Self-consistent population synthesis of active galactic nuclei from observational constraints in the X-rays

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Table 1.

Overview of the models explored, their free parameters, and priors as discussed in Sect. 3.3.

Model ¹	μ (log/cm⁻²) ²	σ (log/ cm⁻²) ²	R₀³^a	α³	R₁⁴^a
0pt1emSimple torus	21.5–25.5	0.01–2.5	–	–	0.01–1.5
LD torus	21.5–25.5	0.01–2.5	0.01–1.5	0.01–1.0	–
LD+AD	21.5–25.5	0.01–2.5	0.01–1.5	0.01–1.0	–

Notes.

Simple torus, luminosity-dependent (LD) torus, and LD torus with an accretion disc (AD).

Mean, μ, and standard deviation, σ, of the tori N_H,eq distribution.

Normalisation, R₀, and slope, α, in Eq. (3).

⁴

Scaling parameter, R₁, of the simple torus.

Arbitrary units for models without AD and measured in parsec for the AD model.

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