activity
20022026
most citedSimulating the joint evolution of quasars, galaxies and their large-scale distribution

5.1k citations · 21.2k across the 99 of their papers we have counts for

collaborators

100 papers

astro-ph.CO2026

Cosmological constraining power of the redshifts, heights, and angular clustering of weak gravitational lensing peaks

Jeger C. Broxterman, Matthieu Schaller, Ian G. McCarthy +8

Weak gravitational lensing (WL) peaks probe non-Gaussian information of the large-scale distribution of matter that is not captured by two-point lensing statistics. We study the co…

astro-ph.CO2026★ 2 cited

The FLAMINGO simulations data release

John C. Helly, Robert J. McGibbon, Joop Schaye +15

We describe the public release of petabytes of data from the FLAMINGO cosmological simulations. The suite consists of hydrodynamical simulations that include radiative cooli…

astro-ph.CO2026★ 1 cited

The FLAMINGO Project: Exploring the X-ray--cosmic-shear cross-correlation as a probe of large-scale structure

William McDonald, Joop Schaye, Konrad Kuijken +3

Baryonic feedback processes associated with galaxy formation directly influence the large-scale structure by redistributing gas. Recent measurements of the kinetic Sunyaev-Zel'dovi…

astro-ph.CO2025

Self-consistent secondary cosmic microwave background anisotropies and extragalactic foregrounds in the FLAMINGO simulations

Tianyi Yang, Ian G. McCarthy, Fiona McCarthy +6

Secondary anisotropies in the cosmic microwave background (CMB) contain information that can be used to test both cosmological models and models of galaxy formation. Starting from…

astro-ph.GA2025★ 1 cited

Ripples in the baryon to dark matter ratio in CDM: implications for galaxy formation

Owen Jessop, Adrian Jenkins, Andrew Pontzen +3

We use the FLAMINGO galaxy formation model to quantify the impact of baryon-CDM isocurvature perturbations on galaxy formation in CDM. In linear theory, these perturbations repr…

astro-ph.CO2025★ 2 cited

FLAMINGO: Tracing the co-evolution of hot gas and black holes in galaxy groups and clusters

Emily E. Costello, Ian G. McCarthy, Jaime Salcido +4

The gas mass fraction of galaxy groups and clusters is a key physical quantity for constraining the impact of feedback processes on large-scale structure. While several modern cosm…