Table 6
Results from fitting the four hard state observations individually with phabs(diskbb+powerlaw+relconv∗xillver) using a full bandpass.
| Model | Parameter | 1 | 2 | 3 | 4 | 2b |
|
|
||||||
| q = 3 | ||||||
|
|
||||||
| phabs | NH (× 1022) | 0.62 ± 0.04 | 0.30 ± 0.01 | 0.24 ± 0.01 | 0.32 ± 0.03 | 0.38 |
| diskbb | Tin (keV) | 0.16 ± 0.01 | ... | ... | 0.22 |
0.27 ± 0.01 |
| NBB (× 103) | 3.72 |
... | ... | 14.0 |
3.94 |
|
| powerlaw | Γ | 1.68 ± 0.02 | 1.45 ± 0.01 | 1.49 ± 0.01 | 1.60 ± 0.01 | 1.90 ± 0.01 |
| N PL | 0.013 ± 0.001 | 0.086 ± 0.003 | 0.16 ± 0.01 | 0.41 ± 0.07 | 0.13 ± 0.01 | |
| relconv | θ (°) | 42 | ||||
| rin (risco) | >320 | 213 |
110 |
69 |
17 |
|
| xillver | log (ξ) | 1.83 |
2.61 |
2.63 ± 0.01 | 2.86 ± 0.03 | 2.78 |
| NR (10-6) | 1.60 |
3.29 |
5.11 ± 0.08 | 20.3 |
1.33 |
|
|
|
||||||
| χ 2 / ν | 2275/2227 | 1774/1614 | 2920/1614 | 1671/1612 | 2378/2226 | |
|
|
||||||
| q = 2.5 | ||||||
|
|
||||||
| phabs | NH (× 1022) | 0.62 ± 0.04 | 0.30 ± 0.01 | 0.24 ± 0.01 | 0.32 ± 0.03 | 0.38 |
| diskbb | Tin (keV) | 0.16 ± 0.01 | ... | ... | 0.22 ± + 0.02 | 0.27 ± 0.01 |
| NBB (× 103) | 3.72 |
... | ... | 14.0 |
3.81 |
|
| powerlaw | Γ | 1.68 ± 0.02 | 1.45 ± 0.01 | 1.49 ± 0.01 | 1.60 |
1.89 ± 0.01 |
| N PL | 0.013 ± 0.001 | 0.087 ± 0.003 | 0.16 ± 0.01 | 0.41 |
0.13 ± 0.01 | |
| relconv | θ (°) | 42 | ||||
| rin (risco) | >317 | 211 |
107 |
53 |
14 |
|
| xillver | log (ξ) | 1.83 |
2.60 |
2.63 ± 0.01 | 2.86 |
2.80 |
| NR (10-6) | 1.60 |
3.29 |
5.11 ± 0.08 | 20.4± 0.8 | 1.25 |
|
|
|
||||||
| χ 2 / ν | 2276/2227 | 1774/1614 | 2921/1614 | 1671/1612 | 2380/2226 | |
Notes. Results are presented for emissivity profiles of r-3 and r-2.5 (bottom). The photon index in the reflection models is tied to that of the continuum power-law and the Fe abundance is assumed to be solar. The same fixed values are used as for Table 3. In some cases the inner radius parameter has reached the largest tabulated value in the model (1000 rg), therefore we only present the lower limit in this case.
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