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 …

We review open questions and prospects for progress in ultrahigh-energy cosmic ray
(UHECR) research, based on a series of discussions that took place during the “The High …

The new capabilities that JWST offers in the near-and mid-infrared (IR) are used to
investigate in unprecedented detail the nature of optical/near-IR-faint, mid-IR-bright sources …

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 …

Cosmic dust is an essential component sha** 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 …

Aims. We present the detailed characterisation of a sample of 56 sources serendipitously
detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early …

We analyse the physical properties of a large, homogeneously selected sample of ALMA-
located sub-millimetre galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across …

We present the first results from the Map** Obscuration to Reionization with ALMA
(MORA) survey, the largest Atacama Large Millimeter/submillimeter Array (ALMA) blank-field …

Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …