Table 3.
Results of fits to the XMM-Newton spectra between 0.5 and 10 keV.
| PexJGAL parameter | Unit | 0093630101 | 0306230101 | 0553300301 | 0553300401 |
|---|---|---|---|---|---|
| NH | [1022 cm−2] |
 |
 |
 |
8.4 ± 0.4 |
| Cov-frac |
 |
 |
 |
 |
|
| Γ | <1.2 | <1.2 |
 |
 |
|
| χ2/d.o.f. | 168.0/118 | 432.5/309 | 409.5/298 | 426.7/317 | |
| PexiJGAL parameter | |||||
| NH, high | [1022 cm−2] |
 |
 |
 |
9.1 ± 0.5 |
| Cov-frac |
 |
 |
 |
 |
|
| Γ |
 |
 |
 |
 |
|
| NH, low | [1022 cm−2] |
 |
 |
 |
 |
| ξ | [erg cm s−1] | <2.1 | <0.4 | <0.2 | <1.9 |
| χ2/d.o.f. | 128.3/116 | 385.1/307 | 370.7/296 | 389.2/315 | |
| FAGN, 0.5−10 | [10−11 erg s−1 cm−2] | 1.6 ± 0.7 | 0.91 ± 0.06 | 1.14 ± 0.08 | 1.26 ± 0.08 |
| LAGN, 0.5−10 | [1041 erg s−1] | 7 ± 3 | 3.8 ± 0.2 | 4.6 ± 0.3 | 5.2 ± 0.3 |
| Fjgal, 0.5−10 | [10−13 erg s−1 cm−2] | 3.30 ± 0.10 | 3.40 ± 0.08 | 3.50 ± 0.16 | 3.40 ± 0.23 |
| Ljgal, 0.5−10 | [1040 erg s−1] | 1.36 ± 0.04 | 1.40 ± 0.04 | 1.44 ± 0.06 | 1.40 ± 0.09 |
| Refl | 0.03 ± 0.02 | 0.06 ± 0.01 | 0.05 ± 0.01 | 0.050 ± 0.007 | |
| FAGN, 2−10 | [10−11 erg s−1 cm−2] | 1.03 ± 0.20 | 0.70 ± 0.03 | 0.84 ± 0.04 | 0.90 ± 0.02 |
| LAGN, 2−10 | [1041 erg s−1] | 4.2 ± 0.6 | 2.9 ± 0.1 | 3.4 ± 0.2 | 3.74 ± 0.08 |
| Fjgal, 2−10 | [10−13 erg s−1 cm−2] | 1.1 ± 0.05 | 1.10 ± 0.02 | 1.1 ± 0.05 | 1.10 ± 0.08 |
| Ljgal, 2−10 | [1039 erg s−1] | 4.5 ± 0.2 | 4.5 ± 0.1 | 4.5 ± 0.2 | 4.5 ± 0.3 |
| FAGN, 0.5−2 | [10−12 erg s−1 cm−2] | 6.4 ± 4.3 | 2.1 ± 0.4 | 3.0 ± 0.5 | 3.6 ± 0.5 |
| LAGN, 0.5−2 | [1041 erg s−1] | 2.6 ± 1.8 | 0.9 ± 0.2 | 1.2 ± 0.2 | 1.5 ± 0.2 |
| Fjgal, 0.5−2 | [10−13 erg s−1 cm−2] | 2.2 ± 0.1 | 2.3 ± 0.1 | 2.4 ± 0.1 | 2.3 ± 0.2 |
| Ljgal, 0.5−2 | [1039 erg s−1] | 9.1 ± 0.4 | 9.5 ± 0.4 | 9.9 ± 0.4 | 9.5 ± 0.4 |
Notes. The models are: PexJGAL: tbabs*(zpcfabs*pow+pexmon+mekal+pow). The last two mekal+pow components in the model represent the extended emission from the jet and galaxy and have parameters fixed to the model found for the jet and galaxy region from Chandra data (see Table 2 and text for details). PexiJGAL: tbabs*(zpcfabs*absori*pow+pexmon+mekal+pow). FAGN, 0.5−10 is the sum between the primary radiation and the reflected component. 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 (defined as L/n R2 where L is the luminosity, n the number density, and R the distance to the ionising source). The luminosities are derived from the fluxes at a distance from NGC1052 of 19.1 Mpc (luminosity distance from NED). Refl is the reflection fraction, derived as the ratio between the fluxes of the reflected radiation to the total AGN radiation between 2 and 10 keV.
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