On the basis of the original photometric data, the light curves of several transits in the exoplanet system TrES-3 were simulated by Monte Carlo method. Using these curves, the estimates of precise values of mid-transit time were calculated to assess the possibility of finding new planets by timing method in already known exoplanet systems using ground-based observations at small telescopes. More accurate values of the some orbital and physical parameters of TrES-3 system were also obtained including following the planet-star radius ratio (R_P/R_*), the angle of the planet orbital plane inclination (i).