CORDIS Project
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This project explores the relationship between supermassive black holes and their host galaxies, focusing on clustering properties of X-ray active galactic nuclei. It aims to test theories of black hole formation and co-evolution with galaxies using observational data.
The presence of a supermassive black hole (BH) in almost all galaxies in the Universe is an accepted paradigm in astronomy.
How these BHs form and how they co-evolve with the host galaxy is one of the most intriguingunanswered problems in modern Cosmology and of extreme relevance to understand the issue of galaxy formation.Clustering measurements can powerfully test theoretical model predictions of BH triggering scenarios and put constraints on the typical environment where AGN live in, through…
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