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Fig. 7

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[C/Fe] against [Fe/H] for 3D CEMP and 1D measurements of Galactic stars from a MS + sub-giant subsample of the SAGA database. The dashed red line represents the mean, uncorrected 1D and the solid blue line the 3D CEMP-corrected data. Shaded regions correspond to standard deviations of the observed sample in the respective metallicity bin ±0.5 dex. The dotted grey line represents the dividing CEMP classification abundance of [C/Fe] = 0.7.

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