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Table 3.
Percentages of AGN galaxies in pair systems with high luminosity and extremely powerful nuclear activity, taking into account the properties of the galaxy pair companion.
| Restrictions | L[OIII] > 106.4 L⊙ | L[OIII] > 107.0 L⊙ |
|---|---|---|
| Q1: (Mr)Comp < −20.5 | 58.4 ± 1.1 | 34.8 ± 2.2 |
| Q4: (Mr)Comp > −18.7 | 42.7 ± 0.9 | 20.4 ± 1.9 |
| Q1: (log(M*))Comp < 9.5 | 47.5 ± 1.0 | 25.3 ± 1.6 |
| Q4: (log(M*))Comp > 10.5 | 55.8 ± 1.2 | 33.5 ± 1.7 |
| Q1: (12 + log(O/H))Comp < 8.67 | 51.0 ± 1.2 | 28.4 ± 2.6 |
| Q4: (12 + log(O/H))Comp > 9.0 | 62.2 ± 1.3 | 38.7 ± 2.5 |
| Q1: ((Mu − Mr))Comp < 1.65 | 55.9 ± 0.8 | 32.7 ± 2.7 |
| Q4: ((Mu − Mr))Comp > 2.65 | 49.5 ± 0.9 | 27.9 ± 2.5 |
| Q1: (log(SFR/M*))Comp < -11.54 | 50.7 ± 1.4 | 27.8 ± 2.4 |
| Q4: (log(SFR/M*))Comp > -9.87 | 58.6 ± 1.2 | 35.2 ± 2.4 |
| Q1: (Dn(4000))Comp < 1.4 | 54.5 ± 1.0 | 34.5 ± 1.8 |
| Q4: (Dn(4000))Comp > 1.96 | 51.0 ± 0.9 | 28.1 ± 2.1 |
Note: Q1 and Q4 correspond to the first and the fourth quartile of the distributions of the pair companion properties.
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