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Hybrid method for study multi TeV gamma rays in the TAIGA astrophysical complex: methodics and results. / TAIGA Collaboration ; Вайдянатан, Арун .

в: Proceedings of Science, Том 444, 685, 27.09.2024.

Результаты исследований: Научные публикации в периодических изданияхстатья по материалам конференцииРецензирование

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TAIGA Collaboration, Вайдянатан А. Hybrid method for study multi TeV gamma rays in the TAIGA astrophysical complex: methodics and results. Proceedings of Science. 2024 сент. 27;444:685. doi: 10.22323/1.444.0685

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BibTeX

@article{165b1a4ab7c14c6b9cf27a5e5d4edfb6,
title = "Hybrid method for study multi TeV gamma rays in the TAIGA astrophysical complex: methodics and results",
abstract = "The TAIGA astrophysical complex includes now 3 IACTs at the distance 300-500 m between each other and 1 km2 area wide-angle timing array TAIGA-HiSCORE. At energies above 40 TeV, a hybrid approach to the detection of gamma-rays becomes possible - the detection of EAS by both IACTs and the TAIGA-HiSCORE installation. The main advantage of the joint operation of the IACTs and timing array HiSCORE is a good gamma/hadron separation by image parameters information, and core position, direction and energy reconstruction by the timing array data. In this paper the following topics of a hybrid method are discussed: data processing and analysis, a comparison experimental results with Monte-Carlo simulations, selection of the first events with the energy more than 100 TeV from Crab Nebula in 250 hours of observation. The data were taken during the period of installation deployment, with one IACT in operation and half of the area of TAIGA-HiSCORE installation.",
author = "{the TAIGA Collaboration} and Elshoukrofy, {A. Sh.M} and E. Okuneva and L. Sveshnikova and I. Astapov and Bezyazeekov, {P. A.} and Blinov, {A. E.} and Bonvech, {E. A.} and A. Borodin and Budnev, {N. M.} and A. Bulan and A. Chiavassa and Chernov, {D. V.} and Dyachok, {A. N.} and Gafarov, {A. R.} and A. Garmash and V. Grebenyuk and O. Gress and E. Gress and Gress, {T. I.} and A. Grinyuk and O. Grishin and A. Ivanova and M. Ilushin and N. Kalmykov and V. Kindin and S. Kiryuhin and R. Kokoulin and N. Kolosov and K. Kompaniets and E. Korosteleva and Kozhin, {V. A.} and E. Kravchenko and A. Kryukov and L. Kuzmichev and A. Lagutin and M. Lavrova and Lemeshev, {Y. E.} and B. Lubsandorzhiev and N. Lubsandorzhiev and S. Malakhov and Mirgazov, {R. R.} and R. Monkhoev and E. Osipova and A. Pakhorukov and A. Pan and L. Pankov and A. Panov and G. Rubtsov and V. Samoliga and A. Sokolov and Арун Вайдянатан",
note = "The work was carried out at the UNU “Astrophysical Complex of MSU-IGU”, supported by the Ministry of Education and Science of Russia (EB agreement-075-15-2021-675,Topics of the state assignment (FZZE-2020-0017, FZZE-2020-0024, FSUS-2020-0039) and the Russian Science Foundation (project No. 23-72-00019 (section 3,4,5)). Публикация для корректировки.; 38th International Cosmic Ray Conference, ICRC 2023 ; Conference date: 26-07-2023 Through 03-08-2023",
year = "2024",
month = sep,
day = "27",
doi = "10.22323/1.444.0685",
language = "English",
volume = "444",
journal = "Proceedings of Science",
issn = "1824-8039",
publisher = "Sissa Medialab Srl",

}

RIS

TY - JOUR

T1 - Hybrid method for study multi TeV gamma rays in the TAIGA astrophysical complex: methodics and results

AU - the TAIGA Collaboration

AU - Elshoukrofy, A. Sh.M

AU - Okuneva, E.

AU - Sveshnikova, L.

AU - Astapov, I.

AU - Bezyazeekov, P. A.

AU - Blinov, A. E.

AU - Bonvech, E. A.

AU - Borodin, A.

AU - Budnev, N. M.

AU - Bulan, A.

AU - Chiavassa, A.

AU - Chernov, D. V.

AU - Dyachok, A. N.

AU - Gafarov, A. R.

AU - Garmash, A.

AU - Grebenyuk, V.

AU - Gress, O.

AU - Gress, E.

AU - Gress, T. I.

AU - Grinyuk, A.

AU - Grishin, O.

AU - Ivanova, A.

AU - Ilushin, M.

AU - Kalmykov, N.

AU - Kindin, V.

AU - Kiryuhin, S.

AU - Kokoulin, R.

AU - Kolosov, N.

AU - Kompaniets, K.

AU - Korosteleva, E.

AU - Kozhin, V. A.

AU - Kravchenko, E.

AU - Kryukov, A.

AU - Kuzmichev, L.

AU - Lagutin, A.

AU - Lavrova, M.

AU - Lemeshev, Y. E.

AU - Lubsandorzhiev, B.

AU - Lubsandorzhiev, N.

AU - Malakhov, S.

AU - Mirgazov, R. R.

AU - Monkhoev, R.

AU - Osipova, E.

AU - Pakhorukov, A.

AU - Pan, A.

AU - Pankov, L.

AU - Panov, A.

AU - Rubtsov, G.

AU - Samoliga, V.

AU - Sokolov, A.

AU - Вайдянатан, Арун

N1 - Conference code: 38

PY - 2024/9/27

Y1 - 2024/9/27

N2 - The TAIGA astrophysical complex includes now 3 IACTs at the distance 300-500 m between each other and 1 km2 area wide-angle timing array TAIGA-HiSCORE. At energies above 40 TeV, a hybrid approach to the detection of gamma-rays becomes possible - the detection of EAS by both IACTs and the TAIGA-HiSCORE installation. The main advantage of the joint operation of the IACTs and timing array HiSCORE is a good gamma/hadron separation by image parameters information, and core position, direction and energy reconstruction by the timing array data. In this paper the following topics of a hybrid method are discussed: data processing and analysis, a comparison experimental results with Monte-Carlo simulations, selection of the first events with the energy more than 100 TeV from Crab Nebula in 250 hours of observation. The data were taken during the period of installation deployment, with one IACT in operation and half of the area of TAIGA-HiSCORE installation.

AB - The TAIGA astrophysical complex includes now 3 IACTs at the distance 300-500 m between each other and 1 km2 area wide-angle timing array TAIGA-HiSCORE. At energies above 40 TeV, a hybrid approach to the detection of gamma-rays becomes possible - the detection of EAS by both IACTs and the TAIGA-HiSCORE installation. The main advantage of the joint operation of the IACTs and timing array HiSCORE is a good gamma/hadron separation by image parameters information, and core position, direction and energy reconstruction by the timing array data. In this paper the following topics of a hybrid method are discussed: data processing and analysis, a comparison experimental results with Monte-Carlo simulations, selection of the first events with the energy more than 100 TeV from Crab Nebula in 250 hours of observation. The data were taken during the period of installation deployment, with one IACT in operation and half of the area of TAIGA-HiSCORE installation.

UR - https://www.scopus.com/record/display.uri?eid=2-s2.0-85212268534&origin=inward&txGid=e7e471cebe9ecc62c27ca3ee49ddecdc

UR - https://www.mendeley.com/catalogue/93cb9f6b-6e13-365f-9761-e5c042f07e82/

U2 - 10.22323/1.444.0685

DO - 10.22323/1.444.0685

M3 - Conference article

VL - 444

JO - Proceedings of Science

JF - Proceedings of Science

SN - 1824-8039

M1 - 685

T2 - 38th International Cosmic Ray Conference

Y2 - 26 July 2023 through 3 August 2023

ER -

ID: 62699210