\begin{table}%t4
   	 \caption{The flux of \object{LBQS~2212-1759} as a function of
	 wavelength, from the near-IR to the EUV. The values in the
	 optical and  UV have been obtained by averaging fluxes from individual
	 OM exposures. All fluxes have been corrected for foreground 
	 galactic reddening.}
   	    \label{MeanFlux}
   	    %\centering
\par
	 \begin{tabular}{c c c c c c} % 6 columns 	 
         \hline\hline
Instrument  & ${\rm \lambda_{obs}}$ & ${\rm \Delta\lambda_{obs}}$ & ${\rm \lambda_{rest}}$ & ${\rm \Delta\lambda_{rest}}$ & Flux \\
            &  \multicolumn{4}{c}{(\AA)} & (${\rm 10^{-16}~erg~cm^{-2}~s^{-1}~\AA^{-1}}$) \\
         \hline
2MASS $K$ & 21~590               &  2620                  & 6711 & 814 & $0.945\pm0.047$    \\  
2MASS $H$ & 16~620               &  2510                  & 5166 & 780 & $1.006\pm0.071$    \\ 
2MASS $J$ & 12~350               &  1620                  & 3839 & 504 & $0.987\pm0.082$    \\  
OM-$V$    & 5430                &  710                    & 1688 & 221 & $2.957\pm0.040$    \\
OM-$B$    & 4500                &  980                    & 1399 & 305 & $4.673\pm0.018$    \\
OM-$U$    & 3440                &  780                    & 1069 & 242 & $4.478\pm0.026$    \\
OM-$UVW1$ & 2910                &  710                    & 905   & 221 & $4.186\pm0.013$    \\
OM-$UVM2$ & 2310                &  460                    & 718   & 143 & $3.447\pm0.082$    \\
OM-$UVW2$ & 2120                &  460                    & 659   & 143 & $2.868\pm0.379$    \\
 \hline 				        	   
 \end{tabular}
 \end{table}