SED of W0204–0506. The green circles show the measured flux densities and their 1σ uncertainties in the bands described in the text. The solid black line shows the best-fit SED model composed of a heavily obscured luminous AGN (dashed magenta line), a lightly obscured lower-luminosity AGN that accounts for the scattered light component (solid blue line), and a host galaxy from the Sbc template (dashed green line). The best-fit model has χ² = 18, but that is mostly driven by the H-band VHS photometry, which is possibly affected by a large equivalent width of the [O III] λ5007+4959 emission line. Removing this band results in a best-fit model with χ² = 11 with negligible changes to the parameter values.