Table 5.
Polar dust and AGN detection efficiency of the SED decomposition.
| SED configuration | X-ray AGNs | IR-detected AGNs |
Non-IR-detected AGNs | |
|---|---|---|---|---|
| 75% Assef | 90% Assef | |||
| 1956 | 889/1956 (45%) | 689/1956 (35%) | 1067/1956 (55%) | |
| Polar dust (fracAGN > 0.2) | 851/889 (96%) | 671/689 (97%) | 906/1067 (85%) | |
| Polar dust (fracAGN > 0.3) | 795/889 (90%) | 631/689 (92%) | 789/1067 (74%) | |
| W/out polar dust (fracAGN > 0.2) | 740/889 (83%) | 591/689 (86%) | 757/1067 (71%) | |
| W/out polar dust (fracAGN > 0.3) | 603/889 (68%) | 484/689 (70%) | 586/1067 (55%) | |
Notes. The second column presents the number of X-ray AGNs detected by WISE. The third and fourth columns show the number of X-ray detected AGNs that are IR selected, based on the Assef et al. (2018) criteria, with confidence level 75% and 90%, respectively. The last column presents the number of X-ray AGNs that are not IR selected, but for which X-CIGALE finds a strong AGN component, i.e., high AGN fraction.
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