Posterior distributions of κ₁, κ₂, and f for the mixture model. For the κ posteriors, we also show the 1000 corresponding ψ distributions on the right panel. The mode and 68% HDPI are ﹩{\kappa }_{1}=2{6}_{-19}^{+179}﹩, ﹩{\kappa }_{2}={5}_{-3}^{+5}﹩, and ﹩f=0.6{6}_{-0.29}^{+0.21}﹩. This result indicates that there are two distinct stellar spin–orbit angle distributions.