Table 5.
Priors used for the physical true soft excess models.
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
|---|---|---|---|---|---|---|---|---|---|---|
| Model name | log(NHz) | Γh | Γs | log(c) | kTe | q1 | Inclination | log(ξ) | Reflection | norm |
| [cm−2] | [keV] | (degrees) | fraction | |||||||
| Prior | log-uniform | uniform | uniform | log-uniform | log-uniform | uniform | uniform | log-uniform | log-uniform | log-uniform |
| NTH | 20 – 25 | 1 – 3 | 2 – 3.5 | −3 – 1 | 0.1 – 1 | – | – | – | – | −10 – 1 |
| REL | 20 – 25 | 1 – 3 | – | – | – | 3 – 10 | 10 – 80 | 0 – 4 | 0.1 – 10 | −10 – 1 |
Notes. Column (1) gives the shortened name of the model. Column (2) shows the lower and upper limit of the host galaxy absorption. Column (3) shows the lower and upper limit of the hard (coronal) power law component. Columns (4) through (7) show the upper and lower limits of the warm Comptonisation parameters, and columns (8) through (10) shows the constraints placed on the blurred reflection parameters. Column (11) gives the constraint placed on the power law normalisation.
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