\begin{table}%t1
\caption{\label{table_data_sup}Summary of the Subaru/Suprime-Cam and CFHT/Megaprime data.}
%\centering
\par
\begin{tabular}{l r r r r}
\hline
\hline\noalign{\smallskip}
Telescope/Instrument & Filter (abbr.) & $t_{\rm exp}$ [s] & Seeing & $M_{\rm lim}$\\
\hline
\noalign{\smallskip}
Subaru/Suprime-Cam & WJB  ($B$) & 12~240 & 0\farcs82 & 26.7 \\
Subaru/Suprime-Cam & WJV  ($V$) & 5040  & 0\farcs95 & 26.0 \\
Subaru/Suprime-Cam & WCRC ($R$) & 11~400 & 0\farcs83 & 26.6 \\
Subaru/Suprime-Cam & WCIC ($I$) & 4920  & 0\farcs92 & 25.9 \\
Subaru/Suprime-Cam & WSZ  ($z$) & 4380  & 0\farcs76 & 25.1 \\
\hline
CFHT/Megaprime & $u^*$ & 5220  & 0\farcs87 & 25.7\\
CFHT/Megaprime & $g$   & 3400  & 0\farcs85 & 26.0\\
CFHT/Megaprime & $r$   & 14~850 & 0\farcs71 & 26.2\\
CFHT/Megaprime & $i$   & 1280  & 0\farcs71 & 23.7\\
CFHT/Megaprime & $z$   & 1440  & 0\farcs70 & 22.4\\
\hline
\end{tabular}
\tablefoot {The limiting AB magnitudes (50\% completeness limit) are for $10\sigma$~point sources, and are on average 0.8~mag brighter for extended objects.}
\end{table}