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 …

Numerical simulations have become a major tool for understanding galaxy formation and
evolution. Over the decades the field has made significant progress. It is now possible to …

We present the new TNG50 cosmological, magnetohydrodynamical simulation–the third and
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …

We investigate the evolution of galaxy gas-phase metallicity (O/H) over the range z= 0–3.3
using samples of∼ 300 galaxies at z∼ 2.3 and∼ 150 galaxies at z∼ 3.3 from the MOSDEF …

We use cosmological simulations from the FIRE (Feedback In Realistic Environments)
project to study the baryon cycle and galaxy mass assembly for central galaxies in the halo …

We present a novel analytic framework to model the steady-state structure of multiphase
galactic winds comprised of a hot, volume-filling component and a cold, clumpy component …

ABSTRACT A very simple physical model of galaxies is one in which the formation of stars is
instantaneously regulated by the mass of gas in a reservoir with mass loss scaling with the …

We present PHIBSS, the IRAM Plateau de Bure high-z blue sequence CO 3–2 survey of the
molecular gas properties in massive, main-sequence star-forming galaxies (SFGs) near the …

In this paper we present the MOSFIRE Deep Evolution Field (MOSDEF) survey. The
MOSDEF survey aims to obtain moderate-resolution (R= 3000-3650) rest-frame optical …

We present integral field unit observations covering the [o iii] λλ4959, 5007 and Hβ emission
lines of 16 z< 0.2 type 2 active galactic nuclei (AGN). Our targets are selected from a well …