Fig. 9.
Same as Fig. 8, but for nickel, zinc, strontium, and yttrium versus [Fe/H] for individual dSph galaxies. Gray dots show MW stars of Reddy et al. (2003, 2006), Cayrel et al. (2004), Ishigaki et al. (2013), Fulbright (2000), Nissen et al. (1997), Prochaska et al. (2000), Stephens & Boesgaard (2002), Ivans et al. (2003), McWilliam et al. (1995b), Ryan et al. (1996), Gratton & Sneden (1988), Edvardsson et al. (1993).
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