Table 2
Results of continuum fits to our five selected observations using the model phabs∗powerlaw, ordered by increasing flux.
| Observation | Γ | N PL | Flux | χ 2 / ν | ||
|
|
||||||
| 1 | 1.565 ± 0.012 | 0.011 ± 0.001 | 0.82 | 777/791 | ||
| 2 | 1.437 ± 0.008 | 0.098 ± 0.001 | 8.30 | 714/668 | ||
| 2b | 1.807 ± 0.009 | 0.144 ± 0.003 | 8.46 | 882/789 | ||
| 3 | 1.476 ± 0.003 | 0.186 ± 0.001 | 15.05 | 812/666 | ||
| 4 | 1.647 ± 0.004 | 0.919 ± 0.006 | 59.61 | 765/658 | ||
Notes. An additional smedge is added to Observation 4 to account for the significant residual beyond 8 keV. The unabsorbed flux is in units of × 10-10 erg cm-2 s-1 and calculated in the 0.5−10 keV energy range using the model cflux.
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