Fig. C.4

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GLS periodograms of the HARPSterra+CARMENES RV residuals, after removing the best-fit models shown in the second columns of Table C.1–C.2. For each kernel, periodograms of data with and without the correlated activity signal included are shown. The periodograms were calculated with the uncorrelated jitter terms added in quadrature to the formal RV uncertainties.
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