Fig. 6
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Top panel : detrended NIRPS and HARPS RVs (red triangles and blue circles, respectively) phase-folded on the best-fit planetary period. The planet model is shown with a grey line, while the grey shading represents the one (darker) and two (lighter) standard deviations of the fit. Bottom panel : radial velocity residuals after the GP and planet model have been subtracted.
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