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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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