\setcounter{table}{6}
\begin{table*}%t7
\caption[]{\label{tab:abund}Derived stellar atmosphere parameters and Fe abundance.}
\centerline {\begin{tabular}{rcccccccccc} \hline\hline
\smallskip
Star & $T_{\rm eff}$ & $\log g$ & [$m$/H]$^{{a}}$ & $v_{\rm t}$ & log $\epsilon$(Fe~I)& $\sigma$ & $N$& log $\epsilon$(Fe~II)& $\sigma$ &$N$\\
 & ($^\circ$K) & & & (km s$^{-1}$) &  &  &  &  &  & \\ \hline
 665 & 5451 & 4.53 & $+0.05$ & 1.25 & 7.50 & 0.06 & 64 & 7.60 & 0.07 & 5 \\
1560 & 5830 & 4.48 & $+0.13$ & 1.38 & 7.58 & 0.07 & 76 & 7.87 & 0.03 & 5 \\
3359 & 5280 & 4.55 & $-0.01$ & 1.17 & 7.44 & 0.06 & 73 & 7.64 & 0.06 & 4 \\
4362 & 5616 & 4.51 & $+0.05$ & 1.30 & 7.50 & 0.07 & 67 & 7.59 & 0.04 & 5 \\
\hline
\end{tabular}}

\smallskip
  $^{a}$  Input model atmosphere abundance on a scale where 
the solar $\log$ $\epsilon$(Fe)\,=\,$7.45$.
\end{table*}
