  We report an analysis of two poorly studied systems GSC 04396-00605 and GSC
04395-00485, which were recently named as V0455 Dra and V0454 Dra,
respectively. For two eclipsing stars, the periods and epochs were
significantly corrected using our extensive data. The phenomenological
characteristics of the mean light curves were determined using the "New Algol
Variable" (NAV) algorithm. The individual times of Maxima/Minima (ToM) were
determined using the newly developed software MAVKA, which outputs the accurate
parameters using the "asymptotic parabola" approximations. The light curves
were approximated using the Wilson-Devinney model, the best fit parameters are
listed. For both systems, the presence of the dark spot is justified, the
parameters are estimated. Both systems classified to be overcontact binaries of
EW type. The observations were obtained using the 1-m Korean telescope of the
LOAO while monitoring the cataclysmic variable DO Dra within the
"Inter-Longitude Astronomy" (ILA) project.
