Spatial distributions of clusters detected in this work shaded on our derived log t and A_V values. Left: side-on and top-down distribution of clusters in heliocentric coordinates that do not crossmatch to known GCs. The galactic centre is to the right, with the Sun at (0, 0). Only clusters passing two quality cuts are plotted: firstly, those with a CST score above 5σ, meaning they are highly probable astrometric overdensities; and secondly, a median CMD class above 0.5, which are those compatible with single population star clusters. Clusters are plotted in descending age order, meaning points representing young clusters are most visible in crowded regions. Right: as left, except clusters are colour-coded by extinction A_V. Clusters are plotted in ascending order of extinction.