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Table A.2

Results of the spectral fits of the XMM-Newton observations of our sample.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
Source Model kT log ξ1 f 1 log ξ2 f 2 Lines χ2/d.o.f.
[eV] [ erg cm s-1] [10 22 cm-2] [ erg cm s-1] [10 22 cm-2] [10 22 cm-2]

B2 2201+31A A 969.1/927
IC 4329A – I E 2281.6/2079
IC 4329A – II G X 3810.1/3136
NGC 3227 – I F > 0.99 1781.5/1716
NGC 3227 – II F 3603.3/3032
NGC 4151 – I C X 3321.5/2808
NGC 4151 – II C X 3120.4/2785
NGC 4151 – III C X 2839.0/2683
NGC 4151 – IV C X 3304.3/2988
NGC 4151 – V C X 3281.8/2967
NGC 4151 – VI C X 3257.2/3016
NGC 4151 – VII C X 3306.5/2924
NGC 4151 – VIII C X 3420.0/3130
NGC 6814 B 1592.4/1525
NGC 7469 – I C 1954.6/1870
NGC 7469 – II C 2323.4/2088
NGC 7469 – III C 1897.1/1768
NGC 7469 – IV F 1876.3/1759
PG 0050+124 – I B ≥ 0.91 X 1510.0/1394
PG 0050+124 – II C ≥ 0.88 X 1927.1/1910
PG 0157+001 A 364.6/351
PG 0838+770 A 349.6/305
PG 0953+414 A 861.9/827
PG 1004+130 B 127.4/117
PG 1116+215 – I A X 743.0/665
PG 1116+215 – II C 2032.7/1826
PG 1116+215 – III A X 713.5/668
PG 1116+215 – IV C 2216.4/2060
PG 1116+215 – V C 2214.2/2125
PG 1116+215 – VI C 2128.5/1919
PG 1126041 – I D ≥ 0.86 X 383.9/381
PG 1126041 – II D X 268.0/284
PG 1126041 – III D ≥ 0.72 X 168.2/167
PG 1126041 – IV D X 1064.0/953
PG 1229+204 A X 1120.6/1005
PG 1244+026 A 624.0/610
PG 1309+355 A 521.2/495
PG 1411+442 C 162.7/140
PG 1426+015 A 734.8/692
PG 1435067 A 858.5/851
PG 1440+356 – I A 1218.2/1148
PG 1440+356 – II A X 1187.6/1081
PG 1440+356 – III A X 1259.1/1117
PG 1440+356 – IV A X 883.7/874
PG 1448+273 A 941.9/897
PG 1613+658 – I A 302.3/303
PG 1613+658 – II A 431.4/461
PG 1626+554 A 591.1/586
PG 2214+139 C 847.1/766

Notes. (1) Model used for the fit; (2) temperature of the bremsstrahlung component; (3 and 6) ionisation parameters; (4 and 7) column densities and (5 and 8) covering factors of the warm absorbers; (9) column density of the additional neutral absorber; (10) presence of additional emission lines (for details see Sect. 3 and Appendix B); and (11) chi-squared and degrees of freedom of the fit.

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