Kernel density estimations of the MLEs for the stellar mass (top-left), the fraction of initial hydrogen in the core (top-right), the fractional core mass (bottom-left), and the stellar radius (bottom-right), assuming Z = 0.0045. The different colours indicate different threshold on the classification probability from Hey & Aerts (2024) for the star to be considered a g-mode pulsator. The red line in the top-left panel corresponds to a Salpeter IMF with dN/dM ∝ M^−2.35.