Fig. 1.

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Overview of how the individual model components contribute to the summed emission (black). The AGN power-law continuum (blue; accretion disk, or BBB) is enhanced by emission lines including an iron forest (red). The disk model is normalised at the monochromatic luminosity at 5100 Å (blue square), here . The torus (yellow dashed curve) typically dominates the disk continuum above approximately 1 μm. The torus is normalised by the luminosity ratio 5100 Å to 12 μm (yellow diamond). The galaxy components include a stellar population (purple), nebular emission lines (gray at the bottom), and galaxy dust emission (green at the bottom right).
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