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Fig. D.2
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Posterior distribution for a fit of a Keplerian model of the CARMENES RV data (RV) as well as spectroscopic indices: Telluric line contamination (telluric), differential line width (dLW), chromatic index (CRX), and Hα index (Hα). Posteriors for the orbital periods (left) and mean longitudes (right) are shown.
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