Fig. 8
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Phase-folded HARPS RVs (in green) in the period of HD 207496 b. The best model is shown in black. The RVs were corrected for systemic velocity, a fitted RV trend, and stellar activity with the fitted GP model. For clarity, we also show the binned RVs in red. Below the RVs, we show the residuals relative to the best-fit model.
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