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Fig. 6

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Radial velocity measurements of HD 20329 taken with HARPS-N. (a) RV time series and best-fitting model (blue line) including red noise. The best model shown here was computed using the median values of the posterior distribution for each fitted parameter. The orange shaded area around the blue line represent the 1σ uncertainty levels of the fitted model. (b) Residuals of the fit after subtracting the single-planet Keplerian function and systematic noise component from the RVs. (c) Radial velocity measurements in phase after subtracting the red noise and best-fitting model (blue line).

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