A corrected energy dependence of the depth of the maximum in the wide range of energies 10$^{15}$ to 10$^{18}$ eV is obtained using data collected at the Tunka-133 facility over 7 years of operation (2009–2017) and the TAIGA-HiSCORE facility in the 2019–2020 season. At the highest energies, our results match those of the Pierre Auger observatory. The results are converted to parameter ❬ln A❭, which characterizes the mean EAS composition
Accepted for publication by PRLInternational audienceWe describe the measurement of the depth of max...
We describe the measurement of the depth of maximum, X{max}, of the longitudinal development of air ...
We describe the measurement of the depth of maximum, X(max), of the longitudinal development of air ...
The Tunka-133 Cherenkov complex for recording extensive air showers (EAS) collected data over seven ...
We present results of an improved analysis of the experimental data of the EAS Cherenkov array Tunka...
Data obtained with two detectors located at the Tunka Cosmic Ray facility are presented. The Cherenk...
We present results of an improved analysis of the experimental data of the EAS Cherenkov array Tunka...
The Cherenkov light array for the registration of extensive air showers (EAS) Tunka-133 collected da...
The EAS Cherenkov light array Tunka-133, with ~ 3 km 2 geometric area, is taking data since 2009.T...
The extensive air shower Cherenkov light array Tunka-133 collected data during 7 winter seasons from...
The corrected dependence of the mean depth of the EAS maximum $X_{max}$ on the energy was obtained f...
We present the main results of the Extensive Air Shower Cherenkov array Tunka-25. They cover the ene...
Accepted for publication by PRLInternational audienceWe describe the measurement of the depth of max...
We describe the measurement of the depth of maximum, X{max}, of the longitudinal development of air ...
We describe the measurement of the depth of maximum, X(max), of the longitudinal development of air ...
The Tunka-133 Cherenkov complex for recording extensive air showers (EAS) collected data over seven ...
We present results of an improved analysis of the experimental data of the EAS Cherenkov array Tunka...
Data obtained with two detectors located at the Tunka Cosmic Ray facility are presented. The Cherenk...
We present results of an improved analysis of the experimental data of the EAS Cherenkov array Tunka...
The Cherenkov light array for the registration of extensive air showers (EAS) Tunka-133 collected da...
The EAS Cherenkov light array Tunka-133, with ~ 3 km 2 geometric area, is taking data since 2009.T...
The extensive air shower Cherenkov light array Tunka-133 collected data during 7 winter seasons from...
The corrected dependence of the mean depth of the EAS maximum $X_{max}$ on the energy was obtained f...
We present the main results of the Extensive Air Shower Cherenkov array Tunka-25. They cover the ene...
Accepted for publication by PRLInternational audienceWe describe the measurement of the depth of max...
We describe the measurement of the depth of maximum, X{max}, of the longitudinal development of air ...
We describe the measurement of the depth of maximum, X(max), of the longitudinal development of air ...