The AGN fraction in high-redshift protocluster candidates selected by Planck and Herschel
Caleb Gatica,
Ricardo Demarco,
Hervé Dole
et al.
Abstract:A complete understanding of the mass assembly history of structures in the Universe requires the study of the growth of galaxies and their supermassive black holes (SMBHs) as a function of their local environment over cosmic time. In this context, it is important to quantify the effects that the early stages of galaxy cluster development have on the growth of SMBHs. We used a sample of Herschel/SPIRE sources of ∼ 228 red and compact Planck-selected protocluster (PC) candidates to estimate the active galactic n… Show more
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