Workshop on Solar and Stellar Physics through Eclipses, Antalya, Turkey, 27 - 29 March 2006, vol.370, pp.213-214
First complete BVRI light curves and radial velocity measurements of the recently discovered eclipsing binary GSC 4288 0186 are presented. Analyses of the light curves, together with spectroscopic data show that the system is a double-lined detached binary with an eccentric orbit. We determined the preliminary values of the absolute elements of this eclipsing binary and presented here.