Fig. 6
Calibration to the Vegamag system. The points show Milky Way model stars generated with the TRILEGAL model for an area of ~1.4 deg2, and convolved with the typical photometric errors of 2MASS. The dashed lines show the limits for the 3σ clipping. The continuous lines are the best-fitting linear relations with a fixed slope as in Eq. (1).
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