Table 2.
Best-fit parameters of the X-ray continuum components in our radio-loud AGN sample, derived from our modelling of the XMM-Newton observations.
| Object | pow Norm. | powΓ | mbb Norm. | mbbT | refls | Obs. ID | Obs. t. |
|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| 1H 0323+342 | 2.63 ± 0.02 | 1.94 ± 0.01 | 4.6 ± 0.1 | 0.17 ± 0.01 | 0.66 ± 0.06 | 0764670101 | 81 |
| 3C 59 | 6.56 ± 0.09 | 1.71 ± 0.01 | 5.3 ± 0.4 | 0.14 ± 0.01 | 0.36 ± 0.05 | 0205390201 | 82 |
| 3C 120 | 4.38 ± 0.03 | 1.91 ± 0.01 | 0.63 ± 0.02 | 0.23 ± 0.01 | 0.50 ± 0.04 | 0693782401 | 29 |
| 3C 273 | 113.3 ± 0.2 | 1.64 ± 0.01 | 37.2 ± 0.8 | 0.16 ± 0.01 | 0.10 ± 0.01 | 0126700801 | 74 |
| 3C 382 | 7.10 ± 0.04 | 1.76 ± 0.01 | 4.3 ± 0.2 | 0.14 ± 0.01 | 0.50 ± 0.05 | 0790600101 | 31 |
| 3C 390.3 | 5.90 ± 0.04 | 1.68 ± 0.01 | 0.27 ± 0.01 | 0.29 ± 0.01 | 0.35 ± 0.03 | 0203720301 | 53 |
| 4C +31.63 | 38 ± 1 | 1.90 ± 0.03 | 30 ± 4 | 0.18 ± 0.01 | 0.83 ± 0.19 | 0550871001 | 25 |
| 4C +34.47 | 28 ± 2 | 1.81 ± 0.04 | 4.5 ± 0.8 | 0.24 ± 0.02 | 0.49 ± 0.25 | 0102040101 | 8 |
| 4C +74.26 | 20.0 ± 0.2 | 1.82 ± 0.01 | 1.5 ± 0.2 | 0.25 ± 0.02 | 0.43 ± 0.04 | 0200910201 | 34 |
| ESO 075-G041 | 0.31 ± 0.01 | 1.74 ± 0.02 | 0.02 ± 0.01 | 0.29 ± 0.01 | 0.04 ± 0.06 | 0152670101 | 57 |
| III Zw 2 | 3.15 ± 0.08 | 1.67 ± 0.02 | 0.25 ± 0.04 | 0.25 ± 0.02 | 0.37 ± 0.13 | 0127110201 | 16 |
| Mrk 6 | 0.22 ± 0.01 | 1.47 ± 0.02 | 1.7 ± 0.9 | 0.10 ± 0.01 | 0.42 ± 0.05 | 0144230101 | 59 |
| Mrk 896 | 0.37 ± 0.01 | 2.34 ± 0.01 | 0.6 ± 0.3 | 0.09 ± 0.01 | 1.48 ± 0.10 | 0112600501 | 11 |
| PKS 0405-12 | 172 ± 2 | 1.90 ± 0.01 | 56 ± 3 | 0.21 ± 0.01 | 0.42 ± 0.06 | 0202210301 | 82 |
| PKS 0921-213 | 1.11 ± 0.03 | 1.73 ± 0.02 | 0.08 ± 0.01 | 0.23 ± 0.02 | 0.43 ± 0.13 | 0065940501 | 18 |
| PKS 2135-14 | 16.2 ± 0.2 | 1.75 ± 0.01 | 5.7 ± 2.0 | 0.15 ± 0.01 | 0.58 ± 0.10 | 0092850201 | 60 |
Notes. (1) Name of the AGN. (2) Normalisation of the X-ray power-law component in 1052 photons s−1 keV−1 at 1 keV. (3) Photon index of the X-ray power-law component. (4) Normalisation of the modified blackbody component in 1034 cm1/2, which is defined as the emitting area times square root of the electron density. (5) Temperature of the modified blackbody component in keV. (6) Scale parameter of the reflection component. (7) ID of the modelled XMM-Newton observation. (8) Duration of the XMM-Newton observation in ks. The X-ray flux and luminosity corresponding to the above continuum parameters are provided in Table 1 for each AGN.
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