The Illustris Simulation: Public Data Release

Abstract

We present the full public release of all data from the Illustris simulation project. Illustris is a suite of large volume, cosmological hydrodynamical simulations run with the moving-mesh code Arepo and including a comprehensive set of physical models critical for following the formation and evolution of galaxies across cosmic time. Each simulates a volume of (106.5 Mpc)^3 and self-consistently evolves five different types of resolution elements from a starting redshift of z=127 to the present day, z=0. These components are: dark matter particles, gas cells, passive gas tracers, stars and stellar wind particles, and supermassive black holes. This data release includes the snapshots at all 136 available redshifts, halo and subhalo catalogs at each snapshot, and two distinct merger trees. Six primary realizations of the Illustris volume are released, including the flagship Illustris-1 run. These include three resolution levels with the fiducial "full" baryonic physics model, and a dark matter only analog for each. In addition, we provide four distinct, high time resolution, smaller volume "subboxes". The total data volume is ~265 TB, including ~800 full volume snapshots and ~30,000 subbox snapshots. We describe the released data products as well as tools we have developed for their analysis. All data may be directly downloaded in its native HDF5 format. Additionally, we release a comprehensive, web-based API which allows programmatic access to search and data processing tasks. In both cases we provide example scripts and a getting-started guide in several languages: currently, IDL, Python, and Matlab. This paper addresses scientific issues relevant for the interpretation of the simulations, serves as a pointer to published and on-line documentation of the project, describes planned future additional data releases, and discusses technical aspects of the release.

The data is made available at http://www.illustris-project.org/data/ (comments welcome)

References in corpus (36)

• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• The hierarchical formation of the brightest cluster galaxies
• Properties of galaxies reproduced by a hydrodynamic simulation
• Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
• The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas
• A unified model for AGN feedback in cosmological simulations of structure formation
• 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
• Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
• The Illustris simulation: the evolving population of black holes across cosmic time
• Cosmological Simulations of Intergalactic Medium Enrichment from Galactic Outflows
• Direct cosmological simulations of the growth of black holes and galaxies
• Mass, Metal, and Energy Feedback in Cosmological Simulations
• Baryon effects on the internal structure of LCDM halos in the EAGLE simulations
• Moving mesh cosmology: tracing cosmological gas accretion
• The Formation of Massive, Compact Galaxies at z=2 in the Illustris Simulation
• The star formation main sequence and stellar mass assembly of galaxies in the Illustris simulation
• Galactic Angular Momentum in the Illustris Simulation: Feedback and the Hubble Sequence
• Galaxy Morphology and Star Formation in the Illustris Simulation at z=0
• Halo Mass and Assembly History Exposed in the Faint Outskirts: the Stellar and Dark Matter Haloes of Illustris Galaxies
• The impact of feedback on cosmological gas accretion
• The distribution of neutral hydrogen around high-redshift galaxies and quasars in the EAGLE simulation
• Synthetic Galaxy Images and Spectra from the Illustris Simulation
• Metal Cooling in Simulations of Cosmic Structure Formation
• Recoiling black holes: prospects for detection and implications of spin alignment
• Damped Lyman-alpha absorbers as a probe of stellar feedback
• A new formulation of the Type Ia SN rate and its consequences on galactic chemical evolution
• The Impact of Galactic Feedback on the Circumgalactic Medium
• Reproducing the Kinematics of Damped Lyman-alpha Systems
• Lens galaxies in the Illustris simulation: power-law models and the bias of the Hubble constant from time-delays
• Shock finding on a moving-mesh: I. Shock statistics in non-radiative cosmological simulations
• Hot Gaseous Coronae around Spiral Galaxies: Probing the Illustris Simulation
• The colors of satellite galaxies in the Illustris Simulation
• Hydrogen Reionization in the Illustris universe
• Web-Based Visualization of Very Large Scientific Astronomy Imagery

Cited by in corpus (421)

• Simulating Galaxy Formation with the IllustrisTNG Model
• 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: public release of halo and galaxy catalogues
• The stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars
• The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations
• The Arepo public code release
• Simulating cosmic structure formation with the GADGET-4 code
• SDSS-IV MaNGA IFS Galaxy Survey --- Survey Design, Execution, and Initial Data Quality
• The star-formation activity of IllustrisTNG galaxies: main sequence, UVJ diagram, quenched fractions, and systematics
• Massive Black Hole Binary Mergers in Dynamical Galactic Environments
• Size evolution of normal and compact galaxies in the EAGLE simulation
• Lensing is Low: Cosmology, Galaxy Formation, or New Physics?
• Hyper Suprime-Cam Year 3 Results: Cosmology from Cosmic Shear Power Spectra
• The cosmic merger rate of neutron stars and black holes
• Quiescent galaxies 1.5 billion years after the Big Bang and their progenitors
• The BlueTides Simulation: First Galaxies and Reionization
• The role of mergers and halo spin in shaping galaxy morphology
• The cosmic merger rate of stellar black hole binaries from the Illustris simulation
• The abundance, distribution, and physical nature of highly ionized oxygen OVI, OVII, and OVIII in IllustrisTNG
• A whirling plane of satellite galaxies around Centaurus A challenges cold dark matter cosmology
• Morphology and star formation in IllustrisTNG: the build-up of spheroids and discs
• The stellar-to-halo mass relation over the past 12 Gyr
• The Formation of Ultra Diffuse Galaxies in Cored Dark Matter Halos Through Tidal Stripping and Heating
• The cosmic merger rate density of compact objects: impact of star formation, metallicity, initial mass function and binary evolution
• The Gravitational Wave Background from Massive Black Hole Binaries in Illustris: spectral features and time to detection with pulsar timing arrays
• Supermassive black holes in cosmological simulations I: M_BH-M_star relation and black hole mass function
• Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra
• The quenching and morphological evolution of central galaxies is facilitated by the feedback-driven expulsion of circumgalactic gas
• Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing
• Quenched fractions in the IllustrisTNG simulations: comparison with observations and other theoretical models
• Life beyond 30: probing the -20<M_UV<-17 luminosity function at 8<z<13 with the NIRCam parallel field of the MIRI Deep Survey
• High redshift JWST predictions from IllustrisTNG: Dust modelling and galaxy luminosity functions
• The properties of merging black holes and neutron stars across cosmic time
• Public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation
• Hydrodynamical simulations of the galaxy population: enduring successes and outstanding challenges
• The Formation of Ultra-Diffuse Galaxies in Clusters
• Baryonic impact on the dark matter distribution in Milky Way-size galaxies and their satellites
• The mass of our Milky Way
• Red & Dead CANDELS: massive passive galaxies at the dawn of the Universe
• Recoiling black holes: prospects for detection and implications of spin alignment
• Orbits of Massive Satellite Galaxies: I. A Close Look at the Large Magellanic Cloud and a New Orbital History for M33
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).I. Introduction to the Survey
• KMOS^3D: Dynamical constraints on the mass budget in early star-forming disks
• The diverse evolutionary paths of simulated high-z massive, compact galaxies to z=0
• A box full of chocolates: The rich structure of the nearby stellar halo revealed by Gaia and RAVE
• The impact of assembly bias on the halo occupation in hydrodynamical simulations
• Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays
• Angular momentum properties of haloes and their baryon content in the Illustris simulation
• Modeling baryonic physics in future weak lensing surveys
• Formation of Globular Cluster Systems: From Dwarf Galaxies to Giants
• The Diversity and Variability of Star Formation Histories in Models of Galaxy Evolution
• Gravitational wave sources from inspiralling globular clusters in the Galactic Centre and similar environments
• Zooming in on major mergers: dense, starbursting gas in cosmological simulations
• Tidally induced bars in Illustris galaxies
• The impact of baryonic physics on the subhalo mass function and implications for gravitational lensing
• The uniformity and time-invariance of the intra-cluster metal distribution in galaxy clusters from the IllustrisTNG simulations
• The origin of most massive black holes at high-z: BLUETIDES and the next quasar frontier
• Mapping substructure in the HST Frontier Fields cluster lenses and in cosmological simulations
• Cosmicflows-4: The Catalog of ~10000 Tully-Fisher Distances
• The masses and metallicities of stellar haloes reflect galactic merger histories
• The Origin and Evolution of Fast and Slow Rotators in the Illustris Simulation
• Massive Close Pairs Measure Rapid Galaxy Assembly in Mergers at High Redshift
• Galaxy gas as obscurer: II. Separating the galaxy-scale and nuclear obscurers of Active Galactic Nuclei
• SDSS IV MaNGA - An archaeological view of the Cosmic Star Formation History
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - II: Size-luminosity relations and the deficit of bulge-dominated galaxies in Illustris at low mass
• A Keck Survey of Gravitationally-Lensed Star-Forming Galaxies: High Spatial Resolution Studies of Kinematics and Metallicity Gradients
• A Deep Learning Approach to Galaxy Cluster X-ray Masses
• Lens galaxies in the Illustris simulation: power-law models and the bias of the Hubble constant from time-delays
• On the Assembly of Dwarf Galaxies in Clusters and their Efficient Formation of Globular Clusters
• Large-scale mass distribution in the Illustris simulation
• On the OVI Abundance in the Circumgalactic Medium of Low-Redshift Galaxies
• The Horizon Run 5 Cosmological Hydrodynamic Simulation: Probing Galaxy Formation from Kilo- to Giga-parsec Scales
• Astrophysical Sources of High Energy Neutrinos in the IceCube Era
• Massive BH Binaries as Periodically-Variable AGN
• The MEGaN project II. Gravitational waves from intermediate mass- and binary black holes around a supermassive black hole
• Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers
• Intrinsic Alignments of Galaxies in the Illustris Simulation
• Populations of filaments from the distribution of galaxies in numerical simulations
• Formation channels of single and binary stellar-mass black holes
• Interacting galaxies in the IllustrisTNG simulations -- I: Triggered star formation in a cosmological context
• The abundance of satellites around Milky Way- and M31-like galaxies with the TNG50 simulation: a matter of diversity
• The cosmic evolution of the spatially-resolved star formation rate and stellar mass of the CALIFA survey
• Revisiting the tension between fast bars and the $\Lambda$CDM paradigm
• Spin evolution and feedback of supermassive black holes in cosmological simulations
• Massive Dead Galaxies at z~2 with HST Grism Spectroscopy I. Star Formation Histories and Metallicity Enrichment
• An EAGLE's View of Ex-situ Galaxy Growth
• Tangos: the agile numerical galaxy organization system
• The information content of stellar halos: Stellar population gradients and accretion histories in early-type Illustris galaxies
• Co-evolution of massive black holes and their host galaxies at high redshift: discrepancies from six cosmological simulations and the key role of JWST
• Origins of scaling relations of globular cluster systems
• Quiescent Ultra-diffuse galaxies in the field originating from backsplash orbits
• QSO obscuration at high redshift ($z\gtrsim 7$): Predictions from the BlueTides simulation
• The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
• The relationship between fine galaxy stellar morphology and star formation activity in cosmological simulations: a deep learning view
• Suspicious Siblings: The Distribution of Mass and Spin Across Component Black Holes in Isolated Binary Evolution
• Aperture-free star formation rate of SDSS star-forming galaxies
• Intrinsic alignments of disk and elliptical galaxies in the MassiveBlack-II and Illustris simulations
• Flux-ratio anomalies from discs and other baryonic structures in the Illustris simulation
• Machine Learning and Cosmological Simulations II: Hydrodynamical Simulations
• The stellar halos of ETGs in the IllustrisTNG simulations: the photometric and kinematic diversity of galaxies at large radii
• Assessing the Jeans Anisotropic Multi-Gaussian Expansion method with the Illustris simulation
• The Frequency of Dwarf Galaxy Multiples at Low Redshift in SDSS vs. Cosmological Expectations
• New criteria for the selection of galaxy close pairs from cosmological simulations: evolution of the major and minor merger fraction in MUSE deep fields
• The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk survival through mergers
• The origin and properties of massive prolate galaxies in the Illustris simulation
• Stellar Halos in Illustris- Probing the Histories of Milky Way-Mass Galaxies
• Bounding Alternative Theories of Gravity with Multi-Band GW Observations
• Orbits of massive satellite galaxies: II. Bayesian Estimates of the Milky Way and Andromeda masses using high precision astrometry and cosmological simulations
• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• Black-hole remnants from black-hole--neutron-star mergers
• A moving mesh unstaggered constrained transport scheme for magnetohydrodynamics
• Advances in Constraining Intrinsic Alignment Models with Hydrodynamic Simulations
• Testing the effect of galactic feedback on the IGM at z ~ 6 with metal-line absorbers
• The missing light of the Hubble Ultra Deep Field
• Convergence of Lobatto-type Runge-Kutta methods for partitioned differential-algebraic systems of index 2
• Baryonic effects on the matter bispectrum
• Alignment between filaments and galaxy spins from the MaNGA integral-field survey
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• The host galaxies of double compact objects merging in the local Universe
• Kinematic decomposition of IllustrisTNG disk galaxies: morphology and relation with morphological structures
• Strong-lensing Measurement of the Mass-density Profile out to 3 Effective Radii for $z\sim 0.5$ Early-type Galaxies
• On the origin of star-gas counterrotation in low-mass galaxies
• Diagnosing galactic feedback with the line broadening in the low redshift Lyman-alpha forest
• The origin of the enhanced metallicity of satellite galaxies
• Imprints of temperature fluctuations on the $z\sim 5$ Lyman-$\alpha$ forest: a view from radiation-hydrodynamic simulations of reionization
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Chandra and XMM-Newton Observations of the Abell 3391/Abell 3395 Intercluster Filament
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• Galaxies lacking dark matter in the Illustris simulation
• Anisotropic satellite galaxy quenching modulated by supermassive black hole activity
• The Next Generation Virgo Cluster Survey (NGVS). XXIV. The Red Sequence to $\sim$10${}^6$ L${}_{\odot }$ and Comparisons with Galaxy Formation Models
• The star clusters that make black hole binaries across cosmic time
• X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at $z\gtrsim 2$
• Multi-flavour SMBH seeding and evolution in cosmological environments
• Determining star-formation rates in Active Galactic Nuclei hosts via stellar population synthesis
• Evaluating the ability of triaxial Schwarzschild modelling to estimate properties of galaxies from the Illustris simulation
• Discrepancies between CFHTLenS cosmic shear & Planck: new physics or systematic effects?
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• The growth of brightest cluster galaxies in the TNG300 simulation:dissecting the contributions from mergers and in situ star formation
• Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
• Simulating the effect of high column density absorbers on the one-dimensional Lyman-alpha forest flux power spectrum
• Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• Synthetic observations of star formation and the interstellar medium
• The first Super Massive Black Holes: indications from models for future observations
• Forecasts for the WFIRST High Latitude Survey using the BlueTides Simulation
• Submillimetre galaxies in cosmological hydrodynamical simulations -- an opportunity for constraining feedback models
• The effect of differential accretion on the Gravitational Wave Background and the present day MBH Binary population
• The Mass Profile of the Milky Way to the Virial Radius from the Illustris Simulation
• ERGO-ML I: Inferring the assembly histories of IllustrisTNG galaxies from integral observable properties via invertible neural networks
• Accelerated Bayesian SED Modeling using Amortized Neural Posterior Estimation
• The Lopsidedness of Satellite Galaxy Systems in $\Lambda$CDM simulations
• Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass
• Cosmic variance of $z>7$ galaxies: Prediction from BlueTides
• Shock finding on a moving-mesh: II. Hydrodynamic shocks in the Illustris universe
• Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
• SDSS--IV MaNGA : The Inner Density Slopes of nearby galaxies
• Gravitational Self-Lensing in Populations of Massive Black Hole Binaries
• Accretion of Galaxy Groups into Galaxy Clusters
• BlueTides simulation: establishing black hole-galaxy relations at high-redshift
• The role of gas infall in the evolution of disc galaxies
• The boundary of cosmic filaments
• Velocity Dispersions of Brightest Cluster Galaxies and Their Host Clusters
• The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
• CosmoGridV1: a simulated $w$CDM theory prediction for map-level cosmological inference
• The ${\chi }_{\mathrm{eff}}-z$ correlation of field binary black hole mergers and how 3G gravitational-wave detectors can constrain it
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• Correlations in the three-dimensional Lyman-alpha forest contaminated by high column density absorbers
• Gravitational imaging through a triple source plane lens: revisiting the $\Lambda$CDM-defying dark subhalo in SDSSJ0946+1006
• Properties and Origin of Galaxy Velocity Bias in the Illustris Simulation
• Galaxies with prolate rotation in Illustris
• The Effect Of AGN Heating On The Low-Redshift Lyα Forest
• A gradient based method for modeling baryons and matter in halos of fast simulations
• The host galaxies of double compact objects across cosmic time
• The morphology and kinematics of the gaseous circumgalactic medium of Milky Way mass galaxies -- II. comparison of IllustrisTNG and Illustris simulation results
• The formation of low surface brightness galaxies in the IllustrisTNG simulation
• Evolution of the Stellar Mass--Metallicity Relation - I: Galaxies in the z~0.4 Cluster Cl0024
• Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\ge 10$?
• Galaxy assembly bias of central galaxies in the Illustris simulation
• [CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST
• Small-scale galaxy clustering in the EAGLE simulation
• Tidal destruction in a low mass galaxy environment: the discovery of tidal tails around DDO 44
• Simulating the effect of photoheating feedback during reionization
• Unequal-Time Correlators for Cosmology
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• The impact of galactic feedback on the shapes of dark-matter haloes
• On the relative effect of nodes and filaments of the cosmic web on the quenching of galaxies and the orientation of their spin
• Beyond two-point statistics: using the minimum spanning tree as a tool for cosmology
• Simulating the Spatial Distribution and Kinematics of Globular Clusters within Galaxy Clusters in Illustris
• IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies
• Cosmological simulations of massive black hole seeds: predictions for next generation electromagnetic and gravitational wave observations
• $\Lambda$CDM Predictions for the Satellite Population of M33
• Black hole clustering and duty cycles in the Illustris simulation
• Discriminating Topology in Galaxy Distributions using Network Analysis
• AGN jet feedback on a moving mesh: lobe energetics and X-ray properties in a realistic cluster environment
• Gas outflows from the z= 7.54 quasar : predictions from the BlueTides Simulation
• X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback
• The impact of Lyman-$\alpha$ radiative transfer on large-scale clustering in the Illustris simulation
• Evolution of CIV Absorbers I. The Cosmic Incidence
• The Active Assembly of the Virgo Cluster: Indications for Recent Group Infall From Early-Type Dwarf Galaxies
• The Local Group: The Ultimate Deep Field
• Cosmological insights into the assembly of the radial and compact stellar halo of the Milky Way
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• A few StePS forward in unveiling the complexity of galaxy evolution: light-weighted stellar ages of intermediate redshift galaxies with WEAVE
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
• Simba: The average properties of the circumgalactic medium of $2\le z\le 3$ quasars are determined primarily by stellar feedback
• Evolution of galaxy groups in the Illustris simulation
• The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
• The Impact of baryonic physics on the kinetic Sunyaev-Zel'dovich Effect
• Intergalactic filaments spin
• The DESI PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) Mock Challenge
• Dark-matter-deficient galaxies in hydrodynamical simulations
• An improved probabilistic approach for linking progenitor and descendant galaxy populations using comoving number density
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. I. Construction and analysis of the mock data cubes
• REQUIEM-2D: Spatially Resolved Stellar Populations from HST 2D Grism Spectroscopy
• Quenching in Cosmic Sheets: Tracing the Impact of Large Scale Structure Collapse on the Evolution of Dwarf Galaxies
• Systematic errors in strong gravitational lensing reconstructions, a numerical simulation perspective
• Hot and counter-rotating star-forming disk galaxies in IllustrisTNG and their real-world counterparts
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• Quantifying the energy balance between the turbulent ionised gas and young stars
• The stellar mass - size relation for cluster galaxies at z=1 with high angular resolution from the Gemini/GeMS multi-conjugate adaptive optics system
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• The Dependence of Halo Mass on Galaxy Size at Fixed Stellar Mass Using Weak Lensing
• Prospects for Recovering Galaxy Intrinsic Shapes from Projected Quantities
• Giant Lyman-Alpha Nebulae in the Illustris Simulation
• Spherical Cows in Dark Matter Indirect Detection
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• TARDIS Paper II: Synergistic Density Reconstruction from Lyman-alpha Forest and Spectroscopic Galaxy Surveys with Applications to Protoclusters and the Cosmic Web
• Considerations for the Observability of Kinematically Offset Binary AGN
• Turnaround radius of galaxy clusters in N-body simulations
• Lyα emitters in a cosmological volume I: the impact of radiative transfer
• Redshift Evolution of the Fundamental Plane Relation in the IllustrisTNG Simulation
• REQUIEM-2D: A diversity of formation pathways in a sample of spatially-resolved massive quiescent galaxies at z~2
• MUSE-ALMA Haloes VII: Survey Science Goals & Design, Data Processing and Final Catalogues
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• 21st Century Statistical and Computational Challenges in Astrophysics
• The SAMI Galaxy Survey: Environmental analysis of the orbital structures of passive galaxies
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• Hydrodynamical structure formation in Milgromian cosmology
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• Investigating Cosmological GAN Emulators Using Latent Space Interpolation
• The early growth of supermassive black holes in cosmological hydrodynamic simulations with constrained Gaussian realizations
• Physical properties of galaxies: toward a consistent comparison between hydrodynamical simulations and SDSS
• The SELGIFS data challenge: generating synthetic observations of CALIFA galaxies from hydrodynamical simulations
• Radiative Transfer Distortions of Lyman-$\alpha$ Emitters: a New Fingers-of-God Damping in the Clustering in Redshift Space
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• Simulating the Carbon Footprint of Galactic Halos
• Through a Smoother Lens: An expected absence of LCDM substructure detections from hydrodynamic and dark matter only simulations
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Resolving Disks & Mergers in $z\sim 2$ Heavily Reddened Quasars and their Companion Galaxies with ALMA
• The Case for Strangulation in Low-Mass Hosts: DDO 113
• Supermassive black hole fueling in IllustrisTNG: Impact of environment
• Backlighting extended gas halos around luminous red galaxies: kinematic Sunyaev-Zel'dovich effect from DESI Y1 x ACT
• Clumpy galaxies in cosmological simulations: The effect of ISM model
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
• What Is Inside Matters: Simulated Green Valley Galaxies Have Centrally Concentrated Star Formation
• Constraints on the Galactic Inner Halo Assembly History from the Age Gradient of Blue Horizontal-branch Stars
• An accurate analytic mass model for lensing galaxies
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• Spatially resolved spectroscopy across stellar surfaces. IV. F, G, & K-stars: Synthetic 3D spectra at hyper-high resolution
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• PopSED: Population-Level Inference for Galaxy Properties from Broadband Photometry with Neural Density Estimation
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• Interactive 3D Visualization for Theoretical Virtual Observatories
• The evolutionary pathways of disk galaxies with different sizes
• The cosmic epoch dependence of environmental effects on size evolution of red-sequence early-type galaxies
• Two channels for the formation of compact dwarf galaxies in clusters of galaxies
• Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• An estimate of the stochastic gravitational wave background from the MassiveBlackII simulation
• Visual Analysis of Large Multivariate Scattered Data using Clustering and Probabilistic Summaries
• Multi-wavelength properties of 850-$\mu$m selected sources from the North Ecliptic Pole SCUBA-2 survey
• Probing the Metal Enrichment of the Intergalactic Medium at $z=5-6$ Using the Hubble Space Telescope
• On the small scale clustering of quasars: constraints from the MassiveBlack II simulation
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• Baryonic feedback measurement from KV450 cosmic shear analysis
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption
• MIND THE GAP: Is The Too Big To Fail Problem Resolved?
• Exploring the Fate of Stellar Core Collapse with Supernova Relic Neutrinos
• The origin of star-gas misalignments in simulated galaxies
• Galaxies with kinematically distinct cores in Illustris
• SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
• IllustrisTNG Insights: Factors Affecting the Presence of Bars in Disk Galaxies
• Evidence for anisotropic quenching in massive galaxy clusters at $z\approx 0.5$
• How do galaxy properties affect void statistics?
• Compact Galaxies at Intermediate Redshifts Quench Faster than Normal-sized Galaxies
• The parallelism between galaxy clusters and early-type galaxies: I. The light and mass profiles
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• The hot gas mass fraction in halos. From Milky Way-like groups to massive clusters
• Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
• Neural Stellar Population Synthesis Emulator for the DESI PROVABGS
• Galaxy stellar and total mass estimation using machine learning
• Velocity Dispersions of Massive Quiescent Galaxies from Weak Lensing and Spectroscopy
• Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman-$\alpha$ Forest Tomography at $z=2$
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• Universal scaling laws and density slope for dark matter haloes
• The Star-Formation Properties of the Observed and Simulated AGN Universe: BAT vs EAGLE
• The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• Revealing the Galaxy-Halo Connection Through Machine Learning
• Resolution Convergence in Cosmological Hydrodynamical Simulations Using Adaptive Mesh Refinement
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• Simultaneous Dependence of Matter Clustering on Scale and Environment
• Detecting preheating in proto-clusters with Lyman-$\alpha$ Forest Tomography
• The Magellanic Clouds are very rare in the IllustrisTNG simulations
• Dark matter halo mass functions and density profiles from mass and energy cascade
• Multiple stellar populations in Schwarzschild modeling and the application to the Fornax dwarf
• Quantifying Observational Projection Effects with a Simulation-based hot CGM model
• Can HI 21 cm line trace the Missing Baryons in the Filamentary Structures?
• Implications of galaxy buildup for putative IMF variations in massive galaxies
• PAC.V. The Roles of Mass and Environment in the Quenching of Galaxies
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• On the detectability of massive black hole merger eventsby LISA
• Star Formation in Massive Galaxies at Redshift $z\sim 0.5$
• Discrimination of heavy elements originating from Pop III stars in z = 3 intergalactic medium
• Comparing galaxy morphology in hydrodynamical simulation and in semi-analytic model
• Can $\Lambda$CDM model reproduce MOND-like behavior?
• What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies
• Searching for the shadows of giants II: the effect of local ionisation on the Lyman-$\alpha$ absorption signatures of protoclusters at redshift $z\sim 2.4$
• Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
• Gravitational Wave Peeps from EMRIs and their Implication for LISA Signal Confusion Noise
• Resolved star formation in TNG100 central and satellite galaxies
• Quenched, bulge-dominated, but dynamically cold galaxies in IllustrisTNG and their real-world counterparts
• Asymmetric Drift of Andromeda Analogs in the IllustrisTNG Simulation
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• SCONCE: A cosmic web finder for spherical and conic geometries
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• A Novel Estimator for the Equation of State of the IGM by Ly$\alpha$ Forest Tomography
• Photometry and kinematics of dwarf galaxies from the Apertif HI survey
• Haloes at the ragged edge: The importance of the splashback radius
• Host Galaxy Demographics Of Individually Detectable Supermassive Black-hole Binaries with Pulsar Timing Arrays
• $\text{slick}$: Modeling a Universe of Molecular Line Luminosities in Hydrodynamical Simulations
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• Mitigating baryon feedback bias in cosmic shear through a theoretical error covariance in the matter power spectrum
• Satellite galaxies in the Illustris-1 simulation: anisotropic locations around relatively isolated hosts
• The Fundamental Plane in the hierarchical context
• The effects of the orbital configurations of mergers on reshaping galaxy structures
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Mass Reconstruction of Galaxy-scale Strong Gravitational Lenses Using a Broken Power-law Model
• SHARP -- IX. The dense, low-mass perturbers in B1938+666 and J0946+1006: implications for cold and self-interacting dark matter
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• On the Effects of Local Environment on Active Galactic Nucleus (AGN) in the Horizon Run 5 Simulation
• The Shape of FIREbox Galaxies and a Potential Tension with Low-mass Disks
• Probing $z\gtrsim 6$ massive black holes with gravitational waves
• Satellite Galaxies in the Illustris-1 Simulation: Poor Tracers of the Mass Distribution
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• Star formation across cosmic time
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
• The scaling relations of galaxies back in time: the road toward virialization
• A statistical study of lopsided galaxies using random forest
• Retrieving the hot circumgalactic medium physics from the X-ray radial profile from eROSITA with an IlustrisTNG-based forward model
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Conditional Colour-Magnitude Distribution of Central Galaxies in Galaxy Formation Models
• Probing the earliest phases in the formation of massive galaxies with simulated HST+JWST imaging data from Illustris
• SpArcFiRe: morphological selection effects due to reduced visibility of tightly winding arms in distant spiral galaxies
• Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations
• Evolution of dwarf spheroidal satellites in the common surface-density dark halos
• A new framework for understanding the evolution of early-type galaxies
• Cosmic filament spin -- I: a comparative study in observation
• Not so-dark: High resolution HI imaging of J0139+4328 and identification of an optical counterpart
• Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
• FLAMINGO: Galaxy formation and feedback effects on the gas density and velocity fields
• Continuous Simulation Data Stream: A dynamical timescale-dependent output scheme for simulations
• The evolution of the barred galaxy population in the TNG50 simulation
• The mass and galaxy distribution around SZ-selected clusters
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
• Inferring Galactic Parameters from Chemical Abundances: A Multi-Star Approach
• Tracing the origins of galaxy lopsidedness across cosmic time
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• Multiscale Cosmic Curvature: from Local Structures to Cosmology
• Extremely Isolated Galaxies I. Sample and Simulation Analysis
• The Cosmic Evolution of CIV Absorbers at $1.4<z<4.5$: Insights from $100,000$ Systems in DESI Quasars
• Dispersion Measures of Fast Radio Bursts through the Epoch of Reionization
• Merger Tree-based Galaxy Matching: A Comparative Study Across Different Resolutions
• Dynamics of merging: Post-merger mixing and relaxation of an Illustris galaxy
• Line-of-Sight Velocity Projection Impact on the Local Group Mass
• The FLAMINGO simulations data release
• Galaxy infall models for arbitrary velocity directions
• Cosmic quenching and scaling laws for the evolution of supermassive black holes and host galaxies
• Photometric and Kinematic Misalignments and Their Evolution Among Fast and Slow Rotators in the Illustris Simulation
• Are all post-starbursts mergers? HST reveals hidden disturbances in the majority of PSBs
• Detecting and analysing the topology of the cosmic web with spatial clustering algorithms I: Methods
• A novel analysis of contamination in Lyman-break galaxy samples at $\mathbf{z}\sim 6-8$: spatial correlation with intermediate-redshift galaxies at $\mathbf{z}\sim 1.3-2$
• A hierarchical clustering method for quantifying satellite abundance
• Constraining Galaxy-Halo Connection Using Machine Learning
• Strong-lensing rates of massive black hole binaries in LISA
• Gas-rich dwarf galaxy multiples in the Apertif HI survey
• Investigating the residuals in the $M_{\bullet }-M_{\ast }$ relation using the SIMBA cosmological simulation
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• CosmoGLINT: Cosmological Generative Model for Line Intensity Mapping with Transformer
• On a critical acceleration scale of dark matter in Lambda-CDM and dynamical dark energy
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• Semi-empirical constraints on the HI mass function of star-forming galaxies and ${\Omega }_{\mathrm{HI}}$ at $z\sim 0.37$ from interferometric surveys
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• The Delegate Survey: KOALA/AAOmega-IFU spectroscopy of three nearby dwarf galaxies
• High and low Sérsic index bulges in Milky Way- and M31-like galaxies: origin and connection to the bar with TNG50
• The major merger origin of the Andromeda II kinematics
• The black hole population in low-mass galaxies in large-scale cosmological simulations
• The Distribution of Satellite Galaxies in the TNG100 Simulation
• Islands in Simulated Cosmos: Probing the Hubble Flow around Groups and Clusters
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• The galaxy starburst/main-sequence bimodality over five decades in stellar mass at z ~ 3-6.5
• Lack of influence of the environment in the earliest stages of massive galaxy formation