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Fig. A.3.
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[X/Fe] vs [Fe/H] for Na, Mg, Ni, and Ba for GHS143 (red dots), compared to the sample from Caffau et al. (2023, blue dots) and Cescutti et al. (2022, black dots), and from stars from the Sculptor dwarf galaxy taken from the SAGA database (Suda et al. 2008, 2017, light blue dots).
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