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Fig. 14

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TOI-1736 SOPHIE RVs in phase with the orbits of the planets. In the top panel, the gray points show the RVs phase-folded in the period of planet b, where the orbit of planet c and the linear trend have been subtracted. In the bottom panel, the gray points show the RVs phase-folded in the period of planet c, where the orbit of planet b and the linear trend has been subtracted. The red points show the binned data, where we use a bin size of 0.05 in units of orbital phase. The green lines represent the best-fit orbit model for each respective planet.

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