activity
20092024
most citedThe primary cosmic-ray energy spectrum measured with the Tunka-133 array

62 citations · 113 across the 8 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2024

Four years of wide-field search for nanosecond optical transients with the TAIGA-HiSCORE Cherenkov array

A. D. Panov, I. I. Astapov, G. M. Beskin +75

It has been previously demonstrated [Panov et al. Physics of Atomic Nuclei 84(2021)1037] that the TAIGA-HiSCORE Cherenkov array, originally built for cosmic ray physics and ultrahi…

astro-ph.IM2021★ 7 cited

Search for Astrophysical Nanosecond Optical Transients with TAIGA-HiSCORE Array

A. D. Panov, I. I. Astapov, A. K. Awad +81

A wide-angle Cerenkov array TAIGA-HiSCORE (FOV 0.6 sr), was originally created as a part of TAIGA installation for high-energy gamma-ray astronomy and cosmic ray physics. Arr…

astro-ph.HE2021★ 62 cited

The primary cosmic-ray energy spectrum measured with the Tunka-133 array

N. M. Budnev, A. Chiavassa, O. A. Gress +21

The EAS Cherenkov light array Tunka-133, with 3 km geometric area, is taking data since 2009.The array permits a detailed study of energy spectrum and mass composition o…

astro-ph.IM2019★ 4 cited

Tunka Advanced Instrument for cosmic rays and Gamma Astronomy

D. Kostunin, I. Astapov, P. Bezyazeekov +79

The paper is a script of a lecture given at the ISAPP-Baikal summer school in 2018. The lecture gives an overview of the Tunka Advanced Instrument for cosmic rays and Gamma Astrono…

physics.ed-ph2015★ 4 cited

Remote Access Mössbauer Spectrometry

A. A. Silaev, S. K. Godovikov, E. B. Postnikov +1

The authors' design for a Mössbauer spectroscopy unit accessed via the Internet is presented. The spectrometer's configuration, operational peculiarities, key specifications, and r…

astro-ph.HE2009★ 25 cited

The Cosmic Ray Mass Composition in the Energy Range 10^15 - 10^18 eV measured with the Tunka Array: Results and Perspectives

N. M. Budnev, O. A. Chvalaiev, O. A. Gress +21

The final analysis of the Extensive Air Shower (EAS) maximum X_max depth distribution derived from the data of Tunka-25 atmospheric Cherenkov light array in the energy range 3.10^1…