Fig. A.1
Correlation diagram from our MCMC fit to the observed Doppler shadow, as well as 1D histograms. The model consists of five parameters: scaled semimajor axis (a∕R*), projected obliquity (λ), orbital inclination (ip), projected stellar rotation speed (v sin i*), and a globalRV offset. Red lines denote literature values for the parameters (Talens et al. 2018).
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