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

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

Our knowledge of relations between supermassive black holes and their host galaxies at z  ≳ 1 is still limited, even though being actively sought out to z  ∼ 6. Here, we use the high resolution and sensitivity of JWST to measure the host galaxy properties for 107 X-ray-selected type-I active galacti...

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Bibliografski detalji
Glavni autori: Takumi S. Tanaka, John D. Silverman, Xuheng Ding, Knud Jahnke, Benny Trakhtenbrot, Erini Lambrides, Masafusa Onoue, Irham Taufik Andika, Angela Bongiorno, Andreas L. Faisst, Steven Gillman, Christopher C. Hayward, Michaela Hirschmann, Anton Koekemoer, Vasily Kokorev, Zhaoxuan Liu, Georgios E. Magdis, Alvio Renzini, Caitlin Casey, Nicole E. Drakos, Maximilien Franco, Ghassem Gozaliasl, Jeyhan Kartaltepe, Daizhong Liu, Henry Joy McCracken, Jason Rhodes, Brant Robertson, Sune Toft
Format: Članak
Jezik:English
Izdano: IOP Publishing 2025-01-01
Serija:The Astrophysical Journal
Teme:
Supermassive black holes
Active galactic nuclei
AGN host galaxies
Galaxy evolution
Online pristup:https://doi.org/10.3847/1538-4357/ad9d0a

Internet

https://doi.org/10.3847/1538-4357/ad9d0a

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