Fig. 10
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Planetary-parameter posteriors of our best model (d4; Fig. 7; blue dot-hatched) against the posteriors from our FWHM model with three activity sine terms (green square-hatched). Parameters share period- and phase priors across models. We use semi-amplitude panels (g,h,i) to show the median uncertainty of RV and FWHM measurements (dashed lines in respective colour).
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