ASTRI SST-2M prototype and mini-array simulation chain, data reduction software, and archive in the framework of the Cherenkov Telescope Array
S. Lombardi, C. Bigongiari, S. Gallozzi, L.A. Antonelli, D. Bastieri,, I. Donnarumma, F. Lucarelli, M. Mastropietro, P. Munar, M. Perri, A., Stamerra, F. Visconti, M.C. Maccarone (for the CTA ASTRI Project)

TL;DR
This paper presents the development of data reduction software, simulation validation, and archiving systems for the ASTRI SST-2M prototype and mini-array, supporting the CTA gamma-ray observatory's data management and performance evaluation.
Contribution
It introduces an end-to-end software package, simulation validation methods, and a data archive system specifically for the ASTRI SST-2M prototype and mini-array within the CTA project.
Findings
Validated simulation chain with Monte Carlo data
Developed data reduction software for ASTRI telescopes
Established a prototype data archive system
Abstract
The Cherenkov Telescope Array (CTA) is a worldwide project aimed at building the next-generation ground-based gamma-ray observatory. Within the CTA project, the Italian National Institute for Astrophysics (INAF) is developing an end-to-end prototype of the CTA Small-Size Telescopes with a dual-mirror (SST-2M) Schwarzschild-Couder configuration. The prototype, named ASTRI SST-2M, is located at the INAF "M.C. Fracastoro" observing station in Serra La Nave (Mt. Etna, Sicily) and is currently in the scientific and performance validation phase. A mini-array of (at least) nine ASTRI telescopes has been then proposed to be deployed at the Southern CTA site, by means of a collaborative effort carried out by institutes from Italy, Brazil, and South-Africa. The CTA/ASTRI team is developing an end-to-end software package for the reduction of the raw data acquired with both ASTRI SST-2M prototype…
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