Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
TAIGA experiment : Present status and perspectives. / TAIGA Collaboration.
в: Journal of Instrumentation, Том 12, № 8, C08018, 16.08.2017.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - TAIGA experiment
T2 - Present status and perspectives
AU - the TAIGA Collaboration
AU - Budnev, N.
AU - Astapov, I.
AU - Bezyazeekov, P.
AU - Boreyko, V.
AU - Borodin, A.
AU - Brückner, M.
AU - Chiavassa, A.
AU - Gafarov, A.
AU - Grebenyuk, V.
AU - Gress, O.
AU - Gress, T.
AU - Grinyuk, A.
AU - Grishin, O.
AU - Dyachok, A.
AU - Fedorov, O.
AU - Haungs, A.
AU - Horns, D.
AU - Huege, T.
AU - Ivanova, A.
AU - Kalmykov, N.
AU - Kazarina, Y.
AU - Kindin, V.
AU - Kiryuhin, S.
AU - Kokoulin, R.
AU - Kompaniets, K.
AU - Kostunin, D.
AU - Korosteleva, E.
AU - Kozhin, V.
AU - Kravchenko, E.
AU - Kunnas, M.
AU - Kuzmichev, L.
AU - Lemeshev, Yu
AU - Lenok, V.
AU - Lubsandorzhiev, B.
AU - Lubsandorzhiev, N.
AU - Mirgazov, R.
AU - Mirzoyan, R.
AU - Monkhoev, R.
AU - Nachtigall, R.
AU - Osipova, E.
AU - Pakhorukov, A.
AU - Panasyuk, M.
AU - Pankov, L.
AU - Poleschuk, V.
AU - Popesku, M.
AU - Popova, E.
AU - Porelli, A.
AU - Postnikov, E.
AU - Prosin, V.
AU - Sokolov, A.
PY - 2017/8/16
Y1 - 2017/8/16
N2 - 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 . TAIGA will be located in the Tunka valley, ∼ 50 km West from Lake Baikal. The different detectors of the TAIGA will be grouped in 6 arrays to measure Cherenkov and radio emission as well as electron and muon components of atmospheric showers. The combination of the wide angle Cherenkov detectors of the TAIGA-HiSCORE array and the 4-m Imaging Atmospheric Cherenkov Telescopes of the TAIGA-IACT array with their FoV of 10×10 degrees and underground muon detectors offers a very cost effective way to construct a 5 km2 array for gamma-ray astronomy.
AB - 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 . TAIGA will be located in the Tunka valley, ∼ 50 km West from Lake Baikal. The different detectors of the TAIGA will be grouped in 6 arrays to measure Cherenkov and radio emission as well as electron and muon components of atmospheric showers. The combination of the wide angle Cherenkov detectors of the TAIGA-HiSCORE array and the 4-m Imaging Atmospheric Cherenkov Telescopes of the TAIGA-IACT array with their FoV of 10×10 degrees and underground muon detectors offers a very cost effective way to construct a 5 km2 array for gamma-ray astronomy.
KW - Cherenkov detectors
KW - Gamma telescopes
KW - Image processing
KW - HISCORE
KW - RAY
UR - http://www.scopus.com/inward/record.url?scp=85030996004&partnerID=8YFLogxK
U2 - 10.1088/1748-0221/12/08/C08018
DO - 10.1088/1748-0221/12/08/C08018
M3 - Article
AN - SCOPUS:85030996004
VL - 12
JO - Journal of Instrumentation
JF - Journal of Instrumentation
SN - 1748-0221
IS - 8
M1 - C08018
ER -
ID: 12669628