Table 3.
Best-fit parameters of the ionised AGN wind and the neutral ISM gas in the host galaxy of the radio-loud AGN in our sample, derived from our modelling of the XMM-Newton observations.
| Object | Wind NH | Wind logξ | Wind vout | Neutral NH | C-stat/d.o.f. |
|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) |
| 1H 0323+342 | 9 ± 2, 7.2 ± 0.7 | 2.17 ± 0.02, 0.15 ± 0.12 | −830 ± 170, −880 ± 120 | < 0.01 | 2296/1488 |
| 3C 59 | 40 ± 2, 81 ± 8 | 1.20 ± 0.05, 2.42 ± 0.03 | −3530 ± 130, −1000 ± 120 | < 2 | 2036/1477 |
| 3C 120 | 14 ± 3 | 2.65 ± 0.04 | −2160 ± 360 | < 0.02 | 1949/1496 |
| 3C 273 | 0.7 ± 0.2 | 1.90 ± 0.08 | −3670 ± 170 | < 0.01 | 2588/1532 |
| 3C 382 | 7 ± 2 | 2.44 ± 0.06 | −1350 ± 370 | < 0.02 | 1805/1467 |
| 3C 390.3 | 3.7 ± 0.6, 11 ± 5 | 1.63 ± 0.11, 2.77 ± 0.06 | −1550 ± 160, +50 ± 100 | < 0.2 | 1847/1481 |
| 4C +31.63 | 11 ± 3 | −0.00 ± 0.20 | −960 ± 200 | < 0.3 | 1783/1423 |
| 4C +34.47 | 31 ± 11 | 2.12 ± 0.05 | −1500 ± 210 | < 0.3 | 1546/1398 |
| 4C +74.26 | 36 ± 3, 68 ± 8 | 1.69 ± 0.04, 2.46 ± 0.04 | −1490 ± 90, −3000 ± 500 | < 0.09 | 1986/1511 |
| ESO 075−G041 | 7 ± 1 | −0.03 ± 0.11 | −210 ± 180 | < 0.05 | 1832/1415 |
| III Zw 2 | 7 ± 4 | 2.07 ± 0.13 | −1780 ± 670 | < 0.2 | 1763/1468 |
| Mrk 6 | 116 ± 8 | 1.38 ± 0.06 | −4000 ± 500 | 27 ± 4 | 2287/1449 |
| Mrk 896 | 73 ± 6 | 2.23 ± 0.02 | −130 ± 150 | < 0.2 | 1679/1429 |
| PKS 0405−12 | 6 ± 2 | 1.71 ± 0.17 | −130 ± 200 | < 0.05 | 1715/1465 |
| PKS 0921−213 | 8 ± 3 | 1.92 ± 0.12 | −3540 ± 360 | < 0.2 | 1700/1458 |
| PKS 2135−14 | 5 ± 3 | 2.14 ± 0.08 | −1240 ± 530 | < 0.1 | 1831/1414 |
Notes. (1) Name of the AGN. (2) Column density NH of the ionised wind components (xabs) in 1020 cm−2. (3) Logarithm of the ionisation parameter ξ of the ionised wind components (xabs) in erg cm s−1. (4) Velocity of the outflowing ionised wind components (xabs) in km s−1. (5) Column density NH of neutral ISM gas component (hot) in the host galaxy of the AGN in 1020 cm−2. (6) Best-fit C-stat over degrees of freedom for the modelled XMM-Newton observation. As the positive and negative uncertainties on the wind parameters from our fits were comparable, we give their average in the table.
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