14–24 Jul 2025
CICG - International Conference Centre - Geneva, Switzerland
Europe/Zurich timezone
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Design and Performance Assessment of the Antarctic Demonstrator for APT (ADAPT): A Next-Generation Gamma-Ray space-borne Telescope

16 Jul 2025, 13:35
15m
CICG - International Conference Centre - Geneva, Switzerland

CICG - International Conference Centre - Geneva, Switzerland

17 rue de Varembé CH - 1211 Geneva Switzerland
Talk Gamma-Ray Astrophysics GA

Speaker

Davide Serini (INFN - National Institute for Nuclear Physics)

Description

The astrophysical community is currently focusing on the development of next-generation gamma-ray telescopes designed to detect low-energy photons in the MeV-GeV range, operating in both the Compton and pair conversion regimes. The proposed Advanced Particle-astrophysics Telescope (APT) is a planned space-based, MeV-TeV gamma-ray mission aimed at providing an order of magnitude improvement in sensitivity over any current mission with a design optimized for dark-matter and multimessenger science. The APT collaboration is an international team focused now on designing and building a high-altitude balloon-borne prototype, the Antarctic Demonstrator for APT (ADAPT), which is anticipated to fly in the 2026-27 season. The current design of the ADAPT instrument includes an imaging CsI calorimeter (ICC) and a scintillating fiber tracker. An ICC module is composed of a 3x3 array of 150 mm x 150 mm x 5 mm CsI(Na) tiles, with top and bottom surfaces covered by 2 mm wavelength-shifting (WLS) fibers, oriented orthogonally along the x- and y-axes and read out by silicon photomultipliers (SiPMs). The ICC modules also have edge-mounted SiPMs for calorimetry. The fiber tracker consists of 1.5 mm round scintillating fibers, arranged in two interleaved layers for both the x- and y-coordinates. Additionally, the ADAPT design includes a Silicon Strip Detector (SSD) to enhance Compton reconstruction and cosmic ray (CR) measurements. The instrument is also equipped with an Anti-Coincidence Detector (ACD) made of plastic scintillators as an outermost detector. The ACD's primary role is to discriminate gamma rays from charged particles and provide complementary measurements for nuclei identification. The performance of each sub-detector, as well as the overall performance of ADAPT, has been extensively evaluated through simulation modeling, laboratory tests, and beam tests. In this contribution, we present an overview of the current design of the ADAPT instrument, its scientific objectives, and its ongoing performance assessment (with a focus on event reconstruction in the Compton regime and real-time gamma-ray burst localization).

Collaboration(s) APT

Authors

Davide Serini (INFN - National Institute for Nuclear Physics) Leonardo Di Venere (INFN - National Institute for Nuclear Physics)

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