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Table C.3
Best fit parameters for a coronal model using a cutoff power-law and relativistic reflection where the emissivity follows a broken power-law (Model 3).
| Parameter | Obs1 | Obs2 | Obs3 | Obs4 |
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| A pl | 1.88 ± 0.08 | 1.08 ± 0.10 |
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| Γpl | 1.748 ± 0.014 |
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| Efold [keV] |
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170 ± 9 |
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| A disk | (163 ± 10) × 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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| ξ [erg cm s-1] |
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| ϵ 1 |
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| ϵ 2 | 3.0 | 3.0 | 3.0 | 3.0 |
| r br [GM/c2] |
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| a |
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0.86 ± 0.05 |
| i [deg] |
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28 ± 4 |
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| F6.4 keV [103 cgs] | 1.37 ± 0.20 |
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0.73 ± 0.20 |
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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 |
| τ [10-3] | ≤ 1.2 | 3.2 ± 2.7 | 4.7 ± 2.0 | ≤ 4.17 |
| Egabs [keV] | 6.955 | 6.955 | 6.955 | 6.955 |
| τ [10-3] |
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≤ 2.0 | ≤ 2.39 |
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| c HEXTE | 0.844 ± 0.006 | 0.823 ± 0.007 | 0.834 ± 0.004 | 0.826 ± 0.005 |
| c PN |
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0.813 ± 0.004 |
| c ISGRI | 0.923 ± 0.009 | 0.916 ± 0.010 | 0.903 ± 0.008 | 0.905 ± 0.008 |
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| s gainshift |
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| χ2/ d.o.f. | 544.6/386 | 394.6/318 | 574.3/441 | 397.7/330 |
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1.41 | 1.24 | 1.30 | 1.21 |
Notes. See Sect. 3.3.3 for more details.
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