108 papers found
Refreshing results…
The BUFFALO HST Survey
Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
Setting the scene for BUFFALO: A study of the matter distribution in the HFF galaxy cluster MACS J0416.1-2403 and its parallel field
Hydrostatic mass estimates of massive galaxy clusters: a study with varying hydrodynamics flavours and non-thermal pressure support
Energy equipartition between stellar and dark matter particles in cosmological simulations results in spurious growth of galaxy sizes
Constraining the inner density slope of massive galaxy clusters
The signal of decaying dark matter with hydrodynamical simulations
The gas fractions of dark matter haloes hosting simulated ∼L⋆ galaxies are governed by the feedback history of their black holes
The relationship between the morphology and kinematics of galaxies and its dependence on dark matter halo structure in EAGLE
SEAGLE--II: Constraints on feedback models in galaxy formation from massive early type strong lens galaxies
The evolution of the baryon fraction in haloes as a cause of scatter in the galaxy stellar mass in theeaglesimulation
The oxygen abundance gradients in the gas discs of galaxies in the EAGLE simulation
Ring galaxies in the EAGLE hydrodynamical simulations
SEAGLE – I. A pipeline for simulating and modelling strong lenses from cosmological hydrodynamic simulations
SWIFT: Maintaining weak-scalability with a dynamic range of $10^4$ in time-step size to harness extreme adaptivity
SWIFT: SPH With Inter-dependent Fine-grained Tasking
The evolution of the baryon fraction in halos as a cause of scatter in the galaxy stellar mass in the EAGLE simulation
The rapid growth phase of supermassive black holes
The origin of diverse α-element abundances in galaxy discs
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