Fig. 7
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Comparison of the 4MOST-ified input spectra to model spectra corresponding to the cINN MAP estimates for four low-metallicity stars, focusing on prominent absorption lines of Mg, Ca, Li and Fe. We note that the re-simulation employed all 13 stellar parameters predicted by the cINN, but used the bias correction from Sect. 4.3 only for the abundances of Ca, Mg, Li, and Fe (see also Table B.5).
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