activity
20022023
most citedThe Inner Structure of LambdaCDM Halos III: Universality and Asymptotic Slopes

1.1k citations · 8k across the 130 of their papers we have counts for

collaborators

131 papers

astro-ph.GA2023

SimSpin v2.6.0 -- Constructing synthetic spectral IFU cubes for comparison with observational surveys

K. E. Harborne, A. Serene, E. J. A. Davies +10

In this work, we present a methodology and a corresponding code-base for constructing mock integral field spectrograph (IFS) observations of simulated galaxies in a consistent and…

astro-ph.GA2022★ 5 cited

SAMI-HI: the connection between global asymmetry in the ionised and neutral atomic hydrogen gas in galaxies

Adam B. Watts, Luca Cortese, Barbara Catinella +7

Observations of the neutral atomic hydrogen (HI) gas in galaxies are predominantly spatially unresolved, in the form of a global HI spectral line. There has been substantial work o…

astro-ph.HE2022★ 6 cited

CosmoDRAGoN simulations -- I. Dynamics and observable signatures of radio jets in cosmological environments

Patrick M. Yates-Jones, Stanislav S. Shabala, Chris Power +4

We present the Cosmological Double Radio Active Galactic Nuclei (CosmoDRAGoN) project: a large suite of simulated AGN jets in cosmological environments. These environments sample t…

astro-ph.CO2022★ 10 cited

Thermal and Reionisation History within a Large-Volume Semi-Analytic Galaxy Formation Simulation

Sreedhar Balu, Bradley Greig, Yisheng Qiu +4

We predict the 21-cm global signal and power spectra during the Epoch of Reionisation using the MERAXES semi-analytic galaxy formation and reionisation model, updated to include X-…

astro-ph.GA2022★ 7 cited

A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations

Yang Wang, Nicola R. Napolitano, Weiguang Cui +7

The star formation history (SFH) of galaxies is critical for understanding galaxy evolution. Hydrodynamical simulations enable us to precisely reconstruct the SFH of galaxies and e…

astro-ph.GA2022★ 4 cited

Spin transfer from dark matter to gas during halo formation

Jie Li, Danail Obreschkow, Chris Power +1

In the protogalactic density field, diffuse gas and collision-less cold dark matter (DM) are often assumed sufficiently mixed that both components experience identical tidal torque…