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 a multiwavelength analysis using the Submillimeter Array (SMA), James Clerk
Maxwell Telescope, NOEMA, JWST, the Hubble Space Telescope (HST), and the Spitzer …

CO line emission represents the most accessible and widely used tracer of the molecular
ISM. This renders the translation of observed CO intensity into total H2 gas mass critical to …

The ALESS survey has followed up on a sample of 122 sub-millimeter sources in the
Extended Chandra Deep Field South at 870 μm with the Atacama Large Millimeter Array …

Over the past decade, observations of the cool interstellar medium (ISM) in distant galaxies
via molecular and atomic fine structure line (FSL) emission have gone from a curious look …

We present PHIBSS, the IRAM Plateau de Bure high-z blue sequence CO 3–2 survey of the
molecular gas properties in massive, main-sequence star-forming galaxies (SFGs) near the …

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 …

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 …

Stars form within molecular clouds but our understanding of this fundamental process
remains hampered by the complexity of the physics that drives their evolution. We review our …