Chemical composition of the young open clusters IC 2602 and IC 2391

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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
JP133^a	5710	4.54	1.88	$0.08 \pm 0.06$	$- 0.09 \pm 0.07$	$-0.02\pm0.1$	$- 0.17 \pm 0.11$	$- 0.16 \pm 0.08$
JP133^b	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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