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Fig. B.3.
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Difference between I magnitudes from our XPSP samples and OGLE-III for 315080 stars in common between the two samples having |ΔI|< 1.0 (LMC; upper panel) and 90115 stars in common between the two samples having |ΔI|< 1.0 (SMC; lower panel). In each panel, the red line is the median difference computed in bins 0.2 mag wide.
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