De Palma G, Cecca M, Di Venere L, Licciulli F, Mazziotta MN, Bissaldi E, Buckley J, Bal B, Bose R, Zink A (2026)
Publication Type: Journal article
Publication year: 2026
Book Volume: 9
Article Number: 14
Journal Issue: 1
The Advanced Particle–astrophysics Telescope (APT) is a mission concept for a future space-based MeV-TeV observatory, designed to combine a Compton and (Formula presented.) pair telescope, aiming to improve the sensitivity of the instruments to (Formula presented.) rays in the MeV-GeV range by at least one order of magnitude. To validate and study the technologies that will be employed on the observatory, a small-scale prototype, the Antarctic Demonstrator for APT (ADAPT), is currently being developed to fly on a balloon in Antarctica during the local 2026–2027 flight season. Among its subdetectors there is an Imaging CsI calorimeter (ICC), consisting of 4 layers of CsI(Na) crystals with crossed WLS fibers, coupled to Silicon Photomultipliers (SiPMs). A key element of the design is the multichannel front-end electronics, based on the SMART (SiPM Multichannel ASIC for high-Resolution Cherenkov Telescopes) ASIC, which combines compactness, cost-effectiveness, and a high level of integration. This work reports the results of quality-control tests performed on the custom readout boards for the ICC, and provides an overview of the present status of the mission.
APA:
De Palma, G., Cecca, M., Di Venere, L., Licciulli, F., Mazziotta, M.N., Bissaldi, E.,... Zink, A. (2026). Performance Evaluation of the Readout Electronics Board Based on the Smart Asic for the Adapt Instrument. , 9(1). https://doi.org/10.3390/particles9010014
MLA:
De Palma, Gaia, et al. "Performance Evaluation of the Readout Electronics Board Based on the Smart Asic for the Adapt Instrument." 9.1 (2026).
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