Cherenkov Gamma-Ray Telescopes: Past, Present, Future. The ALEGRO Project

Bykov, A. M.; Aharonian, F. A.; Krassilchtchikov, A. M.; Kholupenko, E. E.; Aruev, P. N.; Baiko, D. A.; Bogdanov, A. A.; Vasilyev, G. I.; Zabrodskii, V. V.; Troitsky, S. V.; Tuboltsev, Yu. V.; Kozhberov, A. A.; Levenfish, K. P.; Chichagov, Yu. V.

doi:10.1134/S106378421706007X

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Cherenkov Gamma-Ray Telescopes: Past, Present, Future. The ALEGRO Project

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Aharonian, F. A.
Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society;

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引用

Bykov, A. M., Aharonian, F. A., Krassilchtchikov, A. M., Kholupenko, E. E., Aruev, P. N., Baiko, D. A., Bogdanov, A. A., Vasilyev, G. I., Zabrodskii, V. V., Troitsky, S. V., Tuboltsev, Y. V., Kozhberov, A. A., Levenfish, K. P., & Chichagov, Y. V. (2017). Cherenkov Gamma-Ray Telescopes: Past, Present, Future. The ALEGRO Project. Technical Physics, 62(6), 819-836. doi:10.1134/S106378421706007X.

引用: https://hdl.handle.net/21.11116/0000-0000-CDFE-C

要旨

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.