A Multi-Code Analysis Toolkit for Astrophysical Simulation Data

Abstract

The analysis of complex multiphysics astrophysical simulations presents a unique and rapidly growing set of challenges: reproducibility, parallelization, and vast increases in data size and complexity chief among them. In order to meet these challenges, and in order to open up new avenues for collaboration between users of multiple simulation platforms, we present yt (available at http://yt.enzotools.org/), an open source, community-developed astrophysical analysis and visualization toolkit. Analysis and visualization with yt are oriented around physically relevant quantities rather than quantities native to astrophysical simulation codes. While originally designed for handling Enzo's structure adaptive mesh refinement (AMR) data, yt has been extended to work with several different simulation methods and simulation codes including Orion, RAMSES, and FLASH. We report on its methods for reading, handling, and visualizing data, including projections, multivariate volume rendering, multi-dimensional histograms, halo finding, light cone generation and topologically-connected isocontour identification. Furthermore, we discuss the underlying algorithms yt uses for processing and visualizing data, and its mechanisms for parallelization of analysis tasks.

18 pages, 6 figures, emulateapj format. Resubmitted to Astrophysical Journal Supplement Series with revisions from referee. yt can be found at http://yt.enzotools.org/

References in corpus (25)

• The cosmological simulation code GADGET-2
• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES
• PLUTO: a Numerical Code for Computational Astrophysics
• Adaptive Refinement Tree - a new high-resolution N-body code for cosmological simulations
• The Statistics of Supersonic Isothermal Turbulence
• HOP: A New Group-Finding Algorithm for N-body Simulations
• The Formation of Population III Binaries from Cosmological Initial Conditions
• Bimodal gas accretion in the Horizon-MareNostrum galaxy formation simulation
• Simulating Radiating and Magnetized Flows in Multi-Dimensions with ZEUS-MP
• Embedding Lagrangian Sink Particles in Eulerian Grids
• The HII Region of a Primordial Star
• Equations and Algorithms for Mixed Frame Flux-Limited Diffusion Radiation Hydrodynamics
• Three Modes of Metal-Enriched Star Formation in the Early Universe
• Metal Cooling in Simulations of Cosmic Structure Formation
• Numerical Simulations of Supernova Dust Destruction. I. Cloud-crushing and Post-processed Grain Sputtering
• Galaxy Clusters at the Edge: Temperature, Entropy, and Gas Dynamics at the Virial Radius
• The Santa Fe Light Cone Simulation Project: I. Confusion and the WHIM in Upcoming Sunyaev-Zel'dovich Effect Surveys
• The effect of massive neutrinos on the matter power spectrum
• Galaxy Mergers with Adaptive Mesh Refinement: Star Formation and Hot Gas Outflow
• The Via Lactea INCITE Simulation: Galactic Dark Matter Substructure at High Resolution
• Parallel HOP: A Scalable Halo Finder for Massive Cosmological Data Sets
• Self-Consistent Solution of Cosmological Radiation-Hydrodynamics and Chemical Ionization
• The Santa Fe Light Cone Simulation Project: II. The Prospects for Direct Detection of the WHIM with SZE Surveys
• Gravitational Collapse and Fragmentation in Molecular Clouds with Adaptive Mesh Refinement

Cited by in corpus (919)

• The Astropy Project: Building an inclusive, open-science project and status of the v2.0 core package
• Modules for Experiments in Stellar Astrophysics (MESA): Pulsating Variable Stars, Rotation, Convective Boundaries, and Energy Conservation
• The Circumgalactic Medium
• A model for cosmological simulations of galaxy formation physics
• Enzo: An Adaptive Mesh Refinement Code for Astrophysics
• Modules for Experiments in Stellar Astrophysics (MESA): Time-Dependent Convection, Energy Conservation, Automatic Differentiation, and Infrastructure
• The Baryon Census in a Multiphase Intergalactic Medium: 30% of the Baryons May Still Be Missing
• The Birth of a Galaxy: Primordial Metal Enrichment and Stellar Populations
• Chaotic cold accretion onto black holes
• Momentum Injection by Supernovae in the Interstellar Medium
• The Birth of a Galaxy - III. Propelling reionisation with the faintest galaxies
• The SILCC (SImulating the LifeCycle of molecular Clouds) project: I. Chemical evolution of the supernova-driven ISM
• Grackle: a Chemistry and Cooling Library for Astrophysics
• 3D maps of the local ISM from inversion of individual color excess measurements
• Galaxy Formation with BECDM: I. Turbulence and relaxation of idealised haloes
• Simulations of solitonic core mergers in ultra-light axion dark matter cosmologies
• The growth and entrainment of cold gas in a hot wind
• The AGORA High-Resolution Galaxy Simulations Comparison Project
• Nyx: A Massively Parallel AMR Code for Computational Cosmology
• nbodykit: an open-source, massively parallel toolkit for large-scale structure
• Three-phase Interstellar medium in Galaxies Resolving Evolution with Star formation and Supernova feedback (TIGRESS): Algorithms, Fiducial model, and Convergence
• Figuring Out Gas & Galaxies in Enzo (FOGGIE). I. Resolving Simulated Circumgalactic Absorption at 2 < z < 2.5
• Modeling UV Radiation Feedback from Massive Stars: II. Dispersal of Star-Forming Giant Molecular Clouds by Photoionization and Radiation Pressure
• The SILCC (SImulating the LifeCycle of molecular Clouds) project - II. Dynamical evolution of the supernova-driven ISM and the launching of outflows
• Black hole formation in the early universe
• Exploring Fundamentally Three-dimensional Phenomena in High-fidelity Simulations of Core-collapse Supernovae
• Formation of massive black holes in rapidly growing pre-galactic gas clouds
• The Local Group on FIRE: Dwarf galaxy populations across a suite of hydrodynamic simulations
• Formation and structure of ultralight bosonic dark matter halos
• The Launching of Cold Clouds by Galaxy Outflows I: Hydrodynamic Interactions with Radiative Cooling
• A Global Model For Circumgalactic and Cluster-Core Precipitation
• Cosmic-ray Driven Outflows in Global Galaxy Disk Models
• Simulating the Common Envelope Phase of a Red Giant Using SPH and Uniform Grid Codes
• Galaxy Properties and UV Escape Fractions During Epoch of Reionization: Results from the Renaissance Simulations
• The SILCC project: III. Regulation of star formation and outflows by stellar winds and supernovae
• The Impact of Enhanced Halo Resolution on the Simulated Circumgalactic Medium
• Cooling, AGN Feedback and Star Formation in Simulated Cool-Core Galaxy Clusters
• The Formation of Submillimetre-Bright Galaxies from Gas Infall over a Billion Years
• Enzo+Moray: Radiation Hydrodynamics Adaptive Mesh Refinement Simulations with Adaptive Ray Tracing
• Numerical Simulations of Multiphase Winds and Fountains from Star-Forming Galactic Disks: I. Solar Neighborhood TIGRESS Model
• The Fragmentation of Magnetized, Massive Star-Forming Cores with Radiative Feedback
• The Impact of Star Formation Feedback on the Circumgalactic Medium
• Global simulations of galactic winds including cosmic ray streaming
• The Birth of a Galaxy. II. The Role of Radiation Pressure
• Do cloud-cloud collisions trigger high-mass star formation? I. Small cloud collisions
• Modelling the supernova-driven ISM in different environments
• Sloshing of the Magnetized Cool Gas in the Cores of Galaxy Clusters
• The characteristic black hole mass resulting from direct collapse in the early universe
• Properties of the Circumgalactic Medium in Cosmic Ray-Dominated Galaxy Halos
• Turbulence and Radio Mini-halos in the Sloshing Cores of Galaxy Clusters
• How cold gas continuously entrains mass and momentum from a hot wind
• Cosmic ray feedback in the FIRE simulations: constraining cosmic ray propagation with GeV gamma ray emission
• Modeling AGN Feedback in Cool-Core Clusters: The Formation of Cold Clumps
• Magnetic Fields in Population III Star Formation
• The Tidal Disruption of Giant Stars and Their Contribution to the Flaring Supermassive Black Hole Population
• Cooler and smoother -- the impact of cosmic rays on the phase structure of galactic outflows
• General Relativistic Three-Dimensional Multi-Group Neutrino Radiation-Hydrodynamics Simulations of Core-Collapse Supernovae
• Characterizing mass, momentum, energy and metal outflow rates of multi-phase galactic winds in the FIRE-2 cosmological simulations
• Accretion disc dynamo activity in local simulations spanning weak-to-strong net vertical magnetic flux regimes
• The First Population II Stars Formed in Externally Enriched Mini-halos
• Ram Pressure Stripping of the Large Magellanic Cloud's Disk as a Probe of the Milky Way's Circumgalactic Medium
• Neutrinos And Big Bang Nucleosynthesis
• The Two States of Star Forming Clouds
• The AGORA High-Resolution Galaxy Simulations Comparison Project. II: Isolated Disk Test
• Isolating signatures of major cloud-cloud collisions using position-velocity diagrams
• Radiation-Hydrodynamic Simulations of Massive Star Formation with Protostellar Outflows
• Formation and mass growth of axion stars in axion miniclusters
• Impact of type ia supernova ejecta on binary companions in the single-degenerate scenario
• A Theory for the Excitation of CO in Star Forming Galaxies
• Public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation
• Impact of Cosmic Ray Transport on Galactic Winds
• Constraints on Hydrodynamical Subgrid Models from Quasar Absorption Line Studies of the Simulated Circumgalactic Medium
• Modeling AGN Feedback in Cool-Core Clusters: The Balance between Heating and Cooling
• Star formation histories of dwarf galaxies in the FIRE simulations: dependence on mass and Local Group environment
• An Unstable Truth: How Massive Stars get their Mass
• Chaotic cold accretion on to black holes in rotating atmospheres
• Cosmic rays can drive strong outflows from gas-rich high-redshift disk galaxies
• Cosmological MHD Simulations of Galaxy Cluster Radio Relics: Insights and Warnings for Observations
• A Theory for the Variation of Dust Attenuation Laws in Galaxies
• Star Cluster Formation in Turbulent, Magnetized Dense Clumps with Radiative and Outflow Feedback
• The Nature of the Warm/Hot Intergalactic Medium I. Numerical Methods, Convergence, and OVI Absorption
• Black hole formation from axion stars
• Asymmetric Accretion Flows within a Common Envelope
• The Turbulent Origin of Spin-Orbit Misalignment in Planetary Systems
• Dwarf galaxy formation with H2-regulated star formation
• Simulating an Isolated Dwarf Galaxy with Multi-Channel Feedback and Chemical Yields from Individual Stars
• Star Formation Efficiency and Dispersal of Giant Molecular Clouds with UV Radiation Feedback: Dependence on Gravitational Boundedness and Magnetic Fields
• MPI-AMRVAC 3.0: updates to an open-source simulation framework
• Hydrodynamic Simulations of the Inner Accretion Flow of Sagittarius A* Fueled By Stellar Winds
• Quantifying Supernovae-Driven Multiphase Galactic Outflows
• Common Envelope Wind Tunnel: Coefficients of Drag and Accretion in a Simplified Context for Studying Flows Around Objects Embedded Within Stellar Envelopes
• SILCC VI -- Multi-phase ISM structure, stellar clustering, and outflows with supernovae, stellar winds, ionising radiation and cosmic rays
• The SILCC project --- IV. Impact of dissociating and ionising radiation on the interstellar medium and Halpha emission as a tracer of the star formation rate
• The IRX-Beta Dust Attenuation Relation in Cosmological Galaxy Formation Simulations
• The relative impact of photoionizing radiation and stellar winds on different environments
• Formation of an embryonic supermassive star in the first galaxy
• Super-Eddington Accretion and Feedback from the First Massive Seed Black Holes
• Cosmic ray feedback heating of the intracluster medium
• The Growth of Black Holes from Population III Remnants in the Renaissance Simulations
• Sample variance in the local measurements of the Hubble constant
• The impact of the supersonic baryon-dark matter velocity difference on the z~20 21cm background
• SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
• Episodic accretion: the interplay of infall and disc instabilities
• Cosmological particle-in-cell simulations with ultralight axion dark matter
• Survival and mass growth of cold gas in a turbulent, multiphase medium
• SIGAME simulations of the [CII], [OI] and [OIII] line emission from star forming galaxies at z ~ 6
• How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes
• How galaxies form stars: the connection between local and global star formation in galaxy simulations
• The Properties of Short gamma-ray burst Jets Triggered by neutron star mergers
• When did Population III star formation end?
• Role of Cosmic Rays in the Circumgalactic Medium
• Turbulent Cold Flows Gave Birth to the First Quasars
• The Obelisk simulation: galaxies contribute more than AGN to HI reionization of protoclusters
• Trident: a universal tool for generating synthetic absorption spectra from astrophysical simulations
• Giant Impact: An Efficient Mechanism for the Devolatilization of Super-Earths
• Simulating the Formation of Massive Protostars: I. Radiative Feedback and Accretion Disks
• The Impact of Cosmic Rays on Thermal Instability in the Circumgalactic Medium
• Impact of Protostellar Outflows on Turbulence and Star Formation Efficiency in Magnetized Dense Cores
• Feedback Effects on Low-Mass Star Formation
• Cradles of the first stars: self-shielding, halo masses, and multiplicity
• On the Three-Dimensional Structure of Local Molecular Clouds
• Gravitational contraction versus Supernova driving and the origin of the velocity dispersion-size relation in molecular clouds
• Investigations of Protostellar Outflow Launching and Gas Entrainment: Hydrodynamic Simulations and Molecular Emission
• Chaos and Variance in Galaxy Formation
• Supermassive Black Hole Formation at High Redshifts via Direct Collapse: Physical Processes in the Early Stage
• Radiative Mixing Layers: Insights from Turbulent Combustion
• The formation of the first cosmic structures and the physics of the z~20 Universe
• Late Pop III Star Formation During the Epoch of Reionization: Results from the Renaissance Simulations
• Formation of Globular Cluster Candidates in Merging Proto-galaxies at High Redshift: A View from the FIRE Cosmological Simulations
• High Angular Momentum Halo Gas: a Feedback and Code-Independent Prediction of LCDM
• Population III Stars and Remnants in High Redshift Galaxies
• AxioNyx: Simulating Mixed Fuzzy and Cold Dark Matter
• Fast galaxy bars continue to challenge standard cosmology
• GAMER-2: a GPU-accelerated adaptive mesh refinement code -- accuracy, performance, and scalability
• The Post-Merger Magnetized Evolution of White Dwarf Binaries: The Double-Degenerate Channel of Sub-Chandrasekhar Type Ia Supernovae and the Formation of Magnetized White Dwarfs
• A UV flux constraint on the formation of direct collapse black holes
• The effect of feedback and reionization on star formation in low-mass dwarf galaxy haloes
• Legacy of star formation in the pre-reionization universe
• Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes. I: Feedback-regulated Star Formation and Black Hole Growth
• The Direct Collapse of a Massive Black Hole Seed Under the Influence of an Anisotropic Lyman-Werner Source
• The environmental dependence of the X_CO conversion factor
• Turbulence production and turbulent pressure support in the intergalactic medium
• Equation of State Dependent Dynamics and Multimessenger Signals from Stellar-mass Black Hole Formation
• Baseline Metal Enrichment from Population III Star Formation in Cosmological Volume Simulations
• The small scale dynamo and the amplification of magnetic fields in massive primordial haloes
• The importance of magnetic fields for the initial mass function of the first stars
• The Neutrino Fast Flavor Instability in Three Dimensions
• Spoon-Feeding Giant Stars to Supermassive Black Holes: Episodic Mass Transfer from Evolving Stars and Their Contribution to the Quiescent Activity of Galactic Nuclei
• Project AMIGA: The Circumgalactic Medium of Andromeda
• Cold Fronts and Gas Sloshing in Galaxy Clusters with Anisotropic Thermal Conduction
• Companion-launched jets and their effect on the dynamics of common envelope interaction simulations
• The Metagalactic Ionizing Background: A Crisis in UV Photon Production or Incorrect Galaxy Escape Fractions?
• AGN Heating in Simulated Cool-Core Clusters
• Numerical resolution effects on simulations of massive black hole seeds
• Morphology of Hydrodynamic Winds: A Study of Planetary Winds in Stellar Environments
• A Common Origin for Globular Clusters and Ultra-faint Dwarfs in Simulations of the First Galaxies
• Galaxy Cluster Radio Relics in Adaptive Mesh Refinement Cosmological Simulations: Relic Properties and Scaling Relationships
• Particle-in-cell Simulation of the Neutrino Fast Flavor Instability
• Stellar Tidal Disruption Events with Abundances and Realistic Structures (STARS): Library of Fallback Rates
• Numerical and Perturbative Computations of the Fuzzy Dark Matter Model
• The critical dark matter halo mass for Population III star formation: dependence on Lyman-Werner radiation, baryon-dark matter streaming velocity, and redshift
• Diverse Structural Evolution at z > 1 in Cosmologically Simulated Galaxies
• Is Multiphase Gas Cloudy or Misty?
• Metal Transport and Chemical Heterogeneity in Early Star Forming Systems
• Gravitational Wave Emission from Collisions of Compact Scalar Solitons
• The Formation and Evolution of Wide-Orbit Stellar Multiples In Magnetized Clouds
• Formation of the first stars and black holes
• Do Giant Molecular Clouds Care About the Galactic Structure?
• Stellar Radiation is Critical for Regulating Star Formation and Driving Outflows in Low Mass Dwarf Galaxies
• GMC Collisions as Triggers of Star Formation. III. Density and Magnetically Regulated Star Formation
• Reproducing sub-millimetre galaxy number counts with cosmological hydrodynamic simulations
• H_2 Suppression with Shocking Inflows: Testing a Pathway for Supermassive Black Hole Formation
• The Keck Baryonic Structure Survey: Using foreground/background galaxy pairs to trace the structure and kinematics of circumgalactic neutral hydrogen at $z\sim 2$
• High resolution studies of massive primordial haloes
• The Bridge: a transient phenomenon of forming stellar multiples
• Gas Loss by Ram Pressure Stripping and Internal Feedback From Low Mass Milky Way Satellites
• Distinguishing Mergers and Disks in High Redshift Observations of Galaxy Kinematics
• Gravitational waves from Population III binary black holes formed by dynamical capture
• Tangos: the agile numerical galaxy organization system
• Mass Transport and Turbulence in Gravitationally Unstable Disk Galaxies. I: The Case of Pure Self-Gravity
• Formation of Massive, Dense Cores by Cloud-Cloud Collisions
• Galaxies lacking dark matter produced by close encounters in a cosmological simulation
• Fermi and eRosita bubbles as relics of the past activity of the Galactic black hole
• The SILCC project - V. The impact of magnetic fields on the chemistry and the formation of molecular clouds
• Low-mass galaxy assembly in simulations: regulation of early star formation by radiation from massive stars
• Supplement: Going the Distance: Mapping Host Galaxies of LIGO and Virgo Sources in Three Dimensions Using Local Cosmography and Targeted Follow-up
• Baryon-driven growth of solitonic cores in fuzzy dark matter halos
• The Dynamics, Destruction, and Survival of Supernova-Formed Dust Grains
• Equation of State Dependence of Gravitational Waves in Core-Collapse Supernovae
• Evolution Of Post-Impact Remnant Helium Stars In Type Ia Supernova Remnants Within The Single-Degenerate Scenario
• Physical Origins of Gas Motions in Galaxy Cluster Cores: Interpreting Hitomi Observations of the Perseus Cluster
• The Effect of Anisotropic Viscosity on Cold Fronts in Galaxy Clusters
• Powderday: Dust Radiative Transfer for Galaxy Simulations
• Suppression of star formation in dwarf galaxies by grain photoelectric feedback
• On the Origin of the Hubble Sequence: I. Insights on Galaxy Color Migration from Cosmological Simulations
• Numerical Simulations of Supernova Dust Destruction. II. Metal-Enriched Ejecta Knots
• Two-Dimensional Core-Collapse Supernova Simulations with the Isotropic Diffusion Source Approximation for Neutrino Transport
• The Impact of Radio AGN Bubble Composition on the Dynamics and Thermal Balance of the Intracluster Medium
• GMC Collisions as Triggers of Star Formation. II. 3D Turbulent, Magnetized Simulations
• Short-lived radioisotopes in meteorites from Galactic-scale correlated star formation
• Accretion Disk Assembly During Common Envelope Evolution: Implications for Feedback and LIGO Binary Black Hole Formation
• Seeding the Second Star: enrichment from population III, dust evolution, and cloud collapse
• Galaxy mergers moulding the circum-galactic medium - I. The impact of a major merger
• Scaling relations of Fuzzy Dark Matter haloes I: individual systems in their cosmological environment
• How the super-Eddington regime regulates black hole growth in high-redshift galaxies
• A universal route for the formation of massive star clusters in giant molecular clouds
• Direct Numerical Simulation of Reionization II: Recombinations, Clumping Factors, and the Photon Budget for Reionization
• Triggering and Delivery Algorithms for AGN Feedback
• The Fate of the Merger Remnant in GW170817 and its Imprint on the Jet Structure
• Cosmic Ray Transport, Energy Loss, and Influence in the Multiphase Interstellar Medium
• On the coexistence of the streaming instability and the vertical shear instability in protoplanetary disks
• A No-Go Theorem for Direct Collapse Black Holes Without a Strong Ultraviolet Background
• It's Cloud's Illusions I Recall: Mixing Drives the Acceleration of Clouds from Ram Pressure Stripped Galaxies
• Star Formation and Clumps in Cosmological Galaxy Simulations with Radiation Pressure Feedback
• Dense gas formation and destruction in a simulated Perseus-like galaxy cluster with spin-driven black hole feedback
• The Role of Outflows, Radiation Pressure, and Magnetic Fields in Massive Star Formation
• Observing Simulated Protostars with Outflows: How Accurate are Protostellar Properties Inferred from SEDs?
• Time Varying Dynamical Star Formation Rate
• The Evolution of Binaries in a Gaseous Medium: Three-Dimensional Simulations of Binary Bondi-Hoyle-Lyttleton Accretion
• Mixing and transport of metals by gravitational instability-driven turbulence in galactic discs
• Heating the IGM by X-rays from Population III Binaries in High Redshift Galaxies
• Magnetic fields during the formation of supermassive black holes
• Stellar Mass Black Hole Formation and Multi-messenger Signals from Three Dimensional Rotating Core-Collapse Supernova Simulations
• Modeling UV Radiation Feedback from Massive Stars: I. Implementation of Adaptive Ray Tracing Method and Tests
• Self-generated turbulence in magnetic reconnection
• The Ties that Bind? Galactic Magnetic Fields and Ram Pressure Stripping
• Double-Degenerate Carbon-Oxygen and Oxygen-Neon White Dwarf Mergers: A New Mechanism for Faint and Rapid Type Ia Supernovae
• Mass and Magnetic distributions in Self Gravitating Super Alfvenic Turbulence with AMR
• Gas and stellar spiral structures in tidally perturbed disc galaxies
• Simulating Neutron Star Mergers as r-process Sources in Ultra Faint Dwarf Galaxies
• The formation of massive Pop III stars in the presence of turbulence
• Construction of Wave Dark Matter Halos: Numerical Algorithm and Analytical Constraints
• SILCC-ZOOM: The early impact of ionizing radiation on forming molecular clouds
• The Survival of Multiphase Dusty Clouds in Hot Winds
• The Journey Counts: The Importance of Including Orbits when Simulating Ram Pressure Stripping
• SILCC VII -- Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
• How Does the Surface Density and Size of Disk Galaxies Measured in Hydrodynamic Simulations Correlate with the Halo Spin Parameter?
• Robustness of Inflation to Large Tensor Perturbations
• Witnessing the birth of a supermassive protostar
• A simple model for mixing and cooling in cloud-wind interactions
• Evolution of Post-Impact Companion Stars in SN Ia Remnants within the Single-Degenerate Scenario
• Kinetic energy from supernova feedback in high-resolution galaxy simulations
• Modelling of the Effects of Stellar Feedback during Star Cluster Formation Using a Hybrid Gas and N-Body Method
• How Gas Accretion Feeds Galactic Disks
• Cosmic-Ray Diffusion Suppression in Star-forming Regions Inhibits Clump Formation in Gas-rich Galaxies
• Effect of Angular Momentum Alignment and Strong Magnetic Fields on the Formation of Protostellar Disks
• A fundamental test for stellar feedback recipes in galaxy simulations
• Following the Cosmic Evolution of Pristine Gas II: The search for Pop III-Bright Galaxies
• Modeling UV Radiation Feedback from Massive Stars: III. Escape of Radiation from Star-forming Giant Molecular Clouds
• Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
• Magnetic field amplification in accretion discs around the first stars: implications for the primordial IMF
• Impact of dust cooling on direct collapse black hole formation
• Outflows Driven by Direct and Reprocessed Radiation Pressure in Massive Star Clusters
• 2HOT: An Improved Parallel Hashed Oct-Tree N-Body Algorithm for Cosmological Simulation
• What Physics Determines the Peak of the IMF? Insights from the Structure of Cores in Radiation-Magnetohydrodynamic Simulations
• Pebble dynamics and accretion onto rocky planets. I. Adiabatic and convective models
• Tracing Molecular Gas in z $\simeq$ 6 Galaxies with [C$\mathrm{II}$]
• Collisional N-Body Dynamics Coupled to Self-Gravitating Magnetohydrodynamics Reveals Dynamical Binary Formation
• Common Envelope Evolution on a Moving Mesh
• Constrained Simulation of the Bullet Cluster
• Assessing inflow rates in atomic cooling halos: implications for direct collapse black holes
• The Low Redshift Circumgalactic Medium in Simba
• Simulating a binary system that experiences the grazing envelope evolution
• Environmental dependence of star formation induced by cloud collisions in a barred galaxy
• The anatomy of a star-forming galaxy: Pressure-driven regulation of star formation in simulated galaxies
• How Do Supernovae Impact the Circumgalactic Medium? I. Large-Scale Fountains Around a Milky Way-Like Galaxy
• The formation of massive primordial stars in the presence of moderate UV backgrounds
• Deep Chandra observation and numerical studies of the nearest cluster cold front in the sky
• The Orion Fingers: Near-IR Adaptive Optics Imaging of an Explosive Protostellar Outflow
• Evolution and Distribution of Magnetic Fields from AGNs in Galaxy Clusters II. The Effects of Cluster Size and Dynamical State
• Metallicity and the Universality of the IMF
• Are fibres in molecular cloud filaments real objects?
• The Galactic Dust-Up: Modeling Dust Evolution in FIRE
• Impact of Winds from Intermediate-Mass Stars on Molecular Cloud Structure and Turbulence
• Formation of Relativistic Axion Stars
• Figuring Out Gas & Galaxies in Enzo (FOGGIE). II. Emission from the z=3 Circumgalactic Medium
• Cosmological Fluid Mechanics with Adaptively Refined Large Eddy Simulations
• The Circumgalactic Medium of the Milky Way is Half Hidden
• Cosmological baryon transfer in the SIMBA simulations
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• Solitons in the dark: non-linear structure formation with fuzzy dark matter
• Tracking the distribution of ${}^{26}$Al and ${}^{60}$Fe during the early phases of star and disk evolution
• Ultra Long Gamma-Ray Bursts from the collapse of Blue Super Giant stars: an end-to-end simulation
• Black hole obscuration and duty cycles mediated by AGN feedback in high redshift galaxies
• Soliton Oscillations and Revised Constraints from Eridanus II of Fuzzy Dark Matter
• The halo mass function and filaments in full cosmological simulations with fuzzy dark matter
• Numerical Calibration of the HCN$-$Star Formation Correlation
• Large scale simulations of H and He reionization and heating driven by stars and more energetic sources
• The Spatially Uniform Spectrum of the Fermi Bubbles: the Leptonic AGN Jet Scenario
• How runaway stars boost galactic outflows
• Spiral Disk Instability Can Drive Thermonuclear Explosions in Binary White Dwarf Mergers
• Star formation and ISM morphology in tidally induced spiral structures
• Prominence formation by levitation-condensation at extreme resolutions
• Possible Origin of the G2 Cloud from the Tidal Disruption of a Known Giant Star by Sgr A*
• Stellar winds pump the heart of the Milky Way
• Properties of the Simulated Circumgalactic Medium
• Massive Star Formation via the Collapse of Subvirial and Virialized Turbulent Massive Cores
• A Novel High-Order, Entropy Stable, 3D AMR MHD Solver with Guaranteed Positive Pressure
• Feeding vs. Falling: The growth and collapse of molecular clouds in a turbulent interstellar medium
• Impact of baryonic streaming velocities on the formation of supermassive black holes via direct collapse
• Common Envelope Wind Tunnel: The Effects of Binary Mass Ratio and Implications for the Accretion-Driven Growth of LIGO Binary Black Holes
• Growth and Evolution of Thermal Instabilities in Idealized Galaxy-Cluster Cores
• First Light: exploring the Spectra of High-Redshift Galaxies in the Renaissance Simulations
• Core-collapse supernovae in the hall of mirrors. A three-dimensional code-comparison project
• Early growth of typical high redshift black holes seeded by direct collapse
• Dwarf Galaxies with Ionizing Radiation Feedback. I: Escape of Ionizing Photons
• Thermal instabilities: Fragmentation and field misalignment of filament fine structure
• Visualizing Astronomical Data with Blender
• Classification of Magnetohydrodynamic Simulations using Wavelet Scattering Transforms
• Dark Matter Deficient Galaxies And Their Member Star Clusters Form Simultaneously During High-velocity Galaxy Collisions In 1.25 pc Resolution Simulations
• Magnetic Seismology of Interstellar Gas Clouds: Unveiling a Hidden Dimension
• What Do the Hitomi Observations Tell Us About the Turbulent Velocities in the Perseus Cluster? Probing the Velocity Field with Mock Observations
• Deep zoom-in simulation of a fuzzy dark matter galactic halo
• Three-Dimensional Hydrodynamic Simulations of Convective Nuclear Burning In Massive Stars Near Iron Core Collapse
• The fate of the gaseous disks of galaxies that fall into clusters
• Bondi or not Bondi: the impact of resolution on accretion and drag force modelling for Supermassive Black Holes
• Filamentary flow and magnetic geometry in evolving cluster-forming molecular cloud clumps
• Dust Polarization Maps from TIGRESS: E/B power asymmetry and TE correlation
• Adaptive Mesh Refinement Simulations of Galaxy Formation: Exploring Numerical and Physical Parameters
• Streaming instability in the quasi-global protoplanetary discs
• How merger-driven gas motions in galaxy clusters can turn AGN bubbles into radio relics
• Synthetic Observations of Magnetic Fields in Protostellar Cores
• Figuring Out Gas & Galaxies In Enzo (FOGGIE). IV. The Stochasticity of Ram Pressure Stripping in Galactic Halos
• The AGORA High-resolution Galaxy Simulations Comparison Project. III: Cosmological zoom-in simulation of a Milky Way-mass halo
• Ram Pressure Stripping of Hot Coronal Gas from Group and Cluster Galaxies and the Detectability of Surviving X-ray Coronae
• On the effective turbulence driving mode of molecular clouds formed in disc galaxies
• Direct Collapse to Supermassive Black Hole Seeds with Radiative Transfer: Isolated Halos
• Striations in molecular clouds: Streamers or MHD waves?
• Supermassive Black Hole Seed Formation at High Redshifts: Long-Term Evolution of the Direct Collapse
• Optimized Multi-Frequency Spectra for Applications in Radiative Feedback and Cosmological Reionization
• PHANGS-JWST First Results: Rapid Evolution of Star Formation in the Central Molecular Gas Ring of NGC1365
• Gravitational Collapse in the Post-Inflationary Universe
• A detailed framework to incorporate dust in hydrodynamical simulations
• Three-dimensional hydrodynamical models of wind and outburst-related accretion in symbiotic systems
• ALMA observations of Lyman-alpha Blob 1: halo sub-structure illuminated from within
• The Decoupling of Binaries from Their Circumbinary Disks
• Catastrophic Cooling in Superwinds: Line Emission and Non-equilibrium Ionization
• Stellar splashback: the edge of the intracluster light
• Modeling Dust Polarization Observations of Molecular Clouds through MHD Simulations
• White Dwarf Mergers on Adaptive Meshes I. Methodology and Code Verification
• Empirically Constrained Predictions for Metal-Line Emission from the Circumgalactic Medium
• Black hole growth and AGN feedback under clumpy accretion
• Songlines from Direct Collapse Seed Black Holes: Effects of X-rays on Black Hole Growth and Stellar Populations
• Scaling Relations for Galaxies Prior to Reionization
• AGN Feedback and Multi-phase Gas in Giant Elliptical Galaxies
• Structure and Expansion Law of HII Regions in structured Molecular Clouds
• Cloudy with A Chance of Rain: Accretion Braking of Cold Clouds
• Synthetic [CII] emission maps of a simulated molecular cloud in formation
• Hydrodynamic Effects in the Symmetron and $f(R)$-gravity Models
• Simulation of a Compact Object with Outflows Moving Through a Gaseous Background
• Population III Star Formation In Large Cosmological Simulations I. Halo Temporal and Physical Environment
• Testing Secondary Models for the Origin of Radio Mini-Halos in Galaxy Clusters
• Rise of the First Super-Massive Stars
• Understanding `galaxy groups' as a unique structure in the universe
• The Emergence of the First Star-free Atomic Cooling Haloes in the Universe
• Forming Super-Massive Black Hole Seeds under the Influence of a Nearby Anisotropic Multi-Frequency Source
• The Impact of Different Neutrino Transport Methods on Multidimensional Core-collapse Supernova Simulations
• Magnetic fields in the formation of the first stars.--II Results
• Non-equilibrium ionization in mixed-morphology supernova remnants
• Quenching and the UVJ diagram in the SIMBA cosmological simulation
• Spatial Decorrelation of Young Stars and Dense Gas as a Probe of the Star Formation-Feedback Cycle in Galaxies
• IDEFIX: a versatile performance-portable Godunov code for astrophysical flows
• Cosmic Ray Driven Outflows from the Large Magellanic Cloud: Contributions to the LMC Filament
• Radiation pressure in super star cluster formation
• Shock and Splash: Gas and Dark Matter Halo Boundaries around LambdaCDM Galaxy Clusters
• From giant clumps to clouds -- III. The connection between star formation and turbulence in the ISM
• Numerical simulations of the random angular momentum in convection II: delayed explosions of red supergiants following "failed'' supernovae
• Simulating intergalactic gas for DESI-like small scale Lymanα forest observations
• On The Development of Multidimensional Progenitor Models For Core-collapse Supernovae
• Cosmic Reionization On Computers III. The Clumping Factor
• Effect of the heating rate on the stability of the three-phase interstellar medium
• Evolution of primordial magnetic fields during large-scale structure formation
• How Unusual is the Milky Way's Assembly History?
• Lyman-alpha transmission properties of the intergalactic medium in the CoDaII simulation
• Direct collapse to supermassive black hole seeds: the critical conditions for suppression of ${\mathrm{H}}_2$ cooling
• The origins of Calcium-rich supernovae from disruptions of CO white-dwarfs by hybrid He-CO white-dwarfs
• Direct Collapse to Supermassive Black Hole Seeds with Radiation Transfer: Cosmological Halos
• The Role of the Parker Instability in Structuring the Interstellar Medium
• Implementation of CR Energy SPectrum (CRESP) algorithm in PIERNIK MHD code. I. Spectrally resolved propagation of CR electrons on Eulerian grids
• Calibrating Core Overshooting Parameters With Two-dimensional Hydrodynamical Simulations
• The impact of cosmic rays on dynamical balance and disk-halo interaction in Lstar disk galaxies
• A Comparison of Circumgalactic MgII Absorption between the TNG50 Simulation and the MEGAFLOW Survey
• Kiloparsec-Scale Simulations of Star Formation in Disk Galaxies. I. The unmagnetized and zero-feedback limit
• Giant Molecular Cloud Formation in Disk Galaxies: Characterizing Simulated versus Observed Cloud Catalogues
• unyt: Handle, manipulate, and convert data with units in Python
• Dwarf Galaxies with Ionizing Radiation Feedback. II: Spatially-resolved Star Formation Relation
• Abundance anomalies in metal-poor stars from Population III supernova ejecta hydrodynamics
• Low-metallicity star formation: Relative impact of metals and magnetic fields
• Revealing the physical properties of gas accreting to haloes in the EAGLE simulations
• Figuring Out Gas & Galaxies in Enzo (FOGGIE). III. The Mocky Way: Investigating Biases in Observing the Milky Way's Circumgalactic Medium
• Axion minivoids and implications for direct detection
• Formation of inflaton halos after inflation
• Comparisons of Cosmological MHD Galaxy Cluster Simulations to Radio Observations
• Radiation shielding of protoplanetary discs in young star-forming regions
• Adaptive mesh refinement simulations of a galaxy cluster merger - I. Resolving and modelling the turbulent flow in the cluster outskirts
• A general hybrid radiation transport scheme for star formation simulations on an adaptive grid
• Galaxy cluster mergers as triggers for the formation of jellyfish galaxies: case study of the A901/2 system
• Inhomogeneous initial conditions for inflation: A wibbly-wobbly timey-wimey path to salvation
• The density structure of supersonic self-gravitating turbulence
• Formation of globular clusters in dwarf galaxies of the Local Group
• The Formation of Compact Elliptical Galaxies in The Vicinity of A Massive Galaxy: The Role of Ram-pressure Confinement
• The Impact of Type Ia Supernovae in Quiescent Galaxies: II. Energetics and Turbulence
• Simulating the UV Escape Fractions from Molecular Cloud Populations in Star-forming Dwarf and Spiral Galaxies
• Simulating Astro-H Observations of Sloshing Gas Motions in the Cores of Galaxy Clusters
• Fragmentation inside atomic cooling haloes exposed to Lyman-Werner radiation
• Barred spiral galaxies in modified gravity theories
• Magneto-Hydrodynamical Effects on Nuclear Deflagration Fronts in Type Ia Supernovae
• Figuring Out Gas & Galaxies In Enzo (FOGGIE) VI: The Circumgalactic Medium of $L^{\ast }$ Galaxies is Supported in an Emergent, Non-Hydrostatic Equilibrium
• Mixing matters
• The effect of photoionising feedback on star formation in isolated and colliding clouds
• Light Curves and Spectra from a Thermonuclear Explosion of a White Dwarf Merger
• 3D simulations of clump formation in stellar wind collisions
• KODIAQ-Z: Metals and Baryons in the Cool Intergalactic and Circumgalactic Gas at 2.2<z<3.6
• A Massive Star is Born: How Feedback from Stellar Winds, Radiation Pressure, and Collimated Outflows Limits Accretion onto Massive Stars
• The contribution of binary star formation via core-fragmentation on protostellar multiplicity
• Flipping-up the field: gravitational feedback as a mechanism for young clusters dispersal
• Embryo impacts and gas giant mergers II: Diversity of Hot Jupiters' internal structure
• Quantifying the effects of spatial resolution and noise on galaxy metallicity gradients
• Hybrid Cosmological Simulations with Stream Velocities
• Probing the Circum-Galactic Medium with Fast Radio Bursts: Insights from the CAMELS Simulations
• How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-Dust Geometry Model in SED Fitting
• Observability of Low-Luminosity AGN in the Early Universe with JWST
• X-ray Background at High Redshifts from Pop III Remnants: Results from Pop III star formation rates in the Renaissance Simulations
• Report on the Third Workshop on Sustainable Software for Science: Practice and Experiences (WSSSPE3)
• Virial shocks are suppressed in cosmic ray-dominated galaxy halos
• Radiative turbulent mixing layers at high Mach numbers
• Violent starbursts and quiescence induced by FUV radiation feedback in metal-poor galaxies at high-redshift
• Composition of Low Redshift Halo Gas
• Tidal disruption events from eccentric orbits and lessons learned from the noteworthy ASASSN-14ko
• Infrared Radiation Feedback Does Not Regulate Star Cluster Formation
• Atomic Chemistry In Turbulent Astrophysical Media I: Effect of Atomic Cooling
• Quokka: A code for two-moment AMR radiation hydrodynamics on GPUs
• A Model for Line Absorption and Emission from Turbulent Mixing Layers
• A Dynamical Model for Clustered Star Formation in the Galactic Disk
• The coexistence of the streaming instability and the vertical shear instability in protoplanetary disks: Planetesimal formation thresholds explored in two-dimensional global models
• The Goldilocks problem of the quasar contribution to reionization
• Thermal History Of Cbb Chondrules And Cooling Rate Distributions Of Ejecta Plumes
• Constraining The Single-Degenerate Channel of Type Ia Supernovae With Stable Iron-Group Elements in SNR 3C 397
• Massive core/star formation triggered by cloud-cloud collision: Effect of magnetic field
• Gravity Versus Magnetic Fields in Forming Molecular Clouds
• What Sets the Slope of the Molecular Kennicutt-Schmidt Relation?
• Asymmetric core collapse of rapidly rotating massive star
• Primordial star formation: relative impact of H2 three-body rates and initial conditions
• Understanding Heating in Active Region Cores through Machine Learning I. Numerical Modeling and Predicted Observables
• Heavy dust obscuration of z=7 galaxies in a cosmological hydrodynamic simulation
• Modelling a bright z = 6 galaxy at the faint end of the AGN luminosity function
• Viscosity, pressure, and support of the gas in simulations of merging cool-core clusters
• The Effects of Magnetic Fields and Outflow Feedback on the Shape and Evolution of the Density PDF in Turbulent Star-Forming Clouds
• Heliospheric Compression due to Recent Nearby Supernova Explosions
• Cosmological Simulations of Dwarf Galaxies with Cosmic Ray Feedback
• Simulating highly-eccentric common envelope jets supernova (CEJSN) impostors
• Probing the Curious Case of a Galaxy Cluster Merger in Abell 115 with High Fidelity Chandra X-ray Temperature and Radio Maps
• The Interplay of Kinetic and Radiative Feedback in Galaxy Clusters
• Formation of carbon-enhanced metal-poor stars in the presence of far ultraviolet radiation
• The role of initial magnetic field structure in the launching of protostellar jets
• Turbulence driven by structure formation in the circum-galactic medium
• The CH+ Abundance in Turbulent, Diffuse Molecular Clouds
• Simulating Metal Mixing of Both Common and Rare Enrichment Sources in a Low Mass Dwarf Galaxy
• Entropy Driven Winds: Outflows and Fountains Lifted Gently by Buoyancy
• The Gravitational Afterglow of Boson Stars
• Advanced Data Visualization in Astrophysics: the X3D Pathway
• Halo Abundance and Assembly History with Extreme-Axion Wave Dark Matter at $z\ge 4$
• On the Interpretation of Far-infrared Spectral Energy Distributions. I: The 850 $\mu$m Molecular Mass Estimator
• How long do high-redshift massive black hole seeds remain outliers in black hole vs. host galaxy relations?
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• The Distribution and Evolution of Quasar Proximity Zone Sizes
• A Framework for Modeling Polycyclic Aromatic Hydrocarbon Emission in Galaxy Evolution Simulations
• The interaction of Type Iax supernova ejecta with a helium companion star
• A Dusty Locale: Evolution of Galactic Dust Populations from Milky Way to Dwarf-Mass Galaxies
• The Impact of Cosmic Rays on the Kinematics of the Circumgalactic Medium
• Dust charge distribution in the interstellar medium
• Numerical studies on the link between radioisotopic signatures on Earth and the formation of the Local Bubble. II. Advanced modeling of interstellar 26Al, 53Mn, 60Fe, and 244Pu influxes as traces of past supernovae in the solar neighborhood
• The Effect of Turbulence on Nebular Emission Line Ratios
• Comparing Simulations of AGN Feedback
• OVI Traces Photoionized Streams With Collisionally Ionized Boundaries in Cosmological Simulations of $z\sim 1$ Massive Galaxies
• Zooming in on supermassive black holes: how resolving their gas cloud host renders their accretion episodic
• Better Together: The Complex Interplay Between Radiative Cooling and Magnetic Draping
• TAPAS IV. TYC 3667-1280-1 b - the most massive red giant star hosting a warm Jupiter
• Early-Forming Massive Stars Suppress Star Formation and Hierarchical Cluster Assembly
• Common envelope light-curves - I. grid-code module calibration
• Impact of supernova and cosmic-ray driving on the surface brightness of the galactic halo in soft X-rays
• Troubled cosmic flows: turbulence, enstrophy and helicity from the assembly history of the intracluster medium
• Hot and Turbulent Gas in Clusters
• The implications of dust for high-redshift protogalaxies and the formation of binary disks
• VETTAM: A scheme for radiation hydrodynamics with adaptive mesh refinement using the variable Eddington tensor method
• Amplification of turbulence in contracting prestellar cores in primordial minihalos
• Cooling driven coagulation
• Toward $abinitio$ extremely metal poor stars
• Photospheric Logarithmic Velocity Spirals as MHD Wave Generation Mechanisms
• The role of the H${}_2$ adiabatic index in the formation of the first stars
• Near-Chandrasekhar-Mass Type Ia Supernovae from the Double-Degenerate Channel
• Seeding the second star -- II. CEMP star formation enriched from faint supernovae
• Alignment of the magnetic field in star forming regions and why it might be difficult to observe
• Impact of an accurate modeling of primordial chemistry in high resolution studies
• Improved Coupling of Hydrodynamics and Nuclear Reactions via Spectral Deferred Corrections
• The Interstellar Medium and Star Formation of Galactic Disks. I. ISM and GMC properties with Diffuse FUV and Cosmic Ray Backgrounds
• Primordial Obliquities of Brown Dwarfs and Super-Jupiters from Fragmenting Gravito-Turbulent Discs
• The imprint of cosmic ray driven outflow on Lyman-alpha spectra
• Clumpiness of Observed and Simulated Cold Circumgalactic Gas
• Figuring Out Gas & Galaxies In Enzo (FOGGIE) V: The Virial Temperature Does Not Describe Gas in a Virialized Galaxy Halo
• The highly variable time evolution of star-forming cores identified with dendrograms
• The Strength of the Sheared Magnetic Field in the Galactic's Circum-Nuclear Disk
• Efficiency of Thermal Conduction in a Magnetised Circumgalactic Medium
• Turnaround radius of galaxy clusters in N-body simulations
• Thermal Instability and Multiphase Gas in the Simulated Interstellar Medium with Conduction, Viscosity and Magnetic Fields
• General-relativistic radiation transport scheme in $\text{Gmunu}$ I: Implementation of two-moment based multi-frequency radiative transfer and code tests
• Collapse and Fragmentation of Magnetic Molecular Cloud Cores with the Enzo AMR MHD Code. I. Uniform Density Sphere
• Early Evolution and 3D Structure of Embedded Star Clusters
• Large-eddy simulations of isolated disc galaxies with thermal and turbulent feedback
• Fragmentation in Dusty Low-Metallicity Star Forming Halos
• 3D adaptive mesh refinement simulations of the gas cloud G2 born within the disks of young stars in the Galactic Center
• Dust in the first galaxies
• Evolution of Cold Streams and Emergence of the Hubble Sequence
• Cosmic rays and thermal instability in self-regulating cooling flows of massive galaxy clusters
• Local support against gravity in magneto-turbulent fluids
• Cosmological Simulations of Two-Component Wave Dark Matter
• An Operator-Based Local Discontinuous Galerkin Method Compatible With the BSSN Formulation of the Einstein Equations
• The Fate of Supernova-Heated Gas in Star-Forming Regions of the LMC: Lessons for Galaxy Formation?
• Ab Initio Cosmological Simulations of CR7 as an Active Black Hole
• Dark-matter halo mergers as a fertile environment for low-mass Population III star formation
• X-ray Spectra of Circumgalactic Medium Around Star-Forming Galaxies: Connecting Simulations to Observations
• Gamma-ray bursts and kilonovae from the accretion-induced collapse of white dwarfs
• Tracking Advanced Planetary Systems (TAPAS) with HARPS-N. VI. HD 238914 and TYC 3318-01333-1 - two more Li-rich giants with planets
• A black box for dark sector physics: Predicting dark matter annihilation feedback with conditional GANs
• Low Mach Number Modeling of Convection in Helium Shells on Sub-Chandrasekhar White Dwarfs II: Bulk Properties of Simple Models
• A GPU accelerated Barnes-Hut Tree Code for FLASH4
• The Location and Environments of Neutron Star Mergers in an Evolving Universe
• Effects of turbulence and rotation on protostar formation as a precursor to seed black holes
• Warm Gas in and Around Simulated Galaxy Clusters as Probed by Absorption Lines
• High-redshift Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes: Stellar Feedback and Quasar Growth
• Atomic Chemistry in Turbulent Astrophysical Media II: Effect of the Redshift Zero Metagalactic Background
• GMC Collisions as Triggers of Star Formation. VII. The Effect of Magnetic Field Strength on Star Formation
• The Launching of Cold Clouds by Galaxy Outflows V: The Role of Anisotropic Thermal Conduction
• The Impact of Type Ia Supernovae in Quiescent Galaxies: I. Formation of the Multiphase Interstellar medium
• GMC Collisions as Triggers of Star Formation. VI. Collision-Induced Turbulence
• Ultraviolet Signatures of the Multiphase Intracluster and Circumgalactic Media in the RomulusC Simulation
• A Parameter Space Exploration of Galaxy Cluster Mergers II: Effects of Magnetic Fields
• 3D Hydrodynamics of Pre-supernova Outbursts in Convective Red Supergiant Envelopes
• Multiple Beads-on-a-string: Dark Matter-Deficient Galaxy Formation in a Mini-bullet Satellite-satellite Galaxy Collision
• Structure and Turbulence in Simulated Galaxy Clusters and the Implications for the Formation of Radio Halos
• AGN jets do not prevent the suppression of conduction by the heat buoyancy instability in simulated galaxy clusters
• 3D Hydrodynamical Simulations of Helium-Ignited Double-degenerate White Dwarf Mergers
• The Fate of AGB Wind in Massive Galaxies and the ICM
• No double detonations but core carbon ignitions in high-resolution, grid-based simulations of binary white dwarf mergers
• The Connection between Mergers and AGN Activity in Simulated and Observed Massive Galaxies
• The AGORA High-resolution Galaxy Simulations Comparison Project. VI. Similarities and Differences in the Circumgalactic Medium
• Synthetic Large-Scale Galactic Filaments -- on their Formation, Physical Properties, and Resemblance to Observations
• The small and the beautiful: How the star formation law affects galactic disk structure
• Multi-thermal jet formation triggered by flux emergence
• A new method for measuring the 3D turbulent velocity dispersion of molecular clouds
• Hydrodynamics and survivability during post-main-sequence planetary engulfment
• The role of turbulence during the formation of circumbinary discs
• Effects of Grain Alignment Efficiency on Synthetic Dust Polarization Observations of Molecular Clouds
• Distribution and kinematics of 26Al in the Galactic disc
• Simulations of the merging galaxy cluster Abell 2034: what determines the level of separation between gas and dark matter
• Galactic winds and bubbles from nuclear starburst rings
• Simulating Gas Inflow at the Disk-Halo Interface
• Imprints of the first billion years: Lyman limit systems at $z\sim 5$
• On The Road To More Realistic Galaxy Cluster Simulations: The Effects of Radiative Cooling and Thermal Feedback Prescriptions on the Observational Properties of Simulated Galaxy Clusters
• Black hole formation in relativistic Oscillaton collisions
• Physics of Thermonuclear Explosions: Magnetic Field Effects on Deflagration Fronts and Observable Consequences
• Environmental Dependence of Self-Regulating Black-hole Feedback in Massive Galaxies
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• The complexity that the first stars brought to the Universe: Fragility of metal enriched gas in a radiation field
• Frequent Spin Reorientation of Galaxies due to Local Interactions
• Exploring Simulated Early Star Formation in the Context of the Ultrafaint Dwarf Galaxies
• Non-equilibrium Ionization States Within Galactic Outflows: Explaining Their O VI and N V Column Densities
• Magnetohydrodynamic Simulations of the Tayler Instability in Rotating Stellar Interiors
• Stellar angular momentum can be controlled from cosmological initial conditions
• External Enrichment of Minihalos by the First Supernovae
• Magnetic fields during galaxy mergers
• Non-ideal MHD simulations of subcritical prestellar cores with non-equilibrium chemistry
• Global radiation signature from early structure formation
• The Catalogue for Astrophysical Turbulence Simulations (CATS)
• Infrared Properties of z=7 Galaxies from Cosmological Simulations
• A Moving Mesh Hydrodynamic Solver for ChaNGa
• Positive or Negative? The Impact of X-ray Feedback on the Formation of Direct Collapse Black Hole Seeds
• Ram pressure stripping of the multiphase ISM: a detailed view from TIGRESS simulations
• Direct-collapse black hole formation induced by internal radiation of host halos
• The dependence of episodic accretion on eccentricity during the formation of binary stars
• Phase spirals in cosmological simulations of Milky Way-size galaxies
• Catalogue of model star clusters in the Milky Way and M31 galaxies
• One-Two Quench: A Double Minor Merger Scenario
• GMC Evolution in a Barred Spiral Galaxy with Star Formation and Thermal Feedback
• The Obsidian model: Three regimes of black hole feedback
• Energy-dependent and energy-integrated two-moment general-relativistic neutrino transport simulations of hypermassive neutron star
• The Dispersion Measure Contributions of the Cosmic Web
• Gravitational dynamics in Higgs inflation: Preinflation and preheating with an auxiliary field
• Cosmological Simulations of Isotropic Conduction in Galaxy Clusters
• The formation of the primitive star SDSS J102915+172927: effect of the dust mass and the grain-size distribution
• Cosmological simulations of self-interacting Bose-Einstein condensate dark matter
• Simulations of gas sloshing induced by a newly discovered gas poor substructure in galaxy cluster Abell 1644
• Probing the CGM of Low-redshift Dwarf Galaxies Using FIRE Simulations
• The turbulent life of dust grains in the supernova-driven, multi-phase interstellar medium
• It's a Breeze: The Circumgalactic Medium of a Dwarf Galaxy is Easy to Strip
• Stellar Influence on Heavy Ion Escape from Unmagnetized Exoplanets
• Shattering and growth of cold clouds in galaxy clusters: the role of radiative cooling, magnetic fields and thermal conduction
• Cosmic Reionization On Computers: The Galaxy-Halo Connection between $5\le z\le 10$
• A Parsec-Scale Catalog of Molecular Clouds in the Solar Neighborhood Based on 3D Dust Mapping: Implications for the Mass-Size Relation
• Time Dependent Radiation Hydrodynamics on a Moving Mesh
• The Effect of Mixing on the Observed Metallicity of the Smith Cloud
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• The Response of Metal Rich Gas to X-Ray Irradiation from a Massive Black Hole at High Redshift: Proof of Concept
• Probing the Dependence of the Intergalactic Medium on Large Scale Environment Using the Low Redshift Lyman Alpha Forest
• An Extension of the Athena++ Framework for Fully Conservative Self-Gravitating Hydrodynamics
• Cosmic Ray Transport in the Ionized and Neutral ISM: MHD-PIC Simulations and Effective Fluid Treatments
• One-Armed Spiral Instability in Double-Degenerate Post-Merger Accretion Disks
• Tidal disruption of star clusters in galaxy formation simulations
• Radiative Turbulent Mixing Layers and the Survival of Magellanic Debris
• Catastrophic Cooling in Superwinds. III. Non-equilibrium Photoionization
• Dynamical signatures of Rossby vortices in cavity-hosting disks
• Stress-Testing Cosmic Ray Physics: The Impact of Cosmic Rays on the Surviving Disk of Ram Pressure Stripped Galaxies
• Evolution and the quasistationary state of collective fast neutrino flavor conversion in three dimensions without axisymmetry
• The Effects of Ram Pressure on the Cold Clouds in the Centers of Galaxy Clusters
• Radiation-driven turbulent accretion onto massive black holes
• Magnetic field draping around clumpy high-velocity clouds in galactic halo
• G-virial: Gravity-based structure analysis of molecular clouds
• Houdini for Astrophysical Visualization
• Turbulent Reacceleration of Streaming Cosmic Rays
• On the effect of Lyman alpha trapping during the initial collapse of massive black hole seeds
• The properties of magnetised cold filaments in a cool-core galaxy cluster
• Repeating Partial Tidal Encounters of Sun-like Stars Leading to their Complete Disruption
• The impact of magnetic fields on the chemical evolution of the supernova-driven ISM
• The Manhattan Suite: Accelerated galaxy evolution in the early Universe
• The Association of Molecular Gas and Natal Super Star Clusters in Henize 2-10
• The Three-Dimensional Collapse of a Rapidly Rotating 16 $M_{\odot }$ Star
• Numerical Stability of Detonations in White Dwarf Simulations
• The effect of dark matter resolution on the collapse of baryons in high redshift numerical simulations
• Chemistry as a diagnostic of prestellar core geometry
• Carbon Detonation Initiation in Turbulent Electron-Degenerate Matter
• High Resolution Study of Planetesimal Formation by Gravitational Collapse of Pebble Clouds
• Detecting the neutral IGM in filaments with the SKA
• Gray Two-moment Neutrino Transport: Comprehensive Tests and Improvements for Supernova Simulations
• Simulations of the symbiotic recurrent nova V407 Cyg. I. Accretion and shock evolutions
• Probabilistic cosmic web classification using fast-generated training data
• Role of magnetic fields in the formation of direct collapse black holes
• Thermal emission from bow shocks II: 3D magnetohydrodynamic models of Zeta Ophiuchi
• Fast cloud-cloud collisions in a strongly barred galaxy: Suppression of massive star formation
• General Relativistic Hydrodynamics on a Moving-mesh I: Static Spacetimes
• Dynamics of Laterally Propagating Flames in X-ray Bursts. I. Burning Front Structure
• Can we observe the ion-neutral drift velocity in prestellar cores?
• Clouds accreting from the IGM are not able to feed the star formation of low-redshift disc galaxies
• Effects of Galactic Disc Inclination and Resolution on Observed GMC Properties and Larson's Scaling Relations
• Kinetic and internal energy transfer in implicit large eddy simulations of forced compressible turbulence
• Modeling Photoionized Turbulent Material in the Circumgalactic Medium
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• The Co-Evolution of a Magnetized Intracluster Medium and Hot Galactic Coronae: Magnetic Field Amplification and Turbulence Generation
• A Magnetized, Moon-Forming Giant Impact
• Sloshing of Galaxy Cluster Core Plasma in the Presence of Self-Interacting Dark Matter
• An Improved Method for Coupling Hydrodynamics with Astrophysical Reaction Networks
• Column Density Profiles of Cold Clouds Driven by Galactic Outflows
• The Antesonic Condition for the Explosion of Core-Collapse Supernovae I: Spherically Symmetric Polytropic Models: Stability & Wind Emergence
• Fragmentation in Population III Galaxies formed through Ionizing Radiation
• Weighing the IMBH candidate CO-0.40-0.22* in the Galactic Centre
• Modeling Photoionized Turbulent Material in the Circumgalactic Medium II: Effect of Turbulence within a Stratified Medium
• thornado-hydro: a discontinuous Galerkin method for supernova hydrodynamics with nuclear equations of state
• On estimating angular momenta of infalling protostellar cores from observations
• Evolution of Main-Sequence-like Surviving Companions in Type Ia Supernova Remnants
• The Physical Nature of Circumgalactic Medium Absorbers in Simba
• Production Efficiencies of Sound Waves in the Intracluster Medium Driven by AGN Jets
• Modeling gravitational instabilities in self-gravitating protoplanetary disks with adaptive mesh refinement techniques
• Cinematic Visualization of Multiresolution Data: Ytini for Adaptive Mesh Refinement in Houdini
• Turbulence-driven thermal and kinetic energy fluxes in the atmospheres of hot Jupiters
• Collapse and Fragmentation of Magnetic Molecular Cloud Cores with the Enzo AMR MHD Code. II. Prolate and Oblate Cores
• On Architecture and Performance of Adaptive Mesh Refinement in an Electrostatics Particle-In-Cell Code
• Fully Coupled Simulation of Cosmic Reionization. III. Stochastic Early Reionization by the Smallest Galaxies
• Efficient radial migration by giant molecular clouds in the first several hundred Myr after the stellar birth
• Signatures of Massive Black Hole Merger Host Galaxies from Cosmological Simulations I: Unique Galaxy Morphologies in Imaging
• A Numerical Study of the Impact of Jet Magnetic Topology on Radio Galaxy Evolution
• Exploring the Observability of Surviving Companions of Stripped-Envelope Supernovae: A Case Study of Type Ic SN 2020oi
• The Role of Quasar Radiative Feedback on Galaxy Formation during Cosmic Reionization
• The Gaia-ESO Survey: Matching Chemo-Dynamical Simulations to Observations of the Milky Way
• Orbital Migration of Protoplanets in a Marginally Gravitationally Unstable Disk. II. Migration, Merging, and Ejection
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning
• If dark matter is fuzzy, the first stars form in massive pancakes
• Unveiling the role of galactic rotation on star formation
• Exploring the effects of primordial non-Gaussianity at galactic scales
• Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition
• Gravitational Fragmentation of Extremely Metal-poor Circumstellar Discs
• On the Mass Loading of AGN-Driven Outflows in Elliptical Galaxies and Clusters
• Emulating Sunyaev-Zeldovich Images of Galaxy Clusters using Auto-Encoders
• Constraining the Fluctuating Gunn-Peterson Approximation Using Lyman-$\alpha$ Forest Tomography at $z=2$
• Terapixel imaging of cosmological simulations
• How do supernova remnants cool? -- I. Morphology, optical emission lines, and shocks
• Neural Networks for Nuclear Reactions in MAESTROeX
• Direct Collapse to Supermassive Black Hole Seeds: Comparing the AMR and SPH Approaches
• The Evaporation and Survival of Cluster Galaxies' Coronae Part I: The Effectiveness of Isotropic Thermal Conduction Including Saturation
• Amplification and saturation of turbulent magnetic field in collapsing primordial gas clouds
• A multishock scenario for the formation of radio relics
• Influence of neutrino-electron scattering and neutrino-pair annihilation on hypermassive neutron star
• Thermal and Chemical Evolution of Collapsing Filaments
• The causal effect of environment on halo mass and concentration
• Connecting Primordial Star Forming Regions and Second Generation Star Formation in the Phoenix Simulations
• Comparing Simulated Emission from Molecular Clouds Using Experimental Design
• Sensitivity of non-radiative cloud-wind interactions to the hydrodynamics solver
• Intergalactic medium rotation measure of primordial magnetic fields
• The Merger Dynamics of the Galaxy Cluster Abell 1775: New Insights from Chandra and XMM-Newton for a Cluster Simultaneously Hosting a WAT and a NAT Radio Sources
• Induced metal-free star formation around a massive black hole seed
• Manufacturing cosmic rays in the evolving dynamical states of galaxy clusters
• The Interstellar Medium and Star Formation in Local Galaxies: Variations of the Star Formation Law in Simulations
• ASymba: HI global profile asymmetries in the Simba simulation
• Unravelling cosmic velocity flows: a Helmholtz-Hodge decomposition algorithm for cosmological simulations
• Massive core/star formation triggered by cloud-cloud collision: II High-speed collisions of magnetized clouds
• Galactic disc heating by density granulation in fuzzy dark matter simulations
• Constraining black hole feedback in galaxy clusters from X-ray power spectra
• Cosmic Reionization On Computers: Reionization Histories of Present-day Galaxies
• Rethinking Thorne-Żytkow Object Formation: The Fate of X-ray Binary LMC X-4 and Implications for Ultra-long Gamma-ray Bursts
• Structure in the 3D Galaxy Distribution: II. Voids and Watersheds of Local Maxima and Minima
• Does modified gravity predict fast stellar bars in spiral galaxies?
• The velocity structure of the intracluster medium during a major merger: simulated microcalorimeter observations
• Linear dust polarization during the embedded phase of protostar formation
• Impact of Rotation on the Multimessenger Signatures of a Hadron-quark Phase Transition in Core-collapse Supernovae
• First Star Formation in the Presence of Primordial Magnetic Fields
• Magnetic Island Merging: Two-dimensional MHD Simulation and Test-Particle Modeling
• The formation and stability of a cold disc made out of stellar winds in the Galactic Centre
• Halo formation and evolution in scalar field dark matter and cold dark matter: New insights from the fluid approach
• Hyenas: X-ray Bubbles and Cavities in the Intra-Group Medium
• High angular momentum hot differentially rotating equilibrium star evolutions in conformally flat spacetime
• Cloud-cloud collisions triggering star formation in galaxy simulations
• The kinetic and magnetic energy budget of hub-filament systems during the gravitational fragmentation of molecular clouds
• Inflationary and phase-transitional primordial magnetic fields in galaxy clusters
• Dynamical friction of a massive black hole in a turbulent gaseous medium
• Firefly: a browser-based interactive 3D data visualization tool for millions of data points
• Type Ia supernova ejecta-donor interaction: explosion model comparison
• The Impact of Resolution on Double-Detonation Models for Type Ia Supernovae
• Influence of adaptive mesh refinement and the hydro solver on shear-induced mass stripping in a minor-merger scenario
• Entropy-Conserving Scheme for Modeling Nonthermal Energies in Fluid Dynamics Simulations
• Dynamics of Laterally Propagating Flames in X-ray Bursts. II. Realistic Burning & Rotation
• Distinguishing AGN Feedback Models with the Thermal Sunyaev-Zel'dovich Effect
• When Gas Dynamics Decouples from Galactic Rotation: Characterizing ISM Circulation in Disk Galaxies
• Evolution and feedback of AGN Jets of different Cosmic-ray Composition
• The parameter-free Finger-Of-God model and its application to 21cm intensity mapping
• A common origin for the circumnuclear disc and the nearby molecular clouds in the Galactic Centre
• Numerical Study of Cosmic Ray Confinement through Dust Resonant Drag Instabilities
• Formation and evolution of the local interstellar environment: combined constraints from nucleosynthetic and X-ray data
• C IV and He II Line Emission of Lyman Alpha Blobs: Powered by Shock Heated Gas
• An uncertainty principle for star formation -- V. The influence of dust extinction on star formation rate tracer lifetimes and the inferred molecular cloud lifecycle
• Radio-relic and the diffuse emission trail discovered in a low mass galaxy cluster Abell 1697
• MPRAD: A Monte Carlo and ray-tracing code for the proton radiography in high-energy-density plasma experiments
• Interpreting Observations of Absorption Lines in the Circumgalactic Medium with a Turbulent Medium
• GMC Collisions As Triggers of Star Formation. IV. The Role of Ambipolar Diffusion
• The life cycle of starbursting circumnuclear gas discs
• Amplification of Magnetic Fields in a Primordial HII Region and Supernova
• Formation and fate of the born-again planetary nebula HuBi 1
• Bringing Simulation and Observation Together to Better Understand the Intergalactic Medium
• Seeking Self-Regulating Simulations of Idealized Milky Way-Like Galaxies
• Long-term evolution of post-explosion Helium-star Companions of Type Iax Supernovae
• Escaping the maze: a statistical sub-grid model for cloud-scale density structures in the interstellar medium
• The Alamo multiphysics solver for phase field simulations with strong-form mechanics and block structured adaptive mesh refinement
• Magnetic fields limit the mass of Population III stars even before the onset of protostellar radiation feedback
• Numerical study of solar eruption, extreme-ultraviolet wave propagation, and wave-induced prominence dynamics
• Tree-less 3d Friends-of-Friends using Spatial Hashing
• Population III star formation in the presence of turbulence, magnetic fields and ionizing radiation feedback
• Radiative transfer of Lyman-$\alpha$ photons at cosmic dawn with realistic gas physics
• The Evaporation and Survival of Cluster Galaxies' Coronae Part II: The Effectiveness of Anisotropic Thermal Conduction and Survival of Stripped Galactic Tails
• Modeling molecular hydrogen in low metallicity galaxies
• The influence of the cloud virial parameter on the initial mass function
• Moving and Reactive Boundary Conditions in Moving-Mesh Hydrodynamics
• The Intrinsic Stochasticity of the ${}^{56}$Ni Distribution of Single-Degenerate Type Ia Supernovae
• Atmospheric Circulation in Simulations of the AGN-CGM Connection at Halo Masses $\sim 10^{13.5},M_{\odot }$
• Saturation level of turbulence in collapsing gas clouds
• Gas accretion and Ram Pressure Stripping of Haloes in Void Walls
• Biconical-dominated Accretion Flow onto Seed Black Holes in a Hyper-accretion Regime
• Inverse Compton cooling of thermal plasma in colliding-wind binaries
• The Evolution of Binaries Embedded Within Common Envelopes
• The Impact of Shocks on the Vertical Structure of Eccentric Disks
• An adaptive particle-mesh gravity solver for ENZO
• General-relativistic resistive-magnetohydrodynamics simulations of self-consistent magnetized rotating neutron stars
• Varying Driver Velocity Fields in Photospheric MHD Wave Simulations
• Hungry or Not: How Stellar-Mass Black Holes Grow (or Don't) in Dark Matter Mini-Haloes at High-Resolution
• Deep Neural Networks for Modeling Astrophysical Nuclear Reacting Flows
• The Antesonic Condition for the Explosion of Core-Collapse Supernovae II: Rotation and Turbulence
• The impact of cosmic ray heating on the cooling of the low-metallicity interstellar medium
• The Effect of Impact Parameter on Tidal Disruption Events
• Consistency analysis of a Dark Matter velocity dependent force as an alternative to the Cosmological Constant
• Toward Resolved Simulations of Burning Fronts in Thermonuclear X-ray Bursts
• Relative baryon-dark matter velocities in cosmological zoom simulations
• Dipolar dark matter simulations on galaxy scales with the RAMSES code
• CosmoDRAGoN simulations -- I. Dynamics and observable signatures of radio jets in cosmological environments
• Dynamical Properties of Molecular-forming Gas Clumps in Galaxies at the Epoch of Reionization
• Tracking Advanced Planetary Systems (TAPAS) with HARPS-N. V.: A Massive Jupiter orbiting the very low metallicity giant star BD+03 2562 and a possible planet around HD~103485
• Particle-in-Cell Simulations of Relativistic Magnetic Reconnection with Advanced Maxwell Solver Algorithms
• The Effect of Warm Dark Matter on Early Star Formation Histories of Massive Galaxies: Predictions from the CROC Simulations
• Effects of Anisotropic Viscosity on the Evolution of Active Galactic Nuclei Bubbles in Galaxy Clusters
• GMC Collisions As Triggers of Star Formation. VIII. The Core Mass Function
• Kinetics of the chiral phase transition in a linear $\sigma$ model
• Modeling Photoionized Turbulent Material in the Circumgalactic Medium III: Effects of Co-rotation and Magnetic Fields
• Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping
• Understanding biases in measurements of molecular cloud kinematics using line emission
• Post-inflationary structure formation boosted by parametric self-resonance
• Comparing Early Evolution of Flames in X-ray Bursts in Two and Three Dimensions
• 3D AMR hydrosimulations of a compact source scenario for the Galactic Centre cloud G2
• The Hierarchical Structure of Galactic Haloes: Classification and characterisation with Halo-OPTICS
• Tracking Advanced Planetary Systems (TAPAS) with HARPS-N VII. Elder suns with low-mass companions
• Simulating the pericentre passage of the Galactic centre star S2
• Galaxy pairs in The Three Hundred simulations II: studying bound ones and identifying them via machine learning
• Large Scale Dynamo in a Primordial Accretion Flow -- An Interpretation from Hydrodynamic Simulation
• Suppression of H2-cooling in protogalaxies aided by trapped Lyα cooling radiation
• The Physical Nature of the Most Metal-Poor Damped Lyman Alpha Systems
• Honing and proofing Astrophysical codes on the road to Exascale. Experiences from code modernization on many-core systems
• Paicos: A Python package for analysis of (cosmological) simulations performed with Arepo
• A toy model for gas sloshing in galaxy clusters
• Nonlinear cosmological structure with ultralight bosons via modified gravity
• Investigating dusty Red Supergiant outflows in Westerlund 1 with 3D Hydrodynamic simulations
• Resilience of Sloshing Cold Fronts against Subsequent Minor Mergers
• XMAGNET: Velocity structure functions of active galactic nucleus-driven turbulence in the multiphase intracluster medium
• Temporal Self-Organization in Galaxy Formation
• The environments of the radio galaxy population in SIMBA
• Eigenvalue Method for NEI Unit in FLASH Code
• Can Cooling and Heating Functions be Modeled with Homogeneous Radiation Fields?
• Jet interaction with galaxy cluster mergers
• Accelerated growth of seed black holes by dust in the early universe
• Comparison of Electron Capture Rates in the N=50 Region using 1D Simulations of Core-collapse Supernovae
• Molecular Shattering
• Hydrodynamic simulations of WD-WD mergers and the origin of RCB stars
• Protostellar spin-up and fast rotator formation through binary star formation
• Bimodal Star Formation in Simulations of Strongly Magnetized Giant Molecular Clouds
• Thermal emission from bow shocks. III. Variable diffuse X-ray emission from stellar-wind bow shocks driven by dynamical instabilities
• Touching the Stars: Using High-Resolution 3D Printing to Visualize Stellar Nurseries
• The AGORA High-resolution Galaxy Simulations Comparison Project. VIII: Disk Formation and Evolution of Simulated Milky Way Mass Galaxy Progenitors at $1<z<5$
• Local two-dimensional simulations of the ignition of a helium shell detonation on a white dwarf by an impacting stream
• Geometry and Scaling Laws of Excursion and Iso-sets of Enstrophy and Dissipation in Isotropic Turbulence
• Fuzzy dark matter simulations
• Cosmic Reionization On Computers: Statistics, Physical Properties and Environment of Lyman Limit Systems at $z\sim 6$
• The Castro AMR Simulation Code: Current and Future Developments
• Hydrodynamical simulations of proton ingestion flashes in Type I X-ray Bursts
• Predicting Localized Primordial Star Formation with Deep Convolutional Neural Networks
• Thermonuclear (Type Ia) Supernovae and Progenitor Evolution
• The Convergence of Particle-in-Cell Schemes for Cosmological Dark Matter Simulations
• Wide-binary eccentricity distribution in young star clusters: dependence on the binary separation and mass
• Tracing the Origins of Hot Halo Gas in Milky Way-Type Galaxies with SMUGGLE
• Evolving beyond z=0: insights about the future of stars and the intergalactic medium
• Formation of Compact Clusters from High Resolution Hybrid Cosmological Simulations
• From theory to observation: understanding filamentary flows in high-mass star-forming clusters
• Cospatial 21 cm and metal-line absorbers in the epoch of reionization -- I : Incidence and observability
• Capturing Turbulence with Numerical Dissipation: a Simple Dynamical Model for Unresolved Turbulence in Hydrodynamic Simulations
• Forming the local starburst galaxy Haro 11 through hydrodynamical merger simulations
• Rotation measure and synchrotron emission signatures in simulations of magnetized galactic discs
• Using dust to constrain dark matter models
• Reconciling the magnetic field in central disc galaxies with the dynamical mass using the cosmological simulations
• Tests of AGN Feedback Kernels in Simulated Galaxy Clusters
• Formation of a Bose Star in a Rotating Cloud
• Direct Collapse Accretion Disks Within Dark Matter Halos: Saturation of the Magnetorotational Instability and the Field Expulsion
• OVI Emission From the Supernovae-regulated Interstellar Medium: Simulation Vs Observation
• Triggered Population III star formation: the effect of H${}_2$ self-shielding
• Emerging planetary nebulae within 3D spiral patterns
• Tree-based solvers for adaptive mesh refinement code FLASH -- IV: An X-ray radiation scheme to couple discrete and diffuse X-ray emission sources to the thermochemistry of the interstellar medium
• SWIFTGalaxy: a Python package to work with particle groups from SWIFT simulations
• Spectral Characteristics of a Rotating Solar Prominence in Multiple Wavelengths
• gadfly: A pandas-based Framework for Analyzing GADGET Simulation Data
• Catastrophic Cooling in Superwinds. II. Exploring the Parameter Space
• Slow Cooling in Low Metallicity Clouds: An Origin of Globular Cluster Bimodality?
• Observing galaxy mergers at the epoch of reionization
• Star-forming galaxies in the cosmic web in the last 11 Gyr
• 3D Convective Urca Process in a Simmering White Dwarf
• HI asymmetries in spatially resolved SIMBA galaxies
• SIGAME v3: Gas Fragmentation in Post-processing of Cosmological Simulations for More Accurate Infrared Line Emission Modeling
• Direct Collapse to Precursors of Supermassive Black Hole Seeds:Radiation-feedback-generated Outflows
• Radiation magnetohydrodynamics simulations of Population III star formation during the Epoch of Reionization
• A Parametric Study of the SASI Comparing General Relativistic and Nonrelativistic Treatments
• An Observationally Driven Multifield Approach for Probing the Circum-Galactic Medium with Convolutional Neural Networks
• X-ray stacking reveals average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4 <~ z <~ 7
• The imprint of magnetic fields on absorption spectra from circumgalactic wind-cloud systems
• Simulating Lateral H/He Flame Propagation in Type I X-ray Bursts
• Simulated Rotation Measure Sky from Primordial Magnetic Fields
• Identifying Halos in Cosmological Simulations with Continuous Wavelet Analysis: The 2D Case
• Intergalactic-Absorption Confounding Circumgalactic Observations
• Quokka-based understanding of outflows (QED) -- II. X-ray metallicity gradients as a signature of galactic wind metal loading
• Bunch-Davies initial conditions and non-perturbative inflationary dynamics in Numerical Relativity
• An adaptive mesh, GPU-accelerated, and error minimized special relativistic hydrodynamics code
• The Observed O VI is Just the Tip of the Iceberg: Estimating the Hidden Material in Circumgalactic and Intergalactic Clouds
• Tidal phenomena in the Galactic Center: The curious case of X7
• Origin of Weak MgII and Higher Ionization Absorption Lines in an Outflow from an Intermediate-Redshift Dwarf Satellite Galaxy
• Reduced Gas Accretion onto Galaxies due to Effects of External Giant Radio Lobes
• Effect of cosmic rays and ionizing radiation on observational ultraviolet plasma diagnostics in the circumgalactic medium
• Constraining cosmic ray transport models using circumgalactic medium properties and observables
• Free-floating molecular clumps and gas mixing: hydrodynamic aftermaths of the intracluster$-$interstellar medium interaction
• CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform
• Multi-cloud crushing -- the collective survival of cold clouds in galactic outflows
• SILCC -- IX. The multi-phase interstellar medium at low metallicity
• Neutron Star-Main Sequence Collisions Robustly Form Dynamically Stable Thorne-Żytkow Objects
• Investigating the residuals in the $M_{\bullet }-M_{\ast }$ relation using the SIMBA cosmological simulation
• What goes around comes around: the fate of stars in stripped tails of gas
• Numerical Simulations of the Random Angular Momentum in Convection: Implications for Supergiant Collapse to Form Black Holes
• Hyperaccreting Neutron Stars inside Massive Envelopes: The Implausibility of Thorne-Żytkow Objects
• Toward First-Principles Multi-Messenger Predictions: Coupling Nuclear Networks with GR Radiation-MHD in {\tt Gmunu}
• How do supernova remnants cool? II. Machine learning analysis of supernova remnant simulations
• Multi-wavelength emission from leptonic processes in ageing galaxy bubbles
• Early Stages of Dusty Tori: The First Infrared Spectra from a Highly Multiscale Quasar Simulation
• Software Abstractions and Methodologies for HPC Simulation Codes on Future Architectures
• Tidal disruption events as the origin of the eROSITA and Fermi bubbles
• Quokka-based understanding of outflows (QED) -- IV. Limitations of H$\alpha$ as an outflow diagnostic
• Sensitivity of 3D Convective Urca Simulations to Changes in Urca Reactions
• Validating the CROCODILE model within the AGORA galaxy simulation framework
• The role of gas fragmentation during the formation of supermassive black holes
• Gas flows in galaxy mergers: supersonic turbulence in bridges, accretion from the circumgalactic medium, and metallicity dilution
• EWOCS-V: Is Wd1-72 a recent post-interaction WR+O binary?
• libyt: an In Situ Interface Connecting Simulations with yt, Python, and Jupyter Workflows
• Supernovae in colliding-wind binaries: observational signatures in the first year
• Redshift effects implications on revised models of Stephan's quintet
• On the Importance of the Convective Urca Process in 3D Simulations of a Simmering White Dwarf
• Controlled Experiments on Dark-Matter Halo Structure and Galaxy Morphology I: What Sets Galaxy Sizes?
• Evidence for mixing between ICM and stripped ISM by the analysis of the gas metallicity in the tails of jellyfish galaxies
• Momentum deposition of supernovae with cosmic rays
• A resolution criterion based on characteristic timescales for MHD simulations of molecular clouds
• Transferring Data from a Voronoi Mesh to an Adaptive Cartesian Grid in Pursuit of Self-consistent Top-down Star Formation
• Real time, cross platform visualizations with zero dependencies for the N-body package REBOUND
• Simulating Jellyfish Galaxies: A Case Study for a Gas-Rich Dwarf Galaxy
• Modeling turbulent and self-gravitating fluids with Fourier neural operators
• The cosmic journey of dust grains -- from nucleation to planetary system
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• Turbulence in the intragroup and circumgalactic medium
• A Discontinuous Galerkin Method for General Relativistic Hydrodynamics in thornado
• Magnetized Decaying Turbulence in the Weakly Compressible Taylor-Green Vortex
• Simulating High-Velocity Clouds in the Observational Plane: An Initial Study with the Smith Cloud
• The DORCHA suite: nature, nurture, and the phase space distribution of the Milky Way's high redshift progenitors today
• Direct Collapse Pre-supermassive Black Hole Objects as Ly$\alpha$ Emitters
• Identification of Candidate Halos Hosting Massive Black Hole Seeds in the $\text{Renaissance}$ Simulations with Support Vector Machines