What drives the growth of black holes: a decade of progress
D.M. Alexander (CEA-Durham), R.C. Hickox (Dartmouth College), J. Aird (Edinburgh), F. Combes (Obs de Paris), T. Costa (Newcastle), M. Habouzit (Geneva), C.M. Harrison (Newcastle), R.I. Leng (Edinburgh), L.K. Morabito (CEA-Durham), S.L. Uckelman (Durham), P. Vickers (Durham)

TL;DR
Over the past decade, significant advances have been made in understanding super-massive black hole growth, AGN physics, and their impact on galaxy evolution, driven by new data, techniques, and facilities.
Contribution
This review synthesizes a decade of progress in SMBH and AGN research, highlighting new insights, methodologies, and the influence of technological advancements.
Findings
Enhanced understanding of SMBH accretion physics
Identification of AGNs up to redshift 10
Comprehensive census of AGN activity across cosmic time
Abstract
The last decade has witnessed significant progress in our understanding of the growth of super-massive black holes (SMBHs). It is now clear that an Active Galactic Nucleus (AGN: the observed manifestation of a growing SMBH) is an "event" within the broader lifecycle of a galaxy, which can significantly influence the shape and evolution of the galaxy itself. Our view of the obscuring medium that affects the observed properties of an AGN has also undergone a revolution, and we now have a more physical understanding of the connection between the fuelling of (and feedback from) the SMBH and the broader host-galaxy and larger-scale environment. We have a greater understanding of the physics of SMBH accretion, can identify AGNs out to z = 8-10 witnessing the very earliest phases of SMBH growth, and have a more complete census of AGN activity than ever before. This great progress has been…
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Taxonomy
TopicsRelativity and Gravitational Theory · Cosmology and Gravitation Theories
