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Budnev, N.M.; Chiavassa, A.; Gress, O.A.; Gress, T.I.; Dyachok, A.N.; Karpov, N.I.; Kalmykov, N.N.; Korosteleva, E.E.; Kozhin, V.A.; Kuzmichev, L.A.; Lubsandorzhiev, B.K.; Lubsandorzhiev, N.B.; Mirgazov, R.R.; Osipova, E.A.; Panasyuk, M.I.; Pankov, L.V.; Popova, E.G.; Prosin, V.V.; Ptuskin, V.S.; Semeney, Yu.A.; Silaev, A.A.; Silaev(junior), A.A.; Skurikhin, A.V.; Spiering, C.; Sveshnikova, L.G.; Zagorodnikov, A.V.
Astroparticle physics, January 2020, 2020-01-00, Volume: 117Journal Article
The EAS Cherenkov light array Tunka-133, with ~ 3 km2 geometric area, is taking data since 2009.The array permits a detailed study of energy spectrum and mass composition of cosmic rays in the energy range from 6 · 1015 to 1018 eV. We describe the methods of time and amplitude calibration of the array and the methods of EAS parameters reconstruction. We present the all-particle energy spectrum, based on 7 seasons of operation.
