activity
20172020
most citedThe evolution of SMBH spin and AGN luminosities for within a semi-analytic model of galaxy formation

59 citations · 166 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2020★ 1 cited

The evolution of radio jets across cosmic time

Andrew J. Griffin, Cedric G. Lacey, Violeta Gonzalez-Perez +1

We present predictions for the evolution of radio emission from Active Galactic Nuclei (AGNs). We use a model that follows the evolution of Supermassive Black Hole (SMBH) masses an…

astro-ph.GA2020★ 39 cited

Do model emission line galaxies live in filaments at z~1?

V. Gonzalez-Perez, W. Cui, S. Contreras +7

Current and future cosmological surveys are targeting star-forming galaxies at with nebular emission lines. We use a state-of-the-art semi-analytical model of galaxy form…

astro-ph.GA2019★ 13 cited

AGNs at the cosmic dawn: predictions for future surveys from a CDM cosmological model

Andrew J. Griffin, Cedric G. Lacey, Violeta Gonzalez-Perez +3

Telescopes to be launched over the next decade-and-a-half, such as JWST, EUCLID, ATHENA and Lynx, promise to revolutionise the study of the high redshift Universe and greatly advan…

astro-ph.GA2019★ 41 cited

The first Super Massive Black Holes: indications from models for future observations

Stergios Amarantidis, José Afonso, Hugo Messias +12

We present an exploration of the expected detection of the earliest Active Galactic Nuclei (AGN) in the Universe from state-of-art galaxy formation and evolution semi-analytic mode…

astro-ph.GA2018★ 59 cited

The evolution of SMBH spin and AGN luminosities for within a semi-analytic model of galaxy formation

Andrew J. Griffin, Cedric G. Lacey, Violeta Gonzalez-Perez +3

Understanding how Active Galactic Nuclei (AGN) evolve through cosmic time allows us to probe the physical processes that control their evolution. We use an updated model for the ev…

astro-ph.GA2017★ 13 cited

The environment of radio galaxies: A signature of AGN feedback at high redshifts

David Izquierdo-Villalba, Alvaro A. Orsi, Silvia Bonoli +3

We use the semi-analytical model of galaxy formation GALFORM to characterise an indirect signature of AGN feedback in the environment of radio galaxies at high redshifts. The predi…