Table 2
Continuum parameters of the time resolved spectral analysis.
| epa | LXb | Γ | Efold | AFec | WFe | EG | AGc | σG | cb | cHEXTE | cISGRI |  /d.o.f. |
||
| [keV] | [10-3] | [eV] | [keV] | [keV] | ||||||||||
|
|
||||||||||||||
| 1 |
|
|
|
|
|
|
|
|
|
|
– | 1.13/50 | ||
| 2 |
|
|
|
|
|
|
|
|
|
|
|
1.12/77 | ||
| 3 |
|
|
|
|
|
|
|
|
|
|
– | 1.32/48 | ||
| 4 |
|
|
|
|
|
|
|
|
|
|
– | 0.88/48 | ||
| 5 |
|
|
|
|
|
|
|
|
|
|
– | 0.79/48 | ||
| 6 |
|
|
|
|
|
|
|
|
|
|
|
1.09/75 | ||
| 7 |
|
|
|
|
|
|
|
|
|
|
|
1.18/75 | ||
| 8 |
|
|
|
|
|
|
|
|
|
|
– | 1.27/48 | ||
| 9 |
|
|
|
|
|
|
|
|
|
|
|
0.99/77 | ||
| 10 |
|
|
|
|
|
|
|
|
|
|
|
1.11/77 | ||
| 11 |
|
|
|
|
|
|
|
|
|
|
– | 1.17/48 | ||
| 12 |
|
|
|
|
|
|
|
|
|
|
– | 1.10/48 | ||
| 13 |
|
|
|
|
|
|
|
|
|
|
|
0.96/81 | ||
| 14 |
|
|
|
|
|
|
|
|
|
|
|
0.86/81 | ||
|
|
||||||||||||||
| epa | E0 | W0 | τ0 | E1 | W1 | τ1 | E2 | τ2 | E3 | τ3 | E4 | τ4 | ||
| [keV] | [keV] | [keV] | [keV] | [keV] | [keV] | [keV] | ||||||||
|
|
||||||||||||||
| 1 |
|
|
|
|
|
|
– | – | – | – | – | – | ||
| 2 |
|
|
|
|
|
|
|
|
|
|
– | – | ||
| 3 |
|
|
|
|
|
|
|
|
– | – | – | – | ||
| 4 |
|
|
|
|
|
|
|
|
– | – | – | – | ||
| 5 |
|
|
|
|
|
|
|
|
– | – | – | – | ||
| 6 |
|
|
|
|
|
|
|
|
|
|
|
|
||
| 7 |
|
|
|
|
|
|
|
|
|
|
|
|
||
| 8 |
|
|
|
|
|
|
|
|
– | – | – | – | ||
| 9 |
|
|
|
|
|
|
|
|
|
|
– | – | ||
| 10 |
|
|
|
|
|
|
|
|
|
|
– | – | ||
| 11 |
|
|
|
|
|
|
|
|
– | – | – | – | ||
| 12 |
|
|
|
|
|
|
|
|
– | – | – | – | ||
| 13 |
|
|
|
|
|
|
– | – | – | – | – | – | ||
| 14 |
|
|
|
|
|
|
– | – | – | – | – | – | ||
Notes. Fits were performed with the CutoffPL model and a varying number of CRSFs. Uncertainties and upper limits are at the 90% confidence level for one interesting parameter.
Absorbed luminosity in units of 1037 erg s-1. LX covers the energy band 3–50 keV and was calculated using a distance of 7 kpc (Negueruela & Okazaki 2001).
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