Ben Keller

Massive disc galaxies too dominated by dark matter in cosmological hydrodynamical simulations

The IllustrisTNG simulations: public data release

First results from the IllustrisTNG simulations: matter and galaxy clustering

Theoretical Challenges in Galaxy Formation

The kinematics and dark matter fractions of TNG50 galaxies at z = 2 from an observational perspective

The new semi-analytic code GalICS 2.0 – reproducing the galaxy stellar mass function and the Tully–Fisher relation simultaneously

The fraction of dark matter within galaxies from the IllustrisTNG simulations

A small-scale dynamo in feedback-dominated galaxies – II. The saturation phase and the final magnetic configuration

The EAGLE simulations: atomic hydrogen associated with galaxies

A small-scale dynamo in feedback-dominated galaxies as the origin of cosmic magnetic fields – I. The kinematic phase

First results from the IllustrisTNG simulations: radio haloes and magnetic fields

A model for core formation in dark matter haloes and ultra-diffuse galaxies by outflow episodes

First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies

Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model

The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations

The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time

Non-circular motions and the diversity of dwarf galaxy rotation curves

The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end

First results from the IllustrisTNG simulations: the galaxy colour bimodality

First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback

Simulating galaxy formation with the IllustrisTNG model

NIHAO project II: halo shape, phase-space density and velocity distribution of dark matter in galaxy formation simulations

Gasoline2: a modern smoothed particle hydrodynamics code

Cosmological galaxy evolution with superbubble feedback – I. Realistic galaxies with moderate feedback

Cosmological galaxy evolution with superbubble feedback – II. The limits of supernovae

NIHAO III: the constant disc gas mass conspiracy

NIHAO – IV: core creation and destruction in dark matter density profiles across cosmic time

NIHAO project – I. Reproducing the inefficiency of galaxy formation across cosmic time with a large sample of cosmological hydrodynamical simulations

A superbubble feedback model for galaxy simulations