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Table 4:

Atmospheric parameters, abundance ratios, and space velocities for stars with NOT/FIES spectra.
ID $T_{\rm eff}$ log g $\displaystyle {\rm\left[\frac{Fe}{H}\right]}$ $\xi_{\rm turb}$ $\displaystyle {\rm\left[\frac{Na}{Fe}\right]}$ $\displaystyle {\rm\left[\frac{Mg}{Fe}\right]}$ $\displaystyle {\rm\left[\frac{Si}{Fe}\right]}$ $\displaystyle {\rm\left[\frac{Ca}{Fe}\right]}$ $\displaystyle {\rm\left[\frac{Ti}{Fe}\right]}$ $\displaystyle {\rm\left[\frac{Cr}{Fe}\right]}$ $\displaystyle {\rm\left[\frac{Ni}{Fe}\right]}$ $U_{\rm LSR}$ $V_{\rm LSR}$ $W_{\rm LSR}$ Classa
  (K)     (km s-1)               (km s-1) (km s-1) (km s-1)  

G05-36 		6013 4.23 -1.23 1.4 -0.01 0.33 0.37 0.38 0.34 -0.01 -0.01 -41 -297 -60 high-$\alpha $
G13-38 5263 4.54 -0.88 0.9 0.05 0.35 0.31 0.30 0.32 0.06 0.00 109 -143 89 high-$\alpha $
G15-23 5297 4.57 -1.10 1.0 -0.02 0.40 0.33 0.32 0.33 0.06 -0.01 19 -176 -57 high-$\alpha $
G16-20 5625 3.64 -1.42 1.5 -0.13 0.22 0.33 0.32 0.19 -0.07 0.01 208 -143 75 (low-$\alpha $)
G20-15b 6072 4.36 -1.41 1.1 -0.23 0.20 0.15 0.25 0.22 -0.03 -0.05 161 -60 -210 (low-$\alpha $)
G21-22 5901 4.24 -1.09 1.4 -0.26 0.09 0.07 0.17 0.03 -0.02 -0.16 247 -258 -31 low-$\alpha $
G24-13 5673 4.31 -0.72 1.0 0.08 0.34 0.27 0.29 0.25 0.02 0.01 164 -38 -128 high-$\alpha $
G24-25 5828 3.86 -1.40 1.2 -0.03 0.34 0.41 0.32 0.31 -0.04 0.00 -197 -242 43 (high-$\alpha $)
G31-55 5638 4.30 -1.10 1.4 0.07 0.28 0.33 0.29 0.25 0.05 0.01 -23 -184 -45 high-$\alpha $
G49-19 5772 4.25 -0.55 1.2 0.12 0.30 0.27 0.28 0.23 0.04 0.02 37 -236 58 high-$\alpha $
G53-41 5859 4.27 -1.20 1.3 0.23 0.24 0.24 0.31 0.14 -0.03 -0.09 -31 -299 -150 low-$\alpha $
G56-30 5830 4.26 -0.89 1.3 -0.19 0.10 0.12 0.17 0.06 -0.03 -0.16 32 -283 -53 low-$\alpha $
G56-36 5933 4.28 -0.94 1.4 -0.06 0.19 0.19 0.25 0.17 -0.02 -0.08 -105 -247 8 low-$\alpha $
G57-07 5676 4.25 -0.47 1.1 0.12 0.34 0.29 0.29 0.30 0.05 0.05 -73 -162 -50 high-$\alpha $
G74-32 5772 4.36 -0.72 1.1 0.10 0.37 0.29 0.30 0.26 0.02 0.02 -143 -151 74 high-$\alpha $
G75-31 6010 4.02 -1.03 1.4 -0.19 0.12 0.17 0.31 0.19 -0.06 -0.13 -259 -206 109 low-$\alpha $
G81-02 5859 4.19 -0.69 1.3 0.06 0.25 0.19 0.20 0.11 -0.01 -0.04 -175 -201 18 high-$\alpha $
G85-13 5628 4.38 -0.59 1.0 0.13 0.33 0.28 0.27 0.25 0.04 0.03 -184 -43 35 high-$\alpha $
G87-13 6085 4.13 -1.09 1.5 -0.25 0.10 0.18 0.32 0.22 -0.04 -0.12 -201 -286 15 low-$\alpha $
G94-49 5373 4.50 -0.80 1.1 0.06 0.34 0.32 0.29 0.28 0.03 0.01 172 -96 -2 high-$\alpha $
G96-20 6293 4.41 -0.89 1.5 0.13 0.30 0.30 0.27 0.25 -0.06 0.00 -128 -91 118 high-$\alpha $
G98-53 5848 4.23 -0.87 1.3 -0.07 0.20 0.17 0.25 0.12 0.01 -0.09 -156 -263 -96 low-$\alpha $
G99-21 5487 4.39 -0.67 0.9 0.11 0.33 0.27 0.29 0.26 0.05 0.02 -64 -182 22 high-$\alpha $
G119-64 6181 4.18 -1.48 1.5 -0.15 0.25 0.21 0.37 0.29 -0.01 -0.06 237 -291 -120 (low-$\alpha $)
G125-13 5848 4.28 -1.43 1.5 -0.17 0.30 0.28 0.30 0.20 -0.09 -0.09 215 -228 -157 (high-$\alpha $)
G127-26 5791 4.14 -0.53 1.2 0.10 0.31 0.22 0.22 0.20 0.03 0.00 171 -83 -50 high-$\alpha $
G150-40 5968 4.09 -0.81 1.4 0.28 0.14 0.19 0.19 0.12 0.01 -0.08 -63 -318 14 low-$\alpha $
G161-73 5986 4.00 -1.00 1.4 -0.36 0.13 0.13 0.25 0.14 -0.06 -0.15 228 -250 42 low-$\alpha $
G170-56 5994 4.12 -0.92 1.5 -0.11 0.17 0.14 0.24 0.12 -0.02 -0.11 -52 -289 -29 low-$\alpha $
G172-61 5225 4.47 -1.00 0.9 -0.18 0.16 0.17 0.26 0.16 0.04 -0.10 -14 -267 57 low-$\alpha $
G176-53 5523 4.48 -1.34 1.0 -0.36 0.15 0.15 0.25 0.15 -0.01 -0.12 -230 -271 61 low-$\alpha $
G180-24 6004 4.21 -1.39 1.5 -0.14 0.31 0.31 0.39 0.31 0.03 -0.04 111 -245 -21 high-$\alpha $
G187-18 5607 4.39 -0.67 1.1 0.06 0.29 0.26 0.26 0.23 0.02 0.00 109 -130 72 high-$\alpha $
G192-43 6170 4.29 -1.34 1.5 -0.21 0.19 0.23 0.33 0.29 -0.05 -0.09 -327 -224 -15 low-$\alpha $
G232-18 5559 4.48 -0.93 1.3 -0.06 0.35 0.34 0.34 0.26 0.05 0.00 72 -242 99 high-$\alpha $
HD 148816b 5840 4.14 -0.70 1.4 0.14 0.32 0.27 0.26 0.20 0.02 0.02 98 -260 -73 high-$\alpha $
HD 159482 5737 4.31 -0.73 1.3 0.15 0.34 0.32 0.30 0.25 0.05 0.02 -164 -47 95 high-$\alpha $
HD 160693 5714 4.27 -0.49 1.1 0.05 0.24 0.19 0.21 0.14 -0.01 -0.01 215 -105 92 high-$\alpha $
HD 177095 5349 4.39 -0.74 0.9 0.05 0.38 0.30 0.31 0.28 0.02 0.01 140 -138 -23 high-$\alpha $
HD 179626b 5855 4.19 -1.00 1.4 0.06 0.36 0.32 0.34 0.26 0.03 -0.05 91 -215 45 high-$\alpha $
HD 189558b 5623 3.81 -1.12 1.4 -0.01 0.38 0.38 0.36 0.27 -0.01 0.01 80 -109 48 TD
HD 193901b 5676 4.41 -1.07 1.4 -0.30 0.17 0.16 0.23 0.11 -0.04 -0.14 -148 -233 -66 low-$\alpha $
HD 194598b 5926 4.32 -1.08 1.4 -0.10 0.23 0.21 0.22 0.14 -0.03 -0.09 -65 -267 -29 low-$\alpha $
HD 230409 5318 4.54 -0.85 1.1 0.05 0.30 0.25 0.26 0.26 0.06 0.00 164 -114 -4 high-$\alpha $
HD 233511 6006 4.23 -1.55 1.3 -0.19 0.36 0.28 0.40 0.30 -0.05 -0.05 -131 -243 31 (high-$\alpha $)
HD 237822 5603 4.33 -0.45 1.1 0.15 0.35 0.26 0.28 0.26 0.04 0.05 81 -131 131 high-$\alpha $
HD 250792A 5489 4.47 -1.01 1.1 -0.18 0.23 0.13 0.33 0.26 0.04 -0.12 245 -237 104 low-$\alpha $

Notes. aClassification as thick disk (TD), low-$\alpha $, or high-$\alpha $. For halo stars with $\mbox{\rm [Fe/H]}< -1.4$, the classification is uncertain and given in parentheses. b Data are also available from UVES spectra (see Table 3). In the figures, abundance data based on the UVES spectra are plotted.


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