Fig. 8.
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Power spectra of β Aql showing solar-like oscillations from four time series in radial velocity and one in TESS photometry, with measurements of νmax and amplitude per radial mode (see Sect. 5.1). The bottom panel shows the reconstructed power spectrum from the combined SONG and TESS data, smoothed to a resolution of 1 μHz (see Sect. 5.5).
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