Photometric Analysis of the Exoplanet Containing System Kepler-491

In this study, we present solutions of the transit light curves of the recently discovered planet Kepler-491h observed by Kepler space-telescope within a span of four years. In order to obtain stellar, planetary and orbital properties, WINFITTER code was applied to light curve data available at the NASA Exoplanet Archive (NEA). We also searched for significant signals at the transit timing variation (TIV).