Fig. 3

Smoothed power density spectrum (with an apodized 300-μHz FWHM window) in log-scale axes. The dashed line represents the contributions of the granulation signal and of the photon noise. The dotted line is a Gaussian fit of the excess power envelope. The mixed line is the smoothed spectrum of HD 181420, with the same treatment and an offset accounting for the different photon-noise levels.
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