The IllustrisTNG Simulations: Public Data Release
arXiv:1812.05609
Abstract
We present the full public release of all data from the TNG50, TNG100 and TNG300 simulations of the IllustrisTNG project. IllustrisTNG is a suite of large volume, cosmological, gravo-magnetohydrodynamical simulations run with the moving-mesh code Arepo. TNG includes a comprehensive model for galaxy formation physics, and each TNG simulation self-consistently solves for the coupled evolution of dark matter, cosmic gas, luminous stars, and supermassive blackholes from early time to the present day, z=0. Each of the flagship runs -- TNG50, TNG100, and TNG300 -- are accompanied by lower-resolution and dark-matter only counterparts, and we discuss scientific and numerical cautions and caveats relevant when using TNG. Full volume snapshots are available at 100 redshifts; halo and subhalo catalogs at each snapshot and merger trees are also released. The data volume now directly accessible online is ~1.1 PB, including 2,000 full volume snapshots and ~110,000 high time-resolution subbox snapshots. Data access and analysis examples are available in IDL, Python, and Matlab. We describe improvements and new functionality in the web-based API, including on-demand visualization and analysis of galaxies and halos, exploratory plotting of scaling relations and other relationships between galactic and halo properties, and a new JupyterLab interface. This provides an online, browser-based, near-native data analysis platform which supports user computation with fully local access to TNG data, alleviating the need to download large simulated datasets.
arXiv commentTNG50 joins TNG100 and TNG300 in public release (1 Feb 2021) at http://www.tng-project.org/data
References in corpus (85)
- The Sloan Digital Sky Survey: Technical Summary
- 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
- E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
- Cosmological SPH simulations: A hybrid multi-phase model for star formation
- Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
- Modeling feedback from stars and black holes in galaxy mergers
- CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
- Simulating Galaxy Formation with the IllustrisTNG Model
- The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
- First results from the IllustrisTNG simulations: matter and galaxy clustering
- First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
- First results from the IllustrisTNG simulations: the galaxy color bimodality
- The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
- Properties of galaxies reproduced by a hydrodynamic simulation
- First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and europium
- Simulating galaxy formation with black hole driven thermal and kinetic feedback
- CALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation
- From dwarf spheroidals to cDs: Simulating the galaxy population in a LCDM cosmology
- FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation
- Simba: Cosmological Simulations with Black Hole Growth and Feedback
- First results from the IllustrisTNG simulations: radio haloes and magnetic fields
- Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
- A model for cosmological simulations of galaxy formation physics
- Halos and galaxies in the standard cosmological model: results from the Bolshoi simulation
- First Results from the TNG50 Simulation: The evolution of stellar and gaseous disks across cosmic time
- Dancing in the dark: galactic properties trace spin swings along the cosmic web
- The merger rate of galaxies in the Illustris Simulation: a comparison with observations and semi-empirical models
- A New Calculation of the Ionizing Background Spectrum and the Effects of HeII Reionization
- 3D-HST: A wide-field grism spectroscopic survey with the Hubble Space Telescope
- The Illustris simulation: the evolving population of black holes across cosmic time
- Gravitationally Consistent Halo Catalogs and Merger Trees for Precision Cosmology
- The KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7
- The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time
- The SAMI Galaxy Survey: instrument specification and target selection
- The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars
- Supermassive black holes and their feedback effects in the IllustrisTNG simulation
- The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations
- NIHAO project I: Reproducing the inefficiency of galaxy formation across cosmic time with a large sample of cosmological hydrodynamical simulations
- Improving the convergence properties of the moving-mesh code AREPO
- The MassiveBlack-II Simulation: The Evolution of Halos and Galaxies to z~0
- MUFASA: Galaxy Formation Simulations With Meshless Hydrodynamics
- The Romulus Cosmological Simulations: A Physical Approach to the Formation, Dynamics and Accretion Models of SMBHs
- A physical model for cosmological simulations of galaxy formation: multi-epoch validation
- Simulations of magnetic fields in isolated disk galaxies
- The Size Evolution of Star-forming and Quenched Galaxies in the IllustrisTNG simulation
- Magnetohydrodynamics on an unstructured moving grid
- The star-formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics
- The SPHINX Cosmological Simulations of the First Billion Years: the Impact of Binary Stars on Reionization
- Massive Black Hole Binary Mergers in Dynamical Galactic Environments
- The evolution of the mass-metallicity relation in IllustrisTNG
- SZ effects in the Magneticum Pathfinder Simulation: Comparison with the Planck, SPT, and ACT results
- The BlueTides Simulation: First Galaxies and Reionization
- Baryons in the CosmicWeb of IllustrisTNG - I: Gas in Knots, Filaments, Sheets and Voids
- The role of mergers and halo spin in shaping galaxy morphology
- The VLT LEGA-C Spectroscopic Survey: The Physics of Galaxies at a Lookback Time of 7 Gyr
- The abundance, distribution, and physical nature of highly ionized oxygen OVI, OVII, and OVIII in IllustrisTNG
- Following the flow: tracer particles in astrophysical fluid simulations
- The fraction of dark matter within galaxies from the IllustrisTNG simulations
- Jellyfish galaxies with the IllustrisTNG simulations: I. Gas-stripping phenomena in the full cosmological context
- Non-circular motions and the diversity of dwarf galaxy rotation curves
- Recoiling black holes: prospects for detection and implications of spin alignment
- Modeling the atomic-to-molecular transition in cosmological simulations of galaxy formation
- Angular momentum properties of haloes and their baryon content in the Illustris simulation
- Similar star formation rate and metallicity evolution timescales drive the fundamental metallicity relation
- Atomic hydrogen in IllustrisTNG galaxies: the impact of environment parallelled with local 21-cm surveys
- The uniformity and time-invariance of the intra-cluster metal distribution in galaxy clusters from the IllustrisTNG simulations
- A census of cool core galaxy clusters in IllustrisTNG
- The Hubble Sequence at in the IllustrisTNG simulation with deep learning
- Linking galaxy structural properties and star formation activity to black hole activity with IllustrisTNG
- Dark Sky Simulations: Early Data Release
- Shock finding on a moving-mesh: I. Shock statistics in non-radiative cosmological simulations
- Halo and Galaxy Formation Histories from the Millennium Simulation: Public release of a VO-oriented and SQL-queryable database for studying the evolution of galaxies in the LambdaCDM cosmogony
- Peaks above the Maxwellian Sea: A New Approach to Finding Substructure in N-Body Haloes
- The Millennium Run Observatory: First Light
- The EAGLE simulations of galaxy formation: Public release of particle data
- Formation of a Malin 1 analogue in IllustrisTNG by stimulated accretion
- Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
- Introducing the Dark Energy Universe Simulation Series (DEUSS)
- Shock finding on a moving-mesh: II. Hydrodynamic shocks in the Illustris universe
- Chemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulations
- Interactive 3D Visualization for Theoretical Virtual Observatories
- Skies And Universes: Accessing cosmological simulations and theoretical predictions
- A web portal for hydrodynamical, cosmological simulations
- AMADA-Analysis of Multidimensional Astronomical Datasets
Cited by in corpus (15)
- Baryons in the CosmicWeb of IllustrisTNG - I: Gas in Knots, Filaments, Sheets and Voids
- An unexpected high concentration for the dark substructure in the gravitational lens SDSSJ0946+1006
- Physical Correlations of the Scatter between Galaxy Mass, Stellar Content, and Halo Mass
- SDSS--IV MaNGA : The Inner Density Slopes of nearby galaxies
- Rivers of Gas I.: Unveiling The Properties of High Redshift Filaments
- Baryon-CDM isocurvature galaxy bias with IllustrisTNG
- Surrogate modelling the Baryonic Universe I: The colour of star formation
- Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
- The CO universe: Modelling CO emission and H abundance in cosmological galaxy formation simulations
- Machine learning synthetic spectra for probabilistic redshift estimation: SYTH-Z
- Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
- A Stringent Upper Limit on Dark Matter Self-Interaction Cross Section from Cluster Strong Lensing
- Probing Macro-Scale Gas Motions and Turbulence in Diffuse Cosmic Plasmas
- Capturing the inside-out quenching by black holes with far-infrared atomic line ratios
- Scalar Field Wave (Fuzzy) Dark Matter and the Formation of Galaxies