Abstract
A brief overview of the history of atmospheric Cherenkov gamma-ray telescopes is given. Topical problems of modern astrophysics and fundamental physics to be solved with these instruments are listed. The ALEGRO project of a low-threshold gamma-ray observatory is characterized in detail. The aim of this project is to examine cosmic gamma-ray sources (especially the rapidly variable gamma-ray sources, gamma-ray transients) with high statistics of detected photons in the energy range of 5–50 GeV.
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Original Russian Text © A.M. Bykov, F.A. Aharonian, A.M. Krassilchtchikov, E.E. Kholupenko, P.N. Aruev, D.A. Baiko, A.A. Bogdanov, G.I. Vasilyev, V.V. Zabrodskii, S.V. Troitsky, Yu.V. Tuboltsev, A.A. Kozhberov, K.P. Levenfish, Yu.V. Chichagov, 2017, published in Zhurnal Tekhnicheskoi Fiziki, 2017, Vol. 87, No. 6, pp. 803–821.
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Bykov, A.M., Aharonian, F.A., Krassilchtchikov, A.M. et al. Cherenkov gamma-ray telescopes: Past, present, future. The ALEGRO project. Tech. Phys. 62, 819–836 (2017). https://doi.org/10.1134/S106378421706007X
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DOI: https://doi.org/10.1134/S106378421706007X