Table 3.
KS test p-values results for the null hypothesis that the samples under consideration have the same distribution for different parameters of the AGN or host galaxy.
| Sample 1 | Sample 2 | p-values | |||||
|---|---|---|---|---|---|---|---|
| Cobs | E(B − V) | log10[F(Hαn)/F(Hβn)] | LAGN | LGAL | LAGN/LGAL | ||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| 1.0 | 1.2 | 0.006 | 0.117 | 0.383 | 0.074 | 0.113 | 0.029 |
| 1.2 | 1.5 | 0.506 | 0.534 | 0.637 | 0.815 | 0.245 | 0.462 |
| 1.5 | 1.8–9 | 0.000 | 0.000 | 0.422 | 0.855 | 0.000 | 0.005 |
| 1.8–9 | 2.0 | 0.086 | 0.607 | 0.055 | 0.184 | 0.072 | 0.880 |
| 1.0 | 1.5 | 0.009 | 0.014 | 0.331 | 0.012 | 0.339 | 0.020 |
| 1.2 | 1.8–9 | 0.000 | 0.000 | 0.458 | 0.939 | 0.056 | 0.009 |
| 1.5 | 2.0 | 0.000 | 0.000 | 0.086 | 0.918 | 0.000 | 0.005 |
| 1.0–5 | 1.8–2.0 | 0.000 | 0.000 | 0.856 | 0.062 | 0.001 | 0.000 |
| 1.0–5Low E(B − V) | 1.8–2.0Low E(B − V) | ... | ... | ... | 0.009 | 0.000 | 0.000 |
Notes. We consider a result as significant if it is greater than 3σ (P(H0) < 0.003). In this case, we mark the result in bold. If the result lies between 3σ and 2σ (0.003 < P(H0) < 0.05) we display it in italic. Columns 1, 2: samples evaluated by the KS test; Col. 3: observed contrast of the AGN over the total flux at rest-frame 5100 Å; Col 4: extinction of the AGN emission; Col 5: Balmer decrement of the narrow emission lines; Col 6: host-galaxy luminosity at rest-frame 5100 Å weighted by redshift distributions (see Sect. 4.3); Col 7: absorption-corrected luminosity of the AGN at rest-frame 5100 Å weighted by redshift distributions (see Sect. 4.3); Col 8: ratio between host galaxy and AGN optical luminosity at rest-frame 5100 Å.
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