\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}