Title: Supermassive black holes in the Universe
Speaker: Jian-Min Wang
Outlines
- Formation of SMBHs
- Masses and spins
- SMBH binaries and nanohertz GWs
- Satellite BHs and observational consequences
- Opportunities in the era of JWST and VLTI
First quasar: 3C 273


So broad H
Formation of SMBHs


Does the mass of BH grow first or that of the host galaxy?
The masses of BHs are mainly from accretion. SMBHs favor super-Eddington accretion.

Masses an spins

“It is hard to say that the spin depends on the mass.”
SMBH binaries and nanohertz GWs

Pile-up mass function
