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Fig. 1


A comparison between 2MASS and VVV J − H photometry for the regions encompassing Pismis 19 and NGC 4349. A 1:1 correlation (red line) exists to within the uncertainties. The data for Pismis 19 were deliberately offset from zero for presentation purposes. Pertinent details regarding the pipeline employed here to process the VVV data are described in Moni Bidin et al. (2011) and Mauro et al. (in prep.).

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