Fig. 1
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Distribution of the ATLAS9 model atmospheres of the new grid (blue circles) in the log10(Teff)–log g plane superimposed (upper panel) to four theoretical BaSTI-IAC isochrones with 15 Myr, 100 Myr, 1 Gyr, and 13 Gyr and a solar-scaled metallicity (Hidalgo et al. 2018) and compared (lower panel) to the distribution of MARCS (Gustafsson et al. 2008), PHOENIX (Husser et al. 2013), and TLUSTY (Lanz & Hubeny 2003, 2007) model atmospheres.
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