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Table 3.
Parameters derived by adapting the baseline Model C to the archival data.
| Mission | Comp. | Par. | Visit 1 | Visit 2 | Visit 3 | Units |
|---|---|---|---|---|---|---|
| ASCA | tbabs | NH | 1.0±0.2 | ×1021 cm−2 | ||
| Borus | log NH | > 23.1 | ||||
| Norm | 1.6±1.5 | ×10−2 ph keV−1 cm−2 s−1 | ||||
| power-law | Γ | 1.91±0.08 | ||||
 |
500 | keV | ||||
| Norm | 3.9 ± 0.3 | ×10−3 ph keV−1 cm−2 s−1 | ||||
| χ2/d.o.f. | 360/403 | |||||
| p.null | 0.9 | |||||
| Flux0.5 − 2 keV | 6.0±0.1 | ×10−12 erg cm−2 s−1 | ||||
| Flux2 − 10 keV | 14.0±0.5 | ×10−12 erg cm−2 s−1 | ||||
| XMM-Newton | bb | Tbb | 180±15 | eV | ||
| Norm | 3.2±0.4 | ×10−5 L39 | ||||
| bb | Tbb | 75±10 | eV | |||
| Norm | 1.0±0.2 | ×10−4 L39 | ||||
| relxill | rin | 25 |
Rg | |||
| logξ | 1.5±0.2 | |||||
| Norm | 1.8±0.6 | ×10−5 ph keV−1 cm−2 s−1 | ||||
| Borus | log NH | 23.8±0.3 | ||||
| Norm | 3.0±0.6 | ×10−3 ph keV−1 cm−2 s−1 | ||||
| Power-law | Γ | 1.88±0.02 | ||||
| Norm | 6.5±0.1 | ×10−3 ph keV−1 cm−2 s−1 | ||||
| χ2/d.o.f. | 180/160 | |||||
| p.null | 0.2 | |||||
| Flux0.5 − 2 keV | 15.0±0.5 | ×10−12 erg cm−2 s−1 | ||||
| Flux2 − 10 keV | 20.0±0.5 | ×10−12 erg cm−2 s−1 | ||||
| Suzaku | bb | Tbb | 84±5 | 85±6 | 115±15 | eV |
| Norm | 1.3±0.8 | 1.4±0.3 | 1.1±0.3 | ×10−4 L39 | ||
| Relxill | rin | - | >2 | >10 | Rg | |
| logξ | >1.2 | 2.7±0.2 | 2.9±0.2 | |||
| Norm | 0.85±55 | 0.75±0.35 | 2.1±1.2 | ×10−5 ph keV−1 cm−2 s−1 | ||
| Borus | log NH | 22.7±0.4 | 23.7±0.2 | 23.4±0.5 | ||
| Norm | 2.0±1.0 | 2.1±0.4 | 2.3±0.4 | ×10−2 ph keV−1 cm−2 s−1 | ||
| Power-law | Γ | 1.77±0.02 | 1.80±0.02 | 1.85±0.02 | ||
| Ec | 500† | >120 | > 450 | keV | ||
| Norm | 3.35±0.4 | 5.0±0.1 | 7.4±0.3 | ×10−3 ph keV−1 cm−2 s−1 | ||
| Const | k | - | 1.3±0.10 | 1.16±0.08 | ||
| χ2/d.o.f. | 312/306 | 1527/1437 | 1017/967 | |||
| p.null | 0.42 | 0.04 | 0.097 | |||
| Flux0.5 − 2 keV | 8.2±0.4 | 11.7±0.3 | 21.0±0.7 | ×10−12 erg cm−2 s−1 | ||
| Flux2 − 10 keV | 13.0±0.5 | 19.1±0.3 | 27.7±0.4 | ×10−12 erg cm−2 s−1 | ||
Notes. The L39 stands for the luminosity in units of 1039 ergs s−1, and D10 is the distance in units of 10 kpc.
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