\begin{table}%t4
%\centering
\par
\caption{\label{tab4}Solar iron abundances based on 15 \ion{Fe}{ii} lines (Table~\ref{tab3}) with our  \mbox{$gf$-values} and different model atmospheres.}
\small \begin{tabular}{ccc} 
\hline\hline                
{Model}  & $v_{\rm mic}$ & $A_{\rm FeII}$($\sigma$) \\
{     }  & (km~s$^{-1}$) & (dex)  \\
\hline    
  HM         & 1.09 & 7.46 ($\sigma = 0.028$)   \\
Kurucz OVER  & 0.98 & 7.48 ($\sigma = 0.026$)   \\
Kurucz NOVER & 0.91 & 7.43 ($\sigma = 0.027$)   \\
MARCS 1997   & 0.92 & 7.44 ($\sigma = 0.029$)   \\
MARCS 2008   & 0.91 & 7.42 ($\sigma = 0.028$)   \\
$\langle$3D$\rangle$     & 0.92 & 7.47 ($\sigma = 0.027$)   \\
 3D  &  & 7.45 (re-scaled from A00) \\
%\hline                                 
 mean   &  & 7.45 ($\sigma = 0.022$) \\
\hline                                 
\end{tabular}
\end{table}