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 …

A cosmologically significant population of very luminous high-redshift galaxies has recently
been discovered at submillimeter (submm) wavelengths. Advances in submm detector …

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 …

We present a catalogue of∼ 3,000 submillimetre sources detected (≥ 3.5 σ) at 850μm
over∼ 5 deg2 surveyed as part of the James Clerk Maxwell Telescope (JCMT) SCUBA-2 …

We present far-infrared (FIR) photometry at 150 and 205 μ m of eight low-redshift starburst
galaxies obtained with the Infrared Space Observatory (ISO) ISOPHOT. Five of the eight …

Abstract We exploit Atacama Large Millimeter Array (ALMA) 870 μm observations of sub-
millimetre sources in the Extended Chandra Deep Field South to investigate the far-infrared …

We present a theoretical framework in which bound stellar clusters arise naturally at the high-
density end of the hierarchy of the interstellar medium (ISM). Due to short free-fall times …

We have obtained spectroscopic redshifts using the Keck I telescope for a sample of 73
submillimeter galaxies (SMGs), with a median 850 μm flux density of 5.7 mJy, for which …

The presence of dust in galaxies removes one‐half or more of the stellar energy from the UV‐
optical budget of the universe and has a profound impact on our understanding of how …