The photometric period of the cataclysmic variable HV Andromedae

We present four nights of time-resolved photometry of the cataclysmic variable star HV And. Our time series analysis has revealed a prominent period at 3.368 ± 0.060 h, as well as some low frequency power. We interpret this signal, from saw-tooth waves in the light curve, as evidence of superhumps in HV And.

► We present four nights of time-resolved photometry of the cataclysmic variable star HV And.
► We find a period at 3.368 ± 0.060 h, as well as some low frequency power.
► We interpret this signal as superhumps in HV And.