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 …

The chemical enrichment of dust and metals in the interstellar medium of galaxies
throughout cosmic time is one of the key driving processes of galaxy evolution. Here we …

We describe the scientific goals and survey design of the First Large Absorption Survey in H
i (FLASH), a wide field survey for 21-cm line absorption in neutral atomic hydrogen (H i) at …

Proximate molecular quasar absorbers (PH 2) are an intriguing population of absorption
systems that was recently uncovered through strong H 2 absorption at a small velocity …

We present details of the Automated Radio Telescope Imaging Pipeline (ARTIP) and the
results of a sensitive blind search for H i and OH absorbers at z< 0.4 and z< 0.7 …

We study the properties of long gamma-ray burst (GRB) host galaxies using a statistical
modelling framework derived to model damped Lyman-absorbers (DLAs) in quasar spectra …

We present a systematic study of deuterated molecular hydrogen (HD) at high redshift,
detected in absorption in the spectra of quasars. We present four new identifications of HD …

Abstract We report Hubble Space Telescope Cosmic Origins Spectrograph spectroscopy of
10 quasars with foreground star-forming galaxies at 0.02< z< 0.14 within impact parameters …

This work presents a new detection of H 2 absorption arising in a high-velocity cloud
associated with either the Milky Way or the Large Magellanic Cloud (LMC). The absorber …

We present the results of an analysis of the physical conditions (number density, intensity of
UV field, kinetic temperature) in the cold H2-bearing interstellar medium of local and high …