SST-1M observation of Markarian 421

Markarian 421 (Mrk 421) is the closest and one of the brightest high-frequency peaked blazars, located at a redshift of z = 0.031. It is a strong source of gamma rays, and its broadband emission has been extensively studied over the years through multi-wavelength observations. Mrk 421 has been the target of an observational campaign from January to May 2024, with 23 nights of observation conducted by the SST-1M telescopes – two single-mirror, small-size Cherenkov telescopes at the Ondřejov Observatory, Czech Republic. These telescopes operate in mono and stereoscopic modes, utilizing the imaging atmospheric Cherenkov technique to detect very high-energy gamma rays in the 1–300 TeV energy range. Using about 32.92 hours of data collected by the telescopes in stereo mode, we find that the gamma-ray spectrum above 1 TeV is well described by a power-law function with an index of 3.24 ± 0.26. In this work, we present our recent SST-1M stereo observations, data analysis, and the results of preliminary physical modeling of Mrk 421’s emission mechanisms.

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Publication Details

Published
2025-09-24
DOI
https://doi.org/10.22323/1.501.0776
Primary Topic
Astronomical Observations and Instrumentation
Type
article
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SST-1M observation of Markarian 421

F. Cadoux, Anabella Araudo, Matteo Balbo, R. Walter et al.
Astronomical Observations and Instrumentation
article

SST-1M observation of Markarian 421

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, Petr Janecek, Dusan Mandat, Petr Hamal, Vlastimil Jílek, T. Tavernier, Petr Schovánek, Premysl Dedic, Bastien Lacave, Ernest Glowacki, Michal Miron
article en

Abstract

Markarian 421 (Mrk 421) is the closest and one of the brightest high-frequency peaked blazars, located at a redshift of z = 0.031. It is a strong source of gamma rays, and its broadband emission has been extensively studied over the years through multi-wavelength observations. Mrk 421 has been the target of an observational campaign from January to May 2024, with 23 nights of observation conducted by the SST-1M telescopes – two single-mirror, small-size Cherenkov telescopes at the Ondřejov Observatory, Czech Republic. These telescopes operate in mono and stereoscopic modes, utilizing the imaging atmospheric Cherenkov technique to detect very high-energy gamma rays in the 1–300 TeV energy range. Using about 32.92 hours of data collected by the telescopes in stereo mode, we find that the gamma-ray spectrum above 1 TeV is well described by a power-law function with an index of 3.24 ± 0.26. In this work, we present our recent SST-1M stereo observations, data analysis, and the results of preliminary physical modeling of Mrk 421’s emission mechanisms.

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Astronomical Observations and Instrumentation
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