Fig. 9
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Wolf 327b radial velocity measurements taken with CARMENES. (a) RV time series and best-fitting model (blue line). The best-fitting model was computed using the median values of the posterior distribution of the fitted parameters, (b) Residuals of the fit after subtracting the single-planet Keplerian, the velocity linear trend seen here was included in the RV modeling, (c) Phase-folded RV measurements.
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