Derived measurements for the stellar mass (top left), the fractional convective core mass (top right), the core hydrogen-mass fraction compared to the initial hydrogen-mass fraction (bottom left), and the stellar radius (bottom right) of 96 γ Dor stars (circles) and three SPB stars (squares) modelled via the grid with solar metallicity. The quantities are derived using the effective temperature, luminosity, and near-core rotation frequency from the dominant dipole prograde mode detected in the Gaia DR3 light curves (x-axis) versus the higher-precision value deduced from the slope of a period spacing pattern of dipole prograde modes of consecutive radial order following Li et al. (2020) and Pedersen et al. (2021) (y-axis).