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Sphenix: Smoothed Particle Hydrodynamics for the next generation of galaxy formation simulations
Josh Borrow, Matthieu Schaller, Richard G. Bower +1
Smoothed Particle Hydrodynamics (SPH) is a ubiquitous numerical method for solving the fluid equations, and is prized for its conservation properties, natural adaptivity, and simpl…
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…
The Star-Formation Properties of the Observed and Simulated AGN Universe: BAT vs EAGLE
Thomas M. Jackson, D. J. Rosario, D. M. Alexander +3
In this paper we present data from 72 low redshift, hard X-ray selected AGN taken from the {\it Swift}-BAT 58 month catalogue. We utilise spectral energy distribution fitting to th…
Supermassive black holes in cosmological simulations I: M_BH-M_star relation and black hole mass function
Melanie Habouzit, Yuan Li, Rachel S. Somerville +15
The past decade has seen significant progress in understanding galaxy formation and evolution using large-scale cosmological simulations. While these simulations produce galaxies i…
Galactic inflow and wind recycling rates in the EAGLE simulations
Peter D. Mitchell, Joop Schaye, Richard G. Bower
The role of galactic wind recycling represents one of the largest unknowns in galaxy evolution, as any contribution of recycling to galaxy growth is largely degenerate with the inf…