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This article has an erratum: [https://doi.org/10.1051/0004-6361/202243508e]


Fig. A.1.

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Individual [Fe/H] measurements and their errors as a function of SMA radius in units of the 2D half-light radius for the dwarf galaxies. The solid orange line and blue shaded area represent the result of the Gaussian process regression analysis (using a Gaussian kernel) and the associated 1-σ confidence interval. The legend box of each panel reports the name of the corresponding dwarf galaxy.

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