Fig. D.1.

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HR diagram for sources having spectroscopic masses ℳ1≥ 5.0 M⊙ and the closest STAREVOL (Siess et al. 2000) evolutionary tracks from Lagarde et al. (2012). The spectroscopic masses and metallicities from GSP-Spec and XGBoost (if available) are in the title of each panel. The parameters from XGBoost and the associated mass were adopted.
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