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 the 2464 gravity-mode pulsators modelled via the grid with solar metallicity. The quantities on the abscissa are derived using the effective temperature and luminosity as input, while for the quantities on the ordinate, the near-core rotation frequency is added as an extra observable. The red lines indicate perfect correspondence.