Table A.1
Results of the spectral fits of the XMM-Newton observations of our sample.
| Source | 2–10 keV continuum | Narrow Fe Kα line | Broad Fe Kα line | Molecular torus | ||||||||||||
|
|
|
|
|
|||||||||||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | ||||
| Model | Γ | log f 2 − 10 | log L 2 − 10 | E Kα | EW | log fKα | log LKα | p | EW | f obs |
|
Ref. | ||||
| [ erg cm-2 s-1] | [ erg s-1] | [keV] | [eV] | [ erg cm-2 s-1] | [ erg s-1] | [eV] | [ cm-2] | |||||||||
|
|
||||||||||||||||
| B2 2201+31A | A |
|
|
45.05 |
|
|
|
43.05 | 13% | – | 0.09 | 23.76 | 1 | |||
| IC 4329A – I | E |
|
|
44.00 |
|
|
|
41.76 | 4% | – | 0.24 | 24.45 | 2 | |||
| IC 4329A – II | G |
|
|
43.75 |
|
|
|
41.47 | > 99% |
|
// | // | // | |||
| NGC 3227 – I | F |
|
|
41.67 |
|
|
|
39.98 | ~ 0% | – | 0.86 | 24.63 | 2 | |||
| NGC 3227 – II | F |
|
|
42.06 |
|
|
|
40.02 | > 99% |
|
// | // | // | |||
| NGC 4151 – I | C |
|
|
42.26 |
|
|
|
40.61 | > 99% |
|
0.16 | 24.57 | 2 | |||
| NGC 4151 – II | C |
|
|
42.22 |
|
|
|
40.63 | > 99% |
|
// | // | // | |||
| NGC 4151 – III | C |
|
|
42.22 |
|
|
|
40.64 | 98% |
|
// | // | // | |||
| NGC 4151 – IV | C |
|
|
42.88 |
|
|
|
40.75 | 97% |
|
// | // | // | |||
| NGC 4151 – V | C |
|
|
42.87 |
|
|
|
40.78 | 96% |
|
// | // | // | |||
| NGC 4151 – VI | C |
|
|
42.95 |
|
|
|
40.79 | > 99% |
|
// | // | // | |||
| NGC 4151 – VII | C |
|
|
42.35 |
|
|
|
40.79 | > 99% |
|
// | // | // | |||
| NGC 4151 – VIII | C |
|
|
42.62 |
|
|
|
40.70 | 96% |
|
// | // | // | |||
| NGC 6814 | B |
|
|
42.29 | 6.4 f |
|
|
40.08 | 91% | – | 0.13 | 23.67 | 3 | |||
| NGC 7469 – I | C |
|
|
43.16 |
|
|
|
41.34 | ~ 0% | – | 0.20 | 24.64 | 2 | |||
| NGC 7469 – II | C |
|
|
43.39 |
|
|
|
41.22 | ~ 0% | – | // | // | // | |||
| NGC 7469 – III | C |
|
|
43.40 |
|
|
|
41.29 | ~ 0% | – | // | // | // | |||
| NGC 7469 – IV | F |
|
|
43.29 |
|
|
|
41.24 | 92% | – | // | // | // | |||
| PG 0050+124 – I | B |
|
|
43.88 |
|
|
|
41.45 | > 99% |
|
0.63 | 23.31 | 1 | |||
| PG 0050+124 – II | C |
|
|
43.63 |
|
|
|
41.05 | > 99% |
|
// | // | // | |||
| PG 0157+001 | A |
|
|
43.80 | 6.4 f |
|
|
42.16 | 56% | – | 0.53 | 23.86 | 1 | |||
| PG 0838+770 | A |
|
|
43.40 |
|
|
|
41.96 | ~ 0% | – | 0.48 | 23.71 | 1 | |||
| PG 0953+414 | A |
|
|
44.70 | 6.4 f |
|
≤ − 13.8 | ≤ 42.43 | ~ 0% | – | 0.10 | 23.98 | 1 | |||
| PG 1004+130 | B |
|
|
43.75 | 6.4 f |
|
≤ − 14.20 | ≤ 42.04 | 63% | – | 0.20 | 23.50 | 1 | |||
| PG 1116+215 – I | A |
|
|
44.45 | 6.4 f |
|
≤ − 13.6 | ≤ 42.34 | 85% | – | 0.23 | 23.60 | 1 | |||
| PG 1116+215 – II | C |
|
|
44.76 |
|
|
|
42.24 | ~ 0% | – | // | // | // | |||
| PG 1116+215 – III | A |
|
|
44.48 | 6.4 f |
|
≤ − 13.4 | ≤ 42.59 | 88% | – | // | // | // | |||
| PG 1116+215 – IV | C |
|
|
44.88 | 6.4 f |
|
≤ − 13.5 | ≤ 42.44 | ~ 0% | – | // | // | // | |||
| PG 1116+215 – V | C |
|
|
44.80 |
|
|
|
42.14 | ~ 0% | – | // | // | // | |||
| PG 1116+215 – VI | C |
|
|
44.65 |
|
|
|
42.24 | ~ 0% | – | // | // | // | |||
| PG 1126−041 – I | D |
|
|
43.20 | 6.4 f |
|
|
41.14 | 51% | – | 0.37 | 23.88 | 1 | |||
| PG 1126−041 – II | D |
|
|
43.56 |
|
|
≤ − 13.4 | ≤ 41.54 | 55% | – | // | // | // | |||
| PG 1126−041 – III | D |
|
|
43.59 | 6.4 f |
|
≤ − 13.5 | ≤ 41.44 | 21% | – | // | // | // | |||
| PG 1126−041 – IV | D |
|
|
43.35 |
|
|
|
41.74 | 98% |
|
// | // | // | |||
| PG 1229+204 | A |
|
|
43.48 |
|
|
|
41.49 | 35% | – | 0.31 | 23.97 | 1 | |||
| PG 1244+026 | A |
|
|
43.07 | 6.4 f |
|
≤ − 13.4 | ≤ 41.34 | 42% | – | 0.33 | 23.93 | 1 | |||
| PG 1309+355 | A |
|
|
43.80 |
|
|
|
42.07 | 44% | – | 0.16 | 23.92 | 1 | |||
| PG 1411+442 | C |
|
|
43.20 | 6.4 f |
|
≤ − 13.5 | ≤ 41.80 | > 99% |
|
0.48 | 23.46 | 1 | |||
| PG 1426+015 | A |
|
|
44.18 |
|
|
|
42.06 | ~ 0% | – | 0.33 | 23.89 | 1 | |||
| PG 1435−067 | A |
|
|
44.03 | 6.4 f |
|
|
41.94 | 65% | – | 0.32 | 23.17 | 1 | |||
| PG 1440+356 – I | A |
|
|
43.56 |
|
|
≤ − 13.7 | ≤ 41.46 | 86% | – | 0.36 | 23.53 | 1 | |||
| PG 1440+356 – II | A |
|
|
43.65 | 6.4 f |
|
≤ − 13.6 | ≤ 41.56 | 88% | – | // | // | // | |||
| PG 1440+356 – III | A |
|
|
43.54 |
|
|
≤ − 13.7 | ≤ 41.46 | 71% | – | // | // | // | |||
| PG 1440+356 – IV | A |
|
|
43.41 | 6.4 f |
|
≤ − 13.7 | ≤ 41.46 | 80% | – | // | // | // | |||
| PG 1448+273 | A |
|
|
43.30 |
|
|
|
41.30 | 61% | – | 0.15 | 23.99 | 1 | |||
| PG 1613+658 – I | A |
|
|
44.29 |
|
|
≤ − 13.1 | ≤ 42.61 | 5% | – | 0.45 | 23.69 | 1 | |||
| PG 1613+658 – II | A |
|
|
44.39 |
|
|
≤ − 12.9 | ≤ 42.81 | 5% | – | // | // | // | |||
| PG 1626+554 | A |
|
|
44.12 |
|
|
|
42.36 | 4% | – | 0.18 | 23.32 | 1 | |||
| PG 2214+139 | C |
|
|
43.71 |
|
|
|
41.63 | 6% | – | 0.13 | 23.77 | 1 | |||
Notes. (1) Model used for the fit (for details see Table A.2 and Sect. 3); (2) photon index of the power-law continuum; (3) flux and (4) luminosity of the 2–10 keV power-law continuum; (5) energy; (6) equivalent width; (7) flux; and (8) luminosity of the narrow component of the iron Kα line; (9) probability of the presence of a broad relativistic component of the iron Kα line and (10) its equivalent width. The table also lists the characteristics of the molecular torus obtained by fitting MIR spectra of AGN: (11) covering factor and (12) equatorial column density of the torus (calculated using Eq. (2), the values are ~6 times higher if calculated with Eq. (3)); (13) bibliographical reference for the value.
energy of the line fixed to 6.4 keV. The values of the torus parameters were taken from: (1) Mor et al. (2009); (2) Alonso-Herrero et al. (2011); (3) Ramos Almeida et al. (2011). Typical uncertainties on the torus parameters are about 30%.
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