Probabilistic constraints on ﹩{\nu }_{\max }﹩ and ﹩{\rm{\Delta }}\nu ﹩ from the inference shown in Figure 8 compared to the published value (blue error bars) based on several years of Kepler observations (Pinsonneault et al. 2014). The two-dimensional contours show the 0.5σ, 1σ, 1.5σ, and 2σ credible regions in the marginalized planes, and the histograms along the diagonal show the marginalized posterior for each parameter.