We present PHANGS–ALMA, the first survey to map CO J= 2→ 1 line emission at∼ 1''∼ 100
pc spatial resolution from a representative sample of 90 nearby (d≲ 20 Mpc) galaxies that lie …

Inference of the physical properties of stellar populations from observed photometry and
spectroscopy is a key goal in the study of galaxy evolution. In recent years, the quality and …

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 …

How do galaxies transform from blue, star-forming spirals to red, quiescent early-type
galaxies? To answer this question, we analyzed a set of 26 gas-rich, shocked post-starburst …

We present a modified version of the l-galaxies2020 semi-analytic model of galaxy
evolution, which includes significantly increased direct metal enrichment of the …

The evolution of satellite galaxies is shaped by their constant interaction with the
circumgalactic medium surrounding central galaxies, which in turn may be affected by gas …

We explore how the star formation and metal enrichment histories of present-day galaxies
have been affected by environment combining stellar population parameter estimates and …

We derive ages, metallicities, and individual element abundances of early-and late-type
galaxies (ETGs and LTGs) out to 1.5 R e. We study a large sample of 1900 galaxies …

We present a variation of the recently updated Munich semi-analytical galaxy formation
model, l-Galaxies, with a new gas stripping method. Extending earlier work, we directly …

ABSTRACT We have used Galaxy Zoo DECaLS (GZD) to study strong and weak bars in disc
galaxies. Out of the 314 000 galaxies in GZD, we created a volume-limited sample (0.01< z< …