Table 2
Reliability and completeness of AGN selection techniques.
| X-ray | MIR | SED | OIII | Radio | Any | |
|---|---|---|---|---|---|---|
| X-ray | – | 25.7% (106/412) | 38.6% (159/412) | 21.1% (87/412) | 74.5% (307/412) | 88.6% (365/412) |
| MIR | 38.1% (106/278) | – | 67.6% (188/278) | 22.7% (63/278) | 64.0% (178/278) | 88.5% (246/278) |
| SED | 16.1% (159/988) | 19.0% (188/988) | – | 5.4% (53/988) | 93.0% (919/988) | 97.3% (961/988) |
| [O III] | 32.5% (87/268) | 23.5% (63/268) | 19.8% (53/268) | – | 40.7% (109/268) | 66.0% (177/268) |
| Radio | 8.1% (307/3791) | 4.7% (178/3791) | 24.2% (919/3791) | 2.9% (109/3791) | – | 30.5% (1155/3791) |
| All | 10.1% (412/4087) | 6.8% (278/4087) | 24.2% (988/4087) | 6.6% (268/4087) | 92.8% (3791/4087) | – |
Notes. For reliability, the table should be read from left to right. For example, the percentage of X-ray AGN that are MIR AGN is 25.7% and the percentage of radio AGN that are any other kind of AGN is 30.5%. For completeness, the table should be read top to bottom. For example, X-ray AGN probe 16.1% of SED AGN and MIR AGN probe 23.5% of [O III] AGN.
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