PoS - Proceedings of Science
Volume 312 - 7th International Fermi Symposium (IFS2017) - Session Future Gamma-ray Missions
Development and Testing of the AMEGO Silicon Tracker System
S. Griffin* on behalf of the AMEGO Team
*corresponding author
Full text: pdf
Published on: December 12, 2017
The All-sky Medium Energy Gamma-ray Observatory (AMEGO) is a probe-class mission in consideration for the 2020 decadal review designed to operate at energies from $\sim$ 200 keV to $>$ 10 GeV. Operating a detector in this energy regime is challenging due to the crossover in the interaction cross-section for Compton scattering and pair production. AMEGO is made of four major subsystems: a plastic anticoincidence detector for rejecting cosmic-ray events, a silicon tracker for measuring the energies of Compton scattered electrons and pair-production products, a CZT calorimeter for measuring the energy and location of Compton scattered photons, and a CsI calorimeter for measuring the energy of the pair-production products at high energies. The tracker comprises layers of dual-sided silicon strip detectors which provide energy and localization information for Compton scattering and pair-production events. A prototype tracker system is under development at GSFC; in this contribution we provide details on the verification, packaging, and testing of the prototype tracker, as well as present plans for the development of the front-end electronics, beam tests, and a balloon flight.
DOI: https://doi.org/10.22323/1.312.0186
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