Fig. A.3.
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Time series and GLS of the RVs and activity indicators derived from the FEROS spectra (left and middle panels, respectively). The right panels show the correlation with respect to the FEROS RVs for the derived key activity indicators. The type of activity indicator is given in each of the panels of the middle column. The vertical red line shows the suspected planetary period (P = 109.8 d), from the model with linear trend of the combined RVs (FEROS+HARPS) and photometric (TESS) data.
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