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  • The $M_{\rm BH}-M_*$ relation up to $z\sim2$ through decomposition of COSMOS-Web NIRCam images
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The $M_{\rm BH}-M_*$ relation up to $z\sim2$ through decomposition of COSMOS-Web NIRCam images

Fuente: arXiv
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Bibliographic Details
Main Authors: 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
Format: Preprint
Published: 2024
Subjects:
Astrophysics of Galaxies
Online Access:
Acceder al recurso
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Internet

https://arxiv.org/abs/2401.13742

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