Table 7.
Merger fractions in the MIR, X-ray, and SED AGNs and their respective non-AGN control sample, in different redshift bins.
| fmerger in | fmerger in | fmerger in | fmerger in | fmerger in | fmerger in | |
|---|---|---|---|---|---|---|
| z | MIR AGNs | non-MIR AGNs | X-ray AGNs | non-X-ray AGNs | SED AGNs | non-SED AGNs |
| (control) | (control) | (control) | ||||
| Main | ||||||
| [0.1, 0.31) | 55.1 ± 6.0% | 27.0 ± 1.7% | 33.2 ± 3.4% | 24.6 ± 1.0% | 22.1 ± 1.1% | 10.7 ± 0.3% |
| (38/69) | (186/690) | (64/193) | (475/1930) | (324/1467) | (1571/14 670) | |
| [0.31, 0.52) | 45.1 ± 5.9% | 28.0 ± 1.7% | 30.1 ± 2.3% | 23.0 ± 0.7% | 14.1 ± 0.8% | 7.0 ± 0.2% |
| (32/71) | (199/710) | (120/399) | (916/3990) | (245/1741) | (1223/17 410) | |
| [0.52, 0.76) | 43.7 ± 5.6% | 18.2 ± 1.4% | 27.6 ± 1.9% | 15.1 ± 0.5% | 11.8 ± 0.4% | 5.7 ± 0.1% |
| (35/80) | (146/800) | (152/550) | (831/5500) | (965/8151) | (4677/81 510) | |
| Worst-case | ||||||
| [0.1, 0.31) | 40.4 ± 5.1% | 20.5 ± 1.3% | 22.9 ± 2.5% | 16.8 ± 0.7% | 16.5 ± 0.8% | 8.1 ± 0.2% |
| (38/94) | (193/940) | (65/284) | (478/2840) | (325/1968) | (1596/19 680) | |
| [0.31, 0.52) | 28.7 ± 4.2% | 18.0 ± 1.1% | 17.4 ± 1.4% | 14.6 ± 0.4% | 10.0 ± 0.6% | 5.5 ± 0.2% |
| (33/115) | (207/1150) | (120/690) | (1008/6900) | (245/2450) | (1350/24 500) | |
| [0.52, 0.76) | 26.4 ± 3.7% | 12.9 ± 0.9% | 18.6 ± 1.4% | 11.0 ± 0.3% | 9.1 ± 0.3% | 4.6 ± 0.1% |
| (38/144) | (186/1440) | (153/825) | (909/8250) | (971/10 609) | (4925/106 090) | |
Notes. The top half of the table corresponds to galaxies classified using the main classification scheme. The bottom half corresponds to the worst-case scenario, where all unclassified galaxies are labelled as non-mergers. Errors are calculated through binomial statistics. In brackets are the number of mergers out of the total number of AGNs and non-AGN controls, per AGN type and z-bin.
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