\begin{table}%t8
\caption{Results of PDR~models for [CI] in Henize~2-10 and NGC~253. We
  reported also observations from Tables~\ref{tab:obs1}
  and~\ref{tab:obs2}. The PDR~model predictions have been multiplied 
 by the line width ratio, $\frac{\Delta v({\rm galaxy})}{\Delta v({\rm PDR})}$, and
  by the surface filling factor, PDR\_FF, (see~Table~\ref{tab:pdr2}).}\label{tab:CI}
%\centering
\par
\begin{tabular}{c|cc}
\hline
\hline
 $E$ & NGC~253 & Henize~2-10 \\
(erg~cm$^{-2}$~s$^{-1}$~sr$^{-1}$)& observations & observations\\
\hline
CI($^{3}$P$_{1}$--$^{3}$P$_{0}$) & $3.5\times 10^{-5}$ &  $3.0\times 10^{-7}$\\
%\hline
CI($^{3}$P$_{2}$--$^{3}$P$_{1}$) & $3.2\times 10^{-5}$ & Not observed\\
\hline
& PDR model & PDR model\\
\hline
CI($^{3}$P$_{1}$--$^{3}$P$_{0}$) & $1.1\times 10^{-4}$ & $5.1\times 10^{-7}$\\
%\hline
CI($^{3}$P$_{2}$--$^{3}$P$_{1}$) & $3.9\times 10^{-4}$ &  $1.9\times 10^{-6}$\\
\hline
 \end{tabular}
\end{table}