JWST MIRI data from the CEERS survey yield a first mid-infrared AGN luminosity function, suggesting obscured black hole accretion density peaks at z 1 to 3 and may exceed X-ray estimates at z about 3.
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Inferring Obscured Cosmic Black Hole Accretion History from AGN Found by JWST/MIRI CEERS Survey
JWST MIRI data from the CEERS survey yield a first mid-infrared AGN luminosity function, suggesting obscured black hole accretion density peaks at z 1 to 3 and may exceed X-ray estimates at z about 3.