Fig. 2
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Stellar abundances within the GALAH catalogue (orange; Ν = 91 202) and within the sample for which we ran condensation sequence models (blue; Ν = 1000). Given our adjusted selection procedure, the selected sample places more emphasis on the tails of the distribution presented by the GALAH catalogue. Solar abundances are shown as a dashed black line (Asplund et al. 2009).
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