FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation

Abstract

The Feedback In Realistic Environments (FIRE) project explores feedback in cosmological galaxy formation simulations. Previous FIRE simulations used an identical source code (FIRE-1) for consistency. Motivated by the development of more accurate numerics - including hydrodynamic solvers, gravitational softening, and supernova coupling algorithms - and exploration of new physics (e.g. magnetic fields), we introduce FIRE-2, an updated numerical implementation of FIRE physics for the GIZMO code. We run a suite of simulations and compare against FIRE-1: overall, FIRE-2 improvements do not qualitatively change galaxy-scale properties. We pursue an extensive study of numerics versus physics. Details of the star-formation algorithm, cooling physics, and chemistry have weak effects, provided that we include metal-line cooling and star formation occurs at higher-than-mean densities. We present new resolution criteria for high-resolution galaxy simulations. Most galaxy-scale properties are robust to numerics we test, provided: (1) Toomre masses are resolved; (2) feedback coupling ensures conservation, and (3) individual supernovae are time-resolved. Stellar masses and profiles are most robust to resolution, followed by metal abundances and morphologies, followed by properties of winds and circum-galactic media (CGM). Central (~kpc) mass concentrations in massive (L*) galaxies are sensitive to numerics (via trapping/recycling of winds in hot halos). Multiple feedback mechanisms play key roles: supernovae regulate stellar masses/winds; stellar mass-loss fuels late star formation; radiative feedback suppresses accretion onto dwarfs and instantaneous star formation in disks. We provide all initial conditions and numerical algorithms used.

arXiv comment64 pages, 40 figures. Simulation animations and visualizations available at http://www.tapir.caltech.edu/~phopkins/Site/animations and http://fire.northwestern.edu . Paper includes complete FIRE algorithms and public ICs (http://www.tapir.caltech.edu/~phopkins/publicICs). Updated to match published version

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• Baryon Cycles in the Biggest Galaxies
• On the Survival of Cool Clouds in the Circum-Galactic Medium
• Deep learning predictions of galaxy merger stage and the importance of observational realism
• AREPO-RT: Radiation hydrodynamics on a moving mesh
• Radiative Stellar Feedback in Galaxy Formation: Methods and Physics
• Semi-analytic forecasts for JWST -- II. physical properties and scaling relations for galaxies at z = 4-10
• Timing the Early Assembly of the Milky Way with the H3 Survey
• The time-scales probed by star formation rate indicators for realistic, bursty star formation histories from the FIRE simulations
• The Diversity and Variability of Star Formation Histories in Models of Galaxy Evolution
• The physics of Lyman-alpha escape from high-redshift galaxies
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• Supernova-driven winds in simulated dwarf galaxies
• Supernova feedback in numerical simulations of galaxy formation: separating physics from numerics
• Robust HI kinematics of gas-rich ultra-diffuse galaxies: hints of a weak-feedback formation scenario
• Green Bank and Effelsberg Radio Telescope Searches for Axion Dark Matter Conversion in Neutron Star Magnetospheres
• Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields
• Post-Newtonian Dynamics in Dense Star Clusters: Binary Black Holes in the LISA Band
• The effects of cosmic rays on the formation of Milky Way-mass galaxies in a cosmological context
• Predicting the binary black hole population of the Milky Way with cosmological simulations
• Heart of Darkness: the influence of galactic dynamics on quenching star formation in galaxy spheroids
• Testing Physical Models for Cosmic Ray Transport Coefficients on Galactic Scales: Self-Confinement and Extrinsic Turbulence at GeV Energies
• Galaxy Formation with BECDM -- II. Cosmic Filaments and First Galaxies
• Spatially resolved star formation and fuelling in galaxy interactions
• Dynamical Friction in a Fuzzy Dark Matter Universe
• The physics of multiphase gas flows: fragmentation of a radiatively cooling gas cloud in a hot wind
• Cooling flow solutions for the circumgalactic medium
• How galaxies form stars: the connection between local and global star formation in galaxy simulations
• Self-consistent proto-globular cluster formation in cosmological simulations of high-redshift galaxies
• Diversity of dark matter density profiles in the Galactic dwarf spheroidal satellites
• Efficient early stellar feedback can suppress galactic outflows by reducing supernova clustering
• The effect of magnetic fields on properties of the circumgalactic medium
• A survey of high-$z$ galaxies: SERRA simulations
• SIDM on FIRE: Hydrodynamical Self-Interacting Dark Matter simulations of low-mass dwarf galaxies
• Disruption of giant molecular clouds and formation of bound star clusters under the influence of momentum stellar feedback
• Hot-mode accretion and the physics of thin-disk galaxy formation
• Simulating Groups and the IntraGroup Medium: The Surprisingly Complex and Rich Middle Ground Between Clusters and Galaxies
• What Causes The Formation of Disks and End of Bursty Star Formation?
• The dark matter interpretation of the 3.5-keV line is inconsistent with blank-sky observations
• No cores in dark matter-dominated dwarf galaxies with bursty star formation histories
• Formation of Globular Cluster Candidates in Merging Proto-galaxies at High Redshift: A View from the FIRE Cosmological Simulations
• Predictions for the spatial distribution of the dust continuum emission in 1<z<5 star-forming galaxies
• First Light And Reionisation Epoch Simulations (FLARES) II: The Photometric Properties of High-Redshift Galaxies
• A model for the formation of stellar associations and clusters from giant molecular clouds
• The Life Cycle of the Central Molecular Zone. I: Inflow, Star Formation, and Winds
• Black Hole -- Galaxy Correlations in Simba
• A tale of two sites -- I: Inferring the properties of minihalo-hosted galaxies from current observations
• NIHAO-UHD: The properties of MW-like stellar disks in high resolution cosmological simulations
• The rapid growth phase of supermassive black holes
• SatGen: a semi-analytical satellite galaxy generator -- I. The model and its application to Local-Group satellite statistics
• Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters
• Semi-analytic forecasts for JWST -- IV. Implications for cosmic reionization and LyC escape fraction
• The Formation Times and Building Blocks of Milky Way-mass Galaxies in the FIRE Simulations
• Ultra-diffuse galaxies in the Auriga simulations
• STARFORGE: The effects of protostellar outflows on the IMF
• Dark Matter Cores and Cusps in Spiral Galaxies and their Explanations
• Which AGN Jets Quench Star Formation in Massive Galaxies?
• Effects of Gas on Formation and Evolution of Stellar Bars and Nuclear Rings in Disk Galaxies
• Project AMIGA: The Circumgalactic Medium of Andromeda
• Cosmic-Ray Driven Outflows to Mpc Scales from $L_{\ast }$ Galaxies
• JADES: The incidence rate and properties of galactic outflows in low-mass galaxies across 3 < z < 9
• Physical Processes in Star Formation
• A multi-messenger study of the Milky Way's stellar disc and bulge with LISA, Gaia and LSST
• Planes of satellites around Milky Way/M31-mass galaxies in the FIRE simulations and comparisons with the Local Group
• The Fates of the Circumgalactic Medium in the FIRE Simulations
• The physics of gas phase metallicity gradients in galaxies
• Magnetising the circumgalactic medium of disk galaxies
• Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
• Simulating galaxies in the reionization era with FIRE-2: morphologies and sizes
• Warm dust in high-z galaxies: origin and implications
• The abundance of satellites around Milky Way- and M31-like galaxies with the TNG50 simulation: a matter of diversity
• Core-collapse, evaporation and tidal effects: the life story of a self-interacting dark matter subhalo
• A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
• Dwarf Galaxies in CDM, WDM, and SIDM: Disentangling Baryons and Dark Matter Physics
• The THESAN project: ionizing escape fractions of reionization-era galaxies
• Modeling the Connection Between Subhalos and Satellites in Milky Way-like Systems
• Inside Out and Upside-Down: The Roles of Gas Cooling and Dynamical Heating in Shaping the Stellar Age-Velocity Relation
• High-redshift quasars and their host galaxies I: kinematical and dynamical properties and their tracers
• The maximum accretion rate of hot gas in dark matter halos
• Two can play at that game: constraining the role of supernova and AGN feedback in dwarf galaxies with cosmological zoom-in simulations
• Spurious heating of stellar motions in simulated galactic disks by dark matter halo particles
• Stellar Radiation is Critical for Regulating Star Formation and Driving Outflows in Low Mass Dwarf Galaxies
• The dust-continuum size of TNG50 galaxies at $z=1-5$: a comparison with the distribution of stellar light, stars, dust and H${}_2$
• From diffuse gas to dense molecular cloud cores
• The role of mergers and interactions in driving the evolution of dwarf galaxies over cosmic time
• The Keck Baryonic Structure Survey: Using foreground/background galaxy pairs to trace the structure and kinematics of circumgalactic neutral hydrogen at $z\sim 2$
• The bursty origin of the Milky Way thick disc
• First results from SMAUG: Uncovering the Origin of the Multiphase Circumgalactic Medium with a Comparative Analysis of Idealized and Cosmological Simulations
• Rapid disc settling and the transition from bursty to steady star formation in Milky Way-mass galaxies
• NIHAO XX: The impact of the star formation threshold on the cusp-core transformation of cold dark matter haloes
• LYRA I: Simulating the multi-phase ISM of a dwarf galaxy with variable energy supernovae from individual stars
• Galaxies lacking dark matter produced by close encounters in a cosmological simulation
• On The Nature of Variations in the Measured Star Formation Efficiency of Molecular Clouds
• The failure of stellar feedback, magnetic fields, conduction, and morphological quenching in maintaining red galaxies
• The Time Domain Spectroscopic Survey: Changing-Look Quasar Candidates from Multi-Epoch Spectroscopy in SDSS-IV
• Fast and energetic AGN-driven outflows in simulated dwarf galaxies
• Seeds Don't Sink: Even Massive Black Hole "Seeds" Cannot Migrate to Galaxy Centers Efficiently
• Effects of Different Cosmic Ray Transport Models on Galaxy Formation
• Dancing in the Dark: Uncertainty in ultra-faint dwarf galaxy predictions from cosmological simulations
• Nitrogen enrichment and clustered star formation at the dawn of the Galaxy
• Identification of Low Surface Brightness Tidal Features in Galaxies Using Convolutional Neural Networks
• No Assembly Required: Mergers are Mostly Irrelevant for the Growth of Low-mass Dwarf Galaxies
• Galaxy formation with L-GALAXIES: Modelling the environmental dependency of galaxy evolution and comparing with observations
• Metallicity dependence of the H/H${}_2$ and C${}^{+}$/C/CO distributions in a resolved self-regulating interstellar medium
• Powderday: Dust Radiative Transfer for Galaxy Simulations
• Gas infall and radial transport in cosmological simulations of Milky Way-mass disks
• Future constraints on halo thermodynamics from combined Sunyaev-Zel'dovich measurements
• Extraterrestrial Axion Search with the Breakthrough Listen Galactic Center Survey
• Modeling the Impact of Baryons on Subhalo Populations with Machine Learning
• A Framework for Multiphase Galactic Wind Launching using TIGRESS
• Evolution of Stellar Feedback in HII Regions
• The RWST, a comprehensive statistical description of the non-Gaussian structures in the ISM
• Reconciling observed and simulated stellar halo masses
• Outflows and extended [CII] halos in high redshift galaxies
• Velocity dispersion in the interstellar medium of early galaxies
• Extinguishing the FIRE: environmental quenching of satellite galaxies around Milky Way-mass hosts in simulations
• Identification of a transition from stochastic to secular star formation around $z=9$ with JWST
• The Magellanic Stream at 20 kpc: A New Orbital History for the Magellanic Clouds
• Gas Kinematics in FIRE Simulated Galaxies Compared to Spatially Unresolved HI Observations
• Under the Firelight: Stellar Tracers of the Local Dark Matter Velocity Distribution in the Milky Way
• Live Fast, Die Young: GMC lifetimes in the FIRE cosmological simulations of Milky Way-mass galaxies
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• The Magellanic Corona and the formation of the Magellanic Stream
• Environmental Quenching of Low-Mass Field Galaxies
• The cumulative star-formation histories of dwarf galaxies with TNG50. I: Environment-driven diversity and connection to quenching
• 3-D gas-phase elemental abundances across the formation histories of Milky Way-mass galaxies in the FIRE simulations: initial conditions for chemical tagging
• Cosmic Rays or Turbulence can Suppress Cooling Flows (Where Thermal Heating or Momentum Injection Fail)
• The physics of Lyman-alpha escape from disc-like galaxies
• First Predicted Cosmic Ray Spectra, Primary-to-Secondary Ratios, and Ionization Rates from MHD Galaxy Formation Simulations
• From the Top Down and Back Up Again: Star Cluster Structure from Hierarchical Star Formation
• The COS CGM Compendium. III: Metallicity and Physical Properties of the Cool Circumgalactic Medium at z<1
• The star formation rate and stellar content contributions of morphological components in the EAGLE simulations
• Hot Extended Galaxy Halos Around Local L* Galaxies From Sunyaev-Zeldovich Measurements
• Cluster assembly and the origin of mass segregation in the STARFORGE simulations
• Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
• Universal Scaling Relations in Scale-Free Structure Formation
• Born this way: thin disc, thick disc, and isotropic spheroid formation in FIRE-2 Milky-Way-mass galaxy simulations
• Simulating the interstellar medium of galaxies with radiative transfer, non-equilibrium thermochemistry, and dust
• Standard Self-Confinement and Extrinsic Turbulence Models for Cosmic Ray Transport are Fundamentally Incompatible with Observations
• Gaia May Detect Hundreds of Well-characterised Stellar Black Holes
• On the Appearance of Thresholds in the Dynamical Model of Star Formation
• Spectral separation of the stochastic gravitational-wave background for LISA in the context of a modulated Galactic foreground
• A Relationship Between Stellar Metallicity Gradients and Galaxy Age in Dwarf Galaxies
• Photochemistry and Heating/Cooling of the Multiphase Interstellar Medium with UV Radiative Transfer for Magnetohydrodynamic Simulations
• Swirls of FIRE: Spatially Resolved Gas Velocity Dispersions and Star Formation Rates in FIRE-2 Disk Environments
• The role of galactic dynamics in shaping the physical properties of giant molecular clouds in Milky Way-like galaxies
• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• How Biased Are Halo Properties in Cosmological Simulations?
• Rapid early coeval star formation and assembly of the most massive galaxies in the universe
• The central densities of Milky Way-mass galaxies in cold and self-interacting dark matter models
• How low does it go? Too few Galactic satellites with standard reionization quenching
• Pressure balance in the multiphase ISM of cosmologically simulated disk galaxies
• Formation, vertex deviation and age of the Milky Way's bulge: input from a cosmological simulation with a late-forming bar
• The merger-starburst connection across cosmic times
• Star formation at the edge of the Local Group: a rising star formation history in the isolated galaxy WLM
• The COS CGM Compendium. II: Metallicities of the Partial and Lyman Limit Systems at z<1
• Reionization inference from the CMB optical depth and E-mode polarization power spectra
• Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
• Constraints on the assembly history of the Milky Way's smooth, diffuse stellar halo from the metallicity-dependent, radially-dominated velocity anisotropy profiles probed with K giants and BHB stars using LAMOST, SDSS/SEGUE, and Gaia
• On the origin of surprisingly cold gas discs in galaxies at high redshift
• Self-Interacting Dark Matter and the Origin of Ultra-Diffuse Galaxies NGC1052-DF2 and -DF4
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• Evolution of giant molecular clouds across cosmic time
• Anatomy of a buckling galactic bar
• Inhomogeneous Reionization Models in Cosmological Hydrodynamical Simulations
• Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
• The assembly of dusty galaxies at $z\ge 4$: the build-up of stellar mass and its scaling relations with hints from early JWST data
• Motivations for a Large Self-Interacting Dark Matter Cross Section from Milky Way Satellites
• Roll of the Dice: A Stochastically Sampled IMF Alters the Stellar Content of Simulated Dwarf Galaxies
• Hot phase generation by supernovae: resolution, chemistry and thermal conduction
• Kinematic decomposition of IllustrisTNG disk galaxies: morphology and relation with morphological structures
• Disk settling and dynamical heating: histories of Milky Way-mass stellar disks across cosmic time in the FIRE simulations
• The Galactic Dust-Up: Modeling Dust Evolution in FIRE
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• Cosmological baryon transfer in the SIMBA simulations
• Impact of relativistic jets on the star formation rate: a turbulence-regulated framework
• Characterizing the local relation between star formation rate and gas-phase metallicity in MaNGA spiral galaxies
• Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
• The little things matter: relating the abundance of ultrafaint satellites to the hosts' assembly history
• Momentum feedback from marginally-resolved HII regions in isolated disc galaxies
• SIRIUS project. I. Star formation models for star-by-star simulations of star clusters and galaxy formation
• Dissipative Dark Matter on FIRE: I. Structural and kinematic properties of dwarf galaxies
• The MOSDEF Survey: A Comprehensive Analysis of the Rest-optical Emission-line Properties of $z\sim 2.3$ Star-forming Galaxies
• The effects of subgrid models on the properties of giant molecular clouds in galaxy formation simulations
• How runaway stars boost galactic outflows
• A needle in a haystack? Catching Pop III stars in the Epoch of Reionization: I. Pop III star forming environments
• A tale of two sites -- II: Inferring the properties of minihalo-hosted galaxies with upcoming 21-cm interferometers
• TangoSIDM: Tantalizing models of Self-Interacting Dark Matter
• What drives the evolution of gas kinematics in star-forming galaxies?
• The Galaxy Progenitors of Stellar Streams around Milky Way-mass Galaxies in the FIRE Cosmological Simulations
• The minimum metallicity of globular clusters and its physical origin -- implications for the galaxy mass-metallicity relation and observations of proto-globular clusters at high redshift
• INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars
• Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations
• A diversity of starburst-triggering mechanisms in interacting galaxies and their signatures in CO emission
• Efficacy of early stellar feedback in low gas surface density environments
• New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
• Milky Way total Mass derived by Rotation Curve and Globular Cluster kinematics from Gaia EDR3
• How fast do young star clusters expel their natal gas?: Estimating the upper limit of the gas expulsion time-scale
• Numerical Problems in Coupling Photon Momentum (Radiation Pressure) to Gas
• Illustrating galaxy-halo connection in the DESI era with IllustrisTNG
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• A Predicted Correlation Between Age Gradient and Star Formation History in FIRE Dwarf Galaxies
• Great Balls of FIRE I: The formation of star clusters across cosmic time in a Milky Way-mass galaxy
• An uncertainty principle for star formation -- III. The characteristic emission time-scales of star formation rate tracers
• NIHAO -- XXV. Convergence in the cusp-core transformation of cold dark matter haloes at high star formation thresholds
• Warm FIRE: Simulating Galaxy Formation with Resonant Sterile Neutrino Dark Matter
• The challenge of simulating the star cluster population of dwarf galaxies with resolved interstellar medium
• Cosmic-Ray Transport in Simulations of Star-forming Galactic Disks
• Streams on FIRE: Populations of Detectable Stellar Streams in the Milky Way and FIRE
• Introducing galactic structure finder: the multiple stellar kinematic structures of a simulated Milky Way mass galaxy
• The first Super Massive Black Holes: indications from models for future observations
• The sensitivity of stellar feedback to IMF averaging versus IMF sampling in galaxy formation simulations
• Aemulus $\nu$: Precise Predictions for Matter and Biased Tracer Power Spectra in the Presence of Neutrinos
• A Simple Non-equilibrium Feedback Model for Galaxy-Scale Star Formation: Delayed Feedback and SFR Scatter
• Correlations Between Black Holes and Host Galaxies in the Illustris and IllustrisTNG Simulations
• Measuring dynamical masses from gas kinematics in simulated high-redshift galaxies
• Local positive feedback in the overall negative: the impact of quasar winds on star formation in the FIRE cosmological simulations
• Stellar feedback in M83 as observed with MUSE -- II. Analysis of the HII region population: ionisation budget and pre-SN feedback
• The Dark Matter Distributions in Low-Mass Disk Galaxies. II. The Inner Density Profiles
• The diversity of rotation curves of simulated galaxies with cusps and cores
• H$\alpha$ Morphologies of Star Clusters in 16 LEGUS Galaxies: Constraints on HII region evolution timescales
• The [CII]--SFR correlation in dwarf galaxies across cosmic time
• A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
• Chasing Accreted Structures within Gaia DR2 using Deep Learning
• A physical approach to modelling large-scale galactic magnetic fields
• The origin of metal-poor stars on prograde disk orbits in FIRE simulations of Milky Way-mass galaxies
• NIHAO XVI: The properties and evolution of kinematically selected discs, bulges and stellar haloes
• Neutral CGM as damped Lyα absorbers at high redshift
• Bursting Bubbles: Feedback from Clustered SNe and the Trade-off Between Turbulence and Outflows
• Galaxies Probing Galaxies in PRIMUS - II. The Coherence Scale of the Cool Circumgalactic Medium
• Ring Galaxies in the EAGLE Hydrodynamical Simulations
• Action-based distribution function modelling for constraining the shape of the Galactic dark matter halo
• The LOFAR Two-metre Sky Survey: the radio view of the cosmic star formation history
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• Code Comparison in Galaxy Scale Simulations with Resolved Supernova Feedback: Lagrangian vs. Eulerian Methods
• Satellites of Milky Way- and M31-like galaxies with TNG50: quenched fractions, gas content, and star formation histories
• Active galactic nucleus jet feedback in hydrostatic halos
• The connection between galactic outflows and the escape of ionizing photons
• Great Balls of FIRE II: The evolution and destruction of star clusters across cosmic time in a Milky Way-mass galaxy
• Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at $z\sim 3$
• Spatial Decorrelation of Young Stars and Dense Gas as a Probe of the Star Formation-Feedback Cycle in Galaxies
• RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars
• Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
• The impact of magnetic fields on cosmological galaxy mergers. I: Reshaping gas and stellar discs
• Connecting the structure of dark matter haloes to the primordial power spectrum
• From giant clumps to clouds -- II. The emergence of thick disc kinematics from the conditions of star formation in high redshift gas rich galaxies
• On the stability of tidal streams in action space
• Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
• The impact of early massive mergers on the chemical evolution of Milky Way-like galaxies: insights from NIHAO-UHD simulations
• HALO7D II: The Halo Velocity Ellipsoid and Velocity Anisotropy with Distant Main Sequence Stars
• The impact of cosmic rays on dynamical balance and disk-halo interaction in Lstar disk galaxies
• Magnetic Fields on FIRE: Comparing B-fields in the multiphase ISM and CGM of Simulated L${}_{\ast }$ Galaxies to Observations
• Formation of Galactic Disks I: Why Did the Milky Way's Disk Form Unusually Early?
• An analytic model for OIII fine structure emission from high redshift galaxies
• $5\sigma$ tension between Planck cosmic microwave background and eBOSS Lyman-alpha forest and constraints on physics beyond $\Lambda$CDM
• Stars made in outflows may populate the stellar halo of the Milky Way
• The global structure of magnetic fields and gas in simulated Milky Way-analogue galaxies
• 3D Radiation hydrodynamics of a dynamical torus
• Defining the (Black Hole)-Spheroid Connection with the Discovery of Morphology-Dependent Substructure in the $M_{\mathrm{BH}}$--${\mathrm{n}}_{\mathrm{sph}}$ and $M_{\mathrm{BH}}$--${\mathrm{R}}_{\mathrm{e},\mathrm{sph}}$ Diagrams: New Tests for Advanced Theories and Realistic Simulations
• Dwarf Galaxy Mass Estimators vs. Cosmological Simulations
• Chemical Evolution with Radial Mixing Redux: Extending beyond the Solar Neighborhood
• Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales
• The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
• WARPFIELD Population Synthesis: The physics of (extra-)Galactic star formation and feedback driven cloud structure and emission from sub-to-kpc scales
• An observational test for star formation prescriptions in cosmological hydrodynamical simulations
• Rapid Filamentary Accretion as the Origin of Extended Thin Discs
• An almost dark galaxy with the mass of the Small Magellanic Cloud
• Effects of initial density profiles on massive star cluster formation in giant molecular clouds
• Thermal Instability in the CGM of $L_{\star }$ Galaxies: Testing "Precipitation" Models with the FIRE Simulations
• Finding binary black holes in the Milky Way with LISA
• IQ Collaboratory II: The Quiescent Fraction of Isolated, Low Mass Galaxies Across Simulations and Observations
• Spatially Resolved Stellar Spectroscopy of the Ultra-diffuse Galaxy Dragonfly 44. III. Evidence for an Unexpected Star-Formation History
• SMBH Seeds from Dissipative Dark Matter
• Resolution Requirements and Resolution Problems in Simulations of Radiative Feedback in Dusty Gas
• Direct Detection of Mirror Matter in Twin Higgs Models
• The Pandora project. I: the impact of radiation and cosmic rays on baryonic and dark matter properties of dwarf galaxies
• Formation of star clusters and enrichment by massive stars in simulations of low-metallicity galaxies with a fully sampled initial stellar mass function
• The connection between the escape of ionizing radiation and galaxy properties at z~3 in the Keck Lyman Continuum Spectroscopic Survey
• Barred spiral galaxies in modified gravity theories
• Amplified J-factors in the Galactic Center for velocity-dependent darkmatter annihilation in FIRE simulations
• Is it possible to reconcile extragalactic IMF variations with a universal Milky Way IMF?
• Revisiting dynamical friction: the role of global modes and local wakes
• The effects of LMC-mass environments on their dwarf satellite galaxies in the FIRE simulations
• Uncertainties in supernova input rates drive qualitative differences in simulations of galaxy evolution
• The impact of AGN-driven winds on physical and observable galaxy sizes
• Origin of highly $r$-process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy
• Figuring Out Gas & Galaxies In Enzo (FOGGIE) VI: The Circumgalactic Medium of $L^{\ast }$ Galaxies is Supported in an Emergent, Non-Hydrostatic Equilibrium
• The Elephant in the Room: The Importance of Where and When Massive Stars Form in Molecular Clouds
• A Parametric Model for Self-Interacting Dark Matter Halos
• High-resolution, 3D radiative transfer modelling. II. The early-type spiral galaxy M81
• Mixing matters
• Balmer Break Galaxy Candidates at $z\sim 6$: a Potential View on the Star-Formation Activity at $z\gtrsim 14$
• PDFchem: A new fast method to determine ISM properties and infer environmental parameters using probability distributions
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• Virial shocks are suppressed in cosmic ray-dominated galaxy halos
• VINTERGATAN IV: Cosmic phases of star formation in Milky Way-like galaxies
• Stellar feedback strongly alters the amplification and morphology of galactic magnetic fields
• Towards a consistent framework of comparing galaxy mergers in observations and simulations
• Exploring metallicity-dependent rates of Type Ia supernovae and their impact on galaxy formation
• Linking globular cluster formation at low and high redshift through the age-metallicity relation in E-MOSAICS
• Dust temperature uncertainties hamper the inference of dust and molecular gas masses from the dust continuum emission of quiescent high-redshift galaxies
• [CII] halos in ALPINE galaxies: smoking-gun of galactic outflows?
• The WAGGS project - II. The reliability of the calcium triplet as a metallicity indicator in integrated stellar light
• Violent starbursts and quiescence induced by FUV radiation feedback in metal-poor galaxies at high-redshift
• ELVES III: Environmental Quenching by Milky Way-Mass Hosts
• Reading the CARDs: the Imprint of Accretion History in the Chemical Abundances of the Milky Way's Stellar Halo
• GLASS: Generator for Large Scale Structure
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• Substructure at High Speed II: The Local Escape Velocity and Milky Way Mass with Gaia DR2
• Shapes of Milky-Way-Mass Galaxies with Self-Interacting Dark Matter
• The Origin of the Dust Extinction Curve in Milky Way-like Galaxies
• Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA
• Orbital dynamics and histories of satellite galaxies around Milky Way-mass galaxies in the FIRE simulations
• Relating the Diverse Merger Histories and Satellite Populations of Nearby Galaxies
• The effect of warm gas on the buckling instability in galactic bars
• The 3D structure of CO depletion in high-mass prestellar regions
• Photoionising feedback in spiral arm molecular clouds
• The Life Cycle of the Central Molecular Zone. II: Distribution of atomic and molecular gas tracers
• EAGLE-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies
• The observable properties of galaxy accretion events in Milky Way-like galaxies in the FIRE-2 cosmological simulations
• The Einasto model for dark matter haloes
• Cataloging Accreted Stars within Gaia DR2 using Deep Learning
• Empirically-motivated early feedback: momentum input by stellar feedback in galaxy simulations inferred through observations
• Constraining Compact Object Formation with 2M0521
• A Search for Dark Matter Lines at the Galactic Center with 14 Years of Fermi Data
• Spiral Arms are Metal Freeways: Azimuthal Gas-Phase Metallicity Variations in Simulated Cosmological Zoom-in Flocculent Disks
• Prospects for distinguishing galaxy evolution models with surveys at redshifts $z\gtrsim 4$
• On the Interpretation of Far-infrared Spectral Energy Distributions. I: The 850 $\mu$m Molecular Mass Estimator
• The Dawn of Disk Formation in a Milky Way-sized Galaxy Halo: Thin Stellar Disks at $z>4$
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• Galaxy inclination and the IRX-beta relation: Effects on UV star-formation rate measurements at intermediate to high redshifts
• A Dusty Locale: Evolution of Galactic Dust Populations from Milky Way to Dwarf-Mass Galaxies
• A Framework for Modeling Polycyclic Aromatic Hydrocarbon Emission in Galaxy Evolution Simulations
• A New Discrete Dynamical Friction Estimator Based on $N$-body Simulations
• The relationship between age, metallicity, and abundances for disk stars in a simulated Milky Way galaxy
• The galaxy-halo size relation of low-mass galaxies in FIRE
• Testing the Relationship Between Bursty Star Formation and Size Fluctuations of Local Dwarf Galaxies
• MACER improved: AGN feedback computed in rotating early-type galaxies at high resolution
• Comparing Models for IMF Variation Across Cosmological Time in Milky Way-like Galaxies
• Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
• Quenching in Cosmic Sheets: Tracing the Impact of Large Scale Structure Collapse on the Evolution of Dwarf Galaxies
• Comparison of cosmological simulations and deep submillimetre galaxy surveys
• Hyper-Eddington Black Hole Growth in Star-Forming Molecular Clouds and Galactic Nuclei: Can It Happen?
• Detection of thermal Sunyaev-Zel'dovich Effect in the circumgalactic medium of low-mass galaxies -- a surprising pattern in self-similarity and baryon sufficiency
• The interplay between feedback, accretion, transport and winds in setting gas-phase metal distribution in galaxies
• Predicting sub-millimeter flux densities from global galaxy properties
• Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers
• The observability of galaxy merger signatures in nearby gas-rich spirals
• Impact of galactic distributions in celestial capture of dark matter
• Stellar feedback in M83 as observed with MUSE -- I. Overview, an unprecedented view of the stellar and gas kinematics and evidence of outflowing gas
• Simulating cosmological substructure in the solar neighbourhood
• LIMFAST. I. A Semi-Numerical Tool for Line Intensity Mapping
• The effect of the environment-dependent stellar initial mass function on the photometric properties of star-forming galaxies
• Astrophysical Tests of Dark Matter Self-Interactions
• Entering the Era of Dark Matter Astronomy? Near to Long-Term Forecasts in X-Ray and Gamma-Ray Bands
• Dark Matter Candidates and Searches
• The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
• Reproducing the CO-to-H${}_2$ conversion factor in cosmological simulations of Milky Way-mass galaxies
• Balmer breaks in simulated galaxies at z>6
• Ultra-Diffuse Galaxies as Extreme Star-forming Environments I: Mapping Star Formation in HI-Rich UDGs
• New Analytic Solutions for Galaxy Evolution II: Wind Recycling, Galactic Fountains and Late-Type Galaxies
• The In-situ Origins of Dwarf Stellar Outskirts in FIRE-2
• From Peculiar Morphologies to Hubble-type Spirals: The relation between galaxy dynamics and morphology in star-forming galaxies at z~1.5
• High-redshift Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes: Stellar Feedback and Quasar Growth
• Applying the metallicity-dependent binary fraction to double white dwarf formation: Implications for LISA
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• Ultraviolet Signatures of the Multiphase Intracluster and Circumgalactic Media in the RomulusC Simulation
• EDGE: The emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• The cusp-core problem in gas-poor dwarf spheroidal galaxies
• A jolt to the system: ram pressure on low-mass galaxies in simulations of the Local Group
• The mass-metallicity relation as a ruler for galaxy evolution: insights from the James Webb Space Telescope
• The AGORA High-resolution Galaxy Simulations Comparison Project. V: Satellite Galaxy Populations In A Cosmological Zoom-in Simulation of A Milky Way-mass Halo
• The OSIRIS Lens-Amplified Survey (OLAS) I: Dynamical Effects of Stellar Feedback in Low Mass Galaxies at z ~ 2
• Realistic HI scale heights of Milky Way-mass galaxies in the FIREbox cosmological volume
• Hydrodynamical structure formation in Milgromian cosmology
• Numerical Challenges in Modeling Gravothermal Collapse in Self-Interacting Dark Matter Halos
• The dark side of FIRE: predicting the population of dark matter subhaloes around Milky Way-mass galaxies
• Higgsino Dark Matter Confronts 14 years of Fermi Gamma Ray Data
• Effects of Varying Mass Inflows on Star Formation in Nuclear Rings of Barred Galaxies
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
• Toward the ultimate reach of current imaging atmospheric Cherenkov telescopes and their sensitivity to TeV dark matter
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• Early galaxy growth: mergers or gravitational instability?
• A Stable Finite-Volume Method for Scalar-Field Dark Matter
• Synchrotron Emission on FIRE: Equipartition Estimators of Magnetic Fields in Simulated Galaxies with Spectrally-Resolved Cosmic Rays
• The AGORA High-resolution Galaxy Simulations Comparison Project. VI. Similarities and Differences in the Circumgalactic Medium
• H2 chemistry in galaxy simulations: an improved supernova feedback model
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• The IllustrisTNG Simulations: Public Data Release
• SIEGE III: The formation of dense stellar clusters in sub-parsec resolution cosmological simulations with individual star feedback
• Energy balance SED modelling can be effective at high redshifts regardless of UV-FIR offsets
• Local photoionization feedback effects on galaxies
• Stellar winds and photoionization in a spiral arm
• A Lower Limit on the Mass of Our Galaxy from the H3 Survey
• Molecular gas and star formation in nearby starburst galaxy mergers
• The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
• Galaxy merger challenge: A comparison study between machine learning-based detection methods
• Ultra-Diffuse Galaxies as Extreme Star-forming Environments II: Star Formation and Pressure Balance in HI-Rich UDGs
• Cosmic Reionization On Computers: The Galaxy-Halo Connection between $5\le z\le 10$
• Clumpy galaxies in cosmological simulations: The effect of ISM model
• The MOSDEF-LRIS Survey: Connection between Galactic-scale Outflows and the Properties of $z$~2 star-forming Galaxies
• Bursting Bubbles: Clustered Supernova Feedback in Local and High-redshift Galaxies
• MaNGA galaxy properties -- II. A detailed comparison of observed and simulated spiral galaxy scaling relations
• The Obsidian model: Three regimes of black hole feedback
• The Borg Cube Simulation: Cosmological Hydrodynamics with CRK-SPH
• The Role of AGN in Luminous Infrared Galaxies from the Multiwavelength Perspective
• Probing the CGM of Low-redshift Dwarf Galaxies Using FIRE Simulations
• Variations in the slope of the resolved star-forming main sequence: a tool for constraining the mass of star-forming regions
• Dust diffusion in SPH simulations of an isolated galaxy
• From Seeds to Supermassive Black Holes: Capture, Growth, Migration, and Pairing in Dense Proto-Bulge Environments
• Filamentary structures of ionized gas in Cygnus X
• The Origin and Evolution of Lyman-alpha Blobs in Cosmological Galaxy Formation Simulations
• Momentum Injection by Clustered Supernovae: Testing Subgrid Feedback Prescriptions
• ART${}^2$: 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
• A New Public Release of the GIZMO Code
• A general-purpose timestep criterion for simulations with gravity
• Lyman-$\alpha$ feedback prevails at Cosmic Dawn: Implications for the first galaxies, stars, and star clusters
• Galactic Chemical Evolution Models Favor an Extended Type Ia Supernova Delay-Time Distribution
• Galactic coronae in Milky Way-like galaxies: the role of stellar feedback in gas accretion
• The role of gas kinematics in setting metallicity gradients at high redshift
• The galaxy - halo connection in low mass halos
• Simulating ionization feedback from young massive stars: impact of numerical resolution
• Where infall meets outflows: turbulent dissipation probed by CH${}^{+}$ and Ly$\alpha$ in the starburst/AGN galaxy group SMM J02399$-$0136 at z$\sim$2.8
• JWST MIRI and NIRCam observations of NGC 891 and its circumgalactic medium
• Imaging Spectroscopy of Ionized Gaseous Nebulae around Optically Faint AGN at Redshift z ~ 2
• The Implications of Local Fluctuations in the Galactic Midplane for Dynamical Analysis in the Gaia Era
• The Duration of Star Formation in Galactic Giant Molecular Clouds. I. The Great Nebula in Carina
• Simplified galaxy formation with mesh-less hydrodynamics
• Testing Feedback from Star Clusters in Simulations of the Milky Way Formation
• Formation of proto-globular cluster candidates in cosmological simulations of dwarf galaxies at $z>4$
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• Magnetic fields in elliptical galaxies: Using the Laing-Garrington effect in radio galaxies and polarized emission from background radio sources
• The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• Spatially resolved mock observations of stellar kinematics: full radiative transfer treatment of simulated galaxies
• How Metals Are Transported In And Out Of A Galactic Disk: Dependence On The Hydrodynamic Schemes In Numerical Simulations
• A shallow dark matter halo in Ultra Diffuse Galaxy AGC 242019: are UDGs structurally similar to low surface brightness galaxies?
• The Manhattan Suite: Accelerated galaxy evolution in the early Universe
• Modeling of Spiral Structure in a Multi-Component Milky~Way-Like Galaxy
• Properties of the Magellanic Corona
• On the likelihoods of finding very metal-poor (and old) stars in the Milky Way's disc, bulge, and halo
• Galactic Mass Estimates using Dwarf Galaxies as Kinematic Tracers
• The fate of the interstellar medium in early-type galaxies. III. The mechanism of ISM removal and quenching of star formation
• The role of physical and numerical viscosity in hydrodynamical instabilities
• Self-regulation of black hole accretion via jets in early protogalaxies
• Probing Hot Gas Components of Circumgalactic Medium in Cosmological Simulations with the Thermal Sunyaev-Zel'dovich Effect
• The contribution of globular clusters to cosmic reionization
• Using Action Space Clustering to Constrain the Accretion History of Milky Way like Galaxies
• Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM
• Determining the Timescale over Which Stellar Feedback Drives Turbulence in the ISM: A Study of four Nearby Dwarf Irregular Galaxies
• Local and global gas metallicity versus stellar age relation in MaNGA galaxies
• Simulating Globular Clusters in Dark Matter Sub-Halos
• The THESAN-ZOOM project: Population III star formation continues until the end of reionization
• Spatially Resolved Gas-phase Metallicity in FIRE-2 Dwarfs: Late-Time Evolution of Metallicity Relations in Simulations with Feedback and Mergers
• Simulating Hydrodynamics in Cosmology with CRK-HACC
• Active galactic nuclei jets simulated with smoothed particle hydrodynamics
• Fiery Cores: Bursty and Smooth Star Formation Distributions across Galaxy Centers in Cosmological Zoom-in Simulations
• Dwarf galaxy formation with and without dark matter-baryon streaming velocities
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• On the distribution of the Cold Neutral Medium in galaxy discs
• Clouds accreting from the IGM are not able to feed the star formation of low-redshift disc galaxies
• Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation
• Impact of H${}_2$-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
• A Dusty Dawn: Galactic Dust Buildup at $z\gtrsim 5$
• Accurate mass estimates from the proper motions of dispersion-supported galaxies
• Robust Clustering of the Local Milky Way Stellar Kinematic Substructures with Gaia eDR3
• Progenitor-mass-dependent yields amplify intrinsic scatter in dwarf-galaxy elemental abundance ratios
• Galactic satellite systems in CDM, WDM and SIDM
• Cuspy dark matter density profiles in massive dwarf galaxies
• A Semi-Analytical Line Transfer (SALT) Model III: Galactic Inflows
• The ALPINE-ALMA [CII] Survey: Dust emission effective radius up to 3 kpc in the Early Universe
• Novel Conservative Methods for Adaptive Force Softening in Collisionless and Multi-Species N-Body Simulations
• Shaping the Milky Way: The interplay of mergers and cosmic filaments
• SIEGE IV: compact star clusters in cosmological simulations with high star formation efficiency and sub-parsec resolution
• Inconsistencies arising from the coupling of galaxy formation sub-grid models to Pressure-Smoothed Particle Hydrodynamics
• Efficient and accurate force replay in cosmological-baryonic simulations
• The possible hierarchical scales of observed clumps in high-redshift disc galaxies
• Metallicity profiles of Ultra Diffuse Galaxies in NIHAO simulations
• Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants
• HI within and around observed and simulated galaxy discs -- Comparing MeerKAT observations with mock data from TNG50 and FIRE-2
• The Dark Matter Tidal Stripping History of the Sagittarius Core with N-body simulations
• Running Late: Testing Delayed Supermassive Black Hole Growth Models Against the Quasar Luminosity Function
• Comparing Implementations of Self-Interacting Dark Matter in the Gizmo and Arepo Codes
• Critical Metallicity of Cool Supergiant Formation. I. Effects on Stellar Mass Loss and Feedback
• Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies
• Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
• LMC-driven anisotropic boosts in stream--subhalo interactions
• Testing the Breathing Mode in Intermediate Mass Galaxies and its Predicted Star Formation Rate-Size Anti-Correlation
• The AGORA High-Resolution Galaxy Simulations Comparison Project VII: Satellite quenching in zoom-in simulation of a Milky Way-mass halo
• Census of Gaseous Satellites around Local Spiral Galaxies
• Constraints on Fluctuating Star Formation Rates for Intermediate-mass Galaxies with H$\alpha$ and UV Luminosities
• Great Balls of FIRE III: Modeling Black Hole Mergers from Massive Star Clusters in Simulations of Galaxies
• Bursty Star Formation in Dwarfs is Sensitive to Numerical Choices in Supernova Feedback Models
• Milky Way-like galaxies: stellar population properties of dynamically defined disks, bulges and stellar halos
• Abundance matching for low mass galaxies in the CDM and FDM models
• Colour-magnitude diagram in simulations of galaxy formation
• Rapid Growth of Galactic Supermassive Black Holes through Accreting Giant Molecular Clouds during Major Mergers of their Host Galaxies
• Orbital pericenters and the inferred dark matter halo structure of satellite galaxies
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• Observing the stellar halo of Andromeda in cosmological simulations: the Auriga2PAndAS pipeline
• An Empirical Determination of the Dependence of the Circumgalactic Mass Cooling Rate and Feedback Mass Loading Factor on Galactic Stellar Mass
• Spatially-resolved Spectroscopic Analysis of Ly$\alpha$ Haloes: Radial Evolution of the Ly$\alpha$ Line Profile out to 60 kpc
• Investigating the ultraviolet and infrared radiation through the turbulent life of molecular clouds
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• A quantitative demonstration that stellar feedback locally regulates galaxy growth
• Sliding into DM: Determining the local dark matter density and speed distribution using only the local circular speed of the Galaxy
• Searching for HI around MHONGOOSE Galaxies via Spectral Stacking
• Constraints on galactic outflows from the metallicity-stellar mass-SFR relation of EAGLE simulation and SDSS galaxies
• Cold Exponential Disks From Interstellar Fountains
• On the Origin of High-velocity Clouds in the Galaxy
• X-ray Line Diagnostics of Ion Temperature at Cosmic-Ray Accelerating Collisionless Shocks
• Firefly: a browser-based interactive 3D data visualization tool for millions of data points
• High-Resolution Chemical Abundances of the Nyx Stream
• Implications of multi-axion dark matter on structure formation
• Cloud-cloud collisions triggering star formation in galaxy simulations
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• Feedback-regulated Seed Black Hole Growth in Star-Forming Molecular Clouds and Galactic Nuclei
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• Explaining the Weak Evolution of the High-Redshift Mass-Metallicity Relation with Galaxy Burst Cycles
• Playing with FIRE: A Galactic Feedback-Halting Experiment Challenges Star Formation Rate Theories
• Resolved star formation in TNG100 central and satellite galaxies
• Stability of galaxies across morphological sequence
• Emergence of Galactic Morphologies at Cosmic Dawn: Input from Numerical Modeling
• Star Formation in Splash Bridges
• Implementing Dust Shielding as a Criteria for Star Formation
• Diverse dark matter profiles in FIRE dwarfs: black holes, cosmic rays and the cusp-core enigma
• Redshift dependence of FRB host dispersion measures across cosmic epochs
• The physical origin of positive metallicity radial gradients in high-redshift galaxies: insights from the FIRE-2 cosmological hydrodynamic simulations
• Seeking Self-Regulating Simulations of Idealized Milky Way-Like Galaxies
• On the limitations of H alpha luminosity as a star formation tracer in spatially resolved observations
• Gusts in the Headwind: Uncertainties in Direct Dark Matter Detection
• Chromium Nucleosynthesis and Silicon-Carbon Shell Mergers in Massive Stars
• Escaping the maze: a statistical sub-grid model for cloud-scale density structures in the interstellar medium
• Inverse Compton cooling of thermal plasma in colliding-wind binaries
• Exploring the ex-situ components within Gaia DR3
• Modelling H${}_2$ and its effects on star formation using a joint implementation of GADGET-3 and KROME
• Predictions for Complex Distributions of Stellar Elemental Abundances in Low-Mass Galaxies
• Pre-supernova stellar feedback in nearby starburst dwarf galaxies
• Lux ex tenebris: The imprint of annihilating dark matter on the intergalactic medium during Cosmic Dawn
• Baryonic Post-Processing of N-body Simulations, with Application to Fast Radio Bursts
• Recovering Injected Astrophysics from the LISA Galactic Double White Dwarf Binaries
• Where Did the Outskirts Go? Outer Stellar Haloes as a Sensitive Probe of Supernova Feedback
• EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
• Non-explosive pre-supernova feedback in the COLIBRE model of galaxy formation
• A Novel Scheme for Dark Matter Annihilation Feedback in Cosmological Simulations
• Understanding the Baryon Cycle: Fueling Star Formation via Inflows in Milky Way-like Galaxies
• Dipolar dark matter simulations on galaxy scales with the RAMSES code
• ZTF SN Ia DR2: Properties of the low-mass host galaxies of Type Ia supernovae in a volume-limited sample
• The relationship between cluster environment and molecular gas content of star-forming galaxies in the EAGLE simulation
• The recent star formation history of NGC 628 on resolved scales
• HALO7D III: Chemical Abundances of Milky Way Halo Stars from Medium Resolution Spectra
• GalaxyFlow: Upsampling Hydrodynamical Simulations for Realistic Mock Stellar Catalogs
• Dark Matter-Induced Baryonic Feedback in Galaxies
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• Numerical Discreteness Errors in Multi-Species Cosmological N-body Simulations
• A Simple Sub-Grid Model For Cosmic Ray Effects on Galactic Scales
• CEERS: Forging the First Dust Grains in the Universe? A Population of Galaxies with spectroscopically-derived Extremely Low Dust Attenuation (GELDA) at 4.0<z<11.4
• The Shape of FIREbox Galaxies and a Potential Tension with Low-mass Disks
• Determining the time before or after a galaxy merger event
• A MARVEL-ous study of how well galaxy shapes reflect Dark Matter halo shapes in Cold Dark Matter Simulations
• The life cycle of giant molecular clouds in simulated Milky Way-mass galaxies
• Trial by FIRE: Probing the dark matter density profile of dwarf galaxies with GraphNPE
• TeV gamma-ray sensitivity to velocity-dependent dark matter models in the Galactic Center
• Substructure at High Speed I: Inferring the Escape Velocity in the Presence of Kinematic Substructure
• Substructure in the Globular Cluster Populations of the Virgo Cluster Elliptical Galaxies M84 and M86
• Testing $\Lambda$CDM With Dwarf Galaxy Morphology
• Astrophysics with the Laser Interferometer Space Antenna
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• A Simulation Based Inference Approach to the Dynamics of the MW-LMC System -- Validation
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• No need for dark matter: resolved kinematics of the ultra-diffuse galaxy AGC 114905
• Wavelet-Harmonic Integration Methods
• SWIFT: Maintaining weak-scalability with a dynamic range of $10^4$ in time-step size to harness extreme adaptivity
• Sensitivity Estimation for Dark Matter Subhalos in Synthetic Gaia DR2 using Deep Learning
• NIHAO-RiNG: A Comparison of Simulated Disc Galaxies from GASOLINE and GIZMO
• Intertwined Formation of ${\mathrm{H}}_2$, Dust, and Stars in Cosmological Simulations
• Partial Rate Matrix for Dark Matter Scattering
• Central densities of dark matter halos in FIRE-2 simulations of low-mass galaxies with cold dark matter and self-interacting dark matter
• Internal r-process abundance spread of M15 and a single stellar population model
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
• The imprint of dark matter on the Galactic acceleration field
• The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data
• On the Metallicities and Kinematics of the Circumgalactic Media of Damped Ly$\alpha$ Systems at $z\sim 2.5$
• An Improved and Physically-Motivated Scheme for Matching Galaxies with Dark Matter Halos
• Testing the Momentum-driven Supernova Feedback Paradigm in M31
• Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
• The AGORA High-resolution Galaxy Simulations Comparison Project. VIII: Disk Formation and Evolution of Simulated Milky Way Mass Galaxy Progenitors at $1<z<5$
• Warm dark matter model with a few keV mass is bad for the too-big-to-fail problem
• The Impact of Classical Bulges on Stellar Bars and Box-Peanut-X-Features in Disk Galaxies
• Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
• Improving Performance of Zoom-In Cosmological Simulations using Initial Conditions with Customized Grids
• Weighing the Darkness II: Astrometric Measurement of Partial Orbits with Gaia
• Can radial motions in the stellar halo constrain the rate of change of mass in the Galaxy?
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Searching for Conformity Across Cosmic Time with Local Group and Local Volume Star Formation Histories
• A Rich Satellite Population of the NGC 4437 Group and Implications of a Magnitude Gap for Galaxy Group Assembly History
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• Cosmological Zoom-In Simulations of Milky Way Host Mass Dark Matter Halos with a Blue-Tilted Primordial 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
• Constraining gas metal mixing strength in simulations using observations of the Milky Way's disc
• Orbital phase-driven biases in Galactic mass constraints from stellar streams
• A general relativistic extension to mesh-free methods for hydrodynamics
• Refracting into Ultra Diffuse Galaxy NGC 1052-DF2 by Passing near the Center of NGC 1052
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• Machine-guided Exploration and Calibration of Astrophysical Simulations
• Devouring The Centaurus A Satellites: Modeling Dwarf Galaxies with Galacticus
• IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L${}^{\star }$ Galaxies
• Impact of radiation feedback on the assembly of star clusters in galactic context
• The imprint of bursty star formation on alpha-element abundance patterns in Milky Way-like galaxies
• Galaxy mass profiles with convolutional neural networks
• Auriga Streams II: orbital properties of tidally disrupting satellites of Milky Way-mass galaxies
• Self-generated ultraviolet radiation in molecular shock waves I. Effects of Lyman $\alpha$, Lyman $\beta$, and two-photon continuum
• Formation of Substructure in Luminous Submillimeter Galaxies (FOSSILS): Evidence of Multiple Pathways to Trigger Starbursts in Luminous Submillimeter Galaxies
• Feedback from intermediate mass black holes on dwarf galaxy morphology at z=2
• Performance Enhancement of Tree-based Friends-of-friend Galaxy-finder for High-resolution Simulations of Galaxy Formation
• The Color Gradients of the Globular Cluster Systems in M87 and M49
• The imprint of dark subhaloes on the circumgalactic medium
• MEGS: Morphological Evaluation of Galactic Structure
• A graph model for the clustering of dark matter halos
• A path towards constraining the evolution of the interstellar medium and outflows in the Milky Way using APOGEE
• Auriga Superstars: Improving the resolution and fidelity of stellar dynamics in cosmological galaxy simulations
• A general relativistic magnetohydrodynamics extension to mesh-less schemes in the code GIZMO
• An Observationally Driven Multifield Approach for Probing the Circum-Galactic Medium with Convolutional Neural Networks
• New insights on low-mass dark matter subhalo tidal tracks via numerical simulations
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• Dissecting stellar populations with manifold learning I. Validation of the method on a synthetic Milky Way-like galaxy
• The MOSDEF Survey: A New View of a Remarkable z=1.89 Merger
• The First Star-by-star $N$-body/Hydrodynamics Simulation of Our Galaxy Coupling with a Surrogate Model
• Constraints on dark matter models from the stellar cores observed in ultra-faint dwarf galaxies: Self-interacting dark matter
• The Arp 240 Galaxy Merger: A Detailed Look at the Molecular Kennicutt-Schmidt Star Formation Law on Sub-kpc Scales
• Wind of Change: Faraday Rotation in a Simulated Large Magellanic Cloud
• New families in our Solar neighborhood: applying Gaussian Mixture models for objective classification of structures in the Milky Way and in simulations
• Constraining cosmic ray transport models using circumgalactic medium properties and observables
• Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos
• Rise of the forsaken relics: connecting present-day stellar streams and phase-mixed galaxies to the Epoch of Reionization
• A test of invariance of halo surface density for FIRE-2 simulations with cold dark matter and self-interacting dark matter
• How Many Bursts Does it Take to Form a Core at the Center of a Galaxy?
• The Formation of Dwarf Galaxy Disks
• Gravitational wave energy spectral density properties from BPASS Galactic binary population in the Milky Way galaxy
• Hot accretion onto spiral galaxies: the origin of extended and warped HI discs
• Effects of Varied Cosmic Ray Feedback from AGN on Massive Galaxy Properties
• ARCHITECTS I: Impact of subgrid physics on the simulated properties of the circumgalactic medium
• The In Situ Growth of Stellar-mass "Light" Seed Black Holes in Nuclear Star Clusters
• Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE
• Chemodynamics of BoötesI with $S^5$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints
• The chemical and spatial variations of the bulge's velocity ellipsoids
• The multi-component fitting to the star formation histories in the TNG simulation
• Effect of cosmic rays and ionizing radiation on observational ultraviolet plasma diagnostics in the circumgalactic medium
• Constraining Gamma-ray Lines from Dark Matter Annihilation using Fermi-LAT and H.E.S.S. data
• Extracting Halo Independent Information from Dark Matter Electron Scattering Data
• A New Model For Including Galactic Winds in Simulations of Galaxy Formation II: Implementation of PhEW in Cosmological Simulations
• The NewHorizon Simulation -- To Bar Or Not To Bar
• Unequal-mass mergers of dark matter haloes with rare and frequent self-interactions
• NIHAO-LG: The uniqueness of Local Group dwarf galaxies
• Numerical Methods for Simulating Star Formation
• Towards characterizing dark matter subhalo perturbations in stellar streams with graph neural networks
• On the scale-height of the molecular gas disc in Milky Way-like galaxies
• Hydromagnetic waves in an expanding universe -- cosmological MHD code tests using analytic solutions
• The Impact of Star Formation Histories on the Inner Dark Matter Density Slopes of Galaxies
• 3D elemental abundances of stars at formation across the histories of Milky Way-mass galaxies in the FIRE simulations
• Extending the SAGA Survey (xSAGA) I: Satellite Radial Profiles as a Function of Host Galaxy Properties
• Validating the CROCODILE model within the AGORA galaxy simulation framework
• How non-thermal pressure impacts the modelling of star formation in galaxy formation simulations
• The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
• On the detection of stellar wakes in the Milky Way: a deep learning approach
• An ancient system hidden in the Galactic plane?
• Analysis of shape and angular orientation parameters of velocity-dependent dark matter annihilation signals in Galactic Centers for FIRE simulations
• The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
• Quokka-based understanding of outflows (QED) -- IV. Limitations of H$\alpha$ as an outflow diagnostic
• Supernovae and photoionizing feedback in spiral arm molecular clouds
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• Modeling Cosmological Evolution of Jetted Seyfert Galaxies for z<10
• Tidal adaptive softening and artificial fragmentation in cosmological simulations
• Search for gamma-ray spectral lines from dark matter annihilation with the H.E.S.S. Inner Galaxy Survey
• The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\mathrm{X}}$--$T$ relation of early-type galaxies
• Momentum deposition of supernovae with cosmic rays
• Ergodicity of FIRE: star formation variations within and between simulated galaxies
• Determination of the best dark matter profile for the Milky Way with Gaia DR3 using Bayesian Model Comparison
• No Stream Left Unscathed: The imprint of a host galaxy
• Multi-component, axisymmetric dynamical models of dSphs based on distribution functions: inferences on dark matter and intermediate-mass black holes in Draco and Ursa Minor
• Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
• Cold vs. Hot Gas Accretion and Angular Momentum in FIRE Simulations: From Halo to Galaxy Scales
• FEASTS and MHONGOOSE: HI Column Density Distribution at $z=0$ for $N_{\mathrm{HI}}>10^{17.8}{\mathrm{cm}}^{-2}$
• A New Method to Simulate Dark Matter-Baryon Interactions and Application to an Isolated Disk Galaxy
• Controlled Experiments on Dark-Matter Halo Structure and Galaxy Morphology I: What Sets Galaxy Sizes?
• How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood
• Metallicity Structure in Galactic Longitude-Velocity Diagrams of the Milky Way Disk and FIRE-2 Simulations
• Testing subhalo abundance matching with galaxy kinematics
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• Formation of massive multiple-star systems: early migration and mergers
• The Cosmic Rush Hour: Rapid Formation of Bright, Massive, Disky, Star-Forming Galaxies as Signatures of Early-Universe Physics
• Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations
• Turning Points in the Age-Metallicity Relations -- Created by Late Satellite Infall and Enhanced by Radial Migration
• The Effects of Cosmic-Ray Diffusion and Radiative Cooling on the Galactic Wind from the Milky Way
• Hierarchical Inducing Point Gaussian Process for Inter-domain Observations
• SHARP(ening the) view of unresolved globular clusters in ultra diffuse galaxies
• Machine Learning for Galactic Archaeology: A chemistry-based neural network method for identification of accreted disc stars