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

The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …

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 …

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 …

We introduce serra, a suite of zoom-in high-resolution (, at z= 7.7) cosmological simulations
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …

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 …

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 make use of sensitive (9.3 μJy beam− 1 rms) 1.2 mm continuum observations from the
Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble …

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 …

ABSTRACT We present new [] 88-observations of five bright z∼ 7 Lyman-break galaxies
spectroscopically confirmed by ALMA through [] 158, unlike recent [] detections where …