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In this work we present time-resolved photometry of a few poorly-studied dwarf novae during recent superoutbursts. Observations were made using 50-cm and 60-cm telescopes of Sternberg Astronomical Institute in Crimea in 2012, 2013. Superhumps were detected in the light curves of all dwarf novae. The amplitudes and periods of detected light variations were calculated. Superhumps evolution was also followed up for all systems and classification is precised.