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Table 2.
Results of the fit on Spectrum 1 and Spectrum 2, adopting the 1-seed and 2-seed models together with a component that takes into account the contribution of a local warm absorber, respectively.
| Model: warm_1seed |
Model: warm_2seed |
||||
|---|---|---|---|---|---|
| Component | Parameter | Spectrum 1 | Spectrum 2 | Spectrum 1 | Spectrum 2 |
| PHABS | NH (1022) | 0.432 |
0.47 ± 0.02 | 0.46 ± 0.02 | 0.47 ± 0.02 |
| ZXIPCF | NH (1022) | 160 ± 120 | 13 |
140 |
13 |
| Log(ξ) | 5.2 |
4.35 |
5.1 ± 0.5 | 4.35 |
|
| CvrFract | > 0.87 | 1 | > 0.87 | > 0.97 | |
| Redshift | 0 | 0 | 0 | 0 | |
| GABS | LineE (keV) | – | 4.38 |
– | 4.38 |
| Sigma(keV) | – | 0.72 |
– | 0.72 ± 0.2 | |
| Strength | – | 0.07 |
– | 0.07 |
|
| EDGE | edgeE (keV) | – | 0.870 |
– | 0.869 |
| MaxTau | – | 0.11 |
– | 0.113 |
|
| BBODY | kT (keV) |  |
 |
2.0 ± 0.3 |  |
| Norm. (10−5) | < 45 | ≤50 | ≤128 | ≤20 | |
| BBODY UNABS. FLUX (erg cm2 s−1) | < 4 × 10−11 | < 4 × 10−11 | < 1 × 10−10 | < 2 × 10−11 | |
| DISKBB | Tin (keV) |  |
0.51 |
0.52 |
0.50 ± 0.05 |
| (Rin/D10)2 cos(θ) (km2 kpc−2) | 47 |
78 |
< 28 | 82 |
|
| DISKBB UNABS. FLUX (erg cm2 s−1) | (2.0 ± 0.2) ×10−10 | (1.1 ± 0.1) ×10−10 | < 6 × 10−11 | (1.1 ± 0.1) ×10−10 | |
| NTHCOMP | Γ |  |
 |
2.4 ± 0.5 | 1.8 ± 0.4 |
| kTe (keV) | 7 ± 1 | 6 ± 1 | 12 |
6 ± 1 | |
| kTbb (keV) |  |
 |
2.0 ± 0.3 | 0.72 |
|
| inp_type (0/1) | 0 | 0 | 0 | 0 | |
| Redshift | 0 | 0 | 0 | 0 | |
| Norm. (10−3) |  |
 |
< 2.1 | 11.2 |
|
| NTHCOMP UNABS. FLUX (erg cm2 s−1) | (4.0 ± 0.4) ×10−10 | (4.0 ± 0.4) ×10−10 | < 3 × 10−10 | (4.0 ± 0.4) ×10−10 | |
| NTHCOMP | Γ | – | – | 2.4 ± 0.5 | 1.8 ± 0.4 |
| kTe (keV) | – | – | 12 |
6 ± 1 | |
| kTbb (keV) | – | – | 0.52 |
0.50 ± 0.05 | |
| inp_type (0/1) | – | – | 1 | 1 | |
| Redshift | – | – | 0 | 0 | |
| Norm. (10−3) | – | – |  |
< 8 | |
| NTHCOMP UNABS. FLUX (erg cm2 s−1) | – | – | (4.0 ± 0.4) ×10−10 | < 9 × 10−11 | |
| TOTAL UNABS. FLUX (×10−10 erg cm2 s−1) | 6.0 ± 0.6 | 5.1 ± 0.5 | 6.0 ± 0.6 | 5.1 ± 0.5 | |
| χ2/d.o.f. | 698.30/618 | 707.51/605 | 691.30/617 | 707.48/604 | |
Notes. The errors for each spectral parameter are quoted at 90% of statistical confidence.
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