97 citations · 298 across the 7 of their papers we have counts for
7 papers
The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
Tomás Hough, Sofía A. Cora, Roan Haggar +6
In this work, we combine the semi-analytic model of galaxy formation and evolution SAG with the relaxed simulated galaxy clusters from The Three Hundred project, and we study…
The Three Hundred project: Galaxy groups do not survive cluster infall
Roan Haggar, Ulrike Kuchner, Meghan E. Gray +4
Galaxy clusters grow by accreting galaxies as individual objects, or as members of a galaxy group. These groups can strongly impact galaxy evolution, stripping the gas from galaxie…
The Three Hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies
Ana Contreras-Santos, Alexander Knebe, Frazer Pearce +10
Using the data set of The Three Hundred project, i.e. a suite of 324 hydrodynamical resimulations of cluster-sized haloes, we study galaxy cluster mergers and their effect on colou…
The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
Roan Haggar, Frazer R. Pearce, Meghan E. Gray +2
Dark matter-only simulations are able to produce the cosmic structure of a CDM universe, at a much lower computational cost than more physically motivated hydrodynamical simulat…
The Three Hundred project: shapes and radial alignment of satellite, infalling, and backsplash galaxies
Alexander Knebe, Matias Gamez-Marin, Frazer R. Pearce +6
Using 324 numerically modelled galaxy clusters we investigate the radial and galaxy-halo alignment of dark matter subhaloes and satellite galaxies orbiting within and around them.…
Mapping and characterisation of cosmic filaments in galaxy cluster outskirts: strategies and forecasts for observations from simulations
Ulrike Kuchner, Alfonso Aragón-Salamanca, Frazer R. Pearce +11
Upcoming wide-field surveys are well-suited to studying the growth of galaxy clusters by tracing galaxy and gas accretion along cosmic filaments. We use hydrodynamic simulations of…