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TAIGA—A hybrid array for high energy gamma-ray astronomy and cosmic-ray physics. / the TAIGA Collaboration.

In: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Vol. 1039, 167047, 11.09.2022.

Research output: Contribution to journalArticlepeer-review

Harvard

the TAIGA Collaboration 2022, 'TAIGA—A hybrid array for high energy gamma-ray astronomy and cosmic-ray physics', Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 1039, 167047. https://doi.org/10.1016/j.nima.2022.167047

APA

the TAIGA Collaboration (2022). TAIGA—A hybrid array for high energy gamma-ray astronomy and cosmic-ray physics. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 1039, [167047]. https://doi.org/10.1016/j.nima.2022.167047

Vancouver

the TAIGA Collaboration. TAIGA—A hybrid array for high energy gamma-ray astronomy and cosmic-ray physics. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 2022 Sept 11;1039:167047. doi: 10.1016/j.nima.2022.167047

Author

the TAIGA Collaboration. / TAIGA—A hybrid array for high energy gamma-ray astronomy and cosmic-ray physics. In: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 2022 ; Vol. 1039.

BibTeX

@article{1f4f2ba0cc854646963fabbb3094254c,
title = "TAIGA—A hybrid array for high energy gamma-ray astronomy and cosmic-ray physics",
abstract = "The concept of the TAIGA experiment is to combine wide-angle timing and imaging Cherenkov telescopes as well as electron and muon detectors. The TAIGA facility aims at gamma-ray astrophysics at energies from a few TeV to several PeV and cosmic-ray physics from 100 TeV to several EeV but also pursues searches for astrophysical nanosecond transients, axion-like particles, Lorentz invariance violation and other unexpected manifestations of New Physics. TAIGA-1, a hybrid detector complex with an area of 1 km2, operating since 2021 in the Tunka valley, 50 km to the West from the southernmost tip of lake Baikal, and the plans for its upgrade are presented.",
keywords = "Cosmic ray, Gamma astronomy, Imaging TAIGA-IACT array, Timing TAIGA-HiSCORE array",
author = "{the TAIGA Collaboration} and N. Budnev and I. Astapov and P. Bezyazeekov and E. Bonvech and A. Borodin and A. Bulan and A. Chiavassa and D. Chernov and A. Dyachok and A. Gafarov and A. Garmash and V. Grebenyuk and O. Gress and E. Gress and T. Gress and A. Grinyuk and O. Grishin and Ivanova, {A. D.} and Ivanova, {A. L.} and N. Kalmykov and V. Kindin and S. Kiryuhin and R. Kokoulin and K. Komponiets 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 A. Lukanov and D. Lukyantsev and S. Malakhov and R. Mirgazov and R. Monkhoev and E. Okuneva and E. Osipova and A. Pakhorukov and A. Pan and L. Panasenko and L. Pankov and Panov, {A. D.} and A. Petrukhin and I. Poddubny and A. Sokolov and A. Vaidyanathan",
note = "Funding Information: The work was performed at the UNU “Astrophysical Complex of MSU-ISU” (agreement 13.UNU.21.0007). The work is supported by the Russian Foundation for Basic Research (grants 19-52-44002 , 19-32-60003 ), the Russian Science Foundation (grant 19-72-20067 (Section 2), and the Russian Federation Ministry of Science and High Education (projects FZZE-2020-0017 , FZZE-2020-0024 ). Publisher Copyright: {\textcopyright} 2022 Elsevier B.V.",
year = "2022",
month = sep,
day = "11",
doi = "10.1016/j.nima.2022.167047",
language = "English",
volume = "1039",
journal = "Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment",
issn = "0168-9002",
publisher = "Elsevier Science B.V.",

}

RIS

TY - JOUR

T1 - TAIGA—A hybrid array for high energy gamma-ray astronomy and cosmic-ray physics

AU - the TAIGA Collaboration

AU - Budnev, N.

AU - Astapov, I.

AU - Bezyazeekov, P.

AU - Bonvech, E.

AU - Borodin, A.

AU - Bulan, A.

AU - Chiavassa, A.

AU - Chernov, D.

AU - Dyachok, A.

AU - Gafarov, A.

AU - Garmash, A.

AU - Grebenyuk, V.

AU - Gress, O.

AU - Gress, E.

AU - Gress, T.

AU - Grinyuk, A.

AU - Grishin, O.

AU - Ivanova, A. D.

AU - Ivanova, A. L.

AU - Kalmykov, N.

AU - Kindin, V.

AU - Kiryuhin, S.

AU - Kokoulin, R.

AU - Komponiets, 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 - Lukanov, A.

AU - Lukyantsev, D.

AU - Malakhov, S.

AU - Mirgazov, R.

AU - Monkhoev, R.

AU - Okuneva, E.

AU - Osipova, E.

AU - Pakhorukov, A.

AU - Pan, A.

AU - Panasenko, L.

AU - Pankov, L.

AU - Panov, A. D.

AU - Petrukhin, A.

AU - Poddubny, I.

AU - Sokolov, A.

AU - Vaidyanathan, A.

N1 - Funding Information: The work was performed at the UNU “Astrophysical Complex of MSU-ISU” (agreement 13.UNU.21.0007). The work is supported by the Russian Foundation for Basic Research (grants 19-52-44002 , 19-32-60003 ), the Russian Science Foundation (grant 19-72-20067 (Section 2), and the Russian Federation Ministry of Science and High Education (projects FZZE-2020-0017 , FZZE-2020-0024 ). Publisher Copyright: © 2022 Elsevier B.V.

PY - 2022/9/11

Y1 - 2022/9/11

N2 - The concept of the TAIGA experiment is to combine wide-angle timing and imaging Cherenkov telescopes as well as electron and muon detectors. The TAIGA facility aims at gamma-ray astrophysics at energies from a few TeV to several PeV and cosmic-ray physics from 100 TeV to several EeV but also pursues searches for astrophysical nanosecond transients, axion-like particles, Lorentz invariance violation and other unexpected manifestations of New Physics. TAIGA-1, a hybrid detector complex with an area of 1 km2, operating since 2021 in the Tunka valley, 50 km to the West from the southernmost tip of lake Baikal, and the plans for its upgrade are presented.

AB - The concept of the TAIGA experiment is to combine wide-angle timing and imaging Cherenkov telescopes as well as electron and muon detectors. The TAIGA facility aims at gamma-ray astrophysics at energies from a few TeV to several PeV and cosmic-ray physics from 100 TeV to several EeV but also pursues searches for astrophysical nanosecond transients, axion-like particles, Lorentz invariance violation and other unexpected manifestations of New Physics. TAIGA-1, a hybrid detector complex with an area of 1 km2, operating since 2021 in the Tunka valley, 50 km to the West from the southernmost tip of lake Baikal, and the plans for its upgrade are presented.

KW - Cosmic ray

KW - Gamma astronomy

KW - Imaging TAIGA-IACT array

KW - Timing TAIGA-HiSCORE array

UR - http://www.scopus.com/inward/record.url?scp=85133180042&partnerID=8YFLogxK

U2 - 10.1016/j.nima.2022.167047

DO - 10.1016/j.nima.2022.167047

M3 - Article

AN - SCOPUS:85133180042

VL - 1039

JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

SN - 0168-9002

M1 - 167047

ER -

ID: 36525912