E. B. Postnikov, I. I. Astapov, P. A. Bez’’yazykov, A. V. Blinov, E. A. Bonvech, A. N. Borodin, N. M. Budnev, A. V. Bulan, D. V. Chernov, A. Chiavassa, A. N. Dyachok, A. R. Gafarov, A. Yu. Garmash, V. M. Grebenyuk, E. O. Gres’, O. A. Gres’, T. I. Gres’, A. A. Grinyuk, O. G. Grishin, A. D. Ivanova, A. L. Ivanova, M. A. Ilyushin, N. N. Kalmykov, V. V. Kindin, S. N. Kiryukhin, R. P. Kokoulin, N. I. Kolosov, K. G. Kompaniets, E. E. Korosteleva, V. A. Kozhin, E. A. Kravchenko, A. P. Kryukov, L. A. Kuzmichev, A. A. Lagutin, M. V. Lavrova, Yu. E. Lemeshev, B. K. Lubsandorzhiev, N. B. Lubsandorzhiev, A. D. Lukanov, S. D. Malakhov, R. R. Mirgazov, R. D. Monkhoev, E. A. Okuneva, E. A. Osipova, A. L. Pakhorukov, A. Pan, A. D. Panov, L. V. Pankov, A. A. Petrukhin, I. A. Poddubnyi, D. A. Podgrudkov, E. G. Popova, V. V. Prosin, V. S. Ptuskin, A. A. Pushnin, R. I. Raikin, A. V. Razumov, E. V. Ryabov, G. I. Rubtsov, V. S. Samoliga, I. Satyshev, A. V. Shaykovskiy, A. Yu. Sidorenkov, A. A. Silaev, A. A. Silaev Jr., A. V. Skurikhin, A. V. Sokolov, L. G. Sveshikova, V. A. Tabolenko, A. B. Tanaev, M. Yu. Ternovoy, L. G. Tkachev, N. A. Ushakov, P. A. Volchugov, N. V. Volkov, D. M. Voronin, I. I. Yashin, A. V. Zagorodnikov, D. P. Zhurov, V. N. Zirakashvili
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V. Shaykovskiy, A. Yu. Sidorenkov, A. A. Silaev, A. A. Silaev Jr., A. V. Skurikhin, A. V. Sokolov, L. G. Sveshikova, V. A. Tabolenko, A. B. Tanaev, M. Yu. Ternovoy, L. G. Tkachev, N. A. Ushakov, P. A. Volchugov, N. V. Volkov, D. M. Voronin, I. I. Yashin, A. V. Zagorodnikov, D. P. Zhurov, V. N. Zirakashvili","doi":"10.1134/S1063779624702125","DOIUrl":null,"url":null,"abstract":"<p>The astrophysical experiment TAIGA-10 (Tunka Advanced Instrument for cosmic ray physics and Gamma-ray Astronomy) is planned to extend by mounting new telescopes with improved parameters: a smaller camera pixel size of a larger mirror diameter. 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Hadron Rejection in an Imaging Air Cherenkov Telescope Depending on the Mirror Diameter and Camera Pixel Size
The astrophysical experiment TAIGA-10 (Tunka Advanced Instrument for cosmic ray physics and Gamma-ray Astronomy) is planned to extend by mounting new telescopes with improved parameters: a smaller camera pixel size of a larger mirror diameter. The simulation of new and already installed telescopes has been conducted, and expected improvement in the hadron background rejection after transition to smaller pixel sizes and a larger mirror diameter has been quantitatively estimated.
期刊介绍：
The journal Fizika Elementarnykh Chastits i Atomnogo Yadr of the Joint Institute for Nuclear Research (JINR, Dubna) was founded by Academician N.N. Bogolyubov in August 1969. The Editors-in-chief of the journal were Academician N.N. Bogolyubov (1970–1992) and Academician A.M. Baldin (1992–2001). Its English translation, Physics of Particles and Nuclei, appears simultaneously with the original Russian-language edition. Published by leading physicists from the JINR member states, as well as by scientists from other countries, review articles in this journal examine problems of elementary particle physics, nuclear physics, condensed matter physics, experimental data processing, accelerators and related instrumentation ecology and radiology.
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