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Fig. 1.

image

Fourier transform of TESS light curve of Ross 548. Left panels: sub-Nyquist frequency range where the signal exceeds the 0.1% FAP (S/N = 4.54, horizontal dashed line). The peaks correspond to f3 and f4 from Table 3 (red lines), and the aliases (reflected across the Nyquist frequency) of f1 and f2 (blue vertical lines). Right-hand panels: transform above the Nyquist frequency, where the real periodicity – alias situation is reversed. Two bottom panels: residuals in the spectrum after pre-whitening by the least-squares fit sinusoids f1, f2, f3, f4 listed in Table 4.

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