\begin{table}%t5
\caption{\label{MODELtable}Parameters of the fitted models of SEDs of 47  \mbox{ADF-S} galaxies with the highest quality photometric data.}
%\centering
 \begin{tabular}{ccccccccccc} 
\hline\hline
ID  &  \multicolumn{2}{c}{Modified black body} & \multicolumn{1}{c}{Dale \& Helou} & \multicolumn{4}{c}{Li \& Draine} \\
%\hline
(ADF-S)  &  Dust temp.\ [K] &  Stellar temp.\ [K]  & $\alpha$ & U${\rm min}$ & U${\rm max}$ & ${\rm PAH}$ (\%) & Name\\
 \hline
1 & 26.9 $\pm$ 0.2 & 2800 $\pm$ 40 & 2.4375 & 4.00 & 4.00 & 2.37 & LMC2 \\  
2 & 37.8$\pm$  0.3 & 3060 $\pm$ 30 & 2.1250 & 0.10 & 100 & 4.58 & MW3.1 \\  
3 & 22.9 $\pm$ 0.2 & 2950 $\pm$ 30 & 2.1250 & 0.50 & 0.50 & 2.37 & LMC2 \\  
4 & 36.3 $\pm$ 0.1 & 7000 $\pm$ 120& 1.0000 & 1.20 & 100 & 2.37 & LMC2    \\   
5 & 33.6 $\pm$ 0.3 & 3260 $\pm$ 50 & 1.3125 & 0.10 & 100 & 2.37 & LMC2 \\  
6 & 32.6 $\pm$ 0.3 & 2110 $\pm$ 70 & 1.3125 & 5.00 & 5.00 & 2.37 & LMC2 \\  
7 & 47.8 $\pm$ 0.4 & 5110 $\pm$ 50 & 0.0625 & 8.00 & 1e4 & 2.37 & LMC2 \\  
8 & 36.8 $\pm$ 0.4 & 2020 $\pm$ 70 & 0.0625 & 0.10 & 1e4 & 1.12 & MW3.1 \\  
9 & -- & 3890 $\pm$ 50 & 1.1875 & 0.80 & 1e4 & 3.90 & MW3.1 \\  
10 & 27.8 $\pm$ 0.2 & 3230 $\pm$ 30 & 4.0000 & 2.00 & 2.00 & 2.37 & LMC2 \\  
11 & 28.9 $\pm$ 0.3 & 3030 $\pm$ 40 & 4.0000 & 2.00 & 2.00 & 2.37 & LMC2 \\  
12 & 36.0 $\pm$ 0.6 & 2070 $\pm$ 120 & 4.0000 & 5.00 & 1e4 & 2.37 & LMC2 \\  
13 & 33.2 $\pm$ 0.4 & -- & 4.0000 & 0.10 & 100 & 0.75 & LMC2 \\  
14 & 32.4 $\pm$ 0.4 & -- & 0.0625 & 8.00 & 100 & 2.37 & LMC2 \\  
15 & 32.1 $\pm$ 0.2 & 1980 $\pm$ 10 & 0.0625 & 0.10 & 100 & 0.75 & LMC2 \\  
16 & 28.2 $\pm$ 0.7 & -- & 0.0625 & 0.10 & 100 & 4.58 & MW3.1 \\  
17 & 33.2 $\pm$ 0.6 & 5890 $\pm$ 60 & 0.0625 & 0.10 & 1e4 & 0.75 & LMC2 \\  
18 & 28.8 $\pm$ 0.2 & 2260 $\pm$ 70 & 0.0625 & 4.00 & 4.00 & 2.37 & LMC2 \\  
19 & 33.8 $\pm$ 0.1 & 2050 $\pm$ 10 & 0.0625 & 15.0 & 15.0 & 0.75 & LMC2 \\  
20 & 33.0 $\pm$ 0.5 & 1980 $\pm$ 70 & 0.0625 & 0.10 & 1e4 & 0.75 & LMC2 \\  
21 & 29.4 $\pm$ 0.2 & 2210 $\pm$ 10 & 0.0625 & 4.00 & 4.00 & 2.37 & LMC2 \\  
22 & 38.0 $\pm$ 0.1 & 2060 $\pm$ 40 & 4.0000 & 0.10 & 100 & 0.75 & LMC2 \\  
23 & 28.1 $\pm$ 0.3 & 2340 $\pm$ 70 & 4.0000 & 0.10 & 100 & 2.37 & LMC2 \\  
24 & 33.4 $\pm$ 0.6 & 2140 $\pm$ 10 & 4.0000 & 0.10 & 1e6 & 0.75 & LMC2 \\  
26 & 43.5 $\pm$ 0.1 & -- & 0.0625 & 4.00 & 1e4 & 0.75 & LMC2 \\  
27 & 35.7 $\pm$ 0.3 & -- & 0.0625 & 0.80 & 100 & 2.37 & LMC2 \\  
29 & 27.5 $\pm$ 0.8 & 2950 $\pm$ 20 & 0.0625 & 0.10 & 100 & 0.75 & LMC2 \\  
30 & 32.7 $\pm$ 0.7 & 1900 $\pm$ 10 & 0.0625 & 0.10 & 1e6 & 4.58 & MW3.1 \\  
31 & 32.8 $\pm$ 0.3 & 1970 $\pm$ 120 & 0.0625 & 8.00 & 8.00 & 2.37 & LMC2 \\  
39 & 47.4 $\pm$ 0.4 & 3500 $\pm$ 60 & 0.0625 & 0.20 & 1e6 & 0.47 & MW3.1 \\  
41 & 32.5 $\pm$ 0.1 & 1950 $\pm$ 10 & 0.0625 & 12.0 & 12.0 & 0.75 & LMC2 \\  
42 & -- & 2210 $\pm$ 30 & 0.0625 & 0.10 & 1e5 & 0.75 & LMC2 \\  
43 & 33.3 $\pm$ 0.7 & 1970 $\pm$ 10 & 0.0625 & 0.10 & 1e6 & 0.75 & LMC2 \\  
45 & 28.5 $\pm$ 0.1 & 4160 $\pm$ 80 & 3.8750 & 0.10 & 100 & 0.75 & LMC2 \\  
46 & -- & 1650 $\pm$ 20 & 3.8750 & 0.10 & 1e6 & 4.58 & MW3.1 \\  
48 & 24.3 $\pm$ 0.1 & 2010 $\pm$ 10 & 3.8750 & 1.20 & 1.20 & 2.37 & LMC2 \\  
49 & 26.6 $\pm$ 0.1 & -- & 3.8750 & 0.10 & 100 & 0.75 & LMC2 \\  
50 & 33.6 $\pm$ 0.1 & 3380 $\pm$ 60 & 3.8750 & 0.10 & 1e6 & 1.49 & LMC2 \\  
51 & 29.7 $\pm$ 0.2 & 3120 $\pm$ 30 & 2.2500 & 0.10 & 100 & 0.75 & LMC2 \\  
52 & -- & 2000 $\pm$ 30 & 2.2500 & 2.00 & 1e6 & 2.37 & LMC2 \\  
56 & 34.8 $\pm$ 0.1 & -- & 2.2500 & 0.10 & 1e6 & 4.58 & MW3.1 \\  
64 & 23.1 $\pm$ 0.1 & 1940 $\pm$ 10 & 2.2500 & 0.70 & 0.70 & 2.37 & LMC2 \\  
65 & 28.0 $\pm$ 0.1 & 4600 $\pm$ 110 & 4.0000 & 1.50 & 1.50 & 2.37 & LMC2 \\  
69 & 26.4 $\pm$ 0.1 & 1770 $\pm$ 80 & 4.0000 & 2.00 & 2.00 & 2.37 & LMC2 \\  
73 & -- & -- & 4.0000 & 1.50 & 1e6 & 2.37 & LMC2 \\  
82 & 27.8 $\pm$  0.1 & -- & 4.0000 & 2.00 & 2.00 & 3.19 & MW3.1 \\  
103 & 20.2 $\pm$ 0.1 & 2910 $\pm$ 50 & 4.0000 & 0.10 & 0.10 & 2.37 & LMC2 \\
\hline
\end{tabular}
\tablefoot{The table contains  \mbox{ADF-S} identification numbers (first column), indicative temperatures of dust and stellar 
component resulting from the best-fit modified black-body models, 
the parameter $\alpha$ of the \citet{dale2001} model, three 
parameters, and the name of the best-fit \citet{li2001} model.}
\end{table}