Fig. A.3
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HARPS-N YARARA-V1 RV and spectroscopic activity indicators of HD 147379. Similar description to Fig. A.2, except with the periodogram computation. The long-period trends observed in the time-series of the spectroscopic indicators are better fitted by quadratic drifts instead of Keplerians. The corresponding periodograms were computed from the residuals of these fits.
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