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Table 5:

Re-analysis of a NGC1039 member (JP133) and of R66 (IC 2602).
Star $T_{\rm eff}$ $\log~g$ $\xi$ [Fe/H] [Si/Fe] [Ca/Fe] [Ti/Fe] [Ni/Fe]
  (K)   (km s-1)          
JP133 $_{\rm Schuler}$ 5710 4.54 1.88 $0.07 \pm 0.05$ $-0.02 \pm 0.08$ $0.02 \pm 0.08$ $- 0.17 \pm 0.08$ -0.13$\pm$0.05
JP133a 5710 4.54 1.88 $0.08 \pm 0.06$ $- 0.09 \pm 0.07$ $-0.02\pm0.1$ $- 0.17 \pm 0.11$ $- 0.16 \pm 0.08$
JP133b 5710 4.54 1.88 $0.05 \pm 0.14$ - $-0.02\pm0.16$ - $-0.18\pm0.11$
                 
R66 5640 4.45 1.30 $-0.02\pm 0.07$ $-0.02\pm 0.07$ $0.05 \pm 0.06$ $- 0.03\pm0.05$ $-0.04\pm0.05$

a With the line list by Schuler et al. (2003) and our method; b EWs by Schuler et al. and our $\log gf$ for common lines.


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