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 analyse the physical properties of a large, homogeneously selected sample of ALMA-
located sub-millimetre galaxies (SMGs). This survey, AS2UDS, identified 707 SMGs across …

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 …

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

We present a self-consistent cross-calibration of the three main molecular gas mass tracers
in galaxies, namely the 12CO (1–0),[C i](3 P 1–3 P 0) lines, and the submm dust continuum …

We present the results from a survey of 12CO emission in 40 luminous sub-millimetre
galaxies (SMGs), with 850-μm fluxes of S 850 μm= 4–20 mJy, conducted with the Plateau de …

We present the first photometric redshift distribution for a large sample of 870 μm
submillimeter galaxies (SMGs) with robust identifications based on observations with ALMA …

We investigate the CO excitation of normal (near-IR selected BzK) star-forming (SF) disk
galaxies at z= 1.5 using IRAM Plateau de Bure observations of the CO [2–1], CO [3–2], and …