Big and young supermassive black holes in the early Universe
Tullia Sbarrato

TL;DR
This paper reviews the discovery and implications of extremely massive blazars at high redshifts, shedding light on the early formation and growth of supermassive black holes and their jets in the universe.
Contribution
It provides a systematic overview of high-redshift blazar discoveries and discusses their significance for models of supermassive black hole evolution in the early universe.
Findings
Massive blazars at z>4 challenge existing black hole formation models.
Different formation epochs observed for jetted and non-jetted black holes.
Open questions identified for future research in black hole and jet evolution.
Abstract
Blazars are Active Galactic Nuclei characterized by relativistic jets launched in the vicinity of the central engine (i.e. a supermassive black hole), that are oriented close to our line of sight. Their peculiar orientation makes them very efficient tracers of the overall jetted population, and due to their brightness they can be visible up to very high redshifts. A deep knowledge of these objects can provide fundamental clues to the models of formation and growth of the first supermassive black holes, but their search in the early Universe must be careful and follow a systematic approach. The discovery in the last years of extremely massive blazars at very high redshifts () revolutionized our perception of their earliest evolution: there seem to be different formation epochs for extremely massive black holes hosted in jetted () and…
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