We present the full public release of all data from the TNG100 and TNG300 simulations of
the IllustrisTNG project. IllustrisTNG is a suite of large volume, cosmological, gravo …

We present a new cosmological, magnetohydrodynamical simulation for galaxy formation:
TNG50, the third and final instalment of the IllustrisTNG project. TNG50 evolves 2× 21603 …

We introduce the first two simulations of the IllustrisTNG project, a next generation of
cosmological magnetohydrodynamical simulations, focusing on the optical colours of …

We have generated synthetic images of∼ 27 000 galaxies from the IllustrisTNG and the
original Illustris hydrodynamic cosmological simulations, designed to match Pan-STARRS …

Using the IllustrisTNG simulations, we investigate the connection between galaxy
morphology and star formation in central galaxies with stellar masses in the range 109 …

We explore the abundance, spatial distribution, and physical properties of the O vi, O vii, and
O viii ions of oxygen in circumgalactic and intergalactic media (the CGM, IGM, and WHIM) …

We study the z= 0 gas kinematics, morphology and angular momentum content of isolated
galaxies in a suite of cosmological zoom-in simulations from the FIRE project spanning M …

We analyse the merger and assembly histories of Milky Way (MW) and Andromeda (M31)-
like galaxies to quantify how, and how often, disc galaxies of this mass can survive recent …

We study the abundance of satellite galaxies around 198 Milky Way-(MW) and M31-like
hosts in TNG50, the final installment in the IllustrisTNG suite of cosmological …

We use the TNG100 simulation of the IllustrisTNG project to investigate the stellar specific
angular momenta (j*) of∼ 12 000 central galaxies at z= 0 in a full cosmological context, with …