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 …

Neutral-atomic and molecular outflows are a common occurrence in galaxies, near and far.
They operate over the full extent of their galaxy hosts, from the innermost regions of galactic …

This article gives an overview of the constitution, physical conditions, and observables of
dust in the interstellar medium of nearby galaxies. We first review the macroscopic, spatial …

Observations of evolution in the dust-to-metal ratio allow us to constrain the dominant dust
processing mechanisms. In this work, we present a study of the dust-to-metal and dust-to …

We present a joint analysis of the galaxy S04590 at z= 8.496 based on NIRSpec, NIRCam,
and NIRISS observations obtained as part of the Early Release Observations program of the …

We present predictions for the evolution of the galaxy dust-to-gas ratio (DGR) and dust-to-
metal ratio (DTM) from z= 0→ 6, using a model for the production, growth, and destruction of …

We study the dust content of galaxies from z= 0 to z= 9 in semi-analytic models of galaxy
formation that include new recipes to track the production and destruction of dust. We …

Line intensity mapping (LIM) is rapidly emerging as a powerful technique to study galaxy
formation and cosmology in the high-redshift Universe. We present LIM estimates of select …

Dust temperature is an important property of the interstellar medium (ISM) of galaxies. It is
required when converting (sub) millimetre broad-band flux to total infrared luminosity (L IR) …

We present a systematic investigation of the circumgalactic medium (CGM) within projected
distances d< 160 kpc of luminous red galaxies (LRGs). The sample comprises 16 …