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 were performed with an enhanced version of the GADGET code that includes a modified hydrodynamics solver, time-step limiter and subgrid treatments of baryonic physics, such as stellar mass loss, element-by-element radiative cooling, star formation and feedback from star formation and black hole accretion. The simulation suite includes runs performed in volumes ranging from 25 to 100 comoving megaparsecs per side, with numerical resolution chosen to marginally resolve the Jeans mass of the gas at the star formation threshold. The free parameters of the subgrid models...
We present results from 13 cosmological simulations that explore the parameter space of the ‘Evoluti...
We introduce the Virgo Consortium's EAGLE project, a suite of hydrodynamical simulations that follow...
The Hubble sequence provides a useful classification of galaxy morphology at low redshift. However, ...
We present the public data release of halo and galaxy catalogues extracted from the EAGLE suite of c...
We present the public data release of halo and galaxy catalogues extracted from the eagle suite of c...
We investigate the evolution of galaxy masses and star formation rates in the Evo-lution and Assembl...
We present results from thirteen cosmological simulations that explore the parameter space of the "E...
We investigate the evolution of galaxy masses and star formation rates in the Evolution and Assembly...
We introduce the Virgo Consortium's Evolution and Assembly of GaLaxies and their Environments (EAGLE...
We present results from thirteen cosmological simulations that explore the parameter space of the "E...
We present results from thirteen cosmological simulations that explore the parameter space of the "E...
We introduce the Virgo Consortium's EAGLE project, a suite of hydrodynamical simulations that follow...
We investigate the evolution of galaxy masses and star formation rates in the Evolution and Assembly...
We introduce the Virgo Consortium's Evolution and Assembly of GaLaxies and their Environments (EAGLE...
We introduce the Virgo Consortium's Evolution and Assembly of GaLaxies and their Environments (EAGLE...
We present results from 13 cosmological simulations that explore the parameter space of the ‘Evoluti...
We introduce the Virgo Consortium's EAGLE project, a suite of hydrodynamical simulations that follow...
The Hubble sequence provides a useful classification of galaxy morphology at low redshift. However, ...
We present the public data release of halo and galaxy catalogues extracted from the EAGLE suite of c...
We present the public data release of halo and galaxy catalogues extracted from the eagle suite of c...
We investigate the evolution of galaxy masses and star formation rates in the Evo-lution and Assembl...
We present results from thirteen cosmological simulations that explore the parameter space of the "E...
We investigate the evolution of galaxy masses and star formation rates in the Evolution and Assembly...
We introduce the Virgo Consortium's Evolution and Assembly of GaLaxies and their Environments (EAGLE...
We present results from thirteen cosmological simulations that explore the parameter space of the "E...
We present results from thirteen cosmological simulations that explore the parameter space of the "E...
We introduce the Virgo Consortium's EAGLE project, a suite of hydrodynamical simulations that follow...
We investigate the evolution of galaxy masses and star formation rates in the Evolution and Assembly...
We introduce the Virgo Consortium's Evolution and Assembly of GaLaxies and their Environments (EAGLE...
We introduce the Virgo Consortium's Evolution and Assembly of GaLaxies and their Environments (EAGLE...
We present results from 13 cosmological simulations that explore the parameter space of the ‘Evoluti...
We introduce the Virgo Consortium's EAGLE project, a suite of hydrodynamical simulations that follow...
The Hubble sequence provides a useful classification of galaxy morphology at low redshift. However, ...