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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

Molecular outflows
OF 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%

Ionised outflows
OF 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%

X-ray outflows
OF vs. Lbol 1.12 ± 0.16 0.75 27 < 10-5
Ėkin vs. Lbol 2.0± 0.4 0.69 27 < 10-5

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%

Ultra fast outflows
OF 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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