\begin{table}%t5
%\centering
\par
\caption{\label{tab:fitq}Residuals between the model and the observation.
For each COBE/DIRBE map we present the percentage of the 
Galaxy's area with residuals less than $<$10\%, $<$20\%, and $<$50\%.} 
\small%\centering
\par
\begin{tabular}{lccc}
\hline\hline
Wavelength ($\mu$m) & $<$10\%  & $<$20\% & $<$50\% \\
\hline
1.2                  &   29\% &  53\% &   92\% \\
2.2                  &   32\% &  55\% &   87\% \\
60                   &   26\% &  52\% &   88\% \\
100                  &   23\% &  43\% &   81\% \\
140                  &   28\% &  51\% &   81\% \\
240                  &   18\% &  37\% &   75\% \\
\hline
HI                   &   17\% &  38\% &   85\% \\
H$_2$                &   17\% &  35\% &   67\% \\
\hline
\end{tabular}
\end{table}