Fig. 9
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Phase-folded RV data for the NGTS-30/TOI-4862 system. Top: collected RV data with the joint planet model over-plotted in black. Bottom: RV residuals after subtracting the RV model. For clarity, a dashed grey line is plotted at zero on the residuals plot. The eccentricity of NGTS-30 b/TOI-4862 b’s orbit is clearly shown by the asymmetry of the RV model.
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