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 …

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

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

The ALESS survey has followed up on a sample of 122 sub-millimeter sources in the
Extended Chandra Deep Field South at 870 μm with the Atacama Large Millimeter Array …

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 …

Our current knowledge of cosmic star-formation history during the first two billion years
(corresponding to redshift z> 3) is mainly based on galaxies identified in rest-frame …

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 …