Fig. 1
Grid nodes (surface gravities and effective temperatures) at which the non-LTE radiative transfer calculations were carried out. The missing nodes are where standard MARCS model atmospheres do not presently exist, owing to convergence issues (see Sect. 5.4 of Gustafsson et al. 2008). Also shown in black are the parameters of the 50126 stars drawn from GALAH DR3, studied in this work.
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