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Fig. 7


Dataset of the FWHM of the cross-correlation function from the HARPS and ESPRESSO data. The systemic offset for each instrument as retrieved from the two-planet model has been removed. The median GP model is shown as the solid black line, and the 1σ and 3σ confidence intervals are shown as shaded dark and light gray regions, respectively. Bottom panel: residuals after removing the GP model.

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