Fig. 11
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Direct comparison between the derived stellar abundance ratio [C/Fe] in this work, using the synthetic grid from Knowles et al. (2021) (left) and the BOSZ library (Mészáros et al. 2024, right), and the abundance estimate for stars in common with the literature, with their respective reported uncertainties as error bars. The dashed black line is the same as in Fig. 5.
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