collaborators

6 papers

astro-ph.CO2024

The FLAMINGO project: the coupling between baryonic feedback and cosmology in light of the tension

Willem Elbers, Carlos S. Frenk, Adrian Jenkins +12

Large-scale structure surveys have reported measurements of the density of matter, , and the amplitude of clustering, , that are in tension with the values infer…

astro-ph.CO2023

The FLAMINGO project: Baryonic impact on weak gravitational lensing convergence peak counts

Jeger C. Broxterman, Matthieu Schaller, Joop Schaye +12

Weak gravitational lensing convergence peaks, the local maxima in weak lensing convergence maps, have been shown to contain valuable cosmological information complementary to commo…

astro-ph.GA2023

The FLAMINGO Project: Galaxy clusters in comparison to X-ray observations

Joey Braspenning, Joop Schaye, Matthieu Schaller +10

Galaxy clusters are important probes for both cosmology and galaxy formation physics. We test the cosmological, hydrodynamical FLAMINGO simulations by comparing to observations of…

astro-ph.CO2023

Inferring the dark matter splashback radius from cluster gas and observable profiles in the FLAMINGO simulations

Imogen Towler, Scott T. Kay, Joop Schaye +10

The splashback radius, coinciding with the minimum in the dark matter radial density gradient, is thought to be a universal definition of the edge of a dark matter halo. Observatio…

astro-ph.CO2023

Revisiting the effects of baryon physics on small-scale redshift space distortions

Juliana Kwan, Ian G. McCarthy, Jaime Salcido

Redshift space distortions are an important probe of the growth of large-scale structure and for constraining cosmological parameters in general. As galaxy redshift surveys approac…

astro-ph.CO2023

Cosmic-Enu: An emulator for the non-linear neutrino power spectrum

Amol Upadhye, Juliana Kwan, Ian G. McCarthy +4

Cosmology is poised to measure the neutrino mass sum and has identified several smaller-scale observables sensitive to neutrinos, necessitating accurate predictions of neutri…