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 …

We present an analysis of the deepest Herschel images in four major extragalactic fields
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …

We present a new version of the galform semi-analytical model of galaxy formation. This
brings together several previous developments of galform into a single unified model …

Over the past two decades, an avalanche of new data from multiwavelength imaging and
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …

Aims. We present a 69 arcmin 2 ALMA survey at 1.1 mm, GOODS-ALMA, matching the
deepest HST-WFC3 H-band part of the GOODS-South field. Methods. We tapered the 0 ″24 …

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 …

Over the past decade, several works have used the ratio between total (rest 8− 1000 μm)
infrared and radio (rest 1.4 GHz) luminosity in star-forming galaxies (q IR), often referred to …