Fig. 11
Positions of the source (marked by an empty blue dot with error bars) and RGC centroid (red dot) in the instrumental color-magnitude diagrams. For the events KMT-2016-BLG-2397 and OGLE-2017-BLG-1375, the CMDs are constructed using the pyDIA photometry of the KMTC data set. For KMT-2016-BLG-2364 and OGLE-2017-BLG-0604, the CMDs are based on the combinations of the OGLE (gray points) and HST (yellow points) data sets.
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