Abstract
The observational data for the Galactic source Cygnus X-3 collected with the SHALON mirror Cherenkov telescope are presented. The Cygnus X-3 binary have been regularly observed since 1995 with the average γ-ray flux F (E > 0.8 TeV ) = (6.8 ± 0.7) × 10-13 cm -2 s -1. The flux in year 2003 was (1.79 ± 0.33) × 10-12 cm -2 s -1. Earlier, in 1997, an increase of the flux was also observed.
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