\begin{table}%t6
\par
\caption{Derived parameters from model fits.}

\begin{tabular}{lcclllcccccc}
\hline\hline\\[-3mm]
IRAS & \begin{sideways}H/L\end{sideways} & \begin{sideways}Comp\end{sideways} & $\xi$ & & type & Sp. & $L_{\rm bol}$ & $M_{\rm env} ^c$ & $R_{\rm env}$ & $\theta_{\rm p}$ & {\it i}$^d$ \\ 
    &    &   &    &   &       & Cl.  & \begin{sideways}({10$^3$~\lsun})\end{sideways}       & (\textrm{\msun})       & \begin{sideways}(10$^4$~AU)\end{sideways}        & (\adeg)  & (\adeg)     \\ \hline
05137+3919	& L  & A/1 & \textbf{0.12} & & IR-P & O8 & 255 & 2890 & 25 & 20 & 66 \\
			            &    & B/2 & \textbf{0.11} & & IR-S1 & B1 & 5.5 & 120  & 10 & 20 & 72 \\
05345+3157	& L & A/3 & \textbf{0.09} & & IR-S1 & B5 & 0.5   & 7   & 6    & 40 & 60 \\
		             	&    & B/1  &  0.11$^f$ & & MM-P  &    & 1.7    & 35   &     &  & \\
	            		&    & 2     &  & & MM-S &     & 0.8    & 20   &     &  & \\
05373+2349	& L & A/1 & \textbf{0.04} & & IR-P & B5 & 0.4     & 26    & 6 & 0 & 60 \\
08211$-$4158 & L & A   &  & & IR-S2  & B3 & 1.0  &  3  & 8 & 20 & 53 \\
       & & 1   & \multirow{-2}{0.25cm}{0.15$^g$} &   & MM-P & & 1.1  & 80 &  &  & \\   
\par
       &    & B  & \textbf{0.01} & & IR-S1  & B5 & 0.4    & 8 & 6 & 20 & 53 \\
08470$-$4243 & H & A/1 & \textbf{0.22} & & IR-P & B1 & 4.8   & 85      & 8 & 20 & 66 \\
08477$-$4359 & L & A     & \textbf{0.06} & & IR-S1 & B5 & 0.45       & 0.1        & 1   & 40 & 60 \\
                            &    & 1  & & & MM-P  &       & 0.7       & 85         &                &   \\
08589$-$4714 & H & A/1  & \textbf{0.11} & & IR-P & B5 & 0.3       &  20    & 8   & 40 & 0 \\
08563$-$4225 & L  & A/1 & \textbf{0.06} & & IR-P & B3 & 1.0     & 23      & 8   & 20 & 60 \\
09131$-$4723 & L  & A/1  & \textbf{0.15} & & IR-P & B5 &  0.45    & 26       & 8   & 20 & 66 \\
                            &     & B    & \textbf{0.02} & & IR-S1 & B5 &  0.3      & 4.3         & 8   & 40 & 60 \\
                            &     & 2    & & & MM-S &     & 0.47       & 25        &   &   & \\
                            &     & 3    & & & MM-S &     & 0.3       & 21.5        &   &   & \\
10019$-$5712 & H & A/1 & \textbf{0.13} & & IR-P & B3 & 0.65     & 11      & 6  & 40 & 37 \\
                            &     & B/2 & \textbf{0.09} & & IR-S1 & B5 & 0.3      & 7        & 6   & 40 & 37 \\
10095$-$5843$^b$ & L  & A    & \textbf{0.17}$^l$ & & IR-P & B1 & 4.8   & 85     & 8   & 20 & 66\\
10184$-$5748 & H & A/1 & \textbf{0.09} & & IR-P & O5 & 255 & 2890    & 30 & 20 & 66\\
                            &     & B  & \textbf{0.02} & & IR-S1 & B0  & 15  & 54      &  8  & 40 & 37 \\
                            &     & C  & \textbf{0.02} & & IR-S1 & B1 &  4.5     &  21.6       &  4  & 40 & 60 \\
                            &   & G/2 & \textbf{0.14} & & IR-S1 & B1 &  3.5     & 62      & 8  & 40 & 45  \\
10501$-$5556 & H & A/1 & \textbf{0.07} & & IR-P & B1 &  3.3     &  88     & 8 & 40 & 37 \\
10555$-$6242 & H & A/1 & \textbf{0.18} & & IR-P & B1 & 3.3      &   88    &  8 & 40 & 37 \\
11380$-$6311$^a$ & L  & A/1 & \textbf{0.10} & & IR-P & B5 & 0.3        & 20   & 8 & 40 & 37 \\
12063$-$6259 & H & A/1 & \textbf{0.04} & & IR-P & O5 & 373 & 2890  & 30 & 20 & 78 \\                                                      
12127$-$6244 & H & A/1 & \textbf{0.13} & & IR-P & O3 & 888 & 2050 & 30 & 20 & 72 \\
                            &     & 2  & & & MM-S &      & 105 &  1352   &             &   &  \\
14000$-$6104 & L & A   &  & & IR-S2  & B0 & 19   & 54      & 8    & 40 & 53 \\
       	&  & 1 & \multirow{-2}{0.25cm}{0.31} &  & MM-P &  & 21   & 1965 & & & \\
            			&    & B     & \textbf{0.13} & & IR-S1  & B1 & 3.6     & 88       & 10    & 40 & 45 \\
			            &    & C    & \textbf{0.01} & & IR-S1  & B3 & 1.0     & 2.5        & 8    & 0 & 53 \\
			            &    & D    & \textbf{0.01} & & IR-S1  & B1 & 8.6   & 21.5      & 4  & 40 & 78 \\
			            &    & H    & \textbf{0.31}$^h$ & & IR-S1  & B1 & 4.9      & 132     & 10    & 0 & 0 \\
			            &    & I      & \textbf{0.34}$^h$ & & IR-S1 & B1 & 5.0       & 132    & 10    & 0 & 45 \\
14057$-$6032$^a$ & H & A/1 & \textbf{0.02} & & IR-P & B5 & 0.25        &   6.5      & 4    & 40 & 25 \\
15068$-$5733$^b$ & H & A & \textbf{0.21} & & IR-P & O5 & 176 & 2145 & 30 & 40 & 37 \\
15454$-$5335$^b$ & H & A & \textbf{0.27} & & IR-P & O5 & 225  &  2890   & 30  & 20 & 37 \\
                                 &     & B   & \textbf{0.02} & & IR-S1 & O8 & 50  & 720 & 25  & 20 &  53 \\
15519$-$5430$^a$ & L & A   & & & IR-S2  & B3 & 1.1    &  4    &  8 & 40 & 53\\
	   	&  & 1  & \multirow{-2}{0.25cm}{0.56} &   & MM-P &  & 9.8  & 485 & &  &  \\
		                    	&    & G   & \textbf{0.01} & & IR-S1  & B5 &  0.5     & 3     & 8  & 20 & 60 \\
15557$-$5337$^a$ & L & A/1 & \textbf{0.05} & & IR-P & O8 & 65.4 & 721 & 25 & 20 & 73 \\
	                    		&    & B/2 & \textbf{0.06} & & IR-S1 & O8 & 57 & 721 & 25 & 20 & 66 \\
                    			&    & C    & \textbf{0.01} & & IR-S1 & B0 & 13   & 4.4      & 6  & 40 & 25 \\
                      			&    & D    & \textbf{0.05} & & IR-S1 & B1 & 4.1  & 1    & 2  & 40 & 53 \\
16148$-$5011$^a$ & L & A  & \textbf{0.03} & & IR-S1 & O8 & 71.5  & 20       & 10 & 0 & 72 \\
		                     	&    & C   & \textbf{0.16} & & IR-S1 & O5 & 255 & 2890 & 30 & 40 & 66 \\
	                      		&    & 1    & & & MM-P$^e$ &     & 240 & 2650 &      &  &  \\
	                    		&    & 2    & & & MM-S &     & 43.2   & 1160 &      &  &  \\
16232$-$4917$^a$ & L & A/1 & \textbf{0.06} & & IR-P & B1 & 4.25   & 88  & 10 & 40 & 53 \\
16501$-$4314$^a$ & L & A    &  & & IR-S2 & B1 & 6.1   & 26     & 10 & 0 & 78 \\
	  &  & 1  & \multirow{-2}{0.25cm}{0.26$^i$} &  & MM-P &  & 24.7 & 610 & & & \\
	                      		&    & 2    & & & MM-S &     & 24.7 & 610 &  &   &  \\
16535$-$4300$^a$ & L & A   &  & & IR-S2 & B3 & 2    & 0.4    & 1 & 40 & 84 \\
		      & & 1 & \multirow{-2}{0.25cm}{0.54} &  & MM-P &  & 13.4 & 750 & & & \\
	                     		&    & C   & \textbf{0.01} & & IR-S1 & B1 & 7.5  & 1.2  & 2 & 0 & 84 \\
\hline
    17082$-$4114$^a$ & L & A   & & & IR-S2 & B3 & 2.1   & 0.1 & 1 & 20 & 84 \\
	        &  & 1 & \multirow{-2}{0.25cm}{0.36} &  & MM-P &  & 2.5   & 282 & & & \\
	                     		 &    & 2   & & & MM-S &     & 1.4   & 166  &   & & \\
	                     		 &    & 3   & & & MM-S &     & 1.5   & 185   &  &  & \\
17425$-$3017 & L & A  & & & IR-S2 & B1 & 5.1  & 13 & 10 & 40 & 53 \\
		&  & 1 & \multirow{-2}{0.25cm}{0.53} &  & MM-P & & 23.1 &1250 &   &  & \\
18024$-$2119$^b$ & L & G/1 & 0.53 & & MM-P &   & 84.2 & 5850 &   & & \\
18144$-$1723$^b$ & L & A    &\textbf{0.20} & & IR-P & O5 & 176  & 2145      & 30 & 40 &  37 \\
18278$-$1009 & L & A    & \textbf{0.13} & & IR-P & B1 & 9.1  & 120 & 10 & 20 & 84 \\
18511+0146    & L & A1  &  & & IR-S2 & B1 & 6.4 & 1.2   & 2 & 0 & 72\\ 
       & & 1 &  \multirow{-2}{0.25cm}{0.17$^m$} &   & MM-P  & & 9.2  & 330 & & & \\
			             &    & A2  & \textbf{0.21} & & IR-S1  &  B1   & 4.5  & 120 & 10  & 20 & 60 \\
19092+0841$^a$ &  L  & A    &  & & IR-S2 & B3 & 1.1  & 8   & 6 & 0 & 66 \\
		 &  & 1 & \multirow{-2}{0.25cm}{0.43} &   & MM-P &  & 7.8 & 738  &   & & \\
20062+3550	& H & A   & \textbf{0.15} & & IR-P & B1 & 4.8   & 85 & 8 & 20 & 66 \\
20106+3545$^b$	& L & A   & \textbf{0.11}$^n$ & & IR-P & B1 & 3.6 & 88 & 10 & 40 & 45 \\
		                    	&    & 1    & & & MM-S &     & 1.8 & 45   &  &  &  \\
21307+5049	& L & A/1 & \textbf{0.16} & & IR-P & B1 & 3.6 & 88 & 10 & 40 & 45 \\
21519+5613	& H & A/1 & \textbf{0.18} & & IR-P & B1 & 5.4 & 85 & 8 & 20 & 75 \\
22172+5549	& L & A/1 & \textbf{0.16} & & IR-P & B1 & 3.6 & 88 & 10 & 40 & 45 \\
22305+5803	& H & A/1& \textbf{0.05} & & IR-P & B1 & 4.8 & 86 & 8 & 20 & 66 \\
22506+5944	& H & A   & & & IR-S2 & B1 & 7 & 25 & 10 & 20 & 78 \\
         &  &  1   & \multirow{-2}{0.25cm}{0.31} &   & MM-P & & 8.9 & 671 &   & & \\
23385+6053	& L & 1    & 0.36 & & MM-P &     & 17.5 & 222 & &  & \\
\hline
\end{tabular}
\smallskip
{$^a$ Near distance adopted.}\\
{$^b$ Far distance adopted.}\\
{$^c$ A correction factor of 0.4 has been applied to all envelope masses of IR sources to account for different mass opacity assumptions in Whitney et~al.'s models and in our greybody mass estimates.}\\
{$^d$ Between polar axis and plane of the sky.}\\
{$^e$ Source MM1 is assumed as primary instead of C because source C is not part of the A/MM1/MM2 complex (it's a different IRAS source), although we assume it connected to the same star forming region.}\\
{$^f$ Model rejected, see Sect.~\ref{mol011}.}\\
{$^g$ Model rejected, see Sect.~\ref{l08211}.}\\
{$^h$ Model accepted, see Sect.~\ref{l14000}.}\\
{$^i$ Model rejected, see Sect.~\ref{l16501}.}\\
{$^l$ This is not the minimum-$\xi$ model (see Sect.~\ref{l10095}), but it is chosen among the 10 best-$\xi$ models. The minimum $\xi$ model ($\xi=0.14$) provides a better fit to the mid-IR portion, but misses the 100~\um\ by slightly more than 50\%.}\\
{$^m$ Model rejected, see Sect.~\ref{m075}.}\\
{$^n$ Same as footnote $l$; see Sect.~\ref{m118}.}
\label{restab}
\end{table}