\begin{table}%t8
%\centering
\par
\caption{Contamination of ground-based sample for individual galaxies.
  $N_{\rm tot}$ is the total number of cluster candidates identified in the
  ground-based surveys, $N_{\rm HST}$ is the subset of those candidates covered
  by HST images and $N_{<0.5 {\rm pc}}$ is the number of unresolved
  sources. The adopted distance moduli are also listed (see Paper~I for 
  references).}
\label{tab:contam}
\begin{tabular}{lllllll} \hline \hline
  Galaxy   & $m-M$ & $N_{\rm tot}$ & $N_{\rm HST}$ & $N_{<0.5 {\rm pc}}$ & 
    \multicolumn{2}{c}{$L_{\rm HST}$/$L_{>0.5 {\rm pc}}$} \\ 
           &               &               &          &          & $V$ & $U$ \\
  \hline
% \input ../contam.tex
NGC  628 & 29.6 &  38 &  22 &   3 &  0.84 &  0.82 \\
NGC 1156 & 29.5 &  22 &  21 &   5 &  0.85 &  0.86 \\
NGC 1313 & 28.2 &  45 &  20 &   2 &  0.81 &  0.68 \\
NGC 2835 & 28.9 &   9 &   8 &   6 &  0.20 &  0.17 \\
NGC 2997 & 29.9 &  34 &   8 &   1 &  0.96 &  0.98 \\
NGC 3184 & 29.5 &  13 &   9 &   3 &  0.79 &  0.83 \\
% NGC 3521 &      &  13 &   0 &   0 &  1.00 &  1.00 \\
NGC 3621 & 29.1 &  45 &  29 &   6 &  0.79 &  0.75 \\
NGC 4258 & 29.47 &  44 &  26 &   2 &  0.91 &  0.91 \\
NGC 5055 & 29.2 &  24 &  13 &   3 &  0.77 &  0.76 \\
NGC 5194 & 29.6 &  69 &  33 &   2 &  0.99 &  0.99 \\
NGC 5204 & 28.4 &   7 &   6 &   5 &  0.23 &  0.26 \\
NGC 5236 & 27.9 & 149 &  29 &   9 &  0.79 &  0.82 \\
NGC 5585 & 29.2 &   9 &   7 &   5 &  0.49 &  0.60 \\
NGC 6744 & 28.5 &  18 &   4 &   0 &  1.00 &  1.00 \\
NGC 6946 & 28.9 & 107 &  78 &  11 &  0.88 &  0.90 \\
NGC 7424 & 30.5 &  10 &   6 &   0 &  1.00 &  1.00 \\
NGC 7793 & 27.6 &  20 &  11 &   6 &  0.46 &  0.53 \\
\hline
\end{tabular}
\end{table}