\begin{table}%t1
%\centering
\par
\caption
{\label{tab:photom} 
Table of photometry \citep[taken from][]{larsen04_cat}, ``background factors'' 
and the average background contribution
for the five clusters  observed. 
%Both the cluster nomenclature and the
%  photometry is taken from the catalogue   of \citet{larsen04_cat}. 
%  The sky factors indicate the value by which each galaxy
%  background fibre (low, mid and high) needs to be multiplied to
%  match the value of the galaxy background 
%  adjacent to each cluster, as implied from  aperture photometry.
%{\bf The relative contribution of the scaled, average background
%  spectra to the cluster~+~background  spectra are also included.}
}
\begin{tabular}{lccccccccc} \hline\hline
%%
Cluster &\multicolumn{5}{c}{Photometry (mag)}     &\multicolumn{3}{c}{Background factors} & Background  \\
        &$V$    &$U-B$  &$B-V$  &$V-I$  &$814W$  & Low & Mid & High &contribution ($\%$)\\ \hline
347     &18.27  &--0.62  &--0.06  &0.40   &19.61   & 1.0 & 0.7 & 0.5  &79\\
645     &18.16  &--0.38  &0.23   &0.39   &19.56   & 1.2 & 0.8 & 0.6  &89\\
747     &17.36  &--0.65  &0.25   &0.57   &19.80   & 1.4 & 1.0 & 0.7  &76\\
805     &16.60  &--0.55  &0.19   &0.65   &17.68   & 1.5 & 1.1 & 0.8  &62\\
897     &16.95  &--0.16  &0.51   &0.75   &19.83   & 1.7 & 1.3 & 0.9  &86\\ \hline
\end{tabular}
\end{table}