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Fig. 8


Phase-folded radial velocity signal of the candidate planet LHS 1140 d in the three-planet model. Upper panel: radial velocity data (color-coded as in the legend), binned radial velocities (open black symbols) with a bin size corresponding to 15% of the phase, the median model from the joint three-planet analysis (see Sect. 6) as the solid black line, and the 68.7 and 95% confidence intervals as shaded dark and light gray regions. Bottom panels: residuals of the median model.

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