Primary CR energy spectrum and mass composition by the data of Tunka-133 array
- Prosin V.V.
- Berezhnev S.F.
- Budnev N.M.
- Chiavassa A.
- Chvalaev O.A.
- Dyachok A.V.
- Epimakhov S.N.
- Gress O.A.
- Gress T.I.
- Kalmykov N.N.
- Karpov N.I.
- Konstantinov E.N.
- Korobchenko A.V.
- Korosteleva E.E.
- Kozhin V.A.
- Kuzmichev L.A.
- Lubsandorzhiev B.K.
- Lubsandorzhiev N.B.
- Mirgazov R.R.
- Monkhoev R.D.
- Osipova E.A.
- Pakhorukov A.L.
- Panasyuk M.I.
- Pankov L.V.
- Popova E.G.
- Ptuskin V.S.
- Semeney Y.A.
- Silaev A.A.
- (jun.) A.A. Silaev
- Skurikhin A.V.
- Spiering C.
- Sveshnikova L.G.
- Zagorodnikov A.V.
DOIAbstract
The Cherenkov light array for the registration of extensive air showers (EAS) Tunka-133 collected data during 5 winter seasons from 2009 to 2014. The differential energy spectrum of all particles and the dependence of the average maximum depth on the energy in the range of 6 ⋅ 1015–1018 eV measured for 1540 hours of observation are presented
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