The evolution of the content of heavy elements in galaxies, the relative chemical
abundances, their spatial distribution, and how these scale with various galactic properties …

Characterizing the relationship between stars, gas, and metals in galaxies is a critical
component of understanding the cosmic baryon cycle. We compile contemporary censuses …

We introduce a suite of cosmological volume simulations to study the evolution of galaxies
as part of the Feedback in Realistic Environments project. FIREbox, the principal simulation …

Aims. We propose to infer the output of the ionising continuum-leaking properties of galaxies
based upon their Lyα line profiles. Methods. We carried out Lyα radiation transfer …

We study metal depletion due to dust in the interstellar medium (ISM) to infer the properties
of dust grains and characterize the metal and dust content of galaxies down to low metallicity …

We study the link between galaxies and H i-selected absorption systems at z∼ 3–4 in the
MUSE Analysis of Gas around Galaxies (MAGG) survey, an ESO large programme …

Damped absorbers, seen in the spectra of background quasars, are unique probes to select
H i-rich galaxies. These galaxies allow one to estimate the neutral gas mass over …

Starting from a summary of detection statistics of our recent X-shooter campaign, we review
the major surveys, both space and ground based, for emission counterparts of high-redshift …

We describe the execution and data reduction of the European Southern Observatory Large
Programme “Quasars and their absorption lines: a legacy survey of the high-redshift …

We report the serendipitous detection of a 0.2 L*, Lyα emitting galaxy at redshift 2.5 at an
impact parameter of 50 kpc from a bright background QSO sightline. A high-resolution …