Understanding the properties of dust attenuation curves in galaxies and the physical
mechanisms that shape them are among the fundamental questions of extragalactic …

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 the thesan project, a suite of large volume () radiation-magnetohydrodynamic
simulations that simultaneously model the large-scale statistical properties of the …

We present a detailed stellar population analysis of 11 bright (H< 26.6) galaxies at z= 9–11
(three spectroscopically confirmed) to constrain the chemical enrichment and growth of …

We include a fully coupled treatment of metal and dust enrichment into the Delphi semi-
analytic model of galaxy formation to explain the dust content of 13 Lyman break galaxies …

Cosmic dust is an essential component shaping both the evolution of galaxies and their
observational signatures. How quickly dust builds up in the early Universe remains an open …

Recent observations with the JWST are yielding tantalizing hints of an early population of
massive, bright galaxies at z> 10, with Atacama Large Millimeter/submillimeter Array (ALMA) …

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 …

ABSTRACT JWST is set to transform many areas of astronomy, one of the most exciting is
the expansion of the redshift frontier to z> 10. In its first year, alone JWST should discover …

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 …