Table 2.
Best-fit parameters obtained applying Model 3 (Rfxconv) and Model 4 (Relxillns) to the data.
Model | Parameter | Model 3(#) | Model 4 (#) | ||
---|---|---|---|---|---|
Oct. | 15 Apr. | Oct. | 15 Apr. | ||
Tbfeo | nH (1022) |
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O |
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|
Fe | 0.5 ± 0.4 |
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0.5 ± 0.3 | 0.7 ± 0.5 | |
Expabs | E (keV) | kTs( † ) | kTs( † ) | kTs( † ) | kTs( † ) |
Powerlaw | Index | 2.7 ± 0.2 |
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2.606 ( * ) |
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Norm |
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0.25 ± 0.04 |
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|
diskbb | Tin (keV) |
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0.61 ± 0.06 |
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Norm |
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|
Comptb | kTs (keV) |
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Γ | 3 ( * ) | 3 ( * ) | 3 ( * ) | 3 ( * ) | |
α |
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|
Δ | 0 ( * ) | 0 ( * ) | 0 ( * ) | 0 ( * ) | |
kTe (keV) | 2.88 ± 0.02 |
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2.91 ± 0.04 |
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|
log (A) | 8 ( * ) | 8 ( * ) | 8 ( * ) | 8 ( * ) | |
Norm | 0.051 ± 0.001 | 0.065 ± 0.002 | 0.052 ± 0.001 | 0.067 ± 0.002 | |
Reflection | Index |
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2.3 ( * ) |
Rin (Rg) |
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10 ± 2 ( ⊙ ) | < 35 |
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|
Rout | 1.0 ( * ) | 1.0 ( * ) | 1.0 ( * ) | 1.0 ( * ) | |
Incl (deg) |
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|
Rel refl |
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−1 ( * ) | −1 ( * ) | |
Feabund |
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< 0.77 ( ⋆ ) | < 1.26 ( ⋆ ) | |
log N | – | – | < 17.6 | < 16.5 | |
log ξ |
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2.8 ± 0.2 | |
Norm (10−4) | – | – |
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|
χ2/d.o.f. | 762/810 | 317/414 | 763/810 | 326/414 |
Notes. Uncertainties are calculated at the 90% confidence level. ( † )Linked to the seed-photon temperature. ( * )Kept frozen during the fit. ( ⊙ )Linked to the emitting radius of the diskbb component. ( ⋆ )Upper limit at 90% confidence level obtained fixing the seed photons and blackbody temperature. (#)Model 3: const*TBfeo*(expabs*powlaw+rdblur*rfxconv*Comptb+Comptb+diskbb) Model 4: const*TBfeo*(expabs*powlaw+Relxillns+Comptb+diskbb).
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