\begin{table}%T1
\caption{Derived stellar parameters and abundances of sulphur and zinc.
LTE sulphur abundances are given for each of the three \SI~lines. The LTE Zn abundance is
the average of the values derived from the $\lambda\lambda 4722.2, 4810.5$ \ZnI~lines.
In calculating \sfe\ and \znfe , solar abundances \logFesun\ = 7.50, \logSsun\ = 7.20
and \logZnsun\ = 4.60 have been adopted. The non-LTE values of \sfe\ and \znfe\ are
based on the non-LTE corrections calculated by Takeda et~al. (\cite{takeda05}) for
a hydrogen collisional parameter $S_{\rm H} = 1$.}
\label{table:par}
\small%\centerline
{
\begin{tabular}{lcccccclcccrr}
\noalign{\smallskip}
\hline\hline
\noalign{\smallskip}
  ID   &   \teff & \logg &  \feh & \micro & \multicolumn{3}{c}{\logSlte} & \sfe & \sfe & \logZn & \znfe & \znfe \\
       &   (K)   & (cgs) &       & (\kmprs) & $\lambda 9212.9$ & $\lambda 9237.5 $ & $\lambda 8694.6$ & LTE  & 
 non-LTE & LTE    & LTE      & non-LTE  \\
\hline
Paper~~I stars    &         &     &  & & & & & & & & &      \\
\noalign{\smallskip}
\object{BD~$-13\degr3442$} & 6366 &   3.99 &  $-$2.69 &   1.5 &   4.92 &   4.95 &        &   0.43 &   0.23 &   1.99 &   0.08 &   0.19  \\
\object{CD~$-30\degr18140$}& 6272 &   4.12 &  $-$1.89 &   1.5 &   5.59 &   5.68 &   5.52 &   0.29 &   0.21 &   2.74 &   0.03 &   0.10  \\
\object{CD~$-35\degr14849$}& 6294 &   4.26 &  $-$2.34 &   1.5 &   5.14 &   5.16 &        &   0.29 &   0.18 &   2.33 &   0.07 &   0.14  \\
\object{CD~$-42\degr14278$}& 6085 &   4.39 &  $-$2.03 &   1.5 &   5.35 &   5.40 &        &   0.20 &   0.14 &   2.65 &   0.08 &   0.12  \\
\object{G~11-44}        &    6178 &   4.35 &  $-$2.03 &   1.5 &   5.54 &   5.49 &        &   0.34 &   0.27 &   2.76 &   0.19 &   0.24  \\
\object{G~13-09}        &    6343 &   4.01 &  $-$2.29 &   1.5 &   5.38 &        &        &   0.47 &   0.31 &   2.40 &   0.09 &   0.18  \\
\object{G~18-39}        &    6093 &   4.19 &  $-$1.46 &   1.5 &   6.05 &   6.09 &   6.08 &   0.33 &   0.26 &   3.22 &   0.08 &   0.13  \\
\object{G~20-08}        &    6194 &   4.29 &  $-$2.19 &   1.5 &   5.26 &   5.40 &        &   0.32 &   0.24 &   2.56 &   0.15 &   0.21  \\
\object{G~24-03}        &    6084 &   4.23 &  $-$1.62 &   1.5 &   5.98 &   5.91 &   5.89 &   0.34 &   0.29 &   3.04 &   0.06 &   0.11  \\
\object{G~29-23}        &    6194 &   4.04 &  $-$1.69 &   1.5 &   5.76 &   5.79 &   5.84 &   0.29 &   0.20 &   2.86 &  $-$0.05 &   0.02  \\
\object{G~53-41}        &    5993 &   4.22 &  $-$1.29 &   1.3 &   6.18 &   6.16 &   6.19 &   0.27 &   0.20 &   3.33 &   0.02 &   0.06  \\
\object{G~64-12}        &    6435 &   4.26 &  $-$3.24 &   1.5 &   4.41 &        &        &   0.45 &   0.19 &   1.77 &   0.41 &   0.52  \\
\object{G~64-37}        &    6432 &   4.24 &  $-$3.08 &   1.5 &   4.45 &        &        &   0.33 &   0.10 &   1.96 &   0.44 &   0.55  \\
\object{G~66-30}$^{a}$& 6470 &   4.29 &  $-$1.48 &   1.5 &   6.03 &   6.11 &   5.84 &   0.28 &   0.18 &   3.10 &  $-$0.02 &   0.05  \\
\object{G~126-62}$^{a}$&6224 &   4.11 &  $-$1.55 &   1.5 &   5.95 &   5.96 &   5.78 &   0.25 &   0.16 &   3.04 &  $-$0.01 &   0.05  \\
\object{G~186-26}       &    6417 &   4.42 &  $-$2.54 &   1.5 &   4.85 &   4.85 &        &   0.19 &   0.07 &   2.25 &   0.19 &   0.26  \\
\object{HD~106038}      &    6027 &   4.36 &  $-$1.37 &   1.2 &   6.28 &   6.22 &   6.29 &   0.43 &   0.38 &   3.37 &   0.14 &   0.18  \\
\object{HD~108177}      &    6156 &   4.28 &  $-$1.71 &   1.5 &        &   5.86 &   5.78 &   0.33 &   0.30 &   2.96 &   0.07 &   0.12  \\
\object{HD~110621}      &    6157 &   4.08 &  $-$1.59 &   1.5 &   6.03 &   5.92 &   5.74 &   0.29 &   0.21 &   3.02 &   0.01 &   0.07  \\
\object{HD~140283}      &    5849 &   3.72 &  $-$2.38 &   1.5 &   5.07 &   5.06 &   5.17 &   0.28 &   0.20 &   2.30 &   0.08 &   0.14  \\
\object{HD~160617}      &    6047 &   3.84 &  $-$1.75 &   1.5 &   5.81 &   5.80 &   5.85 &   0.37 &   0.28 &   2.82 &  $-$0.03 &   0.04  \\
\object{HD~179626}      &    5881 &   4.02 &  $-$1.12 &   1.4 &   6.37 &        &   6.31$^{b}$ &   0.26 &   0.17 &   3.48 &   0.00 &   0.04  \\
\object{HD~181743}      &    6044 &   4.39 &  $-$1.87 &   1.5 &   5.62 &   5.62 &        &   0.29 &   0.23 &   2.81 &   0.08 &   0.12  \\
\object{HD~188031}      &    6234 &   4.16 &  $-$1.72 &   1.5 &   5.76 &   5.75 &   5.78 &   0.28 &   0.21 &   2.91 &   0.03 &   0.09  \\
\object{HD~193901}      &    5699 &   4.42 &  $-$1.10 &   1.2 &   6.29 &   6.30 &   6.34 &   0.21 &   0.17 &   3.38 &  $-$0.12 &  $-$0.10  \\
\object{HD~194598}      &    6020 &   4.30 &  $-$1.15 &   1.4 &   6.26 &   6.30 &   6.20$^{b}$ &   0.20 &   0.13 &   3.37 &  $-$0.08 &  $-$0.04  \\
\object{HD~215801}      &    6071 &   3.83 &  $-$2.28 &   1.5 &   5.28 &   5.16 &        &   0.30 &   0.17 &   2.41 &   0.09 &   0.17  \\
\object{LP~815-43}      &    6483 &   4.21 &  $-$2.71 &   1.5 &   4.87 &   4.81 &        &   0.35 &   0.17 &   2.17 &   0.28 &   0.38  \\
\noalign{\smallskip}
New stars   &         &     &  & & & & & & & & &     \\
\noalign{\smallskip}
\object{CD~$-24\degr17504$} &6338 &   4.32 &  $-$3.21 &   1.5 &   4.51 &        &        &   0.52 &   0.30 &   1.96 &   0.57 &   0.66  \\
\object{CD~$-71\degr1234$}$^{a}$ & 6325 &   4.18 &  $-$2.38 &   1.5 &   5.13 &   5.19 &        &   0.34 &   0.22 &   2.34 &   0.12 &   0.20  \\
\object{CS~22943-095}   &    6349 &   4.18 &  $-$2.24 &   1.5 &   5.36 &   5.33 &        &   0.38 &   0.26 &   2.49 &   0.13 &   0.20  \\
\object{G~04-37}        &    6308 &   4.25 &  $-$2.45 &   1.5 &   5.05 &   4.98 &        &   0.26 &   0.15 &   2.29 &   0.14 &   0.21  \\
\object{G~48-29}        &    6482 &   4.25 &  $-$2.60 &   1.5 &   4.94 &   5.03 &        &   0.39 &   0.23 &   2.13 &   0.13 &   0.23  \\
\object{G~59-27}$^{a}$& 6272 &   4.23 &  $-$1.93 &   1.5 &   5.57 &   5.57 &        &   0.30 &   0.20 &   2.73 &   0.06 &   0.12  \\
\object{G~126-52}       &    6396 &   4.20 &  $-$2.21 &   1.5 &   5.21 &        &        &   0.22 &   0.09 &   2.50 &   0.11 &   0.19  \\
\object{G~166-54}       &    6407 &   4.28 &  $-$2.58 &   1.5 &   5.04 &   5.06 &        &   0.43 &   0.29 &   2.10 &   0.08 &   0.16  \\
\object{HD~84937}       &    6357 &   4.07 &  $-$2.11 &   1.5 &   5.47 &   5.38 &   5.40 &   0.33 &   0.23 &   2.55 &   0.06 &   0.15  \\
\object{HD~338529}      &    6373 &   4.03 &  $-$2.26 &   1.5 &   5.36 &   5.32 &        &   0.40 &   0.25 &   2.48 &   0.14 &   0.23  \\
\object{LP~635-14}      &    6367 &   4.11 &  $-$2.39 &   1.5 &   5.12 &   5.07 &        &   0.29 &   0.14 &   2.36 &   0.15 &   0.24  \\
\object{LP~651-4}       &    6371 &   4.20 &  $-$2.63 &   1.5 &   4.83 &        &        &   0.26 &   0.11 &   2.04 &   0.07 &   0.16  \\
\hline
\end{tabular}}
\smallskip
 $^{a}$ Single-lined spectroscopic binary star.\\
 $^{b}$ The weaker $\lambda 8694.0$ \SI~line is included in
the determination of this S abundance.
\end{table}