The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys
ABSTRACT We introduce the Virgo Consortium's FLAMINGO suite of hydrodynamical
simulations for cosmology and galaxy cluster physics. To ensure the simulations are …
simulations for cosmology and galaxy cluster physics. To ensure the simulations are …
FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning
To fully take advantage of the data provided by large-scale structure surveys, we need to
quantify the potential impact of baryonic effects, such as feedback from active galactic nuclei …
quantify the potential impact of baryonic effects, such as feedback from active galactic nuclei …
The FLAMINGO project: revisiting the S8 tension and the role of baryonic physics
ABSTRACT A number of recent studies have found evidence for a tension between
observations of large-scale structure (LSS) and the predictions of the standard model of …
observations of large-scale structure (LSS) and the predictions of the standard model of …
First Light And Reionization Epoch Simulations (FLARES)–I. Environmental dependence of high-redshift galaxy evolution
ABSTRACT We introduce the First Light And Reionisation Epoch Simulations (FLARES), a
suite of zoom simulations using the EAGLE model. We resimulate a range of overdensities …
suite of zoom simulations using the EAGLE model. We resimulate a range of overdensities …
First Light And Reionization Epoch Simulations (FLARES)--II: The photometric properties of high-redshift galaxies
We present the photometric properties of galaxies in the First Light And Reionization Epoch
Simulations (FLARES). The simulations trace the evolution of galaxies in a range of …
Simulations (FLARES). The simulations trace the evolution of galaxies in a range of …
Semi-analytic galaxies–I. Synthesis of environmental and star-forming regulation mechanisms
We present results from the semi-analytic model of galaxy formation sagapplied on the
MultiDark simulation MDPL2. sag features an updated supernova (SN) feedback scheme …
MultiDark simulation MDPL2. sag features an updated supernova (SN) feedback scheme …
Semi-analytic forecasts for JWST – II. Physical properties and scaling relations for galaxies at z = 4–10
ABSTRACT The long anticipated James Webb Space Telescope (JWST) will be able to
directly detect large samples of galaxies at very high redshift. Using the well-established …
directly detect large samples of galaxies at very high redshift. Using the well-established …
[HTML][HTML] Aerosol and physical atmosphere model parameters are both important sources of uncertainty in aerosol ERF
Changes in aerosols cause a change in net top-of-the-atmosphere (ToA) short-wave and
long-wave radiative fluxes; rapid adjustments in clouds, water vapour and temperature; and …
long-wave radiative fluxes; rapid adjustments in clouds, water vapour and temperature; and …
Exploring how eruption source parameters affect volcanic radiative forcing using statistical emulation
The radiative forcing caused by a volcanic eruption is dependent on several eruption source
parameters such as the mass of sulfur dioxide (SO2) emitted, the eruption column height …
parameters such as the mass of sulfur dioxide (SO2) emitted, the eruption column height …
MultiDark-Galaxies: data release and first results
We present the public release of the MultiDark-Galaxies: three distinct galaxy catalogues
derived from one of the Planck cosmology MultiDark simulations (ie mdpl2, with a volume of …
derived from one of the Planck cosmology MultiDark simulations (ie mdpl2, with a volume of …