Abstract
The precise reconstruction of Compton-scatter events is paramount for an imaging medium-energy gamma-ray telescope. The proposed AMEGO-X is enabled by a silicon tracker utilizing AstroPix chips - a pixelated silicon HVCMOS sensor novel for space use. To achieve science goals, each 500 × 500 µm2 pixel must be sensitive for energy deposits ranging from 25-700 keV with an energy resolution of 5 keV at 122 keV (< 10%). This is achieved through depletion of the 500 µm thick sensor, although complete depletion poses an engineering and design challenge. This talk will summarize the current status of depletion measurements highlighting direct measurement with TCT laser scanning and the agreement with simulation. Future plans for further testing will also be identified.
Original language | English |
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Title of host publication | Space Telescopes and Instrumentation 2024 |
Subtitle of host publication | Ultraviolet to Gamma Ray |
Editors | Jan-Willem A. den Herder, Shouleh Nikzad, Kazuhiro Nakazawa |
Publisher | SPIE |
ISBN (Electronic) | 9781510675094 |
DOIs | |
State | Published - 2024 |
Event | Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray - Yokohama, Japan Duration: Jun 16 2024 → Jun 21 2024 |
Publication series
Name | Proceedings of SPIE - The International Society for Optical Engineering |
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Volume | 13093 |
ISSN (Print) | 0277-786X |
ISSN (Electronic) | 1996-756X |
Conference
Conference | Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray |
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Country/Territory | Japan |
City | Yokohama |
Period | 06/16/24 → 06/21/24 |
Funding
This work is funded in part by 18-APRA18-0084 and 20-RTF20-0003. AS acknowledges that research was sponsored by NASA through a contract with ORAU.
Keywords
- AMEGO-X
- AstroPix
- CMOS
- depletion depth
- edge TCT
- gamma-ray instrumentation
- pixelated silicon tracker
- silicon