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Table C.1
Best fit parameters for a coronal model using a cutoff power-law and relativistic reflection with fixed emissivity index ϵ = 3 (Model 1).
| Parameter | Obs1 | Obs2 | Obs3 | Obs4 |
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| Apl |
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1.56 ± 0.10 |
| Γpl | 1.724 ± 0.012 |
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| Efold [keV] | 181 ± 14 | 175 ± 13 |
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| A disk |
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(69 ± 7) × 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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| Fe/Fe⊙ |
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| Γ | 1.72 | 1.61 | 1.61 | 1.58 |
| ξ [erg cm s-1] |
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| ϵ 1 | 3.0 | 3.0 | 3.0 | 3.0 |
| a |
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| i [deg] |
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| F6.4 keV [103 cgs] | 1.44 ± 0.20 | 0.75 ± 0.18 | 0.75 ± 0.19 | 1.52 ± 0.29 |
| 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] | ≤ 0.6 |
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≤ 1.82 |
| Egabs [keV] | 6.955 | 6.955 | 6.955 | 6.955 |
| Eσ [keV] | 0.0013 | 0.0013 | 0.0013 | 0.0013 |
| τ [10-03] | ≤ 1.2 | ≤ 2.2 | ≤ 1.7 |
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| c HEXTE | 0.843 ± 0.006 | 0.826 ± 0.006 | 0.834 ± 0.004 | 0.826 ± 0.005 |
| c PN |
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0.813 ± 0.004 |
| c ISGRI |
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0.921 ± 0.009 | 0.903 ± 0.008 | 0.905 ± 0.008 |
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| s gainshift |
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| χ2/ d.o.f. | 574.0/393 | 418.7/320 | 582.1/443 | 406.1/332 |
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1.46 | 1.31 | 1.31 | 1.22 |
Notes. See Sect. 3.3.1 for more details.
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