Fig. 7
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Results of the juliet fit of TOI-5786. First panel: radial velocity curve of TOI-5786 with the best fit Keplerian model for the two-planet case in black. Second panel: RVs phase-folded to TOI-5786 b. The dark blue data points represent the MaHPS RV data binned at 0.05 phases. Third Panel: RVs phase-folded to the period of the inner companion candidate. Fourth Panel: Residuals after subtracting the signals of both planets.
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