CC BY 4.0 UnportedTrebitsch, MaximeHutter, AnneDayal, PratikaGottlöber, StefanLegrand, LaurentYepes, Gustavo2023-06-022023-06-022022https://oa.tib.eu/renate/handle/123456789/12222http://dx.doi.org/10.34657/11254In this work, the sixth of a series, we use the seminumerical rAdiative tranSfer coupling of galaxy formaTion and Reionization in N-body dark-matter simUlationS (ASTRAEUS) framework to investigate the nature of the sources that reionized the Universe. We extend ASTRAEUS, which already couples a galaxy formation semi-analytical model with a detailed seminumerical reionization scheme, to include a model for black-hole formation, growth, and the production of ionizing radiation from associated active galactic nuclei (AGNs). We calibrate our fiducial AGN model to reproduce the bolometric luminosity function at z ≃ 5, and explore the role of the resulting AGN population in reionizing the Universe. We find that in all the models yielding a reasonable AGN luminosity function, galaxies dominate overwhelmingly the ionizing budget during the Epoch of Reionization, with AGN accounting for 1-10 per cent of the ionizing budget at z = 6 and starting to play a role only below z ≾ 5.enghttps://creativecommons.org/licenses/by/4.0520dark ages, reionization, first starsgalaxies: activegalaxies: high-redshiftintergalactic mediummethods: numericalArticle