The cold interstellar medium (ISM) plays a central role in the galaxy evolution process. It is
the reservoir that fuels galaxy growth via star formation, the repository of material formed by …

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∼ …

Abstract The Widefield ASKAP L-band Legacy All-sky Blind surveY (wallaby) is a next-
generation survey of neutral hydrogen (H i) in the Local Universe. It uses the widefield, high …

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 …

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 framework for forecasting cosmological constraints from future neutral
hydrogen intensity map** experiments at low to intermediate redshifts. In the process, we …

We use the energy-balance code magphys to determine stellar and dust masses, and dust
corrected star formation rates for over 200 000 GAMA galaxies, 170 000 G10-COSMOS …

We present a new semi-analytic model that self-consistently traces the growth of
supermassive black holes (BH) and their host galaxies within the context of the Lambda cold …

Abstract The recently initiated Arecibo Legacy Fast ALFA (ALFALFA) survey aims to map∼
7000 deg 2 of the high Galactic latitude sky visible from Arecibo, providing a HI line spectral …