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Fig. 1


Positions on the sky for the microlensed dwarf sample. The bulge contour lines based on observations with the COBE satellite are shown as solid lines (Weiland et al. 1994). The dotted lines are concentric circles in steps of 2°. OGLE-2013-BLG-0911S that is excluded from the final bulge sample (see Sect. 4) is marked by a lightgrey circle.

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