Table 2.
Priors used for simple spectral models.
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
|---|---|---|---|---|---|---|---|---|---|
| Model name | log(NHz) | Γh | log(nHabs) | log(ξwa) | Covering | Γs | log(c) | kT | norm |
| [cm−2] | [cm−2] | fraction | [keV] | ||||||
| Prior | log-uniform | Uniform | Uniform | Uniform | Uniform | Uniform | log-uniform | log-uniform | log-uniform |
| PL | 20 – 25 | 1 – 3 | – | – | – | – | – | – | −10 – 1 |
| PL+PCF | 20 – 25 | 1 – 3 | 20 – 25 | – | 0 – 1 | – | – | – | −10 – 1 |
| PL+WA | 20 – 25 | 1 – 3 | 20 – 24 | −4 – 4 | – | – | – | – | −10 – 1 |
| PL+BB | 20 – 25 | 1 – 3 | – | – | – | – | −3 – 1 | 0.04 – 0.4 | −10 – 1 |
| PL+PL | 20 – 25 | 1 – 3 | – | – | – | 2.25 – 10 | −3 – 1 | – | −10 – 1 |
Notes. Column (1) gives the shortened name of the model. Columns (2) shows the lower and upper limit of the host galaxy absorption. Columns (3) shows the lower and upper limit of the hard (coronal) power law component. Columns (4) and (5) show the upper and lower limits of the warm or partial covering absorber column density and ionisation component, respectively. Column (6) shows the upper and lower limit placed on the neutral absorption covering fraction. Column (7) shows the upper and lower limit placed on the soft X-ray photon index. Column (8) gives the constraints placed on the cross-normalisation placed on the soft excess component, and column (9) shows the constraints placed on the blackbody temperature. Column (10) gives the constraint placed on the hard power law normalisation.
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