sHRD containing all stars from Table A.2. Top: stars are colour-coded according to their spectroscopic information. The hatched symbols are SB1 binaries. Bottom: same as in the top panel, but now the photometric variability is indicated by different symbols. They are colour-coded according to their v sin i values. Stars with dominant rotational variability are hatched with white horizontal lines, and symbols hatched with white vertical lines show stars that can either have variability according to the symbol or rotational variability. The right panels show a zoom in of the region below the SPB instability strip. Typical errors are plotted, both the statistical error returned by zeta-Payne and the error including the internal uncertainties. Non-rotating MESA evolutionary tracks for different initial stellar masses (in grey) and the g-mode instability strip (red shaded area) from Burssens et al. (2020) are shown as well.