Intrinsic 2–10 keV luminosity of the SW nucleus estimated for the reflection-dominated model SW-R, as a function of assumed inclination angle (θ_i) of the obscuring torus. The intrinsic luminosity, , is in units of 10⁴³ erg s⁻¹. For θ_i = 42° −72°, θ_i = θ_op + 2° is assumed. For the point for θ_i = 82°, θ_op = 70° is used as it is the upper bound of the etorus model. The thick horizontal line indicates the best-estimate of erg s⁻¹, which was obtained by combining the X-ray and mid-IR feature based estimates (see Sect. 4.1) and the 95% CI is indicated by two dotted-lines. The value derived from the nominal SW-A model (see Table 2) is 0.2 × 10⁴³ erg s⁻¹, i.e. the bottom of the panel, but it could go up within the shaded area depending on an assumed geometry (see text) in the absorption model.