Stereo performance of SST-1M at different altitudes

The SST-1M telescopes are a pair of Imaging Atmospheric Cherenkov Telescopes (IACTs) that have been operating at the Ondřejov Observatory (510m a.s.l.) in the Czech Republic since 2022. Optimized for detecting gamma rays in the energy range 1-300 TeV, they are capable of performing both mono and stereo observations. Despite challenging atmospheric conditions, SST-1M has successfully detected several galactic and extragalactic gamma-ray sources with energies reaching up to 200 TeV during its ongoing commissioning. In this study, we analyze the performance of the SST-1M telescopes at different locations to assess the impact of altitude and relative telescope spacing on their physics performance. The low-altitude site at 510m a.s.l. has already been investigated using both Monte Carlo simulations and real data. For comparison, we selected an intermediate-altitude site at 1420m a.s.l. corresponding to Pampa Amarilla in Argentina and a high-altitude site at 4270m a.s.l. corresponding to Hanle in India – both of which offer favorable astronomical conditions.

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Publication Details

Published
2025-09-24
DOI
https://doi.org/10.22323/1.501.0908
Primary Topic
Advanced Vision and Imaging
Type
article
Field-Weighted Citation Impact
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article

Stereo performance of SST-1M at different altitudes

Anabella Araudo, Matteo Balbo, R. Walter, J. Borkowski et al.
Advanced Vision and Imaging
article

Stereo performance of SST-1M at different altitudes

Anabella Araudo, Matteo Balbo, R. Walter, J. Borkowski, Jiří Blažek, Vasyl Beshley, S. Casanova, Stella Boula, M. Jelínek, M. Ostrowski, A. Christov, Cyril Martin Alispach, E. Mach, Paweł Świerk, M. Hrabovský, A. Nagai, P. Trávnı́ček, Ł. Stawarz, M. Nikołajuk, I. Troyano Pujadas, J. Vícha, L. Chytka, Vladimír Novotný, V. Karas, M. Palatka, Vitalii Sliusar, M. Stodulska, J. Štrobl, J. Niemiec, Matthieu Heller, R. Moderski, R. Sternberger, L. Gibaud, Patrik Čechvala, M. Garczarczyk, T. Montaruli, Jakub Jurýšek, Dominik Neise, M. Prouza, T. Bulik, Krzysztof Ziȩtara, Ana Laura Muller, E. Lyard, Tomasz Gieras, Adam Muraczewski, Srija Reddy Muthyala, Krzysztof Nalewajski, Jerzy Michalowksi, J. Chudoba, Wojciech Marek, Stanislav Michal, Yannick Favre, Jacek Świerblewski, Miroslav Pech, Petr Janecek, Dusan Mandat, Franck Cadoux, Petr Hamal, Vlastimil Jílek, T. Tavernier, Petr Schovánek, Premysl Dedic, Bastien Lacave, Domenico della Volpe, Ernest Glowacki, Michal Miron
article en

Abstract

The SST-1M telescopes are a pair of Imaging Atmospheric Cherenkov Telescopes (IACTs) that have been operating at the Ondřejov Observatory (510m a.s.l.) in the Czech Republic since 2022. Optimized for detecting gamma rays in the energy range 1-300 TeV, they are capable of performing both mono and stereo observations. Despite challenging atmospheric conditions, SST-1M has successfully detected several galactic and extragalactic gamma-ray sources with energies reaching up to 200 TeV during its ongoing commissioning. In this study, we analyze the performance of the SST-1M telescopes at different locations to assess the impact of altitude and relative telescope spacing on their physics performance. The low-altitude site at 510m a.s.l. has already been investigated using both Monte Carlo simulations and real data. For comparison, we selected an intermediate-altitude site at 1420m a.s.l. corresponding to Pampa Amarilla in Argentina and a high-altitude site at 4270m a.s.l. corresponding to Hanle in India – both of which offer favorable astronomical conditions.

European Commission, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Ministerstvo Školství, Mládeže a Tělovýchovy, Grantová Agentura České Republiky, Université de Genève
Openalex Percentile: Top 74%
Advanced Vision and Imaging
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