Line-intensity mapping (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 rest-frame optical data of the compact z= 5.55 galaxy GS_3073 obtained using
the integral field spectroscopy mode of the Near-InfraRed Spectrograph on board the James …

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 …

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 present new stellar mass functions at z∼ 6, z∼ 7, z∼ 8, z∼ 9 and, for the first time, z∼
10, constructed from∼ 800 Lyman-break galaxies previously identified over the eXtreme …

We present specific star formation rates (sSFRs) for 40 ultraviolet (UV)-bright galaxies at z∼
7–8 observed as part of the Reionization Era Bright Emission Line Survey (REBELS) …

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 …

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) …

The ALMA-ALPINE [CII] survey is aimed at characterizing the properties of a sample of
normal star-forming galaxies (SFGs). The ALMA Large Program to INvestigate (ALPINE) …