Magnitudes for the “sEdd” and “overm” models and SMC-like dust. The orange triangles and gray circles show separately the flux of AGN and galaxies, when selecting systems with L_bol >  10⁴⁴ erg s⁻¹ and m444W < 28 (total flux, summing both AGN and galaxy contribution). The red dots have both of the above, plus the UNCOVER color selection, and show the combined galaxy+AGN flux. We have limited the y axis to 50 to highlight the relevant parameter space. At 115 and 200 the galaxy is almost always brighter than the AGN, whose contribution increases as the wavelength increases. For the “overm” case some AGN are brighter than the galaxy also at short wavelenghts.