Fig. 18.
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Fundamental parameter coverage of the XSL stars, for dwarfs (left panel) and giants (right panel). Dwarfs and giants are separated at log g = 3. The stars that are used to construct static, variable (O-rich TP-AGB), and carbon (C-rich TP-AGB) star sequences are not included, as we ignore the information about their metallicity in the models (Sect. 3.2).
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