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Fig. 5

image

Abundance measurement errors as a function of errors on the stellar parameters: [Fe/H] (upper left panel), microturbulence velocity (upper right panel) and effective temperature (lower left panel). Errors as a function of the corresponding [Fe/H] value are also displayed (lower right panel). In all panels errors for [Ca/H] abundances are shown as red empty circles and errors for [Mg/H] as red filled circles.

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