\begin{table}%T2 
\caption{\label{UVOT2}Values plotted in Fig.~\ref{SFD}.}
\small%\centerline
{
\begin{tabular}{lcccc}
\hline\hline
Filter & $\lambda$  &  $\nu$($1+z$) &   mag  &  $F_\nu$ \\
       & (\AA)      &($10^{15}$~Hz)&        &  ($\mu$Jy)\\
\hline
$R_{\rm C}$  & 6588 &   2.17  &  $18.83\pm0.04$    & $90.40 \pm3.33$ \\
$v$    & 5402 &   2.65  &  $20.03\pm0.2$     & $35.38 \pm6.52$ \\
$b$    & 4329 &   3.31  &  $21.28\pm0.3$     & $13.09 \pm3.62$ \\
$u$    & 3501 &   4.09  &  $>$$22.13  $	     & $ <$$ 2.54 $	\\
$uvw1$ & 2634 &   5.43  &  $>$$21.33  $	     & $ < $$2.56 $	\\
$uvm2$ & 2231 &   6.41  &  $>$$23.33  $	     & $ < $$0.41 $	\\
$uvw2$ & 2030 &   7.05  &  $>$$21.33  $	     & $ < $$2.82 $	\\
\hline
\end{tabular}}
\smallskip
 The $u$, $uvw1$,  $uvm2$ and
$uvw2$ data are upper limits.  For all filters except~$R_{\rm C}$,  $\lambda$ is
from  Poole et~al. (\cite{Poole2008}). Data refer to $t=0.27$~days.  A
redshift of $z=3.773$ was assumed. The values have been corrected for
Galactic extinction. The fluxes have been calculated assuming the  conversion
factors from Bessell (\cite{Bessell1979}) and Poole et~al. (\cite{Poole2008}). 
\end{table}