The results of new photometric observations of two SU UMa type dwarf novae are presented. Superhumps were detected on the light curves of these systems during superoutbursts and their periods and amplitudes determined. The classification of objects as dwarf novae of the ER UMa subclass (for RZ LMi) and subclass WZ Sge (for KV Dra) has been clarified. Orbital period 0d. 0586 for KV Dra was determined.
Voloshina et al. (Mon,) studied this question.