Fig. 4.
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Optical CMDs of sources in the LMC outer regions. Top panel: sources with VMC and Gaia EDR3 photometry as well as STARHORSE distances (black) and the MW stars from our training sample that have STARHORSE distance estimates d < 10 kpc (blue). Bottom panel: likely Magellanic stars with STARHORSE distance estimates d > 20 kpc (based on Schmidt et al. 2020).
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