Table 6: Derived abundances relative hydrogen, [X/H], where X denotes the different elements as indicated. Each element has three columns, mean abundance ([X/H]), standard deviation of the mean abundance ( $\sigma _{\rm [X/H]}$), and the number of spectra lines (N) that has been used in computing the mean abundance. The abundances have been normalized with respect to the solar photospheric abundances as given in Grevesse & Sauval (1998), see also Table 4. The second column indicates if the star belongs to the thin disk ( ${\rm mem=1}$) or the thick disk ( ${\rm mem}=2$) ( ${\rm mem=3}$indicates the Sun). The full table is available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/410/527.
  mem Fe I Fe II Na I Mg I $\ldots$
    [X/H] $\sigma _{\rm [X/H]}$ $N_{\rm lines}$ [X/H] $\sigma _{\rm [X/H]}$ $N_{\rm lines}$ [X/H] $\sigma _{\rm [X/H]}$ $N_{\rm lines}$ [X/H] $\sigma _{\rm [X/H]}$ $N_{\rm lines}$ $\ldots$

Sun		 3 0.00 0.09 147 0.00 0.09 29 0.00 0.04 4 0.00 0.00 7 $\ldots$
Hip 3086 2 -0.11 0.09 145 -0.18 0.07 24 -0.10 0.03 4 0.03 0.05 6 $\ldots$
Hip 3142 1 -0.45 0.09 131 -0.45 0.08 25 -0.33 0.04 4 -0.27 0.05 7 $\ldots$
$\vdots$ $\vdots$ $\vdots$ $\vdots$ $\vdots$ $\vdots$ $\vdots$ $\vdots$ $\vdots$ $\vdots$ $\vdots$ $\vdots$ $\vdots$ $\vdots$ $\ddots$


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