Table 3.
Inferred maximum a posteriori value and central 95% credible interval for the modelling of the spectrum and differential phase of IRAS 09149−6206.
| Parameters | Circular Keplerian model | Outflow model |
|---|---|---|
| RBLR (μas) |
 |
 |
| Rmin (μas) |
 |
 |
| β |
 |
 |
| θo (°) |
 |
 |
| i (°) |
 |
 |
| PA (° E of N) |
 |
 |
| κ | ... |
 |
| γ | ... |
 |
| ξ | ... |
 |
| Offset (μas) |
 |
 |
| log (MBH/M⊙) |
 |
 |
| fellip | 1 |
 |
| fflow | ... |
 |
| θe | ... |
 |
| log σturb | 0 |
 |
| ΔvBLR (km s−1) |
 |
 |
 |
1.39 | 1.38 |
| ln K | 0 | 7.1 ± 0.2 |
| Δ AIC | 0 | −12.6 |
| Δ BIC | 0 | 44.0 |
Notes. ΔvBLR is the difference between the velocity derived from the best-fit λemit and the systemic velocity based on the [O III] line (Perez et al. 1989). 
is the reduced χ2 of the models with the best-fit parameters. The Bayes factor, AIC, and BIC are relative to the Keplerian model.
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