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First Season of Operation of the TAIGA Hybrid Cherenkov Array

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Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

Work is currently under way in the Tunka Valley, 50 km from Lake Baikal, to create the TAIGA gamma observatory for studying gamma radiation and cosmic ray fluxes in the 1013–1018 eV range of energies. To detect gamma rays with energies above tens of TeV, a hybrid method of detecting showers is implemented. It is based on data obtained by the TAIGA Imaging Atmospheric Cherenkov Telescope (IACT) and the wide-angle TAIGA-HiSCORE array. The preliminary results from processing the telescope’s data for the low-energy region (>2–3 TeV) are presented. Joint events with energy more than 50 TeV are analyzed and compared to Monte Carlo calculations.

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ACKNOWLEDGMENTS

This work was performed on equipment at the Tunka Astrophysical Center as part of an agreement with the RF Ministry of Science and Higher Education, unique identifier RFMEFI59317X0005.

Funding

This work was supported by the RF Ministry of Science and Higher Education as part of State Tasks 3.9678.2017/BCh, 3.904.2017/PCh, 3.6787.2017/ITR, and 1.6790.2017/ITR; and by the Russian Foundation for Basic Research, project no. 16-29-13035.

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Correspondence to L. G. Sveshnikova.

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Translated by M. Chubarova

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Sveshnikova, L.G., Astapov, I.I., Bezyazeekov, P.A. et al. First Season of Operation of the TAIGA Hybrid Cherenkov Array. Bull. Russ. Acad. Sci. Phys. 83, 962–966 (2019). https://doi.org/10.3103/S1062873819080379

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  • DOI: https://doi.org/10.3103/S1062873819080379

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