\begin{table}%t3
\caption{Total column densities and abundances in  the
\zabs~= 4.383 DLA towards QSO 1202-0725.}\label{colden} 
%\centerline
{
\begin{tabular}{lllc}
\hline
\hline
 Ion & $\lambda_{{\rm rest}}$  & log $N$ ($X$)   & [$X$/H]$^a$    \\
\hline
 \HI  & 1215 & 20.55 $\pm$ 0.03 &  \\
 \CII & 1334 & 15.13 $\pm$ 0.05 & $-$2.01 $\pm$ 0.06 \\
 \CIV & 1548 & 12.86  $\pm$ 0.04 & \\
      & 1550 && \\
 \NI & 1200.2 & 13.81 $\pm$ 0.05 & $-$2.67 $\pm$ 0.06 \\
     & 1200.7 && \\
 \OI  & 1302 &  15.75 $\pm$ 0.06 & $-$1.54 $\pm$ 0.07 \\
      & 1039 & & \\
      & 971 && \\
\SiII & 1304 & 14.39 $\pm$ 0.05 & $-$1.70 $\pm$ 0.06 \\
      & 1526 && \\ 
\SiIV & 1393 & 12.71 $\pm$ 0.02 & \\
      & 1402 && \\
\FeIII & 1122 & 12.83 $\pm$ 0.09 & \\
\NiII  & 1317 & $<$12.5 & $<$$-$2.3 \\
       & 1370 & & \\
\hline
\end{tabular}}
\medskip
$^a$   [X/H] = log (X/H) -- log (X/H)$_{\sun}$.
For N and O updated photospheric solar values given by
\citet{holweger} were used, for the rest of the 
elements we used the meteorite values given by
\citep{sol:abun}. 
\end{table}