  The CCD observations for the W UMa type binary systems GSC 2362-2866 and GSC
107-596 have been analyzed using the Wilson-Devinney Code to determine their
photometric orbital and physical parameters. The results show that both systems
may be classified as A-subtype of W-UMa eclipsing binary. The mass ratio of GSC
2362-2866 is found to be q = 0.73, with an over-contact degree of f = 0.122%.
While the mass ratio of the system GSC 107-596 is found to be q = 0.70 with an
over-contact degree of f = 0.166% in V_band and q = 0.69 and f = 0.111% in R
band
