Table A.2: The number of stars in given ${\it TD}/D$ intervals for different values on the local density of thick disk stars ( $X_{\rm TD}$ ). The second column indicates the factor by which the ${\it TD}/D$ ratios change when varying the normalization (with the 10% density as base). The corresponding CM-diagrams can be seen in Fig. A.2.
$X_{\rm TD}$ -------- $N_{\rm stars}$ --------

<0.1 0.1-1 1-10 >10

2% 0.2 11781 362 166 261

6% 0.6 11305 689 238 347

10% 1 10969 946 285 383

14% 1.5 10623 1215 327 421

**Table A.2:** The number of stars in given ${\it TD}/D$ intervals for different values on the local density of thick disk stars ( $X_{\rm TD}$ ). The second column indicates the factor by which the ${\it TD}/D$ ratios change when varying the normalization (with the 10% density as base). The corresponding CM-diagrams can be seen in Fig. A.2.
$X_{\rm TD}$		-------- $N_{\rm stars}$ --------
		<0.1	0.1-1	1-10	>10
2%	0.2	11781	362	166	261
6%	0.6	11305	689	238	347
10%	1	10969	946	285	383
14%	1.5	10623	1215	327	421

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