Table A.1.
Best-fit model parameters with consistent flux and shape for model C.
| Component | Parameter | model C |
|---|---|---|
| Interstellar absorption | NH(1022 cm−2) | 0.14(f) |
| Photon Index | 1.400 | |
| Power law | cut-off(keV) | 300(f) |
| Norm | 0.678 | |
| Flux | 4.89×10−8 | |
| rin (Rg) | 2.71 | |
| rout (Rg) | 1000(f) | |
| ξshape (≊ξflux) | 8.84×103 | |
| Inner reflection | ξin | 3.53×104 |
| n (1015 cm−3) | 1.49×104 | |
| Norm | 1.24 | |
| Flux | 4.27×10−9 | |
| rin (Rg) | 445 | |
| rout (Rg) | 1000(f) | |
| ξshape (≊ξflux) | 100(f) | |
| Outer reflection | ξin | 231 |
| n (1015 cm−3) | 1.10×103 | |
| Norm | 198.91 | |
| Flux | 3.08×10−8 | |
| χ2/ν | 2141/1865 | |
Notes. Due to the delicacy involved in manual iteration, reasonably good fit (with ξshape and ξflux lie within 5% range) is achieved, not the best fit, which also prohibits to find the errors associated to the fitted parameters. ξ at inner radius of the disk (ξin) is computed from the fitted ξshape ≊ ξflux. The tabulated flux is the unabsorbed one in units of ergs.cm−2.sec−1, calculated from XSPEC within energy range 1 eV - 1 MeV. The frozen parameters during fitting are indicated as (f).
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