\begin{table}%T1
%\centering
\par
   \caption{Contribution to the CIB of $S_{24} \ge 60~\mu$Jy
galaxies. Sources of uncertainty come from photometry, calibration,
and large scale structure. The CIB column gives the best estimate
from the discussion in Sect.~\ref{section:ValueCIB}.}
   \label{tab:CIBcontrib}
   \begin{tabular}{lcccc}
   \hline \hline
        $\lambda$  & $\nu I_{\nu}$  & B$_{\lambda}$  &    CIB    & \% CIB \\
        $\mu$m     & nW~m$^{-2}$~sr$^{-1}$ &~MJy/sr &  ~MJy/sr  & resolved\\%[+5pt]
        \hline%\\[-5pt]
                24      & $ 2.16 \pm  0.34 $  &  $  0.017 \pm 15 $\%  &  $  0.022 $  &  $   79 $ \\
                70      & $ 5.93 \pm  1.02 $  &  $  0.138 \pm 17 $\%  &  $  0.15 $  &  $   92 $ \\
                160     & $10.70 \pm  2.28 $  &  $  0.571 \pm 21 $\%  &  $  0.82 $  &  $   69 $ \\
    \hline
    \end{tabular}
 \end{table}