Radial profile of stellar density, centered at RA = 12^h14^m32.15^s, Dec =−62°58′50.1′′ and binned by 5 arcseconds. Gray bars represent the whole population with K_S< 15, and green bars show the fraction of these that fall within the color range of OB cluster members (0.4 ≤ H−K_S ≤ 0.7). For the sake of clarity, the density values of the first bin (0.2037 and 0.2164) are outside the axis range. The radial cuts for HST and VVV photometry are shown as red vertical lines, and the density limit we use to establish the outer boundary of the cluster is indicated as a red dashed line. For each cluster region, we also provide the probability that a star that fulfills the color cut is actually a contaminant.