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Table 1
Correlations of wind parameters with AGN bolometric luminosity and host galaxies SFR.
Correlation | Slope | Spearman Rank (SR) | d.o.f. | Null hypothesis probability |
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Molecular outflows | ||||
ṀOF vs. Lbol | 0.76 ± 0.06 | 0.86 | 15 | < 10-5 |
Ėkin vs. Lbol | 1.29 ± 0.08 | 0.87 | 15 | < 10-5 |
vmax vs. Lbol | 3.4 ± 0.5 | 0.80 | 15 | < 10-5 |
Lbol vs. SFR | 0.9 ± 0.3 | 0.45 | 15 | 3.6% |
Ėkin vs. SFR | 1.2 ± 0.4 | 0.33 | 15 | 4.3% |
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Ionised outflows | ||||
ṀOF vs. Lbol | 1.29 ± 0.38 | 0.72 | 49 | < 10-5 |
Ėkin vs. Lbol | 1.48 ± 0.37 | 0.75 | 49 | < 10-5 |
vmax vs. Lbol | 6.1 ± 4.4 | 0.34 | 49 | 0.7% |
Lbol vs. SFR | 2.2 ± 1.6 | 0.34 | 34 | 2% |
Ėkin vs. SFR | 4.9 ± 4.4 | 0.19 | 34 | 13% |
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X-ray outflows | ||||
ṀOF vs. Lbol | 1.12 ± 0.16 | 0.75 | 27 | < 10-5 |
Ėkin vs. Lbol | 2.0± 0.4 | 0.69 | 27 | < 10-5 |
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Molecular + Ionised outflows | ||||
vmax vs. Lbol | 4.6 ± 1.8 | 0.57 | 67 | < 10-5 |
Lbol vs. SFR | 1.5 ± 0.6 | 0.44 | 52 | 4 × 10-4 |
Ėkin vs. SFR | 2.1 ± 1.4 | 0.28 | 52 | 2% |
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Ultra fast outflows | ||||
ṀOF vs. Lbol | 1.13 ± 0.11 | 0.90 | 18 | < 10-5 |
Ėkin vs. Lbol | 1.44 ± 0.11 | 0.87 | 18 | < 10-5 |
vmax vs. Lbol | 3.9 ± 1.4 | 0.46 | 18 | 0.4% |
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