Fig. 4

Comparison of 2MASS and VVV photometry for stars observed in tile/field d003. In each case an iterative clipping algorithm has been applied to each one of the 20 adaptive bins of the distribution. The selected stars of the clipping algorithm (grey) have been used to calculate the linear fit, and the individual photometric uncertainties of each star were considered.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.