Table A.1.
Results of fits to the XMM-Newton spectra between 0.5 and 10 keV.
OBSID |
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Model | Parameter | Unit | 0093630101 | 0306230101 | 0553300301 | 0553300401 |
P-JGAL | ||||||
χ2/d.o.f. | 231.0/119 | 571.1/310 | 499.0/299 | 563.0/318 | ||
PG-JGAL | ||||||
NH, high | [1022 cm−2] |
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Cov-frac |
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Γ |
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EW | [eV] |
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χ2/d.o.f. | 211.8/118 | 430.2/309 | 406.2/298 | 430.7/317 | ||
PGI-JGAL | ||||||
NH, high | [1022 cm−2] |
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Cov-frac |
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Γ |
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NH, low | [1022 cm−2] |
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ξ | [erg cm s−1] | <2.5 | <0.6 | <0.2 | <2.5 | |
EW | [eV] |
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χ2/d.o.f. | 129.7/116 | 385.7/307 | 370.4/296 | 394.5/315 |
Notes. The models are P-JGAL:tbabs*(zpcfabs*pow+mekal+pow). PG-JGAL: tbabs*(zpcfabs*pow+GAUSS+mekal+pow). PGI-JGAL: tbabs*(zpcfabs*absori*pow+GAUSS+mekal+pow). The last two mekal+POW components in all three models represent the extended emission from the jet and galaxy (see Table 2 and text for details). All fluxes and luminosities are unabsorbed. NH, high and NH, low are the column densities of the zpcfabs and absori models, respectively, and ξ is ionisation parameter of absori. EW is the equivalent width of the narrow iron line.
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