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Table 3
Best-fit parameter values for the broken power-law model
| Mrk 509 | |||||
| Obs. | Γs | Eb (keV) | Γh | Ch(10-3) | χ2/d.o.f. |
|
|
|||||
| 1 |
|
|
|
|
743/726 |
| 2 |
|
|
|
|
849/677 |
| 3 |
|
|
|
|
902/652 |
| 4 |
|
|
|
|
936/689 |
| 2+3+4 |
|
|
|
|
1248/721 |
|
|
|||||
| Mrk 841 | |||||
| Obs. | Γs | Eb (keV) | Γh | Ch(10-3) | χ2/d.o.f. |
|
|
|||||
| 1 |
|
|
|
|
686/651 |
| 2 |
|
|
|
|
604/613 |
| 1+2 |
|
|
|
|
804/694 |
Notes. XIS/FI data between 0.6 and 10 keV and XIS1 data between 0.5 and 8.5 keV were considered. The power-law normalization Ch is the number of photons keV-1 cm-2 s-1 at 1 keV.
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