99 citations · 470 across the 11 of their papers we have counts for
37 papers
The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
Evgenii Chaikin, Joop Schaye, Matthieu Schaller +3
Supernova (SN) feedback plays a crucial role in simulations of galaxy formation. Because blastwaves from individual SNe occur on scales that remain unresolved in modern cosmologica…
SIBELIUS-DARK: a galaxy catalogue of the Local Volume from a constrained realisation simulation
Stuart McAlpine, John C. Helly, Matthieu Schaller +7
We present SIBELIUS-DARK, a constrained realisation simulation of the local volume to a distance of 200~Mpc from the Milky Way. SIBELIUS-DARK is the first study of the \textit{Simu…
A sparse regression approach to modeling the relation between galaxy stellar masses and their host halos
M. Icaza-Lizaola, Richard G. Bower, Peder Norberg +3
Sparse regression algorithms have been proposed as the appropriate framework to model the governing equations of a system from data, without needing prior knowledge of the underlyi…
Stellar splashback: the edge of the intracluster light
Alis J. Deason, Kyle A. Oman, Azadeh Fattahi +8
We examine the outskirts of galaxy clusters in the C-EAGLE simulations to quantify the `edges' of the stellar and dark matter distribution. The radius of the steepest slope in the…
Inconsistencies arising from the coupling of galaxy formation sub-grid models to Pressure-Smoothed Particle Hydrodynamics
Josh Borrow, Matthieu Schaller, Richard G. Bower
Smoothed Particle Hydrodynamics (SPH) is a Lagrangian method for solving the fluid equations that is commonplace in astrophysics, prized for its natural adaptivity and stability. T…
A high-resolution cosmological simulation of a strong gravitational lens
Jack Richings, Carlos Frenk, Adrian Jenkins +2
We present a cosmological hydrodynamical simulation of a 10^13 Msun galaxy group and its environment (out to 10 times the virial radius) carried out using the EAGLE model of galaxy…