A model for cosmological simulations of galaxy formation physics

Abstract

We present a new comprehensive model of the physics of galaxy formation designed for large-scale hydrodynamical simulations of structure formation using the moving mesh code AREPO. Our model includes primordial and metal line cooling with self-shielding corrections, stellar evolution and feedback processes, gas recycling, chemical enrichment, a novel subgrid model for the metal loading of outflows, black hole (BH) seeding, BH growth and merging procedures, quasar- and radio-mode feedback, and a prescription for radiative electro-magnetic (EM) feedback from active galactic nuclei (AGN). The metal mass loading of outflows can be adjusted independently of the wind mass loading. This is required to simultaneously reproduce the stellar mass content of low mass haloes and their gas oxygen abundances. Radiative EM AGN feedback is implemented assuming an average spectral energy distribution and a luminosity-dependent scaling of obscuration effects. This form of feedback suppresses star formation more efficiently than continuous thermal quasar-mode feedback alone, but is less efficient than mechanical radio-mode feedback in regulating star formation in massive haloes. We contrast simulation predictions for different variants of our galaxy formation model with key observations. Our best match model reproduces, among other things, the cosmic star formation history, the stellar mass function, the stellar mass - halo mass relation, g-, r-, i-, z-band SDSS galaxy luminosity functions, and the Tully-Fisher relation. We can achieve this success only if we invoke very strong forms of stellar and AGN feedback such that star formation is adequately reduced in both low and high mass systems. In particular, the strength of radio-mode feedback needs to be increased significantly compared to previous studies to suppress efficient cooling in massive, metal-enriched haloes.

38 pages, 16 figures, MNRAS accepted (including corrections of erratum). Volume-rendering movies and high-resolution images can be found at http://www.cfa.harvard.edu/itc/research/arepogal/

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• An Observational Determination of the Bolometric Quasar Luminosity Function
• The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas
• A unified model for AGN feedback in cosmological simulations of structure formation
• SPLASH: An interactive visualisation tool for Smoothed Particle Hydrodynamics simulations
• Star Formation and Feedback in Smoothed Particle Hydrodynamic Simulations--I. Isolated Galaxies
• A New Calculation of the Ionizing Background Spectrum and the Effects of HeII Reionization
• Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
• Cosmological Simulations of Intergalactic Medium Enrichment from Galactic Outflows
• The stellar mass assembly of galaxies from z=0 to z=4. Analysis of a sample selected in the rest-frame near-infrared with Spitzer
• Ubiquitous outflows in DEEP2 spectra of star-forming galaxies at z=1.4
• Direct cosmological simulations of the growth of black holes and galaxies
• Mass, Metal, and Energy Feedback in Cosmological Simulations
• A primer on hierarchical galaxy formation: the semi-analytical approach
• The Galaxy Mass Function up to z=4 in the GOODS-MUSIC sample: into the epoch of formation of massive galaxies
• Modelling discontinuities and Kelvin-Helmholtz instabilities in SPH
• Chemical enrichment of galaxy clusters from hydrodynamical simulations
• Moving mesh cosmology: tracing cosmological gas accretion
• Bimodal gas accretion in the Horizon-MareNostrum galaxy formation simulation
• Inviscid SPH
• z~7-10 Galaxies in the HUDF and GOODS fields, and their UV Luminosity Functions
• On the onset of galactic winds in quiescent star forming galaxies
• HeII Reionization and its Effect on the IGM
• Dissipation and Extra Light in Galactic Nuclei: II. 'Cusp' Ellipticals
• On the Lack of Evolution in Galaxy Star Formation Efficiency
• Evolution of the Intergalactic Opacity: Implications for the Ionizing Background, Cosmic Star Formation, and Quasar Activity
• A Direct Precision Measurement of the Intergalactic Lyman-alpha Opacity at 2<z<4.2
• Phase-space structure in the local dark matter distribution and its signature in direct detection experiments
• Simulations of AGN feedback in galaxy clusters and groups: impact on gas fractions and the Lx-T scaling relation
• Cosmic ray feedback in hydrodynamical simulations of galaxy formation
• Dissipation and Extra Light in Galactic Nuclei: I. Gas-Rich Merger Remnants
• Dissipation and Extra Light in Galactic Nuclei: III. 'Core' Ellipticals and 'Missing' Light
• Feedback from central black holes in elliptical galaxies. I: models with either radiative or mechanical feedback but not both
• Minimally Parametric Power Spectrum Reconstruction from the Lyman-alpha Forest
• Metal Cooling in Simulations of Cosmic Structure Formation
• On the Origin of Cores in Simulated Galaxy Clusters
• Kinematic Dynamos using Constrained Transport with High Order Godunov Schemes and Adaptive Mesh Refinement
• TRAPHIC - Radiative Transfer for Smoothed Particle Hydrodynamics Simulations
• A new formulation of the Type Ia SN rate and its consequences on galactic chemical evolution
• Thermal conduction in cosmological SPH simulations
• The impact of radio feedback from active galactic nuclei in cosmological simulations: Formation of disk galaxies
• Quasars: What turns them off?
• Rhapsody. I. Structural Properties and Formation History From a Statistical Sample of Re-simulated Cluster-size Halos
• Multi-frequency, thermally coupled radiative transfer with TRAPHIC: Method and tests
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies

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• The MassiveBlack-II Simulation: The Evolution of Halos and Galaxies to z~0
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• On the interplay between star formation and feedback in galaxy formation simulations
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• The role of mergers and halo spin in shaping galaxy morphology
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• Ingredients for 21cm intensity mapping
• The cosmic merger rate of stellar black hole binaries from the Illustris simulation
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• The SINS/zC-SINF survey of z~2 galaxy kinematics: Evidence for powerful AGN-driven nuclear outflows in massive star-forming galaxies
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• Resolving small-scale cold circumgalactic gas in TNG50
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• The Auriga Stellar Haloes: Connecting stellar population properties with accretion and merging history
• Semi-analytic forecasts for JWST - I. UV luminosity functions at z = 4 - 10
• Vertical disc heating in Milky Way-sized galaxies in a cosmological context
• Accurate, Meshless Methods for Magneto-Hydrodynamics
• The Gravitational Wave Background from Massive Black Hole Binaries in Illustris: spectral features and time to detection with pulsar timing arrays
• The Mass and Momentum Outflow Rates of Photoionized Galactic Outflows
• Supermassive black holes in cosmological simulations I: M_BH-M_star relation and black hole mass function
• Metal flows of the circumgalactic medium, and the metal budget in galactic halos
• The quenching and morphological evolution of central galaxies is facilitated by the feedback-driven expulsion of circumgalactic gas
• Neutral hydrogen in galaxy halos at the peak of the cosmic star formation history
• Magnetic fields in cosmological simulations of disk galaxies
• Halo Mass and Assembly History Exposed in the Faint Outskirts: the Stellar and Dark Matter Haloes of Illustris Galaxies
• The impact of feedback on cosmological gas accretion
• First star-forming structures in fuzzy cosmic filaments
• Scaling Relations Between Warm Galactic Outflows and Their Host Galaxies
• Dust Formation in Milky Way-like Galaxies
• The MillenniumTNG Project: The hydrodynamical full physics simulation and a first look at its galaxy clusters
• The impact of mechanical AGN feedback on the formation of massive early-type galaxies
• Chemodynamics of barred galaxies in cosmological simulations: On the Milky Way's quiescent merger history and in-situ bulge
• High redshift JWST predictions from IllustrisTNG: Dust modelling and galaxy luminosity functions
• The fraction of dark matter within galaxies from the IllustrisTNG simulations
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• Simulating the dust content of galaxies: successes and failures
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• Why stellar feedback promotes disc formation in simulated galaxies
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• The properties of merging black holes and neutron stars across cosmic time
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• Origin of chemically distinct discs in the Auriga cosmological simulations
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• The Structure of Multiphase Galactic Winds
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• Zooming in on accretion - II. Cold Circumgalactic Gas Simulated with a super-Lagrangian Refinement Scheme
• Damped Lyman-alpha absorbers as a probe of stellar feedback
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• The diverse evolutionary paths of simulated high-z massive, compact galaxies to z=0
• Shape of Dark Matter Haloes in the Illustris Simulation: Effects of Baryons
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• Modeling the atomic-to-molecular transition in cosmological simulations of galaxy formation
• The impact of assembly bias on the halo occupation in hydrodynamical simulations
• The splashback radius of halos from particle dynamics. II. Dependence on mass, accretion rate, redshift, and cosmology
• AREPO-RT: Radiation hydrodynamics on a moving mesh
• Single Sources in the Low-Frequency Gravitational Wave Sky: properties and time to detection by pulsar timing arrays
• Simulating galactic dust grain evolution on a moving mesh
• A Quantification of the Butterfly Effect in Cosmological Simulations and Implications for Galaxy Scaling Relations
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• Evolution of the Cool Gas in the Circumgalactic Medium (CGM) of Massive Halos -- A Keck Cosmic Web Imager (KCWI) Survey of Ly$\alpha$ Emission around QSOs at $z\approx 2$
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• The ARTEMIS simulations: stellar haloes of Milky Way-mass galaxies
• The physics of multiphase gas flows: fragmentation of a radiatively cooling gas cloud in a hot wind
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• On the origin of the fundamental metallicity relation and the scatter in galaxy scaling relations
• Revealing the galaxy-halo connection in IllustrisTNG
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• The effect of magnetic fields on properties of the circumgalactic medium
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• From 'bathtub' galaxy evolution models to metallicity gradients
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• Supermassive black holes in cosmological simulations II: the AGN population and predictions for upcoming X-ray missions
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• Dancing in the Dark: Uncertainty in ultra-faint dwarf galaxy predictions from cosmological simulations
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• Preventing Star Formation in Early-Type Galaxies with Late-Time Stellar Heating
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• Automated Distant Galaxy Merger Classifications from Space Telescope Images using the Illustris Simulation
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• Physics of Galactic Metals: Evolutionary Effects due to Production, Distribution, Feedback & Interaction with Black Holes
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• Stellar feedback by radiation pressure and photoionization
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• Dark Matter Deficient Galaxies Produced Via High-velocity Galaxy Collisions In High-resolution Numerical Simulations
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• Machine Learning and Cosmological Simulations II: Hydrodynamical Simulations
• nIFTy galaxy cluster simulations II: radiative models
• Size matters: abundance matching, galaxy sizes, and the Tully-Fisher relation in EAGLE
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• The baryon content of groups and clusters of galaxies in the FABLE simulations
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• Subhalo Demographics in the Illustris Simulation: Effects of Baryons and Halo-to-Halo Variation
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• On the origin of excess cool gas in quasar host halos
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• 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
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• Effects of simulated cosmological magnetic fields on the galaxy population
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• The Survival of Multiphase Dusty Clouds in Hot Winds
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• Does circumgalactic OVI trace low-pressure gas beyond the accretion shock? Clues from HI and low-ion absorption, line kinematics, and dust extinction
• Exploring AGN and Star Formation Activity of Massive Galaxies at Cosmic Noon
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• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• The splashback boundary of haloes in hydrodynamic simulations
• Metallicity gradients in small and nearby spiral galaxies
• Origin and evolution of ultra-diffuse galaxies in different environments
• Testing the effect of galactic feedback on the IGM at z ~ 6 with metal-line absorbers
• A moving mesh unstaggered constrained transport scheme for magnetohydrodynamics
• Baryonic effects on the matter bispectrum
• On CMB B-Mode Non-Gaussianity
• Simple Yet Powerful: Hot Galactic Outflows Driven by Supernovae
• Dark matter cores in the Fornax and Sculptor dwarf galaxies: joining halo assembly and detailed star formation histories
• MUFASA: The assembly of the red sequence
• ETHOS -- an effective theory of structure formation: predictions for the high-redshift Universe -- abundance of galaxies and reionization
• Increasing blackhole feedback induced quenching with anisotropic thermal conduction
• The Dark Matter Halos of Moderate Luminosity X-ray AGN as Determined from Weak Gravitational Lensing and Host Stellar Masses
• Alignment between filaments and galaxy spins from the MaNGA integral-field survey
• Modeling Galactic Conformity with the Color-Halo Age Relation in the Illustris Simulation
• The prevalence and properties of cold gas inflows and outflows around galaxies in the local Universe
• Time Delay Lens Modelling Challenge
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• The host galaxies of double compact objects merging in the local Universe
• nIFTy Galaxy Cluster simulations IV: Quantifying the Influence of Baryons on Halo Properties
• Galaxy Formation with local photoionisation feedback I. Methods
• Resolving flows around black holes: numerical technique and applications
• Origin of the galaxy HI size-mass relation
• Diffuse gas properties and stellar metallicities in cosmological simulations of disc galaxy formation
• On the origin of star-gas counterrotation in low-mass galaxies
• AGN jet feedback on a moving mesh: gentle cluster heating by weak shocks and lobe disruption
• The origin of the enhanced metallicity of satellite galaxies
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Impact of relativistic jets on the star formation rate: a turbulence-regulated framework
• Imprints of temperature fluctuations on the $z\sim 5$ Lyman-$\alpha$ forest: a view from radiation-hydrodynamic simulations of reionization
• Diagnosing galactic feedback with the line broadening in the low redshift Lyman-alpha forest
• A Link Between Ram Pressure Stripping and Active Galactic Nuclei
• How runaway stars boost galactic outflows
• The effects of subgrid models on the properties of giant molecular clouds in galaxy formation simulations
• Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• Galaxies lacking dark matter in the Illustris simulation
• Galaxies Probing Galaxies at High Resolution: Co-Rotating Gas Associated with a Milky Way Analog at z=0.4
• Efficacy of early stellar feedback in low gas surface density environments
• A Genetic Approach to the History of the Magellanic Clouds
• The growth of brightest cluster galaxies in the TNG300 simulation:dissecting the contributions from mergers and in situ star formation
• Bulges and disks in the local Universe. Linking the galaxy structure to star formation activity
• [OIII] Emission Line Properties in a New Sample of Heavily Reddened Quasars at $z>2$
• The Distribution of Satellites Around Central Galaxies in a Cosmological Hydrodynamical Simulation
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• Characterizing hydrostatic mass bias with Mock-X
• Baryons in the CosmicWeb of IllustrisTNG -- II: the Connection among Galaxies, Halos, their Formation Time and their Location in the Cosmic Web
• Young and turbulent: the early life of massive galaxy progenitors
• Satellite Alignment: I. Distribution of Substructures and Their Dependence On Assembly History From N-Body Simulations
• Realistic estimation for the detectability of dark matter sub-halos with Fermi-LAT
• Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
• Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
• The specific star formation rate function at different mass scales and quenching: A comparison between cosmological models and SDSS
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe I. - The Effect of the Group Environment on Star Formation in Spiral Galaxies
• Simulating the effect of high column density absorbers on the one-dimensional Lyman-alpha forest flux power spectrum
• Stellar Velocity Dispersion: Linking Quiescent Galaxies to their Dark Matter Halos
• The sensitivity of stellar feedback to IMF averaging versus IMF sampling in galaxy formation simulations
• The MASSIVE Survey - XII Connecting Stellar Populations of Early-Type Galaxies to Kinematics and Environment
• Forecasts for the WFIRST High Latitude Survey using the BlueTides Simulation
• The effect of differential accretion on the Gravitational Wave Background and the present day MBH Binary population
• Satellites Around Milky Way Analogs: Tension in the Number and Fraction of Quiescent Satellites Seen in Observations Versus Simulations
• Submillimetre galaxies in cosmological hydrodynamical simulations -- an opportunity for constraining feedback models
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - I: Bulge+disc decompositions, methods, and biases
• The Bacco Simulation Project: Bacco Hybrid Lagrangian Bias Expansion Model in Redshift Space
• Correlations Between Black Holes and Host Galaxies in the Illustris and IllustrisTNG Simulations
• The Mass Profile of the Milky Way to the Virial Radius from the Illustris Simulation
• Kinematics and Dynamics of Multiphase Outflows in Simulations of the Star-Forming Galactic ISM
• Simulating disc galaxy bulges that are consistent with observed scaling relations
• Neutron Star Stability in Light of the Neutron Decay Anomaly
• Early chemo-dynamical evolution of dwarf galaxies deduced from enrichment of r-process elements
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
• Cosmic variance of $z>7$ galaxies: Prediction from BlueTides
• Chandra Survey of Nearby Highly Inclined Disc Galaxies - III: Comparison with Hydrodynamical Simulations of Circumgalactic Coronae
• The descendants of the first quasars in the BlueTides simulation
• nIFTY galaxy cluster simulations III: The Similarity & Diversity of Galaxies & Subhaloes
• 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
• Accretion of Galaxy Groups into Galaxy Clusters
• The Impact of Dust on the Sizes of Galaxies in the Epoch of Reionization
• Modeling for Stellar Feedback in Galaxy Formation Simulations
• BlueTides simulation: establishing black hole-galaxy relations at high-redshift
• How Environment Affects Galaxy Metallicity through Stripping and Formation History: Lessons from the Illustris Simulation
• AGN Feedback in SDSS-IV MaNGA: AGNs have Suppressed Central Star Formation Rates
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• The role of gas infall in the evolution of disc galaxies
• Active galactic nucleus jet feedback in hydrostatic halos
• The Angular Momentum of the Circumgalactic Medium in the TNG100 Simulation
• Structural and photometric properties of barred galaxies from the Auriga cosmological simulations
• The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations
• Simulated Bars May Be Shorter But Are Not Slower Than Observed: TNG50 vs. MaNGA
• RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars
• The impact of magnetic fields on cosmological galaxy mergers. I: Reshaping gas and stellar discs
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
• AGN Feedback models: Correlations with star formation and observational implications of time evolution
• The host galaxies of double compact objects across cosmic time
• Formation of Galactic Disks I: Why Did the Milky Way's Disk Form Unusually Early?
• A gradient based method for modeling baryons and matter in halos of fast simulations
• Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations
• Non-parametric Morphologies of Galaxies in the EAGLE Simulation
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• The Effect Of AGN Heating On The Low-Redshift Lyα Forest
• Enhancing AGN efficiency and cool-core formation with anisotropic thermal conduction
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• The Supersonic Project: Shining Light on SIGOs - a New Formation Channel for Globular Clusters
• An ever-present $Gaia$ snail shell triggered by a dark matter wake
• The combined and respective roles of imaging and stellar kinematics in identifying galaxy merger remnants
• Tidal destruction in a low mass galaxy environment: the discovery of tidal tails around DDO 44
• The impact of modified gravity on the Sunyaev-Zel'dovich effect
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• Rapid Filamentary Accretion as the Origin of Extended Thin Discs
• Satellites of Satellites: The Case for Carina and Fornax
• Forward and backward galaxy evolution in comoving number density space
• Simulating the effect of photoheating feedback during reionization
• The First Quiescent Galaxies in TNG300
• The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
• WARPFIELD Population Synthesis: The physics of (extra-)Galactic star formation and feedback driven cloud structure and emission from sub-to-kpc scales
• R-process enrichment in ultrafaint dwarf galaxies
• Self-regulated AGN feedback of light jets in cool-core galaxy clusters
• The Missing Satellite Problem in 3D
• The impact of galactic feedback on the shapes of dark-matter haloes
• Probing the $z\gtrsim 6$ quasars in a universe with IllustrisTNG physics: Impact of gas-based black hole seeding models
• IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies
• Simulating the Spatial Distribution and Kinematics of Globular Clusters within Galaxy Clusters in Illustris
• Gas outflows from the z= 7.54 quasar : predictions from the BlueTides Simulation
• Cosmological simulations of massive black hole seeds: predictions for next generation electromagnetic and gravitational wave observations
• Discriminating Topology in Galaxy Distributions using Network Analysis
• Black hole clustering and duty cycles in the Illustris simulation
• Gas flows in the circumgalactic medium around simulated high-redshift galaxies
• Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time
• X-ray-inferred kinematics of the core ICM in Perseus-like clusters: Insights from the TNG-Cluster simulation
• Probing hot gas around luminous red galaxies through the Sunyaev-Zel'dovich effect
• Shattering of Cosmic Sheets due to Thermal Instabilities: a Formation Channel for Metal-Free Lyman Limit Systems
• Simulating a metallicity-dependent initial mass function: Consequences for feedback and chemical abundances
• Thermal Instabilities and Shattering in the High-Redshift WHIM: Convergence Criteria and Implications for Low-Metallicity Strong HI Absorbers
• Strong stellar-driven outflows shape the evolution of galaxies at cosmic dawn
• A New Model For Including Galactic Winds in Simulations of Galaxy Formation I: Introducing the Physically Evolved Winds (PhEW) Model
• Kinematic Evolution of Simulated Star-Forming Galaxies
• Chemical evolution of disc galaxies from cosmological simulations
• Cosmological insights into the assembly of the radial and compact stellar halo of the Milky Way
• Tidal disruption events in the first billion years of a galaxy
• How AGN feedback drives the size growth of the first quasars
• The host galaxies of z=7 quasars: predictions from the BlueTides simulation
• PRIYA: A New Suite of Lyman-alpha Forest Simulations for Cosmology
• Linking the brightest stellar streams with the accretion history of Milky Way-like galaxies
• The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
• Chemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulations
• Diffuse coronae in cosmological simulations of Milky Way-sized galaxies
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
• Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
• Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
• The Interplay of Kinetic and Radiative Feedback in Galaxy Clusters
• AGN feedback and the origin and fate of the hot gas in early-type galaxies
• Simba: The average properties of the circumgalactic medium of $2\le z\le 3$ quasars are determined primarily by stellar feedback
• Evolution of galaxy groups in the Illustris simulation
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• Resolving flows around black holes: the impact of gas angular momentum
• The stellar halo in Local Group Hestia simulations II. The accreted component
• The relation between star formation rate and stellar mass of galaxies at z $\sim$ 1-4
• On the relevance of chaos for halo stars in the Solar Neighbourhood
• Variations of Observed Lyman-α Spectra Shapes due to the Intergalactic Absorption
• Nuclear processes in Astrophysics: Recent progress
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• The THESAN-ZOOM project: Burst, quench, repeat -- unveiling the evolution of high-redshift galaxies along the star-forming main sequence
• The Impact of baryonic physics on the kinetic Sunyaev-Zel'dovich Effect
• KETJU -- resolving small-scale supermassive black hole dynamics in GADGET-4
• A Framework for Modeling Polycyclic Aromatic Hydrocarbon Emission in Galaxy Evolution Simulations
• Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
• On the Cosmic Web Elongation in Fuzzy Dark Matter Cosmologies: Effects on Density Profiles, Shapes and Alignments of Halos
• Are fossil groups early-forming galaxy systems?
• A Fundamental Test for Galaxy Formation Models: Matching the Lyman-$\alpha$ Absorption Profiles of Galactic Halos over Three Decades in Distance
• The impact of baryonic physics and massive neutrinos on weak lensing peak statistics
• Zooming in on supermassive black holes: how resolving their gas cloud host renders their accretion episodic
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• Galaxy Zoo: Morphological classification of galaxy images from the Illustris simulation
• Redshift evolution of stellar mass versus gas fraction relation in 0<z<2 regime: observational constraint for galaxy formation models
• The THESAN project: connecting ionized bubble sizes to their local environments during the Epoch of Reionization
• Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
• Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
• Hot and counter-rotating star-forming disk galaxies in IllustrisTNG and their real-world counterparts
• Quenching in Cosmic Sheets: Tracing the Impact of Large Scale Structure Collapse on the Evolution of Dwarf Galaxies
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• Predictions for the Abundance of High-redshift Galaxies in a Fuzzy Dark Matter Universe
• Characterizing Protoclusters and Protogroups at z $\sim$ 2.5 Using Ly$\alpha$ Tomography
• The complementary roles of feedback and mergers in building the gaseous halo and the X-ray corona of Milky Way-sized galaxies
• Considerations for the Observability of Kinematically Offset Binary AGN
• Simulation techniques for modified gravity
• Redshift Evolution of the Fundamental Plane Relation in the IllustrisTNG Simulation
• Spherical Cows in Dark Matter Indirect Detection
• A disturbing FABLE of mergers, feedback, turbulence, and mass biases in simulated galaxy clusters
• Observing the host galaxies of high-redshift quasars with JWST: predictions from the BlueTides simulation
• Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and $N$-body simulations
• Is the Universe Simpler than LCDM?
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• nIFTy galaxy cluster simulations V: Investigation of the Cluster Infall Region
• Stellar and Weak Lensing Profiles of Massive Galaxies in the Hyper-Suprime Cam Survey and in Hydrodynamic Simulations
• CHANG-ES XXV: HI Imaging of Nearby Edge-on Galaxies -- Data Release 4
• Baryonic effects on CMB lensing and neutrino mass constraints
• On the Optimal Choice of Nucleosynthetic Yields, IMF and Number of SNe Ia for Chemical Evolution Modelling
• Effects of Spatial Discretization in Lyman-alpha Line Radiation Transfer Simulations
• The stellar mass function and star formation rate-stellar mass relation of galaxies at z ~ 4 - 7
• Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
• The diversity of the circumgalactic medium around z = 0 Milky Way-mass galaxies from the Auriga simulations
• Efficient long-range AGN feedback affects the low redshift Lyman-$\alpha$ forest
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• A high baryon fraction in massive haloes at z~3
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• The Milky Way and Andromeda galaxies in a constrained hydrodynamical simulation: morphological evolution
• Quantifying substructures in {\it Hubble Frontier Field} clusters: comparison with $\Lambda CDM$ simulations
• On the correlation between the local dark matter and stellar velocities
• SEAGLE--II: Constraints on feedback models in galaxy formation from massive early type strong lens galaxies
• The cosmic web in Lyman-alpha emission
• Galaxy Formation with Local Photoionization Feedback -II. Effect of X-Ray Emission from Binaries and Hot Gas
• The globular cluster system of the Auriga simulations
• On the origin of star formation quenching in massive galaxies at $z\gtrsim 3$ in the cosmological simulations IllustrisTNG
• ETHOS - an effective theory of structure formation: formation of the first haloes and their stars
• Redshift space distortions of the {\rm HI} 21-cm intensity mapping signal due to the internal motions within galaxies
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• A tiny host galaxy for the first giant black hole: $z=7.5$ quasar in BlueTides
• Simulating the Carbon Footprint of Galactic Halos
• The local PNG bias of neutral Hydrogen, ${\mathrm{H}}_{\mathrm{I}}$
• The early growth of supermassive black holes in cosmological hydrodynamic simulations with constrained Gaussian realizations
• 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
• The morphology and kinematics of neutral hydrogen in the vicinity of z=0 galaxies with Milky Way masses -- a study with the Illustris simulation
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• The IllustrisTNG Simulations: Public Data Release
• The Case for Strangulation in Low-Mass Hosts: DDO 113
• Realistic synthetic integral field spectroscopy with RealSim-IFS
• What Is Inside Matters: Simulated Green Valley Galaxies Have Centrally Concentrated Star Formation
• The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
• Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
• There and back again: understanding the critical properties of backsplash galaxies
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Clumpy galaxies in cosmological simulations: The effect of ISM model
• Spatially Resolved Outflows in a Seyfert Galaxy at z = 2.39
• Galaxies with Shells in the Illustris Simulation: Metallicity Signatures
• Supermassive black hole fueling in IllustrisTNG: Impact of environment
• On the relevance of chaos for halo stars in the solar neighbourhood II
• Dynamical friction and evolution of black holes in cosmological simulations: a new implementation in OpenGadget3
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• Momentum Injection by Clustered Supernovae: Testing Subgrid Feedback Prescriptions
• Galactic coronae in Milky Way-like galaxies: the role of stellar feedback in gas accretion
• Gas around galaxy haloes - III: hydrogen absorption signatures around galaxies and QSOs in the Sherwood simulation suite
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• Quantifying the stellar ages of dynamically separated bulges and disks of CALIFA spiral galaxies
• The Effects of Metallicity and Abundance Pattern of the ISM on Supernova Feedback
• Cosmic Web Dissection in Fuzzy Dark Matter Cosmologies
• Colour and infall time distributions of satellite galaxies in simulated Milky-Way analogs
• The Supersonic Project: To cool or not to cool Supersonically Induced Gas Objects (SIGOs)?
• Momentum and energy injection by a supernova remnant into an inhomogeneous medium
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• The metallicity and star formation activity of long gamma-ray burst hosts for z$<$3: insights from the Illustris simulation
• Metal Enrichment in the Reionization Epoch
• s-process Enirchment of Ultrafaint Dwarf Galaxies
• Non-parametric Morphologies of Mergers in the Illustris Simulation
• The magnetised and thermally unstable tails of jellyfish galaxies
• The THESAN-ZOOM project: central starbursts and inside-out quenching govern galaxy sizes in the early Universe
• Star Formation and Gas Phase History of the Cosmic Web
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• Stellar migration in the Auriga simulations
• The THESAN-ZOOM project: Population III star formation continues until the end of reionization
• Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption
• Quenching, Mergers and Age Profiles for z=2 Galaxies in IllustrisTNG
• Exploring the Fate of Stellar Core Collapse with Supernova Relic Neutrinos
• Extreme Spheres: Counts-in-cells for 21cm intensity mapping
• nIFTy Galaxy Cluster simulations VI: The dynamical imprint of substructure on gaseous cluster outskirts
• FORECAST: a flexible software to forward model cosmological hydrodynamical simulations mimicking real observations
• IllustrisTNG Insights: Factors Affecting the Presence of Bars in Disk Galaxies
• Grain Physics and IR Dust Emission in AGN Environments
• Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
• Testing the Impact of Satellite Anisotropy on Large and Small Scale Intrinsic Alignments using Hydrodynamical Simulations
• Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
• The CO universe: Modelling CO emission and H${}_2$ abundance in cosmological galaxy formation simulations
• Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
• Is the core-cusp problem a matter of perspective: Jeans Anisotropic Modeling against numerical simulations
• The cooler past of the intracluster medium in TNG-Cluster
• Feedback and dynamical masses in high-$z$ galaxies: the advent of high-resolution NIRSpec spectroscopy
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• The space density distribution of galaxies in the absolute magnitude - rotation velocity plane: a volume-complete Tully-Fisher relation from CALIFA stellar kinematics
• Metal content of the circumgalactic medium around star-forming galaxies at z $\sim$ 2.6 as revealed by the VIMOS Ultra-Deep Survey
• Anisotropic satellite accretion onto the Local Group with HESTIA
• Hubble Space Telescope [O III] Emission-Line Kinematics in Two Nearby QSO2s: A Case for X-ray Feedback
• Differential rotation of the halo traced by the K-giant stars
• Formation of disc galaxies around z~2
• Gas Accretion Traced in Absorption in Galaxy Spectroscopy
• Rapid Growth of Galactic Supermassive Black Holes through Accreting Giant Molecular Clouds during Major Mergers of their Host Galaxies
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• Gas Cooling in Hydrodynamic Simulations with An Exact Time Integration Scheme
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• Can Stellar Discs in a Cosmological Setting Avoid Forming Strong Bars?
• Colour-magnitude diagram in simulations of galaxy formation
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• Particle ejection during mergers of dark matter halos
• Bursty Star Formation in Dwarfs is Sensitive to Numerical Choices in Supernova Feedback Models
• Connecting Primordial Star Forming Regions and Second Generation Star Formation in the Phoenix Simulations
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• Relating galaxies across different redshift to study galaxy evolution
• The BlueTides Mock Image Catalogue: Simulated observations of high-redshift galaxies and predictions for JWST imaging surveys
• Simultaneous Dependence of Matter Clustering on Scale and Environment
• Properties of the circumgalactic medium in simulations compared to observations
• The Challenge to MOND from ultra faint dwarf galaxies
• Implications of galaxy buildup for putative IMF variations in massive galaxies
• Can HI 21 cm line trace the Missing Baryons in the Filamentary Structures?
• Using large galaxy surveys to distinguish z~0.5 quiescent galaxy models
• Modified Baryonic Dynamics: two-component cosmological simulations with light sterile neutrinos
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• First results from SMAUG: Insights into star formation conditions from spatially-resolved ISM properties in TNG50
• The Supersonic Project: The Early Evolutionary Path of SIGOs
• Accretion onto supermassive and intermediate mass black holes in cosmological simulations
• Not all peaks are created equal: the early growth of Supermassive Black Holes
• Formation and fate of low metallicity stars in IllustrisTNG50
• A field-level emulator for modeling baryonic effects across hydrodynamic simulations
• A quantitative demonstration that stellar feedback locally regulates galaxy growth
• The Baltimore Oriole's Nest: Cool Winds from the Inner and Outer Parts of a Star-Forming Galaxy at z=1.3
• On the connection between AGN radiative feedback and massive black hole spin
• Cosmological gas accretion history onto the stellar discs of Milky Way-like galaxies in the Auriga simulations -- (I) Temporal dependency
• Entropy-Conserving Scheme for Modeling Nonthermal Energies in Fluid Dynamics Simulations
• Mass-morphology relation of TNG50 galaxies
• The role of accreted and in situ populations in shaping the stellar halos of low-mass galaxies
• An observational testbed for cosmological zoom-in simulations: constraining stellar migration in the solar cylinder using asteroseismology
• Oxygen Loss from Simulated Galaxies and the Metal Flow Main Sequence: Predicting the Dependence on Mass and Environment
• How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations
• Gamma-ray Production in the Extended Halo of the Galaxy and Possible Implications for the Origin of Galactic Cosmic Rays
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• The parametrization of gas flows in discs in the Auriga simulations
• Where binary neutron stars merge: predictions from IllustrisTNG
• Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization
• The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
• The Formation of a Milky Way-sized Disk Galaxy 1. A Comparison of Numerical Methods
• Discrimination of heavy elements originating from Pop III stars in z = 3 intergalactic medium
• Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
• IllustrisTNG Snapshots for 10 Gyr of Dynamical Evolution of Brightest Cluster Galaxies and Their Host Clusters
• Modeling Post-Reionization HI Distributions in Fuzzy Dark Matter Cosmologies Using Conditional Normalizing Flows
• Observational Diagnostics of Gas Flows: Insights from Cosmological Simulations
• Quantifying the intrinsic variability due to randomness of the Auriga galaxy formation model
• Quenched, bulge-dominated, but dynamically cold galaxies in IllustrisTNG and their real-world counterparts
• Simulated [CII] in high-z galaxies
• Impact of star formation models on the growth of simulated galaxies at high redshifts
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• Measuring the mass and concentration of dark matter halos from the velocity dispersion profile of their stars
• Galaxy populations in protoclusters at cosmic noon
• The impact of the cosmological constant on past and future star formation
• Positive and negative feedback by AGN jets in high-redshift galaxies
• The impact of filaments on dwarf galaxy properties in the Auriga simulations
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• CosmoDRAGoN simulations -- I. Dynamics and observable signatures of radio jets in cosmological environments
• Understanding the Baryon Cycle: Fueling Star Formation via Inflows in Milky Way-like Galaxies
• The life cycle of giant molecular clouds in simulated Milky Way-mass galaxies
• Disc-Halo Interactions in ΛCDM
• Revisiting the Relationship between the Long GRB Rate and Cosmic Star Formation History Based on a Large Swift Sample
• The Inner Dynamical Mass Across Galaxy Morphology: A Weak Scaling with Total Stellar Mass
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• A Simple Sub-Grid Model For Cosmic Ray Effects on Galactic Scales
• Understanding Dwarf Galaxies in order to Understand Dark Matter
• Stacking Redshifted 21cm Images of HII Regions Around High Redshift Galaxies as a Probe of Early Reionization
• The BACCO Simulation Project: A baryonification emulator with Neural Networks
• FIRST J1419+3940 as the First Observed Radio Flare from a Neutron Star Merger
• A Simulated Galaxy Laboratory: Exploring the Observational Effects on UV Spectral Absorption Line Measurements
• The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• Can Cooling and Heating Functions be Modeled with Homogeneous Radiation Fields?
• Premature supermassive black hole mergers in cosmological simulations of structure formation
• Differentiable Cosmological Hydrodynamics for Field-Level Inference and High Dimensional Parameter Constraints
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• Prospects for detecting cosmic filaments in Lyman-alpha emission across redshifts $z=2-5$
• Measuring Resolved Star Formation Histories from High-Precision Color-Magnitude Diagrams with StarFormationHistories.jl
• Dark matter deficient galaxies in the Illustris flat-$\Lambda$CDM model structure formation simulation
• Comparing the interstellar and circumgalactic origin of gas in the tails of jellyfish galaxies
• IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50
• Recovering the pattern speeds of edge-on barred galaxies via an orbit-superposition method
• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• Cosmological gas accretion history onto the stellar discs of Milky Way-like galaxies in the Auriga simulations -- (II) The inside-out growth of discs
• Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
• The Milky Way in context: The formation of galactic discs and chemical sequences from a cosmological perspective
• An Improved and Physically-Motivated Scheme for Matching Galaxies with Dark Matter Halos
• A systematic study of AGN feedback in a disk galaxy I: global overview
• Complexity Phenomena and ROMA of the Magnetospheric Cusp, Hydrodynamic Turbulence, and the Cosmic Web
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• The Reliability of Type Ia Supernovae Delay Time Distributions Recovered from Galaxy Star Formation Histories
• IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
• VALES VIII: Weak ionized gas outflows in star-forming galaxies at $z\sim 0.15$ traced with VLT/MUSE
• Galaxy formation with wave/fuzzy dark matter: The core-halo structure and the solitonic imprint
• A Swift X-ray view of the SMS4 sample -- X-ray properties of 31 quasars and radio galaxies
• The evolution of the barred galaxy population in the TNG50 simulation
• Growth and Feedback from the First Black Holes
• FLAMINGO: Galaxy formation and feedback effects on the gas density and velocity fields
• The role of magnetic fields in ram pressure stripping of satellite galaxies in the circumgalactic medium around massive galaxies
• A new strategy for matching observed and simulated lensing galaxies
• High-redshift AGN population in radiation-hydrodynamics simulations
• Auriga Streams II: orbital properties of tidally disrupting satellites of Milky Way-mass galaxies
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Merger Tree-based Galaxy Matching: A Comparative Study Across Different Resolutions
• HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
• The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z=3.55$
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• Broad [CII] line wings as tracer of molecular and multi-phase outflows in infrared bright galaxies
• FAST drift scan survey for HI intensity mapping: simulation on hunting HI filament with pairwise stacking
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• Accreted stars and stellar haloes of simulated galaxies in TNG50
• Atomic Hydrogen Shows its True Colours: Correlations between HI and Galaxy Colour in Simulations
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• Spatial field reconstruction with INLA: Application to simulated galaxies
• Inferring halo masses with Graph Neural Networks
• The THESAN project: environmental drivers of Local Group reionization
• Auriga Superstars: Improving the resolution and fidelity of stellar dynamics in cosmological galaxy simulations
• Extended Hernquist-Springel formalism for cosmic star formation
• Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
• A novel analysis of contamination in Lyman-break galaxy samples at $\mathbf{z}\sim 6-8$: spatial correlation with intermediate-redshift galaxies at $\mathbf{z}\sim 1.3-2$
• The AURORA Survey: Tracing Galactic Outflows at $z\gtrsim 2.5$ with JWST/NIRSpec NUV Absorption Lines
• Tracing black hole and galaxy growth across environments since cosmic noon
• Galaxy-halo internal alignments across cosmic time
• The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
• Host galaxies and electromagnetic counterparts to binary neutron star mergers across the cosmic time: Detectability of GW170817-like events
• Suppression of galactic outflows by cosmological infall and circumgalactic medium
• Momentum deposition of supernovae with cosmic rays
• Machine Learning for Galactic Archaeology: A chemistry-based neural network method for identification of accreted disc stars
• Modeling Multiphase Galactic Outflows: A Multifluid Moving Mesh Approach
• Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
• Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• COSMOS-Web: Galaxy Size and Surface Brightness Evolution at Rest-Frame 1.22 $\mu$m Since $z=3$
• ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations
• Imladris: a detailed and flexible model for galaxy simulations with individual stars
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Stellar populations of stellar halos: Results from the Illustris simulation
• Extreme Metallicity Dwarf Galaxies in IllustrisTNG
• Gas flows in galaxy mergers: supersonic turbulence in bridges, accretion from the circumgalactic medium, and metallicity dilution
• 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
• Boosting (In)direct Detection of Dark Matter