\begin{table}%t2
%%\centering
\par
\caption{\label{table_mir_continuum}Parameters from the Spitzer IRS spectra.}
%\centerline
 {\small \begin{tabular}{lrrrrrr}
\hline \hline
2MASS & $LW$2 / & $F$15  &  $F$24  &  $F$35  &[Ne~III]&[S~III]  \\
 & 6--10~$\mu$m & mJy  &  mJy  &  mJy  & 15.55   & 18.71    \\
\hline                                          
00285431$-$7726146  & 0.57 & 7.03 &   9.3 &  27.2 &    6.1 &  16.0 \\ %  264 
00445167$-$2653191                        &      &      &   4.8 &  11.7 &    --   &   --   \\ % 7672 
01051501$-$2612466                        & 0.49 & 2.88 &   4.6 &  11.6 &    5.8 &  12.0 \\ % 7729 
02542961$+$1509122                        & 0.52 & 2.15 &   3.0 &   8.1 &    1.6 &   4.2 \\ %11224 
03574895$-$1340458                        & 0.61 &14.48 &  25.2 &  85.0 &    3.6 &  19.1 \\ % 9160 
06033357$-$4509412                        &      &      &  89.3 & 468.5 &    --   &   --   \\ % 5223 
12482307$-$0344102                        &      &      &   4.7 &  12.0 &    --   &   2.4 \\ % 9959  
13165999$-$3336459                        &      &      &   5.3 &  14.2 &    --   &   2.6 \\ % 6153 
13371721$+$0904430                        &      &      &   6.2 &  22.8 &    --   &   2.1 \\ %10888  
15160785$-$1608098                        &      &      &   3.3 &   9.5 &    --   &   3.0 \\ % 9023 
15554606$+$1532218\parbox{0cm}{$^{\rm ~*}$} & 0.40 & 2.88 &   5.3 &  13.7 &    2.5 &   5.9 \\ %11233 
16132299$+$4203418                        &      &      &  13.6 &  51.4 &    --   &   6.1 \\ %13447 
19184395$-$3815471                        &      &      &   7.7 &  24.8 &    --   &   0.8 \\ % 5792 
21573517$+$0114331                        & 0.42 & 3.06 &   3.9 &   9.6 & $<$0.7 &   3.2 \\ %10416 
22023161$-$5657577                        & 0.58 & 4.34 &   7.6 &  18.7 & $<$2.0 &   8.1 \\ % 4261 
22565483$-$3649515                        & 0.58 & 1.60 &   2.2 &   6.0 & $<$1.0 &   5.2 \\ % 5973 
23055422$-$3539591                        &      &      &   3.0 &   7.7 &    --   &   --   \\ % 6039 
23075850$+$0537063                        &      &      &   3.2 &   9.5 &    --   &   --   \\ %10702 
23080919$+$0538305                        & 0.41 & 3.22 &   4.6 &  11.6 & $<$0.7 &   4.1 \\ %10707 
\hline
\end{tabular}}
\medskip
The second column gives the fraction of the 6--10~$\mu$m flux seen 
in the $LW2$ passband (5--8.5~$\mu$m).  F15 refers to the flux integrated over the ISOCAM  $LW3$ passband (12--18~$\mu$m). The uncertainty of the continua F15, F24, and F35 are about 10\%. Emission line fluxes are given in 10$^{\rm -15}$~erg/s/cm$^{2}$ with $\sim$10--20\% uncertainties; $^*$)~absolute photometry uncertain, see footnote in Sect.~\ref{sect_data_mir_spectroscopy}.
\end{table}