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 …

Hydrodynamical cosmological simulations are increasing their level of realism by
considering more physical processes and having greater resolution or larger statistics …

We present an analysis of the galaxy-scale gaseous outflows from the Feedback in Realistic
Environments (FIRE) simulations. This suite of hydrodynamic cosmological zoom …

The dramatic first images with JWST demonstrated its power to provide unprecedented
spatial detail for galaxies in the high-redshift universe. Here, we leverage the resolution and …

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 …

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 …

Observations of galaxy isophotes, long-slit kinematics, and high-resolution photometry
suggested a possible dichotomy between two distinct classes of elliptical galaxies. But these …

We use FIRE simulations to study disc formation in z∼ 0, Milky Way-mass galaxies, and
conclude that a key ingredient for the formation of thin stellar discs is the ability for accreting …