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Fig. 9

image

VVV CL088 field-star decontaminated CMD with main sequence (1.0, 4.9, and 10.0 Myr, Lejeune & Schaerer 2001) isochrones (Left), and CCD (right, top). For the CMD and CCD, we use the same colour code as in Fig. 3. Right, bottom: VVV CL088 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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