Left: VVV CL028 field-star decontaminated CMD. Main-sequence (1.0, 4.9, and 10.0 Myr, Lejeune & Schaerer 2001) isochrones are shown in the diagram. For the CMD and CCD we use the same colour code than Fig. 3. Right, top: VVV CL028 field-decontaminated CCD. Right, bottom: VVV CL028 P-DMF. The points show the central position in the mass ranges indicated above them, and the lines correspond to the best fit (red, segmented) and the Kroupa IMF fitted (blue, dotted) to the data.
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