\begin{table}%t4
\caption{\label{params}Parameters of the stars (Col.~1) obtained with MA$\chi$ for
  both types of analysis discussed in the text.}
%\begin{center}
\par
\begin{tabular}{c| c c c| c c c| c c c c}
\hline\hline \\
& \multicolumn{3}{c|}{MA$\chi$, free} & \multicolumn{3}{c|}{MA$\chi$,
  restr.} & \multicolumn{4}{c}{Classical, $EW$} \\
Star	&$T_{\rm eff}$ (K) & $\log g$ & [Fe/H]&$T_{\rm eff}$ (K)
& $\log g$ & [Fe/H]& $T_{\rm eff}$ (K) & $\log g$& [Fe/H]&$v_t$ (km~s$^{-1}$)\\ \\
\hline \\
HD~3567 & 6103.5& 4.79&--1.200 &6176.0 &4.20 &--1.223 & 6035.0 &  4.08& --1.200& 1.50\\
HD~19445 & -- &--&--&5746.5 &4.10 &--2.293 & 5982.0  & 4.38 &--2.075 &1.40\\
HD~22879 &5770.6&4.31&--0.877& 5778.1& 4.31& --0.880 & 5792.0&   4.29& --0.885 &1.20\\
HD~25704& 5638.9 &3.61&--1.094 & 5864.4 &4.19 &--0.912  &5700.0   &4.18 &--1.010 &1.00\\
HD~63077&5795.5&4.21&--0.796 &5787.7& 4.21& --0.793&  5629.0 &  4.15 &--0.935 &0.90\\
HD~63598&6078.6&4.79&--0.681&5804.1 &4.23 &--0.901 & 5680.0   &4.16 &--0.885 &0.90\\
HD~97320 &5601.1&4.65&--1.411&6025.1& 4.24 &--1.183 & 6105.0&   4.18 &--1.175 &1.20\\
HD~103723 &5999.2&4.29&--0.896&6004.4 &4.29 &--0.896 & 6128.0  & 4.28 &--0.805 &1.50\\
HD~105004 &5802.5&4.33&--0.900&5802.5& 4.33& --0.900 & 5900.0&   4.30& --0.800 &1.10\\
HD~106038&5994.6&4.48&--1.392& 5995.5 &4.48 &--1.392  &5950.0   &4.33 &--1.390 &1.10\\
HD~113679 &6037.3&4.73&--0.500&5757.5 &4.35& --0.708  &5759.0  & 4.04 &--0.590 &0.90\\
HD~116064&5757.7&4.58&--2.41 &5757.7 &4.58 &--2.401  &5999.0   &4.33 &--2.000 &1.50\\
HD~121004&5509.2&4.05& --0.670&5657.8 &4.40 &--0.650  &5711.0   &4.46 &--0.725 &0.65\\
HD~122196 &5811.8&3.50&--1.954&5810.2 &3.56 &--1.954  &6048.0   &3.89 &--1.760 &1.20\\
HD~126681&5556.9&4.44&--1.055 &5521.6 &4.68 &--1.075  &5532.0   &4.58 &--1.170 &0.60\\
HD~160617 &5804.1&3.50&--1.961&5985.2 &3.75 &--1.794  &6028.0   &3.79 &--1.785 &1.30\\
HD~175179 &6080.5&5.00&--0.500&5779.5 &4.47 &--0.691  &5758.0   &4.16 &--0.690 &0.90\\
HD~188510 &5568.8&4.35&--1.341&5500.0 &4.65 &--1.231  &5536.0   &4.63 &--1.600 &1.00\\
HD~189558 &5610.8&3.58&--1.191&5500.0 &3.75 &--1.181  &5712.0   &3.79 &--1.145 &1.20\\
HD~195633 &6318.2&4.61&--0.500&6037.7 &3.99 &--0.687  &6005.0   &3.86 &--0.625 &1.40\\
HD~205650 &5693.7&4.93&--1.195&5754.0 &4.47 &--1.208  &5842.0   &4.49 &--1.170 &0.90\\
HD~298986 &5891.5&3.66&--1.592&6297.9 &4.22 &--1.304  &6144.0   &4.18 &--1.410 &1.40\\
CD--333337 &5808.2&3.66&--1.598&5946.9 &3.85 &--1.490 &5952.0 &3.95 &--1.435 &1.40\\
CD--453283 &5500.0&4.26&--0.978&5885.5 &5.00 &--0.685 &5657.0 &4.97 &--0.835 &0.80\\
CD--571633 &5939.9&4.37&--0.893&5939.9 &4.37 &--0.893 &5907.0 &4.26 &--0.930 &1.10\\
CD--3018140& 6143.1&3.50&--2.095&6246.5& 3.50& --1.980 &6340.0 &4.13 &--1.870 &1.00\\
G005--040 & 6228.2&5.00&--0.584&5930.4  &4.52 &--0.794 & 5766.0   &4.23 &--0.840 &0.80\\
G013--009 &6529.5&4.58&--2.29& 6556.0&  4.08 &--2.299 & 6416.0  & 3.95& --2.225 &1.40\\
\hline
\end{tabular}
\tablefoot{In the first
  analysis all three parameters are determined with only the
  spectrum, while in the second one $\log g$ was determined
  independently by using parallaxes according to Eq.~(14), as for the classical method (EW; last four columns).}\vspace*{3.4mm}
%\end{center}
\par
\end{table}