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Fig. B.1

image

Abundances ratios vs. Teff for RGB stars with –1.0 < [Fe/H] < –0.5 dex in our sample, in blue; and in the sample of Letarte et al. (2010), in cyan. We also show the values determined for Arcturus by Van der Swaelmen et al. (2013) in green; and by ourselves, using the same method as for our Fornax sample, in red.

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