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Period Variation Study and Light Curve Analysis of the Eclipsing Binary GSC 02013-00288

given by Hanna and Awadalla [ 11 ]. Fig. 3 The best match between the synthetic light curves and the observed light curves of binary IK Boo. The rectangle shows a hump like distortion in all the LCs. 3 Light curve analysis The observed light curves of IK Boo indicate typical short period (7 h . 27) W UMa eclipsing binary with narrow minima and broad maxima. To find the geometrical and physical parameters for the system, we proceed to solve the light curves simultaneously using the software PHOEBE (Prša and Zwitter [ 19 ]). First, we have to

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