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Table 5:

Parameters of the fitted models of SEDs of 47 ADF-S galaxies with the highest quality photometric data.
ID Modified black body Dale & Helou Li & Draine
(ADF-S) Dust temp. [K] Stellar temp. [K] $\alpha $ U${\rm min}$ U${\rm max}$ ${\rm PAH}$ (%) Name
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

Notes. The table contains 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 Dale & Helou (2001) model, three parameters, and the name of the best-fit Li & Draine (2001) model.


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