Colour-magnitude diagram of the upper main sequence of the Pleiades. We mark our discovered g-mode pulsators with orange and known p-mode pulsators from Bedding et al. (2023) with black dots. The dotted and dashed lines crossing the cluster sequence indicate the γ Dor and δ Sct instability strips, respectively (Dupret et al. 2004; Murphy et al. 2019). The grey lines show the isochrones from Fig. 1 with MIST dashed, PARSEC dotted, and MIST with the YBC bolometric corrections adopted in PARSEC dash-dotted. Stars with proper names are labelled.