SED of the radiative transfer Circinus model for different inclination angles of the gas disk (solid red line: best-fit model with i = 65° and with a homogeneous screen of τ_V = 20; solid black line: i = 65° without a homogeneous screen; dashed black lines: i = 0, 30, 60, and 90°; blue dashed line: Tristram et al. 2014 model). Blue diamonds: observations from Prieto et al. (2010). The typical uncertainties are on the order of 10%. Blue pluses: low resolution IRAS photometry. These points can be regarded as upper limits.