\begin{table}%t3
%\centering
\par
\caption{Iron abundance (\feh) for the Sun determined from Solar atlas
spectrum (Wallace et~al. \cite{whl98}) and FEROS spectra,
respectively. 131~Fe~I and 20 Fe~II lines, measured in both spectra, were
used. Results from ATLAS9 models and MARCS models are compared. }\label{tab:sun_feh}
\small
\begin{tabular}{lcc}
\hline
\hline
&  Fe~I                      & Fe~II               \\ 
\hline
ATLAS9:              &                   &          \\
Solar atlas          & $+0.11 \pm 0.10$            & $-0.02 \pm 0.07$      \\ 
FEROS                & $+0.11 \pm 0.10$            & $-0.04 \pm 0.07$      \\ 
\noalign{\smallskip}  
MARCS:               &                                                &    \\
Solar atlas          & $+0.07 \pm 0.09$            & $+0.00 \pm 0.10$      \\ 
FEROS                & $+0.07 \pm 0.10$            & $-0.01 \pm 0.09$      \\ 
\hline
\end{tabular}            
\end{table}