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

E. Bernhard, L. P. Grimmett, J. R. Mullaney +3

We explore the distribution of RMS=SFR/SFR_MS (where SFR_MS is the star formation rate of "Main Sequence" star-forming galaxies) for AGN hosts at z=1. We split our sample into two…