Piercing through Highly Obscured and Compton-thick AGNs in the Chandra Deep Fields. II. Are Highly Obscured AGNs the Missing Link in the Merger-triggered AGN-Galaxy Coevolution Models?

By using a large, highly obscured ( N-H > 10(23) cm(-2)) active galactic nucleus (AGN) sample (294 sources at z similar to 0-5) selected from detailed X-ray spectral analyses in the deepest Chandra.surveys, we explore distributions of these X-ray sources in various optical/infrared/X-ray color-co...

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Detalles Bibliográficos
Autores principales: Li, Junyao, Xue, Yongquan, Sun, Mouyuan, Brandt, William N., Yang, Guang, Vito, Fabio, Tozzi, Paolo, Vignali, Cristian, Comastri, Andrea, Shu, Xinwen, Fang, Guanwen, Fan, Lulu, Luo, Bin, Chen, Chien-Ting, Zheng, Xuechen
Formato: Artículo (Article)
Idioma:Inglés (English)
Publicado: 2025
Materias:
AGN host galaxies
Active galaxies
X-ray active galactic nuclei
Acceso en línea:https://repositorio.uc.cl/handle/11534/100378

Internet

https://repositorio.uc.cl/handle/11534/100378

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