Research output: Contribution to journal › Article › peer-review
TAIGA—A hybrid array for high-energy gamma astronomy and cosmic-ray physics. / the TAIGA Collaboration ; Вайдянатан, Арун .
In: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Vol. 958, 162113, 01.04.2020.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - TAIGA—A hybrid array for high-energy gamma astronomy and cosmic-ray physics
AU - the TAIGA Collaboration
AU - Budnev, N.
AU - Astapov, I. I.
AU - Bezyazeekov, P. A.
AU - Borodin, A.
AU - Brückner, M.
AU - Chernykh, D.
AU - Chiavassa, A.
AU - Dyachok, A.
AU - Fedorov, O.
AU - Gafarov, A.
AU - Garmash, A.
AU - Grebenyuk, V.
AU - Gress, O.
AU - Gress, T.
AU - Grinyuk, A.
AU - Grishin, O.
AU - Horns, D.
AU - Ivanova, A.
AU - Kalmykov, N.
AU - Kazarina, Yu
AU - Kindin, V.
AU - Kiryuhin, S.
AU - Kokoulin, R.
AU - Komponiets, K.
AU - Korosteleva, E.
AU - Kostunin, D.
AU - Kozhin, V.
AU - Kravchenko, E.
AU - Kryukov, A.
AU - Kuzmichev, L.
AU - Lagutin, A.
AU - Lubsandorzhiev, B.
AU - Lubsandorzhiev, N.
AU - Mirgazov, R.
AU - Mirzoyan, R.
AU - Monkhoev, R.
AU - Osipova, E.
AU - Pakhorukov, A.
AU - Pan, A.
AU - Panasyuk, M.
AU - Pankov, L.
AU - Petrukhin, A.
AU - Poleschuk, V.
AU - Popesku, M.
AU - Popova, E.
AU - Porelli, A.
AU - Postnikov, E.
AU - Prosin, V.
AU - Rubtsov, G.
AU - Sokolov, A.
AU - Вайдянатан, Арун
N1 - Publisher Copyright: © 2019 Elsevier B.V. Copyright: Copyright 2019 Elsevier B.V., All rights reserved.
PY - 2020/4/1
Y1 - 2020/4/1
N2 - The combination of a wide angle timing Cherenkov array and Imaging Atmospheric Cherenkov Telescopes operated in mono mode offers a cost-effective way to construct a few square kilometers array for ultrahigh-energy gamma astronomy. The first stage of the TAIGA Observatory (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) is described here. It will comprise TAIGA-HiSCORE - 120 wide angle Cherenkov stations distributed over an area of 1.0 km 2 and three IACTs (TAIGA-IACT).
AB - The combination of a wide angle timing Cherenkov array and Imaging Atmospheric Cherenkov Telescopes operated in mono mode offers a cost-effective way to construct a few square kilometers array for ultrahigh-energy gamma astronomy. The first stage of the TAIGA Observatory (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) is described here. It will comprise TAIGA-HiSCORE - 120 wide angle Cherenkov stations distributed over an area of 1.0 km 2 and three IACTs (TAIGA-IACT).
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=85065524064&partnerID=8YFLogxK
U2 - 10.1016/j.nima.2019.04.067
DO - 10.1016/j.nima.2019.04.067
M3 - Article
AN - SCOPUS:85065524064
VL - 958
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 - 162113
ER -
ID: 20044561