Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991izssr..55..737a&link_type=abstract
(Vsesoiuznaia Konferentsiia po Kosmicheskim Lucham, Dagomys, USSR, Nov. 1-3, 1990) Akademiia Nauk SSSR, Izvestiia, Seriia Fizich
Astronomy and Astrophysics
Astronomy
Cerenkov Counters, Flux Density, Gamma Rays, Quantum Counters, Gamma Ray Astronomy, Particle Energy, Photomultiplier Tubes, Primary Cosmic Rays
Scientific paper
The design and performance characteristics of an experimental installation for the detection of discrete gamma quanta sources in the energy range 10 to the 12th - 10 to the 13th eV, now being constructed in Tien Shan, are examined. Estimates of the efficiency of gamma quanta detection indicate that the minimum detectable flux for energies of 10 to the 13th eV and greater will be 10 to the -13th/cm s sr, exceeding the background of primary protons and nuclei by five standard deviations.
Akopian A. M.
Anokhina A. M.
Antonov Andrey Radoslavov
Galkin Vladimir I.
Golynskaia R. M.
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