P. A. Volchugov, I. I. Astapov, P. A. Bez’’yazykov, E. A. Bonvech, A. N. Borodin, N. M. Budnev, A. V. Bulan, A. Vaidyanatan, N. V. Volkov, D. M. Voronin, A. R. Gafarov, E. O. Gres’, O. A. Gres’, T. I. Gres’, O. G. Grishin, A. Yu. Garmash, V. M. Grebenyuk, A. A. Grinyuk, A. N. Dyachok, D. P. Zhurov, A. V. Zagorodnikov, 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. Kuz’michev, A. K’yavassa, A. A. Lagutin, M. V. Lavrova, Yu. E. Lemeshev, B. K. Lubsandorzhiev, N. B. Lubsandorzhiev, S. D. Malakhov, R. R. Mirgazov, R. D. Monkhoev, E. A. Okuneva, E. A. Osipova, A. D. Panov, A. L. Pakhorukov, A. Pan, L. V. Pan’kov, A. A. Petrukhin, D. A. Podgrudkov, E. G. Popova, E. B. Postnikov, V. V. Prosin, V. S. Ptuskin, A. A. Pushnin, A. Yu. Razumov, R. I. Raikin, G. I. Rubtsov, E. V. Ryabov, V. S. Samoliga, I. Satyshev, L. G. Sve..
{"title":"在立体观测模式下利用 TAIGA-IACT 装置进行 γ 射线探测","authors":"P. A. Volchugov, I. I. Astapov, P. A. Bez’’yazykov, E. A. Bonvech, A. N. Borodin, N. M. Budnev, A. V. Bulan, A. Vaidyanatan, N. V. Volkov, D. M. Voronin, A. R. Gafarov, E. O. Gres’, O. A. Gres’, T. I. Gres’, O. G. Grishin, A. Yu. Garmash, V. M. Grebenyuk, A. A. Grinyuk, A. N. Dyachok, D. P. Zhurov, A. V. Zagorodnikov, 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. Kuz’michev, A. K’yavassa, A. A. Lagutin, M. V. Lavrova, Yu. E. Lemeshev, B. K. Lubsandorzhiev, N. B. Lubsandorzhiev, S. D. Malakhov, R. R. Mirgazov, R. D. Monkhoev, E. A. Okuneva, E. A. Osipova, A. D. Panov, A. L. Pakhorukov, A. Pan, L. V. Pan’kov, A. A. Petrukhin, D. A. Podgrudkov, E. G. Popova, E. B. Postnikov, V. V. Prosin, V. S. Ptuskin, A. A. Pushnin, A. Yu. Razumov, R. I. Raikin, G. I. Rubtsov, E. V. Ryabov, V. S. Samoliga, I. Satyshev, L. G. Sve..","doi":"10.1134/s0020441224700106","DOIUrl":null,"url":null,"abstract":"<h3 data-test=\"abstract-sub-heading\">Abstract—</h3><p>The paper is devoted to the modeling and analysis of data detected by the TAIGA-IACT installation in the stereo mode. Five Imaging Atmospheric Cherenkov Telescopes (IACT) with a viewing angle of 9.6° are expected to be included in the installation. Today there are three telescopes spaced far apart (from 320 to 500 m) in the installation. The effective area of the installation is as large as 0.6 km<sup>2</sup>; therefore, it is possible to conduct statistically significant measurements of weak γ-ray sources in the energy range above 10 TeV over a reasonable observation time (300–400 h). The Monte Carlo procedure for simulating the hadrons and γ-rays detected by the telescopes is described as is the procedure for reconstructing the parameters of extensive air showers, such as the arrival direction of an event, the axis position, the depth of the maximum of shower development (<i>X</i><sub>max</sub>), and the primary-particle energy. In order to solve the problem of γ-hadron separation, the criteria for selecting γ-rays detected in the stereo mode have been optimized and the effective area of the installation has been calculated.</p>","PeriodicalId":587,"journal":{"name":"Instruments and Experimental Techniques","volume":null,"pages":null},"PeriodicalIF":0.4000,"publicationDate":"2024-06-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"γ-Ray Detection with the TAIGA-IACT Installation in the Stereo Mode of Observation\",\"authors\":\"P. A. Volchugov, I. I. Astapov, P. A. 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The Monte Carlo procedure for simulating the hadrons and γ-rays detected by the telescopes is described as is the procedure for reconstructing the parameters of extensive air showers, such as the arrival direction of an event, the axis position, the depth of the maximum of shower development (<i>X</i><sub>max</sub>), and the primary-particle energy. 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γ-Ray Detection with the TAIGA-IACT Installation in the Stereo Mode of Observation
Abstract—
The paper is devoted to the modeling and analysis of data detected by the TAIGA-IACT installation in the stereo mode. Five Imaging Atmospheric Cherenkov Telescopes (IACT) with a viewing angle of 9.6° are expected to be included in the installation. Today there are three telescopes spaced far apart (from 320 to 500 m) in the installation. The effective area of the installation is as large as 0.6 km2; therefore, it is possible to conduct statistically significant measurements of weak γ-ray sources in the energy range above 10 TeV over a reasonable observation time (300–400 h). The Monte Carlo procedure for simulating the hadrons and γ-rays detected by the telescopes is described as is the procedure for reconstructing the parameters of extensive air showers, such as the arrival direction of an event, the axis position, the depth of the maximum of shower development (Xmax), and the primary-particle energy. In order to solve the problem of γ-hadron separation, the criteria for selecting γ-rays detected in the stereo mode have been optimized and the effective area of the installation has been calculated.
期刊介绍：
Instruments and Experimental Techniques is an international peer reviewed journal that publishes reviews describing advanced methods for physical measurements and techniques and original articles that present techniques for physical measurements, principles of operation, design, methods of application, and analysis of the operation of physical instruments used in all fields of experimental physics and when conducting measurements using physical methods and instruments in astronomy, natural sciences, chemistry, biology, medicine, and ecology.
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