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Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models
Quan Guo, Violeta Gonzalez-Perez, Qi Guo +12
We compare global predictions from the EAGLE hydrodynamical simulation, and two semi-analytic (SA) models of galaxy formation, L-GALAXIES and GALFORM. All three models include the…
The APOSTLE simulations: solutions to the Local Group's cosmic puzzles
Till Sawala, Carlos S. Frenk, Azadeh Fattahi +13
The Local Group of galaxies offer some of the most discriminating tests of models of cosmic structure formation. For example, observations of the Milky Way (MW) and Andromeda satel…
Size evolution of normal and compact galaxies in the EAGLE simulation
M. Furlong, R. G. Bower, R. A. Crain +7
We present the evolution of galaxy sizes, from redshift 2 to 0, for actively star forming and passive galaxies in the cosmological hydrodynamical 1003 cMpc3 simulation of the EAGLE…
The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues
Stuart McAlpine, John C. Helly, Matthieu Schaller +16
We present the public data release of halo and galaxy catalogues extracted from the EAGLE suite of cosmological hydrodynamical simulations of galaxy formation. These simulations we…
A unified multi-wavelength model of galaxy formation
Cedric G. Lacey, Carlton M. Baugh, Carlos S. Frenk +7
We present a new version of the GALFORM semi-analytical model of galaxy formation. This brings together several previous developments of GALFORM into a single unified model, includ…
The COpernicus COmplexio: Statistical Properties of Warm Dark Matter Haloes
Sownak Bose, Wojciech A. Hellwing, Carlos S. Frenk +4
The recent detection of a 3.5 keV X-ray line from the centres of galaxies and clusters by Bulbul et al. (2014a) and Boyarsky et al. (2014a) has been interpreted as emission from th…