Variation in the resulting [Fe/H] with increasing Teff by 200 K (lower panels) and ξ by 0.2 km s-1 (upper panels) as a function of the initial Teff(left panels) and of the initial [Fe/H] value (right panels). The hotter and less metallic stars are the most sensitive to a modification of Teff whereas the cooler and more metallic stars are the most sensitive to a modification of ξ.
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