Fig. 2
Top: best Keplerian fit to the absorption line RVs for the combined FEROS and HARPS RV data set (with RVlin). The different colors indicate different observing seasons (-1 stands for the first half of the year, -2 for the second half). Circles represent FEROS and squares HARPS data points. Middle: residua with the same color and shape coding. Bottom: emission line RVs with the same color and shape coding.
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