γ-Ray Detection with the TAIGA-IACT Installation in the Stereo Mode of Observation
— 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...
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| Veröffentlicht in: | Instruments and experimental techniques (New York) 2024-02, Vol.67 (1), p.143-152 |
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| creator | Volchugov, P. A. Astapov, I. I. Bez’’yazykov, P. A. Bonvech, E. A. Borodin, A. N. Budnev, N. M. Bulan, A. V. Vaidyanatan, A. Volkov, N. V. Voronin, D. M. Gafarov, A. R. Gres’, E. O. Gres’, O. A. Gres’, T. I. Grishin, O. G. Garmash, A. Yu Grebenyuk, V. M. Grinyuk, A. A. Dyachok, A. N. Zhurov, D. P. Zagorodnikov, A. V. Ivanova, A. D. Ivanova, A. L. Ilyushin, M. A. Kalmykov, N. N. Kindin, V. V. Kiryukhin, S. N. Kokoulin, R. P. Kolosov, N. I. Kompaniets, K. G. Korosteleva, E. E. Kozhin, V. A. Kravchenko, E. A. Kryukov, A. P. Kuz’michev, L. A. K’yavassa, A. Lagutin, A. A. Lavrova, M. V. Lemeshev, Yu. E. Lubsandorzhiev, B. K. Lubsandorzhiev, N. B. Malakhov, S. D. Mirgazov, R. R. Monkhoev, R. D. Okuneva, E. A. Osipova, E. A. Panov, A. D. Pakhorukov, A. L. Pan, A. Pan’kov, L. V. Petrukhin, A. A. Podgrudkov, D. A. Popova, E. G. Postnikov, E. B. Prosin, V. V. Ptuskin, V. S. Pushnin, A. A. Razumov, A. Yu Raikin, R. I. Rubtsov, G. I. Ryabov, E. V. Samoliga, V. S. Satyshev, I. Sveshnikova, L. G. Silaev, A. A. Silaev (Jr.), A. A. Sidorenkov, A. Yu Skurikhin, A. V. Sokolov, A. V. Tabolenko, V. A. Tanaev, A. B. Ternovoi, M. Yu Tkachev, L. G. Ushakov, N. A. Chernov, D. V. Yashin, I. I. |
| description | —
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
2
; 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 (
X
max
), 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. |
| doi_str_mv | 10.1134/S0020441224700106 |
| format | Article |
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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
2
; 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 (
X
max
), 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.</description><identifier>ISSN: 0020-4412</identifier><identifier>EISSN: 1608-3180</identifier><identifier>DOI: 10.1134/S0020441224700106</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Biology ; Electrical Engineering ; Measurement Science and Instrumentation ; Medicine ; Physical Chemistry ; Physical Instruments for Ecology ; Physics ; Physics and Astronomy</subject><ispartof>Instruments and experimental techniques (New York), 2024-02, Vol.67 (1), p.143-152</ispartof><rights>Pleiades Publishing, Ltd. 2024. ISSN 0020-4412, Instruments and Experimental Techniques, 2024, Vol. 67, No. 1, pp. 143–152. © Pleiades Publishing, Ltd., 2024.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c170t-53216c5d4f3ab009539b169ba99c0a975f5b541ba6a4549ba3cc3ce476f9a7a03</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S0020441224700106$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S0020441224700106$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>Volchugov, P. A.</creatorcontrib><creatorcontrib>Astapov, I. I.</creatorcontrib><creatorcontrib>Bez’’yazykov, P. A.</creatorcontrib><creatorcontrib>Bonvech, E. 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A.</creatorcontrib><creatorcontrib>Osipova, E. A.</creatorcontrib><creatorcontrib>Panov, A. D.</creatorcontrib><creatorcontrib>Pakhorukov, A. L.</creatorcontrib><creatorcontrib>Pan, A.</creatorcontrib><creatorcontrib>Pan’kov, L. V.</creatorcontrib><creatorcontrib>Petrukhin, A. A.</creatorcontrib><creatorcontrib>Podgrudkov, D. A.</creatorcontrib><creatorcontrib>Popova, E. G.</creatorcontrib><creatorcontrib>Postnikov, E. B.</creatorcontrib><creatorcontrib>Prosin, V. V.</creatorcontrib><creatorcontrib>Ptuskin, V. S.</creatorcontrib><creatorcontrib>Pushnin, A. A.</creatorcontrib><creatorcontrib>Razumov, A. Yu</creatorcontrib><creatorcontrib>Raikin, R. I.</creatorcontrib><creatorcontrib>Rubtsov, G. I.</creatorcontrib><creatorcontrib>Ryabov, E. V.</creatorcontrib><creatorcontrib>Samoliga, V. S.</creatorcontrib><creatorcontrib>Satyshev, I.</creatorcontrib><creatorcontrib>Sveshnikova, L. G.</creatorcontrib><creatorcontrib>Silaev, A. A.</creatorcontrib><creatorcontrib>Silaev (Jr.), A. A.</creatorcontrib><creatorcontrib>Sidorenkov, A. Yu</creatorcontrib><creatorcontrib>Skurikhin, A. V.</creatorcontrib><creatorcontrib>Sokolov, A. V.</creatorcontrib><creatorcontrib>Tabolenko, V. A.</creatorcontrib><creatorcontrib>Tanaev, A. B.</creatorcontrib><creatorcontrib>Ternovoi, M. Yu</creatorcontrib><creatorcontrib>Tkachev, L. G.</creatorcontrib><creatorcontrib>Ushakov, N. A.</creatorcontrib><creatorcontrib>Chernov, D. V.</creatorcontrib><creatorcontrib>Yashin, I. I.</creatorcontrib><title>γ-Ray Detection with the TAIGA-IACT Installation in the Stereo Mode of Observation</title><title>Instruments and experimental techniques (New York)</title><addtitle>Instrum Exp Tech</addtitle><description>—
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
2
; 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 (
X
max
), 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.</description><subject>Biology</subject><subject>Electrical Engineering</subject><subject>Measurement Science and Instrumentation</subject><subject>Medicine</subject><subject>Physical Chemistry</subject><subject>Physical Instruments for Ecology</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><issn>0020-4412</issn><issn>1608-3180</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><recordid>eNp9kEFOwzAURC0EEqVwAHa-gOH_2I7rZVSgjVRUiZZ15LgOTRUSZBtQz8U9OBNJyw6J1ZfmzXyNhpBrhBtELm5XAAkIgUkiFABCekJGmMKEcZzAKRkNmA38nFyEsAMArZQakdX3F3sye3rnorOx7lr6WcctjVtH11k-y1ieTdc0b0M0TWMOhro94FV03nX0sds42lV0WQbnPw6OS3JWmSa4q987Js8P9-vpnC2Ws3yaLZhFBZFJnmBq5UZU3JR9H8l1iakujdYWjFaykqUUWJrUCCl6nVvLrRMqrbRRBviY4PGv9V0I3lXFm69fjd8XCMWwSvFnlT6THDOh97Yvzhe77t23fc1_Qj-eF2Lw</recordid><startdate>20240201</startdate><enddate>20240201</enddate><creator>Volchugov, P. 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M. ; Gafarov, A. R. ; Gres’, E. O. ; Gres’, O. A. ; Gres’, T. I. ; Grishin, O. G. ; Garmash, A. Yu ; Grebenyuk, V. M. ; Grinyuk, A. A. ; Dyachok, A. N. ; Zhurov, D. P. ; Zagorodnikov, A. V. ; Ivanova, A. D. ; Ivanova, A. L. ; Ilyushin, M. A. ; Kalmykov, N. N. ; Kindin, V. V. ; Kiryukhin, S. N. ; Kokoulin, R. P. ; Kolosov, N. I. ; Kompaniets, K. G. ; Korosteleva, E. E. ; Kozhin, V. A. ; Kravchenko, E. A. ; Kryukov, A. P. ; Kuz’michev, L. A. ; K’yavassa, A. ; Lagutin, A. A. ; Lavrova, M. V. ; Lemeshev, Yu. E. ; Lubsandorzhiev, B. K. ; Lubsandorzhiev, N. B. ; Malakhov, S. D. ; Mirgazov, R. R. ; Monkhoev, R. D. ; Okuneva, E. A. ; Osipova, E. A. ; Panov, A. D. ; Pakhorukov, A. L. ; Pan, A. ; Pan’kov, L. V. ; Petrukhin, A. A. ; Podgrudkov, D. A. ; Popova, E. G. ; Postnikov, E. B. ; Prosin, V. V. ; Ptuskin, V. S. ; Pushnin, A. A. ; Razumov, A. Yu ; Raikin, R. I. ; Rubtsov, G. I. ; Ryabov, E. V. ; Samoliga, V. S. ; Satyshev, I. ; Sveshnikova, L. G. ; Silaev, A. A. ; Silaev (Jr.), A. A. ; Sidorenkov, A. Yu ; Skurikhin, A. V. ; Sokolov, A. V. ; Tabolenko, V. A. ; Tanaev, A. B. ; Ternovoi, M. Yu ; Tkachev, L. G. ; Ushakov, N. A. ; Chernov, D. V. ; Yashin, I. I.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c170t-53216c5d4f3ab009539b169ba99c0a975f5b541ba6a4549ba3cc3ce476f9a7a03</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Biology</topic><topic>Electrical Engineering</topic><topic>Measurement Science and Instrumentation</topic><topic>Medicine</topic><topic>Physical Chemistry</topic><topic>Physical Instruments for Ecology</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Volchugov, P. A.</creatorcontrib><creatorcontrib>Astapov, I. I.</creatorcontrib><creatorcontrib>Bez’’yazykov, P. A.</creatorcontrib><creatorcontrib>Bonvech, E. A.</creatorcontrib><creatorcontrib>Borodin, A. N.</creatorcontrib><creatorcontrib>Budnev, N. M.</creatorcontrib><creatorcontrib>Bulan, A. V.</creatorcontrib><creatorcontrib>Vaidyanatan, A.</creatorcontrib><creatorcontrib>Volkov, N. V.</creatorcontrib><creatorcontrib>Voronin, D. M.</creatorcontrib><creatorcontrib>Gafarov, A. R.</creatorcontrib><creatorcontrib>Gres’, E. O.</creatorcontrib><creatorcontrib>Gres’, O. A.</creatorcontrib><creatorcontrib>Gres’, T. I.</creatorcontrib><creatorcontrib>Grishin, O. G.</creatorcontrib><creatorcontrib>Garmash, A. Yu</creatorcontrib><creatorcontrib>Grebenyuk, V. M.</creatorcontrib><creatorcontrib>Grinyuk, A. A.</creatorcontrib><creatorcontrib>Dyachok, A. N.</creatorcontrib><creatorcontrib>Zhurov, D. P.</creatorcontrib><creatorcontrib>Zagorodnikov, A. V.</creatorcontrib><creatorcontrib>Ivanova, A. D.</creatorcontrib><creatorcontrib>Ivanova, A. L.</creatorcontrib><creatorcontrib>Ilyushin, M. A.</creatorcontrib><creatorcontrib>Kalmykov, N. N.</creatorcontrib><creatorcontrib>Kindin, V. V.</creatorcontrib><creatorcontrib>Kiryukhin, S. N.</creatorcontrib><creatorcontrib>Kokoulin, R. P.</creatorcontrib><creatorcontrib>Kolosov, N. I.</creatorcontrib><creatorcontrib>Kompaniets, K. G.</creatorcontrib><creatorcontrib>Korosteleva, E. E.</creatorcontrib><creatorcontrib>Kozhin, V. A.</creatorcontrib><creatorcontrib>Kravchenko, E. A.</creatorcontrib><creatorcontrib>Kryukov, A. P.</creatorcontrib><creatorcontrib>Kuz’michev, L. A.</creatorcontrib><creatorcontrib>K’yavassa, A.</creatorcontrib><creatorcontrib>Lagutin, A. A.</creatorcontrib><creatorcontrib>Lavrova, M. V.</creatorcontrib><creatorcontrib>Lemeshev, Yu. E.</creatorcontrib><creatorcontrib>Lubsandorzhiev, B. K.</creatorcontrib><creatorcontrib>Lubsandorzhiev, N. B.</creatorcontrib><creatorcontrib>Malakhov, S. D.</creatorcontrib><creatorcontrib>Mirgazov, R. R.</creatorcontrib><creatorcontrib>Monkhoev, R. D.</creatorcontrib><creatorcontrib>Okuneva, E. A.</creatorcontrib><creatorcontrib>Osipova, E. A.</creatorcontrib><creatorcontrib>Panov, A. D.</creatorcontrib><creatorcontrib>Pakhorukov, A. L.</creatorcontrib><creatorcontrib>Pan, A.</creatorcontrib><creatorcontrib>Pan’kov, L. V.</creatorcontrib><creatorcontrib>Petrukhin, A. A.</creatorcontrib><creatorcontrib>Podgrudkov, D. A.</creatorcontrib><creatorcontrib>Popova, E. G.</creatorcontrib><creatorcontrib>Postnikov, E. B.</creatorcontrib><creatorcontrib>Prosin, V. V.</creatorcontrib><creatorcontrib>Ptuskin, V. S.</creatorcontrib><creatorcontrib>Pushnin, A. A.</creatorcontrib><creatorcontrib>Razumov, A. Yu</creatorcontrib><creatorcontrib>Raikin, R. I.</creatorcontrib><creatorcontrib>Rubtsov, G. I.</creatorcontrib><creatorcontrib>Ryabov, E. V.</creatorcontrib><creatorcontrib>Samoliga, V. S.</creatorcontrib><creatorcontrib>Satyshev, I.</creatorcontrib><creatorcontrib>Sveshnikova, L. G.</creatorcontrib><creatorcontrib>Silaev, A. A.</creatorcontrib><creatorcontrib>Silaev (Jr.), A. A.</creatorcontrib><creatorcontrib>Sidorenkov, A. Yu</creatorcontrib><creatorcontrib>Skurikhin, A. V.</creatorcontrib><creatorcontrib>Sokolov, A. V.</creatorcontrib><creatorcontrib>Tabolenko, V. A.</creatorcontrib><creatorcontrib>Tanaev, A. B.</creatorcontrib><creatorcontrib>Ternovoi, M. Yu</creatorcontrib><creatorcontrib>Tkachev, L. G.</creatorcontrib><creatorcontrib>Ushakov, N. A.</creatorcontrib><creatorcontrib>Chernov, D. V.</creatorcontrib><creatorcontrib>Yashin, I. I.</creatorcontrib><collection>CrossRef</collection><jtitle>Instruments and experimental techniques (New York)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Volchugov, P. A.</au><au>Astapov, I. I.</au><au>Bez’’yazykov, P. A.</au><au>Bonvech, E. A.</au><au>Borodin, A. N.</au><au>Budnev, N. M.</au><au>Bulan, A. V.</au><au>Vaidyanatan, A.</au><au>Volkov, N. V.</au><au>Voronin, D. M.</au><au>Gafarov, A. R.</au><au>Gres’, E. O.</au><au>Gres’, O. A.</au><au>Gres’, T. I.</au><au>Grishin, O. G.</au><au>Garmash, A. Yu</au><au>Grebenyuk, V. M.</au><au>Grinyuk, A. A.</au><au>Dyachok, A. N.</au><au>Zhurov, D. P.</au><au>Zagorodnikov, A. V.</au><au>Ivanova, A. D.</au><au>Ivanova, A. L.</au><au>Ilyushin, M. A.</au><au>Kalmykov, N. N.</au><au>Kindin, V. V.</au><au>Kiryukhin, S. N.</au><au>Kokoulin, R. P.</au><au>Kolosov, N. I.</au><au>Kompaniets, K. G.</au><au>Korosteleva, E. E.</au><au>Kozhin, V. A.</au><au>Kravchenko, E. A.</au><au>Kryukov, A. P.</au><au>Kuz’michev, L. A.</au><au>K’yavassa, A.</au><au>Lagutin, A. A.</au><au>Lavrova, M. V.</au><au>Lemeshev, Yu. E.</au><au>Lubsandorzhiev, B. K.</au><au>Lubsandorzhiev, N. B.</au><au>Malakhov, S. D.</au><au>Mirgazov, R. R.</au><au>Monkhoev, R. D.</au><au>Okuneva, E. A.</au><au>Osipova, E. A.</au><au>Panov, A. D.</au><au>Pakhorukov, A. L.</au><au>Pan, A.</au><au>Pan’kov, L. V.</au><au>Petrukhin, A. A.</au><au>Podgrudkov, D. A.</au><au>Popova, E. G.</au><au>Postnikov, E. B.</au><au>Prosin, V. V.</au><au>Ptuskin, V. S.</au><au>Pushnin, A. A.</au><au>Razumov, A. Yu</au><au>Raikin, R. I.</au><au>Rubtsov, G. I.</au><au>Ryabov, E. V.</au><au>Samoliga, V. S.</au><au>Satyshev, I.</au><au>Sveshnikova, L. G.</au><au>Silaev, A. A.</au><au>Silaev (Jr.), A. A.</au><au>Sidorenkov, A. Yu</au><au>Skurikhin, A. V.</au><au>Sokolov, A. V.</au><au>Tabolenko, V. A.</au><au>Tanaev, A. B.</au><au>Ternovoi, M. Yu</au><au>Tkachev, L. G.</au><au>Ushakov, N. A.</au><au>Chernov, D. V.</au><au>Yashin, I. I.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>γ-Ray Detection with the TAIGA-IACT Installation in the Stereo Mode of Observation</atitle><jtitle>Instruments and experimental techniques (New York)</jtitle><stitle>Instrum Exp Tech</stitle><date>2024-02-01</date><risdate>2024</risdate><volume>67</volume><issue>1</issue><spage>143</spage><epage>152</epage><pages>143-152</pages><issn>0020-4412</issn><eissn>1608-3180</eissn><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 km
2
; 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 (
X
max
), 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.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S0020441224700106</doi><tpages>10</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0020-4412 |
| ispartof | Instruments and experimental techniques (New York), 2024-02, Vol.67 (1), p.143-152 |
| issn | 0020-4412 1608-3180 |
| language | eng |
| recordid | cdi_crossref_primary_10_1134_S0020441224700106 |
| source | Springer Nature - Complete Springer Journals |
| subjects | Biology Electrical Engineering Measurement Science and Instrumentation Medicine Physical Chemistry Physical Instruments for Ecology Physics Physics and Astronomy |
| title | γ-Ray Detection with the TAIGA-IACT Installation in the Stereo Mode of Observation |
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