\begin{table}%t3
\caption{The compiled spectral energy distribution of
Cluster~5. Aperture size are listed when appropriate (i.e. mostly for
single-beam measurements). A few telescopes and filter bandwidths are
missing because we were unable to find the information in the original
papers.\label{tab:sed}}
%\centerline
{\begin{tabular}{llrrrrl}
\hline\hline
Telescope/instrument & Filter name & $\lambda$ & $\Delta\lambda$ & Aperture 
& Flux & Source \\
 & & \mic & \mic & \arcsec & mJy & \\
\hline
HST/WFPC2      & $F255W$ & 0.2574 & 0.041 & & 0.179 & C97 \\
HST/WFPC2      & $F547M$ & 0.5465 & 0.049 & & 0.259 & C97 \\
HST/WFPC2      & $F814W$ & 0.8370 & 0.176 & & 0.198 & C97 \\
VLT/ISAAC      & $K\rm s$    & 2.16   & 0.27  & & 2.65 & this work \\
VLT/ISAAC      & $L'$    & 3.78   & 0.58  & & 77.2 & this work \\
ISO/ISOCAM     & $LW1$   & 4.5    & 1.0   & &     $ 125\pm30 $& this work \\
CTIO 1.5   4~m &	   & 7.8    & 0.6	& 8.2 & $ 866\pm234$ & \citet{fro82} \\
ESO 3.6~m      & $N1$    & 8.3    & 0.85  & 7.5 & $ 676\pm32 $& \citet{moo82} \\
CTIO 1.5   4~m &	   & 8.6    & 1.0	& 8.2 & $ 817\pm106$ & \citet{fro82} \\
ESO 3.6~m      & $N2$    & 9.4    & 1.65  & 7.5 & $ 904\pm43 $& \citet{moo82} \\
CTIO 1.5   4~m &	   & 9.6    & 0.9	& 8.2 & $1070\pm150$ & \citet{fro82} \\
CTIO 1.5   4~m &	   & 10.0   & 5.1	& 8.2 & $1300\pm80 $& \citet{fro82} \\
               &       & 10.0   & 5.4   & 6.0 & $2130\pm150$$^a$ & \citet{rie72} \\
ESO 3.6~m       & $N$     & 10.3   & 5.2   & 7.5 & $1210\pm60 $& \citet{moo82} \\
CTIO 1.5   4~m &       & 10.4   & 1.8   & 8.2 & $1540\pm170$ & \citet{fro82} \\
               &       & 10.4   & 1.3   & 8.5 & $1365\pm90 $& \citet{leb79} \\
               &       & 10.6   & 5     & 8.5 & 1500 & \citet{leb79} \\
CTIO 1.5   4~m &       & 11.4   & 2.1   & 8.2 & $1570\pm190$ & \citet{fro82} \\
Keck/LWS       &       & 11.7   & 1.0   & & $2200\pm200$ & \citet{gor01} \\
ESO 3.6~m       & $N3$    & 12.0   & 3.7   & 7.5 & $1670\pm200$ & \citet{moo82} \\
ISO/ISOCAM     & $LW10$  & 12.0   & 7.0   & & $1900\pm300$ & this work \\
IRAS           & 12    & 12.0   & 7.0   & & $2610\pm131$$^b$ 
& \citet{mos90} \\
CTIO 1.5   4~m &       & 12.4   & 1.3   & 8.2 & $2040\pm450$ & \citet{fro82} \\
ISO/ISOCAM     & $LW9$   & 14.9   & 2.0   & & $3900\pm400$ & this work \\
ESO 3.6~m       & $Q$     & 17.4   & 5.6   & 7.5 & $5500\pm539$ & \citet{moo82} \\
Keck/LWS       &       & 18.7   & 0.5   & &     $2900\pm300$$^{a}$ & 
\citet{gor01} \\
CTIO 1.5   4~m &       & 20.0   & 5.9   & 8.2 & $6100\pm900$ & \citet{fro82} \\
               & $Q$     & 21.0   &       & 6.0 & $3700\pm400$$^{a}$ & 
\citet{rie72} \\
IRAS           & 25    & 25.0   & 11.15 & & $12~000\pm600$$^{b}$ & 
\citet{mos90} \\
IRAS           & 60    & 60.0   & 32.5  & & $30~500\pm1220$$^{b}$ & 
\citet{mos90} \\
IRAS           & 100   & 100.0  & 31.5  & & $29~400\pm1760$$^{b}$ & 
\citet{mos90} \\
JCMT/SCUBA     &       & 850.0  & 62    & 41 & $151\pm23$$^c$ & \citet{jam02} \\  
SEST/SIMBA     &       & 1200.0 & 465   & & $71\pm4^{c}$ & this work \\
OVRO           &       & 2600.0 & 22.6  & & $<$$26^{c}$ & \citet{tur97} \\
\hline
\end{tabular}}
\par
\smallskip
$^a$ This 
measurement is not used as a constraint for the SED fit, see text for 
details.\\
$^b$ Only 75\% 
of this flux is used as a constraint for the SED fit, see text for details.\\
$^c$ Corresponds
to the dust-only flux, see text for details.
\end{table}