Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
The TAIGA—a Hybrid Detector Complex in Tunka Valley for Astroparticle Physics, Cosmic Ray Physics and Gamma-Ray Astronomy. / TAIGA Collaboration ; Вайдянатан, Арун .
в: Physics of Atomic Nuclei, Том 86, № 4, 01.09.2023, стр. 471-477.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - The TAIGA—a Hybrid Detector Complex in Tunka Valley for Astroparticle Physics, Cosmic Ray Physics and Gamma-Ray Astronomy
AU - the TAIGA Collaboration
AU - Astapov, I.
AU - Bezyazeekov, P.
AU - Bonvech, E.
AU - Borodin, A.
AU - Budnev, N.
AU - Bulan, A.
AU - Chernov, D.
AU - Chiavassa, A.
AU - Dyachok, A.
AU - Gafarov, A.
AU - Garmash, A.
AU - Grebenyuk, V.
AU - Gress, E.
AU - Gress, O. A.
AU - Gress, T.
AU - Grinyuk, A.
AU - Grishin, O.
AU - Ivanova, A. D.
AU - Ivanova, A. L.
AU - Iliushin, M.
AU - Kalmykov, N.
AU - Kindin, V.
AU - Kiryuhin, S.
AU - Kokoulin, R.
AU - Kompaniets, K.
AU - Korosteleva, E.
AU - Kozhin, V.
AU - Kravchenko, E.
AU - Kryukov, A.
AU - Kuzmichev, L.
AU - Lagutin, A.
AU - Lavrova, M.
AU - Lemeshev, Y.
AU - Lubsandorzhiev, B.
AU - Lubsandorzhiev, N.
AU - Malakhov, S.
AU - Mirgazov, R.
AU - Monkhoev, R.
AU - Okuneva, E.
AU - Osipova, E.
AU - Pakhorukov, A.
AU - Pankov, L.
AU - Pan, A.
AU - Panov, A.
AU - Petrukhin, A.
AU - Podgrudkov, D.
AU - Popova, E.
AU - Postnikov, E.
AU - Sokolov, A.
AU - Вайдянатан, Арун
N1 - The work was performed at the UNU “Astrophysical Complex of MSU-ISU” (agreement EB 075-15-2021-675). The work is supported the Russian Science Foundation (grant 23-72-00016 (Section 3), 23-72-00019 (Section 4), by the Russian Federation Ministry of Science and High Education (projects 23-72-00016, FZZE-2023-0004, FSUS2020-0039, FSUS-2022-0015), Federal academic leadership program Priority-2030).
PY - 2023/9/1
Y1 - 2023/9/1
N2 - Abstract: The physical motivations and performance of the TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) project are presented. The TAIGA observatory addresses ground-based gamma-ray astronomy at energies from a few TeV to several PeV, as well as cosmic ray physics from 100 TeV to several EeV and astroparticle physics. The pilot TAIGA-1 complex locates in the Tunka valley, km West from the southern tip of the lake Baikal. It includes integrated air Cherenkov TAIGA-HiSCORE array with 120 wide-angle optical stations distributed over on area 1.1 square kilometer about and three 4-m class Imaging Atmospheric Cherenkov Telescopes of the TAIGA-IACT array. The latter array has a shape of triangle with side lengths of about 300, 400 and 500 m. The integral sensitivity of the 1-km TAIGA-1 detector is about TeV cm s for detection of TeV gamma-rays in 300 hours of source observations. The combination of the wide-angle Cherenkov array and IACTs could offer a cost effective-way to build a large (up to 10 km) array for very high energy gamma-ray astronomy. The reconstruction of a given EAS energy, incoming direction, and the core position, based on the TAIGA-HiSCORE data, allows one to increase the distance between the relatively expensive IACTs up to 600–800 m. These, together with the surface and underground electron/Muon detectors, will be used for selection of gamma-ray-induced EAS. Present status of the project, together with the current array description, the first experimental results and plans for the future are reported.
AB - Abstract: The physical motivations and performance of the TAIGA (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) project are presented. The TAIGA observatory addresses ground-based gamma-ray astronomy at energies from a few TeV to several PeV, as well as cosmic ray physics from 100 TeV to several EeV and astroparticle physics. The pilot TAIGA-1 complex locates in the Tunka valley, km West from the southern tip of the lake Baikal. It includes integrated air Cherenkov TAIGA-HiSCORE array with 120 wide-angle optical stations distributed over on area 1.1 square kilometer about and three 4-m class Imaging Atmospheric Cherenkov Telescopes of the TAIGA-IACT array. The latter array has a shape of triangle with side lengths of about 300, 400 and 500 m. The integral sensitivity of the 1-km TAIGA-1 detector is about TeV cm s for detection of TeV gamma-rays in 300 hours of source observations. The combination of the wide-angle Cherenkov array and IACTs could offer a cost effective-way to build a large (up to 10 km) array for very high energy gamma-ray astronomy. The reconstruction of a given EAS energy, incoming direction, and the core position, based on the TAIGA-HiSCORE data, allows one to increase the distance between the relatively expensive IACTs up to 600–800 m. These, together with the surface and underground electron/Muon detectors, will be used for selection of gamma-ray-induced EAS. Present status of the project, together with the current array description, the first experimental results and plans for the future are reported.
UR - https://www.mendeley.com/catalogue/74f3238e-38a5-360a-b66e-b03cda6c8f0c/
U2 - 10.1134/S1063778823040051
DO - 10.1134/S1063778823040051
M3 - Article
VL - 86
SP - 471
EP - 477
JO - Physics of Atomic Nuclei
JF - Physics of Atomic Nuclei
SN - 1063-7788
IS - 4
ER -
ID: 60225186