\begin{table}%t6
    %\centering
\par
\caption{Results from model SEDs for known cluster galaxies in Cl~0024+1654. The columns list: LW3
identification number; best-fit SED~model; number of data points in the observed SED; $\chi^2$ of the fit;
rejection probability of the fit; other acceptable models (rejection probability 95\% or less); 15~$\mu$m
\mbox{k-correction}; luminosity at 15~$\mu$m ($h=0.7$, $\Omega_{\rm m}=0.3$, $\Omega_l=0.7$) using the transformation from
Boselli et~al. (\cite{1998AetA...335...53B}), and k-corrected using best-fit SED; total infrared luminosity
including the \mbox{k-correction} using the best-fit SED and computed using the transformation from Elbaz et~al.
(\cite{2002AetA...384..848E}); SFR from total IR luminosity using the transformation of Kennicutt
(\cite{1998ARAetA..36..189K}); position in the $V-I$ vs. $I$~colour--magnitude diagram (Fig.~\ref{fig:color}) where
"MS'' stands for "Main Sequence'', "BO'' for "Butcher-Oemler'', "U'' for "Unknown''; EW~[\ion{O}{ii}] line from
Czoske et~al. (\cite{2001AetA...372..391C}); SFR computed from the [\ion{O}{ii}] emission line using the
transformation to the optical SFR; ratio infrared to optical SFR. \label{sfrir}}
    \leavevmode\scriptsize\begin{tabular}{cccccccccccccc}
\hline
         \hline
id. & Best-fit & $\sharp$ of & $\chi^2$&Rejection  & Other SED & k-corr.&$L_{15~\mu {\rm m}}$& $L_{\rm IR}$&{\it SFR}[IR]&Colour&{\it EW}[\ion{O}{ii}]   & {\it SFR}[\ion{O}{ii}]& {\it SFR}[IR]/\\
   & model    & data points &         &Probability& models    &             & ($L_\odot$)          &  ($L_\odot$)   & ($M_\odot$~yr$^{-1}$)& Fig.~8 &(\AA)&($M_\odot$~yr$^{-1}$)&   {\it SFR}[\ion{O}{ii}]\\
\hline \noalign{\smallskip}
 05& S    & 12 & 17.8 & 96.2 &None              & 1.45 & 2.03e+09 & 9.56e+10 & 16 & U  & --    &  -- &  --  \\
 08& SB+1 & 15 & 23.4 & 97.6 &None              & 1.80 & 9.66e+09 & 4.54e+11 & 77 & BO & --    &  -- &  --  \\
 10& S    & 4  & 1.9  & 79.8 &S, SB+1    & 1.46 & 2.21e+09 & 1.04e+11 & 18 & BO & --    &  -- &  --  \\
 18& S    & 11 & 3.9  & 13.4 &E, S, SB+1  & 1.46 & 7.85e+09 & 3.69e+11 & 63 & BO &--    &  -- &  --  \\
 21& S    & 7  & 5.4  & 74.7 &SB+1, S         & 1.46 & 2.11e+09 & 9.93e+10 & 17 & BO & --    &  -- &  --  \\
 22& S    & 11 & 7.6  & 52.6 &S, SB+1  & 1.46 & 3.96e+09 & 1.87e+11 & 32 & BO & 17.5 & 4.9& 6.5\\
 24& S    & 4  & 1.2  & 79.8 &E, SB+1, S       & 1.42 & 2.07e+09 & 9.74e+10 & 17 & MS & 5.0  & 0.8& 21.3\\
 26& S    & 4  & 1.4  & 79.8 &S, SB+1       & 1.73 & 4.51e+09 & 2.17e+11 & 36 & --  & --    & --  &  --  \\
 27& SB+1 & 8  & 6.7  & 87.8 &SB              & 1.80 & 5.50e+09 & 2.59e+11 & 44 & MS & --    & --  &  --  \\
 1s& S    & 10 & 8.6  & 71.4 &E, E, S, SB+1   & 1.73 & 1.96e+09 & 9.23e+10 & 16 & BO & 9.6  & 1.0& 16.0\\
 3s& SB+1 & 4  & 1.3  & 79.8 &S, SB+1, E  & 1.80 & 1.59e+09 & 7.48e+10 & 13 & MS & --    &  -- &  --  \\
 4s& E    & 20 & 9.4  & 7.3  &E, S, SB+1 & 0.78 & 9.87e+08 & 4.66e+10 & 8  & MS & --    &  -- &  --  \\
   \hline
      \end{tabular}
\end{table}