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Fig. A.3
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Comparison of the abundance of (from left to right) [Y/H], [Zr/H], [Ba/H], [La/H], [Ce/H], [Nd/H], and [Eu/H] reported by SUL24, Carretta et al. (2013, 2011, 2014), and the Gaia-ESO DR5.1 for in-common stars. The figure follows the same description as Fig. A.2.
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