Fig. 16

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TOI-1470 CARMENES RVs (blue dots) and the best model (black line) from the combined photometric and spectroscopic fit folded in phase with the orbital period of the Keplerian components: TOI-1470 b and c. The GP component has been removed from the data. The binned data are plotted as open black symbols. All error bars include the quoted CARMENES uncertainties and the RV jitter as obtained from the model added in quadrature. The gray shadowed area denotes the 68% confidence interval.
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