Table 9: Derived abundances relative to hydrogen. Each element has three columns, mean abundance ([X/H]), standard deviation of the mean abundance ( $\sigma _{\rm [X/H]}$ ), and the number of spectral lines ( $N_{\rm X}$ ) that were used in the abundance analysis (Cols. 4 and onwards). The abundances have been normalized with respect to the Sun (see Sect. 5.1 and Table 5). Column 1 gives the Hipparcos number; Col. 2 indicates with which spectrograph the star was observed (S = SOFIN, F = FEROS, U = UVES); Col. 3 indicates if the star belongs to the thin disk (Mem. = 1), the thick disk (Mem. = 2), or a "transition object'' (Mem. = 3). The full table is available in electronic form at the CDS.
HIP Inst. Mem. [Fe I/H] $\sigma_{\rm [Fe {\sc i}/H]}$ $N_{\rm Fe {\sc i}}$ $\ldots$

699 S 1 -0.20 0.06 79 $\ldots$

910 S 1 -0.36 0.07 68 $\ldots$

$\vdots$ $\vdots$ $\vdots$ $\vdots$ $\vdots$ $\vdots$ $\ddots$

**Table 9:** Derived abundances relative to hydrogen. Each element has three columns, mean abundance ([X/H]), standard deviation of the mean abundance ( $\sigma _{\rm [X/H]}$ ), and the number of spectral lines ( $N_{\rm X}$ ) that were used in the abundance analysis (Cols. 4 and onwards). The abundances have been normalized with respect to the Sun (see Sect. 5.1 and Table 5). Column 1 gives the Hipparcos number; Col. 2 indicates with which spectrograph the star was observed (S = SOFIN, F = FEROS, U = UVES); Col. 3 indicates if the star belongs to the thin disk (Mem. = 1), the thick disk (Mem. = 2), or a "transition object'' (Mem. = 3). The full table is available in electronic form at the CDS.
HIP	Inst.	Mem.	[Fe I/H]	$\sigma_{\rm [Fe {\sc i}/H]}$	$N_{\rm Fe {\sc i}}$	$\ldots$
699	S	1	-0.20	0.06	79	$\ldots$
910	S	1	-0.36	0.07	68	$\ldots$
$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\vdots$	$\ddots$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Stellar sample
	3 Observations and data reductions
	4 Stellar model atmospheres
	5 Abundance analysis
	6 Stellar ages
	7 Abundance results
	8 Discussion and summary
	Appendix A: Kinematical criteria for selecting thick disk stars in the solar neighbourhood
	References