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

The first observations of the James Webb Space Telescope (JWST) have revolutionized our
understanding of the Universe by identifying galaxies at redshift z≈ 13 (refs.,–). In addition …

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 …

Over the past decades, rest-frame ultraviolet (UV) observations have provided large
samples of UV luminous galaxies at redshift (z) greater than 6 (refs.,–), during the so-called …

Abstract The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA
Large Program (LP) that is identifying and performing a first characterization of many of the …

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 …

ABSTRACT ALMA observations have revealed the presence of dust in the first generations
of galaxies in the Universe. However, the dust temperature T d remains mostly …

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 …

We report 18 dust continuum detections (≥ 3.3 σ) at∼ 88 and 158 out of 49 ultraviolet (UV)-
bright galaxies (M UV<− 21.3 mag) at> 6.5, observed by the Cycle-7 Atacama Large …

We analyse FIR dust continuum measurements for 14 galaxies (redshift z≈ 7) in the ALMA
Reionization Era Bright Emission Line Survey (REBELS) Large Program to derive their …