The FLAMINGO simulations data release
arXiv:2604.24324 · doi:10.1016/j.ascom.2026.101159
Abstract
We describe the public release of petabytes of data from the FLAMINGO cosmological simulations. The suite consists of hydrodynamical simulations that include radiative cooling, star formation, stellar mass loss and the resulting chemical enrichment, supernova feedback, and two implementations of AGN feedback. Neutrinos are simulated explicitly using particles. Data products include snapshots, halo and galaxy catalogues, HEALPix all-sky lightcone maps, particle data for lightcone maps, and power spectra. The FLAMINGO set includes 22 hydrodynamical simulations. In addition, there are 16 gravity-only simulations, including the particles FLAMINGO-10k run, with initial conditions that match those of the corresponding hydrodynamical runs. The fiducial hydrodynamical simulations span three numerical resolutions that have each been calibrated to reproduce the present-day galaxy stellar mass function and gas fractions in low-redshift clusters. Other simulations systematically vary the galaxy stellar mass function, cluster gas fractions, cosmology (including neutrino masses), and/or the nature of dark matter, in volumes of 1Gpc. The release includes hitherto unpublished simulations that use extra dark matter particles. While we provide a facility for downloading complete simulation outputs, we recognise that for many users this will not be possible due to limited local storage or network bandwidth. We implement a web service that enables users to explore available outputs and selectively download datasets or parts of datasets.
19 pages. Accepted for publication in Astronomy and Computing with minor revisions. For access to the FLAMINGO data see https://flamingo.strw.leidenuniv.nl/
References in corpus (55)
- HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
- Simulating the joint evolution of quasars, galaxies and their large-scale distribution
- The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
- First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
- The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
- Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- Simba: Cosmological Simulations with Black Hole Growth and Feedback
- First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback
- Dancing in the dark: galactic properties trace spin swings along the cosmic web
- The eROSITA X-ray telescope on SRG
- Cosmological simulations of the growth of supermassive black holes and feedback from active galactic nuclei: method and tests
- Black holes in galaxy mergers: The formation of red elliptical galaxies
- Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
- On the relation between the Schmidt and Kennicutt-Schmidt star formation laws and its implications for numerical simulations
- Simulating galactic outflows with thermal supernova feedback
- The Illustris Simulation: Public Data Release
- The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology
- The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues
- An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models
- Towards a realistic population of simulated galaxy groups and clusters
- Quantifying the effect of baryon physics on weak lensing tomography
- The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys
- Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions
- A new method to quantify the effects of baryons on the matter power spectrum
- The MillenniumTNG Project: The hydrodynamical full physics simulation and a first look at its galaxy clusters
- Public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation
- Effect of baryonic feedback on two- and three-point shear statistics: prospects for detection and improved modelling
- HBT+: an improved code for finding subhalos and building merger trees in cosmological simulations
- A fast and accurate method for computing the Sunyaev-Zeldovich signal of hot galaxy clusters
- KiDS-Legacy: Cosmological constraints from cosmic shear with the complete Kilo-Degree Survey
- FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
- Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields
- SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
- Energy equipartition between stellar and dark matter particles in cosmological simulations results in spurious growth of galaxy sizes
- Consistent lensing and clustering in a low- Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000
- Sphenix: Smoothed Particle Hydrodynamics for the next generation of galaxy formation simulations
- The impact of the observed baryon distribution in haloes on the total matter power spectrum
- Millimeter-wave Point Sources from the 2500-square-degree SPT-SZ Survey: Catalog and Population Statistics
- Sunyaev-Zeldovich signal processing and temperature-velocity moment method for individual clusters
- Spurious heating of stellar motions in simulated galactic disks by dark matter halo particles
- An optimal nonlinear method for simulating relic neutrinos
- The CAMELS project: public data release
- Higher-order initial conditions for mixed baryon-CDM simulations
- The importance of black hole repositioning for galaxy formation simulations
- Spin-driven jet feedback in idealised simulations of galaxy groups and clusters
- Large-scale Maps of the Cosmic Infrared Background from Planck
- Cosmic evolution of low-excitation radio galaxies in the LOFAR Two-meter Sky Survey Deep Fields
- A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
- Performance Characteristics of TreePM codes
- Higher-order initial conditions with massive neutrinos
- A unified model for the clustering of quasars and galaxies at
- The FLAMINGO project: Baryon effects on the matter power spectrum
- SOAP: A Python Package for Calculating the Properties of Galaxies and Halos Formed in Cosmological Simulations
- The FLAMINGO project: Baryonic impact on weak gravitational lensing convergence peak counts
- Average X-ray properties of galaxy groups. From Milky Way-like halos to massive clusters