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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 изданияхстатьяРецензирование

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TAIGA Collaboration, Вайдянатан А. The TAIGA—a Hybrid Detector Complex in Tunka Valley for Astroparticle Physics, Cosmic Ray Physics and Gamma-Ray Astronomy. Physics of Atomic Nuclei. 2023 сент. 1;86(4):471-477. doi: 10.1134/S1063778823040051

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BibTeX

@article{47d14861ad8f4f6b8cf882b797c4ac76,
title = "The TAIGA—a Hybrid Detector Complex in Tunka Valley for Astroparticle Physics, Cosmic Ray Physics and Gamma-Ray Astronomy",
abstract = "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.",
author = "{the TAIGA Collaboration} and I. Astapov and P. Bezyazeekov and E. Bonvech and A. Borodin and N. Budnev and A. Bulan and D. Chernov and A. Chiavassa and A. Dyachok and A. Gafarov and A. Garmash and V. Grebenyuk and E. Gress and Gress, {O. A.} and T. Gress and A. Grinyuk and O. Grishin and Ivanova, {A. D.} and Ivanova, {A. L.} and M. Iliushin and N. Kalmykov and V. Kindin and S. Kiryuhin and R. Kokoulin and K. Kompaniets and E. Korosteleva and V. Kozhin and E. Kravchenko and A. Kryukov and L. Kuzmichev and A. Lagutin and M. Lavrova and Y. Lemeshev and B. Lubsandorzhiev and N. Lubsandorzhiev and S. Malakhov and R. Mirgazov and R. Monkhoev and E. Okuneva and E. Osipova and A. Pakhorukov and L. Pankov and A. Pan and A. Panov and A. Petrukhin and D. Podgrudkov and E. Popova and E. Postnikov and A. Sokolov and Арун Вайдянатан",
note = "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).",
year = "2023",
month = sep,
day = "1",
doi = "10.1134/S1063778823040051",
language = "English",
volume = "86",
pages = "471--477",
journal = "Physics of Atomic Nuclei",
issn = "1063-7788",
publisher = "Maik Nauka-Interperiodica Publishing",
number = "4",

}

RIS

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