\begin{table}%t6
\caption{\label{table:literature}The properties of young massive clusters taken from the literature.}
%\centerline
{
\begin{tabular}{c c c c c c c c c c}
\hline\hline
Galaxy &  ID & Age &  $\Delta$age  &   $M_{\rm V}$  &  $R_{\rm eff}$   &
$\Delta$$R_{\rm eff}$ &  $\sigma$ &    $\Delta$$\sigma$ & Reference$^{a}$    \\ 
 & & (log~yr) &  (log~yr) & (mag) & (pc) & (pc) & (km~s$^{-1}$) &
 (km~s$^{-1}$)  \\
\hline
 {Young Massive Star Clusters} \\
 M   82   & F 	 & 7.6(6.6)  &  0.17  &  --14.2 &    1.5   &   0.5     &  13.4   &    0.7 &   1, 10 \\	
 M   82	  & MGG9 & 6.9  &  0.15  &  --13.43 &	  2.6   &   0.4	  &    15.9 &	 0.8 &   4 \\	 
 M   82	  & MGG11& 6.9  &  0.15  &  --13.23 &	  1.2   &   0.17  &    11.4 &	 0.8 &   4  \\	  	   
 NGC 1569 & A	 & 7.08 &  0.2   &  --14.1  &	  1.9	&   0.2	  &    15.7 &	 1.5 &	7, 8 \\	
 NGC 1705 & 1	 & 7.08 &  0.2   &  --14.0  &	  1.6	&   0.2	  &    11.4 &	 1.5 &	1, 9 \\	
 NGC 4038 & W99-15& 6.93 &  0.2  & --13.69  &	  3.6	&   0.5	  &    20.2 &	 0.7 &	6 \\	
 NGC 4038 & W99-2 & 6.95 &  0.2  & --14.79  &	  4.5	&   0.5	  &    14.2 &	 0.4 &	6 \\	
 NGC 4038 & W99-1 & 6.91 &  0.2  & --14.0   &	  3.6	&   0.5	  &    9.1  &	 0.6 &	6 \\	
 NGC 4038 & W99-16& 7.0  &  0.1  &  --12.70 &	  6.0	&   0.5	  &    15.8 &	 1.0 &	6 \\	
 NGC 4214 & 10	 & 8.3  &  0.1   &  --10.22 &	  4.33  &   0.1   &    5.1  &	 1.0 &   3 \\	 
 NGC 4214 & 13	 & 8.3  &  0.1   &  --11.68 &	  3.01  &   0.2   &    14.8 &	 1.0 &   3 \\	 
 NGC 4449 & 27	 & 8.9  &  0.25  &  --9.61  &	  3.72  &   0.32  &    5.0  &	 1.0 &   3 \\	 
 NGC 4449 & 47	 & 8.45 &  0.10  &  --10.74 &	  5.24  &   0.76  &    6.2  &	 1.0 &   3 \\	
 NGC 5236 & 502  & 8.0  &  0.1   &  --11.57 &   7.6   &   1.1	  &    5.5  &    0.2 &   2   \\       
 NGC 5236 & 805	 & 7.1  &  0.2   &  --12.17 &   2.8   &   0.4	  &    8.1  &	 0.2 &   2 \\	 
 NGC 6946 & 1447 & 7.05 &  0.10  &  --14.17 &	  10.2  &   1.6	  &    8.8  &	 1.0 &   3 \\		   
\hline
NGC 1316 & G114	 & 9.47 &  0.1	 & --13.0   &	  4.1	&   0.25  &
42.1 &	 2.8 &   this work \\     
NGC 7252 & W30	 & 8.6 &  0.1	 &  --14.6  &	  9.3   &   1.7	  &
27.5 &	 2.5 &	this work \\	 
NGC 7252 & W3	 & 8.6 &  0.1   &  --16.2  &	  17.5  &   1.8	  & 45   &	 5.0 &   5 \\	
 \hline
{Nuclear Star Clusters} & & & &  $M_{I}^{b}$& \\
NGC 300 & -- & -- & -- & --11.4 & 2.9  & -- &     13.3 & 2.0 & 11, 12\\
NGC 428 & -- & -- & -- & --13.1 & 3.4 & -- &	  24.4 & 3.7 & 11, 12\\
NGC 1042 & -- & -- & -- & --13.1 & 1.9 & -- & 32.0 & 4.8 & 11, 12\\ 
NGC 1493 & -- & -- & -- & --13.1 & 2.6 & -- & 25.0 & 3.8 & 11, 12\\
NGC 3423 & -- & -- & -- & --11.8 & 4.2 & -- & 30.4 & 4.6 & 11, 12\\
NGC 7793 & -- & -- & -- & --13.6 & 7.7 & -- & 24.6 & 3.7 & 11, 12\\
\hline
\end{tabular}}
\smallskip
\begin{list}{}{}
\item[$^{{a}}$] References: 1) Smith \& Gallagher~(\cite{Smith2001}); 2)
Larsen \& Richtler~(\cite{Larsen2004r}); 3) Larsen et~al.~(\cite{Larsen2004e}); 4) McCrady et~al.~(\cite{McCrady2003}); 5) Maraston et~al.~(\cite{Maraston2004}); 6) Mengel et~al.~(\cite{Mengel2002}); 7) Ho
\& Filippenko~(\cite{Ho1996b}); 8) Anders et~al.~(\cite{Anders2004}); 9) Ho \&
Filippenko~(\cite{Ho1996a}); 10) McCrady et~al. (\cite{McCrady2005}); 11) B{\" o}ker et~al. (\cite{ker2004}); 12) Walcher et~al. (\cite{Walcher2005}). 
\item[$^{{b}}$] For Fig.~\ref{fig:kspace} we have assumed $(B-I)=1.0$
which corresponds to a simple stellar population of $\sim$$400$~Myr and
solar metallicity, although we note that the assumed $(B-I)$
colour does not change the conclusions. 
\end{list}
\end{table}