Fig. 5
Photometric contamination level per magnitude bin using the Besançon Galactic model
after selection in both 
and
colors. The plain
histogram corresponds to the number of objects selected as possible members from our
data (and located in the WIRCAM FOV), while the dashed one corresponds to the
selection performed on the synthetic catalog obtained from the Besançon model for
the same WIRCAM pointing.
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