\begin{table}%t2
\caption{\label{results}Parameters for the cold (c) and warm (w) components.}\vspace*{-2mm}
%\centering
\par
\begin{tabular}{lrrrrrrr}
\hline \hline
\noalign{\smallskip}
& $T_{\rm{c}}$ & $M_{\rm{c}}$ & $L_{\rm{c}}$ & $L_{\rm{w}}$ & $L_{\rm{sm}}$ & $\frac{L}{L_{\rm{sm}}}$ &  $M_{850}$ \\
& [K] & [$M_{\odot}$] & [$L_{\odot}$] & [$L_{\odot}$] & [$L_{\odot}$] & & [$M_{\odot}$] \\
\hline 
\par
18223-12 & 31 & 189 & 13~849  & 3898 & 155 & 115 & 452 \\
18223-3  & 18 & 212  & 566    & 36   & 54 & 11  & 413 \\
18223-s2 & 16 & 102  & 157    & --   & 21 & 8   & 169 \\
18223-s1 & 18 & 142  & 372    & --   & 36 & 10  & 249 \\
\hline
\end{tabular}
\tablefoot{$T_{\rm{c}}$, $M_{\rm{c}}$, $L_{\rm{c}}$ and $L_{\rm{w}}$ are fit results. $L_{\rm{sm}}$ is the submm luminosity (longward of 400~$\mu$m, and $M_{850}$ is the mass in the derived from only the 850~$\mu$m flux (see main text).}
\vspace*{-3mm}
\end{table}