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Fig. 3
Dusty torus seen from an altitude Z in the jet under a solid angle dΩ. The torus is sliced according to θt ∈ [θtmin,θtmax] and ϕ ∈ [0,2π]. Each slice is illuminated by the disk and is in radiative equilibrium with a temperature T(θt,ϕ) and emits as a blackbody (ε = 1).
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