Image Details
Caption: Figure 15.
Persistence comparison for ﹩{T}_{\mathrm{eff}}﹩ vs. ﹩\mathrm{log}\;g﹩ for stars with ﹩H\gt 11.﹩ Left panel has stars with all observations outside of persistence region, while right panel has stars with all observations inside of persistence region. Points are color-coded by temperature.
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