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 …

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 …

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

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 the results of the first, deep Atacama Large Millimeter Array (ALMA) imaging
covering the full≃ 4.5 arcmin2 of the Hubble Ultra Deep Field (HUDF) imaged with Wide …

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 …

Star-forming galaxies (SFGs) display a continuous specific star formation rate (sSFR)
distribution, which can be approximated by two log-normal functions: one encompassing the …

We make use of deep 1.2 mm continuum observations (12.7 μJy beam− 1 rms) of a 1 arcmin
2 region in the Hubble Ultra Deep Field to probe dust-enshrouded star formation from 330 …

Dusty star-forming galaxies at high redshift (1< z< 3) represent the most intense star-forming
regions in the universe. Key aspects to these processes are the gas heating and cooling …

Dust temperature is an important property of the interstellar medium (ISM) of galaxies. It is
required when converting (sub) millimetre broad-band flux to total infrared luminosity (L IR) …