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 utilised the unprecedented depth and resolution of recent early-release science (ERS)
JWST observations to define the near-infrared counterparts of sub-millimetre galaxies …

We analyse a robust sample of 30 near-infrared-faint (K AB> 25.3, 5σ) submillimetre
galaxies (SMGs) selected from a 0.96 deg2 field to investigate their properties and the cause …

Matching the number counts of high-z submillimetre-selected galaxies (SMGs) has been a
long-standing problem for galaxy formation models. In this paper, we use 3D dust radiative …

The dust-to-stellar mass ratio (M dust/M⋆) is a crucial, albeit poorly constrained, parameter
for improving our understanding of the complex physical processes involved in the …

We present an ALMA study of the∼ 180 brightest sources in the SCUBA-2 850-μ m map of
the COSMOS field from the S2COSMOS survey, as a pilot study for AS2COSMOS–a full …

Abstract The James Webb Space Telescope Time-Domain Field (JWST-TDF) is an∼
14'diameter field near the North Ecliptic Pole that will be targeted by one of the JWST …

Submillimetre galaxies represent a rapid growth phase of both star formation and massive
galaxies. Mapping SMGs in galaxy protoclusters provides key insights into where and how …

We introduce an ALMA band 3 spectroscopic survey targeting the brightest submillimeter
galaxies (SMGs) in the COSMOS field. Here we present the first results based on the 18 …

We analyse the physical properties of 121 SNR≥ 5 sub-millimetre galaxies (SMGs) from the
STUDIES 450 μ m survey. We model their UV-to-radio spectral energy distributions using …