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∼ …

Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …

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 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 …

We present initial results of a deep near-IR spectroscopic survey covering the 15 fields of the
Keck Baryonic Structure Survey using the recently commissioned MOSFIRE spectrometer on …

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 explore the kinematics of 27 z≳ 6 quasar host galaxies observed in [C ii] 158 μm ([C ii])
emission with the Atacama Large Millimeter/submillimeter Array at a resolution of≈ 025. We …