\begin{table}%t4
%\centering
\par
\caption {\label{Magexcess}Millimeter excess.}
\begin{tabular}{lccccc}
\hline\hline
\noalign{\smallskip}
Freq. & TD  & FF  & Syn & Excess & Total\\
(GHz) & \multicolumn{5}{c}{Jy}\\
\noalign{\smallskip}     
\hline
\noalign{\smallskip}     
\multicolumn{6}{c}{LMC: $T_{\rm d}$ = 25.0 K; $\beta$ = 1.33}\\
245 & 1519 &  99 & 12  &   0 & 1630 \\
150 &  328 & 104 & 13  &  55 &  500 \\ 
93  &   64 & 109 & 18  & 175 &  366 \\
61  &   17 & 113 & 24  &  51 &  205 \\
33  &    2 & 121 & 36  &   0 &  159 \\ 
\noalign{\smallskip}     
\hline
\noalign{\smallskip}     
\multicolumn{6}{c}{SMC: $T_{\rm d}$ = 29.5 K; $\beta$ = 0.91}\\
245 &  311 & 9.0 & 0.3 &   0 &  320 \\
150 &   81 & 9.5 & 0.5 &  69 &  160 \\ 
93  &   19 & 10.0& 0.9 &  58 &   88 \\
61  &  6.1 & 10.4& 1.4 &  23 &   40 \\
33  &  0.8 & 11.1& 1.7 &   7 &   20 \\ 
\noalign{\smallskip}
\hline
\end{tabular}
\par
\tablefoot {TD = Thermal dust emission extrapolated from the spectral fit
published by Aguirre et~al. (\cite{Aguirre03}); FF~=~free-free thermal emission;
Syn~=~synchrotron nonthermal emission; Excess~=~emission in excess
over the sum of the preceding contributions, required to make up the
observed total emission listed in the last column (the 150~GHz flux
being an interpolation). The values for~$T_{\rm d}$ and~$\beta$ were taken
from Aguirre et~al. (\cite{Aguirre03}).}
\end{table}