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Fig. 8

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Coefficients of the VVV-2MASS transformations as a function of the reddening used to correct the zeropoint for 152 VVV fields in the Galactic disk. We included in each plot a linear fit with an iterative clipping algorithm similar to that used to calculate the photometric transformations. Grey points are those rejected during the clipping procedure. Moreover, the Spearman’s rank order correlation coefficient rS has been calculated in each case.

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