Abstract
The TAIGA hybrid gamma-ray observatory is currently being developed in the Tunka Valley, 50 km from Lake Baikal, to study gamma radiation and charged cosmic ray fluxes in the 1013–1018 eV range. The first results are presented for detecting gamma rays from the Crab Nebula in 44 h of observation, and from the blazar Markarian 421 in 62 h of observation with a significance of around 5–6 σ by one of the TAIGA IACT telescopes.
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Funding
This work was supported by the RF Ministry of Science and Education as part of State Task FZZE-2020-0024, agreement no. 075-15-2019-163; by the Russian Science Foundation, project nos. 19-72-20067 (sections 1, 3, 4, 5) and 19-72-20173 (section 2); and by the Russian Foundation for Basic Research, project nos. 19-52-44002 and 19‑32-60003.
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Translated by L. Mukhortova
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Sveshnikova, L.G., Astapov, I.I., Bezyazeekov, P.A. et al. Detecting Gamma Rays with Energies Greater than 3–4 ТeV from the Crab Nebula and Blazar Markarian 421 by Imaging Atmospheric Cherenkov Telescopes in the TAIGA Experiment. Bull. Russ. Acad. Sci. Phys. 85, 398–401 (2021). https://doi.org/10.3103/S1062873821040365
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DOI: https://doi.org/10.3103/S1062873821040365