Fig. 4
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Data and model of the NIRPS RV and DLW time series. The two top panels show the NIRPS RV data (detrended from CRX and BERV), with the best model fit (top; GP + two planets), and the residuals after the fit (bottom), along with the periodograms of both (right). The two bottom panels show the same for the FWHM. The shaded region shows the standard deviation of the GP model.
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