\begin{table}%t2
\caption{\label{sed_fit}Fraction of different stellar populations for the best fit to the SED of J033227.07-274404.7.}
%\centering
\par
\begin{tabular}{l  c   c c    c c    r r   c c   c c c }
\hline\hline
 & &\multicolumn{2}{c}{Young (Myr)} & & &\multicolumn{2}{c}{Intermediate (Gyr)} & & &\multicolumn{3}{c}{Old (Gyr)} \\
            & & 15       & 200  & & & 0.5  & 1    & & & 4    & & 7 \\
\hline
best fit    & & $<$0.01 & 0.16 & & & 0.08 & 0.05 & & & 0.05 & & 0.65 \\
median 68\% & & $<$0.01 & 0.15 & & & 0.22 & 0.07 & & & -- & 0.55 & -- \\
\hline
best fit    & &\multicolumn{2}{c}{0.17} & & &\multicolumn{2}{c}{0.13} & & &\multicolumn{3}{c}{0.70} \\ 
median 68\% & &\multicolumn{2}{c}{0.13 $\pm$ 0.07} & & &\multicolumn{2}{c}{0.32 $\pm$ 0.18} & & & \multicolumn{3}{c}{0.55 $\pm$ 0.21}  \\
\hline 
\end{tabular}
\end{table}