53 citations · 76 across the 9 of their papers we have counts for
10 papers
Wide-field search for submicrosecond optical and gamma transients as manifestation of primordial black holes evaporation with the TAIGA-HiSCORE Cherenkov array
I. I. Astapov, G. M. Beskin, P. A. Bezyazykov +70
We demonstrated in our papers [Panov, 2021; Panov,2025), that the TAIGA-HiSCORE Cherenkov array physics, originally designed for research in cosmic rays and ultra-high-energy gamma…
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…
TAIGA -- an advanced hybrid detector complex for astroparticle physics and high energy gamma-ray astronomy
N. M. Budnev, I. Astapov, P. Bezyazeekov +74
The physical motivations, present status, main results in study of cosmic rays and in the field of gamma-ray astronomy as well future plans of the TAIGA-1 (Tunka Advanced Instrumen…
Primary Cosmic Rays Energy Spectrum and Mean Mass Composition by the Data of the TAIGA Astrophysical Complex
V. Prosin, I. Astapov, P. Bezyazeekov +78
The corrected dependence of the mean depth of the EAS maximum on the energy was obtained from the data of the Tunka-133 array for 7 years and the TAIGA-HiSCORE array for…
The Tunka-Grande scintillation array: current results
A. L. Ivanova, I. Astapov, P. Bezyazeekov +76
The Tunka-Grande experiment is a scintillation array with about 0.5 sq.km sensitive area at Tunka Valley, Siberia, for measuring charged particles and muons in extensive air shower…
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…
Energy spectra of abundant cosmic-ray nuclei in the NUCLEON experiment
Nikolay Gorbunov, Viktor Grebenyuk, Dmitrii Karmanov +12
The NUCLEON satellite experiment is designed to directly investigate the energy spectra of cosmic-ray nuclei and the chemical composition (Z=1-30) in the energy range of 2-500 TeV.…
Hybrid method for identifying mass groups of primary cosmic rays in the joint operation of IACTs and wide angle Cherenkov timing arrays
E. B. Postnikov, A. A. Grinyuk, L. A. Kuzmichev +1
This work is a methodical study of another option of the hybrid method originally aimed at gamma/hadron separation in the TAIGA experiment. In the present paper this technique was…
Background rejection method for tens of TeV gamma-ray astronomy applicable to wide angle timing arrays
A. Sh. M. Elshoukrofy, E. B. Postnikov, L. G. Sveshnikova
A 'knee-like' approximation of Cherenkov light Lateral Distribution Functions, which we developed earlier, now is used for the actual tasks of background rejection methods for high…
First results of the cosmic ray NUCLEON experiment
E. Atkin, V. Bulatov, V. Dorokhov +19
The NUCLEON experiment was designed to study the chemical composition and energy spectra of galactic cosmic ray nuclei from protons to zinc at energies of --\…