1.5 mW/cm2 can currently not be reached due to the digital consumption of 3.08 mW/cm2, while the analog power consumption of 1.04 mW/cm2 and a break down voltage of over 350 V look promising. Based on these results, the design changes in AstroPix4, submitted in May 2023, are presented, containing changes to the time stamp generation and readout architecture. A digital power consumption below 0.25 mW/cm2 is expected by removing the fast 200 MHz clock used to measure the time-over-threshold (ToT) and an LVDS receiver. A maximum resolution of 3.125 ns for time-of-arrival (ToA) and ToT is reached by adding per-pixel Flash-Time-to-Digital Converter (TDCs) controlled by a global delay-locked loop (DLL).
Original language | English |
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Article number | C04010 |
Journal | Journal of Instrumentation |
Volume | 19 |
Issue number | 4 |
DOIs | |
State | Published - Apr 1 2024 |
Funding
Nicolas Striebig acknowledges the support by the Doctoral School \u201CKarlsruhe School of Elementary and Astroparticle Physics: Science and Technology\u201D.
Keywords
- Digital electronic circuits
- Particle tracking detectors (Solid-state detectors)
- Pixelated detectors and associated VLSI electronics
- Space instrumentation