Properties of galaxies reproduced by a hydrodynamic simulation

Abstract

Previous simulations of the growth of cosmic structures have broadly reproduced the 'cosmic web' of galaxies that we see in the Universe, but failed to create a mixed population of elliptical and spiral galaxies due to numerical inaccuracies and incomplete physical models. Moreover, because of computational constraints, they were unable to track the small scale evolution of gas and stars to the present epoch within a representative portion of the Universe. Here we report a simulation that starts 12 million years after the Big Bang, and traces 13 billion years of cosmic evolution with 12 billion resolution elements in a volume of $(106.5\mathrm{Mpc}{)}^3$. It yields a reasonable population of ellipticals and spirals, reproduces the distribution of galaxies in clusters and statistics of hydrogen on large scales, and at the same time the metal and hydrogen content of galaxies on small scales.

arXiv comment32 pages, 5 figures, Nature Article (May 8, 2014). The official Illustris website can be found at http://www.illustris-project.org

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• Mg II Absorption at 2<z<7 with Magellan/FIRE, III. Full Statistics of Absorption Towards 100 High-Redshift QSOs
• Rotation curve fitting and its fatal attraction to cores in realistically simulated galaxy observations
• The Redshift Evolution of the $M_{\bullet }-M_{\star }$ Relation for JWST's Supermassive Black Holes at $z>4$
• A flexible subhalo abundance matching model for galaxy clustering in redshift space
• Assessing the Jeans Anisotropic Multi-Gaussian Expansion method with the Illustris simulation
• 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
• Subhalo Demographics in the Illustris Simulation: Effects of Baryons and Halo-to-Halo Variation
• The massive relic galaxy NGC 1277 is dark matter deficient. From dynamical models of integral-field stellar kinematics out to five effective radii
• Dust in and around galaxies: dust in cluster environments and its impact on gas cooling
• Long-term FRII jet evolution: Clues from three-dimensional simulations
• The origin and properties of massive prolate galaxies in the Illustris simulation
• The Shapes of the Rotation Curves of Star-forming Galaxies Over the Last $\approx$10 Gyr
• Observational signatures of a warped disk associated with cold-flow accretion
• The Impact of Star Formation Histories on Stellar Mass Estimation: Implications from the Local Group Dwarf Galaxies
• Spin-driven jet feedback in idealised simulations of galaxy groups and clusters
• Stellar Halos in Illustris- Probing the Histories of Milky Way-Mass Galaxies
• Cosmological direct detection of dark energy: non-linear structure formation signatures of dark energy scattering with visible matter
• Simultaneous modelling of matter power spectrum and bispectrum in the presence of baryons
• Physical drivers of galaxies' cold-gas content: exploring environmental and evolutionary effects with DARK SAGE
• On the model of the circumgalactic mist: the implications of cloud sizes in galactic winds and halos
• Estimating the Mass of the Milky Way Using the Ensemble of Classical Satellite Galaxies
• Bounding Alternative Theories of Gravity with Multi-Band GW Observations
• Realistic simulations of galaxy formation in f(R) modified gravity
• Orbits of massive satellite galaxies: II. Bayesian Estimates of the Milky Way and Andromeda masses using high precision astrometry and cosmological simulations
• A missing outskirts problem? Comparisons between stellar halos in the Dragonfly Nearby Galaxies Survey and the TNG100 simulation
• The structure and assembly history of cluster-size haloes in Self-Interacting Dark Matter
• 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
• Stellar Feedback and Resolved Stellar IFU Spectroscopy in the nearby Spiral Galaxy NGC 300
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• A Census of Sub-kiloparsec Resolution Metallicity Gradients in Star-forming Galaxies at Cosmic Noon from HST Slitless Spectroscopy
• Black-hole remnants from black-hole--neutron-star mergers
• The splashback boundary of haloes in hydrodynamic simulations
• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• The central densities of Milky Way-mass galaxies in cold and self-interacting dark matter models
• Introducing CGOLS: The Cholla Galactic OutfLow Simulation Suite
• Testing the effect of galactic feedback on the IGM at z ~ 6 with metal-line absorbers
• Baryonic effects on the matter bispectrum
• The missing light of the Hubble Ultra Deep Field
• Convergence of Lobatto-type Runge-Kutta methods for partitioned differential-algebraic systems of index 2
• A moving mesh unstaggered constrained transport scheme for magnetohydrodynamics
• Morpho-kinematics of z~1 galaxies probe the hierarchical scenario
• A study of the circum-galactic medium at z ~ 0.6 using DLA-galaxies
• Modeling Galactic Conformity with the Color-Halo Age Relation in the Illustris Simulation
• Osaka Feedback Model: Isolated Disk Galaxy Simulations
• Alignment between filaments and galaxy spins from the MaNGA integral-field survey
• ETHOS -- an effective theory of structure formation: predictions for the high-redshift Universe -- abundance of galaxies and reionization
• Morphological decomposition of TNG50 galaxies: methodology and catalogue
• Increasing blackhole feedback induced quenching with anisotropic thermal conduction
• Composite Spectral Energy Distributions and Infrared-Optical Colors of Type 1 and Type 2 Quasars
• The host galaxies of double compact objects merging in the local Universe
• Time Delay Lens Modelling Challenge
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• The manifestation of secondary halo bias on the galaxy population from IllustrisTNG300
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• First Gaia dynamical model of the Milky Way disc with six phase space coordinates: a test for galaxy dynamics
• Origin of the galaxy HI size-mass relation
• Near-Field Limits on the Role of Faint Galaxies in Cosmic Reionization
• Strong-lensing Measurement of the Mass-density Profile out to 3 Effective Radii for $z\sim 0.5$ Early-type Galaxies
• Diffuse gas properties and stellar metallicities in cosmological simulations of disc galaxy formation
• Formation of a Malin 1 analogue in IllustrisTNG by stimulated accretion
• Kinematic decomposition of IllustrisTNG disk galaxies: morphology and relation with morphological structures
• On the influence of halo mass accretion history on galaxy properties and assembly bias
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Characterizing the local relation between star formation rate and gas-phase metallicity in MaNGA spiral galaxies
• Imprints of temperature fluctuations on the $z\sim 5$ Lyman-$\alpha$ forest: a view from radiation-hydrodynamic simulations of reionization
• The Formation of Supermassive Black Holes from Population III.1 Seeds. I. Cosmic Formation Histories and Clustering Properties
• Diagnosing galactic feedback with the line broadening in the low redshift Lyman-alpha forest
• Solitons in the dark: non-linear structure formation with fuzzy dark matter
• Signatures of stellar accretion in MaNGA early-type galaxies
• The effects of subgrid models on the properties of giant molecular clouds in galaxy formation simulations
• Gravitational Lensing and the Power Spectrum of Dark Matter Substructure: Insights from the ETHOS N-body Simulations
• The Void Galaxy Survey: Photometry, structure and identity of void galaxies
• Galaxies lacking dark matter in the Illustris simulation
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• Stellar Property Statistics of Massive Halos from Cosmological Hydrodynamics Simulations: Common Kernel Shapes
• The H-alpha luminosity-dependent clustering of star-forming galaxies from z~0.8 to z~2.2 with HiZELS
• The star clusters that make black hole binaries across cosmic time
• The Growth and Enrichment of the Intragroup Gas
• Efficacy of early stellar feedback in low gas surface density environments
• Properties of Cosmological Filaments extracted from Eulerian Simulations
• Prospects for Future Binary Black Hole GW Studies in Light of PTA Measurements
• Discrepancies between CFHTLenS cosmic shear & Planck: new physics or systematic effects?
• The growth of brightest cluster galaxies in the TNG300 simulation:dissecting the contributions from mergers and in situ star formation
• Baryons in the CosmicWeb of IllustrisTNG -- II: the Connection among Galaxies, Halos, their Formation Time and their Location in the Cosmic Web
• Identifying kinematic structures in simulated galaxies using unsupervised machine learning
• Illustrating galaxy-halo connection in the DESI era with IllustrisTNG
• Characterizing hydrostatic mass bias with Mock-X
• Evaluating the ability of triaxial Schwarzschild modelling to estimate properties of galaxies from the Illustris simulation
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• Determining star-formation rates in Active Galactic Nuclei hosts via stellar population synthesis
• Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
• Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
• Simulating the effect of high column density absorbers on the one-dimensional Lyman-alpha forest flux power spectrum
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• Realistic estimation for the detectability of dark matter sub-halos with Fermi-LAT
• HST grism spectroscopy of z~3 massive quiescent galaxies: Approaching the metamorphosis
• BASS XXXI: Outflow scaling relations in low redshift X-ray AGN host galaxies with MUSE
• Dark matter stripping in galaxy clusters: a look at the Stellar to Halo Mass relation in the Illustris simulation
• 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
• Marked clustering statistics in $f(R)$ gravity cosmologies
• Correlations Between Black Holes and Host Galaxies in the Illustris and IllustrisTNG Simulations
• Submillimetre galaxies in cosmological hydrodynamical simulations -- an opportunity for constraining feedback models
• The first Super Massive Black Holes: indications from models for future observations
• From Dark Matter to Galaxies with Convolutional Networks
• The Lopsidedness of Satellite Galaxy Systems in $\Lambda$CDM simulations
• Is there enough star formation in simulated protoclusters?
• Kinematics and Dynamics of Multiphase Outflows in Simulations of the Star-Forming Galactic ISM
• ERGO-ML I: Inferring the assembly histories of IllustrisTNG galaxies from integral observable properties via invertible neural networks
• $\kappa$TNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations
• The Mass Profile of the Milky Way to the Virial Radius from the Illustris Simulation
• Updated Results on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• nIFTY galaxy cluster simulations III: The Similarity & Diversity of Galaxies & Subhaloes
• Tidally induced warps of spiral galaxies in IllustrisTNG
• Climbing Halo Merger Trees with TreeFrog
• An alternate approach to measure specific star formation rates at 2<z<7
• Connecting the dots: a correlation between ionising radiation and cloud mass-loss rate traced by optical integral field spectroscopy
• Morphological signatures of mergers in the TNG50 simulation and the Kilo-Degree Survey: the merger fraction from dwarfs to Milky Way-like galaxies
• Co-orbiting planes of sub-halos are similarly unlikely around paired and isolated hosts
• The modified gravity lightcone simulation project I: Statistics of matter and halo distributions
• GRAMSES: a new route to general relativistic $N$-body simulations in cosmology. Part I. Methodology and code description
• Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass
• Relativistic numerical cosmology with Silent Universes
• The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?
• Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
• Shock finding on a moving-mesh: II. Hydrodynamic shocks in the Illustris universe
• The history of the dark and luminous side of Milky Way-like progenitors
• The Radial Acceleration Relation in Disk Galaxies in the MassiveBlack-II Simulation
• Hydrodynamic Effects in the Symmetron and $f(R)$-gravity Models
• Cooling in a Dissipative Dark Sector
• A redshift-dependent IRX-$\beta$ dust attenuation relation for TNG50 galaxies
• Active galactic nucleus jet feedback in hydrostatic halos
• Response Approach to the Matter Power Spectrum Covariance
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• SDSS--IV MaNGA : The Inner Density Slopes of nearby galaxies
• Gravitational Self-Lensing in Populations of Massive Black Hole Binaries
• How Environment Affects Galaxy Metallicity through Stripping and Formation History: Lessons from the Illustris Simulation
• Accretion of Galaxy Groups into Galaxy Clusters
• The Angular Momentum of the Circumgalactic Medium in the TNG100 Simulation
• Probing Dark Matter Self-interaction with Ultra-faint Dwarf Galaxies
• The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• Globular clusters as tracers of the dark matter content of dwarfs in galaxy clusters
• The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs
• The Close AGN Reference Survey (CARS): IFU survey data and the BH mass dependence of long-term AGN variability
• The impact of magnetic fields on cosmological galaxy mergers. I: Reshaping gas and stellar discs
• Galaxy formation in the brane world I: overview and first results
• Dark matter dynamics in Abell 3827: new data consistent with standard Cold Dark Matter
• Systematic errors in the measurement of neutrino masses due to baryonic feedback processes: Prospects for stage IV lensing surveys
• The MillenniumTNG Project: Intrinsic alignments of galaxies and halos
• Galaxy formation in the PLANCK cosmology - III. The high-redshift universe
• Testing the Accuracy of Halo Occupation Distribution Modelling using Hydrodynamic Simulations
• The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• Properties and Origin of Galaxy Velocity Bias in the Illustris Simulation
• Correlations in the three-dimensional Lyman-alpha forest contaminated by high column density absorbers
• A gradient based method for modeling baryons and matter in halos of fast simulations
• Similar Scaling Relations for the Gas Content of Galaxies across Environments to z ~ 3.5
• The Contribution of In-situ and Ex-situ Star Formation in Early-Type Galaxies: MaNGA versus IllustrisTNG
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• Predicting star formation properties of galaxies using deep learning
• A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
• The host galaxies of double compact objects across cosmic time
• Galaxies with prolate rotation in Illustris
• Non-parametric Morphologies of Galaxies in the EAGLE Simulation
• Formation of massive disk galaxies in the IllustrisTNG simulation
• A Comparison of Circumgalactic MgII Absorption between the TNG50 Simulation and the MEGAFLOW Survey
• The Evolutionary Pathways of Disk-, Bulge-, and Halo-dominated Galaxies
• The Effect Of AGN Heating On The Low-Redshift Lyα Forest
• Identification of filamentary structures in the environment of superclusters of galaxies in the Local Universe
• The morphology and kinematics of the gaseous circumgalactic medium of Milky Way mass galaxies -- II. comparison of IllustrisTNG and Illustris simulation results
• The combined and respective roles of imaging and stellar kinematics in identifying galaxy merger remnants
• $5\sigma$ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond $\Lambda$CDM
• Dynamical model of the Milky Way using APOGEE and Gaia data
• Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at $z\ge 10$?
• Constraining self-interacting dark matter with scaling laws of observed halo surface densities
• Probing sub-galactic mass structure with the power spectrum of surface-brightness anomalies in high-resolution observations of galaxy-galaxy strong gravitational lenses. II.Observational constraints on the sub-galactic matter power spectrum
• Dust entrainment in galactic winds
• Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction
• The formation of low surface brightness galaxies in the IllustrisTNG simulation
• Galaxy assembly bias of central galaxies in the Illustris simulation
• Formation of Globular Cluster Systems II: Impact of the Cutoff of the Cluster Initial Mass Function
• Tidal destruction in a low mass galaxy environment: the discovery of tidal tails around DDO 44
• Regulation of Star Formation by a Hot Circumgalactic Medium
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• Reaching for the Edge I: Probing the Outskirts of Massive Galaxies with HSC, DECaLS, SDSS, and Dragonfly
• What it Takes to Measure Reionization with Fast Radio Bursts
• The First Quiescent Galaxies in TNG300
• The stellar halo of the Milky Way traced by blue horizontal-branch stars in the Subaru Hyper Suprime-Cam Survey
• Simulating the effect of photoheating feedback during reionization
• Forward and backward galaxy evolution in comoving number density space
• The Close AGN Reference Survey (CARS): No obvious signature of AGN feedback on star formation, but subtle trends
• Direct Detection of Mirror Matter in Twin Higgs Models
• Probing the $z\gtrsim 6$ quasars in a universe with IllustrisTNG physics: Impact of gas-based black hole seeding models
• The impact of galactic feedback on the shapes of dark-matter haloes
• 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
• The Missing Satellite Problem in 3D
• On the relative effect of nodes and filaments of the cosmic web on the quenching of galaxies and the orientation of their spin
• UV to submillimetre luminosity functions of TNG50 galaxies
• Cosmological simulations of massive black hole seeds: predictions for next generation electromagnetic and gravitational wave observations
• Discriminating Topology in Galaxy Distributions using Network Analysis
• On the formation of massive quiescent galaxies with diverse morphologies in the TNG50 simulation
• $\Lambda$CDM Predictions for the Satellite Population of M33
• The abundance of compact quiescent galaxies since z ~ 0.6
• DM halo morphological types of MW-like galaxies in the TNG50 simulation: Simple, Twisted, or Stretched
• The impact of AGN-driven winds on physical and observable galaxy sizes
• What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
• Flattened structures of dwarf satellites around massive host galaxies in the MATLAS low-to-moderate density fields
• Black hole clustering and duty cycles in the Illustris simulation
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• The impact of Lyman-$\alpha$ radiative transfer on large-scale clustering in the Illustris simulation
• Weak lensing in the Horizon-AGN simulation lightcone. Small scale baryonic effects
• Gas Accretion Can Drive Turbulence in Galaxies
• Evolution of CIV Absorbers I. The Cosmic Incidence
• The Local Group: The Ultimate Deep Field
• The Active Assembly of the Virgo Cluster: Indications for Recent Group Infall From Early-Type Dwarf Galaxies
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• The SZ flux-mass ($Y$-$M$) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback
• Mapping the stellar population and gas excitation of MaNGA galaxies with MEGACUBES. Results for AGN versus control sample
• The impact of AGN on stellar kinematics and orbits in simulated massive galaxies
• History and destiny of an emerging early-type galaxy: New IFU insights on the major-merger remnant NGC7252
• PRIYA: A New Suite of Lyman-alpha Forest Simulations for Cosmology
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• SDSS-IV MaNGA: Internal mass distributions and orbital structures of early-type galaxies and their dependence on environment
• Cosmological insights into the assembly of the radial and compact stellar halo of the Milky Way
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• The impact of baryonic physics on the abundance, clustering, and concentration of halos
• Super-Eddington growth of black holes in the early Universe: effects of disk radiation spectra
• Fast Generation of Covariance Matrices for Weak Lensing
• The MillenniumTNG Project: The large-scale clustering of galaxies
• On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• SMART: A new implementation of Schwarzschild's Orbit Superposition technique for triaxial galaxies and its application to an N-body merger simulation
• Towards an improved model of self-interacting dark matter haloes
• Mass-concentration relation of clusters of galaxies from CFHTLenS
• Gemini NIFS survey of feeding and feedback processes in nearby Active Galaxies: VI -- Stellar Populations
• Associating Host Galaxy Candidates to Massive Black Hole Binaries resolved by Pulsar Timing Arrays
• VIS3COS: I. survey overview and the role of environment and stellar mass on star formation
• Compound lensing: Einstein Zig-Zags and high multiplicity lensed images
• The origin of the relation between metallicity and size in star-forming galaxies
• Evolution of galaxy groups in the Illustris simulation
• Simba: The average properties of the circumgalactic medium of $2\le z\le 3$ quasars are determined primarily by stellar feedback
• Simulating galaxy formation in f(R) modified gravity: Matter, halo, and galaxy-statistics
• No Tension: JWST Galaxies at $z>10$ Consistent with Cosmological Simulations
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
• On the detection and precise localisation of merging black holes events through strong gravitational lensing
• The Impact of baryonic physics on the kinetic Sunyaev-Zel'dovich Effect
• Modeling the kinematics of globular cluster systems
• Constraints on AGN feedback from its Sunyaev-Zel'dovich imprint on the cosmic background radiation
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• The Very Knotty Lenser: exploring the role of regularization in source and potential reconstructions using Gaussian Process Regression
• Cosmic Shear as a Probe of Galaxy Formation Physics
• A General Precipitation-Limited L_X-T-R Relation Among Early-Type Galaxies
• SHAM through the lens of a hydrodynamical simulation
• Dark-matter-deficient galaxies in hydrodynamical simulations
• A Fundamental Test for Galaxy Formation Models: Matching the Lyman-$\alpha$ Absorption Profiles of Galactic Halos over Three Decades in Distance
• Towards robust determination of non-parametric morphologies in marginal astronomical data: resolving uncertainties with cosmological hydrodynamical simulations
• Galaxy Zoo: Morphological classification of galaxy images from the Illustris simulation
• KURVS: The outer rotation curve shapes and dark matter fractions of $z\sim 1.5$ star-forming galaxies
• An improved probabilistic approach for linking progenitor and descendant galaxy populations using comoving number density
• Large Scale Structures in COSMOS2020: Evolution of Star Formation Activity in Different Environments at 0.4 < z < 4
• The stellar mass - size relation for cluster galaxies at z=1 with high angular resolution from the Gemini/GeMS multi-conjugate adaptive optics system
• Hot and counter-rotating star-forming disk galaxies in IllustrisTNG and their real-world counterparts
• A general framework to test gravity using galaxy clusters IV: Cluster and halo properties in DGP gravity
• Redshift evolution of the dark matter haloes shapes
• The THESAN project: connecting ionized bubble sizes to their local environments during the Epoch of Reionization
• Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
• The Quasar Feedback Survey: Revealing the Interplay of Jets, Winds & Emission Line Gas in Type 2 Quasars with Radio Polarization
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs. I. Construction and analysis of the mock data cubes
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• REQUIEM-2D: Spatially Resolved Stellar Populations from HST 2D Grism Spectroscopy
• SimSpin -- Constructing mock IFS kinematic data cubes
• HELP : The Herschel Extragalactic Legacy Project & The Coming of Age of Multi-Wavelength Astrophysics
• Spherical Cows in Dark Matter Indirect Detection
• Considerations for the Observability of Kinematically Offset Binary AGN
• Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
• Giant Lyman-Alpha Nebulae in the Illustris Simulation
• The Cosmic Microwave Background and the Stellar Initial Mass Function
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• Impact of Baryonic Physics on Intrinsic Alignments
• Redshift Evolution of the Fundamental Plane Relation in the IllustrisTNG Simulation
• Prospects for Recovering Galaxy Intrinsic Shapes from Projected Quantities
• The Supersonic Project: rotational effects of supersonic motions on the first structures in the Universe
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• What Are Those Tiny Things? A First Study of Compact Star Clusters in the SMACS0723 Field with JWST
• TARDIS Paper II: Synergistic Density Reconstruction from Lyman-alpha Forest and Spectroscopic Galaxy Surveys with Applications to Protoclusters and the Cosmic Web
• The impact of $\Lambda$CDM substructure and baryon-dark matter transition on the image positions of quad galaxy lenses
• The Dependence of Halo Mass on Galaxy Size at Fixed Stellar Mass Using Weak Lensing
• The moving mesh code Shadowfax
• A black box for dark sector physics: Predicting dark matter annihilation feedback with conditional GANs
• Baryonic effects on CMB lensing and neutrino mass constraints
• Modeling multi-phase gases in cosmological simulations using compressible multi-fluid hydrodynamics
• A Local Leaky-box Model for the Local Stellar Surface Density - Gas Surface Density - Gas Phase Metallicity Relation
• The assembly of spheroid-dominated galaxies in the EAGLE simulation
• REQUIEM-2D: A diversity of formation pathways in a sample of spatially-resolved massive quiescent galaxies at z~2
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• Mapping Accreted Stars in Early-Type Galaxies Across the Mass-Size Plane
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• Hydrodynamical structure formation in Milgromian cosmology
• Investigating Cosmological GAN Emulators Using Latent Space Interpolation
• AGN and Dwarf Galaxy Gas Kinematics
• Quantifying substructures in {\it Hubble Frontier Field} clusters: comparison with $\Lambda CDM$ simulations
• HI galaxies with little star formation: an abundance of LIERs
• Galaxy And Mass Assembly (GAMA): 'No Smoking' zone for giant elliptical galaxies?
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• Exploring the Cosmic Evolution of Habitability with Galaxy Merger Trees
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• ETHOS - an effective theory of structure formation: formation of the first haloes and their stars
• Does jackknife scale really matter for accurate large-scale structure covariances?
• Local Group timing argument and virial theorem mass estimators from cosmological simulations
• Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
• Simulating the Carbon Footprint of Galactic Halos
• Constraints on self-interacting Bose-Einstein condensate dark matter using large-scale observables
• Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies
• Radiative Transfer Distortions of Lyman-$\alpha$ Emitters: a New Fingers-of-God Damping in the Clustering in Redshift Space
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• The evolution of the baryon fraction in halos as a cause of scatter in the galaxy stellar mass in the EAGLE simulation
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• Resolving Disks & Mergers in $z\sim 2$ Heavily Reddened Quasars and their Companion Galaxies with ALMA
• Dark matter substructures affect dark matter-electron scattering in xenon-based direct detection experiments
• Spatial distribution of dark matter in and around galaxy clusters traced by galaxies, gas and intracluster stars in a simulated universe
• Realistic synthetic integral field spectroscopy with RealSim-IFS
• Identifying galaxy candidates in WSRT HI imaging of ultra-compact high velocity clouds
• The Case for Strangulation in Low-Mass Hosts: DDO 113
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• ALMA [N ıı] 205 μm Imaging Spectroscopy of the Lensed Submillimeter galaxy ID 141 at redshift 4.24
• Group-scale intrinsic galaxy alignments in the Illustris-TNG and MassiveBlack-II simulations
• Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
• Modeling globular clusters in the TNG50 simulation: predictions from dwarfs to giants
• Evolution of the Stellar Mass Function and Infrared Luminosity Function of Galaxies since $z=1.2$
• The IllustrisTNG Simulations: Public Data Release
• On the dearth of ultra-faint extremely metal poor galaxies
• Dark-ages Reionization & Galaxy Formation Simulation VIII. Suppressed growth of dark matter halos during the Epoch of Reionization
• Probing the CGM of Low-redshift Dwarf Galaxies Using FIRE Simulations
• Cosmological simulations of self-interacting Bose-Einstein condensate dark matter
• Dynamical friction in Bose-Einstein condensed self-interacting dark matter at finite temperatures, and the Fornax dwarf spheroidal
• Galaxies with Shells in the Illustris Simulation: Metallicity Signatures
• Backlighting extended gas halos around luminous red galaxies: kinematic Sunyaev-Zel'dovich effect from DESI Y1 x ACT
• 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
• DS+: a method for the identification of cluster substructures
• The building up of observed stellar scaling relations of massive galaxies and the connection to black hole growth in the TNG50 simulation
• There and back again: understanding the critical properties of backsplash galaxies
• Interacting galaxies in the IllustrisTNG simulations -- V: Comparing the influence of star-forming vs. passive companions
• Galaxy merger challenge: A comparison study between machine learning-based detection methods
• Network Analysis of Cosmic Structures : Network Centrality and Topological Environment
• The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Quenching of Massive Disk Galaxies in the IllustrisTNG Simulation
• The number of dwarf satellites of disk galaxies versus their bulge mass in the standard model of cosmology
• Small scale structures in coupled scalar field dark matter
• ART${}^2$: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines
• Inferring the Morphology of Stellar Distribution in TNG50: Twisted and Twisted-Stretched shapes
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• Gravitational lensing in LoTSS DR2 -- Extremely faint 144-MHz radio emission from two highly magnified quasars
• Nonparametric galaxy morphology from stellar and nebular emission with the CALIFA sample
• The evolutionary pathways of disk galaxies with different sizes
• Simulating the LOcal Web (SLOW) II: Properties of local galaxy clusters
• Galactic coronae in Milky Way-like galaxies: the role of stellar feedback in gas accretion
• Spectro-Imaging Forward Model of Red and Blue Galaxies
• On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias
• Unveiling the origins of galactic bars: insights from barred and unbarred galaxies
• Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
• One star, two stars, or both? Investigating metallicity-dependant models for Gamma-Ray Burst progenitors with the IllustrisTNG simulation
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• Massive spheroids can form in single minor mergers
• Detection of the self-regulation of star formation in galaxy discs
• Constraints on small-scale cosmological fluctuations from SNe lensing dispersion
• Local and global gas metallicity versus stellar age relation in MaNGA galaxies
• Testing galaxy formation models with galaxy stellar mass functions
• The Califa and Hipass velocity function for all morphological galaxy types
• Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• The metallicity and star formation activity of long gamma-ray burst hosts for z$<$3: insights from the Illustris simulation
• Non-parametric Morphologies of Mergers in the Illustris Simulation
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• Merger Histories and Environments of Dwarf AGN in IllustrisTNG
• The impact of mass map truncation on strong lensing simulations
• On the complexity and the information content of cosmic structures
• The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
• Active galactic nuclei jets simulated with smoothed particle hydrodynamics
• The impact of magnetic fields on cosmological galaxy mergers -- II. Modified angular momentum transport and feedback
• Planting a Lyman alpha forest on AbacusSummit
• The THESAN-ZOOM project: Population III star formation continues until the end of reionization
• Little Red Dots as Direct-collapse Black Hole Nurseries
• The Co-Evolution of a Magnetized Intracluster Medium and Hot Galactic Coronae: Magnetic Field Amplification and Turbulence Generation
• Void Galaxy Distribution: A Challenge for $\Lambda$CDM
• Morphology and surface photometry of a sample of isolated early-type galaxies from deep imaging
• Luminosity function of [OII] emission-line galaxies in the MassiveBlack-II simulation
• Do satellite galaxies trace matter in galaxy clusters?
• Saying Hallo to M94's Stellar Halo: Investigating the Accretion History of the Largest Pseudobulge Host in the Local Universe
• The parallelism between galaxy clusters and early-type galaxies: I. The light and mass profiles
• Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
• Using GAMA to probe the impact of small-scale galaxy physics on nonlinear redshift-space distortions
• The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
• Evolution of Starburst Galaxies in the Illustris Simulation
• Sloshing of Galaxy Cluster Core Plasma in the Presence of Self-Interacting Dark Matter
• Very Large Array observations of the mini-halo and AGN feedback in the Phoenix cluster
• IllustrisTNG Insights: Factors Affecting the Presence of Bars in Disk Galaxies
• Constraining SN feedback: a tug of war between reionization and the Milky Way satellites
• Galaxies with kinematically distinct cores in Illustris
• Extreme Spheres: Counts-in-cells for 21cm intensity mapping
• A tale of two tails: insights from simulations into the formation of the peculiar dwarf galaxy NGC 1427A
• How do galaxy properties affect void statistics?
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• Impact of tidal environment on galaxy clustering in GAMA
• Cosmological applications of the Brown-York quasilocal mass
• Imprint of baryons and massive neutrinos on velocity statistics
• Neural Stellar Population Synthesis Emulator for the DESI PROVABGS
• A [C II] 158$\mu$m Emitter Associated with an OI Absorber at the End of the Reionization Epoch
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• The space density distribution of galaxies in the absolute magnitude - rotation velocity plane: a volume-complete Tully-Fisher relation from CALIFA stellar kinematics
• Anisotropic satellite accretion onto the Local Group with HESTIA
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman-$\alpha$ Forest Tomography at $z=2$
• On the Cosmic Evolution of Fe/Mg in QSO Absorption Line Systems
• The parallelism between galaxy clusters and early-type galaxies: III. The Mass-Radius Relationship
• The local dark matter distribution in self-interacting dark matter halos
• 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
• Connecting Primordial Star Forming Regions and Second Generation Star Formation in the Phoenix Simulations
• The Large-scale Effect of Environment on Galactic Conformity
• A novel approach to investigate chemical inhomogeneities in GRB host galaxies: The $Z_{\mathrm{abs}}-Z_{\mathrm{emiss}}$ relation
• Emergent Hydrodynamic Mode on SU(2) Plaquette Chains and Quantum Simulation
• The thermal and gravitational energy densities in the large-scale structure of the Universe
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• Mock Galaxy Surveys for HST and JWST from the IllustrisTNG Simulations
• Simultaneous Dependence of Matter Clustering on Scale and Environment
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• Statistics of Two-point Correlation and Network Topology for Lyman Alpha Emitters at $z\approx 2.67$
• Dark against luminous matter around isolated central galaxies: a comparative study between modern surveys and Illustris-TNG
• Discord in Concordance Cosmology and Anomalously Massive Early Galaxies
• Formation and fate of low metallicity stars in IllustrisTNG50
• Reconciling Volumetric and Individual Galaxy Type Ia Supernova Rates
• Multiple stellar populations in Schwarzschild modeling and the application to the Fornax dwarf
• Detecting preheating in proto-clusters with Lyman-$\alpha$ Forest Tomography
• The Supersonic Project: The eccentricity and rotational support of SIGOs and DM GHOSts
• The Magellanic Clouds are very rare in the IllustrisTNG simulations
• Implications of galaxy buildup for putative IMF variations in massive galaxies
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• The Supersonic Project: The Early Evolutionary Path of SIGOs
• Cosmological Simulation of Galaxy Groups and Clusters-I: Global Effect of Feedback from Active Galactic Nuclei
• Addressing via N-body simulations the distribution of the satellite tidal debris in the Milky Way environment
• Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
• Hydrodynamic Attractor in Ultracold Atoms
• PAC.V. The Roles of Mass and Environment in the Quenching of Galaxies
• Gravitational Wave Peeps from EMRIs and their Implication for LISA Signal Confusion Noise
• The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
• High-redshift test of gravity using enhanced growth of small structures probed by the neutral hydrogen distribution
• Smooth stochastic density field reconstruction
• Star Formation in Massive Galaxies at Redshift $z\sim 0.5$
• Comparing galaxy morphology in hydrodynamical simulation and in semi-analytic model
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• Black Hole Weather Forecasting with Deep Learning: A Pilot Study
• Resolved star formation in TNG100 central and satellite galaxies
• A general framework to test gravity using galaxy clusters V: A self-consistent pipeline for unbiased constraints of $f(R)$ gravity
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• Mass-morphology relation of TNG50 galaxies
• The Dark Matter Halos of HI Selected Galaxies
• The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• The four cosmic tidal web elements from the $\beta$-skeleton
• The Direct-Method Oxygen Abundance of Typical Dwarf Galaxies at Cosmic High-Noon
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• The correlations between galaxy properties in different environments of the cosmic web
• Braving the Storm: Quantifying Disk-wide Ionized Outflows in the Large Magellanic Cloud with ULLYSES
• Host Galaxy Demographics Of Individually Detectable Supermassive Black-hole Binaries with Pulsar Timing Arrays
• Photometry and kinematics of dwarf galaxies from the Apertif HI survey
• Galaxy populations in protoclusters at cosmic noon
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• Quantifying the intrinsic variability due to randomness of the Auriga galaxy formation model
• The Next Generation Virgo Cluster Survey. XXXIII. Stellar Population Gradients in the Virgo Cluster Core Globular Cluster System
• The feasibility of constraining DM interactions with high-redshift observations by JWST
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• IllustrisTNG Snapshots for 10 Gyr of Dynamical Evolution of Brightest Cluster Galaxies and Their Host Clusters
• SCONCE: A cosmic web finder for spherical and conic geometries
• Anisotropic correlation functions as tracers of central galaxy alignments in simulations
• Subhalo abundance matching in $f(R)$ gravity
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Multi-wavelength consensus of large-scale linear bias
• Quenched, bulge-dominated, but dynamically cold galaxies in IllustrisTNG and their real-world counterparts
• The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
• The metallicity and elemental abundance maps of kinematically atypical galaxies for constraining minor merger and accretion histories
• Haloes at the ragged edge: The importance of the splashback radius
• Connection Between Galaxies and HI in the Circumgalactic and Intergalactic Media: Variation According to Galaxy Stellar Mass and Star-formation Activity
• Studying galaxy cluster morphological metrics with Mock-X
• The Fundamental Plane in the hierarchical context
• A rising tide: Intrinsic alignments since the turn of the millennium
• Topological data analysis reveals differences between simulated galaxies and dark matter haloes
• Dark-ages reionization and galaxy formation simulation - IX. Economics of reionizing galaxies
• Satellite galaxies in the Illustris-1 simulation: anisotropic locations around relatively isolated hosts
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• Enabling Radiative Transfer on AMR grids in CRASH
• Dwarf Galaxies as Cosmological Probes
• A Novel Scheme for Dark Matter Annihilation Feedback in Cosmological Simulations
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• Revisiting the Relationship between the Long GRB Rate and Cosmic Star Formation History Based on a Large Swift Sample
• Measuring Galaxy Asymmetries in 3D
• The effects of the orbital configurations of mergers on reshaping galaxy structures
• Numerical Discreteness Errors in Multi-Species Cosmological N-body Simulations
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Explaining the formation of bulges with MOND
• Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun?
• Stage IV baryonic feedback correction for non-Gaussianity inference
• Measuring Resolved Star Formation Histories from High-Precision Color-Magnitude Diagrams with StarFormationHistories.jl
• Lessons from the Local Group (and beyond) on dark matter
• Estimation of the Galaxy Quenching Rate in the Illustris Simulation
• The galaxy bias profile of cosmic voids
• Magnesium isotope ratios in Milky Way and dwarf galaxy stars
• The scaling relations of galaxies back in time: the road toward virialization
• The global energetics of radio AGN kinetic feedback in the local universe
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• Structure and large scale environment of galaxy pairs in the S-PLUS DR4
• Galaxy formation from a timescale perspective
• Central galaxy alignments. Dependence on the mass and the large-scale environment
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• The fragility of thin discs in galaxies -- I. Building tailored N-body galaxy models
• Dark matter deficient galaxies in the Illustris flat-$\Lambda$CDM model structure formation simulation
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• Probing $z\gtrsim 6$ massive black holes with gravitational waves
• Red riding on hood: Exploring how galaxy colour depends on environment
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• The BACCO Simulation Project: A baryonification emulator with Neural Networks
• A Stringent Upper Limit on Dark Matter Self-Interaction Cross Section from Cluster Strong Lensing
• Satellite Galaxies in the Illustris-1 Simulation: Poor Tracers of the Mass Distribution
• Searching for dark matter subhalos in the Fermi-LAT catalog with Bayesian neural networks
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• A Sea of Black Holes: Characterizing the LISA Signature for Stellar-Origin Black Hole Binaries
• Dark-ages Reionization and Galaxy Formation Simulation - XIV. Gas accretion, cooling and star formation in dwarf galaxies at high redshift
• The EDGE-CALIFA survey: The effect of active galactic nucleus feedback on the integrated properties of galaxies at different stages of their evolution
• Testing the Momentum-driven Supernova Feedback Paradigm in M31
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• syren-baryon: Analytic emulators for the impact of baryons on the matter power spectrum
• The Impact of Baryons on the Large-Scale Structure of the Universe
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• Predicting Localized Primordial Star Formation with Deep Convolutional Neural Networks
• Improving SDSS cosmological constraints through $\beta$-skeleton weighted correlation functions
• Exploring the Dependence of Gas Cooling and Heating Functions on the Incident Radiation Field with Machine Learning
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Probing the earliest phases in the formation of massive galaxies with simulated HST+JWST imaging data from Illustris
• SEURAT: SPH scheme extended with ultraviolet line radiative transfer
• Massive Black Hole Mergers
• On the scatter of the present-day stellar metallicity-mass relation of cluster dwarf galaxies
• Measuring the Substructure Mass Power Spectrum of 23 SLACS Strong Galaxy-Galaxy Lenses with Convolutional Neural Networks
• Two merging galaxy clusters with very hot shock fronts observed shortly before pericentric passage
• A new framework for understanding the evolution of early-type galaxies
• IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
• A statistical study of lopsided galaxies using random forest
• The assembly of the most rotationally supported disc galaxies in the TNG100 simulations
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• Constraining dark matter halo profiles with symbolic regression
• A cosmic dance at z~3: Detecting the host galaxies of the dual AGN system LBQS0302-0019 and Jil with HAWK-I+GRAAL
• Inferring Galactic Parameters from Chemical Abundances: A Multi-Star Approach
• Tracing the origins of galaxy lopsidedness across cosmic time
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Not so-dark: High resolution HI imaging of J0139+4328 and identification of an optical counterpart
• Growth and Feedback from the First Black Holes
• Eigenmode analysis of perurbations in the primordial medium at and before recombination
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• GrAviPaSt's Lens to the Past: Unveiling the Evolution of Filamentary Structures
• Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
• Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
• Exploring the evolution of a dwarf spheroidal galaxy with SPH simulations: I. Stellar feedback
• Reconciling the magnetic field in central disc galaxies with the dynamical mass using the cosmological simulations
• Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies
• The evolution of the barred galaxy population in the TNG50 simulation
• Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
• The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
• Accreted stars and stellar haloes of simulated galaxies in TNG50
• Dynamics of merging: Post-merger mixing and relaxation of an Illustris galaxy
• The AIDA-TNG project: 3D halo shapes
• The THESAN project: environmental drivers of Local Group reionization
• Line-of-Sight Velocity Projection Impact on the Local Group Mass
• Mapping luminous and dark matter in the Universe
• VEGA: Voids idEntification using Genetic Algorithm
• Galaxy infall models for arbitrary velocity directions
• Inferring halo masses with Graph Neural Networks
• Exploring the halo-galaxy connection with probabilistic approaches
• The Complexity and Information Content of Simulated Universes
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• Extremely Isolated Galaxies I. Sample and Simulation Analysis
• Photometric and Kinematic Misalignments and Their Evolution Among Fast and Slow Rotators in the Illustris Simulation
• Properties of the Environment of Galaxies in Clusters of Galaxies CL 0024+1654 and RX J0152.7-1357
• Spatial field reconstruction with INLA: Application to simulated galaxies
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• Multiscale Cosmic Curvature: from Local Structures to Cosmology
• Auriga Superstars: Improving the resolution and fidelity of stellar dynamics in cosmological galaxy simulations
• Observational biases on rotation curves from IFU data at cosmic noon
• DeepMerge: Classifying High-redshift Merging Galaxies with Deep Neural Networks
• A novel analysis of contamination in Lyman-break galaxy samples at $\mathbf{z}\sim 6-8$: spatial correlation with intermediate-redshift galaxies at $\mathbf{z}\sim 1.3-2$
• Gravitational Wave Peep Contributions to Background Signal Confusion Noise for LISA
• Astrophysical constraints on the simulation hypothesis for this Universe: why it is (nearly) impossible that we live in a simulation
• Disc instability and bar formation: view from the IllustrisTNG simulations
• Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
• Dynamical Mass Determinations and Scaling Relations of Early-Type Galaxies
• Past, present and Future of the Scaling Relations of Galaxies and Active Galactic Nuclei
• Gas-rich dwarf galaxy multiples in the Apertif HI survey
• The large-scale distribution of ionized metals in IllustrisTNG
• Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
• The Stellar Chemical Abundances of Simulated Massive Galaxies at $z=2$
• Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
• Empirical formulae to describe some physical properties of small groups of protogalaxies with multiplicity
• Astrophysical Russian Dolls
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• Recoiling supermassive black holes in analytical and numerical galaxy potential
• Detecting and analysing the topology of the cosmic web with spatial clustering algorithms I: Methods
• Dipole Distortions in the Intergalactic Medium
• A Hydro-Particle-Mesh Code for Efficient and Rapid Simulations of the Intracluster Medium
• Symmetries of the Large Scale Structures of the Universe as a Phenomenology of a Fractal Turbulence: The Role of the Plasma Component
• The haloes that reionized the Universe
• Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
• Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
• Variational autoencoder for generating realistic $N$-body simulations for dark matter halos
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations IV. Testing warm dark matter cosmologies with galaxy scaling relations: A joint simulation-observation study using DREAMS simulations
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• Cavendish experiment with fast radio bursts on cosmological scales
• Islands in Simulated Cosmos: Probing the Hubble Flow around Groups and Clusters
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• The intricate link between galaxy dynamics and intrinsic shape (or why so-called prolate rotation is a misnomer)
• Shape asymmetries and the relation between lopsidedness and radial alignment in simulated galaxies
• The Filament Rift: $\Lambda$CDM's Structural Challenge Against Observation
• Gas flows in galaxy mergers: supersonic turbulence in bridges, accretion from the circumgalactic medium, and metallicity dilution
• Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
• The halo finding problem revisited: a deep revision of the ASOHF code
• How non-thermal pressure impacts the modelling of star formation in galaxy formation simulations
• Stellar populations of stellar halos: Results from the Illustris simulation
• Unravelling the role of merger histories in the population of In situ stars: linking IllustrisTNG cosmological simulation to H3 survey
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• A thick-disk galaxy model and simulations of equal-mass galaxy pair collisions
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• The major merger origin of the Andromeda II kinematics
• The Distribution of Satellite Galaxies in the TNG100 Simulation
• Simulated X-ray Emission in Galaxy Clusters with Feedback from Active Galactic Nuclei
• The BUFFALO HST Survey
• Determining the Dark Matter distribution in galaxies with Deep Learning
• High and low Sérsic index bulges in Milky Way- and M31-like galaxies: origin and connection to the bar with TNG50
• Mimicking the halo-galaxy connection using machine learning
• Response approach to the integrated shear 3-point correlation function: the impact of baryonic effects on small scales
• Astrophysical Black holes: An Explanation for the Galaxy Quenching
• Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
• HINORA, a method for detecting ring-like structures in 3D point distributions I: application to the Local Volume Galaxy catalogue