Stellar obliquities of eight close-in gas giant exoplanets

Open Access

Fig. B.2

Corner plot representing the posterior distributions of the projected rotational velocity (v sin i_∗) and projected obliquity (λ) of our Doppler Shadow analysis of HAT-P-41 Ab. Shown are three MCMC initializations. The result $(λ_{b} = - {7.6}_{- 8.0}^{+ 7.7} deg)$ $\left( {{\lambda _b} = - 7.6_{ - 8.0}^{ + 7.7}{\rm{deg}}} \right)$ prefers an aligned orbit that is consistent with our classical R-M effect analysis.

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