Line-intensity map** (LIM) is an emerging approach to survey the Universe, using
relatively low-aperture instruments to scan large portions of the sky and collect the total …

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 present the JWST cycle 1 53.8 h medium program FRESCO, short for 'First Reionization
Epoch Spectroscopically Complete Observations'. FRESCO covers 62 arcmin2 in each 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 …

Lyman-break galaxy (LBG) candidates at z≳ 10 are rapidly being identified in James Webb
Space Telescope (JWST)/NIRCam observations. Due to the (redshifted) break produced by …

The protagonists of the last great phase transition of the universe—cosmic reionization—
remain elusive. Faint star-forming galaxies are leading candidates because they are found …

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 …

Over the last few years, both Atacama Large Millimeter/submillimeter Array (ALMA) and
Spitzer observations have revealed a population of likely massive galaxies at z> 3 that was …

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 present a search for extremely red, dust-obscured, z> 7 galaxies with JWST/NIRCam+
MIRI imaging over the first 20 arcmin 2 of publicly available Cycle 1 data from the COSMOS …