Possibilities for observing gamma quanta from local sources by Shalon-Alatu Cerenkov mirror telescopes

Details Possibilities for observing gamma quanta from local sources by Shalon-Alatu Cerenkov mirror telescopes Possibilities for observing gamma quanta from local sources by Shalon-Alatu Cerenkov mirror telescopes

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993roizf..57..174a&link_type=abstract

Rossijskaya Akademiya Nauk, Izvestiya, Seriya Fizicheskaya (ISSN 0367-6765), vol. 57, no. 4, p. 174-176.

Astronomy and Astrophysics

Astronomy

Cerenkov Counters, Cosmic Ray Showers, Electron Photon Cascades, Gamma Ray Astronomy, Gamma Ray Telescopes, Monte Carlo Method

Scientific paper

The Shalon-Alatu Cerenkov telescope complex built in Tien Shan for gamma astronomy studies in the quanta energy range 1-30 TeV is briefly described. Particular attention is given to the calibration of the telescope sensitivity. For the Shalon experiment, a Monte Carlo simulation of electron-photon cascades in the atmosphere has been carried out for proton and gamma showers with energies of 1 TeV.

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