Fig. 11.
HRD for the MUSE sample with log Teff [K] > 4.3 (left panel). Right: sHRD (ℒ ≡ 
, Langer & Kudritzki 2014) for the sample indicating the difference in inferred mass between the sHRD and HRD approaches; each hexabin shows the mean value of all stars within it. Evolutionary tracks in both plots are those from Köhler et al. (2015). Stars outside of the evolutionary tracks are not included in the mass analysis.
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