\begin{table}%t3
%\centering
\par
  \caption{Microturbulence determinations from Fe I and Fe II lines.\label{tab3}}
  \begin{tabular}{llcccccl}
\hline\hline
&        & Number &   $\xi_{1}$ &             & $\xi_{2}$   &             & \\
Star&Species &of Lines&(km s$^{-1}$)&$\log N/N_{\rm T}$&(km s$^{-1}$)&$\log N/N_{\rm T}$&$gf$ values\\
\hline
$\theta$ And &Fe I & 34 & 3.9 & $-4.27\pm0.28$ & 3.9 & $-4.27\pm0.28$ & MF + KX\\
             &Fe II& 23 & 3.2 & $-4.22\pm0.24$ & 3.2 & $-4.22\pm0.24$ & MF + KX\\
             & & adopted& 3.6 &         &      &                      & \\
             & &        &    &                 &     &                &  \\
$\epsilon$ Del&Fe II& 32 & 0.0& $-4.56\pm0.21$ & 0.0 & $-4.56\pm0.21$ & MF + KX\\
             & & adopted& 0.0 &  	&      &        	          &\\
             & &        &    &   	       &     &  	          &  \\
$\epsilon$ Aqr & Fe I& 33 &3.1 &$-4.66\pm0.25$ & 3.1 & $-4.66\pm0.25$ & MF + KX \\
        & Fe II & 24   &  2.4 & $-4.60\pm0.26$ & 2.5 & $-4.62\pm0.24$ & MF+KX \\
      & & adopted& 2.8 &         	&     &         	   & \\  
      & &        &    &          	&     &         	   & \\  
$\iota$ And &Fe II& 44 &  1.3 & $-4.71\pm0.19$ & 1.2 & $-4.69\pm0.19$ & MF + KX \\
            &Fe II& 34 &  1.4 & $-4.75\pm0.20$ & 1.4 & $-4.75\pm0.20$ & MF\\
      & & adopted& 1.3 &                &     &                &  \\
\hline
\end{tabular}
\begin{flushleft}
$gf$ value references: MF~=~Fuhr et~al. (\cite{Fuhr88}), KX = Kurucz \& Bell (\cite{Kurucz95}).\\
Note: For $\xi_{1}$ and $\xi_{2}$ the abundances are found so that there is no
trend of values for lines 
 of different equivalent widths and have minimum scatter about the mean,
respectively.
\end{flushleft}
\end{table}