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Fig. 6

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Coefficients of the VVV-2MASS transformations as a function of Galactic longitude and latitude for 152 VVV tiles in the Galactic disk. Top and second row, we divided the sample into low (red; | b| ≲ 1°) and high latitude fields (green; 2.1° ≳ |b| ≳ 1°). A fourth order polynomial was fitted in each case. Third and bottom row, photometric coefficients divided into low longitude (red; l ≳ 320°), and high longitude fields (green; l ≲ 320°).

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