Table 3.
Best-fit values of the spectral models for XMM-Newton data.
Component | Model 1 | Model 3 | Model 4 | |||
---|---|---|---|---|---|---|
Edge | ||||||
EO VIII (keV) | 0.871 (fixed) | 0.871 (fixed) | 0.871 (fixed) | |||
τO VIII | 0.7 ± 0.1 | 0.7 ± 0.1 | 0.7 ± 0.1 | |||
Edge | ||||||
EFe XXVI (keV) | 8.828 (fixed) | 8.828 (fixed) | 8.828 (fixed) | |||
τFe XXVI | 0.05 ± 0.01 | 0.04 ± 0.01 | 0.04 ± 0.01 | |||
phabs | ||||||
nH(1022) | 2.44 ± 0.04 | 2.40 ± 0.02 | 2.42 ± 0.04 | |||
diskbb | ||||||
kTin (keV) |
![]() |
![]() |
![]() |
|||
Rdisc (km) |
![]() |
![]() |
![]() |
|||
Fbb | ||||||
(10−9 erg cm−2 s−1) | 1.3 | |||||
nthComp | ||||||
Γ |
![]() |
![]() |
![]() |
|||
kTe (keV) |
![]() |
![]() |
![]() |
|||
kTseed (keV) |
![]() |
![]() |
0.7 ± 0.1 | |||
Norm |
![]() |
0.08 ± 0.02 |
![]() |
|||
FCompt | ||||||
(10−9 erg cm−2 s−1) | 2.4 | |||||
diskline | ||||||
betor | – |
![]() |
– | |||
θ (deg) | – | 35 ± 3 | – | |||
Rin (km) | – |
![]() |
– | |||
diskline | ||||||
EAr XVIII (keV) | – | 3.32 (fixed) | – | |||
NAr XVIII (×10−4) | – | 4.1 ± 1.2 | – | |||
diskline | ||||||
ECa XIX (keV) | – | 3.90 (fixed) | – | |||
NCa XIX (×10−4) | – |
![]() |
– | |||
diskline | ||||||
EFe XXV (keV) | – | 6.81 ± 0.07 | – | |||
NFe XXV (×10−4) | – | 5.7 ± 1.1 | – | |||
rdblur | ||||||
Betor10 | −2.8 (fixed) | – | −2.5 (fixed) | |||
Rin (km) |
![]() |
– |
![]() |
|||
θ (deg) |
![]() |
– |
![]() |
|||
gauss | ||||||
EAr XVIII (keV) | 3.32 (fixed) | – | 3.32 (fixed) | |||
NAr XVIII (×10−4) |
![]() |
– |
![]() |
|||
gauss | ||||||
ECa XIX (keV) | 3.90 (fixed) | – | 3.90 (fixed) | |||
NCa XIX (×10−4) |
![]() |
– |
![]() |
|||
rfxconv | ||||||
rel_refl |
![]() |
– |
![]() |
|||
logξ |
![]() |
– |
![]() |
|||
χ2(d.o.f.) | 2559(2245) | 2523(2244) | 2550(2245) |
Notes. Uncertainties are reported at 90% confidence level. The spectral parameters are defined as in XSPEC. The units of the line normalisations are in photons/cm2 s−1. Fbb and FCompt represent the unabsorbed fluxes in the (0.1–100) keV energy range associated with the accretion disc and the Comptonisation component, respectively.
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