Fig. 11
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1D NLTE corrections for [Na/Fe] (left) and [Al/Fe] (right) as a function of their [Fe/H]LTE for all MP SAGA stars, derived using the grids from Lind et al. (2022) for Na and Al, and the NLTE Fe I in Fig. 10. Stars with abundances determined from resonance or from subordinate lines are marked with downward and upward triangles, respectively.
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