Performance Evaluation of the Readout Electronics Board Based on the Smart Asic for the Adapt Instrument

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Authors: G. De Palma, Marco Cecca, L. Di Venere, Francesco Licciulli, Mario Nicola Mazziotta, Elisabetta Bissaldi, James Buckley, Blake Bal, Richard Bose, Adrian Zink
Cited by: 1
References: 13

Abstract

The Advanced Particle–astrophysics Telescope (APT) is a mission concept for a future space-based MeV-TeV observatory, designed to combine a Compton and e+e− pair telescope, aiming to improve the sensitivity of the instruments to γ 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.

Fields of Study & Subjects

Radiation Detection and Scintillator Technologies Particle Detector Development and Performance Photocathodes and Microchannel Plates

Publication details

Journal / source
Particles
Publisher
MDPI AG
Volume
9
Issue
1
Pages
14–14
Publication date
10 February 2026
Language
EN