Table E.1.
Frequency of MIR-, X-ray-, and SED-selected AGN in mergers (M) and non-mergers (NM) in different redshift bins.
| MIR AGN | |||
|---|---|---|---|
| z bin | M | NM (ctrl.) | Excess |
| 0.5–1.25 | 1.4 ± 0.4% | 1.1 ± 0.1% | 1.3 ± 0.4 |
| (14/981) | (111/9887) | ||
| 1.25–2.0 | 4.0 ± 0.6% | 2.7 ± 0.2% | 1.4 ± 0.2 |
| (43/1086) | (296/10783) | ||
| X-ray AGN | |||
| z bin | M | NM (ctrl.) | Excess |
| 0.5–1.25 | 1.9 ± 0.4% | 0.7 ± 0.1% | 2.6 ± 0.6 |
| (19/981) | (74/9887) | ||
| 1.25–2.0 | 2.2 ± 0.5% | 0.87 ± 0.08% | 2.6 ± 0.6 |
| (24/1086) | (92/10783) | ||
| SED AGN | |||
| z bin | M | NM (ctrl.) | Excess |
| 0.5–1.25 | 14 ± 1% | 12.5 ± 0.3% | 1.10 ± 0.09 |
| (135/981) | (1234/9887) | ||
| 1.25–2.0 | 22 ± 1% | 17.7 ± 0.4% | 1.25 ± 0.08 |
| (241/1086) | (1909/10783) | ||
Notes. Fractions and relative errors are calculated using bootstrapping with resampling (1000 samples for each population). In brackets, we provide the number of AGN for each type over the total number of mergers and non-merger controls in each z-bin.
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