CMDs of the clusters. For each cluster CMD on the left we have the combination of VISTA and 2MASS, whereas on the right is the Gaia CMD. The filled circles are the decontaminated cluster members from the VVVX data. The open circles in the VISTA and Gaia CMDs are the cluster members identified in the 2MASS data for the respective catalogues. The best isochrone match to the CMDs is represented by the solid blue line. The red arrows represent the reddening vectors in their respective CMDs. The error bars in the photometry have been omitted, but the typical photometric errors are δK_s = 0.01 mag at K_s = 12 mag, δK_s = 0.05 mag at K_s = 16 mag, and δK_s = 0.3 mag at Ks = 17.5 mag,