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We report an analysis of two poorly studied systems GSC 04396-00605 and GSC04395-00485, which were recently named as V0455 Dra and V0454 Dra,respectively. For two eclipsing stars, the periods and epochs weresignificantly corrected using our extensive data. The phenomenologicalcharacteristics of the mean light curves were determined using the "New AlgolVariable" (NAV) algorithm. The individual times of Maxima/Minima (ToM) weredetermined using the newly developed software MAVKA, which outputs the accurateparameters using the "asymptotic parabola" approximations. The light curveswere approximated using the Wilson-Devinney model, the best fit parameters arelisted. For both systems, the presence of the dark spot is justified, theparameters are estimated. Both systems classified to be overcontact binaries ofEW type. The observations were obtained using the 1-m Korean telescope of theLOAO while monitoring the cataclysmic variable DO Dra within the"Inter-Longitude Astronomy" (ILA) project.

Poorly Studied Eclipsing Binaries in the Field of DO Dra: V0455 Dra and V0454 Dra