Table 3
Infrared luminosities.
| ID | νLν(6 μm) | L IR | Ltorus/LIR | log (LX/LIR) | IRAC | Full-SED | Prob. | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | |
|
|
||||||||
| W-4 | 1.0 | 1.4 | 0.14 | –2.7 | AGN | Arp 220/Torus | 0.5 | |
| W-9 | 1.7 | 7.8 | 0.04 | –1.9 | SF | Arp 220/Torus | 3.9 | |
| W-11 | 5.4 | 4.7 | 0.21 | –2.8 | SF | M 82/Torus | 2.1 | |
| W-40 | 0.16 | 0.88 | 0.03 | –2.9 | SF | Arp 220/Torus | 0.4 | |
| W-45† | 0.69 | 1.4 | 0.09 | –3.6 | SF | Arp 220/Torus | 0.9 | |
| W-57 | 2.0 | 1.9 | 0.18 | –2.4 | AGN | Arp 220/Torus | 0.6 | |
| W-59† | 0.06* | 1.7 | 0.006 | –4.15 | SF | Arp 220 | 42. | |
| W-66 | 0.07 | 0.23 | 0.05 | –1.98 | SF | Arp 220/Torus | 3.9 | |
| W-67† | 0.76* | 4.2 | 0.03 | –4.24 | SF | Arp 220 | 47. | |
| W-84 | 1.9 | 5.3 | 0.07 | –2.86 | SF | Arp 220/Torus | 2.7 | |
| W-92 | 0.0* | 3.8 | 0.00 | –3.30 | SF | Arp 220 | 99. | |
| W-101 | 0.22* | 1.30 | 0.03 | –2.92 | SF | Arp 220 | 11.1 | |
| W-108† | 0.002* | 0.02 | 0.03 | –3.84 | SF | M 82 | 17.1 | |
| W-114 | 0.65* | 3.3 | 0.03 | –4.01 | SF | Arp 220/Torus | 5.2 | |
Notes. The columns are: (1) LABOCA ID as in Table 1; (2) Torus 6 μm νLν monochromatic luminosity in units of 1045 erg s-1; (3) 10–1000 μm Infrared Luminosity in units of 1046 erg s-1; (4) Ratio of torus to total 10–1000 μm luminosity; (5) Logarithm of the Ratio of X-ray luminosity to total IR (10–1000 μm) luminosity; (6) mid-IR IRAC template: power-law (AGN) vs. curved (star-forming); (7) Best-fit templates from Polletta et al. (2007); (8) Probability (× 10-2) that the torus component is not needed according to the F-test.
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