New photometry of RZ LMi and KV Dra detects superhumps during superoutbursts, determines periods and amplitudes, clarifies ER UMa and WZ Sge subclassifications, and measures a 0.0586-day orbital period for KV Dra.
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Photometric light curves analysis of SU UMa-type dwarf novae: the case of RZ LMi and KV Dra
New photometry of RZ LMi and KV Dra detects superhumps during superoutbursts, determines periods and amplitudes, clarifies ER UMa and WZ Sge subclassifications, and measures a 0.0586-day orbital period for KV Dra.