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 …

Abstract The Herschel Multi-tiered Extragalactic Survey (HerMES) is a legacy programme
designed to map a set of nested fields totalling∼ 380 deg2. Fields range in size from 0.01 …

We present the characteristics of 2 mm selected sources from the largest Atacama Large
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, the …

Using data from the mid-infrared to millimeter wavelengths for individual galaxies and for
stacked ensembles at 0.5< z< 2, we derive robust estimates of dust masses (M dust) for main …

Spectral energy distribution (SED) fitting in the far-infrared (FIR) is greatly limited by a dearth
of data and an excess of free parameters–from galaxies' dust composition, temperature …

Abstract The South Pole Telescope (SPT) has systematically identified 81 high-redshift,
strongly gravitationally lensed, dusty star-forming galaxies (DSFGs) in a 2500 square …

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) …

We present new ALMA Band 8 (rest-frame m) continuum observations of three massive ()
galaxies at z≈ 7 previously detected in [C ii] m and underlying dust continuum emission in …

The infrared (IR) spectral energy distributions (SEDs) of main-sequence galaxies in the early
Universe (z> 4) is currently unconstrained as IR continuum observations are time …