Histogram of the dominant frequency in the Kepler light curves of 63 asteroseismically modelled g-mode pulsators (blue) compared with the dominant frequency occurring in their Gaia DR3 G-band epoch photometry (black hatched). For reasons of visibility, the x−axis is cut at 6.5 d⁻¹ and the y−axis at 20; 38 of the 63 g-mode pulsators have their Gaia data dominated by instrumental effects with dominant frequency above 6 d⁻¹ rather than by their g modes.