Fig. 2.
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Data-driven (in brown) and dynamical (in yellow-red) detection limits of TOI-1736 in the period-mass space, derived from SOPHIE RVs. Known planets are shown in black (triangle symbol if the mass is beyond the plotted range). Additional planets may only exist in the red-shaded area. A zoomed-in window around the inner planet illustrates nearby low-order MMRs (green: 6:5; gray: 7:6; blue: 8:7).
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