Table 4.
Derived dust parameters and luminosities for our (U)LIRG sample.
| Overall SED fit |
Within IRAM-30 m beam |
|||||||
|---|---|---|---|---|---|---|---|---|
| Source name | Tdust |  |
log(LFIR) | Tdust |  |
 |
log(LFIR) | log(LTIR) |
| (K) | (107 M⊙) | (L⊙) | (K) | (107 M⊙) | (107 M⊙) | (L⊙) | (L⊙) | |
| NGC 0034 | 34.87 ± 0.59 |
 |
 |
36.32 ± 1.08 |
 |
 |
 |
11.02 |
| Arp 256N | 25.65 ± 2.14 |
 |
 |
26.04 ± 0.51 |
 |
 |
 |
10.12 |
| Arp 256S | 31.50 ± 0.64 |
 |
 |
33.22 ± 0.87 |
 |
 |
 |
10.99 |
| IC 1623 | 30.60 ± 0.58 |
 |
 |
32.11 ± 0.85 |
 |
 |
 |
11.21 |
| MCG -03-04-014 | 30.14 ± 0.56 |
 |
 |
30.68 ± 0.74 |
 |
 |
 |
11.27 |
| IRAS F01364−1042 | 34.92 ± 0.82 |
 |
 |
35.89 ± 1.06 |
 |
 |
 |
11.37 |
| IC 0214 | 28.09 ± 0.85 |
 |
 |
29.84 ± 0.69 |
 |
 |
 |
10.96 |
| UGC 01845 | 29.54 ± 0.41 |
 |
 |
29.92 ± 0.72 |
 |
 |
 |
10.73 |
| NGC 0958 | 22.96 ± 0.78 |
 |
 |
23.86 ± 0.45 |
 |
 |
 |
10.50 |
| ESO 550−IG025 | 28.79 ± 0.35 |
 |
 |
28.19 ± 0.64 |
 |
 |
 |
10.96 |
| UGC 03094 | 26.39 ± 0.59 |
 |
 |
27.23 ± 0.60 |
 |
 |
 |
10.91 |
| NGC 1797 | 29.05 ± 0.56 |
 |
 |
30.79 ± 0.76 |
 |
 |
 |
10.62 |
| IRAS F05189−2524 | 37.28 ± 0.76 |
 |
 |
37.63 ± 1.19 |
 |
 |
 |
11.69 |
| IRAS F05187−1017 | 28.98 ± 0.61 |
 |
 |
29.46 ± 0.71 |
 |
 |
 |
10.91 |
| IRAS F06076−2139 | 30.95 ± 0.83 |
 |
 |
32.09 ± 0.85 |
 |
 |
 |
11.22 |
| NGC 2341 | 28.58 ± 0.52 |
 |
 |
30.20 ± 0.72 |
 |
 |
 |
10.59 |
| NGC 2342 | 26.77 ± 0.64 |
 |
 |
28.23 ± 0.64 |
 |
 |
 |
10.55 |
| IRAS 07251−0248 | 33.71 ± 0.81 |
 |
 |
33.28 ± 0.95 |
 |
 |
 |
11.96 |
| IRAS F09111−1007 W | 30.30 ± 0.55 |
 |
 |
29.77 ± 0.72 |
 |
 |
 |
11.52 |
| IRAS F09111−1007 E | 27.79 ± 0.78 |
 |
 |
26.55 ± 0.55 |
 |
 |
 |
11.01 |
| UGC 05101 | 29.49 ± 0.42 |
 |
 |
29.96 ± 0.74 |
 |
 |
 |
11.61 |
| 2MASX J11210825−0259399 | 22.94 ± 2.60 |
 |
 |
25.06 ± 0.49 |
 |
 |
 |
9.67 |
| CGCG 011−076 | 27.01 ± 0.52 |
 |
 |
28.23 ± 0.65 |
 |
 |
 |
10.88 |
| IRAS F12224−0624 | 33.46 ± 0.67 |
 |
 |
32.09 ± 0.85 |
 |
 |
 |
10.82 |
| CGCG 043−099 | 28.89 ± 0.54 |
 |
 |
30.16 ± 0.73 |
 |
 |
 |
11.12 |
| ESO 507−G070 | 33.06 ± 0.61 |
 |
 |
33.67 ± 0.93 |
 |
 |
 |
11.00 |
| NGC 5104 | 27.07 ± 0.43 |
 |
 |
27.75 ± 0.61 |
 |
 |
 |
10.72 |
| IC 4280 | 25.62 ± 0.47 |
 |
 |
26.82 ± 0.57 |
 |
 |
 |
10.53 |
| NGC 5258 | 26.14 ± 0.50 |
 |
 |
27.59 ± 0.59 |
 |
 |
 |
10.75 |
| UGC 08739 | 24.07 ± 0.56 |
 |
 |
24.95 ± 0.49 |
 |
 |
 |
10.57 |
| NGC 5331 | 29.33 ± 0.87 |
 |
 |
28.15 ± 0.62 |
 |
 |
 |
11.12 |
| CGCG 247−020 | 32.02 ± 0.72 |
 |
 |
32.52 ± 0.84 |
 |
 |
 |
10.91 |
| IRAS F14348−1447 | 34.02 ± 0.61 |
 |
 |
32.71 ± 0.90 |
 |
 |
 |
11.96 |
| CGCG 049−057 | 30.98 ± 0.52 |
 |
 |
31.59 ± 0.82 |
 |
 |
 |
10.79 |
| NGC 5936 | 26.55 ± 0.50 |
 |
 |
28.43 ± 0.64 |
 |
 |
 |
10.48 |
| IRAS F16164−0746 | 31.91 ± 0.62 |
 |
 |
32.05 ± 0.85 |
 |
 |
 |
11.01 |
| CGCG 052−037 | 28.57 ± 0.60 |
 |
 |
29.95 ± 0.71 |
 |
 |
 |
10.97 |
| IRAS F16399−0937 | 29.74 ± 1.13 |
 |
 |
29.69 ± 0.76 |
 |
 |
 |
11.06 |
| NGC 6285 | 26.13 ± 0.76 |
 |
 |
28.41 ± 0.62 |
 |
 |
 |
10.17 |
| NGC 6286 | 25.12 ± 0.31 |
 |
 |
26.17 ± 0.53 |
 |
 |
 |
10.84 |
| IRAS F17138−1017 | 31.49 ± 0.60 |
 |
 |
31.33 ± 0.81 |
 |
 |
 |
10.94 |
| UGC 11041 | 26.01 ± 0.47 |
 |
 |
27.56 ± 0.60 |
 |
 |
 |
10.57 |
| CGCG 141−034 | 30.20 ± 0.57 |
 |
 |
30.04 ± 0.73 |
 |
 |
 |
10.70 |
| IRAS 18090+0130 | 28.06 ± 0.92 |
 |
 |
27.49 ± 0.62 |
 |
 |
 |
11.06 |
| NGC 6701 | 27.13 ± 0.46 |
 |
 |
28.87 ± 0.67 |
 |
 |
 |
10.52 |
| NGC 6786 | 27.52 ± 0.47 |
 |
 |
28.52 ± 0.64 |
 |
 |
 |
10.74 |
| UGC 11415 | 29.03 ± 0.58 |
 |
 |
30.18 ± 0.73 |
 |
 |
 |
10.72 |
| ESO 593−IG008 | 28.57 ± 0.54 |
 |
 |
28.74 ± 0.67 |
 |
 |
 |
11.50 |
| NGC 6907 | 24.47 ± 0.51 |
 |
 |
26.75 ± 0.57 |
 |
 |
 |
10.25 |
| IRAS 21101+5810 | 32.71 ± 0.77 |
 |
 |
28.26 ± 0.73 |
 |
 |
 |
11.07 |
| ESO 602−G025 | 27.22 ± 0.51 |
 |
 |
28.75 ± 0.67 |
 |
 |
 |
10.92 |
| UGC 12150 | 28.18 ± 0.36 |
 |
 |
28.87 ± 0.67 |
 |
 |
 |
10.93 |
| IRAS F22491−1808 | 37.05 ± 0.83 |
 |
 |
36.99 ± 1.15 |
 |
 |
 |
11.75 |
| CGCG 453−062 | 28.28 ± 0.62 |
 |
 |
29.26 ± 0.70 |
 |
 |
 |
10.92 |
| 2MASX J23181352+0633267 | 25.38 ± 0.77 |
 |
 |
23.42 ± 0.40 |
 |
 |
 |
9.46 |
Notes. While LFIR is measured between 42.5 and 122.5 μm, LTIR is measured between 3 and 1100 μm and is obtained from Eq. (5). We have assumed an uncertainty in LTIR of 20%. We note that dust masses 
are derived evaluating the modified blackbody function using the dust temperature from the models, in contrast with 
, obtained assuming Tdust = 25 K, as suggested in Scoville et al. (2016). The latter are used as the preferred method in this study.
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