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Table 4:

Derived abundances.
Star $T_{\rm eff}$ $\log~g$ $\xi$ [Fe/H] [Na/Fe] [Si/Fe] [Ca/Fe] [Ti$_{\rm I}$/Fe] [Ti$_{\rm II}$/Fe] [Ni/Fe]
  (K)   (km s-1)              
R1 5050 4.5 1.15 $-0.01 \pm 0.04 \pm 0.05$ $- 0.14 \pm 0.04 \pm 0.06$ $0.02 \pm 0.05 \pm 0.09$ $-0.02 \pm 0.07 \pm 0.06$ $- 0.06 \pm 0.05 \pm 0.06$ $0.22 \pm 0.04 \pm 0.11$ $-0.01 \pm 0.06 \pm 0.08$
R14 5100 4.5 1.1 $0 \pm 0.05 \pm 0.05$ $- 0.07 \pm 0.06\pm0.06$ $0.05\pm0.06\pm0.09$ $0.01 \pm 0.06 \pm 0.06$ $-0.02 \pm 0.07 \pm 0.06$ $0.11\pm0.04\pm0.11$ $- 0.01 \pm 0.08 \pm 0.06$
R15 4770 4.5 0.7 $0 \pm 0.06 \pm 0.06$ $-0.35\pm0.07\pm0.08$ $0.03 \pm 0.07\pm0.09$ $-0.2\pm0.05\pm 0.07$ $-0.4 \pm 0.05 \pm 0.06$ $0.30 \pm 0.05 \pm 0.13$ $0.02 \pm 0.05 \pm 0.08$
R66 5590 4.45 1.15 $- 0.01 \pm 0.03 \pm 0.06$ $- 0.03 \pm 0.04 \pm 0.05$ $0.02 \pm 0.05 \pm 0.05$ $0 \pm 0.05 \pm 0.02$ $- 0.03 \pm 0.04 \pm 0.04$ $0.01 \pm 0.08 \pm 0.09$ $- 0.03 \pm 0.05 \pm 0.04$
R70 5760 4.45 1.1 $0 \pm 0.05 \pm 0.06$ $0 \pm 0.06 \pm 0.05$ $- 0.04 \pm 0.07 \pm 0.06$ $0.03 \pm 0.1 \pm 0.04$ $0 \pm 0.05 \pm 0.03$ $0 \pm 0.04 \pm 0.08$ $-0.04 \pm 0.08 \pm 0.05$
R92 5630 4.45 1.2 $- 0.02 \pm 0.04 \pm 0.06$ $0.02 \pm 0.04 \pm 0.05$ $- 0.02 \pm 0.06 \pm 0.05$ $0.02 \pm 0.05 \pm 0.03$ $0.01 \pm 0.07 \pm 0.02$ $0.02 \pm 0.01 \pm 0.08$ $- 0.02 \pm 0.06 \pm 0.04$
R95 5020 4.5 0.8 $0.02 \pm 0.03 \pm 0.05$ $-0.13 \pm 0.05 \pm 0.06$ $- 0.02 \pm 0.06 \pm 0.07$ $0.04 \pm 0.06 \pm 0.07$ $- 0.07 \pm 0.08 \pm 0.07$ $0.24 \pm 0.04 \pm 0.11$ $-0.05 \pm 0.09 \pm 0.07$
W79 5260 4.5 1.1 $-0.02\pm 0.08 \pm 0.06$ $-0.12\pm 0.09 \pm 0.06$ $0.01 \pm 0.08 \pm 0.07$ $0 \pm 0.08 \pm 0.07$ $0.02 \pm 0.08 \pm 0.05$ $0.12 \pm 0.01 \pm 0.10$ $-0.03\pm 0.12 \pm 0.04$
IC 2602       $0 \pm 0.01$ $-0.10\pm0.12$ $0\pm 0.03$ $-0.02 \pm 0.08$ $-0.06 \pm 0.14$ $0.13 \pm 0.12$ $-0.02 \pm 0.02$
          $-0.07\pm 0.06^a$   $0.01\pm0.02^a$ $-0.01\pm 0.04^a$    
          $0 \pm 0.02^c$          
VXR3 5590 4.45 1.15 $0 \pm 0.04 \pm 0.07$ $- 0.02 \pm 0.05 \pm 0.05$ $0.02 \pm 0.06 \pm 0.05$ $0.01 \pm 0.05 \pm 0.02$ $0.00 \pm 0.06 \pm 0.03$ $0.03 \pm 0.03 \pm 0.09$ $- 0.02 \pm 0.06 \pm 0.04$
VXR31 5630 4.5 1.2 $-0.02 \pm 0.04 \pm 0.07$ $0.02 \pm 0.05 \pm 0.05$ $0.02 \pm 0.05 \pm 0.05$ $0.01 \pm 0.04 \pm 0.01$ $0.03 \pm 0.08 \pm 0.02$ $0.07 \pm 0.03 \pm 0.09$ $0.02 \pm 0.06 \pm 0.02$
VXR67 4680 4.5 0.7 $0.01 \pm 0.05 \pm 0.06$ $- 0.31 \pm 0.09 \pm 0.07$ $0 \pm 0.09 \pm 0.09$ $-0.21 \pm 0.11 \pm 0.08$ $- 0.38 \pm 0.04 \pm 0.06$ $0.25 \pm 0.07 \pm 0.13$ $-0.02 \pm 0.06 \pm 0.06$
VXR70 5557 4.5 1.15 $- 0.03 \pm 0.05 \pm 0.07$ $-0.06 \pm 0.07 \pm 0.05$ $0.04 \pm 0.06 \pm 0.07$ $0.03 \pm 0.06 \pm 0.03$ $-0.03 \pm 0.07 \pm 0.04$ $0.09 \pm 0.04 \pm 0.10$ $0.02 \pm 0.05 \pm 0.05$
VXR72 5257 4.5 1.1 $- 0.02 \pm 0.03 \pm 0.06$ $-0.12 \pm 0.05 \pm 0.06$ $0.01 \pm 0.04 \pm 0.08$ $0.03 \pm 0.08 \pm 0.05$ $0.02 \pm 0.05 \pm 0.05$ $0.17 \pm 0.05 \pm 0.11$ $0.01 \pm 0.04 \pm 0.05$
VXR76a 4343 4.5 1.2 $0 \pm 0.06 \pm 0.07$ $- 0.34 \pm 0.08 \pm 0.07$ $0.06 \pm 0.09 \pm 0.08$ $- 0.38 \pm 0.12 \pm 0.08$ $- 0.35 \pm 0.16 \pm 0.06$ $0.37 \pm 0.06 \pm 0.13$ $0.02 \pm 0.09 \pm 0.08$
SHJM2 5970 4.45 1.2 $0 \pm 0.03 \pm 0.05$ $- 0.03 \pm 0.04 \pm 0.04$ $-0.01\pm0.06\pm0.06$ $0.02 \pm 0.04 \pm 0.04$ $0.01 \pm 0.04 \pm 0.01$ $0 \pm 0.02 \pm 0.08$ $- 0.03 \pm 0.04 \pm 0.03$
IC 2391       $-0.01\pm 0.02$ $- 0.12 \pm 0.14$ $0.01 \pm 0.02$ $-0.07 \pm 0.16$ $-0.10 \pm 0.18$ $0.14 \pm 0.13$ $0 \pm 0.02$
          $-0.04\pm 0.05^b$   $0.02 \pm 0.01^b$ $0 \pm 0.02^b$    
          $-0.02\pm 0.03^c$          
vb 187 5339 4.5 0.92 $0.14 \pm 0.04 \pm 0.06$ $0 \pm 0.03 \pm 0.05$ $0.06\pm 0.02 \pm 0.08$ $0 \pm 0.04 \pm 0.05$ $- 0.07 \pm 0.04 \pm 0.05$ $0.12 \pm 0.09 \pm 0.09$ $0.04 \pm 0.03 \pm 0.05$
Hyades $_{\rm Paulson}$       $0.13 \pm 0.05$ $0.01 \pm 0.09$ $0.05 \pm 0.05$ $0.07 \pm 0.07$ $0.03 \pm 0.05$ - -
Hyades $_{\rm Friel}$       0.13 0.01 0.04 0.06 -0.06 - -
We list again the identifier of each star (1), final stellar parameters (Cols. 2-4), [Fe/H] values (5), and the [X/Fe] ratios (Cols. 6-11). The errors ($\sigma_1$, $\sigma_2$) are also reported. Average abundances for iron and the other elements are also indicated. a] Average values were computed by discarding the coolest star R15; b VXR67 and VXR76a were not included in the average; c average values by considering only stars with $T_{\rm eff} > 5500$ K.

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