Table 4
List of parameters for the simultaneous fit of observations Suz 2 to Suz 6 and the individual fit of the observation Suz 1.
| detconst(1) ∗ (cutoffpl(%)+xillver(%)) ∗ ((1-constant(%))+constant(%) ∗ zxipcfTB(2+%)) ∗ zxipcfTB(1) ∗ zxipcfTB(2) ∗ tbnew_simple(1) | ||||||||
|
|
||||||||
| Suz 1 | Suz 2 | Suz 3 | Suz 4 | Suz 5 | Suz 6 | |||
|
|
||||||||
| PL | norm (× 10-2) | 1.01 ± 0.04 |
|
|
|
|
|
|
| Γ | 1.658 ± 0.017 |
|
|
|
|
|
||
| Ion. Refl. | norm (× 10-5) |
|
0.24 ± 0.05 |
|
|
|
|
|
| log ξ (erg cm s-1) |
|
|
|
|
|
|
||
| WA2 | NH (1022cm-2) |
|
|
6.2 ± 0.5 |
|
10.8 ± 0.7 |
|
|
| log ξ (erg cm s-1) | 2.04 ± 0.04 |
|
|
|
1.21 ± 0.04 |
|
||
| f cvr |
|
|
0.905 ± 0.006 |
|
0.929 ± 0.007 | 0.930 ± 0.009 | ||
|
|
||||||||
| Detconst | XIS 0 | 1 † | 1 † | ′′ | ′′ | ′′ | ′′ | |
| XIS 1 |
|
1.096 ± 0.007 | ′′ | ′′ | ′′ | ′′ | ||
| XIS 3 |
|
1.036 ± 0.006 | ′′ | ′′ | ′′ | ′′ | ||
| HXD | 1.16† | 1.16 † | ′′ | ′′ | ′′ | ′′ | ||
| Ion. Refl. | Z Fe | 2.81 ∗ | 2.81 ± 0.17 | ′′ | ′′ | ′′ | ′′ | |
| WA1 | NH (1022cm-2) |
|
|
′′ | ′′ | ′′ | ′′ | |
| log ξ (erg cm s-1) |
|
−0.9 ± 0.6 | ′′ | ′′ | ′′ | ′′ | ||
| f cvr | 1.00 † | 1.00 † | ′′ | ′′ | ′′ | ′′ | ||
| WA3 | NH (1022cm-2) |
|
|
′′ | ′′ | ′′ | ′′ | |
| log ξ (erg cm s-1) |
|
|
′′ | ′′ | ′′ | ′′ | ||
| f cvr | 1.00 † | 1.00 † | ′′ | ′′ | ′′ | ′′ | ||
|
|
||||||||
|
7.6 ± 0.03 | 7.4 ± 0.05 | 7.3 ± 0.04 | 5.6 ± 0.05 | 6.7 ± 0.04 | 5.6 ± 0.04 | ||
|
2.60 ± 0.03 | 1.80 ± 0.05 | 2.09 ± 0.04 | 9.82 ± 0.05 | 2.15 ± 0.04 | 1.80 ± 0.04 | ||
Notes. We use the same model for both fits. The simultaneous fit consists of time-dependent parameters that are equal for a group comprising XIS and HXD data of one observation, and time-independent parameters that are equal for all data, denoted with quotation marks. Frozen parameters are denoted by the symbol †, ∗ denotes parameters adopted from the simultaneous fit. The redshift is frozen to the systemic value of z = 0.003859 (de Vaucouleurs et al. 1991). All spectra are additionally absorbed by a cold column of Galactic absorption of 1.99 × 1020 cm-2 (Kalberla et al. 2005). Normalizations are given in units of ph keV-1 cm-2 s-1 at 1 keV.
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