Alicavus, Filiz KahramanSoydugan, Esin2025-01-272025-01-272014978-1-10704-517-01743-92131743-9221https://doi.org/10.1017/S1743921313014919https://hdl.handle.net/20.500.12428/27921301st Symposium of the International-Astronomical-Union -- AUG 19-23, 2013 -- Wroclaw, POLANDWe present frequency analysis of the Kepler light curve of KIC 10486425, an eclipsing binary system with a pulsating component. The parameters of the binary were obtained by modelling the light curve with the Wilson-Devinney program. The residuals from this modelling were subject to Fourier analysis which allowed us to detect 120 periodic terms characteristic for gamma Dor-type pulsations. The dominant frequency of these changes amounts to 1.3189 d(-1).eninfo:eu-repo/semantics/openAccessstars: binaries: eclipsingstars: variables: gamma Dorstars: individual: KIC 10486425Conference Object930143343410.1017/S1743921313014919N/AWOS:0004508070000912-s2.0-84894526771Q4