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Table 4
AGN luminosities (in cgs units) and CF values.
| Sources | L X a |
b
|
λ Lλ(6 μm)c |
d
|
CFe |
| [× 1044] | [× 1046] | [× 1046] | [× 1046] | ||
|
|
|||||
| IRAS F00235+1024† | <1.6 | <0.6 | 6.1 ± 1.2 |
|
>30 |
| IRAS 07380-2342† | <2.0 | <0.8 | 3.0 ± 0.3 |
|
>11 |
| IRAS 09104+4109 |
|
|
6.8 ± 0.3 |
|
|
| IRAS F12509+3122 | 1.8 ± 0.2 | 0.73 ± 0.09 | 3.9 ± 0.3 |
|
|
| IRAS 12514+1027 |
|
|
0.88 ± 0.06 |
|
|
| IRAS 14026+4341† | 3.0 ± 1.8 |
|
1.27 ± 0.07 |
|
|
| IRAS F15307+3252 |
|
|
8.1 ± 0.7 |
|
0.7 ± 0.3 |
| IRAS 18216+6418 | 37 ± 4 | 43 ± 5 | 2.11 ± 0.10 |
|
|
(a)
Absorption-corrected X-ray luminosity, from Ruiz et al. (2007). A factor of 60 (Panessa et al. 2006) has been applied to transform the observed X-ray luminosity to intrinsic X-ray luminosity to the sources marked with †.
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