12 citations · 23 across the 8 of their papers we have counts for
9 papers
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…
The morphologies of present-day galaxies in the COLIBRE simulations
Victor J. Forouhar Moreno, Joop Schaye, Matthieu Schaller +9
The diversity of galaxy morphologies and their relations with galaxy and halo properties is fundamental to understanding galaxy formation. Cosmological simulations of representativ…
The evolution of the sizes and angular momentum content of galaxies in the COLIBRE simulations
Aaron D. Ludlow, Katy L. Proctor, Joop Schaye +12
We analyse the sizes and specific angular momentum content of galaxies in the Colibre cosmological hydrodynamical simulations spanning two orders of magnitude in mass resolution. W…
Cosmological Zoom-In Simulations of Milky Way Host Mass Dark Matter Halos with a Blue-Tilted Primordial Power Spectrum
Jianhao Wu, Tsang Keung Chan, Victor J. Forouhar Moreno
Recent observations from the James Webb Space Telescope revealed a surprisingly large number of galaxies at high redshift, challenging the standard Lambda Cold Dark Matter cosmolog…
The FLAMINGO Project: An assessment of the systematic errors in the predictions of models for galaxy cluster counts used to infer cosmological parameters
Roi Kugel, Joop Schaye, Matthieu Schaller +2
Galaxy cluster counts have historically been important for the measurement of cosmological parameters and upcoming surveys will greatly reduce the statistical errors. To exploit th…
The accreted stellar haloes of Milky Way-mass galaxies as a probe of the nature of the dark matter
Victor J. Forouhar Moreno, Azadeh Fattahi, Alis J. Deason +2
Galactic stellar haloes are largely composed of the remnants of galaxies accreted during the assembly of their host galaxies, and hence their properties reflect the mass spectrum a…
The FLAMINGO Project: A comparison of galaxy cluster samples selected on mass, X-ray luminosity, Compton-Y parameter, or galaxy richness
Roi Kugel, Joop Schaye, Matthieu Schaller +5
Galaxy clusters provide an avenue to expand our knowledge of cosmology and galaxy evolution. Because it is difficult to accurately measure the total mass of a large number of indiv…
Galactic satellite systems in CDM, WDM and SIDM
Victor J. Forouhar Moreno, Alejandro Benitez-Llambay, Shaun Cole +1
We investigate the population of bright satellites () of haloes of mass comparable to that of the Milky Way in cosmological simulations in whi…
Baryon-driven decontraction in Milky Way mass haloes
Victor J. Forouhar Moreno, Alejandro Benítez-Llambay, Shaun Cole +1
We select a sample of Milky Way (MW) mass haloes from a high-resolution version of the EAGLE simulation to study their inner dark matter (DM) content and how baryons alter it. As i…