Left panel: Lomb-Scargle periodogram of HD 284149 of the SuperWASP V magnitude time series collected in 2004 and 2006. The normalised power (PN) (black solid line) is plotted versus period. The red dotted line represents the spectral window function, whereas the red horizontal dashed line indicates the power level corresponding to a FAP = 0.1%. Right panel: superWASP V magnitudes of HD 284149 collected in 2006 and phased with the photometric rotation period P = 1.051 ± 0.005 days. Solid lines are the sinusoidal fits to phased data collected in the date range 2 453 995 < HJD < 2 454 057 (red) and in 2 454 065 < HJD < 2 454 125 (blue).
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