\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}