Most frequently occurring variability class for each bin of the latent space shown in Fig. 13 for the set of variable stars that have a variability class label available (see Section 3). The bins are colour-coded with the fraction of stars in the bin that have the shown label. Only the variability classes SPB, γ Dor, β Cep, δ Sct, CP stars, AGNs, LPVs, RR Lyr (ab, c, and d), Cepheids, WDs, eclipsing binaries (EA, EB, EW), ELL variables, Be (BE) variables, and YSO variables were taken into account to generate this figure.