Over the past decade, increasingly robust estimates of the dense molecular gas content in
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …

We summarize what large surveys of the contemporary Universe have taught us about the
physics and phenomenology of the processes that link the formation and evolution of …

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 utilize high-resolution cosmological simulations to reveal that high-redshift galaxies tend
to undergo a robust 'wet compaction'event when near a 'golden'stellar mass of. This is a …

We combine molecular gas masses inferred from CO emission in 500 star-forming galaxies
(SFGs) between z= 0 and 3, from the IRAM-COLDGASS, PHIBSS1/2, and other surveys, with …

We present the KMOS 3D survey, a new integral field survey of over 600 galaxies at 0.7< z<
2.7 using KMOS at the Very Large Telescope. The KMOS 3D survey utilizes synergies with …

We use cosmological simulations to study a characteristic evolution pattern of high-redshift
galaxies. Early, stream-fed, highly perturbed, gas-rich discs undergo phases of dissipative …

In the cold dark matter cosmology, the baryonic components of galaxies—stars and gas—
are thought to be mixed with and embedded in non-baryonic and non-relativistic dark matter …

We introduce a new model for the structure and evolution of the gas in galactic discs. In the
model the gas is in vertical pressure and energy balance. Star formation feedback injects …

Using cosmological simulations, we address the properties of high-redshift star-forming
galaxies (SFGs) across their main sequence (MS) in the plane of star formation rate (SFR) …