Fig. 8
SED of the radiative transfer NGC 1068 model for different inclination angles of the gas disk (red solid line: best-fit model with i = 60° and with a homogeneous screen of τV = 20; black solid line: i = 60° without a homogeneous screen; dashed black lines: i = 0, 30, and 90°). Blue diamonds: observations from Prieto et al. (2010). The typical uncertainties are on the order of 10%.
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