Fig. 3.
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Fourier amplitude spetra of the TESS 2019, WIRE 2006, combined BRITE 2014-16 light curves, and the HARPS radial velocities with the significant TESS frequencies overlaid as vertical red dotted lines. The original spectra are shown in the left panels, whereas right panels give the spectra after prewhitening the one to three most significant frequencies.
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