Fig. B.3.
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KDE spatial distribution. Top panels: Spatial distribution for Garro 03 selected at r ≲ 3′ from the cluster centre, where we can clearly see a circular overdensity of stars at the cluster position. Bottom panels: Spatial distribution of a 3′ field, selected away from the cluster field, for which no central overdensity is visible. For both cases, the samples used VVVX data, cleaned by nearby stars. These panels show the following from left to right: the 2D histogram and the calculated Gaussian KDE on which we overplotted iso-density contours.
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