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Table 3.
Best-fit parameters derived for the different relativistic reflection models applied to the 2003 EPIC spectra of Mrk 1513.
| Model | relxilllp | relxillD |
|---|---|---|
| Galactic absorption (tbabs) | ||
| NH (1020 cm−2) | 3.7 | 3.7 |
| Warm absorber (xabs) | ||
| log ξ1 | 2.0 ± 0.1 | 1.7 ± 0.1 |
| NH, 1 (1021 cm−2) | 5.8 ± 1.1 | 4.3 ± 1.1 |
| log ξ2 | > 2.9 | > 2.5 |
| NH, 2 (1021 cm−2) | 4.8 ± 1.8 | 3.2 ± 2.2 |
| Direct + reflected continuum (relxill* ) | ||
| Γ | 2.02 ± 0.01 | 2.02 ± 0.04 |
| h (rg) | < 2.1 | – |
| ℛ | – | 0.90 ± 0.15 |
| q | – | > 7.9 |
| a* | > 0.997 | 0.15 ± 0.25 |
| log ξd | 1.15 ± 0.15 | 0.8 ± 0.1 |
| log (n/cm−3) | 15 (fixed) | > 18.7 |
| AFe | < 0.62 | 3.3 ± 1.1 |
| i (deg) | 43 ± 2 | 38 ± 3 |
| log F0.3 − 10 keV | −11.04 ± 0.01 | −11.08 ± 0.01 |
| C-stat/d.o.f. | 3245/3128 | 3194/3126 |
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