Fig. A.2
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Top: Formation height of a representative CH line in the atmospheres of 3D M3DIS models at [Fe/H] = −5, log g = 4.0. Bottom: 3D scaled-solar − 1D A(C) abundance corrections as a function of Teff, derived from spectra using the same atmosphere models as in the top panel and applying [C/Fe] = 3.0 as the reference abundance, as in Fig. 6
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