Over the past decade, increasingly robust estimates of the dense molecular gas content in
galaxy populations between redshift z= 0 and the peak of cosmic galaxy/star formation (z∼ …

Ever deeper and wider look-back surveys have led to a fairly robust outline of the cosmic
star-formation history, which culminated around; this period is often nicknamed “cosmic …

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 …

Aims. We present the detailed characterisation of a sample of 56 sources serendipitously
detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early …

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 …

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

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 …

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 …

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 …

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 …