E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
arXiv:0901.4107 · doi:10.1111/j.1365-2966.2009.15715.x
Abstract
Hydrodynamic cosmological simulations at present usually employ either the Lagrangian SPH technique, or Eulerian hydrodynamics on a Cartesian mesh with adaptive mesh refinement. Both of these methods have disadvantages that negatively impact their accuracy in certain situations. We here propose a novel scheme which largely eliminates these weaknesses. It is based on a moving unstructured mesh defined by the Voronoi tessellation of a set of discrete points. The mesh is used to solve the hyperbolic conservation laws of ideal hydrodynamics with a finite volume approach, based on a second-order unsplit Godunov scheme with an exact Riemann solver. The mesh-generating points can in principle be moved arbitrarily. If they are chosen to be stationary, the scheme is equivalent to an ordinary Eulerian method with second order accuracy. If they instead move with the velocity of the local flow, one obtains a Lagrangian formulation of hydrodynamics that does not suffer from the mesh distortion limitations inherent in other mesh-based Lagrangian schemes. In this mode, our new method is fully Galilean-invariant, unlike ordinary Eulerian codes, a property that is of significant importance for cosmological simulations. In addition, the new scheme can adjust its spatial resolution automatically and continuously, and hence inherits the principal advantage of SPH for simulations of cosmological structure growth. The high accuracy of Eulerian methods in the treatment of shocks is retained, while the treatment of contact discontinuities improves. We discuss how this approach is implemented in our new parallel code AREPO, both in 2D and 3D. We use a suite of test problems to examine the performance of the new code and argue that it provides an attractive and competitive alternative to current SPH and Eulerian techniques. (abridged)
updated to agree with accepted version in MNRAS, 67 pages, 50 figures, many of them heavily size-reduced. Full resolution version and videos available at http://www.mpa-garching.mpg.de/~volker/arepo
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- The colors of satellite galaxies in the Illustris Simulation
- LYRA I: Simulating the multi-phase ISM of a dwarf galaxy with variable energy supernovae from individual stars
- Semi-implicit anisotropic cosmic ray transport on an unstructured moving mesh
- The information content of stellar halos: Stellar population gradients and accretion histories in early-type Illustris galaxies
- The CAMELS Multifield Dataset: Learning the Universe's Fundamental Parameters with Artificial Intelligence
- Why Are AGN and Host Galaxies Misaligned?
- Fast and energetic AGN-driven outflows in simulated dwarf galaxies
- Black hole feeding and feedback: the physics inside the "subgrid"
- Lessons from the Auriga discs: The hunt for the Milky Way's ex-situ disc is not yet over
- Quiescent Ultra-diffuse galaxies in the field originating from backsplash orbits
- Faraday rotation maps of disk galaxies
- The relationship between fine galaxy stellar morphology and star formation activity in cosmological simulations: a deep learning view
- The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
- The CAMELS project: public data release
- rpSPH: a novel Smoothed Particle Hydrodynamics Algorithm
- Thermonuclear explosion of a massive hybrid HeCO white-dwarf triggered by a He-detonation on a companion
- Aurigaia: mock Gaia DR2 stellar catalogues from the Auriga cosmological simulations
- The Importance of Quantum Pressure of Fuzzy Dark Matter on Lyman-Alpha Forest
- Higher-order initial conditions for mixed baryon-CDM simulations
- Common-envelope evolution with an asymptotic giant branch star
- The First Stars
- The physical origins and dominant emission mechanisms of Lyman-alpha halos: results from the TNG50 simulation in comparison to MUSE observations
- The formation of hot gaseous haloes around galaxies
- Galaxy formation with L-GALAXIES: Modelling the environmental dependency of galaxy evolution and comparing with observations
- Constructing stable 3D hydrodynamical models of giant stars
- Powderday: Dust Radiative Transfer for Galaxy Simulations
- The interplay of Self-Interacting Dark Matter and baryons in shaping the halo evolution
- GA-NIFS: The core of an extremely massive proto-cluster at the Epoch of Reionization probed with JWST/NIRSpec
- A Survey of Disc Thickness and Viscosity in Circumbinary Accretion: Binary Evolution, Variability, and Disc Morphology
- Automated Distant Galaxy Merger Classifications from Space Telescope Images using the Illustris Simulation
- Simulating Gamma-ray Emission in Star-forming Galaxies
- Hierarchical octree and k-d tree grids for 3D radiative transfer simulations
- Galaxy bias and primordial non-Gaussianity: insights from galaxy formation simulations with IllustrisTNG
- The spin alignment of galaxies with the large-scale tidal field in hydrodynamic simulations
- Precessing spherical shells: flows, dissipation, dynamo and the lunar core
- Galaxy mergers moulding the circum-galactic medium - I. The impact of a major merger
- A flexible modelling of galaxy assembly bias
- Zooming in on Individual Star Formation: Low- and High-mass Stars
- Quenching timescales of dwarf satellites around Milky Way-mass hosts
- Statistical properties of paired fixed fields
- Resolving The Generation of Starburst Winds in Galaxy Mergers
- The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- I: Halo Gas Properties and the Role of SMBH Feedback
- Blandford-Znajek jets in galaxy formation simulations: method and implementation
- On the Survivability and Metamorphism of Tidally Disrupted Giant Planets: the Role of Dense Cores
- Intrinsic alignments of disk and elliptical galaxies in the MassiveBlack-II and Illustris simulations
- Using the PPML approach for constructing a low-dissipation, operator-splitting scheme for numerical simulations of hydrodynamic flows
- Preferential Accretion and Circumbinary Disk Precession in Eccentric Binary Systems
- Astrophysical hydrodynamics with a high-order discontinuous Galerkin scheme and adaptive mesh refinement
- An exact general remeshing scheme applied to physically conservative voxelization
- Scientific Visualization in Astronomy: Towards the Petascale Astronomy Era
- The prevalence of pseudo-bulges in the Auriga simulations
- The natural emergence of the correlation between H2 and star formation rate surface densities in galaxy simulations
- The Impact of Galactic Winds on the Angular Momentum of Disk Galaxies in the Illustris Simulation
- Using 3D Voronoi grids in radiative transfer simulations
- Stellar feedback by radiation pressure and photoionization
- The geometry of the gas surrounding the Central Molecular Zone: on the origin of localised molecular clouds with extreme velocity dispersions
- Machine Learning and Cosmological Simulations II: Hydrodynamical Simulations
- Dark Matter Deficient Galaxies Produced Via High-velocity Galaxy Collisions In High-resolution Numerical Simulations
- nIFTy galaxy cluster simulations II: radiative models
- Hydrogen Reionization in the Illustris universe
- Nucleosynthesis imprints from different Type Ia Supernova explosion scenarios and implications for galactic chemical evolution
- The galaxy-halo connection of emission-line galaxies in IllustrisTNG
- Considerations on the Role of Fall-Back Discs in the Final Stages of the Common Envelope Binary Interaction
- Constraining First Star Formation with 21cm-Cosmology
- The stellar halos of ETGs in the IllustrisTNG simulations: the photometric and kinematic diversity of galaxies at large radii
- Shapley Supercluster Survey: Ram-Pressure Stripping vs. Tidal Interactions in the Shapley Supercluster
- Rotation curve fitting and its fatal attraction to cores in realistically simulated galaxy observations
- Slow-then-rapid quenching as traced by tentative evidence for enhanced metallicities of cluster galaxies at z~0.2 in the slow quenching phase
- Resolving shocks and filaments in galaxy formation simulations: effects on gas properties and star formation in the circumgalactic medium
- Histogram of oriented gradients: a technique for the study of molecular cloud formation
- A flexible subhalo abundance matching model for galaxy clustering in redshift space
- The cumulative star-formation histories of dwarf galaxies with TNG50. I: Environment-driven diversity and connection to quenching
- Moving mesh cosmology: properties of neutral hydrogen in absorption
- Gravothermal solutions of SIDM halos: mapping from constant to velocity-dependent cross section
- Assessing the Jeans Anisotropic Multi-Gaussian Expansion method with the Illustris simulation
- The baryon content of groups and clusters of galaxies in the FABLE simulations
- New criteria for the selection of galaxy close pairs from cosmological simulations: evolution of the major and minor merger fraction in MUSE deep fields
- Galaxy bias from forward models: linear and second-order bias of IllustrisTNG galaxies
- The merger and assembly histories of Milky Way- and M31-like galaxies with TNG50: disk survival through mergers
- Cosmic rays and non-thermal emission in simulated galaxies: III. probing cosmic ray calorimetry with radio spectra and the FIR-radio correlation
- The physics of Lyman-alpha escape from disc-like galaxies
- Instability of Supersonic Cold Streams Feeding Galaxies III: Kelvin-Helmholtz Instability in Three Dimensions
- Subhalo Demographics in the Illustris Simulation: Effects of Baryons and Halo-to-Halo Variation
- Barred Galaxies in the IllustrisTNG Simulation
- Smoothed particle magnetohydrodynamics with a Riemann solver and the method of characteristics
- Cosmological Zoom Simulations of z = 2 Galaxies: The Impact of Galactic Outflows
- Expectations of the size evolution of massive galaxies at from the TNG50 simulation: the CEERS/JWST view
- Well balanced Arbitrary-Lagrangian-Eulerian finite volume schemes on moving nonconforming meshes for the Euler equations of gasdynamics with gravity
- Dust in and around galaxies: dust in cluster environments and its impact on gas cooling
- Extensions to models of the galaxy-halo connection
- The formation of massive Pop III stars in the presence of turbulence
- Calibrating an updated SPH scheme within GCD+
- The origin and properties of massive prolate galaxies in the Illustris simulation
- IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
- Effects of simulated cosmological magnetic fields on the galaxy population
- Dark matter halo shapes in the Auriga simulations
- Magnetically-levitating disks around supermassive black holes
- The effects of dynamical substructure on Milky Way mass estimates from the high velocity tail of the local stellar halo
- Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
- Simulating the interstellar medium of galaxies with radiative transfer, non-equilibrium thermochemistry, and dust
- Approximate tensor-product preconditioners for very high order discontinuous Galerkin methods
- Simulating radio synchrotron emission in star-forming galaxies: small-scale magnetic dynamo and the origin of the far infrared-radio correlation
- Stellar Halos in Illustris- Probing the Histories of Milky Way-Mass Galaxies
- DISCO: A 3D Moving-Mesh Magnetohydrodynamics Code Designed for the Study of Astrophysical Disks
- On the stellar halo metallicity profile of Milky Way-like galaxies in the Auriga simulations
- Realistic simulations of galaxy formation in f(R) modified gravity
- Galaxy simulation with the evolution of grain size distribution
- Simulations of inspiraling and merging double neutron stars using the Spectral Einstein Code
- A dynamical mechanism for the origin of nuclear rings
- The role of galactic dynamics in shaping the physical properties of giant molecular clouds in Milky Way-like galaxies
- Cosmic-Ray Diffusion Suppression in Star-forming Regions Inhibits Clump Formation in Gas-rich Galaxies
- Accurate mass and velocity functions of dark matter halos
- Hydrodynamical moving-mesh simulations of the tidal disruption of stars by supermassive black holes
- The stability of stellar disks in Milky-Way sized dark matter halos
- Predictions for local PNG bias in the galaxy power spectrum and bispectrum and the consequences for constraints
- How an improved implementation of H2 self-shielding influences the formation of massive stars and black holes
- The structure and assembly history of cluster-size haloes in Self-Interacting Dark Matter
- Direct Arbitrary-Lagrangian-Eulerian finite volume schemes on moving nonconforming unstructured meshes
- Formation and Evolution of Binary Neutron Stars: Mergers and Their Host Galaxies
- How Biased Are Halo Properties in Cosmological Simulations?
- The splashback boundary of haloes in hydrodynamic simulations
- GANDALF - Graphical Astrophysics code for N-body Dynamics And Lagrangian Fluids
- A discontinuous Galerkin method for solving the fluid and MHD equations in astrophysical simulations
- High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
- Galaxies undergoing ram-pressure stripping: the influence of the bulge on morphology and star formation rate
- EAGLE and Illustris-TNG predictions for resolved eROSITA X-ray observations of the circumgalactic medium around normal galaxies
- Learning cosmology and clustering with cosmic graphs
- 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
- Cosmic rays and non-thermal emission in simulated galaxies. II. -ray maps, spectra and the far infrared--ray relation
- Common Envelope Evolution on a Moving Mesh
- Evolution of cosmic ray electron spectra in magnetohydrodynamical simulations
- Thermal instabilities in cooling galactic coronae: fuelling star formation in galactic discs
- Baryonic effects on the matter bispectrum
- Grand challenges in protoplanetary disc modelling
- Long-Lived Eccentric Modes in Circumbinary Disks
- Origin and evolution of ultra-diffuse galaxies in different environments
- Formation of an extended stellar halo around an ultra-faint dwarf galaxy following one of the earliest mergers from galactic building blocks
- Increasing blackhole feedback induced quenching with anisotropic thermal conduction
- Type Ia Supernova Sub-classes and Progenitor Origin
- FOREVER22: galaxy formation in protocluster regions
- On GLM curl cleaning for a first order reduction of the CCZ4 formulation of the Einstein field equations
- Hydrodynamic simulations with the Godunov SPH
- ETHOS -- an effective theory of structure formation: predictions for the high-redshift Universe -- abundance of galaxies and reionization
- Learning the Relationship between Galaxies Spectra and their Star Formation Histories using Convolutional Neural Networks and Cosmological Simulations
- Modeling Galactic Conformity with the Color-Halo Age Relation in the Illustris Simulation
- Metallicity-dependent nucleosynthetic yields of Type Ia supernovae originating from double detonations of sub-M white dwarfs
- Probing Cosmic Ray Transport with Radio Synchrotron Harps in the Galactic Center
- Morphological decomposition of TNG50 galaxies: methodology and catalogue
- Deriving star formation histories from photometry using energy balance spectral energy distribution modelling
- Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
- nIFTy Galaxy Cluster simulations IV: Quantifying the Influence of Baryons on Halo Properties
- Fragmentation induced starvation in Population III star formation: a resolution study
- Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
- Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
- PHANGS-JWST First Results: Tracing the Diffuse ISM with JWST Imaging of Polycyclic Aromatic Hydrocarbon Emission in Nearby Galaxies
- The manifestation of secondary halo bias on the galaxy population from IllustrisTNG300
- Accretion and Magnetic Reconnection in the Classical T Tauri Binary DQ Tau
- CO-dark gas and molecular filaments in Milky Way-type galaxies - II: The temperature distribution of the gas
- Bipolar planetary nebulae from common envelope evolution of binary stars
- Relative distribution of dark matter, gas, and stars around cosmic filaments in the IllustrisTNG simulation
- Trapping of HII regions in Population III star formation
- Origin of the galaxy HI size-mass relation
- Kinematic decomposition of IllustrisTNG disk galaxies: morphology and relation with morphological structures
- WISDOM Project -- X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure
- High order ADER schemes and GLM curl cleaning for a first order hyperbolic formulation of compressible flow with surface tension
- Modeling Mid-Infrared Diagnostics of Obscured Quasars and Starbursts
- Hot phase generation by supernovae: resolution, chemistry and thermal conduction
- On the origin of star-gas counterrotation in low-mass galaxies
- Resolving flows around black holes: numerical technique and applications
- On the influence of halo mass accretion history on galaxy properties and assembly bias
- Diffuse gas properties and stellar metallicities in cosmological simulations of disc galaxy formation
- The origin of the enhanced metallicity of satellite galaxies
- The Impact of Different Physical Processes on the Statistics of Lyman-limit and Damped Lyman-alpha Absorbers
- Imprints of temperature fluctuations on the Lyman- forest: a view from radiation-hydrodynamic simulations of reionization
- Diagnosing galactic feedback with the line broadening in the low redshift Lyman-alpha forest
- Formation of sdB-stars via common envelope ejection by substellar companions
- Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
- AGN jet feedback on a moving mesh: gentle cluster heating by weak shocks and lobe disruption
- Magnetogenesis around the first galaxies: the impact of different field seeding processes on galaxy formation
- Metal enrichment in the circumgalactic medium and Lyα haloes around quasars at z 3
- A Constrained Transport Scheme for MHD on Unstructured Static and Moving Meshes
- Characterizing the formation history of Milky Way-like stellar haloes with model emulators
- The halo mass function and filaments in full cosmological simulations with fuzzy dark matter
- Variational integration for ideal magnetohydrodynamics with built-in advection equations
- Star formation from dense shocked regions in supersonic isothermal magneto-turbulence
- Galaxies going MAD: The Galaxy-Finder Comparison Project
- Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
- The impact of numerical viscosity in SPH simulations of galaxy clusters
- The effects of subgrid models on the properties of giant molecular clouds in galaxy formation simulations
- Momentum feedback from marginally-resolved HII regions in isolated disc galaxies
- Jellyfish galaxies with the IllustrisTNG simulations -- When, where, and for how long does ram pressure stripping of cold gas occur?
- Enrichment of the hot intracluster medium: numerical simulations
- A comparison of black hole growth in galaxy mergers with Gasoline and Ramses
- What drives the evolution of gas kinematics in star-forming galaxies?
- Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
- FORGE -- the f(R) gravity cosmic emulator project I: Introduction and matter power spectrum emulator
- The Generation of Vorticity in Cosmological N-body Simulations
- Separate Universe Simulations with IllustrisTNG: baryonic effects on power spectrum responses and higher-order statistics
- Galaxies lacking dark matter in the Illustris simulation
- The emergence of passive galaxies in the early Universe
- Stellar Property Statistics of Massive Halos from Cosmological Hydrodynamics Simulations: Common Kernel Shapes
- Robust Field-level Likelihood-free Inference with Galaxies
- Accretion Does Not Drive the Turbulence in Galactic Disks
- Cosmological Structure Formation and Soliton Phase Transition in Fuzzy Dark Matter with Axion Self-Interactions
- Barred galaxies in the Illustris-1 and TNG100 simulations
- Disentangling the formation history of galaxies via population-orbit superposition: method validation
- Energy wrinkles and phase-space folds of the last major merger
- Efficacy of early stellar feedback in low gas surface density environments
- The cold circumgalactic medium in emission: MgII halos in TNG50
- Magnetized Moving Mesh Merger of a Carbon-Oxygen White Dwarf Binary
- Cosmic rays and non-thermal emission in simulated galaxies. I. Electron and proton spectra compared to Voyager-1 data
- Momentum-driven Winds from Radiatively Efficient Black Hole Accretion and Their Impact on Galaxies
- First Light: exploring the Spectra of High-Redshift Galaxies in the Renaissance Simulations
- Machine-assisted Semi-Simulation Model (MSSM): Estimating Galactic Baryonic Properties from their Dark Matter using a Machine Trained on Hydrodynamic Simulations
- Characterizing hydrostatic mass bias with Mock-X
- Evaluating the ability of triaxial Schwarzschild modelling to estimate properties of galaxies from the Illustris simulation
- Radio Emission from the unbound Debris of Tidal Disruption Events
- Rich: Open Source Hydrodynamic Simulation on a Moving Voronoi Mesh
- High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
- Dynamically Driven Inflow onto the Galactic Center and its Effect upon Molecular Clouds
- Illustrating galaxy-halo connection in the DESI era with IllustrisTNG
- The growth of brightest cluster galaxies in the TNG300 simulation:dissecting the contributions from mergers and in situ star formation
- Cosmology with one galaxy?
- Blandford-Znajek jets in galaxy formation simulations: exploring the diversity of outflows produced by spin-driven AGN jets in Seyfert galaxies
- The scatter in the radial profiles of X-ray luminous galaxy clusters as diagnostic of the thermodynamical state of the ICM
- Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations
- A semi-analytic study of self-interacting dark-matter haloes with baryons
- The challenge of simulating the star cluster population of dwarf galaxies with resolved interstellar medium
- Magnetization of the intergalactic medium in the IllustrisTNG simulations: the importance of extended, outflow-driven bubbles
- The specific star formation rate function at different mass scales and quenching: A comparison between cosmological models and SDSS
- Testing kinematic distances under a realistic Galactic potential
- Simulating the effect of high column density absorbers on the one-dimensional Lyman-alpha forest flux power spectrum
- Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
- Realistic estimation for the detectability of dark matter sub-halos with Fermi-LAT
- How merger-driven gas motions in galaxy clusters can turn AGN bubbles into radio relics
- Recent Progress in Modeling the Macro- and Micro-Physics of Radio Jet Feedback in Galaxy Clusters
- Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
- The velocity anisotropy of the Milky Way satellite system
- Synthetic observations of star formation and the interstellar medium
- Correlations Between Black Holes and Host Galaxies in the Illustris and IllustrisTNG Simulations
- Stellar Velocity Dispersion: Linking Quiescent Galaxies to their Dark Matter Halos
- The first Super Massive Black Holes: indications from models for future observations
- The AGORA High-resolution Galaxy Simulations Comparison Project. III: Cosmological zoom-in simulation of a Milky Way-mass halo
- Submillimetre galaxies in cosmological hydrodynamical simulations -- an opportunity for constraining feedback models
- The sensitivity of stellar feedback to IMF averaging versus IMF sampling in galaxy formation simulations
- Dark matter stripping in galaxy clusters: a look at the Stellar to Halo Mass relation in the Illustris simulation
- Instability of Supersonic Cold Streams Feeding Galaxies II. Nonlinear Evolution of Surface and Body Modes of Kelvin-Helmholtz Instability
- The Incidence of Low-Metallicity Lyman-Limit Systems at z~3.5: Implications for the Cold-Flow Hypothesis of Baryonic Accretion
- TNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations
- Long-term Evolution of Binary Orbits Induced by Circumbinary Disks
- Gas distribution from clusters to filaments in IllustrisTNG
- ERGO-ML I: Inferring the assembly histories of IllustrisTNG galaxies from integral observable properties via invertible neural networks
- The diversity of rotation curves of simulated galaxies with cusps and cores
- Voronoi volume function: A new probe of cosmology and galaxy evolution
- Is there enough star formation in simulated protoclusters?
- Tidally induced warps of spiral galaxies in IllustrisTNG
- High-order Magnetohydrodynamics for Astrophysics with an Adaptive Mesh Refinement Discontinuous Galerkin Scheme
- The effect of cosmic-ray acceleration on supernova blast wave dynamics
- The star formation histories of dwarf galaxies in Local Group cosmological simulations
- Panchromatic SED modelling of spatially-resolved galaxies
- Decoupling the rotation of stars and gas -- I: the relationship with morphology and halo spin
- Simulations of cosmic ray propagation
- White Dwarf Mergers on Adaptive Meshes I. Methodology and Code Verification
- The impact of feedback and the hot halo on the rates of gas accretion onto galaxies
- nIFTY galaxy cluster simulations III: The Similarity & Diversity of Galaxies & Subhaloes
- Assembly bias in the local PNG halo bias and its implication for constraints
- SimpleX2: radiative transfer on an unstructured, dynamic grid
- WIMP DM and first stars: suppression of fragmentation in primordial star formation
- Stellar orbit evolution in close circumstellar disc encounters
- A study of AGN and supernova feedback in simulations of isolated and merging disc galaxies
- Ly Blobs from Cold Streams Undergoing Kelvin-Helmholtz Instabilities
- Shock finding on a moving-mesh: II. Hydrodynamic shocks in the Illustris universe
- Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
- Accretion of Galaxy Groups into Galaxy Clusters
- On the Kelvin-Helmholtz instability with smooth initial conditions -- Linear theory and simulations
- The global stability of M33: still a puzzle
- Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
- The Angular Momentum of the Circumgalactic Medium in the TNG100 Simulation
- Active galactic nucleus jet feedback in hydrostatic halos
- Satellites of Milky Way- and M31-like galaxies with TNG50: quenched fractions, gas content, and star formation histories
- Code Comparison in Galaxy Scale Simulations with Resolved Supernova Feedback: Lagrangian vs. Eulerian Methods
- From 3D hydrodynamic simulations of common-envelope interaction to gravitational-wave mergers
- Fast full N-body simulations of generic modified gravity: conformal coupling models
- Statistical modelling of the cosmological dispersion measure
- Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
- A redshift-dependent IRX- dust attenuation relation for TNG50 galaxies
- The Lagrangian hydrodynamics code MAGMA2
- Dynamic Localised Turbulent Diffusion and its Impact on the Galactic Ecosystem
- SPHYNX: an accurate density-based SPH method for astrophysical applications
- How Environment Affects Galaxy Metallicity through Stripping and Formation History: Lessons from the Illustris Simulation
- Accurately simulating anisotropic thermal conduction on a moving mesh
- DIVE in the cosmic web: voids with Delaunay Triangulation from discrete matter tracer distributions
- Degeneracies Between Self-interacting Dark Matter and Supernova Feedback as cusp-core transformation mechanisms
- A 3D radiation-hydrodynamic AGB binary model
- The impact of magnetic fields on cosmological galaxy mergers. I: Reshaping gas and stellar discs
- The High Fraction of Thin Disk Galaxies Continues to Challenge ΛCDM Cosmology
- The heart of galaxy clusters: demographics and physical properties of cool-core and non-cool-core halos in the TNG-Cluster simulation
- The First Large Absorption Survey in HI (FLASH): I. Science Goals and Survey Design
- RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars
- EvoL: The new Padova T-SPH parallel code for cosmological simulations - I. Basic code: gravity and hydrodynamics
- Magnetic buoyancy in simulated galactic discs with a realistic circum galactic medium
- The Circumgalactic Medium of Milky Way-like Galaxies in the TNG50 Simulation -- II: Cold, Dense Gas Clouds and High-Velocity Cloud Analogs
- Galaxy formation in the brane world I: overview and first results
- Assembly of supermassive black hole seeds
- The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
- DISPATCH: A Numerical Simulation Framework for the Exa-scale Era. I. Fundamentals
- The MillenniumTNG Project: Intrinsic alignments of galaxies and halos
- Spiral-arm instability: giant clump formation via fragmentation of a galactic spiral arm
- The Evolving Effect Of Cosmic Web Environment On Galaxy Quenching
- Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
- Pulsed Accretion in the T Tauri Binary TWA 3A
- Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
- The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
- Galaxies with prolate rotation in Illustris
- Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
- Convergence of AMR and SPH simulations - I. Hydrodynamical resolution and convergence tests
- Globular Clusters Formed within Dark Halos I: present-day abundance, distribution and kinematics
- Properties and Origin of Galaxy Velocity Bias in the Illustris Simulation
- Formation of massive disk galaxies in the IllustrisTNG simulation
- A gradient based method for modeling baryons and matter in halos of fast simulations
- A study of stellar orbit fractions: simulated IllustrisTNG galaxies compared to CALIFA observations
- The Effect Of AGN Heating On The Low-Redshift Lyα Forest
- A Comparison of Circumgalactic MgII Absorption between the TNG50 Simulation and the MEGAFLOW Survey
- Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations
- The Cosmological Simulation Code OpenGadget3 -- Implementation of Meshless Finite Mass
- The Contribution of In-situ and Ex-situ Star Formation in Early-Type Galaxies: MaNGA versus IllustrisTNG
- Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
- Formation of Galactic Disks I: Why Did the Milky Way's Disk Form Unusually Early?
- Simulated Galaxy Interactions as Probes of Merger Spectral Energy Distributions
- The Supersonic Project: Shining Light on SIGOs - a New Formation Channel for Globular Clusters
- The combined and respective roles of imaging and stellar kinematics in identifying galaxy merger remnants
- Disc galaxies formed from major mergers in Illustris
- The morphology and kinematics of the gaseous circumgalactic medium of Milky Way mass galaxies -- II. comparison of IllustrisTNG and Illustris simulation results
- {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
- High-resolution synthetic UV-submm images for simulated Milky Way-type galaxies from the Auriga project
- Dust entrainment in galactic winds
- Modelling Shear Flows with SPH and Grid Based Methods
- Cluster induced quenching of galaxies in the massive cluster XMMXCSJ2215.9-1738 at z~1.5 traced by enhanced metallicities inside half R200
- SEAGLE - I: A pipeline for simulating and modeling strong lenses from cosmological hydrodynamic simulations
- Gas rich and gas poor structures through the stream velocity effect
- An ever-present snail shell triggered by a dark matter wake
- The formation of low surface brightness galaxies in the IllustrisTNG simulation
- From large-scale environment to CGM angular momentum to star forming activities -- I: star-forming galaxies
- Breaking baryon-cosmology degeneracy with the electron density power spectrum
- Small-scale galaxy clustering in the EAGLE simulation
- How Drag Force Evolves in Global Common Envelope Simulations
- Satellites of Satellites: The Case for Carina and Fornax
- Simulating the effect of photoheating feedback during reionization
- Simulated star formation rate functions at z~4-7, and the role of feedback in high-z galaxies
- The impact of modified gravity on the Sunyaev-Zel'dovich effect
- Global HI asymmetries in IllustrisTNG: a diversity of physical processes disturb the cold gas in galaxies
- The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
- The First Quiescent Galaxies in TNG300
- WARPFIELD Population Synthesis: The physics of (extra-)Galactic star formation and feedback driven cloud structure and emission from sub-to-kpc scales
- Stochastic angular momentum slews and flips and their effect on discs in galaxy formation models
- ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman- forest
- The impact of galactic feedback on the shapes of dark-matter haloes
- UV to submillimetre luminosity functions of TNG50 galaxies
- Probing the quasars in a universe with IllustrisTNG physics: Impact of gas-based black hole seeding models
- A divergence-cleaning scheme for cosmological SPMHD simulations
- Baryon-CDM isocurvature galaxy bias with IllustrisTNG
- The dark matter component of the Gaia radially anisotropic substructure
- Fast full -body simulations of generic modified gravity: derivative coupling models
- Accurate tracer particles of baryon dynamics in the adaptive mesh refinement code Ramses
- Simulating the Spatial Distribution and Kinematics of Globular Clusters within Galaxy Clusters in Illustris
- IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies
- R-process enrichment in ultrafaint dwarf galaxies
- The scatter in the galaxy-halo connection: a machine learning analysis
- A general framework to test gravity using galaxy clusters II: A universal model for the halo concentration in gravity
- Effects of initial density profiles on massive star cluster formation in giant molecular clouds
- Simulations of the star-forming molecular gas in an interacting M51-like galaxy: cloud population statistics
- Self-regulated AGN feedback of light jets in cool-core galaxy clusters
- On the relative effect of nodes and filaments of the cosmic web on the quenching of galaxies and the orientation of their spin
- The Missing Satellite Problem in 3D
- The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
- Uncertainties in supernova input rates drive qualitative differences in simulations of galaxy evolution
- Flows around galaxies. I. The dependency of galaxy connectivity on cosmic environments and effects on the star-formation rate
- Powerful quasar outflow in a massive disc galaxy at
- Inner Boundary Condition in Quasi-Lagrangian Simulations of Accretion Disks
- Black hole clustering and duty cycles in the Illustris simulation
- Discriminating Topology in Galaxy Distributions using Network Analysis
- Mixing matters
- Imprints of Chameleon f(R) Gravity on Galaxy Rotation Curves
- The impact of thermodynamics on gravitational collapse: filament formation and magnetic field amplification
- A novel approach for accurate radiative transfer in cosmological hydrodynamic simulations
- AGN jet feedback on a moving mesh: lobe energetics and X-ray properties in a realistic cluster environment
- Origin of highly -process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy
- DM halo morphological types of MW-like galaxies in the TNG50 simulation: Simple, Twisted, or Stretched
- Cosmological simulations of massive black hole seeds: predictions for next generation electromagnetic and gravitational wave observations
- X-ray-inferred kinematics of the core ICM in Perseus-like clusters: Insights from the TNG-Cluster simulation
- Parallel grid library for rapid and flexible simulation development
- Metal Mixing in Minihalos: The Descendants of Pair-Instability Supernovae
- LYRA III: The smallest Reionization survivors
- Morphological and Rotation Structures of Circumgalactic Mg II Gas in the EAGLE Simulation and the Dependence on Galaxy Properties
- Probing the Circum-Galactic Medium with Fast Radio Bursts: Insights from the CAMELS Simulations
- Shattering of Cosmic Sheets due to Thermal Instabilities: a Formation Channel for Metal-Free Lyman Limit Systems
- Evolution of star formation rate-density relation over cosmic time in a simulated universe: the observed reversal reproduced
- Simulating a metallicity-dependent initial mass function: Consequences for feedback and chemical abundances
- The impact of Lyman- radiative transfer on large-scale clustering in the Illustris simulation
- Rapid evolution of the recurrence time in the repeating partial tidal disruption event eRASSt J045650.3-203750
- X-ray metal line emission from the hot circumgalactic medium: probing the effects of supermassive black hole feedback
- The Physical Origin of Galactic Conformity: From Theory to Observation
- Towards a consistent framework of comparing galaxy mergers in observations and simulations
- Radiative effects during the assembly of direct collapse black holes
- A finite volume method for two-moment cosmic-ray hydrodynamics on a moving mesh
- The dispersion measure of Fast Radio Bursts host galaxies: estimation from cosmological simulations
- RHAPSODY-G simulations II - Baryonic growth and metal enrichment in massive galaxy clusters
- Hybrid Cosmological Simulations with Stream Velocities
- Thermal Instabilities and Shattering in the High-Redshift WHIM: Convergence Criteria and Implications for Low-Metallicity Strong HI Absorbers
- Cosmological insights into the assembly of the radial and compact stellar halo of the Milky Way
- Galaxy groups in the 2MASS Redshift Survey
- Constraining the halo mass function with observations
- How AGN feedback drives the size growth of the first quasars
- Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
- The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
- The formation of entropy cores in non-radiative galaxy cluster simulations: SPH versus AMR
- Multi-Dimensional, Compressible Viscous Flow on a Moving Voronoi Mesh
- The impact of the Large Magellanic Cloud on dark matter direct detection signals
- The hierarchical fragmentation of filaments and the role of sub-filaments
- Magnetic field morphology and evolution in the Central Molecular Zone and its effect on gas dynamics
- Cellular Topology Optimization on Differentiable Voronoi Diagrams
- Surrogate modelling the Baryonic Universe I: The colour of star formation
- The SZ flux-mass (-) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback
- A new approach to determine optically thick H2 cooling and its effect on primordial star formation
- Fallback accretion powered supernova light curves based on a neutrino-driven explosion simulation of a 40 Msun star
- Collisionless Stellar Hydrodynamics as an Efficient Alternative to N-body Methods
- Towards an improved model of self-interacting dark matter haloes
- Local simulations of MRI turbulence with meshless methods
- Hydrodynamic capabilities of an SPH code incorporating an artificial conductivity term with a gravity-based signal velocity
- Linking the brightest stellar streams with the accretion history of Milky Way-like galaxies
- Particle splitting in smoothed particle hydrodynamics based on Voronoi diagram
- The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations
- A tight relation between the age distributions of stellar clusters and the properties of the interstellar medium in the host galaxy
- SHAPing the Gas: Understanding Gas Shapes in Dark Matter Haloes with Interpretable Machine Learning
- How galaxies populate haloes in very low-density environments? An analysis of the Halo Occupation Distribution in cosmic voids
- Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies
- ETHOS -- An effective parametrization and classification for structure formation: the non-linear regime at
- A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
- SHOCKFIND - An algorithm to identify magnetohydrodynamic shock waves in turbulent clouds
- Multifrequency radiation hydrodynamics simulations of H2 line emission in primordial, star-forming clouds
- Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
- The MillenniumTNG Project: The large-scale clustering of galaxies
- Star Formation in Nuclear Rings with the TIGRESS Framework
- Evolution and observational signatures of the cosmic ray electron spectrum in SN 1006
- Star formation efficiencies of molecular clouds in a galactic center environment
- On the environmental influence of groups and clusters of galaxies beyond the virial radius: Galactic conformity at few Mpc scales
- SPHINCS_BSSN: A general relativistic Smooth Particle Hydrodynamics code for dynamical spacetimes
- Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
- The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
- Baryonic effects on the detectability of annihilation radiation from dark matter subhaloes around the Milky Way
- Resolving flows around black holes: the impact of gas angular momentum
- The entropy core in galaxy clusters: numerical and physical effects in cosmological grid simulations
- Precision Redshift-Space Galaxy Power Spectra using Zel'dovich Control Variates
- Simba: The average properties of the circumgalactic medium of quasars are determined primarily by stellar feedback
- Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
- The impact of natal kicks on galactic r-process enrichment by neutron star mergers
- Euclid: Modelling massive neutrinos in cosmology -- a code comparison
- Structure, Kinematics, and Observability of the Large Magellanic Cloud's Dynamical Friction Wake in Cold vs. Fuzzy Dark Matter
- EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
- Decoupling the rotation of stars and gas -- II: the link between black hole activity and MaNGA kinematics in TNG
- Simulating galaxy formation in f(R) modified gravity: Matter, halo, and galaxy-statistics
- Evolution of galaxy groups in the Illustris simulation
- Endothermic self-interacting dark matter in Milky Way-like dark matter haloes
- The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
- On the relevance of chaos for halo stars in the Solar Neighbourhood
- High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project
- Primordial magnetic fields in Population III star formation: a magnetised resolution study
- Simulation of sharp interface multi-material flows involving an arbitrary number of components through an extended five-equation model
- Empirically-motivated early feedback: momentum input by stellar feedback in galaxy simulations inferred through observations
- Constraints on AGN feedback from its Sunyaev-Zel'dovich imprint on the cosmic background radiation
- KETJU -- resolving small-scale supermassive black hole dynamics in GADGET-4
- On the Mass Distribution of the Intra-Cluster Light in Galaxy Groups and Clusters
- The THESAN-ZOOM project: Burst, quench, repeat -- unveiling the evolution of high-redshift galaxies along the star-forming main sequence
- A Markov model for non-lognormal density distributions in compressive isothermal turbulence
- ETHOS -- An Effective Theory of Structure Formation: Impact of Dark Acoustic Oscillations on Cosmic Dawn
- Common envelope binary interaction simulations between a thermally-pulsating AGB star and a low mass companion
- Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
- The ultra-diffuse dwarf galaxies NGC 1052-DF2 and 1052-DF4 are in conflict with standard cosmology
- The Impact of baryonic physics on the kinetic Sunyaev-Zel'dovich Effect
- Modeling the kinematics of globular cluster systems
- GOGREEN: a critical assessment of environmental trends in cosmological hydrodynamical simulations at z ~ 1
- The galaxy-halo size relation of low-mass galaxies in FIRE
- The halo mass function and inner structure of ETHOS haloes at high redshift
- WOMBAT: A Scalable and High Performance Astrophysical MHD Code
- Velocity-dependent J-factors for annihilation radiation from cosmological simulations
- A Fundamental Test for Galaxy Formation Models: Matching the Lyman- 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
- Are fossil groups early-forming galaxy systems?
- Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
- An alternative method to generate pre-initial conditions for cosmological -body simulations
- The impact of inelastic self-interacting dark matter on the dark matter structure of a Milky Way halo
- The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
- On the Cosmic Web Elongation in Fuzzy Dark Matter Cosmologies: Effects on Density Profiles, Shapes and Alignments of Halos
- Dark-matter-deficient galaxies in hydrodynamical simulations
- The hot circumgalactic media of massive cluster satellites in the TNG-Cluster simulation: existence and detectability
- Comparing Simulations of AGN Feedback
- On the redshift evolution of the baryon and gas fraction in simulated groups and clusters of galaxies
- Galaxy Zoo: Morphological classification of galaxy images from the Illustris simulation
- Synthetic observations of molecular clouds in a galactic center environment: I. Studying maps of column density and integrated intensity
- SHAM through the lens of a hydrodynamical simulation
- Hot and counter-rotating star-forming disk galaxies in IllustrisTNG and their real-world counterparts
- Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
- Planet-disc interaction on a freely moving mesh
- Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
- The impact of two massive early accretion events in a Milky Way-like galaxy: repercussions for the buildup of the stellar disc and halo
- How Cosmic Rays Mediate the Evolution of the Interstellar Medium
- An Atlas of Gas Motions in the TNG-Cluster Simulation: from Cluster Cores to the Outskirts
- Aging Halos: Implications of the Magnitude Gap on Conditional Statistics of Stellar and Gas Properties of Massive Halos
- Impact of an accurate modeling of primordial chemistry in high resolution studies
- Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
- A general framework to test gravity using galaxy clusters IV: Cluster and halo properties in DGP gravity
- Redshift evolution of stellar mass versus gas fraction relation in 0<z<2 regime: observational constraint for galaxy formation models
- Strongly lensed cluster substructures are not in tension with CDM
- Characterizing Protoclusters and Protogroups at z 2.5 Using Ly Tomography
- GASP. VII. Gas accretion onto an isolated galaxy
- Systematic errors in strong gravitational lensing reconstructions, a numerical simulation perspective
- Redshift Evolution of the Fundamental Plane Relation in the IllustrisTNG Simulation
- The Supersonic Project: rotational effects of supersonic motions on the first structures in the Universe
- A disturbing FABLE of mergers, feedback, turbulence, and mass biases in simulated galaxy clusters
- Giant Lyman-Alpha Nebulae in the Illustris Simulation
- Connecting turbulent velocities and magnetic fields in galaxy cluster simulations with active galactic nuclei jets
- TARDIS Paper II: Synergistic Density Reconstruction from Lyman-alpha Forest and Spectroscopic Galaxy Surveys with Applications to Protoclusters and the Cosmic Web
- Turnaround radius of galaxy clusters in N-body simulations
- nIFTy galaxy cluster simulations V: Investigation of the Cluster Infall Region
- Spherical Cows in Dark Matter Indirect Detection
- Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
- Prospects for Recovering Galaxy Intrinsic Shapes from Projected Quantities
- Parametric instability in a free evolving warped protoplanetary disc
- Arepo-MCRT: Monte Carlo Radiation Hydrodynamics on a Moving Mesh
- On the Optimal Choice of Nucleosynthetic Yields, IMF and Number of SNe Ia for Chemical Evolution Modelling
- SPRAI: Coupling of radiative feedback and primordial chemistry in moving mesh hydrodynamics
- The Kelvin-Helmholtz instability and smoothed particle hydrodynamics
- Efficient long-range AGN feedback affects the low redshift Lyman- forest
- How the first stars shaped the faintest gas-dominated dwarf galaxies
- A study of cool core resiliency and entropy mixing in simulations of galaxy cluster mergers
- The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
- Effects of Spatial Discretization in Lyman-alpha Line Radiation Transfer Simulations
- The diversity of the circumgalactic medium around z = 0 Milky Way-mass galaxies from the Auriga simulations
- An Effective Bias Expansion for 21 cm Cosmology in Redshift Space
- Dynamics of Intermediate-Mass Black Holes Wandering in the Milky Way Galaxy Using the Illustris TNG50 Simulation
- Limits on non-canonical heating and turbulence in the intergalactic medium from the low redshift Lyman-alpha forest
- The nature of core formation in dark matter haloes: adiabatic or impulsive?
- A semi-analytic model comparison: testing cooling models against hydrodynamical simulations
- The moving mesh code Shadowfax
- Chemical evolution of giant molecular clouds in simulations of galaxies
- Testing Hydrodynamics Schemes in Galaxy Disc Simulations
- Modeling multi-phase gases in cosmological simulations using compressible multi-fluid hydrodynamics
- The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
- Braginskii viscosity on an unstructured, moving mesh accelerated with super-time-stepping
- Detecting low-mass haloes with strong gravitational lensing II: constraints on the density profiles of two detected subhaloes
- A high performance and portable all-Mach regime flow solver code with well-balanced gravity. Application to compressible convection
- The Sunyaev-Zel'dovich effect of simulated jet-inflated bubbles in clusters
- Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
- The cosmic web in Lyman-alpha emission
- Effects of Baryonic Feedback on the Cosmic Web
- SEAGLE--II: Constraints on feedback models in galaxy formation from massive early type strong lens galaxies
- Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
- From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral
- Dynamical evolution of massive black holes in galactic-scale N-body simulations - introducing the regularized tree code "rVINE"
- The role of the artificial conductivity in SPH simulations of galaxy clusters: effects on the ICM properties
- From dark matter halos to pre-stellar cores: High resolution follow-up of cosmological Lyman-Werner simulations
- On the correlation between the local dark matter and stellar velocities
- A Comparison of the Baryonic Tully-Fisher Relation in MaNGA and IllustrisTNG
- EDGE: A new approach to suppressing numerical diffusion in adaptive mesh simulations of galaxy formation
- Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
- Continuous wavelet analysis of matter clustering using the Gaussian-derived wavelet
- ALMA reveals sunburn: CO dissociation around AGB stars in the globular cluster 47 Tucanae
- Ionizing photon production and escape fractions during cosmic reionization in the TNG50 simulation
- Santa Barbara Cluster Comparison Test with DISPH
- Multiple Beads-on-a-string: Dark Matter-Deficient Galaxy Formation in a Mini-bullet Satellite-satellite Galaxy Collision
- The Elephant in the Bathtub: when the physics of star formation regulate the baryon cycle of galaxies
- The matter density PDF for modified gravity and dark energy with Large Deviations Theory
- Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
- Multifield Cosmology with Artificial Intelligence
- Galaxy Formation with Local Photoionization Feedback -II. Effect of X-Ray Emission from Binaries and Hot Gas
- Account of the baryonic feedback effect in gamma-ray measurements of intergalactic magnetic fields
- Star-formation quenching of cluster galaxies as traced by metallicity, presence of active galactic nuclei, and galactic conformity
- Characterising Tidal Features Around Galaxies in Cosmological Simulations
- Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
- The local PNG bias of neutral Hydrogen,
- Synthetic Large-Scale Galactic Filaments -- on their Formation, Physical Properties, and Resemblance to Observations
- Evolution of Splashback Boundaries and Gaseous Outskirts: Insights from Mergers of Self-similar Galaxy Clusters
- The Triangulum Extended (TREX) Survey: The Stellar Disk Dynamics of M33 as a Function of Stellar Age
- ETHOS - an effective theory of structure formation: formation of the first haloes and their stars
- Observing gas and dust in simulations of star formation with Monte Carlo radiation transport on Voronoi meshes
- Simulating the Carbon Footprint of Galactic Halos
- The low redshift Lyman- Forest as a constraint for models of AGN feedback
- Resonant scattering of the OVII X-ray emission line in the circumgalactic medium of TNG50 galaxies
- Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
- Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
- Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
- On the origin of star formation quenching in massive galaxies at in the cosmological simulations IllustrisTNG
- The AGORA High-resolution Galaxy Simulations Comparison Project. VI. Similarities and Differences in the Circumgalactic Medium
- Non-ideal magnetohydrodynamics on a moving mesh
- Does jackknife scale really matter for accurate large-scale structure covariances?
- The globular cluster system of the Auriga simulations
- The Spin Evolution of Fast-Rotating, Magnetized Super-Chandrasekhar White Dwarfs in the Aftermath of White Dwarf Mergers
- H2 chemistry in galaxy simulations: an improved supernova feedback model
- Magritte, a modern software library for 3D radiative transfer: II. Adaptive ray-tracing, mesh construction and reduction
- Dynamic Fisheye Grids for Binary Black Holes Simulations
- GAMMA: a new method for modeling relativistic hydrodynamics and non-thermal emission on a moving mesh
- A unified scenario for the origin of spiral and elliptical galaxy structural scaling laws
- A Moving Mesh Hydrodynamic Solver for ChaNGa
- Simulating the magnetorotational instability on a moving mesh with the shearing box approximation
- Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
- Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
- Globular Clusters and Streaming Velocities: Testing the new formation channel in high-resolution cosmological simulations
- Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
- The Catalogue for Astrophysical Turbulence Simulations (CATS)
- Group-scale intrinsic galaxy alignments in the Illustris-TNG and MassiveBlack-II simulations
- Local photoionization feedback effects on galaxies
- The IllustrisTNG Simulations: Public Data Release
- SN-driven mechanism of cusp-core transformation: an appraisal
- Why are thermally- and cosmic ray-driven galactic winds fundamentally different?
- Improved Performances in Subsonic Flows of an SPH Scheme with Gradients Estimated using an Integral Approach
- On the density regime probed by HCN emission
- The morphology and kinematics of neutral hydrogen in the vicinity of z=0 galaxies with Milky Way masses -- a study with the Illustris simulation
- A general framework to test gravity using galaxy clusters III: Observable-mass scaling relations in gravity
- Wave mediated angular momentum transport in astrophysical boundary layers
- Numerical challenges for energy conservation in N-body simulations of collapsing self-interacting dark matter halos
- Realistic synthetic integral field spectroscopy with RealSim-IFS
- ELUCID -- Exploring the Local Universe with the reConstructed Initial Density field. II: Reconstruction diagnostics, applied to numerical halo catalogs
- Interacting galaxies in the IllustrisTNG simulations -- V: Comparing the influence of star-forming vs. passive companions
- Out of sight, out of mind? The impact of correlated clustering in substructure lensing
- On the operation of the chemothermal instability in primordial star-forming clouds
- Network Analysis of Cosmic Structures : Network Centrality and Topological Environment
- Catalogue of model star clusters in the Milky Way and M31 galaxies
- The interaction between rising bubbles and cold fronts in cool core clusters
- DS+: a method for the identification of cluster substructures
- Spiral arm instability -- III. Fragmentation of primordial protostellar discs
- Large-scale ordered magnetic fields generated in mergers of helium white dwarfs
- What Is Inside Matters: Simulated Green Valley Galaxies Have Centrally Concentrated Star Formation
- The dependence of episodic accretion on eccentricity during the formation of binary stars
- The Borg Cube Simulation: Cosmological Hydrodynamics with CRK-SPH
- Galaxies with Shells in the Illustris Simulation: Metallicity Signatures
- Supermassive black hole fueling in IllustrisTNG: Impact of environment
- Clumpy galaxies in cosmological simulations: The effect of ISM model
- The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
- Dissect two-halo galactic conformity effect for central galaxies: The dependence of star formation activities on the large-scale environment
- Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
- Self-consistent MHD simulation of jet launching in a neutron star - white dwarf merger
- Spiral-arm instability - II: magnetic destabilisation
- On the relevance of chaos for halo stars in the solar neighbourhood II
- Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
- WALLABY pre-pilot survey: Two dark clouds in the vicinity of NGC 1395
- Cosmological Probes of Structure Growth and Tests of Gravity
- Galactic coronae in Milky Way-like galaxies: the role of stellar feedback in gas accretion
- Time Dependent Radiation Hydrodynamics on a Moving Mesh
- Smoothed Particle Radiation Hydrodynamics: Two-Moment method with Local Eddington Tensor Closure
- Insights from Synthetic Star-forming Regions: I. Reliable Mock Observations from SPH Simulations
- GenASiS: General Astrophysical Simulation System. I. Refinable Mesh and Nonrelativistic Hydrodynamics
- Information field dynamics for simulation scheme construction
- Impact of gas based seeding on supermassive black hole populations at
- A general-purpose timestep criterion for simulations with gravity
- Quantifying the stellar ages of dynamically separated bulges and disks of CALIFA spiral galaxies
- Simulating ionization feedback from young massive stars: impact of numerical resolution
- The THESAN project: Lyman-alpha emitter luminosity function calibration
- Orbital advection with magnetohydrodynamics and vector potential
- Close Encounters of Tight Binary Stars with Stellar-mass Black Holes
- An Extension of the Athena++ Framework for Fully Conservative Self-Gravitating Hydrodynamics
- Classifying and modelling spiral structures in hydrodynamic simulations of astrophysical discs
- The evolutionary pathways of disk galaxies with different sizes
- We are not the 99 percent: quantifying asphericity in the distribution of Local Group satellites
- The Cloud Factory II: Gravoturbulent Kinematics of Resolved Molecular Clouds in a Galactic Potential
- AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
- ART: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines
- The Robustness of Cosmological Hydrodynamic Simulation Predictions to Changes in Numerics and Cooling Physics
- Ultra-high energy cosmic rays deflection by the Intergalactic Magnetic Field
- Inferring the Morphology of Stellar Distribution in TNG50: Twisted and Twisted-Stretched shapes
- Cosmic Web Dissection in Fuzzy Dark Matter Cosmologies
- Simplified galaxy formation with mesh-less hydrodynamics
- cooling and gravitational collapse of supersonically induced gas objects
- Visual Analysis of Large Multivariate Scattered Data using Clustering and Probabilistic Summaries
- The Supersonic Project: To cool or not to cool Supersonically Induced Gas Objects (SIGOs)?
- Simulations of globular clusters within their parent galaxies: Metallicity spreads and anomalous precursor populations
- On the choice of the most suitable indicator for the assembly state of dark matter haloes through cosmic time
- On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias
- Understanding the early stages of galaxy formation using very metal-poor stars from the Hamburg/ESO survey
- Colour and infall time distributions of satellite galaxies in simulated Milky-Way analogs
- Lopsided Galaxies in a cosmological context: a new galaxy-halo connection
- The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
- The impact of galaxy selection on the splashback boundaries of galaxy clusters
- Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies
- Star formation in mergers with cosmologically motivated initial conditions
- Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
- The Physical Origin of the Mass-Size Relation and Its Scatter of Disk Galaxies
- Forecasting the Cross-Correlation of the CSST galaxy survey with the FAST HI Intensity Map
- Magnetic fields do not suppress global star formation in low metallicity dwarf galaxies
- X-ray morphology of cluster-mass haloes in self-interacting dark matter
- Dark matter annihilation and the Galactic Centre Excess
- Gamma-ray emission from spectrally resolved cosmic rays in galaxies
- Non-parametric Morphologies of Mergers in the Illustris Simulation
- Evaluating hydrodynamical simulations with green valley galaxies
- Tidally induced velocity gradients in the Milky Way dwarf spheroidal satellites
- HyPhy: Deep Generative Conditional Posterior Mapping of Hydrodynamical Physics
- The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
- Merger Histories and Environments of Dwarf AGN in IllustrisTNG
- The role of physical and numerical viscosity in hydrodynamical instabilities
- Stellar populations and origin of thick disks in AURIGA simulations
- s-process Enirchment of Ultrafaint Dwarf Galaxies
- Merging galaxy clusters in IllustrisTNG
- AREPO White Dwarf merger simulations resulting in edge-lit detonation and run-away hypervelocity companion
- The effect of dark matter resolution on the collapse of baryons in high redshift numerical simulations
- Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations
- Exploring the non-linear density field in the Millennium simulations with tessellations - I. The probability distribution function
- The magnetised and thermally unstable tails of jellyfish galaxies
- ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
- High-Resolution Panchromatic Spectral Models of Galaxies including Photoionisation and Dust
- Phurbas: An Adaptive, Lagrangian, Meshless, Magnetohydrodynamics Code. I. Algorithm
- The metallicity and star formation activity of long gamma-ray burst hosts for z3: insights from the Illustris simulation
- Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM
- Ageing and Quenching through the ageing diagram: predictions from simulations and observational constraints
- ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
- The THESAN-ZOOM project: central starbursts and inside-out quenching govern galaxy sizes in the early Universe
- Evolution of central galaxy alignments in simulations
- Synthetic observations of spiral arm tracers of a simulated Milky Way analog
- Pairs of Giant Shock Waves (N-Waves) in Merging Galaxy Clusters
- The THESAN-ZOOM project: Population III star formation continues until the end of reionization
- The Stellar Mass Assembly of Low Redshift, Massive, Central Galaxies in SDSS and the TNG300 simulation
- Simulating Hydrodynamics in Cosmology with CRK-HACC
- Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption
- Stellar migration in the Auriga simulations
- The eXtreme Mesh deformation approach (X-MESH) for the Stefan phase-change model
- Cosmic magnetic fields with MASCLET: an application to galaxy clusters
- The MAGPI Survey: Impact of environment on the total internal mass distribution of galaxies in the last 5 Gyr
- Building the molecular cloud population: the role of cloud mergers
- Constraining the coherence scale of the interstellar magnetic field using TeV gamma-ray observations of supernova remnants
- Empirical derivation of the metallicity evolution with time and radius using TNG50 Milky Way/Andromeda analogues
- General Relativistic Hydrodynamics on a Moving-mesh I: Static Spacetimes
- First emergence of cold accretion and supermassive star formation in the early universe
- On the distribution of the Cold Neutral Medium in galaxy discs
- The impact of magnetic fields on cosmological galaxy mergers -- II. Modified angular momentum transport and feedback
- Mock HUBS observations of hot gas with IllustrisTNG
- Planting a Lyman alpha forest on AbacusSummit
- Dynamics and spin alignment in massive, gravito-turbulent circumbinary discs around supermassive black hole binaries
- MIND THE GAP: Is The Too Big To Fail Problem Resolved?
- An ALE residual distribution scheme for the unsteady Euler equations over triangular grids with local mesh adaptation
- Cosmic Ray-Driven Galactic Winds with Resolved ISM and Ion-Neutral Damping
- Galaxies and Halos on Graph Neural Networks: Deep Generative Modeling Scalar and Vector Quantities for Intrinsic Alignment
- nIFTy Galaxy Cluster simulations VI: The dynamical imprint of substructure on gaseous cluster outskirts
- Is the molecular KS relationship universal down to low metallicities?
- Zooming in on the Circumgalactic Medium with GIBLE: the Topology and Draping of Magnetic Fields around Cold Clouds
- The Column Densities of Molecular Gas across Cosmic Time: Bridging Observations and Simulations
- IllustrisTNG Insights: Factors Affecting the Presence of Bars in Disk Galaxies
- Galaxies with kinematically distinct cores in Illustris
- Age-morphology dependence of the Milky Way boxy/peanut bulge seen in Mira variables
- Sloshing of Galaxy Cluster Core Plasma in the Presence of Self-Interacting Dark Matter
- Fast and accurate Voronoi density gridding from Lagrangian hydrodynamics data
- Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
- Genus statistics using the Delaunay tessellation field estimation method: (I) tests with the Millennium Simulation and the SDSS DR7
- Forecasting the power of Higher Order Weak Lensing Statistics with automatically differentiable simulations
- Principal Component Analysis of Galaxy Clustering in Hyperspace of Galaxy Properties
- PATCHWORK: A Multipatch Infrastructure for Multiphysics/Multiscale/Multiframe Fluid Simulations
- Simulating the tidal disruption of stars by stellar-mass black holes using moving-mesh hydrodynamics
- FORECAST: a flexible software to forward model cosmological hydrodynamical simulations mimicking real observations
- Phurbas: An Adaptive, Lagrangian, Meshless, Magnetohydrodynamics Code. II. Implementation and Tests
- Disk flaring with TNG50: diversity across Milky Way and M31 analogs
- Simulating TeV gamma-ray morphologies of shell-type supernova remnants
- Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift
- How do galaxy properties affect void statistics?
- HI within and around observed and simulated galaxy discs -- Comparing MeerKAT observations with mock data from TNG50 and FIRE-2
- Extreme Spheres: Counts-in-cells for 21cm intensity mapping
- On the evolution of the observed Mass-to-Length relationship for star-forming filaments
- Novel Conservative Methods for Adaptive Force Softening in Collisionless and Multi-Species N-Body Simulations
- Gas Accretion and Angular Momentum
- Toward a Physical Understanding of Galaxy-Halo Alignment
- The Voronoi tessellation method in astronomy
- Nested solitons in two-field fuzzy dark matter
- SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
- Galaxy stellar and total mass estimation using machine learning
- Soft X-ray emission from warm gas in IllustrisTNG circum-cluster environments
- The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
- An IllustrisTNG View of the Caustic Technique for Galaxy Cluster Mass Estimation
- Is the core-cusp problem a matter of perspective: Jeans Anisotropic Modeling against numerical simulations
- Simulating cold shear flows on a moving mesh
- Concordance between observations and simulations in the evolution of the mass relation between supermassive black holes and their host galaxies
- Three-point intrinsic alignments of dark matter halos in the IllustrisTNG simulation
- Revision of Faraday rotation measure constraints on the primordial magnetic field using the IllustrisTNG simulation
- Intrinsic alignments of bulges and discs
- Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman- Forest Tomography at
- Dancing in the void: hydrodynamical N-body simulations of the extremely metal poor galaxy DDO 68
- Emulating Sunyaev-Zeldovich Images of Galaxy Clusters using Auto-Encoders
- Towards the impact of GMC collisions on the star formation rate
- Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
- The cooler past of the intracluster medium in TNG-Cluster
- Galaxy-group (halo) alignments from SDSS DR7 and the ELUCID simulation
- The role of 3-body H formation in the fragmentation of primordial gas
- The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
- Not Hydro: Using Neural Networks to estimate galaxy properties on a Dark-Matter-Only simulation
- Non-Equilibrium Abundances Treated Holistically (NEATH): the molecular composition of star-forming clouds
- Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
- High-fidelity reproduction of central galaxy joint distributions with Neural Networks
- Gravitational wave emission from dynamical stellar interactions
- Anisotropic satellite accretion onto the Local Group with HESTIA
- Comparing Implementations of Self-Interacting Dark Matter in the Gizmo and Arepo Codes
- MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
- Living with Neighbors. III. The Origin of the SpinOrbit Alignment of Galaxy Pairs: A Neighbor versus the Large-scale Structure
- Gas stripping and mixing in galaxy clusters: A numerical comparison study
- The Gaia-ESO Survey: Matching Chemo-Dynamical Simulations to Observations of the Milky Way
- Imprints of Zero-Age Velocity Dispersions and Dynamical Heating on the Age-Velocity dispersion Relation
- Shape and Spin of Minihaloes. II: The Effect of Streaming Velocities
- Bar-driven dispersal of Galactic substructure
- Gas Cooling in Hydrodynamic Simulations with An Exact Time Integration Scheme
- Observing the stellar halo of Andromeda in cosmological simulations: the Auriga2PAndAS pipeline
- Tracing the evolutionary pathways of dust and cold gas in high-z quiescent galaxies with SIMBA
- COALAS III: The ATCA CO(1-0) look at the growth and death of H emitters in the Spiderweb protocluster at z=2.16
- Bursty Star Formation in Dwarfs is Sensitive to Numerical Choices in Supernova Feedback Models
- Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
- Classification of cosmic structures for galaxies with deep learning: connecting cosmological simulations with observations
- Feasibility of detecting shadows in disks induced by infall
- Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
- Formation of super-thin galaxies in Illustris-TNG
- RJ-plots: An improved method to classify structures objectively
- Simultaneous Dependence of Matter Clustering on Scale and Environment
- Cloud properties across spatial scales in simulations of the interstellar medium
- Equalizing resolution in smoothed-particle hydrodynamics calculations using self-adaptive sinc kernels
- A robust determination of halo environment in the cosmic field
- Where are the extremely metal-poor stars in the Milky Way and Andromeda? Expectations from TNG50
- Planet-disc interactions with Discontinuous Galerkin Methods using GPUs
- Mesh-free hydrodynamics in PKDGRAV3 for galaxy formation simulations
- The AGORA High-Resolution Galaxy Simulations Comparison Project VII: Satellite quenching in zoom-in simulation of a Milky Way-mass halo
- The undiscovered ultra-diffuse galaxies of the Local Group
- How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
- Detecting the Cosmic Web: Lyα Emission from Simulated Filaments at z=3
- Gravito-turbulence in local disk simulations with an adaptive moving mesh
- Over-massive Central Black Holes in the Cosmological Simulations ASTRID and Illustris TNG50
- Removal and mixing of the coronal gas from satellites in galaxy groups: cooling the intragoup gas
- Sensitivity of non-radiative cloud-wind interactions to the hydrodynamics solver
- Active Learning for Computationally Efficient Distribution of Binary Evolution Simulations
- Velocity-dependent annihilation radiation from dark matter subhalos in cosmological simulations
- The velocity structure of the intracluster medium during a major merger: simulated microcalorimeter observations
- SEAGLE--III: Towards resolving the mismatch in the dark-matter fraction in early-type galaxies between simulations and observations
- REMIX SPH -- improving mixing in smoothed particle hydrodynamics simulations using a generalised, material-independent approach
- Supernova Shocks Cannot Explain the Inflated State of Hypervelocity Runaways from White Dwarf Binaries
- A field-level emulator for modeling baryonic effects across hydrodynamic simulations
- WVTICs -- SPH initial conditions for everyone
- The Supersonic Project: The eccentricity and rotational support of SIGOs and DM GHOSts
- The dispersion measure and scattering of Fast Radio Bursts: contributions from multi-components, and clues for the intrinsic properties
- A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
- An off-centred bulge or a satellite? Hydrodynamical -body simulations of the disc galaxy NGC 5474
- Detecting preheating in proto-clusters with Lyman- Forest Tomography
- Learning the Universe: Cosmological and Astrophysical Parameter Inference with Galaxy Luminosity Functions and Colours
- High-Frequency Voronoi Noise Reduced by Smoothed Mesh Motion
- Chemodynamics of dwarf galaxies under ram-pressure
- A positivity-preserving and conservative high-order flux reconstruction method for the polyatomic Boltzmann--BGK equation
- Voronoi Tessellation and Non-parametric Halo Concentration
- Formation and fate of low metallicity stars in IllustrisTNG50
- CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- I. Constraining physical processes in local star-forming galaxies
- Probabilistic model for dynamic galaxy decomposition
- Implications of galaxy buildup for putative IMF variations in massive galaxies
- Accretion onto supermassive and intermediate mass black holes in cosmological simulations
- Voronoi binning: Optimal adaptive tessellations of multi-dimensional data
- High-order Discontinuous Galerkin hydrodynamics with sub-cell shock capturing on GPUs
- Close encounters of black hole - star binaries with stellar-mass black holes
- Searching for HI around MHONGOOSE Galaxies via Spectral Stacking
- Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?
- The Sweep Method for radiative Transfer in Arepo
- Towards an accurate model of small-scale redshift-space distortions in modified gravity
- Can HI 21 cm line trace the Missing Baryons in the Filamentary Structures?
- The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
- Magnetically driven outflows in 3D common-envelope evolution of massive stars
- A super-Chandrasekhar mass type Ia supernova progenitor at 49 pc set to detonate in 23 Gyr
- Mass-morphology relation of TNG50 galaxies
- Discrimination of heavy elements originating from Pop III stars in z = 3 intergalactic medium
- A Vorticity-Preserving Hydrodynamical Scheme for Modeling Accretion Disk Flows
- The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
- Baryonic Effects on Lagrangian Clustering and Angular Momentum Reconstruction
- How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
- Studying the Warm Hot Intergalactic Medium in emission: a reprise
- Numerical dependencies of the galactic dynamo in isolated galaxies with SPH
- Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
- Structure-preserving finite-element schemes for the Euler-Poisson equations
- The role of accreted and in situ populations in shaping the stellar halos of low-mass galaxies
- Correlations of Dark Matter, Gas and Stellar Profiles in Dark Matter Halos
- A physically motivated galaxy size definition across different state-of-the-art hydrodynamical simulations
- Physics of a partially ionized gas relevant to galaxy formation simulations -- the ionization potential energy reservoir
- The mass-dependent UVJ diagram at cosmic noon: A challenge for galaxy evolution models and dust radiative transfer
- The Ursa Major Association of Galaxies. VI: A relative dearth of gas-rich dwarf galaxies
- What drives the corpulence of galaxies? I. The formation of central compact dwarf galaxies in TNG50
- Shape and Spin of Minihaloes: From Large Scales to the Centres
- On the detectability of massive black hole merger eventsby LISA
- Entropy-Conserving Scheme for Modeling Nonthermal Energies in Fluid Dynamics Simulations
- Searching for the shadows of giants II: the effect of local ionisation on the Lyman- absorption signatures of protoclusters at redshift
- An observational testbed for cosmological zoom-in simulations: constraining stellar migration in the solar cylinder using asteroseismology
- HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
- Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
- Two Particle-in-Grid Realisations on Spacetrees
- The parametrization of gas flows in discs in the Auriga simulations
- On the Origin of High-velocity Clouds in the Galaxy
- Does the chemothermal instability have any role in the fragmentation of primordial gas
- Zooming in on the Circumgalactic Medium with GIBLE: Tracing the Origin and Evolution of Cold Clouds
- On the effects of rotation in primordial star-forming clouds
- The Alcock Paczynski test with 21cm intensity field
- Cosmological gas accretion history onto the stellar discs of Milky Way-like galaxies in the Auriga simulations -- (I) Temporal dependency
- Well balanced finite volume schemes for shallow water equations on manifolds
- Grid Noise in Moving Mesh Codes: Fixing The Volume Inconsistency Problem
- Deciphering the Milky Way disc formation time encrypted in the bar chrono-kinematics
- The Formation of a Milky Way-sized Disk Galaxy 1. A Comparison of Numerical Methods
- The Origin of Massive Compact Galaxies: Lessons from IllustrisTNG
- Addressing via N-body simulations the distribution of the satellite tidal debris in the Milky Way environment
- Modelling the 3D physical structure of astrophysical sources with GASS
- High-redshift test of gravity using enhanced growth of small structures probed by the neutral hydrogen distribution
- MaNGA DynPop -- VI. Matter density slopes from dynamical models of 6000 galaxies versus cosmological simulations: the interplay between baryonic and dark matter
- Kinematic signatures of impulsive supernova feedback in dwarf galaxies
- The survival of stellar discs in Fornax-like environments, from TNG50 to real galaxies
- Intra-Cluster Light as a Dynamical Clock for Galaxy Clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea and Horizon-AGN Simulations
- Metallicity beats sSFR: The connection between superluminous supernova host galaxy environments and the importance of metallicity for their production
- Space-time adaptive ADER-DG finite element method with LST-DG predictor and a posteriori sub-cell ADER-WENO finite-volume limiting for multidimensional detonation waves simulation
- Simulated [CII] in high-z galaxies
- The impact of hyperons on neutron star mergers: gravitational waves, mass ejection and black hole formation
- Initial sizes of star clusters: implications for cluster dissolution during galaxy evolution
- Anisotropic correlation functions as tracers of central galaxy alignments in simulations
- Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
- From Gas to Stars Over Cosmic Time
- The feasibility of constraining DM interactions with high-redshift observations by JWST
- Tree-less 3d Friends-of-Friends using Spatial Hashing
- Moving and Reactive Boundary Conditions in Moving-Mesh Hydrodynamics
- A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
- Fingerprints of modified gravity on galaxies in voids
- Euclid preparation. LXVIII. Extracting physical parameters from galaxies with machine learning
- Disparate Effects of Circumgalactic Medium Angular Momentum in IllustrisTNG and SIMBA
- Spin speed correlations and the evolution of galaxy-halo systems
- Measuring the mass and concentration of dark matter halos from the velocity dispersion profile of their stars
- Euclid preparation LXXI. Simulations and nonlinearities beyond CDM. 3. Constraints on models from the photometric primary probes
- Quantifying the intrinsic variability due to randomness of the Auriga galaxy formation model
- On the origin of Jupiter's fuzzy core: constraints from N-body, impact and evolution simulations
- Studying galaxy cluster morphological metrics with Mock-X
- Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
- Active galactic nuclei feedback in an elliptical galaxy (III): the impacts and fate of cosmological inflow
- Galilean invariance of shallow cumulus convection large-eddy simulations
- Galaxy populations in protoclusters at cosmic noon
- On the Tremaine-Weinberg method: how much can we trust gas tracers to measure pattern speeds?
- Overmassive black holes in the early Universe can be explained by gas-rich, dark matter-dominated galaxies
- Modeling Post-Reionization HI Distributions in Fuzzy Dark Matter Cosmologies Using Conditional Normalizing Flows
- Testing the effect of resolution on gravitational fragmentation with Lagrangian hydrodynamic schemes
- Quenched, bulge-dominated, but dynamically cold galaxies in IllustrisTNG and their real-world counterparts
- Fragmentation of ring galaxies and transformation to clumpy galaxies
- Dark Matter Annihilation Feedback in cosmological simulations I: Code convergence and idealised halos
- Asymmetric Drift of Andromeda Analogs in the IllustrisTNG Simulation
- The impact of filaments on dwarf galaxy properties in the Auriga simulations
- Haloes at the ragged edge: The importance of the splashback radius
- Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
- Observational Diagnostics of Gas Flows: Insights from Cosmological Simulations
- Conservation of radial actions in time-dependent spherical potentials
- Mass accretion rates of the HectoMAP clusters of galaxies
- Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
- Multidimensional upwind hydrodynamics on unstructured meshes using Graphics Processing Units I. Two-dimensional uniform meshes
- NOEMA: A first kpc resolution study of a main sequence barred galaxy channeling gas into a growing bulge
- A Novel Scheme for Dark Matter Annihilation Feedback in Cosmological Simulations
- Realistic consecutive galaxy mergers form eccentric PTA sources
- A new long gamma-ray burst formation pathway at solar metallicity
- The life cycle of giant molecular clouds in simulated Milky Way-mass galaxies
- Influence of mergers on LyC escape of high redshift galaxies
- A comparison between semi-analytical gas cooling models and cosmological hydrodynamical simulations
- Understanding the Baryon Cycle: Fueling Star Formation via Inflows in Milky Way-like Galaxies
- Mapping gravity in stellar nurseries -- establishing the effectiveness of 2D acceleration maps
- The origin of hypervelocity white dwarfs in the merger-disruption of He-CO white dwarfs
- Matter power spectrum induced by primordial magnetic fields: from the linear to the non-linear regime
- Euclid preparation. Simulations and nonlinearities beyond CDM. 1. Numerical methods and validation
- NeutralUniverseMachine: How Filaments and Dark Matter Halo Influence the Galaxy Cold Gas Content
- Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping
- Accelerating self-gravitating hydrodynamics simulations with adaptive force updates
- Modelling of ionising feedback with Smoothed Particle Hydrodynamics and Monte Carlo Radiative Transfer on a Voronoi grid
- The Effect of Impact Parameter on Tidal Disruption Events
- Revisiting the Relationship between the Long GRB Rate and Cosmic Star Formation History Based on a Large Swift Sample
- How complex is the cosmic web?
- WENO-Wombat: Scalable Fifth-Order Constrained-Transport Magnetohydrodynamics for Astrophysical Applications
- Paicos: A Python package for analysis of (cosmological) simulations performed with Arepo
- What Drives Cluster Cool-Core Transformations? A Population Level Analysis of TNG-Cluster
- Disc fragmentation and oligarchic growth of protostellar systems in low-metallicity gas clouds
- Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
- Internal r-process abundance spread of M15 and a single stellar population model
- Baryon effects on the dark matter halos constrained from strong gravitational lensing
- A deep-learning approach to the 3D reconstruction of dust density and temperature in star-forming regions
- Decaying turbulence in molecular clouds: how does it affect filament networks and star formation?
- Jet interaction with galaxy cluster mergers
- Merger Conditions of Population III Protostar Binaries
- Structure and large scale environment of galaxy pairs in the S-PLUS DR4
- Differentiable Cosmological Hydrodynamics for Field-Level Inference and High Dimensional Parameter Constraints
- Orbit properties of massive prolate galaxies in the Illustris simulation
- Central galaxy alignments. Dependence on the mass and the large-scale environment
- Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
- The galaxy bias profile of cosmic voids
- A self-gravity module for the PLUTO code
- Filament Formation via Collision-induced Magnetic Reconnection -- Formation of a Star Cluster
- Exploring the centre of mass properties of LG-like galaxies
- The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
- Prospects for detecting cosmic filaments in Lyman-alpha emission across redshifts
- Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
- Gas Dynamics in the Central Molecular Zone and its connection with the Galactic Bar
- Galaxy formation from a timescale perspective
- A Sea of Black Holes: Characterizing the LISA Signature for Stellar-Origin Black Hole Binaries
- Integer Lattice Dynamics for Vlasov-Poisson
- Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
- From order to chaos: the blurred out metallicity gradient of the Gaia-Enceladus/Sausage progenitor
- The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies
- Unraveling emission line galaxy conformity at z~1 with DESI early data
- RAM: Rapid Advection Algorithm on Arbitrary Meshes
- The effects of environment on galaxies' dynamical structures: From simulations to observations
- Premature supermassive black hole mergers in cosmological simulations of structure formation
- The internal metallicity distributions of simulated galaxies from EAGLE, Illustris, and IllustrisTNG at z=1.8-4 as probed by Gamma Ray Burst hosts
- Polynomial expansion of the star formation history in galaxies
- The spatial distribution deviation and the power suppression of baryons from dark matter
- The dynamical impact of cosmic rays in the Rhea magnetohydrodynamics simulations
- High order well-balanced Arbitrary-Lagrangian-Eulerian ADER discontinuous Galerkin schemes on general polygonal moving meshes
- Growth of Light Seed Black Holes in the Early Universe
- Constraint on magnetized galactic outflows from LOFAR rotation measure data
- Complexity Phenomena and ROMA of the Magnetospheric Cusp, Hydrodynamic Turbulence, and the Cosmic Web
- Angular-momentum conservation in discretization of Navier-Stokes equation for viscous fluids
- SPH Methods in the Modelling of Compact Objects
- Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation
- Cosmological boost factor for dark matter annihilation at redshifts of - using the power spectrum approach
- Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
- Turbulence revealed by wavelet transform: power spectrum and intermittency for the velocity field of the cosmic baryonic fluid
- Recovering the pattern speeds of edge-on barred galaxies via an orbit-superposition method
- An MHD spectral theory approach to Jeans' magnetized gravitational instability
- IllustrisTNG and S2COSMOS: possible conflicts in the evolution of neutral gas and dust
- Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
- Gaseous Dynamical Friction: a Numerical Study of Extended Perturbers
- The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM
- Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
- An Improved and Physically-Motivated Scheme for Matching Galaxies with Dark Matter Halos
- The evolution of low-mass central galaxies in the vicinity of massive structures and its impact on the two-halo conformity
- Shape and connectivity of groups and clusters: Impact of dynamical state and accretion history
- First resolved stellar halo kinematics of a MW-mass galaxy outside the Local Group: A flat counter-rotating halo in NGC 4945
- CRexit: how different cosmic ray transport modes affect thermal instability in the circumgalactic medium
- Kinematics of the Local Group gas and galaxies in the Hestia simulations
- Population III star formation: multiple gas phases prevent the use of an equation of state at high densities
- TODDLERS: A New UV to Millimeter Emission Library for Star-Forming Regions. II. Star Formation Rate Indicators Using Auriga Zoom Simulations
- Tetrahedral grids in Monte Carlo radiative transfer
- Tracing the Origins of Hot Halo Gas in Milky Way-Type Galaxies with SMUGGLE
- Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
- A statistical study of lopsided galaxies using random forest
- Halo Mergers Enhance the Growth of Massive Black Hole Seeds
- The Impact of Baryons on the Large-Scale Structure of the Universe
- syren-baryon: Analytic emulators for the impact of baryons on the matter power spectrum
- Cosmological gas accretion history onto the stellar discs of Milky Way-like galaxies in the Auriga simulations -- (II) The inside-out growth of discs
- How do uncertainties in galaxy formation physics impact field-level galaxy bias?
- Euclid preparation. Spatially resolved stellar populations of local galaxies with Euclid: a proof of concept using synthetic images with the TNG50 simulation
- Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
- C2-GaMe: Classification of Cluster Galaxy Membership with Machine Learning
- Testing the stability of supersonic ionized Bondi accretion flows with radiation hydrodynamics
- How gravitational softening affects galaxy stability I. Linear mode analysis of disc galaxies
- Spin alignment around TNG300-1 voids
- Impact of primordial black holes on the formation of the first stars and galaxies
- Supersonic turbulence simulations with GPU-based high-order Discontinuous Galerkin hydrodynamics
- The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
- The Impact of Classical Bulges on Stellar Bars and Box-Peanut-X-Features in Disk Galaxies
- Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations
- Machine Learning and Structure Formation in Modified Gravity
- The collaborative effect of ram pressure and merging on star formation and stripping fraction
- Performance of high-order Godunov-type methods in simulations of astrophysical low Mach number flows
- Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
- Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
- On the interaction of a Bonnor-Ebert sphere with a stellar wind
- Turbulence, Thermal Pressure, and Their Dynamical Effects on Cosmic Baryonic Fluid
- Challenges in Cosmic Magnification Reconstruction by Magnification Response
- Auriga Streams II: orbital properties of tidally disrupting satellites of Milky Way-mass galaxies
- Counts-in-Cells of subhaloes in the IllustrisTNG simulations: the role of baryonic physics
- Ionisation in Turbulent Magnetic Molecular Clouds I. Effect on Density and Mass-to-Flux Ratio Structures
- Numerical Simulations of the Dark Universe: State of the Art and the Next Decade
- Stellar halos tracing the assembly of ultra-faint dwarf galaxies
- IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L Galaxies
- The breakBRD Breakdown: Using IllustrisTNG to Track the Quenching of an Observationally-Motivated Sample of Centrally Star-Forming Galaxies
- Gravitational collapse at low to moderate Mach numbers: The relationship between star formation efficiency and the fraction of mass in the massive object
- Redshift and stellar mass dependence of intrinsic shapes of disc-dominated galaxies from COSMOS observations below
- Reorientation Rates of Structural and Kinematic Axes in Simulated Massive Galaxies and the Origins of Prolate Rotation
- New Cold Dark Matter Crisis Revealed by Multiscale Cluster Lensing
- Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos
- Dust destruction by the supernova remnant forward shock in a turbulent interstellar medium
- Angular momentum distribution during the collapse of primordial star-forming clouds
- The AGORA High-resolution Galaxy Simulations Comparison Project. X: Formation and Evolution of Galaxies at the High-redshift Frontier
- Mass-Conserving Implicit-Explicit Methods for Coupled Compressible Navier-Stokes Equations
- Parameterization of Stochasticity in Galaxy Clustering and Reconstruction of Tomographic Matter Clustering
- The mass and galaxy distribution around SZ-selected clusters
- Cosmology with One Galaxy: Auto-Encoding the Galaxy Properties Manifold
- The evolution of the barred galaxy population in the TNG50 simulation
- Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
- Densified pupil spectrograph as high-precision radial velocimetry: From direct measurement of the Universe's expansion history to characterization of nearby habitable planet candidates
- Late encounter-events as a source of disks and spiral structures -- Forming second generation disks
- Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies
- High-redshift AGN population in radiation-hydrodynamics simulations
- Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
- A general relativistic extension to mesh-free methods for hydrodynamics
- Variational Integration for Ideal Magnetohydrodynamics and Formation of Current Singularities
- The role of magnetic fields in ram pressure stripping of satellite galaxies in the circumgalactic medium around massive galaxies
- Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
- Isentropic 'shock waves' in numerical simulations of astrophysical bodies
- GrAviPaSt's Lens to the Past: Unveiling the Evolution of Filamentary Structures
- Balancing the load: A Voronoi based scheme for parallel computations
- Field-Level Comparison and Robustness Analysis of Cosmological N-body Simulations
- Physically motivated modeling of LyC escape fraction during reionization
- Tracing the origins of galaxy lopsidedness across cosmic time
- Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
- Atomic and Molecular Phases of the Interstellar Medium
- Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
- Investigations of MWISP Filaments. I. Filament Identification and Analysis Algorithms, and Source Catalogue
- Uncover 3D Dark Matter Distribution of the Milky Way by an Empirical Triaxial Orbit-Superposition Model: Method Validation
- Population Synthesis of Gravitational Wave Sources
- You Are What You Eat: The Circumgalactic Medium Around BreakBRD Galaxies has Low Mass and Angular Momentum
- SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
- Why take the square root? An assessment of interstellar magnetic field strength estimation methods
- No dilute core produced in simulations of giant impacts on to Jupiter
- Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations
- A scalable exponential-DG approach for nonlinear conservation laws: with application to Burger and Euler equations
- The fragmentation of molecular clouds in starburst environments
- Analytic growth rate of gravitational instability in self-gravitating planar polytropes
- GenASiS: General Astrophysical Simulation System. II. Nonrelativistic Hydrodynamics
- A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos
- Exploring the Angular Momentum -- Atomic Gas Content Connection with EAGLE and IllustrisTNG
- Star Formation for Predictive Primordial Galaxy Formation
- HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
- Improving the Accuracy of Halo Mass Based Statistics For Fast Approximate N-body Simulations
- The THESAN project: environmental drivers of Local Group reionization
- A New Residual Distribution Hydrodynamics Solver for Astrophysical Simulations
- A general relativistic magnetohydrodynamics extension to mesh-less schemes in the code GIZMO
- Photometric and Kinematic Misalignments and Their Evolution Among Fast and Slow Rotators in the Illustris Simulation
- Spatial field reconstruction with INLA: Application to simulated galaxies
- The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
- Cosmology with Topological Deep Learning
- Accreted stars and stellar haloes of simulated galaxies in TNG50
- Auriga Superstars: Improving the resolution and fidelity of stellar dynamics in cosmological galaxy simulations
- On the effects of parameters on galaxy properties in CAMELS and the predictability of
- Deciphering the explosion mechanism of Type Ia SNe using their remnants II: a deep dive into double detonations with SNR 0509-67.5
- Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way
- Thermonuclear explosion criteria for direct and indirect collisions of CO white dwarfs: a study of the impact-parameter threshold for detonation
- Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
- Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
- From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
- The Supersonic Project: SIGOs, a Proposed Progenitor to Globular Clusters, and their Connections to Gravitational Wave Anisotropies
- Exploring the halo-galaxy connection with probabilistic approaches
- Merger Tree-based Galaxy Matching: A Comparative Study Across Different Resolutions
- Novel Hydrodynamic Schemes Capturing Shocks and Contact Discontinuities and Comparison Study with Existing Methods
- Environment matters: stronger magnetic fields in satellite galaxies
- The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
- Magnetic fields in the intracluster medium with TNG-Cluster: properties, morphology, and tangential anisotropy
- Core collapse in resonant self-interacting dark matter across two decades in halo mass
- Evidence of .Ia Supernova Detonations in 3D Hydrodynamical Simulations of Double Degenerate Mergers
- Numerical effects on the stripping of dark matter and stars in IllustrisTNG galaxy groups and clusters
- The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
- An Observationally Driven Multifield Approach for Probing the Circum-Galactic Medium with Convolutional Neural Networks
- A Co-Scaling Grid for Athena++
- Dissecting the mass quenching in TNG50: Galaxy size determines the quenching mode
- The Complexity and Information Content of Simulated Universes
- Plasma processes at the scales of galaxies and clusters of galaxies
- Blueberry and Green Pea galaxies live in low density environments
- Hunting for the signatures of molecular cloud formation
- Violent mergers revisited: The origin of the fastest stars in the Galaxy
- A novel analysis of contamination in Lyman-break galaxy samples at : spatial correlation with intermediate-redshift galaxies at
- Gravitational Self-force Errors of Poisson Solvers on Adaptively Refined Meshes
- Numerical Methods for Simulating Star Formation
- Quantifying Advantages of a Moving Mesh in Nuclear Hydrodynamics
- SPH Entropy Errors and the Pressure Blip
- Towards an Observational Detection of Halo Spin Bias using Spin-Orbit Coherence
- Entropy Stable Discontinuous Galerkin Schemes on Moving Meshes with Summation-by-Parts Property for Hyperbolic Conservation Laws
- Tracing black hole and galaxy growth across environments since cosmic noon
- Galaxy Velocity Bias in Cosmological Simulations: Towards Percent-level Calibration
- Detecting and analysing the topology of the cosmic web with spatial clustering algorithms I: Methods
- The mass and redshift dependence of halo star clustering
- The abundance and origin of cool gas in galaxy clusters in the TNG-Cluster simulation
- Soft X-ray line emission from hot gas in intervening galaxy halos and diffuse gas in the cosmic web
- Neutron Star-Main Sequence Collisions Robustly Form Dynamically Stable Thorne-Żytkow Objects
- Accreted Globular Clusters in External Galaxies: Why Adaptive Dynamics is not the Solution
- Using two point correlation functions to understand the assembly histories of Milky Way-like galaxies
- The asymmetry of white dwarf double detonations and the observed scatter around the Phillips relation
- Galaxy-halo internal alignments across cosmic time
- Resolving vortices with an isothermal HLLC Riemann solver
- Stirring Things Up: Bar-induced substructures in the stellar halo of a cosmological Milky Way analogue
- Constraining the Nature of Dark Matter from Tidal Radii of Cluster Galaxy Subhalos
- How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
- The multi-component fitting to the star formation histories in the TNG simulation
- High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA
- Simulating cosmic ray electron spectra and radio emission from an AGN jet outburst in a cool-core cluster
- The large-scale distribution of ionized metals in IllustrisTNG
- Galaxy clustering in modified gravity from full-physics simulations. I: two-point correlation functions
- The Kelvin-Helmholtz instability and smoothed particle hydrodynamics
- Influence of Barlens on the Bulge Parameters in the 2D Image Decomposition
- Systematics in ETG Mass Profile Modelling: Strong Lensing & Stellar Dynamics
- RIGEL: Feedback-regulated cloud-scale star formation efficiency in a simulated dwarf galaxy merger
- ODIN: Using multiplicity of Lyman-Alpha Emitters to assess star formation activity in dark matter halos
- Quadrupole signature as a kinematic diagnostic to constrain bar properties : implications for the Milky Way
- The PARADIGM project II: The lifetimes and quenching of satellites in Milky Way-mass haloes
- Asymmetrical thermonuclear supernovae triggered by the tidal disruption of white dwarfs
- Boxy/Peanut Bulges: Comparative Analysis of EGIPS Galaxies and TNG50 Models
- Statistical Properties of Cold Streams In Massive Star-Forming Halos in TNG50
- Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
- Towards Higher Order Accuracy in Self-Gravitating Hydrodynamics
- Disc instability and bar formation: view from the IllustrisTNG simulations
- How Many Bursts Does it Take to Form a Core at the Center of a Galaxy?
- Violent mergers can explain the inflated state of some of the fastest stars in the Galaxy
- Exploring the evolution of red and blue galaxies in different cosmic web environments using IllustrisTNG simulation
- Bridging Simulations and Observations: New Insights into Galaxy Formation Simulations via Out-of-Distribution Detection and Bayesian Model Comparison
- The impact of cosmic filaments on the abundance of satellite galaxies
- On the dependence of galaxy assembly bias on the selection criteria, number density, and redshift of galaxy samples
- Variability in Cosmological Hydrodynamical Simulations: how Stochastic Processes, Numerical Effects, and Reproducibility Limits impact Predictability
- Constraining Galaxy-Halo Connection Using Machine Learning
- Centrally concentrated star formation in young clusters
- The frame-dragging vector potential on galaxy scales from Dark-Matter-only Newtonian -body simulations
- Stellar populations of stellar halos: Results from the Illustris simulation
- Newcomers and suburbanites can drive the evolution of the size-stellar mass relation of early type galaxies in galaxy clusters
- Light curves and spectra for stellar collisions between main-sequence stars in galactic nuclei
- Galaxy clustering in the VVV Near-IR Galaxy Catalogue
- The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
- Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling
- Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl
- Dynamic Zoom Simulations of structure formation beyond standard cosmology
- Preferential accretion of binary stars
- On the consistency of jet feedback modelling across different astrophysics hydrodynamical codes
- Extreme Metallicity Dwarf Galaxies in IllustrisTNG
- Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations
- iPTF16geu through the lens of thermonuclear explosion models
- Machine Learning for Galactic Archaeology: A chemistry-based neural network method for identification of accreted disc stars
- Inferring the mass of the circumgalactic medium using X-ray resonant scattering
- A New Method to Simulate Dark Matter-Baryon Interactions and Application to an Isolated Disk Galaxy
- Imladris: a detailed and flexible model for galaxy simulations with individual stars
- The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
- Fast Baryonic Field Painting for Sunyaev-Zel'dovich Analyses: Transfer Function vs. Hybrid Effective Field Theory
- Gas flows in galaxy mergers: supersonic turbulence in bridges, accretion from the circumgalactic medium, and metallicity dilution
- A general framework for unbiased tests of gravity using galaxy clusters
- Network of Star Formation: Fragmentation controlled by scale-dependent turbulent pressure and accretion onto the massive cores revealed in the Cygnus-X GMC complex
- The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around in the IllustrisTNG model
- On the scale-height of the molecular gas disc in Milky Way-like galaxies
- On the interaction of a thin, supersonic shell with a molecular cloud
- DeepVoid: A Deep Learning Void Detector
- Intrinsic alignments of galaxies in multiple projections
- Tracing correlations between galaxy properties across the Cosmic Web: An IllustrisTNG-based study
- ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations
- Spectrally resolved cosmic rays: II -- Momentum-dependent cosmic ray diffusion drives powerful galactic winds
- Modeling Multiphase Galactic Outflows: A Multifluid Moving Mesh Approach
- Optimized smoothing kernels for SPH
- Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
- Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
- Deciphering the explosion mechanism of Type-Ia SNe using their remnants I: general properties and a case study on Tycho's SNR
- The small-scale turbulent dynamo in smoothed particle magnetohydrodynamics
- OpenGadget3 GPU solver tests
- The impact of radial migration on disk galaxy star formation histories: II. Role of bar strength, disk thickness, and merger history
- LYRA II: Cosmological dwarf galaxy formation with inhomogeneous Population III enrichment
- The Filament Rift: CDM's Structural Challenge Against Observation
- Prospects for studying million-degree gas in the Milky Way halo using the forbidden optical [FeX] and [FeXIV] intersystem lines
- SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
- Connecting galaxy evolution in clusters with their radial profiles and phase space distribution: results from the IllustrisTNG hydrodynamical simulations
- Sample Variance Denoising in Cylindrical 21-cm Power Spectra
- High and low Sérsic index bulges in Milky Way- and M31-like galaxies: origin and connection to the bar with TNG50
- Mesoscopic Energy Ranking Constraints in the IllustrisTNG Simulations
- Mimicking the halo-galaxy connection using machine learning
- NeutralUniverseMachine: Predictions of HI gas in Different Theoretical Models
- PatchworkWave: A Multipatch Infrastructure for Multiphysics/Multiscale/Multiframe/Multimethod Simulations at Arbitrary Order
- Time-dependent adaptive mesh refinement solver for the Gross-Pitaevskii-Poisson equations
- Broken Expectations: The Effects of Modelling Assumptions on the Inferred Dark Matter Distribution in the Milky Way's Satellites
- Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
- Hydromagnetic waves in an expanding universe -- cosmological MHD code tests using analytic solutions
- Cosmological simulations predict that AGN preferentially live in gas-rich, star-forming galaxies despite effective feedback
- The halo finding problem revisited: a deep revision of the ASOHF code
- Exploring the effect of baryons on the radial distribution of satellite galaxies with GAMA and IllustrisTNG
- Residual cross-grid flow numerical error in large-eddy simulations of cumulus-topped boundary layers
- Calibrating the SIDM Gravothermal Catastrophe with N-body Simulations
- Why most molecular clouds are gravitationally dominated
- Mainly on the Plane: Observing the Extended, Ionized Disks of Milky Way Analogs in IllustrisTNG
- The DORCHA suite: nature, nurture, and the phase space distribution of the Milky Way's high redshift progenitors today
- Semi-empirical constraints on the HI mass function of star-forming galaxies and at from interferometric surveys
- The History of Galaxy Mergers in IllustrisTNG
- Transferring Data from a Voronoi Mesh to an Adaptive Cartesian Grid in Pursuit of Self-consistent Top-down Star Formation
- Shape asymmetries and the relation between lopsidedness and radial alignment in simulated galaxies
- Stealing galaxies from galaxy clusters
- Interferometer predictions with triangulated images: solving the multi-scale problem
- CWTHF: Subhalo Identification with Continuous Wavelet Transform
- Role of prompt cusps in driving the core collapse of SIDM halos
- On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
- Estimating the triaxiality of massive clusters from 2D observables in MillenniumTNG with machine learning
- Large-scale semi-discrete optimal transport with distributed Voronoi diagrams
- 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