Spatial distribution for Garro 02 selected at r ≲ 4′ (on the top). We also compare the cluster spatial distribution with its relative field (on the bottom) selected at 5′≲r ≲ 8′ from the cluster centre. We used the KDE technique in order to better distinguish the over-densities (yellow and green colours) from lower densities (blue colours). All samples were cleaned by nearby stars. These panels show the following from left to right: the 2D histograms and the calculated Gaussian KDE on the which we overplotted iso-density contours.