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 …

Characterizing the relationship between stars, gas, and metals in galaxies is a critical
component of understanding the cosmic baryon cycle. We compile contemporary censuses …

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 present the MUSE Hubble Ultra Deep Survey, a mosaic of nine MUSE fields covering
90% of the entire HUDF region with a 10-h deep exposure time, plus a deeper 31-h …

Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift - IOPscience
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We combine the recent determination of the evolution of the cosmic density of molecular gas
(H 2) using deep, volumetric surveys, with previous estimates of the cosmic density of stellar …

We present a new, open source, free, semi-analytic model (SAM) of galaxy formation, Shark,
designed to be highly flexible and modular, allowing easy exploration of different physical …

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 introduce a suite of cosmological volume simulations to study the evolution of galaxies
as part of the Feedback in Realistic Environments project. FIREbox, the principal simulation …

We investigate the CO excitation and interstellar medium (ISM) conditions in a cold gas
mass-selected sample of 22 star-forming galaxies at z= 0.46–3.60, observed as part of the …