\begin{table}%t5
\caption{\label{tab:coef}Globular cluster number density profiles.} 
\small%\centering
\par
\begin{tabular}{lllll} 
\hline  \hline\noalign{\smallskip}
& \multicolumn{1}{c}{$N_0$} & \multicolumn{1}{c}{$R_{0}$} 
& \multicolumn{1}{c}{$\alpha$} 
& \multicolumn{1}{c}{$\mathcal{B}\left(\frac{1}{2},\alpha \right)$} 
\\ 
\par
& \multicolumn{1}{c}{[$\rm{GCs~ arcmin}^{-2}$]} & \multicolumn{1}{c}{[arcmin]} 
& \multicolumn{1}{c}{} 
& \multicolumn{1}{c}{}
\\ \hline
Red & 28.43 $\pm$ 7.82 &1.63 $\pm$ 0.34  & 1.02 $\pm$ 0.04 & 1.98 \\
Blue &8.39 $\pm$ 1.05 &2.91 $\pm$ 0.42 & 0.79 $\pm$ 0.03  & 2.32\\
All & 35.54 $\pm$ 6.13 &1.74 $\pm$ 0.27 & 0.84 $\pm$ 0.02 & 2.22 \\
\hline 
\end{tabular}
\tablefoot{Fitting a cored
power-law (Eq.~(\ref{eq:corepl})) to the data given in Table~\ref{tab2} of
\cite{bassino06} yields the parameters listed above (the profile for
``all'' GCs was obtained by adding the number counts of the red and
blue GCs).}
\end{table}