The Primary CR Spectrum by the Data of the Tunka-133 Array

S.F. Berezhnev1, N.M. Budnev2, A. Chiavassa4 , O.A. Chvalaev2, O.A. Gress2, T.I. Gress2, A.N. Dyachok2, S.N. Epimakhov6, N.I. Karpov1, N.N. Kalmykov1, E.N. Konstantinov2, A.V. Korobchenko2, E.E. Korosteleva1, V.A. Kozhin1, L.A. Kuzmichev1,2, B.K. Lubsandorzhiev3, N.B. Lubsandorzhiev1, R.R. Mirgazov2, R.D. Monkhoev2, E.A. Osipova1, A.L. Pakhorukov2, M.I. Panasyuk1, L.V. Pankov2, E.G. Popova1, V.V. Prosin1, V.S. Ptuskin7, Yu.A. Semeney2, A.A. Silaev1, A.A. Silaev(junior)1, A.V. Skurikhin1, C. Spiering5, L.G. Sveshnikova1, A.V. Zagorodnikov2

[1]  A. V. Korobchenko,et al.  Tunka-133: Results of 3 year operation , 2014 .

[2]  C. Spiering,et al.  Tunka-25 Air Shower Cherenkov array: The main results , 2013 .

[3]  N. Budnev,et al.  Tunka-Rex: Status and results of the first measurements , 2013, 1310.8477.

[4]  P. O. Hulth,et al.  Measurement of the cosmic ray energy spectrum with IceTop-73 , 2013 .

[5]  Yasuhiro H. Takahashi,et al.  The energy spectrum of ultra-high-energy cosmic rays measured by the Telescope Array FADC fluorescence detectors in monocular mode , 2013 .

[6]  H. J. Gils,et al.  The spectrum of high-energy cosmic rays measured with KASCADE-Grande , 2012, 1308.1485.

[7]  N. M. Budnev,et al.  The Tunka-133 EAS Cherenkov light array: status of 2011 , 2012, 1201.2122.

[8]  F. T. Collaboration,et al.  Final Results from the High solution Flyʼs Eye (HiRes) Experiment , 2010, 1010.2690.

[9]  S. Ter-Antonyan,et al.  An all-particle primary energy spectrum in the 3–200 PeV energy range , 2008, 0808.1421.

[10]  et al,et al.  The All-Particle Spectrum of Primary Cosmic Rays in the Wide Energy Range from 1014 to 1017 eV Observed with the Tibet-III Air-Shower Array , 2008, 0801.1803.

[11]  E. Korosteleva,et al.  Measurement of Cosmic Ray Primary Energy with the Atmospheric Cherenkov Light Technique in Extensive Air Showers , 2007 .

[12]  E. Korosteleva,et al.  PRIMARY ENERGY MEASUREMENT WITH EAS CHERENKOV LIGHT: EXPERIMENT QUEST AND CORSIKA SIMULATION , 2005 .

[13]  Huang,et al.  Evidence for changing of cosmic ray composition between 10(17) and 10(18) eV from multicomponent measurements , 2000, Physical review letters.

[14]  Pietro Antonioli,et al.  The EAS size spectrum and the cosmic ray energy spectrum in the region 1015–1016 eV , 1999 .