\begin{table}%t1
\caption{\label{tabfit}Results from fitting a single reddened blackbody to the~$K$- and~$L$-band spectra.
In addition to the blackbody temperature and the~$K$-band extinction obtained from the fitting procedure, we list the~$L$-band 
magnitudes ($\pm$0.2~mag uncertainty) we derived from our images.}
%\centering
\par
\begin{tabular}{rccc}
\hline\hline
Source & Blackbody  &~$A_K$  &~$L$-band \\
 & temperature &   & magnitude \\
\hline
IRS 1W& 900 & 3.30 & 5.8 \\
IRS 3  & 800 & 4.20 & 5.3 \\
IRS 7  & 2100& 3.55  &5.0 \\
IRS 9  & 1900& 3.10  &7.4 \\
IRS 21 & 1200& 3.95 &6.8 \\
IRS 29 & 1600& 3.70  &7.4 \\
IRS 16C& 22~600 & 3.45 &8.6 \\
IRS 16CC& 20~200& 4.00 &9.0 \\
IRS 16NE& 22~400& 3.25 &7.7 \\
IRS 16SW& 22~500 & 3.25  &8.4 \\
IRS 13& 1300 & 3.00 & 6.7\\
IRS 13N& 1000& 3.90 & 9.76\\
\hline
\end{tabular}
 \end{table}