Image Details
Caption: Figure 3.
Distribution of bolometric luminosity (top) and Eddington ratio (bottom) for the sample of AGN dwarf galaxies at z < 1 of Mezcua et al. (2023), the new “cosmic noon” sample of AGN in low-mass galaxies reported here, and a compilation of JWST AGN in low-mass galaxies at z > 4.
© 2024. The Author(s). Published by the American Astronomical Society.