Fig. 9.
Locations of the primary and companion source stars with respect to the centroid of the RGC in the instrumental CMD (gray dots). The determinations of the source positions and the construction of the CMD are based on the pyDIA photometry of the KMTC data set. We also present the Hubble Space Telescope CMD (Holtzman et al. 1998, brown dots) to show the source locations on the main-sequence branch.
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