- Ding, Xuheng;
- Silverman, John;
- Treu, Tommaso;
- Schulze, Andreas;
- Schramm, Malte;
- Birrer, Simon;
- Park, Daeseong;
- Jahnke, Knud;
- Bennert, Vardha N;
- Kartaltepe, Jeyhan S;
- Koekemoer, Anton M;
- Malkan, Matthew A;
- Sanders, David
Correlations between the mass of a supermassive black hole and the properties
of its host galaxy (e.g., total stellar mass (M*), luminosity (Lhost)) suggest
an evolutionary connection. A powerful test of a co-evolution scenario is to
measure the relations MBH-Lhost and MBH-M* at high redshift and compare with
local estimates. For this purpose, we acquired HST imaging with WFC3 of 32
X-ray-selected broad-line AGN at 1.2