Fig. 2
OGLE-IV color–magnitude diagrams for stars in 2′× 2′ regions around OGLE-2012-BLG-1323 and OGLE-2017-BLG-0560. Sources are marked with blue squares and are likely located in the Galactic bulge. If sources were M dwarfs, they would have absolute I-band magnitudesof 9.75 (OGLE-2012-BLG-1323) and 13.90 (OGLE-2017-BLG-0560; Pecaut & Mamajek 2013) and would be located at a distance of 140 and 16 pc, respectively, which contradicts the Gaia DR2 parallaxes (0.15 ± 0.14 mas and 0.23 ± 0.19 mas, respectively).
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