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Table C.2
Best fit parameters for a coronal model using a cutoff power-law and relativistic reflection with free emissivity index ϵ (Model 2).
| Parameter | Obs1 | Obs2 | Obs3 | Obs4 |
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| A pl |
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| Γpl | 1.736 ± 0.013 |
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| Efold [keV] |
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181 ± 16 |
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| A disk |
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(115 ± 8) × 102 |
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| kTdisk [keV] | 0.50 | 0.50 | 0.50 | 0.50 |
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| Aref [10-5] |
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1.6 ± 0.4 |
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| Fe/Fe⊙ |
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3.9 ± 0.9 |
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| Γ | 1.74 | 1.63 | 1.61 | 1.58 |
| ξ [erg cm s-1] |
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| ϵ 1 |
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| a | −0.59 ± 0.20 |
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| i [deg] |
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| F6.4 keV [103 cgs] | 1.20 ± 0.20 | 0.83 ± 0.19 |
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| Egauss [keV] | 6.40 | 6.40 | 6.40 | 6.40 |
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| Egabs [keV] | 6.646 | 6.646 | 6.646 | 6.646 |
| Eσ [keV] | 0.028 | 0.028 | 0.028 | 0.028 |
| τ [10-3] | ≤1.2 |
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≤ + 8.23 |
| Egabs [keV] | 6.955 | 6.955 | 6.955 | 6.955 |
| Eσ [keV] | 0.0013 | 0.0013 | 0.0013 | 0.0013 |
| τ [10-3] |
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≤2.6 | ≤ + 1.52 |
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| c HEXTE |
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0.825 ± 0.006 | 0.834 ± 0.004 | 0.827 ± 0.005 |
| c PN |
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0.780 ± 0.005 |
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0.812 ± 0.004 |
| c ISGRI | 0.924 ± 0.009 |
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0.903 ± 0.008 | 0.906 ± 0.008 |
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| s gainshift |
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| χ2/ d.o.f. | 541.1/392 | 411.0/319 | 581.4/442 | 391.3/331 |
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1.38 | 1.29 | 1.32 | 1.18 |
Notes. See Sect. 3.3.2 for more details.
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