Left: CaMD with different variability types shown in different colors. Non-variable member stars are shown as small light gray circles. Right: Same as left panel, but showing tracks derived from GDR3 epoch photometry, limited to up to 200 variables per class with the highest number of epochs in GDR3 and the lowest chance of having blended transits (following cuts in Riello et al. 2021, Sect. 9.4).