학술논문
The $M_{\rm BH}-M_*$ relation up to $z\sim2$ through decomposition of COSMOS-Web NIRCam images
Document Type
Working Paper
Author
Tanaka, Takumi S.; Silverman, John D.; Ding, Xuheng; Jahnke, Knud; Trakhtenbrot, Benny; Lambrides, Erini; Onoue, Masafusa; Andika, Irham Taufik; Bongiorno, Angela; Faisst, Andreas L.; Gillman, Steven; Hayward, Christopher C.; Hirschmann, Michaela; Koekemoer, Anton; Kokorev, Vasily; Liu, Zhaoxuan; Magdis, Georgios E.; Renzini, Alvio; Casey, Caitlin; Drakos, Nicole E.; Franco, Maximilien; Gozaliasl, Ghassem; Kartaltepe, Jeyhan; Liu, Daizhong; McCracken, Henry Joy; Rhodes, Jason; Robertson, Brant; Toft, Sune
Source
Subject
Language
Abstract
Our knowledge of relations between supermassive black holes and their host galaxies at $z\gtrsim1$ is still limited, even though being actively sought out to $z\sim6$. Here, we use the high resolution and sensitivity of JWST to measure the host galaxy properties for 107 X-ray-selected type-I AGNs at $0.68