Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe

Abstract

We introduce the Illustris Project, a series of large-scale hydrodynamical simulations of galaxy formation. The highest resolution simulation, Illustris-1, covers a volume of $(106.5\mathrm{Mpc}{)}^3$, has a dark mass resolution of $6.26\times 10^6{\mathrm{M}}_{\odot }$, and an initial baryonic matter mass resolution of $1.26\times 10^6{\mathrm{M}}_{\odot }$. At $z=0$ gravitational forces are softened on scales of $710\mathrm{pc}$, and the smallest hydrodynamical gas cells have an extent of $48\mathrm{pc}$. We follow the dynamical evolution of $2\times 1820^3$ resolution elements and in addition passively evolve $1820^3$ Monte Carlo tracer particles reaching a total particle count of more than $18$ billion. The galaxy formation model includes: primordial and metal-line cooling with self-shielding corrections, stellar evolution, stellar feedback, gas recycling, chemical enrichment, supermassive black hole growth, and feedback from active galactic nuclei. At $z=0$ our simulation volume contains about $40,000$ well-resolved galaxies covering a diverse range of morphologies and colours including early-type, late-type and irregular galaxies. The simulation reproduces reasonably well the cosmic star formation rate density, the galaxy luminosity function, and baryon conversion efficiency at $z=0$. It also qualitatively captures the impact of galaxy environment on the red fractions of galaxies. The internal velocity structure of selected well-resolved disk galaxies obeys the stellar and baryonic Tully-Fisher relation together with flat circular velocity curves. In the well-resolved regime the simulation reproduces the observed mix of early-type and late-type galaxies. Our model predicts a halo mass dependent impact of baryonic effects on the halo mass function and the masses of haloes caused by feedback from supernova and active galactic nuclei.

32 pages, 26 figures. MNRAS accepted. The official Illustris website can be found at http://www.illustris-project.org

References in corpus (20)

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• The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas
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• Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
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• Effects of Baryons and Dissipation on the Matter Power Spectrum
• Moving mesh cosmology: tracing cosmological gas accretion
• Scaling Relations of Spiral Galaxies
• Dependence of Galaxy Quenching on Halo Mass and Distance from its Centre
• The Fundamental Properties of Galaxies and a New Galaxy Classification System
• Bent by baryons: the low mass galaxy-halo relation
• Cosmic ray feedback in hydrodynamical simulations of galaxy formation
• The Tully-Fisher Relation and Its Residuals for a Broadly Selected Sample of Galaxies
• The abundance of (not just) dark matter haloes
• Thermal conduction in cosmological SPH simulations
• On the baryonic, stellar, and luminous scaling relations of disk galaxies
• The Effect of Gas Physics on the Halo Mass Function
• Rhapsody. I. Structural Properties and Formation History From a Statistical Sample of Re-simulated Cluster-size Halos
• Diffuse gas properties and stellar metallicities in cosmological simulations of disc galaxy formation

Cited by in corpus (487)

• The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
• Simulating galaxy formation with black hole driven thermal and kinetic feedback
• Simba: Cosmological Simulations with Black Hole Growth and Feedback
• The Circumgalactic Medium
• The Illustris simulation: the evolving population of black holes across cosmic time
• Baryon effects on the internal structure of LCDM halos in the EAGLE simulations
• The NANOGrav 15-year Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational Wave Background
• The Size Evolution of Star-forming and Quenched Galaxies in the IllustrisTNG simulation
• The Formation of Massive, Compact Galaxies at z=2 in the Illustris Simulation
• An excess of massive stars in the local 30 Doradus starburst
• The star formation main sequence and stellar mass assembly of galaxies in the Illustris simulation
• Mimetic gravity: a review of recent developments and applications to cosmology and astrophysics
• Dwarf galaxies in CDM and SIDM with baryons: observational probes of the nature of dark matter
• Galactic Angular Momentum in the Illustris Simulation: Feedback and the Hubble Sequence
• On the interplay between star formation and feedback in galaxy formation simulations
• Lensing is Low: Cosmology, Galaxy Formation, or New Physics?
• An Atlas of Color-selected Quiescent Galaxies at $z>3$ in Public $JWST$ Fields
• The role of mergers and halo spin in shaping galaxy morphology
• SDSS-IV MaNGA: Spatially resolved star formation histories in galaxies as a function of galaxy mass and type
• Galaxies as simple dynamical systems: observational data disfavor dark matter and stochastic star formation
• The cosmic merger rate of stellar black hole binaries from the Illustris simulation
• A refined sub-grid model for black hole accretion and AGN feedback in large cosmological simulations
• A chronicle of galaxy mass assembly in the EAGLE simulation
• Morphology and star formation in IllustrisTNG: the build-up of spheroids and discs
• Observational constraints on the merger history of galaxies since $z\approx 6$: Probabilistic galaxy pair counts in the CANDELS fields
• An excess of small-scale gravitational lenses observed in galaxy clusters
• Large-scale dark matter simulations
• Neutral hydrogen in galaxy halos at the peak of the cosmic star formation history
• The SAMI Galaxy Survey: Revisiting Galaxy Classification Through High-Order Stellar Kinematics
• The impact of feedback on cosmological gas accretion
• Full-sky Gravitational Lensing Simulation for Large-area Galaxy Surveys and Cosmic Microwave Background Experiments
• The KMOS^3D Survey: data release and final survey paper
• MUFASA: Galaxy star formation, gas, and metal properties across cosmic time
• ELUCID - Exploring the Local Universe with reConstructed Initial Density field III: Constrained Simulation in the SDSS Volume
• The properties of merging black holes and neutron stars across cosmic time
• Synthetic Galaxy Images and Spectra from the Illustris Simulation
• Are galactic star formation and quenching governed by local, global or environmental phenomena?
• Hydrodynamical simulations of the galaxy population: enduring successes and outstanding challenges
• The formation and evolution of low-surface-brightness galaxies
• HBT+: an improved code for finding subhalos and building merger trees in cosmological simulations
• Galaxy Simulation with Dust Formation and Destruction
• Feedback from Active Galactic Nuclei in Galaxy Groups
• Diverse Stellar Haloes in Nearby Milky Way-Mass Disc Galaxies
• Ages of Type Ia Supernovae Over Cosmic Time
• Revisiting the Integrated Star Formation Law. II. Starbursts and the Combined Global Schmidt Law
• Intracluster Light at the Frontier II: The Frontier Fields Clusters
• Far-infrared and dust properties of present-day galaxies in the EAGLE simulations
• The impact of galactic properties and environment on the quenching of central and satellite galaxies: A comparison between SDSS, Illustris and L-Galaxies
• Orbits of Massive Satellite Galaxies: I. A Close Look at the Large Magellanic Cloud and a New Orbital History for M33
• Lyman-alpha emitters gone missing: evidence for late reionization?
• Damped Lyman-alpha absorbers as a probe of stellar feedback
• The Athena X-ray Integral Field Unit (X-IFU)
• Metal-enriched, sub-kiloparsec gas clumps in the circumgalactic medium of a faint z = 2.5 galaxy
• Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations
• A box full of chocolates: The rich structure of the nearby stellar halo revealed by Gaia and RAVE
• The equilibrium view on dust and metals in galaxies: Galactic outflows drive low dust-to-metal ratios in dwarf galaxies
• Atomic and molecular gas in IllustrisTNG galaxies at low redshift
• A consistent measure of the merger histories of massive galaxies using close-pair statistics I: Major mergers at $z<3.5$
• ProFit: Bayesian Profile Fitting of Galaxy Images
• A Critical Look at the Mass-Metallicity-SFR Relation in the Local Universe. I. An Improved Analysis Framework and Confounding Systematics
• Detailed Shape and Evolutionary Behavior of the X-ray Luminosity Function of Active Galactic Nuclei
• Constraining $M_{\nu }$ with the Bispectrum II: The Total Information Content of the Galaxy Bispectrum
• The Diversity and Variability of Star Formation Histories in Models of Galaxy Evolution
• Inspiraling Halo Accretion Mapped in Lyman-$\alpha$ Emission around a $z\sim 3$ Quasar
• The Impact of Galactic Feedback on the Circumgalactic Medium
• Stochastic modeling of star-formation histories I: the scatter of the star-forming main sequence
• Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium
• Numerical Convergence in Smoothed Particle Hydrodynamics
• The uniformity and time-invariance of the intra-cluster metal distribution in galaxy clusters from the IllustrisTNG simulations
• SDSS IV MaNGA - The spatially resolved transition from star formation to quiescence
• The origin of most massive black holes at high-z: BLUETIDES and the next quasar frontier
• The low-end of the black hole mass function at cosmic dawn
• Quiescence correlates strongly with directly-measured black hole mass in central galaxies
• The KMOS Redshift One Spectroscopic Survey (KROSS): rotational velocities and angular momentum of z~0.9 galaxies
• Simulations of the star-forming molecular gas in an interacting M51-like galaxy
• Host galaxies of merging compact objects: mass, star formation rate, metallicity and colours
• Supermassive black holes as the regulators of star formation in central galaxies
• From light to baryonic mass: the effect of the stellar mass-to-light ratio on the Baryonic Tully-Fisher relation
• MIGHTEE-HI: The HI emission project of the MeerKAT MIGHTEE survey
• Simulating Groups and the IntraGroup Medium: The Surprisingly Complex and Rich Middle Ground Between Clusters and Galaxies
• Massive Close Pairs Measure Rapid Galaxy Assembly in Mergers at High Redshift
• Advanced LIGO Constraints on Neutron Star Mergers and R-Process Sites
• Timing the formation and assembly of early-type galaxies via spatially resolved stellar populations analysis
• Galaxy gas as obscurer: II. Separating the galaxy-scale and nuclear obscurers of Active Galactic Nuclei
• The Scaling of Stellar Mass and Central Stellar Velocity Dispersion for Quiescent galaxies at z < 0.7
• 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
• Reproducing the Kinematics of Damped Lyman-alpha Systems
• Fast Radio Bursts and cosmological tests
• Galaxy Zoo: Morphological Classifications for 120,000 Galaxies in HST Legacy Imaging
• Galaxy Merger Rates up to z $\sim$ 3 using a Bayesian Deep Learning Model $-$ A Major-Merger classifier using IllustrisTNG Simulation data
• Fast galaxy bars continue to challenge standard cosmology
• Hunting for Massive Black Holes in Dwarf Galaxies
• Major Merging History in CANDELS. I. Evolution of the Incidence of Massive Galaxy-Galaxy Pairs from z=3 to z~0
• Black Hole -- Galaxy Correlations in Simba
• Identifying Galaxy Mergers in Observations and Simulations with Deep Learning
• Galaxy Zoo: the effect of bar-driven fueling on the presence of an active galactic nucleus in disc galaxies
• Intrinsic alignments of galaxies in the MassiveBlack-II simulation: analysis of two-point statistics
• Gas and galaxies in filament between clusters of galaxies: The study of A399-A401
• MAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest regions of a protocluster at z=2.5
• The Multi-Wavelength Tully-Fisher relation with spatially resolved HI kinematics
• Storm in a "Teacup": a radio-quiet quasar with ~10kpc radio-emitting bubbles and extreme gas kinematics
• The MUSE Hubble Ultra Deep Field Survey. IX. Evolution of galaxy merger fraction since z~6
• Galactic rotation curves, the baryon-to-dark-halo-mass relation and space-time scale invariance
• Shock finding on a moving-mesh: I. Shock statistics in non-radiative cosmological simulations
• The SAMI Galaxy Survey: Data Release One with Emission-line Physics Value-Added Products
• Dust scaling relations in a cosmological simulation
• The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z=3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early Universe
• Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
• Properties of HI discs in the Auriga cosmological simulations
• ELUCID IV: Galaxy Quenching and its Relation to Halo Mass, Environment, and Assembly Bias
• The evolution of the star formation rate function in the EAGLE simulations: A comparison with UV, IR and H$\alpha$ observations from z ~ 8 to z ~ 0
• Hot Gaseous Coronae around Spiral Galaxies: Probing the Illustris Simulation
• The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
• Chasing passive galaxies in the early Universe: a critical analysis in CANDELS GOODS-South
• Distinguishing Mergers and Disks in High Redshift Observations of Galaxy Kinematics
• Black-hole-regulated star formation in massive galaxies
• An EAGLE's View of Ex-situ Galaxy Growth
• What shapes a galaxy? - Unraveling the role of mass, environment and star formation in forming galactic structure
• The evolution of the Milky Way: New insights from open clusters
• The colors of satellite galaxies in the Illustris Simulation
• Fast and energetic AGN-driven outflows in simulated dwarf galaxies
• The Effects of AGN Feedback on Present-Day Galaxy Properties in Cosmological Simulations
• Co-evolution of massive black holes and their host galaxies at high redshift: discrepancies from six cosmological simulations and the key role of JWST
• The information content of stellar halos: Stellar population gradients and accretion histories in early-type Illustris galaxies
• Black hole feeding and feedback: the physics inside the "subgrid"
• Baryonic and dark matter distribution in cosmological simulations of spiral galaxies
• Quiescent Ultra-diffuse galaxies in the field originating from backsplash orbits
• Light, medium-weight or heavy? The nature of the first supermassive black hole seeds
• On the evolution of galaxy spin in a cosmological hydrodynamic simulation of galaxy clusters
• The origin of dust in galaxies across cosmic time
• Being KLEVER at cosmic noon: ionised gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
• The Argo Simulation: II. The Early Build-up of the Hubble Sequence
• Galaxy mergers moulding the circum-galactic medium - I. The impact of a major merger
• The coherent motion of Cen A dwarf satellite galaxies remains a challenge for $\Lambda$CDM cosmology
• Probing 3D Structure with a Large MUSE Mosaic: Extending the Mass Model of Frontier Field Abell 370
• Identifying the subtle signatures of feedback from distant AGN using ALMA observations and the EAGLE hydrodynamical simulations
• RAiSE II: resolved spectral evolution in radio AGN
• When the Jeans don't fit: How stellar feedback drives stellar kinematics and complicates dynamical modeling in low-mass galaxies
• The fundamental signature of star formation quenching from AGN feedback: A critical dependence of quiescence on supermassive black hole mass not accretion rate
• The galaxy-halo connection of emission-line galaxies in IllustrisTNG
• ALMA measures rapidly depleted molecular gas reservoirs in massive quiescent galaxies at z~1.5
• Impact of Lyman alpha pressure on metal-poor dwarf galaxies
• The ALPINE-ALMA [CII] survey: The contribution of major mergers to the galaxy mass assembly at z~5
• Dynamical evolution of cosmic supermassive binary black holes and their gravitational wave radiation
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk survival through mergers
• Galaxy gas as obscurer: I. GRBs x-ray galaxies and find a N_H ~ M* relation
• NIHAO XIX: How supernova feedback shapes the galaxy baryon cycle
• Constraining the HI-Halo Mass Relation From Galaxy Clustering
• The mass, colour, and structural evolution of today's massive galaxies since z~5
• Thermal and radiative AGN feedback have a limited impact on star formation in high-redshift galaxies
• Host galaxy properties of mergers of stellar binary black holes and their implications for advanced LIGO gravitational wave sources
• The origin and properties of massive prolate galaxies in the Illustris simulation
• The edge of galaxy formation I: formation and evolution of MW-satellites analogues before accretion
• Host galaxies of high-redshift quasars: supermassive black hole growth and feedback
• IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Detailed HI kinematics of Tully-Fisher calibrator galaxies
• Galactic inflow and wind recycling rates in the EAGLE simulations
• Realistic simulations of galaxy formation in f(R) modified gravity
• Bulge plus disc and Sérsic decomposition catalogues for 16,908 galaxies in the SDSS Stripe 82 co-adds: A detailed study of the $ugriz$ structural measurements
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Identification of AGN through SED Fitting and the Evolution of the Bolometric AGN Luminosity Function
• SDSS IV MaNGA: Visual Morphological and Statistical Characterization of the DR15 sample
• A direct measurement of galaxy major and minor merger rates and stellar mass accretion histories at $z<3$ using galaxy pairs in the REFINE survey
• KASHz: No evidence for ionised outflows instantaneously suppressing star formation in moderate luminosity AGN at $z$$\sim$$1.4$-$2.6$
• A missing outskirts problem? Comparisons between stellar halos in the Dragonfly Nearby Galaxies Survey and the TNG100 simulation
• The Relationship Between Star-formation Activity and Galaxy Structural Properties in CANDELS and a Semi-analytic Model
• Galaxy Zoo: Unwinding the Winding Problem - Observations of Spiral Bulge Prominence and Arm Pitch Angles Suggest Local Spiral Galaxies are Winding
• The effects of host galaxy properties on merging compact binaries detectable by LIGO
• Common Envelope Evolution on a Moving Mesh
• The merger-starburst connection across cosmic times
• Sub one percent mass fractions of young stars in red massive galaxies
• Increasing blackhole feedback induced quenching with anisotropic thermal conduction
• Morphological decomposition of TNG50 galaxies: methodology and catalogue
• Direct Measurement of the HI-Halo Mass Relation through Stacking
• Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• No signs of star formation being regulated in the most luminous quasars at z~2 with ALMA
• The Cosmic Microwave Background: The history of its experimental investigation and its significance for cosmology
• Radiation-MagnetoHydrodynamics simulations of cosmic ray feedback in disc galaxies
• The origin of the enhanced metallicity of satellite galaxies
• Following The Cosmic Evolution Of Pristine Gas I: Implications For Milky Way Halo Stars
• Cosmological baryon transfer in the SIMBA simulations
• The Next Generation Virgo Cluster Survey (NGVS). XXIV. The Red Sequence to $\sim$10${}^6$ L${}_{\odot }$ and Comparisons with Galaxy Formation Models
• The combined effect of AGN and supernovae feedback in launching massive molecular outflows in high-redshift galaxies
• Barred galaxies in the Illustris-1 and TNG100 simulations
• Triggering Active Galactic Nuclei in galaxy clusters
• RAMSES-RTZ: Non-Equilibrium Metal Chemistry and Cooling Coupled to On-The-Fly Radiation Hydrodynamics
• The growth of brightest cluster galaxies in the TNG300 simulation:dissecting the contributions from mergers and in situ star formation
• The limited role of galaxy mergers in driving stellar mass growth over cosmic time
• Evaluating the ability of triaxial Schwarzschild modelling to estimate properties of galaxies from the Illustris simulation
• The high redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: Towards addressing the tension between observations and simulations
• NIHAO -- XXV. Convergence in the cusp-core transformation of cold dark matter haloes at high star formation thresholds
• Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
• The Morphology-Density relationship in 1<z<2 clusters
• Simulating the effect of high column density absorbers on the one-dimensional Lyman-alpha forest flux power spectrum
• Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
• VALES: I. The molecular gas content in star-forming dusty H-ATLAS galaxies up to z=0.35
• Large-scale jets from active galactic nuclei as a source of ICM heating: cavities and shocks
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - I: Bulge+disc decompositions, methods, and biases
• The effect of differential accretion on the Gravitational Wave Background and the present day MBH Binary population
• From Dark Matter to Galaxies with Convolutional Networks
• The first Super Massive Black Holes: indications from models for future observations
• Time Evolution of Galaxy Scaling Relations in Cosmological Simulations
• Is there enough star formation in simulated protoclusters?
• Galactic angular momentum in cosmological zoom-in simulations. I. Disk and bulge components and the galaxy--halo connection
• An alternate approach to measure specific star formation rates at 2<z<7
• Morphological signatures of mergers in the TNG50 simulation and the Kilo-Degree Survey: the merger fraction from dwarfs to Milky Way-like galaxies
• The descendants of the first quasars in the BlueTides simulation
• Cooling in a Dissipative Dark Sector
• The edge of galaxy formation II: evolution of Milky Way satellite analogues after infall
• The mass assembly of high-redshift black holes
• Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
• Dust Obscured Star Forming Galaxies in the Early Universe
• Cosmic filaments in galaxy cluster outskirts: quantifying finding filaments in redshift space
• A parametric study of possible solutions to the high-redshift overproduction of stars in modeled dwarf galaxies
• Accretion of Galaxy Groups into Galaxy Clusters
• Modeling for Stellar Feedback in Galaxy Formation Simulations
• Tracing galaxy populations through cosmic time: A critical test of methods for connecting the same galaxies between different redshifts at $z<3$
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• Gravitational Self-Lensing in Populations of Massive Black Hole Binaries
• The Angular Momentum of the Circumgalactic Medium in the TNG100 Simulation
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs
• Connecting the structure of dark matter haloes to the primordial power spectrum
• The vertical structure of gaseous galaxy discs in cold dark matter halos
• Passive galaxies in the early Universe: ALMA confirmation of z~3-5 candidates in the CANDELS GOODS-South field
• Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
• Stellar Dynamics and Star-Formation Histories of z $\sim$ 1 Radio-loud Galaxies
• The Grism lens-amplified survey from space (GLASS). VII. The diversity of the distribution of star formation in cluster and field galaxies at 0.3<z<0.7
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• Galaxies with prolate rotation in Illustris
• SDSS-IV MaNGA: Uncovering the Angular Momentum Content of Central and Satellite Early-type Galaxies
• Galactic outflow and diffuse gas properties at z>=1 using different baryonic feedback models
• The morphology and kinematics of the gaseous circumgalactic medium of Milky Way mass galaxies -- II. comparison of IllustrisTNG and Illustris simulation results
• Defining the (Black Hole)-Spheroid Connection with the Discovery of Morphology-Dependent Substructure in the $M_{\mathrm{BH}}$--${\mathrm{n}}_{\mathrm{sph}}$ and $M_{\mathrm{BH}}$--${\mathrm{R}}_{\mathrm{e},\mathrm{sph}}$ Diagrams: New Tests for Advanced Theories and Realistic Simulations
• On the Determination of Rotation Velocity and Dynamical Mass of Galaxies Based on Integrated H I Spectra
• North Ecliptic Pole merging galaxy catalogue
• The First Quiescent Galaxies in TNG300
• Formation and settling of a disc galaxy during the last 8 billion years in a cosmological simulation
• The stellar halo of the Milky Way traced by blue horizontal-branch stars in the Subaru Hyper Suprime-Cam Survey
• $R_{\mathrm{e}}$. I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population
• Simulating the effect of photoheating feedback during reionization
• Does the Milky Way Obey Spiral Galaxy Scaling Relations?
• UV to submillimetre luminosity functions of TNG50 galaxies
• Supernovae feedback propagation: the role of turbulence
• Barred spiral galaxies in modified gravity theories
• Deviations from tidal torque theory: evolution of the halo spin-filament alignment
• Rivers of Gas I.: Unveiling The Properties of High Redshift Filaments
• The Illustris Simulation: Supermassive Black Hole - Galaxy Connection Beyond the Bulge
• Abell 2744: Too much substructure for Lambda CDM?
• Gas flows in the circumgalactic medium around simulated high-redshift galaxies
• Black hole clustering and duty cycles in the Illustris simulation
• What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
• The dispersion measure of Fast Radio Bursts host galaxies: estimation from cosmological simulations
• SDSS-IV MaNGA: Internal mass distributions and orbital structures of early-type galaxies and their dependence on environment
• Galaxy And Mass Assembly (GAMA): Bulge-disk decomposition of KiDS data in the nearby universe
• The impact of ionised outflows from z$\sim$2.5 quasars is not through instantaneous in-situ quenching: the evidence from ALMA and VLT/SINFONI
• Testing the presence of multiple photometric components in nearby early-type galaxies using SDSS
• A tight relation between the age distributions of stellar clusters and the properties of the interstellar medium in the host galaxy
• Three-dimensional hydrodynamical simulations of the supernovae-driven gas loss in the dwarf spheroidal galaxy Ursa Minor
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• Reducing biases on $H_0$ measurements using strong lensing and galaxy dynamics: results from the EAGLE simulation
• Stacked star formation rate profiles of bursty galaxies exhibit 'coherent' star formation
• Numerical modelling of the lobes of radio galaxies in cluster environments -- IV. Remnant radio galaxies
• Renormalization-group flow of the effective action of cosmological large-scale structures
• Non-thermal radio supernova remnants of exiled Wolf-Rayet stars
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• The stellar populations of high-redshift dwarf galaxies
• Accurate initial conditions in mixed Dark Matter--Baryon simulations
• The effect of stellar and AGN feedback on the low redshift Lyman-$\alpha$ forest in the Sherwood simulation suite
• The fundamental metallicity relation emerges from the local anti-correlation between star formation rate and gas-phase metallicity existing in disk galaxies
• Nonparametric galaxy morphology from UV to submm wavelengths
• Are fossil groups early-forming galaxy systems?
• Stellar populations across the black hole mass - velocity dispersion relation
• The Three Hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies
• An improved probabilistic approach for linking progenitor and descendant galaxy populations using comoving number density
• Aging Halos: Implications of the Magnitude Gap on Conditional Statistics of Stellar and Gas Properties of Massive Halos
• Do AGN triggering mechanisms vary with radio power? I.Optical morphologies of radio-intermediate HERGs
• 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 SAMI galaxy survey: Galaxy Interactions and Kinematic Anomalies in Abell 119
• Predicting sub-millimeter flux densities from global galaxy properties
• Hot and counter-rotating star-forming disk galaxies in IllustrisTNG and their real-world counterparts
• Redshift evolution of the dark matter haloes shapes
• Star formation quenching imprinted on the internal structure of naked red nuggets
• Reconciling galaxy cluster shapes, measured by theorists vs observers
• Impact of Baryonic Physics on Intrinsic Alignments
• Testing Galaxy Quenching Theories with Scatter in the Stellar to Halo Mass Relation
• nIFTy galaxy cluster simulations V: Investigation of the Cluster Infall Region
• Simulation techniques for modified gravity
• Infrared luminosity functions and dust mass functions in the EAGLE simulation
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• Prospects for Recovering Galaxy Intrinsic Shapes from Projected Quantities
• The Dependence of Halo Mass on Galaxy Size at Fixed Stellar Mass Using Weak Lensing
• The clustering of $z>7$ galaxies: Predictions from the BLUETIDES simulation
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• A high baryon fraction in massive haloes at z~3
• Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
• Intermittent AGN episodes drive outflows with a large spread of observable loading factors
• The SAMI Galaxy Survey: Environmental analysis of the orbital structures of passive galaxies
• Galaxy properties in the cosmic web of EAGLE simulation
• Mapping Accreted Stars in Early-Type Galaxies Across the Mass-Size Plane
• The large-scale environment from cosmological simulations II: The redshift evolution and distributions of baryons
• AGN-driven quenching of satellite galaxies
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• The Three Hundred project: connection between star formation quenching and dynamical evolution in and around simulated galaxy clusters
• ETHOS - an effective theory of structure formation: formation of the first haloes and their stars
• Evolution of dwarf galaxies hosting GW150914-like events
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies
• The Effect of Environment on Milky Way-mass galaxies in a Constrained Simulation of the Local Group
• The cosmic spectral energy distribution in the EAGLE simulation
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• A Framework for Empirical Galaxy Phenomenology: The Scatter in Galaxy Ages and Stellar Metallicities
• The diversity of assembly histories leading to disc galaxy formation in a LambdaCDM model
• The morphology and kinematics of neutral hydrogen in the vicinity of z=0 galaxies with Milky Way masses -- a study with the Illustris simulation
• Do galaxies die? Different views from simulations and observations in the Local Universe
• On Mass Concentrations & Magnitude Gaps of Galaxy Systems in the CS82 Survey
• Modeling globular clusters in the TNG50 simulation: predictions from dwarfs to giants
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• A Moving Mesh Hydrodynamic Solver for ChaNGa
• The Smith Cloud: surviving a high speed transit of the Galactic disc
• Mufasa:The strength and evolution of galaxy conformity in various tracers
• Dark-ages Reionization & Galaxy Formation Simulation VIII. Suppressed growth of dark matter halos during the Epoch of Reionization
• Determining AGN luminosity histories using present-day outflow properties: a neural-network based approach
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• Colour gradients of low-redshift galaxies in the DESI Legacy Imaging Survey
• Probing the CGM of Low-redshift Dwarf Galaxies Using FIRE Simulations
• Galaxies with Shells in the Illustris Simulation: Metallicity Signatures
• Predicting fully self-consistent satellite richness, galaxy growth and starformation rates from the STastical sEmi-Empirical modeL STEEL
• Shedding light on low-mass subhalo survival and annihilation luminosity with numerical simulations
• A discrete chemo-dynamical model of M87's globular clusters: Kinematics extending to ~ 400 kpc
• Galaxy-lens determination of $H_0$: the effect of the ellipse+shear modeling assumption
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• Two channels for the formation of compact dwarf galaxies in clusters of galaxies
• SUPER VII. Morphology and kinematics of H$\alpha$ emission in AGN host galaxies at Cosmic noon using SINFONI
• The impact of black hole seeding in cosmological simulations
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• Time Dependent Radiation Hydrodynamics on a Moving Mesh
• Deep Extragalactic VIsible Legacy Survey (DEVILS): Evolution of the ${\sigma }_{\mathrm{SFR}}$-M${}_{\star }$ relation and implications for self-regulated star formation
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• The LEGA-C of nature and nurture in stellar populations of galaxies at z~0.6-1.0: D4000 and H-delta reveal different assembly histories for quiescent galaxies in different environments
• Small scale structures in coupled scalar field dark matter
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• A Precise Benchmark for Cluster Scaling Relations: Fundamental Plane, Mass Plane and IMF in the Coma Cluster from Dynamical Models
• Simplified galaxy formation with mesh-less hydrodynamics
• The impact of galaxy selection on the splashback boundaries of galaxy clusters
• The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• The effect of dark matter resolution on the collapse of baryons in high redshift numerical simulations
• The impact of mass map truncation on strong lensing simulations
• The Califa and Hipass velocity function for all morphological galaxy types
• Analysis of the galaxy size versus stellar mass relation
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Identifying the progenitors of present-day early-type galaxies in observational surveys: correcting `progenitor bias' using the Horizon-AGN simulation
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Do you see what I see? Exploring the consequences of luminosity limits in black hole-galaxy evolution studies
• Impact of H${}_2$-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
• Morphology and surface photometry of a sample of isolated early-type galaxies from deep imaging
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
• A Semi-Analytical Line Transfer (SALT) Model III: Galactic Inflows
• Saying Hallo to M94's Stellar Halo: Investigating the Accretion History of the Largest Pseudobulge Host in the Local Universe
• New dwarf galaxy candidates in the sphere of influence of the Local Volume spiral galaxy NGC2683
• How do galaxy properties affect void statistics?
• Uncovering Mass Segregation with Galaxy Analogues in Dark Matter Simulations
• Compact Galaxies at Intermediate Redshifts Quench Faster than Normal-sized Galaxies
• Active Galactic Nucleus Feedback in an Elliptical Galaxy with the Most Updated AGN Physics: Parameter Explorations
• Tilted outer and inner structures in edge-on galaxies?
• BUDHIES V: The baryonic Tully-Fisher relation at z=0.2 based on direct HI detections
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• Life after AGN switchoff: evolution and properties of fossil galactic outflows
• LyMAS reloaded: improving the predictions of the large-scale Lyman-α forest statistics from dark matter density and velocity fields
• Tracing Dark Matter Halos with Satellite Kinematics and the Central Stellar Velocity Dispersion of Galaxies
• Cosmological applications of the Brown-York quasilocal mass
• MARTINI: Mock Array Radio Telescope Interferometry of the Neutral ISM
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• From Galactic Chemical Evolution to Cosmic Supernova Rates Synchronized with Core-Collapse Supernovae Limited to the Narrow Progenitor Mass Range
• Anisotropic satellite accretion onto the Local Group with HESTIA
• Orbital pericenters and the inferred dark matter halo structure of satellite galaxies
• Jeans that fit: weighing the mass of the Milky Way analogues in the $\Lambda \mathrm{CDM}$ universe
• Reconciling Mass Functions with the Star-Forming Main Sequence Via Mergers
• The Star Formation and AGN luminosity relation: Predictions from a semi-analytical model
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• Modeling Nearly Spherical Pure-Bulge Galaxies with a Stellar Mass-to-Light Ratio Gradient under the $\Lambda$CDM and MOND Paradigms: II. The Orbital Anisotropy of Slow Rotators within the Effective Radius
• A study of the HI gas fractions of galaxies at z ~ 1
• A robust determination of halo environment in the cosmic field
• Cosmological Simulation of Galaxy Groups and Clusters-I: Global Effect of Feedback from Active Galactic Nuclei
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• An Absence of Radio-Loud Active Galactic Nuclei in Geometrically Flat Quiescent Galaxies: Implications for Maintenance-Mode Feedback Models
• Measuring Star-Formation Histories, Distances, and Metallicities with Pixel Color-Magnitude Diagrams I: Model Definition and Mock Tests
• Testing the SZ-based tomographic approach to the thermal history of the universe with pressure-density cross-correlations: Insights from the Magneticum simulation
• Formation and fate of low metallicity stars in IllustrisTNG50
• Galaxy flows within 8,000 km/s from Numerical Action methods
• Multiple stellar populations in Schwarzschild modeling and the application to the Fornax dwarf
• Star formation history and transition epoch of cluster galaxies based on the Horizon-AGN simulation
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
• Stellar Metallicity of Galaxies: New Insight on the Formation and Evolution of Low Surface Brightness Galaxies in the IllustrisTNG Simulation
• Real galaxy mergers from galaxy pair catalogs
• Star Formation in Massive Galaxies at Redshift $z\sim 0.5$
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies
• Measuring Star Formation Histories, Distances, and Metallicities with Pixel Color-Magnitude Diagrams II: Applications to Nearby Elliptical Galaxies
• What is the real accretion rate onto a black hole for low angular momentum accretion?
• Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
• Searching for the shadows of giants II: the effect of local ionisation on the Lyman-$\alpha$ absorption signatures of protoclusters at redshift $z\sim 2.4$
• IllustrisTNG Snapshots for 10 Gyr of Dynamical Evolution of Brightest Cluster Galaxies and Their Host Clusters
• The impact of the cosmological constant on past and future star formation
• Turbulence-induced deviation between baryonic field and dark matter field in the spatial distribution of the Universe
• Bursty star formation feedback and cooling outflows
• SCONCE: A cosmic web finder for spherical and conic geometries
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• Improving Black Hole Accretion Treatment in Hydrodynamical Simulations
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Haloes at the ragged edge: The importance of the splashback radius
• Revisiting the Relationship between the Long GRB Rate and Cosmic Star Formation History Based on a Large Swift Sample
• Substructure in the Globular Cluster Populations of the Virgo Cluster Elliptical Galaxies M84 and M86
• The Effect of Accretion Environment at Large Radius on Hot Accretion Flows
• Local Two-Sample Testing: A New Tool for Analysing High-Dimensional Astronomical Data
• Dark-ages reionization and galaxy formation simulation - IX. Economics of reionizing galaxies
• The MAGPI survey: The interdependence of the mass, star formation rate, and metallicity in galaxies at z~0.3
• Global Preventive Feedback of Powerful Radio Jets on Galaxy Formation
• An Escaping Outflow in a Galaxy with an Intermediate-mass Black Hole
• MOND implications for spectral line profiles of shell galaxies: shell formation history and mass-velocity scaling relations
• The fragility of thin discs in galaxies -- I. Building tailored N-body galaxy models
• Low-redshift quasars in the SDSS Stripe 82 II: associated companion galaxies and signature of star formation
• Domain adaptation techniques for improved cross-domain study of galaxy mergers
• Galactic Cosmic-Ray Induced Production of Lithium in the Small Magellanic Cloud
• Estimation of the Galaxy Quenching Rate in the Illustris Simulation
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• The OTELO survey: the star formation rate evolution of low-mass galaxies
• Efficiently estimating mean, uncertainty and unconstrained large scale fraction of local Universe simulations with paired fixed fields
• 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
• Galaxy-galaxy lensing in the VOICE deep survey
• The fate of the interstellar medium in early-type galaxies. IV. The impact of stellar feedback, mergers, and black holes on the cold ISM in simulated galaxies
• KiDS+VIKING+GAMA: Testing semi-analytic models of galaxy evolution with galaxy-galaxy-galaxy lensing
• Using Artificial Intelligence and real galaxy images to constrain parameters in galaxy formation simulations
• Structure and large scale environment of galaxy pairs in the S-PLUS DR4
• Does radiative feedback make faint z>6 galaxies look small?
• Evolution of dwarf galaxy observable parameters
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Sensitivity analysis of a galaxy formation model
• Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• Dark matter haloes: a multistream view
• Introduction to Tidal Streams
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• TODDLERS: A New UV to Millimeter Emission Library for Star-Forming Regions. II. Star Formation Rate Indicators Using Auriga Zoom Simulations
• Improving Performance of Zoom-In Cosmological Simulations using Initial Conditions with Customized Grids
• Core to Cosmic Edge: SIMBA-C's New Take on Abundance Profiles in the Intragroup Medium at z = 0
• Assembly Conformity of Structure Growth: Fossil versus Normal Groups of Galaxies
• Performance Enhancement of Tree-based Friends-of-friend Galaxy-finder for High-resolution Simulations of Galaxy Formation
• Exploring the evolution of a dwarf spheroidal galaxy with SPH simulations: I. Stellar feedback
• The origin of galaxy colour bimodality in the scatter of the Stellar-to-Halo Mass Relation
• Elliptical (E) and ellicular (ES) galaxies in the M_bh-M_*,sph diagram, and a merger-driven explanation for the origin of ES galaxies, anti-truncated stellar discs in lenticular galaxies, and the Sersicification of E galaxy light profiles
• Feedback from intermediate mass black holes on dwarf galaxy morphology at z=2
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• Virial models and Anisotropy of Velocity Dispersion in e-galaxies
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• The multi-component fitting to the star formation histories in the TNG simulation
• Disc instability and bar formation: view from the IllustrisTNG simulations
• The stability of galaxies in an expanding universe obtained by Newtonian dynamics
• How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
• DeepMerge: Classifying High-redshift Merging Galaxies with Deep Neural Networks
• Effect of cosmic rays and ionizing radiation on observational ultraviolet plasma diagnostics in the circumgalactic medium
• A hierarchical clustering method for quantifying satellite abundance
• A novel analysis of contamination in Lyman-break galaxy samples at $\mathbf{z}\sim 6-8$: spatial correlation with intermediate-redshift galaxies at $\mathbf{z}\sim 1.3-2$
• Radio Galaxies in SIMBA: A MIGHTEE Comparison
• Gas flows in galaxy mergers: supersonic turbulence in bridges, accretion from the circumgalactic medium, and metallicity dilution
• Wind accretion onto compact objects
• Reconciling concentration to virial mass relations
• Lack of influence of the environment in the earliest stages of massive galaxy formation
• A Simulation Driven Deep Learning Approach for Separating Mergers and Star Forming Galaxies: The Formation Histories of Clumpy Galaxies in all the CANDELS Fields
• Yellow Post-Asymptotic-Giant-Branch Stars as Standard Candles. I. Calibration of the Luminosity Function in Galactic Globular Clusters
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG
• The impact of black hole feedback on the UV luminosity and stellar mass assembly of high-redshift galaxies
• Observed structural parameters of EAGLE galaxies: reconciling the mass-size relation in simulations with local observations
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• Review on Dark Matter Tools
• Boosting (In)direct Detection of Dark Matter
• The link between star formation and gas in nearby galaxies