The MBH-M∗ Relation up to z ∼ 2 through Decomposition of COSMOS-Web NIRCam Images

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

doi:10.3847/1538-4357/ad9d0a

research article

The M_BH-M_∗ Relation up to z ∼ 2 through Decomposition of COSMOS-Web NIRCam Images

Tanaka, Takumi S.

•

Silverman, John D.

•

Ding, Xuheng

February 1, 2025

The Astrophysical Journal

Our knowledge of relations between supermassive black holes and their host galaxies at z greater than or similar to 1 is still limited, even though being actively sought out to z similar to 6. 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

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10.3847_1538-4357_ad9d0a.pdf

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