AGN SIG Seminar
Active Galactic Nuclei Science Interest Group
DATE
Sep 13, 2022
TIME
12:00 pm EST
COMMUNITY
AGN SIG
TYPE
Seminar
Measuring AGN Hosts Properties at z > 3 with JWST
Dale Kocevski
AGN have become key components of most galaxy evolution models, yet several open issues remain in our understanding of how the link between galaxies and their SMBHs is established and maintained. Among these are the mechanism(s) responsible for fueling the bulk of SMBH growth across cosmic time and the role that AGN play in quenching the star formation activity of the first generation of massive quiescent galaxies. I will present recent results from the CEERS survey, which is using the James Webb Space Telescope (JWST) to determine the morphologies and stellar populations of AGN hosts at z > 3 for the first time. Surprisingly, we find AGN hosts at these redshifts have optical colors consistent with a quenched or post-starburst stellar population. The presence of AGN in passively evolving galaxies at z > 3 is significant because a rapid feedback mechanism is required in most cosmological simulations to explain the growing population of massive quiescent galaxies observed at these redshifts. I will also discuss what the morphologies of these galaxies tell us about the processes driving their nuclear activity.
Find the schedule and list of speakers on our website.
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