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Fig. 16
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TOI-2141 SOPHIE RVs in phase with the orbit of the planet. The gray points show the RVs phase-folded in the period of planet TOI-2141 b, and 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 TOI-2141 b.
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