Showing 1–20 of 30 results
/ Date/ Name
Mar 23, 2012The effects of halo alignment and shape on the clustering of galaxiesMar 15, 2017A cross-correlation-based estimate of the galaxy luminosity functionDec 13, 2023The FLAMINGO project: Baryonic impact on weak gravitational lensing convergence peak countsMar 19, 2024The FLAMINGO project: the coupling between baryonic feedback and cosmology in light of the $S_8$ tensionNov 30, 2015The galaxy correlation function as a constraint on galaxy formation physicsOct 25, 2024FLAMINGO: combining kinetic SZ effect and galaxy-galaxy lensing measurements to gauge the impact of feedback on large-scale structureSep 4, 2025The resummation model in FLAMINGO: precisely predicting matter power suppression from observed halo baryon fractionsJun 6, 2023The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveysJan 23, 2015The contributions of matter inside and outside of haloes to the matter power spectrumSep 14, 2023The FLAMINGO project: revisiting the $S_8$ tension and the role of baryonic physicsOct 21, 2011The effects of alignment and ellipticity on the clustering of galaxiesOct 28, 2013The impact of baryonic processes on the two-point correlation functions of galaxies, subhaloes and matterAug 18, 2023Non-linear CMB lensing with neutrinos and baryons: FLAMINGO simulations vs. fast approximationsSep 12, 2023The contribution of massive haloes to the matter power spectrum in the presence of AGN feedbackApr 6, 2011The effects of galaxy formation on the matter power spectrum: A challenge for precision cosmologyJun 8, 2023FLAMINGO: Calibrating large cosmological hydrodynamical simulations with machine learningMay 5, 2011Quantifying the effect of baryon physics on weak lensing tomographyDec 13, 2023The FLAMINGO Project: Galaxy clusters in comparison to X-ray observationsOct 22, 2024The FLAMINGO project: Baryon effects on the matter power spectrumMay 22, 2023SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications