We use the high-resolution TNG50 cosmological magnetohydrodynamical simulation to
explore the properties and origin of cold circumgalactic medium (CGM) gas around massive …

We present a study of the metal-enriched cool halo gas traced by Mg ii absorption around
228 galaxies at z∼ 0.8–1.5 within 28 quasar fields from the MUSE Analysis of Gas around …

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 …

We present a study of metal-enriched halo gas traced by Mg ii and C iv absorption at z< 2 in
the MUSE Analysis of Gas around Galaxies survey and the Quasar Sightline and Galaxy …

Observations indicate that a continuous supply of gas is needed to maintain observed star
formation rates in large, discy galaxies. To fuel star formation, gas must reach the inner …

We study the connection between Ly α emitters (LAEs) and metal-enriched ionized gas
traced by C iv absorption at redshift z≈ 3–4 in 28 quasar fields with high-resolution …

Using the exquisite data from the MUSE eXtremely Deep Field (MXDF), we report the
discovery of an Mg II emission nebula with an area above a 2σ significance level of 1000 …

We present initial results from the Cosmic Ultraviolet Baryon Survey (CUBS). CUBS is
designed to map diffuse baryonic structures at redshift z≲ 1 using absorption-line …

Absorbers in the spectrum of background objects probe the circumgalactic medium (CGM)
surrounding galaxies, but its physical properties remain unconstrained. We use the …

Ly α nebulae ubiquitously found around z> 2 quasars can supply unique constraints on the
properties of the circumgalactic medium, such as its density distribution, provided the quasar …