\begin{table}
\scriptsize
\par
\caption{\label{tab:sed_input_IRS}Flux densities, in Jy, obtained from the IRS spectra for the
SED fits.}
%\centerline
 {\begin{tabular}{lrrrrrrrrrrrrrrrrr}
\hline\hline
Name / $\lambda$[$\mu$m] &     10.0 &     10.5 &     11.0 &     11.5 &     12.0 &     12.5 &     13.0 &     13.5 &     14.0 &     14.5 &     15.0 &     15.5 &     16.0 &     16.5 &     17.0 &     17.5 &     18.0\\
\hline
{\it DoAr25}
 & {\it     0.23} & {\it     0.23} & {\it     0.24} & {\it     0.27} & {\it     0.25} & {\it     0.25} & {\it     0.23} & {\it     0.23} & {\it     0.24} & {\it     0.22} & {\it     0.24} & {\it     0.25} & {\it     0.28} & {\it     0.30} & {\it     0.33} & {\it     0.36} & {\it     0.37}\\
{\it IRS14}
 & {\it    0.022} & {\it    0.022} & {\it    0.040} & {\it    0.094} & {\it    0.096} & {\it     0.11} & {\it    0.098} & {\it    0.081} & {\it    0.066} & {\it    0.061} & {\it    0.062} & {\it    0.066} & {\it    0.073} & {\it     0.11} & {\it     0.11} & {\it    0.095} & {\it    0.067}\\
WL12
 &     0.93 &      1.3 &      1.7 &      2.3 &      3.0 &      3.7 &      4.1 &      4.3 &      4.5 &      4.7 &      4.1 &      4.1 &      4.4 &      4.2 &      4.3 &      4.4 &      4.5\\
WL22
 &     0.16 &     0.25 &     0.62 &     0.87 &      1.0 &      1.4 &      1.1 &      1.1 &     0.96 &     0.96 &     0.44 &     0.48 &     0.96 &      1.5 &      1.3 &      1.4 &      1.1\\
WL16
 &      1.3 &      1.5 &      4.4 &      5.1 &      4.8 &      6.3 &      4.4 &      3.8 &      3.2 &      2.9 &      2.6 &      2.4 &      2.9 &      4.4 &      4.0 &      3.9 &      2.7\\
WL17
 &     0.18 &     0.21 &     0.27 &     0.31 &     0.34 &     0.37 &     0.42 &     0.48 &     0.48 &     0.52 &     0.51 &     0.54 &     0.64 &     0.64 &     0.70 &     0.74 &     0.76\\
{\it WL10}
 & {\it     0.17} & {\it     0.18} & {\it     0.19} & {\it     0.20} & {\it     0.21} & {\it     0.21} & {\it     0.21} & {\it     0.22} & {\it     0.22} & {\it     0.22} & {\it     0.23} & {\it     0.24} & {\it     0.25} & {\it     0.26} & {\it     0.27} & {\it     0.27} & {\it     0.28}\\
EL29
 &      7.2 &      9.5 &      12. &      16. &      19. &      22. &      23. &      24. &      24. &      26. &      22. &      22. &      24. &      24. &      24. &      25. &      25.\\
GY224      
 &     0.27 &     0.30 &     0.34 &     0.37 &     0.38 &     0.39 &     0.40 &     0.43 &     0.45 &     0.47 &     0.48 &     0.48 &     0.53 &     0.56 &     0.60 &     0.62 &     0.63\\
{\it WL19}
 & {\it    0.053} & {\it    0.071} & {\it    0.077} & {\it    0.096} & {\it     0.13} & {\it     0.15} & {\it     0.15} & {\it     0.16} & {\it     0.17} & {\it     0.18} & {\it     0.16} & {\it     0.15} & {\it     0.16} & {\it     0.14} & {\it     0.14} & {\it     0.15} & {\it     0.14}\\
{\it WL11}
 & {\it    0.012} & {\it    0.014} & {\it    0.011} & {\it    0.010} & {\it    0.014} & {\it    0.014} & {\it    0.015} & {\it    0.019} & {\it    0.017} & {\it    0.017} & {\it    0.022} & {\it    0.021} & {\it    0.027} & {\it    0.029} & {\it    0.034} & {\it    0.037} & {\it    0.033}\\
WL20
 &     0.34 &     0.45 &     0.59 &     0.73 &     0.83 &     0.89 &      1.0 &      1.2 &      1.4 &      1.6 &      1.6 &      1.8 &      2.3 &      2.5 &      2.8 &      3.1 &      3.4\\
{\it IRS37}
 & {\it     0.13} & {\it     0.17} & {\it     0.22} & {\it     0.26} & {\it     0.29} & {\it     0.33} & {\it     0.35} & {\it     0.37} & {\it     0.39} & {\it     0.43} & {\it     0.40} & {\it     0.42} & {\it     0.49} & {\it     0.53} & {\it     0.57} & {\it     0.63} & {\it     0.66}\\
{\it WL5}
 & {\it    0.015} & {\it    0.021} & {\it    0.029} & {\it    0.037} & {\it    0.052} & {\it    0.064} & {\it    0.062} & {\it    0.066} & {\it    0.065} & {\it    0.066} & {\it    0.047} & {\it    0.047} & {\it    0.068} & {\it    0.079} & {\it    0.088} & {\it     0.11} & {\it    0.098}\\
IRS42
 &      1.8 &      2.0 &      2.3 &      2.4 &      2.1 &      2.1 &      2.1 &      2.1 &      2.1 &      2.2 &      2.1 &      2.1 &      2.4 &      2.4 &      2.4 &      2.6 &      2.7\\
{\it GY253      }
 & {\it  9.4e-05} & {\it  0.00031} & {\it  -0.0015} & {\it  -0.0021} & {\it   0.0024} & {\it  0.00084} & {\it   0.0028} & {\it   0.0059} & {\it   0.0035} & {\it   0.0023} & {\it   0.0051} & {\it   0.0024} & {\it   0.0047} & {\it   0.0048} & {\it   0.0080} & {\it   0.0092} & {\it   0.0058}\\
WL6
 &     0.73 &     0.92 &      1.1 &      1.4 &      1.6 &      1.8 &      2.0 &      2.1 &      2.2 &      2.4 &      1.9 &      2.0 &      2.4 &      2.5 &      2.6 &      2.7 &      2.8\\
{\it CRBR85     }
 & {\it    0.066} & {\it     0.10} & {\it     0.14} & {\it     0.18} & {\it     0.23} & {\it     0.27} & {\it     0.31} & {\it     0.35} & {\it     0.39} & {\it     0.43} & {\it     0.35} & {\it     0.37} & {\it     0.49} & {\it     0.51} & {\it     0.55} & {\it     0.62} & {\it     0.65}\\
IRS43
 &     0.87 &      1.2 &      1.7 &      2.3 &      2.9 &      3.5 &      4.0 &      4.4 &      4.9 &      5.4 &      4.0 &      4.4 &      5.6 &      5.8 &      6.3 &      6.8 &      7.3\\
IRS44
 &      1.5 &      2.4 &      3.5 &      5.3 &      7.2 &      8.7 &      10. &      12. &      13. &      15. &      13. &      14. &      17. &      18. &      20. &      22. &      24.\\
IRS45
 &     0.34 &     0.40 &     0.44 &     0.48 &     0.46 &     0.48 &     0.48 &     0.50 &     0.52 &     0.53 &     0.49 &     0.52 &     0.59 &     0.57 &     0.60 &     0.64 &     0.63\\
IRS46
 &     0.31 &     0.39 &     0.48 &     0.57 &     0.66 &     0.72 &     0.76 &     0.81 &     0.83 &     0.87 &     0.85 &     0.88 &     0.93 &     0.96 &      1.0 &      1.0 &      1.1\\
IRS47
 &      1.2 &      1.3 &      1.5 &      1.6 &      1.6 &      1.6 &      1.6 &      1.6 &      1.7 &      1.7 &      1.4 &      1.5 &      1.7 &      1.6 &      1.7 &      1.7 &      1.8\\
{\it GY289      }
 & {\it   0.0039} & {\it   0.0065} & {\it   0.0080} & {\it    0.011} & {\it    0.013} & {\it    0.014} & {\it    0.015} & {\it    0.021} & {\it    0.018} & {\it    0.019} & {\it    0.024} & {\it    0.023} & {\it    0.030} & {\it    0.035} & {\it    0.037} & {\it    0.041} & {\it    0.036}\\
{\it GY291      }
 & {\it    0.055} & {\it    0.060} & {\it    0.063} & {\it    0.064} & {\it    0.062} & {\it    0.062} & {\it    0.063} & {\it    0.065} & {\it    0.063} & {\it    0.064} & {\it    0.064} & {\it    0.063} & {\it    0.075} & {\it    0.085} & {\it    0.091} & {\it    0.095} & {\it    0.091}\\
IRS48
 &      2.4 &      2.6 &      4.3 &      4.7 &      4.5 &      4.9 &      4.6 &      5.1 &      5.8 &      6.7 &      8.0 &      9.2 &      12. &      14. &      16. &      18. &      20.\\
IRS51
 &      1.2 &      1.3 &      1.3 &      1.3 &      1.3 &      1.2 &      1.2 &      1.3 &      1.3 &      1.4 &      1.1 &      1.3 &      1.7 &      1.8 &      2.0 &      2.1 &      2.2\\
IRS54
 &     0.48 &     0.59 &     0.73 &     0.89 &      1.0 &      1.1 &      1.2 &      1.2 &      1.3 &      1.4 &      1.4 &      1.5 &      1.7 &      1.7 &      1.8 &      1.9 &      2.1\\
\hline
\end{tabular}}
\par
\smallskip
Note: values in italic were considered uncertain and were not used for the SED fits.
\end{table}