\begin{table}%t6
  \caption {\label{t:young}Parameters derived for the candidate young clusters.  }  
%\centerline
 {\begin{tabular}{@{}l@{\hspace{0.05in}}c@{\hspace{0.05in}}l@{\hspace{0.05in}}c@{\hspace{0.05in}}c@{\hspace{0.01in}}c@{\hspace{0.05in}}c@{\hspace{0.01in}}c@{}}
    \hline\hline
 ID & $R_{\rm h}$ & $V$ & ($B-V$) &$E(B-V)$&Age&$E (B-V)$&Age\\ 
    & (arcs) &      &       &             & (Myr)    &              & (Myr)    \\ 
    &          &      &       &\multicolumn{2}{c}{(this paper)} &\multicolumn{2}{c}{(C09)}   \\ 
    \hline
B049-G112 &1.20 & 17.56   & 0.52 & 0.30 & 280  & 0.25 & 400 \\
B090      &0.47 & 18.80   &      &      &      &      & old  \\
B367-G292 &0.94 & 18.45   & 0.32 & 0.25 & 200  & 0.25 & 200 \\
B458-D049 &1.60 & 17.84   & 0.49 & 0.25 & 320  & 0.25 & 500 \\
B515      &1.25 & 18.60$^1$&     &      &      &      &     \\  % 2 0 2 1y    B515               
B521-SK034A&0.75& 19.08$^1$&     & 0.55 & 400  & 0.38 & 250 \\  % 2 0 2 1y    B521      
M039      &0.62 & 18.94   &      & 0.10 & 320  & 0.18 & 320 \\  % 2 0 2 1y    M039$^4$                 
M050      &0.80 & 18.71   &      & 0.15 & 560  & 0.25 & 300 \\  % 2 0 2 1y    M050                   
B057-G118 &0.70 & 17.64   & 0.69 &      &      &      & old \\
    \hline
\end{tabular}}
\par
\smallskip
\par
Photometry is from G04 
  except when otherwise stated. $R_{\rm h}$ indicates the  half-light radius.\\
{$^1$: $V$ magnitude from C09.}
\end{table}