galaxies: evolution

A binning-free method reveals a continuous relationship between galaxies' AGN power and offset from main sequence

Revealing the differences in the SMBH accretion rate distributions of starburst and non-starburst galaxies

Inferring a difference in the star-forming properties of lower versus higher X-ray luminosity AGNs

Evidence for a mass-dependent AGN Eddington ratio distribution via the flat relationship between SFR and AGN luminosity