Fig. C.2
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Joint and marginal posteriors for the orbital periods, semi-amplitudes, eccentricities, and minimum planet masses, Mp sin i, in Earth masses, of the 11-day (left) and 5-day (right) Keplerian signals. These results come from the analysis of the CCF RVs. The estimates at the top of each panel correspond to the median and 68% quantiles of the posteriors.
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