506 citations · 7.4k across the 162 of their papers we have counts for
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The Evolution of the Baryons Associated with Galaxies Averaged over Cosmic Time and Space
Fabian Walter, Chris Carilli, Marcel Neeleman +30
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 s…
The physical drivers of the atomic hydrogen-halo mass relation
Garima Chauhan, Claudia del P. Lagos, Adam R. H. Stevens +3
We use SHARK, a semi-analytic galaxy formation model, to investigate the physical processes involved in dictating the shape, scatter and evolution of the HI-halo mass relation at $…
Physical properties and evolution of (Sub-)millimeter selected galaxies in the galaxy formation simulation Shark
Claudia del P. Lagos, Elisabete da Cunha, Aaron S. G. Robotham +5
We thoroughly explore the properties of (sub)-millimeter (mm) selected galaxies (SMGs) in the Shark semi-analytic model of galaxy formation. Compared to observations, the predicted…
The influence of angular momentum and environment on the HI gas of late-type galaxies
Chandrashekar Murugeshan, Virginia Kilborn, Thomas Jarrett +5
We use high-resolution HI data from the WHISP survey to study the HI and angular momentum properties of a sample of 114 late-type galaxies. We explore the specific baryonic angular…
Constraining the growth rate of structure with phase correlations
Joyce Byun, Felipe Oliveira Franco, Cullan Howlett +2
We show that correlations between the phases of the galaxy density field in redshift space provide additional information about the growth rate of large-scale structure that is com…
Stellar angular momentum distribution linked to galaxy morphology
Sarah M. Sweet, Karl Glazebrook, Danail Obreschkow +4
We study the spatially-resolved stellar specific angular momentum in a high-quality sample of 24 CALIFA galaxies covering a broad range of visual morphology, accounting for s…