426 citations · 2.7k across the 29 of their papers we have counts for
29 papers
Simulating the diversity of shapes of the Lyman- line
Jeremy Blaizot, Thibault Garel, Anne Verhamme +6
The Ly line is a powerful probe of distant galaxies, which contains information about inflowing/outflowing gas through which Ly photons scatter. To develop our understanding…
Baryonic mass budgets for haloes in the EAGLE simulation, including ejected and prevented gas
Peter D. Mitchell, Joop Schaye
Feedback processes are expected to shape galaxy evolution by ejecting gas from galaxies and their associated dark matter haloes, and also by preventing diffuse gas from ever being…
How gas flows shape the stellar-halo mass relation in the EAGLE simulation
Peter D. Mitchell, Joop Schaye
The difference in shape between the observed galaxy stellar mass function and the predicted dark matter halo mass function is generally explained primarily by feedback processes. F…
Explaining the scatter in the galaxy mass-metallicity relation with gas flows
Maria L. van Loon, Peter D. Mitchell, Joop Schaye
The physical origin of the scatter in the relation between galaxy stellar mass and the metallicity of the interstellar medium, i.e. the Mass-Metallicity Relation (MZR), reflects th…
Tracing the simulated high-redshift circum-galactic medium with Lyman alpha emission
Peter Mitchell, Jérémy Blaizot, Corentin Cadiou +3
With the Multi Unit Spectroscopic Explorer (MUSE), it is now possible to detect spatially extended Lyman alpha emission from individual faint (M_UV ~ -18) galaxies at redshifts, 3…
The impact of stellar and AGN feedback on halo-scale baryonic and dark matter accretion in the EAGLE simulations
Ruby J. Wright, Claudia del P. Lagos, Chris Power +1
We use the EAGLE suite of hydrodynamical simulations to analyse accretion rates (and the breakdown of their constituent channels) onto haloes over cosmic time, comparing the behavi…