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Fig. 8.
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Comparison between the stars found in this work (solid symbols) and those found by Meingast et al. (2021) (black circles) in NGC 2516 and its tidal tails. Only stars with G < 17.5 in Meingast et al. (2021) are shown. There are more high probability members found by us outside of the plotted range (see Fig. A.2).
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