Fig. 1

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Histograms (normalised to 100% occurrence) of the gspphot values for Teff for 11 636 Gaia DR3 γ Dor stars (left, grey) and 3426 SPB stars (right, cyan). The width of the bars is in accordance with the average error (150 K for γ Dor and 400 K for the SPB stars). Asteroseismic values obtained from Kepler data are shown for 37 γ Dor (grey, hatched) and 26 SPB stars (black cross-hatched), respectively. For the right panel, 31 SPB stars with a temperature above 22 000 K in the Gaia DR3 sample were omitted for visibility reasons.
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