  We present the first photometric analysis for the newly discovered eclipsing
binary systems of Algole-type GSC 2750-0054 and GSC 03208-02644. Our analysis
was carried out by means of the most recent version of Wilson Devinney (WD)
code, which applies the model atmosphere by Kurucz (1993) with prescription in
pass band for the radiative treatment. The accepted light curve solutions
reveal absolute physical parameters and the spectral classifications for the
components are adopted. Distance to each system was calculated based on the
parameters of the accepted photometric solutions. Comparison with the
evolutionary models are presented.
