Fig. 8
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TOI-6651 RVs (black dots) from 27 spectroscopic observations with PARAS-2 are plotted with time (on the left). TOI-6651 RVs plotted with orbital phase (on the right). In both plots, the best-fit RV model with EXOFASTv2 is represented by the red line, and residuals between the best-fit model and the data are shown in their respective lower panel.
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