Three newly reported clusters randomly selected from the cluster catalogue and ordered by increasing distance, with member stars plotted as a function of their astrometric and photometric data as in Fig. 13. All clusters pass the cuts proposed in Cantat-Gaudin & Anders (2020), have good-quality CMDs passing the cuts from Sect. 4, and have astrometric significances of greater than 5σ, meaning they are almost certainly real overdensities in Gaia data.