Operation of the SST-1M Cherenkov telescope gamma ray stereoscopic system

The Small-Sized single-mirror Telescopes (SST-1Ms) are designed to observe the gamma rays within the TeV range. The two 4-meter diameter Davies-Cotton SST-1M telescopes are operated at the Ondřejov Observatory of the Astronomical Institute of the Czech Academy of Sciences near Prague. The telescopes use White Rabbit for time synchronization, enabling the detection of coincident events in stereo mode to the performance. The telescopes are remotely operated via a graphical user interface, which allows users to define the source list, execute calibration procedures and monitor telescope subsystems during operation. Onsite data analysis is conducted after the observation provides daily analysis results. The observatory is equipped with an atmospheric monitoring system, including All Sky Camera, an infrared lidar (Ceilometer) and an environmental monitoring system, ensuring accurate measurement of observation conditions. Additionally, the optical point spread function, the pointing accuracy and calibration parameters of the telescope are regularly checked to maintain proper operation and reliable data analysis. We present an overview of the telescope hardware, the operation framework and the calibration scheme of the stereoscopic system.

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Publication Details

Published
2025-09-24
DOI
https://doi.org/10.22323/1.501.0746
Primary Topic
Medical Imaging Techniques and Applications
Type
article
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article

Operation of the SST-1M Cherenkov telescope gamma ray stereoscopic system

F. Cadoux, Anabella Araudo, Matteo Balbo, R. Walter et al.
Medical Imaging Techniques and Applications
article

Operation of the SST-1M Cherenkov telescope gamma ray stereoscopic system

F. Cadoux, 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, D. della Volpe, 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, Dusan Mandat, Petr Janeček, Petr Hamal, Vlastimil Jílek, T. Tavernier, Petr Schovánek, Premysl Dedic, Bastien Lacave, Ernest Glowacki, Michal Miron
article en

Abstract

The Small-Sized single-mirror Telescopes (SST-1Ms) are designed to observe the gamma rays within the TeV range. The two 4-meter diameter Davies-Cotton SST-1M telescopes are operated at the Ondřejov Observatory of the Astronomical Institute of the Czech Academy of Sciences near Prague. The telescopes use White Rabbit for time synchronization, enabling the detection of coincident events in stereo mode to the performance. The telescopes are remotely operated via a graphical user interface, which allows users to define the source list, execute calibration procedures and monitor telescope subsystems during operation. Onsite data analysis is conducted after the observation provides daily analysis results. The observatory is equipped with an atmospheric monitoring system, including All Sky Camera, an infrared lidar (Ceilometer) and an environmental monitoring system, ensuring accurate measurement of observation conditions. Additionally, the optical point spread function, the pointing accuracy and calibration parameters of the telescope are regularly checked to maintain proper operation and reliable data analysis. We present an overview of the telescope hardware, the operation framework and the calibration scheme of the stereoscopic system.

Openalex Percentile: Top 61%
Medical Imaging Techniques and Applications
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