\begin{table}%t1
\par
\caption {\label{galpar}Galaxy parameters. Both the stellar and dark mater profiles are
represented by Plummer models, having characteristic masses, respectively,
given by $M_{\rm B}$ and $M_{\rm H}$ and core radii given by $r_{\rm B}$ and $r_{\rm H}$.}
 %\centering
\par
  \begin{tabular}{lcccc}
       \hline\hline
       &  gE0 & gE0l& gE0m& iE0\\
       \hline
       $M_{\rm B}\ [2.3\times 10^9 ~M_{\odot}]$ & 70& 70& 70& 35\\
       $M_{\rm H}\ [2.3\times 10^9 ~M_{\odot}]$ & 30& 30& 30& 15\\
       $r_{\rm B}\ [{\rm kpc}]$ & 4.0&  6.0& 2.0& 2.8\\
       $r_{\rm H}\ [{\rm kpc}]$ & 7.0& 7.0& 7.0& 5.0\\
       $N_{\rm star}$ &80~000 & 80~000& 80~000& 40~000\\
       $N_{\rm DM}$ &40~000 & 40~000& 40~000& 20~000\\
       \hline
  \end{tabular}
\end{table}