activity
20172026
most citedIntroducing the NewHorizon simulation: Galaxy properties with resolved internal dynamics across cosmic time

229 citations · 1.8k across the 45 of their papers we have counts for

collaborators
Showing 2018Show all

5 papers · 1 filter

astro-ph.GA2018★ 109 cited

Super-Eddington Accretion and Feedback from the First Massive Seed Black Holes

John A. Regan, Turlough P. Downes, Marta Volonteri +4

Super-Eddington accretion onto massive black hole seeds may be commonplace in the early Universe, where the conditions exist for rapid accretion. Direct collapse black holes are of…

astro-ph.GA2018★ 24 cited

Zooming in on supermassive black holes: how resolving their gas cloud host renders their accretion episodic

Ricarda S. Beckmann, Julien Devriendt, Adrianne Slyz

Born in rapidly evolving mini-halos during the first billion years of the Universe, super- massive black holes (SMBH) feed from gas flows spanning many orders of magnitude, from th…

astro-ph.CO2018★ 17 cited

Discovery of a diffuse optical line emitting halo in the core of the Centaurus cluster of galaxies: Line emission outside the protection of the filaments

S. L. Hamer, A. C. Fabian, H. R. Russell +6

We present the discovery of diffuse optical line emission in the Centaurus cluster seen with the MUSE IFU. The unparalleled sensitivity of MUSE allows us to detect the faint emissi…

astro-ph.HE2018★ 42 cited

Bondi or not Bondi: the impact of resolution on accretion and drag force modelling for Supermassive Black Holes

Ricarda Sylvia Beckmann, Julien Devriendt, Adrianne Slyz

Whilst in galaxy-size simulations, supermassive black holes (SMBH) are entirely handled by sub-grid algorithms, computational power now allows the accretion radius of such objects…

astro-ph.CO2018★ 187 cited

The impact of baryons on the matter power spectrum from the Horizon-AGN cosmological hydrodynamical simulation

Nora Elisa Chisari, Mark L. A. Richardson, Julien Devriendt +7

Accurate cosmology from upcoming weak lensing surveys relies on knowledge of the total matter power spectrum at percent level at scales /Mpc, for which modelling the im…