\begin{table}%t1
\caption{\label{tab1}GCS radial distribution parameters.}
%\centerline
{
\begin{tabular}{l c c c c c c}
\hline
\hline
{Galaxy} & {$\Sigma_0$} & {$r_{\rm c}$} & {$\gamma$} & {$r_{\max}$}& {$R$}
\\
\hline
{NGC~1400}  & 14.1 & 0.7 & 0.88 &2.3& 2.8\\
{NGC~1407}  & 17.8 & 1.02 & 0.85 &2.34 & 7.3\\
{NGC~3258} & 16.9 & 3.1 & 2.4 &  2.51 & 7.94\\
{NGC~3268} & 24.4 & 2.6 & 1.9 & 2.51 & 7.94\\
{NGC~4374} & 58.4 & 0.31 & 0.278 &  3.84 & 11.8\\
{NGC~4406} & 26.76 & 3.52 & 1.19 & 5.36 & 24\\
{NGC~4472} &107& 8.47 & 0 & 7& 22\\
{NGC~4636} & 77.66 & 0.823 & 0.691 & 4.75 & 6.6\\
\hline
\end{tabular}}
\medskip
Column 1: galaxy name; Cols. 2, 3 and 4: parameters of the modified core model fit for all the galaxies studied; Col. 5: superior limit of the integral giving the number of lost GCs  ($r_{\max}$); Col. 6: superior limit  of the integral performed to estimate the present  number of
GCs ($R$), where $\Sigma_0$ is in arcmin$^{-2}$ and $r_{\rm c}$, $r_{\max}$ and $R$ are in arcmin.
\end{table}