Fig. A.2.
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Same as Fig. 2, but for the LMC. The sources with known spectral types are from Martayan et al. (2006), Evans et al. (2006), Ramachandran et al. (2018). The border between MS and OBe stars lies at the same J − [3.6] color as in the SMC, while the border between He-burning stars and MS/OBe stars lies at U − B = −0.3 (for the SMC we adopt U − B = −0.5).
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