The Abundance of UV-Luminous Galaxies, Massive Galaxies, and Supermassive Black Holes at Early Times
The first data from JWST surprised us all with the revealed high abundance of UV-luminous galaxies, massive galaxies, and super-massive black holes. Now that the early days of discovery are behind us, we can begin to better assess which results stand the test of time, and for those, what physical processes can explain them. I will present recent results from the CEERS, PRIMER and NGDEEP surveys, exploring our current best-possible constraints on the abundance of UV luminous galaxies, whether any early galaxies are “too massive”, and what constraints we can place on the growth of early supermassive black holes.