The SST-1M imaging atmospheric Cherenkov telescope for gamma-ray astrophysics

Abstract The SST-1M (webpage: https://sst-1m.space ) is a Small-Sized Telescope (SST) designed to provide a cost-effective and high-performance solution for gamma-ray astrophysics, particularly for energies beyond a few TeV. The goal is to integrate this telescope into an array of similar instruments, leveraging its lightweight design, earthquake resistance, and established Davies-Cotton configuration. Additionally, its optical system is designed to function without a protective dome, allowing it to withstand the harsh atmospheric conditions typical of mountain environments above 2000 m a.s.l. The SST-1M utilizes a fully digitizing camera system based on silicon photomultipliers (SiPMs). This camera is capable of digitizing all signals from the UV-optical light detectors, allowing for the implementation of various triggers and data analysis methods. We detail the process of designing, prototyping, and validating this system, ensuring that it meets the stringent requirements for gamma-ray detection and performance. An SST-1M stereo system is currently operational and collecting data at the Ondřejov observatory in the Czech Republic, situated at 500 m a.s.l. Preliminary results from this system are promising. A forthcoming paper will provide a comprehensive analysis of the telescope's performance in detecting gamma rays and operating under real-world conditions.

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2025-02-01
DOI
https://doi.org/10.1088/1475-7516/2025/02/047
Citations
2
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
3.74
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article

The SST-1M imaging atmospheric Cherenkov telescope for gamma-ray astrophysics

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Journal of Cosmology and Astroparticle Physics
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The SST-1M imaging atmospheric Cherenkov telescope for gamma-ray astrophysics

F. Cadoux, Anabella Araudo, M. Palatka, Matteo Balbo, R. Walter, A. Christov, J. Borkowski, P. Schovanek, Dušan Mandát, Jiří Blažek, S. Casanova, M. Jelínek, E. Mach, V. Beshley, Krzystof Zietara, Karol Seweryn, C. Alispach, A. Nagai, P. Trávnı́ček, M. Nikołajuk, M. Prouza, J. Vícha, Martin Vacula, Vladimír Novotný, Ana L. Müller, V. Karas, M. Pech, M. Stodulska, P. Rajda, J. Štrobl, J. Niemiec, Matthieu Heller, R. Moderski, R. Sternberger, L. Gibaud, M. Garczarczyk, I. Troyano Pujadas, Jakub Jurýšek, Dominik Neise, T. Bulik, T. Montaruli, E. Lyard, P. Hamal, L. Chytka, Tomasz Gieras, Adam Muraczewski, Srija Reddy Muthyala, Krzysztof Nalewajski, J. Chudoba, A. Biland, Wojciech Marek, Stanislav Michal, J. Michałowski, Jacek Świerblewski, Petr Janeček, Y. Favre, M. Hrabovský, P. Świerk, V. Sliusar, Ł. Stawarz, M. Ostrowski, D. della Volpe, Vlastimil Jílek, T. Tavernier, Premysl Dedic, Bastien Lacave
article en
2 citations

Abstract

Abstract The SST-1M (webpage: https://sst-1m.space ) is a Small-Sized Telescope (SST) designed to provide a cost-effective and high-performance solution for gamma-ray astrophysics, particularly for energies beyond a few TeV. The goal is to integrate this telescope into an array of similar instruments, leveraging its lightweight design, earthquake resistance, and established Davies-Cotton configuration. Additionally, its optical system is designed to function without a protective dome, allowing it to withstand the harsh atmospheric conditions typical of mountain environments above 2000 m a.s.l. The SST-1M utilizes a fully digitizing camera system based on silicon photomultipliers (SiPMs). This camera is capable of digitizing all signals from the UV-optical light detectors, allowing for the implementation of various triggers and data analysis methods. We detail the process of designing, prototyping, and validating this system, ensuring that it meets the stringent requirements for gamma-ray detection and performance. An SST-1M stereo system is currently operational and collecting data at the Ondřejov observatory in the Czech Republic, situated at 500 m a.s.l. Preliminary results from this system are promising. A forthcoming paper will provide a comprehensive analysis of the telescope's performance in detecting gamma rays and operating under real-world conditions.

Journal of Cosmology and Astroparticle PhysicsVol. 2025(02)
University of Geneva (CH), Centrum Badań Kosmicznych (PL), Jagiellonian University (PL), National Academy of Sciences of Ukraine (UA), Czech Academy of Sciences (CZ), Charles University (CZ), Czech Academy of Sciences, Astronomical Institute (CZ), Deutsches Elektronen-Synchrotron DESY (DE), ETH Zurich (CH), Extreme Light Infrastructure Beamlines (CZ), Institute of Nuclear Physics, Polish Academy of Sciences (PL), Nicolaus Copernicus Astronomical Center (PL), Pidstryhach Institute for Applied Problems of Mechanics and Mathematics (UA), Astronomical Observatory (RS), DSW University of Lower Silesia (PL), Institute of Physics of the Slovak Academy of Sciences (SK), University of Warsaw (PL), AGH University of Krakow (PL), Palacký University Olomouc (CZ), Polish Academy of Sciences (PL)
Openalex Percentile: Top 9%
Astrophysics and Cosmic Phenomena
3.74
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