\begin{table}%t3
%\centering
\par
\caption {\label{DIRBEpeakdata}COBE-DIRBE peak flux densities in the Magellanic Clouds.}
\begin{tabular}{cccccccccccccccc}
\hline\hline
\noalign{\smallskip}
          &\multicolumn{12}{c}{LMC}&\multicolumn{3}{c}{SMC}\\  
Pos.\tablefootmark{a} &1&2&3&4 &5 &6 &7 &8 &9 &10 &11 &12&1 & 2& 3 \\ 
Name\tablefootmark{b}&30~Dor&N~159&Ridge&N~206&-- &N~77-94&Bar&N~11&N~44&N~48&N~63&N~57&Wing&NW&SW\\
Pixel& 24, 32& 22, 32& 19, 33& 18, 30& 17, 20& 22, 19& 23, 26& 31, 18& 27, 27& 33, 27& 33, 30& 29, 30& -- & -- &--\\
\hline
$\lambda$& \multicolumn{15}{c}{Flux densities} \\
($\mu$m) & \multicolumn{15}{c}{kJy}\\
\hline
  1.25& 0.174& 0.228&0.121&0.113&0.031&0.090& 0.315&0.053& 0.085&0.047&0.064&0.059&0.102&0.177&0.315 \\
  2.2 & 0.154& 0.196&0.098&0.088&0.022&0.076& 0.251&0.048& 0.066&0.040&0.059&0.046&0.077&0.133&0.238 \\
  3.5 & 0.116& 0.126&0.056&0.049&0.013&0.049& 0.143&0.032& 0.043&0.025&0.035&0.030&0.042&0.071&0.128 \\
  4.9 & 0.084& 0.077&0.031&0.028&0.008&0.030& 0.081&0.019& 0.027&0.015&0.018&0.019&0.023&0.040&0.072 \\
 12   & 0.78 & 0.41 &0.106&0.068&0.026&0.128& 0.21 &0.095& 0.140&0.063&0.040&0.081&0.028&0.060&0.091 \\
 25   & 3.16 & 1.08 &0.114&0.095&0.020&0.25 & 0.35 &0.21 & 0.29 &0.099&0.068&0.186&0.066&0.138&0.180 \\
 60   &24.9  &12.9  &1.56 &1.74 &0.307&3.05 & 6.04 &2.63 & 4.36 &1.43 &0.99 &2.92 &1.21 &2.74 &3.94  \\
100   &35.6  &22.1  &5.26 &4.23 &1.24 &7.21 &11.5  &6.39 & 9.04 &3.98 &2.69 &6.33 &3.06 &6.06 &8.51  \\
140   &39.0  &26.6  &7.92 &5.48 &2.33 &9.03 &13.1  &7.35 &11.1  &5.07 &3.20 &7.17 &3.62 &6.98 &9.47  \\
240   &19.2  &13.8  &5.32 &3.19 &2.04 &6.06 & 6.79 &4.68 & 6.71 &3.36 &2.30 &4.42 &2.68 &4.1  &5.18  \\
\hline\\[-3mm]
&\multicolumn{12}{c}{Luminosity (10$^{7}$~$L_{\odot}$)}\\
  1--240&15.6 &11.4  &3.32 &2.74 &0.90 &3.37 & 7.29 &2.44 & 4.23 &1.77 &1.57 &2.92 &3.21&5.68 &8.99  \\
 12--240&12.9 & 8.4  &1.79 &1.35 &0.43 &2.14 & 3.78 &1.74 & 3.07 &1.14 &0.82 &2.05 &1.52&2.86 &4.07  \\
 12--100& 9.0 & 5.3  &9.02 &0.75 &0.18 &1.23 & 2.36 &1.02 & 1.83 &0.62 &0.46 &1.22 &8.71&1.69 &2.44  \\
\hline
\end{tabular}
\par
\tablefoot {\tablefoottext{a}{Position numbers correspond to WMAP position numbers in
Table~\ref{WMAPpeakdata}, but area covered is not identical}. 
\tablefoottext{b} {The
objects refer to the most prominent features included in the
aperture. These are the giant HII~region complex 30~Doradus (1); the
very bright HII~region complex N159 south of 30~Dor (2); the
prominent ridge of radiating dust and molecular gas south of 30~Dor
and N159 (3); the bright but isolated HII~region complex N206 south of
the LMC Bar (4); a very extended HII~region complex, containing~N77,
N79, N83, N87, N90, N93, N94 at the southwestern corner of the~LMC
(6); the LMC Bar itself~(7); the second brightest HII~region complex
N11 at the northwestern corner of the LMC (8); the third brightest 
HII~region complex N44~north of the Bar (9); the HII~region complexes~N48,
N63, and N57, delineating Shapley Constellation~III (10, 11, 12)}.} 
\end{table}