Fig. 3
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Top : radial velocity phase-folded to the best-fitting period listed in Table 2. The RV data are colour-coded in brown and green for HARPS and FEROS, respectively, and the black circles represent the binned RVs. The red curve and shaded light red region shows the Keplerian model and its 1σ confidence interval. Bottom : residuals of the best-fit model.
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