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Fig. 5

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Power spectrum of the quiescent light curve of FS Aur (left panel) and its corresponding spectral window (right). The strongest peak in the window at fY = 0.00274 day-1 corresponds to the yearly observational cycle. The fVLPP = 0.001114 ± 0.00015 day-1 frequency corresponding to VLPP is the second-highest peak in the power spectrum, with the strongest peak being falias = 0.00114 + 0.00274 = 0.00388 day-1, an alias created by the beat between fVLPP and f1y.

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