  Multi band photometry and light curve analysis for two newly recognized
contact binary systems, TYC 6995-813-1 and NSVS 13602901 are presented. Both
were found to be of extreme low mass ratios 0.11 and 0.17, respectively. The
secondary components of both systems show evidence of considerable evolution
with elevated densities as well as both luminosity and radii well above their
main sequence counterparts. Even in the absence of significant spot activity at
least one of the systems, TYC 6995-813-1, shows features of magnetic and
chromospheric activity. TYC 6995-813-1 is also determined to be a potential
merger candidate with its current separation near the theoretical instability
separation.
