The corrected dependence of the mean depth of the EAS maximum Xmax on
the energy was obtained from the data of the Tunka-133 array for 7 years and
the TAIGA-HiSCORE array for 2 year. The parameter ⟨lnA⟩,
characterizing the mean mass compositon was derived from these results. The
differential energy spectrum of primary cosmic rays in the energy range of
2⋅1014 - 2⋅1016\,eV was reconstructed using the new
parameter Q100 the Cherenkov light flux at the core distance 100 m.}Comment: 6 pages, 3 figures, Submitted to SciPost Phys.Pro