\begin{table}%[h]%t3=>%t2
\caption{Sources classified as YSO.}\label{table:allYSOs}
%\centerline
 {
\begin{tabular}{r l l l l l l l}
    \hline\hline
   (1) & (2) & (3) & (4) & (5) & (6) & (7) & (8)\\
   ID & Assoc. & $N$ & Minimal $\chi^2/N$ & $M_\star$ & $\dot{M}_{\rm env}/ M_\star$ & $M_{\rm disk}/M_\star$ & Stage \\
  &   & &	&  & ($M_\odot$)	& (yr$^{-1}$) &  \\
    \hline\noalign{\smallskip}
    S2  & yes   & 7 & 1.38  & 1--5  &  $10^{-5}$--$2\times10^{-4}$  &  $3\times10^{-5}$--$7\times10^{-2}$   & I\\
    S5  & yes   & 8 & 6.18  & 1--2 & $1$--$3\times10^{-4}$  & $1$--$5\times10^{-2}$ & I \\
    S6  & yes   & 7 & 6.77  & 0.7--8  & $1$--$6\times10^{-5}$  & $3\times10^{-6}$--$5\times10^{-2}$ & I \\
    S7  & yes   & 4 & 0.0875 & 0.2--6 & $5\times10^{-7}$--$2\times10^{-4}$ & $8\times10^{-5}$--$6\times10^{-3}$ & I\\
    S8  & yes   & 8 & 1.99  & 1.5--4 & 0--$5\times10^{-8}$     &  $ 5\times10^{-6}$--$4\times10^{-2}$ & II\\
    S9  & yes   & 8 & 0.126 & 0.3--6 & $2\times10^{-7}$--$3\times10^{-4}$ & $5\times10^{-6}$--$7\times10^{-2}$ & I or (II) \\
    S11 & yes   & 5 & 0.61 & 0.1--5 & 0--$2\times10^{-4}$ & $5\times10^{-8}$--$2\times10^{-1}$ & I or II or (III) \\
    S12 & yes   & 4 & 0.58 & 1.5--6 & $1$--$4\times10^{-4}$ & $2\times10^{-4}$--$3\times10^{-2}$ & I  \\
    S13 & yes   & 5 & 11.9 & $\sim$2  & $\sim10^{-6}$  & $\sim$$10^{-2}$  & $\sim$I \\
    S14 & yes   & 7 & 0.030 & 0.5--4  & 0--$4\times10^{-5}$  & $3\times10^{-8}$--$5\times10^{-2}$ & (I) or II or (III)\\
    S15 & yes   & 4 & 0.515 & 3--4 & $2\times10^{-4}$ & $3\times10^{-4}$--$5\times10^{-3}$ & I \\
    S16 & yes   & 5 & 1.99 & 2--5 & 0--$3\times10^{-4}$ & $3\times10^{-6}$--$4\times10^{-2}$ & I or II \\
    S20 & no    & 5 & 18.6 & $\sim$4--6 & $\sim$0 & $\sim$$10^{-5}$--$10^{-3}$ & $\sim$II \\
    \hline
\end{tabular}}
\smallskip
Object parameters derived from fitting the data points to YSO SEDs (see Sect.~\ref{sec:SEDanalysis}). Column (1) lists the ID of the object, corresponding to the entry in Table~\ref{table:sourcelist}. Column (2) indicates whether the source is thought to be spatially associated with the IRDC filament. The number of available data points, $N$, is listed in Col.~(3). The $\chi^2$ per data point, $\chi^2/N$, is given in Col.~(4). Columns~(5)--(7) list the fitted stellar mass, envelope accretion rate and disk mass, respectively. Note that the latter two are given in terms of $M_\star$, not $M_\odot$. Finally, Col.~(8) lists the Stage in which the sources fall according to the values in Cols.~(6) and~(7) and the Stage definition in Table~\ref{table:stages}. If multiple possibilities are given for the Stage of a source, the less likely one(s) is (are) presented in brackets. A ``$\sim$'' prefix in Cols.~(5)--(7) or~(8) indicates a high uncertainty in the derived parameter, resulting either from a high value of the minimal $\chi^2/N$ and/or a large spread in fitted parameter values. 
\end{table}