\begin{table}%t5
\caption{\label{table:radio:isoflux}Radio flux densities integrated over the 12 SWS apertures and the LWS
  aperture. The official band range in \mum\ is given for every aperture.}
  %\centerline
{
    \begin{tabular}[h]{crrrrrrrrrrrrc}\\
      \hline \hline 
    \multicolumn{1}{c}{} &
    \multicolumn{13}{c}{Integrated flux density (mJy)} 
\\[5pt]
\cline{2-14} \\[-2pt]
 Source & 1A & 1B & 1D & 1E &  2A & 2B & 2C & 3A & 3C & 3D & 3E & 4 & LWS$^\star$\\
&{\scriptsize (2.38--2.61)}&{\scriptsize (2.60--3.03)}& 
{\scriptsize (3.02--3.53)}&{\scriptsize (3.52--4.06)} & 
{\scriptsize (4.05--5.31)}&{\scriptsize (5.30--7.01)} &
{\scriptsize (7.00--12.1)}&{\scriptsize (12.0--16.6)} & 
{\scriptsize (16.5--19.6)}&{\scriptsize (19.5--27.6)} & 
{\scriptsize (27.5--29.0)}&{\scriptsize (28.9--45.2)} &
{\scriptsize (43.0--196.0)}
\\[5pt] \hline \\[-5pt]
IRAS~01045 &205   &204   &205   &206   &210   &210   &207   &230   &235   &232   &238   &230  & $\dagger$   \\
IRAS~10589 &766   &766   &765   &770   &789   &781   &769   &687   &677   &678   &765   &728  & 1210  (19)  \\ 
IRAS~11143 &284   &284   &286   &288   &318   &315   &314   &332   &333   &345   &479   &554  & 1981  (79)  \\
IRAS~12063 &1261  &1261  &1272  &1267  &1300  &1278  &1269  &1484  &1437  &1441  &1534  &1481 & 1959  (23)  \\
IRAS~12073 &3655  &3660  &3684  &3702  &3936  &3886  &3864  &4906  &4708  &4919  &4765  &5502 & 14092 (889) \\
IRAS~12331 &231   &233   &236   &238   &278   &274   &277   &338   &342   &371   &584   &707  & 3059  (310) \\
IRAS~15384 &1495  &1496  &1506  &1508  &1581  &1559  &1549  &1756  &1719  &1749  &1956  &2064 & 4435  (208) \\
IRAS~15502 &1342  &1341  &1367  &1344  &1362  &1286  &1269  &1668  &1642  &1597  &1952  &1875 & 2707  (85)  \\
IRAS~16128 &390   &400   &413   &415   &478   &468   &489   &894   &917   &1021  &1931  &2076 & 7468  (428) \\
IRAS~17160 &563   &567   &578   &575   &621   &605   &611   &860   &850   &890   &1223  &1300 & 3940  (267) \\
IRAS~17221 &343   &344   &347   &349   &392   &386   &385   &405   &419   &431   &636   &731  & 2451  (181) \\
IRAS~17279 &187   &187   &187   &189   &198   &196   &194   &183   &185   &193   &253   &282  & 930   (23)  \\
IRAS~18032 &367   &367   &366   &369   &380   &375   &367   &288   &285   &292   &349   &340  & 609   (11)  \\
IRAS~18479 &2137  &2136  &2128  &2138  &2151  &2120  &2087  &1740  &1710  &1712  &2044  &1880 & 2751  (29)  \\
IRAS~19442 &73    &73    &73    &73    &76    &75    &75    &69    &65    &65    &64    &61   & 93    (2)  \\
IRAS~19598 &3348  &3348  &3351  &3353  &3401  &3410  &3396  &3352  &3326  &3264  &3348  &3030 & 3662  (29)  \\
DR21      &604   &603   &601   &608   &640   &623   &609   &381   &443   &444   &694   &786  & 1556  (52)  \\
IRAS~23133 &619   &619   &621   &622   &626   &621   &613   &670   &672   &654   &702   &669  & 738   (3) 
\\[5pt] \hline 
\multicolumn{14}{l}{{$^\dagger$ No LWS observation available.
$^\star$ Given is the average of the integrated flux density
obtained from two different methods (see Sect.~\ref{sect:radio:iso}).
The number in brackets is the difference
}}\\
\multicolumn{14}{l}{{\small in mJy between these two methods.
}}
      \end{tabular}}
\end{table}