Aktoka, U.Erdem, A.Ozturk, O.Surgit, D.2025-01-272025-01-272017978-0-7354-1483-90094-243Xhttps://doi.org/10.1063/1.4976434https://hdl.handle.net/20.500.12428/2554932nd International Physics Congress of Turkish-Physical-Society (TPS) -- SEP 06-09, 2016 -- Bodrum, TURKEYIn this study, SuperWASP light curves of V342 11cr and V387 Her were analyzed by means of the Wilson Devinney (W-D) code with a Monte Carlo (MC) search method for the first time. The final photometric solutions of these two systems show that while V342 Her has an over contact configuration in which both components overtlows their Roche limiting lobes, V387 Her has a detached configuration. Photometric mass ratios and approximate absolute parameters of the systems are obtained.eninfo:eu-repo/semantics/closedAccessPhysical ParametersComponentsSystemsStarsConference Object181510.1063/1.4976434N/AWOS:0004352051000902-s2.0-85016068220Q4