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Fig. 1

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Fourier periodogram of TESS photometry of HD 192639 during the different sectors. The left-hand panels display the periodogram between 0 and 5 d–1 clearly unveiling the red-noise behaviour. The bestfit red-noise relation is shown in red. The right-hand panels provide a zoomed-in view of the region below 1 d–1. The dashed blue vertical line yields the ν1 frequency previously found in spectroscopic time series by Rauw et al. (2001).

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