\begin{table}%t2
  \caption{\label{tab:IRflux}Net fluxes for the {dust emission by the} entire galaxy used 
             for the modeling.
             The values take account of all the corrections mentioned in the
             text.
             $^a$~Madden et~al. (\cite{Madden2003}), $^b$~Hunter et~al. (\cite{Hunter1989a}),
             $^c$~Hunter et~al. (\cite{Hunter1989b}), $^d$~Stickel et~al. (\cite{Stickel2000})
             \& full catalog in prep., $^e$~this paper, 
             $^f$~Lisenfeld et~al. (\cite{Lisenfeld2002}).}
    %\centering
\par
    \begin{tabular}{*{4}{l}}
     \hline
     \hline
       Instrument & ${\lambda\; (\mu }$m) 
       & ${\Delta\lambda\; (\mu }$m) &   Net flux (mJy)      \\
     \hline
       ISOCAM         & 8.8          & 0.05          & $(370\pm 220)^a$   \\
                      & 10.1         & 0.96          & $(480\pm 230)^a$   \\
                      & 10.8         & 0.87          & $(610\pm 210)^a$   \\
                      & 11.8         & 0.73          & $(860\pm 220)^a$   \\
                      & 12.1         & 0.69          & $(980\pm 220)^a$   \\
                      & 13.2         & 0.54          & $(1070\pm 220)^a$  \\
                      & 13.9         & 0.45          & $(1270\pm 230)^a$  \\
                      & 14.6         & 0.35          & $(1420\pm 240)^a$  \\
                      & 15.0         & 0.30          & $(1470\pm 250)^a$  \\
                      & 16.0         & 0.16          & $(1990\pm 290)^a$  \\
     \hline
       IRAS           & 24.3         & 6.3           & $(8550\pm 1100)^b$ \\
                      & 62.8         & 19            & $(48~900\pm 7000)^b$\\
                      & 103          & 22            & $(54~800\pm 8000)^b$\\
     \hline
       KAO            & 155          & 30            & $(36~000\pm 11~000)^c$\\
     \hline
       ISOPHOT        & 174          & 90            & $(28~000\pm 9800)^d$\\
     \hline
       SCUBA          & 443          & 20            & $(1280\pm 450)^e$  \\
                      & 863          & 70            & $(280\pm 60)^e$    \\
     \hline
       IRAM           & 1200         & 200           & $(190\pm 60)^f$    \\
     \hline
    \end{tabular}
       \end{table}