Showing 1–20 of 23 results
/ Date/ Name
Jul 23, 2024Cosmic Web Dynamics: Forces and StrainsJun 5, 2024The FLAMINGO Project: A comparison of galaxy cluster samples selected on mass, X-ray luminosity, Compton-Y parameter, or galaxy richnessJun 8, 2023FLAMINGO: Calibrating large cosmological hydrodynamical simulations with machine learningAug 30, 2024The FLAMINGO Project: An assessment of the systematic errors in the predictions of models for galaxy cluster counts used to infer cosmological parametersSep 3, 2021The importance of black hole repositioning for galaxy formation simulationsDec 13, 2023The FLAMINGO project: Baryonic impact on weak gravitational lensing convergence peak countsJul 26, 2024Validating the clustering predictions of empirical models with the FLAMINGO simulationsMar 19, 2024The FLAMINGO project: the coupling between baryonic feedback and cosmology in light of the $S_8$ tensionOct 25, 2024FLAMINGO: combining kinetic SZ effect and galaxy-galaxy lensing measurements to gauge the impact of feedback on large-scale structureSep 4, 2025COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phaseJun 6, 2023The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveysMay 8, 2024Dark photon constraints from CMB temperature anisotropiesSep 14, 2023The FLAMINGO project: revisiting the $S_8$ tension and the role of baryonic physicsDec 8, 2023Inferring the dark matter splashback radius from cluster gas and observable profiles in the FLAMINGO simulationsFeb 10, 2025Assessing subhalo finders in cosmological hydrodynamical simulationsApr 27, 2026The FLAMINGO simulations data releaseAug 18, 2023Non-linear CMB lensing with neutrinos and baryons: FLAMINGO simulations vs. fast approximationsApr 12, 2024Relativistic SZ temperatures and hydrostatic mass bias for massive clusters in the FLAMINGO simulationsFeb 27, 2024The FLAMINGO simulation view of cluster progenitors observed in the epoch of reionization with JWSTSep 12, 2024Hydrostatic mass bias for galaxy groups and clusters in the FLAMINGO simulations