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Fig. 3


Images of the AGN torus computed by ray-tracing at viewing directions corresponding to 15° (face-on, bottom), 45° (middle) and 75° (edge-on, top) and from left to right at wavelengths of 1 (gray), 10 (orange), and 100 μm (blue). The images are logarithmically scaled and at each wavelength the flux is normalized to its peak value.

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