Ozalp, G. Z.Ozkardes, B.2025-01-272025-01-272016978-0-7354-1369-60094-243Xhttps://doi.org/10.1063/1.4944138https://hdl.handle.net/20.500.12428/266449th International Physics Conference of the Balkan-Physical-Union (BPU) -- AUG 24-27, 2015 -- Istanbul Univ, Beyazit Campus, Istanbul, TURKEYWe present the photometric solution of the eclipsing binary ET Psc (GSC 00608-00490). The ASAS V-band photometric data of the system was modelled using the Wilson-Devinney method. The result shows that the eclipsing pair could be classified as A-subtype of W UMa-type binary system. The absolute dimensions of the system were also estimated based on the photometric solution.eninfo:eu-repo/semantics/closedAccessSky Automated SurveyLimb-Darkening CoefficientsVariable-StarsCatalogConference Object172210.1063/1.4944138N/AWOS:0003759233000192-s2.0-84984537194Q4