Table 6
Estimates of AGN contribution to IR luminosity.
| No. | Galaxy | log (HX/IR) | CT | log Fagn |
| (1) | (2) | (3) | ||
|
|
||||
| 4 | F05189–2524 | −2.63 | −0.65 | |
| 7 | ESO 60-IG16 | −2.54 | −1.54 | |
| 8 | F08572+3915 | −4.44 | ∗ | −0.94 |
| 9 | 09022–3615 | −3.59 | −1.59 | |
| 12 | UGC 5101 | −3.92 | ° | −0.42 |
| 16 | NGC 3690 W | −4.07 | ° | −0.57 |
| 18 | UGC 8058 | −3.67 | ° | −0.17 |
| 19 | 13120–5453 | −4.25 | ∗ | −0.75 |
| 22 | UGC 8689 | −3.39 | −1.39 | |
| 23 | F14348–1447 S | −4.90 | ∗ | −1.50 |
| 24 | F14378–3651 | −4.28 | ∗ | −0.78 |
| 25 | VV 340 N | −3.86 | ° | −0.36 |
| 30 | NGC 6240 | −2.97 | ° | + 0.53 |
| 36 | 19542+1110 | −3.05 | −1.09 | |
| 42 | ESO 148-IG2 | −3.72 | −1.72 | |
| 44 | F23365+3604 | −4.58 | ∗ | −1.08 |
Notes. (1) Logarithmic luminosity ratio of the observed 2–10 keV and 8–1000 μm bands, reproduced from Table 3. (2) Compton thick AGN with Fe K detection are marked as °. Candidate Compton thick AGN (see text for detail) are marked as ∗ . (3) Logarithmic fraction of the X-ray estimate for AGN contribution to the 8–1000 μm luminosity.
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