Figure 6. Color–magnitude diagrams of OGLE-2018-BLG-0567 (upper panel) and OGLE-2018-BLG-0962 (lower panel). In each panel, the CMD is constructed using stars in the ¢ ´ ¢2 2 field centered on the event location based on KMTNet pyDIA photometry calibrated to the OGLE-III catalog (Szymański et al. 2011). The blue and red circles are the positions of the source and red clump centroid, respectively.
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