\begin{table}%t1
\caption{\label{table:size114}Effective radius of NGC~1316:G114 for various models as
determined from the $F450W$ WFPC2 image.  See text for details.  The
best fitting model (lowest $\chi^2$) is shown in bold.}
%\centerline
{
\begin{tabular}{c c c c c}
\hline\hline
{\bf WFPC2} & Type & Index & $R_{\rm eff}$(pc) & $\chi^2 / \chi^2_{\rm best}$$^{b}$ \\
\hline
 & Gauss & -- & 4.34  &   1.93\\
 & King & 5 &  4.27  &    1.54\\
 & King & 15 & 3.89 &     1.13\\
 & King & 30 & 3.66   &   1.24\\
 & King & 100 & 4.14  &   1.87\\
 & Moffat & 1.5 & 4.34  &  1.09\\
 & Moffat & 2.5 & 4.09  &  1.14\\
\hline
\noalign{\smallskip}
 &  {\bf Moffat$^a$} & {\bf 1.76} & {\bf 4.08} & {\bf 1.0} \\
\noalign{\smallskip}
\hline
{\bf ACS} & Filter & Type & index & $R_{\rm eff}$  \\
\hline
& $F555W$ & Moffat & 1.76 &$4.83  \pm0.25$ \\
& $F814W$ & Moffat & 1.76 &$3.68  \pm0.1$ \\
\hline
\end{tabular}}
\smallskip
\begin{list}{}{}
\item[$^{{a}}$] Best fitting model of the WFPC2 observations.
\item[$^{{b}}$] Calculated individually for the different cameras.
\end{list}
\end{table}