\begin{table}%t4 %\centering \par \caption{\label{table:FIES}Atmospheric parameters, abundance ratios, and space velocities for stars with NOT/FIES spectra.} \par \begin{tabular}{lccccrrrrrrrrrrr} \noalign{\smallskip} \hline\hline \noalign{\smallskip} ID & \teff & \logg & \fracfeh & \micro & \fracnafe & \fracmgfe & \fracsife & \fraccafe & \fractife & \fraccrfe & \fracnife & $U_{\rm LSR}$ & $V_{\rm LSR}$ & $W_{\rm LSR}$ & Class\tablefootmark{a} \\ & (K) & & & (km~s$^{-1}$) & & & & & & & & (km~s$^{-1}$) & (km~s$^{-1}$) & (km~s$^{-1}$) \\ \hline \noalign{\smallskip} 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$) \\ G20-15\tablefootmark{b} & 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~148816\tablefootmark{b} & 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~179626$^{b}$ & 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~189558$^{b}$ & 5623 & 3.81 & $-$1.12 & 1.4 & $-$0.01 & 0.38 & 0.38 & 0.36 & 0.27 & $-$0.01 & 0.01 & 80 & $-$109 & 48 & TD \\ HD~193901$^{b}$ & 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~194598$^{b}$ & 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$ \\ \noalign{\smallskip} \hline \end{tabular} \par \tablefoot {$^{a}$ Classification as thick disk (TD), low-$\alpha$, or high-$\alpha$. For halo stars with $\feh < -1.4$, the classification is uncertain and given in parentheses. $^{b}$ Data are also available from UVES spectra (see Table~\ref{table:UVES}). In the figures, abundance data based on the UVES spectra are plotted. } \par \end{table}