The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues

Abstract

We present the public data release of halo and galaxy catalogues extracted from the EAGLE suite of cosmological hydrodynamical simulations of galaxy formation. These simulations were performed with an enhanced version of the GADGET code that includes a modified hydrodynamics solver, time-step limiter and subgrid treatments of baryonic physics, such as stellar mass loss, element-by-element radiative cooling, star formation and feedback from star formation and black hole accretion. The simulation suite includes runs performed in volumes ranging from 25 to 100 comoving megaparsecs per side, with numerical resolution chosen to marginally resolve the Jeans mass of the gas at the star formation threshold. The free parameters of the subgrid models for feedback are calibrated to the redshift z=0 galaxy stellar mass function, galaxy sizes and black hole mass - stellar mass relation. The simulations have been shown to match a wide range of observations for present-day and higher-redshift galaxies. The raw particle data have been used to link galaxies across redshifts by creating merger trees. The indexing of the tree produces a simple way to connect a galaxy at one redshift to its progenitors at higher redshift and to identify its descendants at lower redshift. In this paper we present a relational database which we are making available for general use. A large number of properties of haloes and galaxies and their merger trees are stored in the database, including stellar masses, star formation rates, metallicities, photometric measurements and mock gri images. Complex queries can be created to explore the evolution of more than 10^5 galaxies, examples of which are provided in appendix. (abridged)

12 pages, 3 figures + appendices. The simulation data is available at http://www.eaglesim.org/database.php (comments welcome). Paper accepted to AstronomyComputing. Note there is a typo in the published version, Section 4.1, replace 3/2 with 2/3 for velocity dispersion

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• RUBIES spectroscopically confirms the high number density of quiescent galaxies from $2<\mathbf{z}<5$
• The physical origin of positive metallicity radial gradients in high-redshift galaxies: insights from the FIRE-2 cosmological hydrodynamic simulations
• A search for the missing baryons with X--ray absorption lines towards the blazar 1ES 1553+113
• A deep learning approach to halo merger tree construction
• A sparse regression approach to modeling the relation between galaxy stellar masses and their host halos
• On the application of dimensionality reduction and clustering algorithms for the classification of kinematic morphologies of galaxies
• A Fast and Accurate Analytic Method of Calculating Galaxy Two-point Correlation Functions
• Star formation concentration as a tracer of environmental quenching in action: a study of the Eagle and C-Eagle simulations
• Gamma rays from dark matter spikes in EAGLE simulations
• Modelling the mass accretion histories of dark matter haloes using a Gamma formalism
• The relationship between cluster environment and molecular gas content of star-forming galaxies in the EAGLE simulation
• On the variation in stellar $\alpha$-enhancements of star-forming galaxies in the EAGLE simulation
• Global Preventive Feedback of Powerful Radio Jets on Galaxy Formation
• Galaxy interactions in filaments and sheets: insights from EAGLE simulations
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• A comprehensive study on the relation between the metal enrichment of ionised and atomic gas in star-forming galaxies
• The case for two-dimensional galaxy-galaxy lensing
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
• Cross-correlation between soft X-rays and galaxies A new benchmark for galaxy evolution models
• The BACCO Simulation Project: A baryonification emulator with Neural Networks
• HST Hα grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation
• The luminosity of cluster galaxies in the Cluster-EAGLE simulations
• The formation and disruption of globular cluster populations in simulations of present-day $L^{\ast }$ galaxies with controlled assembly histories
• CEMPlifying reionization
• The H$\alpha$ luminosity and stellar mass dependent clustering of star-forming galaxies at $0.7<z<1.5$ with 3D-HST
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• Star formation and stellar & AGN feedback in the absence of accretion, not gas stripping, set the quenching timescale in satellite galaxies
• Robust machine learning model of inferring the ex-situ stellar fraction of galaxies from photometric data
• Andromeda's asymmetric satellite system as a challenge to cold dark matter cosmology
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Detection of an orthogonal alignment between parsec scale AGN jets and their host galaxies
• Unveiling galaxy pair alignment in cosmic filaments: A 3D exploration using EAGLE simulation
• Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
• A correlation between accreted stellar kinematics and dark matter halo spin in the ARTEMIS simulations
• Fast radio bursts as probes of feedback from active galactic nuclei
• Detection of the Intrinsic Spin Alignments in Isolated Spiral Pairs
• The average structural evolution of massive galaxies can be reliably estimated using cumulative galaxy number densities
• The contribution of supermassive black holes in stripped nuclei to the supermassive black hole population of UCDs and galaxy clusters
• Diving into dangerous tides: The impact of galaxy cluster tidal environments on satellite galaxy mass densities
• The roles of environment and interactions on the evolution of red and blue galaxies in the EAGLE simulation
• Stellar-gas kinematic misalignments in EAGLE: lifetimes and longevity of misaligned galaxies
• A new strategy for matching observed and simulated lensing galaxies
• MEGS: Morphological Evaluation of Galactic Structure
• The weak connection between the stellar haloes and merger histories of Milky Way-mass galaxies
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Hidden Figures in the Sky: Evolution of low-surface brightness galaxies from a hydro-dynamical perspective
• Stellar initial mass function variation in massive early-type galaxies: the potential role of the deuterium abundance
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation
• A New View of Observed Galaxies through 3D Modelling and Visualisation
• Unsupervised Domain Adaptation for Constraining Star Formation Histories
• A sparse regression approach for populating dark matter halos and subhalos with galaxies
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• No dependence of radio properties of brightest group galaxies on the luminosity gap
• Exploring the Angular Momentum -- Atomic Gas Content Connection with EAGLE and IllustrisTNG
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• Simultaneously Modelling Dusty Star Forming Galaxies and Massive Quiescents: A Calibration Framework for Galaxy Formation Models
• The FLAMINGO simulations data release
• Dynamics of Companion Galaxies of Early-Type Galaxies
• Exploring the outskirts of the EAGLE disc galaxies
• Study of dependence of ram pressure stripping on the orbital parameters of the galaxies
• The long road to the Green Valley: Tracing the evolution of the Green Valley galaxies in the EAGLE simulation
• Beyond mirkwood: Enhancing SED Modeling with Conformal Predictions
• Velocity dispersion functions of pressure-supported galaxies in EAGLE simulations with varying active galactic nucleus feedback
• Emergence of red, star-forming galaxies (red misfits) in a ΛCDM universe
• Gamma Analytical Modeling Evolution (GAME) I: The physical implications of deriving the stellar mass functions from z=0 to z=8
• Reduced Gas Accretion onto Galaxies due to Effects of External Giant Radio Lobes
• On the signature of black holes on the quenched stellar mass function
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• Quenching of satellite galaxies of Milky Way analogues: reconciling theory and observations
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• The Scaling Relation between Galaxy Luminosity and WHIM Density from EAGLE Simulations with application to SDSS data
• Predictions for the X-ray circumgalactic medium of edge-on discs and spheroids
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• Exploring the halo occupation distribution for moderate X-ray luminosity active galactic nuclei in the EAGLE cosmological simulation
• Estimating Transient Rates from Cosmological Simulations and BPASS
• SDSS-IV MaNGA: Exploring the local scaling relations for N/O
• Using the EAGLE simulations to elucidate the origin of disc surface brightness profile breaks as a function of mass and environment
• Aligned and misaligned metallicity gradients in young stars and star-forming regions in the EAGLE discs
• Detection of HI filament: Pair Stacking vs. Filament Stacking
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• Shape, alignment, and mass distribution of baryonic and dark-matter halos in one EAGLE simulation
• Galaxy mergers can initiate quenching by unlocking an AGN-driven transformation of the baryon cycle
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• Modelling the host galaxies of binary compact object mergers with observational scaling relations