Michael Tremmel

The IllustrisTNG simulations: public data release

First results from the IllustrisTNG simulations: matter and galaxy clustering

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

The origin of fast molecular outflows in quasars: molecule formation in AGN-driven galactic winds

Supermassive black holes and their feedback effects in the IllustrisTNG simulation

simba: Cosmological simulations with black hole growth and feedback

AGN feedback in a galaxy merger: Multi-phase, galaxy-scale outflows with a fast molecular gas blob ~6 kpc away from IRAS F08572+3915

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

The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies

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

The cosmic evolution of massive black holes in the Horizon-AGN simulation

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 black hole driven thermal and kinetic feedback

Simulating galaxy formation with the IllustrisTNG model

Off the beaten path: a new approach to realistically model the orbital decay of supermassive black holes in galaxy formation simulations

Introducingromulusc: a cosmological simulation of a galaxy cluster with an unprecedented resolution

The Romulus cosmological simulations: a physical approach to the formation, dynamics and accretion models of SMBHs

How to quench a galaxy

Dancing to changa: a self-consistent prediction for close SMBH pair formation time-scales following galaxy mergers