Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation

Abstract

We present a series of high-resolution cosmological simulations of galaxy formation to z=0, spanning halo masses ~10^8-10^13 M_sun, and stellar masses ~10^4-10^11. Our simulations include fully explicit treatment of both the multi-phase ISM (molecular through hot) and stellar feedback. The stellar feedback inputs (energy, momentum, mass, and metal fluxes) are taken directly from stellar population models. These sources of stellar feedback, with zero adjusted parameters, reproduce the observed relation between stellar and halo mass up to M_halo~10^12 M_sun (including dwarfs, satellites, MW-mass disks, and small groups). By extension, this leads to reasonable agreement with the stellar mass function for M_star<10^11 M_sun. We predict weak redshift evolution in the M_star-M_halo relation, consistent with current constraints to z>6. We find that the M_star-M_halo relation is insensitive to numerical details, but is sensitive to the feedback physics. Simulations with only supernova feedback fail to reproduce the observed stellar masses, particularly in dwarf and high-redshift galaxies: radiative feedback (photo-heating and radiation pressure) is necessary to disrupt GMCs and enable efficient coupling of later supernovae to the gas. Star formation rates agree well with the observed Kennicutt relation at all redshifts. The galaxy-averaged Kennicutt relation is very different from the numerically imposed law for converting gas into stars in the simulation, and is instead determined by self-regulation via stellar feedback. Feedback reduces star formation rates considerably and produces a reservoir of gas that leads to rising late-time star formation histories significantly different from the halo accretion history. Feedback also produces large short-timescale variability in galactic SFRs, especially in dwarfs. Many of these properties are not captured by common 'sub-grid' galactic wind models.

23 pages, 13 figures, accepted to MNRAS. Revised to match published version. For movies of the simulations here, see http://www.tapir.caltech.edu/~phopkins/Site/Movies_cosmo.html or the FIRE project site http://fire.northwestern.edu

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• SatGen: a semi-analytical satellite galaxy generator -- I. The model and its application to Local-Group satellite statistics
• Introducing the FirstLight project: UV luminosity function and scaling relations of primeval galaxies
• Semi-analytic forecasts for JWST -- IV. Implications for cosmic reionization and LyC escape fraction
• A VLT/FORS2 view at $z\sim 6$: Lyman-$\alpha$ emitter fraction and galaxy physical properties at the edge of the epoch of cosmic reionization
• Project AMIGA: The Circumgalactic Medium of Andromeda
• Cosmic-Ray Driven Outflows to Mpc Scales from $L_{\ast }$ Galaxies
• Consequences of bursty star formation on galaxy observables at high redshifts
• Star Cluster Formation in Cosmological Simulations. II. Effects of Star Formation Efficiency and Stellar Feedback
• 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
• Expanded haloes, abundance matching and too-big-to-fail in the Local Group
• Bulge Formation via Mergers in Cosmological Simulations
• The unorthodox evolution of major merger remnants into star-forming spiral galaxies
• The Metal Abundances across Cosmic Time ($\mathcal{M}\mathcal{A}\mathcal{C}\mathcal{T}$) Survey. II. Evolution of the Mass-Metallicity Relation over 8 Billion Years, using [OIII]$\lambda$4363Å-based Metallicities
• Identifying quiescent compact objects in massive Galactic single-lined spectroscopic binaries
• Physical Processes in Star Formation
• Equilibrium Model Constraints on Baryon Cycling Across Cosmic Time
• Delayed Star Formation in Isolated Dwarf Galaxies: HST Star Formation History of the Aquarius Dwarf Irregular
• The Fates of the Circumgalactic Medium in the FIRE Simulations
• Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
• VINTERGATAN II: the history of the Milky Way told by its mergers
• Column Density Profiles of Multi-Phase Gaseous Halos
• A Common Origin for Globular Clusters and Ultra-faint Dwarfs in Simulations of the First Galaxies
• Simulating galaxies in the reionization era with FIRE-2: morphologies and sizes
• The physics of gas phase metallicity gradients in galaxies
• Energy flows in thick accretion disks and their consequences for black hole feedback
• The Evolution and Properties of Rotating Massive Star Populations
• The abundance of satellites around Milky Way- and M31-like galaxies with the TNG50 simulation: a matter of diversity
• The Local Group as a time machine: studying the high-redshift Universe with nearby galaxies
• MultiDark-Galaxies: data release and first results
• The SAMI Galaxy Survey: Data Release One with Emission-line Physics Value-Added Products
• Dwarf Galaxies in CDM, WDM, and SIDM: Disentangling Baryons and Dark Matter Physics
• A contribution of star-forming clumps and accreting satellites to the mass assembly of z ~ 2 galaxies
• Feedback in low-mass galaxies in the early Universe
• Modeling the Connection Between Subhalos and Satellites in Milky Way-like Systems
• CLASSY III: The Properties of Starburst-Driven Warm Ionized Outflows
• Evolution of Intrinsic Scatter in the SFR-Stellar Mass Correlation at 0.5<z<3
• A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
• Diverse Structural Evolution at z > 1 in Cosmologically Simulated Galaxies
• How baryons affect halos and large-scale structure: a unified picture from the Simba simulation
• Deviations from hydrostatic equilibrium in the circumgalactic medium: spinning hot haloes and accelerating flows
• Modelling CO emission from hydrodynamic simulations of nearby spirals, starbursting mergers, and high-redshift galaxies
• No evidence for [CII] halos or high-velocity outflows in z>6 quasar host galaxies
• Discovery of Strongly Inverted Metallicity Gradients in Dwarf Galaxies at $z$$\sim$2
• Cosmic ray feedback from supernovae in dwarf galaxies
• The impact of stellar feedback on the density and velocity structure of the interstellar medium
• The Cosmic Ultraviolet Baryon Survey (CUBS) I. Overview and the diverse environments of Lyman limit systems at z<1
• Return to [Log-]Normalcy: Rethinking Quenching, The Star Formation Main Sequence, and Perhaps Much More
• The host galaxies of X-ray selected Active Galactic Nuclei to z=2.5: Structure, star-formation and their relationships from CANDELS and Herschel/PACS
• Two can play at that game: constraining the role of supernova and AGN feedback in dwarf galaxies with cosmological zoom-in simulations
• Starbursting [O III] emitters and quiescent [C II] emitters in the reionization era
• The Grism Lens-Amplified Survey from Space (GLASS) X. Sub-kpc resolution gas-phase metallicity maps at cosmic noon behind the Hubble Frontier Fields cluster MACS1149.6+2223
• PHANGS-JWST First Results: A statistical view on bubble evolution in NGC628
• 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 spatially resolved Kennicutt-Schmidt relation in the HI dominated regions of spiral and dwarf irregular galaxies
• MC${}^2$: Boosted AGN and star-formation activity in CIZA J2242.8+5301, a massive post-merger cluster at z=0.19
• Supernova-blast waves in wind-blown bubbles, turbulent, and power-law ambient media
• Galaxy Zoo: the dependence of the star formation-stellar mass relation on spiral disk morphology
• A Systematic Survey for Broadened CO Emission Toward Galactic Supernova Remnants
• Spatially adaptive radiation-hydrodynamical simulations of galaxy formation during cosmological reionization
• Supernova Feedback and the Hot Gas Filling Fraction of the Interstellar Medium
• The Relationship Between Molecular Gas, HI, and Star Formation in the Low-Mass, Low-Metallicity Magellanic Clouds
• NIHAO XIII: Clumpy discs or clumpy light in high redshift galaxies?
• Rapid disc settling and the transition from bursty to steady star formation in Milky Way-mass galaxies
• An EAGLE's View of Ex-situ Galaxy Growth
• Variations of the initial mass function in semi-analytical models: implications for the mass assembly and the chemical enrichment of galaxies in the GAEA model
• NIHAO XX: The impact of the star formation threshold on the cusp-core transformation of cold dark matter haloes
• On The Nature of Variations in the Measured Star Formation Efficiency of Molecular Clouds
• Baryonic and dark matter distribution in cosmological simulations of spiral galaxies
• Seeds Don't Sink: Even Massive Black Hole "Seeds" Cannot Migrate to Galaxy Centers Efficiently
• NIHAO VIII: Circum-galactic medium and outflows - The puzzles of HI and OVI gas distributions
• A small-scale dynamo in feedback-dominated galaxies - II. The saturation phase and the final magnetic configuration
• Fast and energetic AGN-driven outflows in simulated dwarf galaxies
• NIHAO VI. The hidden discs of simulated galaxies
• Dancing in the Dark: Uncertainty in ultra-faint dwarf galaxy predictions from cosmological simulations
• Revisiting long-standing puzzles of the Milky Way: the Sun and its vicinity as typical outer disk chemical evolution
• Evolution of galaxy size--stellar mass relation from the Kilo Degree Survey
• Tracing Outflowing Metals in Simulations of Dwarf and Spiral Galaxies
• No Assembly Required: Mergers are Mostly Irrelevant for the Growth of Low-mass Dwarf Galaxies
• Being KLEVER at cosmic noon: ionised gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts
• The Gaia-ESO Survey: a quiescent Milky Way with no significant dark/stellar accreted disc
• Gas infall and radial transport in cosmological simulations of Milky Way-mass disks
• The Argo Simulation: II. The Early Build-up of the Hubble Sequence
• Wet Compaction to a Blue Nugget: a Critical Phase in Galaxy Evolution
• Galaxy mergers moulding the circum-galactic medium - I. The impact of a major merger
• Bursty star formation during the Cosmic Dawn driven by delayed stellar feedback
• The effects of metallicity, UV radiation and non-equilibrium chemistry in high-resolution simulations of galaxies
• Modeling the Impact of Baryons on Subhalo Populations with Machine Learning
• How the super-Eddington regime regulates black hole growth in high-redshift galaxies
• Quenching timescales of dwarf satellites around Milky Way-mass hosts
• FEEDBACK: a SOFIA Legacy Program to Study Stellar Feedback in Regions of Massive Star Formation
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• Assessing Astrophysical Uncertainties in Direct Detection with Galaxy Simulations
• When the Jeans don't fit: How stellar feedback drives stellar kinematics and complicates dynamical modeling in low-mass galaxies
• Mapping Luminous Hot Stars in the Galaxy
• Physics of Galactic Metals: Evolutionary Effects due to Production, Distribution, Feedback & Interaction with Black Holes
• Stellar Populations of over one thousand $z\sim 0.8$ Galaxies from LEGA-C: Ages and Star Formation Histories from D${}_n$4000 and H$\delta$
• Reconciling observed and simulated stellar halo masses
• Star Clusters in Evolving Galaxies
• Outflows and extended [CII] halos in high redshift galaxies
• The natural emergence of the correlation between H2 and star formation rate surface densities in galaxy simulations
• Impact of Lyman alpha pressure on metal-poor dwarf galaxies
• Nearly all Massive Quiescent Disk Galaxies have a Surprisingly Large Atomic Gas Reservoir
• The distribution of mass components in simulated disc galaxies
• Dark Matter Deficient Galaxies Produced Via High-velocity Galaxy Collisions In High-resolution Numerical Simulations
• A Characteristic Mass Scale in the Mass-Metallicity Relation of Galaxies
• VINTERGATAN III: how to reset the metallicity of the Milky Way
• Gas Kinematics in FIRE Simulated Galaxies Compared to Spatially Unresolved HI Observations
• A three-phase amplification of the cosmic magnetic field in galaxies
• Double dark matter vision: twice the number of compact-source lenses with narrow-line lensing and the WFC3 grism
• The impact of quenching on galaxy profiles in the Simba simulation
• Light breeze in the local Universe
• L-GALAXIES 2020: The evolution of radial metallicity profiles and global metallicities in disc galaxies
• A Robust Measurement of the Mass Outflow Rate of the Galactic Outflow from NGC 6090
• Environmental Quenching of Low-Mass Field Galaxies
• First 3D Radiation-Hydrodynamic Simulations of Wolf-Rayet Winds
• Two-Face(s): ionized and neutral gas winds in the local Universe
• A simple method to convert sink particles into stars
• Effect of binary evolution on the inferred initial and final core masses of hydrogen-rich, Type~II supernova progenitors
• Cosmic Rays or Turbulence can Suppress Cooling Flows (Where Thermal Heating or Momentum Injection Fail)
• Rotation curve fitting and its fatal attraction to cores in realistically simulated galaxy observations
• On the Origin of Stochastic, Low-Frequency Photometric Variability in Massive Stars
• MIDIS: Strong (Hb + [OIII]) and Ha emitters at redshift $z\simeq 7-8$ unveiled with JWST/NIRCam and MIRI imaging in the Hubble eXtreme Deep Field (XDF)
• The physics of Lyman-alpha escape from disc-like galaxies
• Fervent: Chemistry-coupled, ionising and non-ionising radiative feedback in magnetohydrodynamical simulations
• The impact of stellar feedback on hot gas in galaxy haloes: the Sunyaev-Zel'dovich effect and soft X-ray emission
• From the Top Down and Back Up Again: Star Cluster Structure from Hierarchical Star Formation
• NIHAO XIX: How supernova feedback shapes the galaxy baryon cycle
• Empirical constraints on the formation of early-type galaxies
• How primordial magnetic fields shrink galaxies
• NIHAO XXI: The emergence of Low Surface Brightness galaxies
• Galaxy-scale AGN Feedback - Theory
• Symphony: Cosmological Zoom-in Simulation Suites over Four Decades of Host Halo Mass
• A panchromatic spatially resolved analysis of nearby galaxies -- II. The main sequence - gas relation at sub-kpc scale in grand-design spirals
• The impact of pre-supernova feedback and its dependence on environment
• Simulating the interstellar medium of galaxies with radiative transfer, non-equilibrium thermochemistry, and dust
• On the model of the circumgalactic mist: the implications of cloud sizes in galactic winds and halos
• The physical nature of the cosmic accretion of baryons and dark matter into halos and their galaxies
• The edge of galaxy formation I: formation and evolution of MW-satellites analogues before accretion
• Spectral separation of the stochastic gravitational-wave background for LISA in the context of a modulated Galactic foreground
• Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA
• Forming early-type galaxies without AGN feedback: a combination of merger-driven outflows and inefficient star formation
• Galactic inflow and wind recycling rates in the EAGLE simulations
• Kinetic energy from supernova feedback in high-resolution galaxy simulations
• An instability of feedback regulated star formation in galactic nuclei
• Stellar Masses of Giant Clumps in CANDELS and Simulated Galaxies Using Machine Learning
• Photochemistry and Heating/Cooling of the Multiphase Interstellar Medium with UV Radiative Transfer for Magnetohydrodynamic Simulations
• Tracing the Quenching History in Galaxy Clusters in the EAGLE Simulation
• Wolf-Rayet stars in the Small Magellanic Cloud as testbed for massive star evolution
• Swirls of FIRE: Spatially Resolved Gas Velocity Dispersions and Star Formation Rates in FIRE-2 Disk Environments
• Cosmological Galaxy Evolution with Superbubble Feedback II: The Limits of Supernovae
• A Census of Sub-kiloparsec Resolution Metallicity Gradients in Star-forming Galaxies at Cosmic Noon from HST Slitless Spectroscopy
• Pressure balance in the multiphase ISM of cosmologically simulated disk galaxies
• Metallicity gradients in small and nearby spiral galaxies
• The central densities of Milky Way-mass galaxies in cold and self-interacting dark matter models
• Collapse in Self-gravitating Turbulent Fluids
• Reionization inference from the CMB optical depth and E-mode polarization power spectra
• The first galaxies: simulating their feedback-regulated assembly
• Incidence, scaling relations and physical conditions of ionised gas outflows in MaNGA
• Gas-phase metallicity gradients in galaxies at $z\sim 6-8$
• Star formation at the edge of the Local Group: a rising star formation history in the isolated galaxy WLM
• Introducing CGOLS: The Cholla Galactic OutfLow Simulation Suite
• A volumetric deep Convolutional Neural Network for simulation of mock dark matter halo catalogues
• Physical properties and scaling relations of molecular clouds: the effect of stellar feedback
• The COS CGM Compendium. II: Metallicities of the Partial and Lyman Limit Systems at z<1
• Validating Semi-Analytic Models of High-Redshift Galaxy Formation using Radiation Hydrodynamical Simulations
• Origins Space Telescope Mission Concept Study Report
• Semi-analytic forecasts for JWST -- III. Intrinsic production efficiency of Lyman-continuum radiation
• Discrete Effects in Stellar Feedback: Individual Supernovae, Hypernovae, and IMF Sampling in Dwarf Galaxies
• HI-selected Galaxies in Hierarchical Models of Galaxy Formation and Evolution
• Evolution of giant molecular clouds across cosmic time
• Low star formation efficiency in typical galaxies at z=5-6
• The Low Redshift Circumgalactic Medium in Simba
• Feedback from OB stars on their parent cloud: Gas exhaustion rather than gas ejection
• Wind-envelope interaction as the origin of the slow cyclic brightness variations of luminous blue variables
• Deriving star formation histories from photometry using energy balance spectral energy distribution modelling
• UVUDF: UV Luminosity Functions at the cosmic high-noon
• Stellar Mass--Gas-phase Metallicity Relation at $0.5\le z\le 0.7$: A Power Law with Increasing Scatter toward the Low-mass Regime
• Kinematic decomposition of IllustrisTNG disk galaxies: morphology and relation with morphological structures
• Scaling relations and baryonic cycling in local star-forming galaxies: II. Gas content and star-formation efficiency
• The Galactic Dust-Up: Modeling Dust Evolution in FIRE
• Roll of the Dice: A Stochastically Sampled IMF Alters the Stellar Content of Simulated Dwarf Galaxies
• Radiation-MagnetoHydrodynamics simulations of cosmic ray feedback in disc galaxies
• On the Star Formation Law for Spiral and Irregular Galaxies
• EDGE-CALIFA survey: Self-regulation of Star formation at kpc scales
• PDRs4All II: JWST's NIR and MIR imaging view of the Orion Nebula
• Characterizing the local relation between star formation rate and gas-phase metallicity in MaNGA spiral galaxies
• Cosmological baryon transfer in the SIMBA simulations
• Impact of relativistic jets on the star formation rate: a turbulence-regulated framework
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• The early phases of galaxy clusters formation in IR: coupling hydrodynamical simulations with GRASIL3D
• Submillimeter flux as a probe of molecular ISM mass in high-$z$ galaxies
• Fast Winds Drive Slow Shells: A Model for the Circumgalactic Medium as Galactic Wind-Driven Bubbles
• How runaway stars boost galactic outflows
• Momentum feedback from marginally-resolved HII regions in isolated disc galaxies
• The Star-Formation Main Sequence: The Dependence of Specific Star Formation Rate and Its Dispersion on Galaxy Stellar Mass
• Cold Dark Matter Substructures in Early-Type Galaxy Halos
• Characterization of star-forming dwarf galaxies at 0.1 $\lesssim z\lesssim$ 0.9 in VUDS: Probing the low-mass end of the mass-metallicity relation
• Star formation and ISM morphology in tidally induced spiral structures
• Dissipative Dark Matter on FIRE: I. Structural and kinematic properties of dwarf galaxies
• The effects of subgrid models on the properties of giant molecular clouds in galaxy formation simulations
• The little things matter: relating the abundance of ultrafaint satellites to the hosts' assembly history
• Cosmological simulations of dwarfs: the need for ISM physics beyond SN feedback alone
• INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars
• What drives the evolution of gas kinematics in star-forming galaxies?
• Properties of the Simulated Circumgalactic Medium
• Star Formation Stochasticity Measured from the Distribution of Burst Indicators
• Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations
• Are star formation rates of galaxies bimodal?
• A tale of two sites -- II: Inferring the properties of minihalo-hosted galaxies with upcoming 21-cm interferometers
• The combined effect of AGN and supernovae feedback in launching massive molecular outflows in high-redshift galaxies
• The Maximum Stellar Surface Density Due to the Failure of Stellar Feedback
• New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
• The Growth and Enrichment of the Intragroup Gas
• Efficacy of early stellar feedback in low gas surface density environments
• Momentum-driven Winds from Radiatively Efficient Black Hole Accretion and Their Impact on Galaxies
• Numerical Problems in Coupling Photon Momentum (Radiation Pressure) to Gas
• The new semianalytic code GalICS 2.0 - Reproducing the galaxy stellar mass function and the Tully-Fisher relation simultaneously
• Galaxies Probing Galaxies at High Resolution: Co-Rotating Gas Associated with a Milky Way Analog at z=0.4
• How fast do young star clusters expel their natal gas?: Estimating the upper limit of the gas expulsion time-scale
• Equilibrium model prediction for the scatter in the star-forming main sequence
• Formation of disk galaxies in preheated media: a preventative feedback model
• Neutral Gas Properties and Ly$\alpha$ Escape in Extreme Green Pea Galaxies
• Great Balls of FIRE I: The formation of star clusters across cosmic time in a Milky Way-mass galaxy
• Young and turbulent: the early life of massive galaxy progenitors
• The Mass and Absorption Columns of Galactic Gaseous Halos
• A chemical model for the interstellar medium in galaxies
• 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
• Nature versus nurture: what regulates star formation in satellite galaxies?
• Multiple Mechanisms Quench Passive Spiral Galaxies
• A Simple Non-equilibrium Feedback Model for Galaxy-Scale Star Formation: Delayed Feedback and SFR Scatter
• Introducing galactic structure finder: the multiple stellar kinematic structures of a simulated Milky Way mass galaxy
• The evolution of turbulent galactic discs: gravitational instability, feedback and accretion
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - I: Bulge+disc decompositions, methods, and biases
• The roles of stellar feedback and galactic environment in star forming molecular clouds
• The sensitivity of stellar feedback to IMF averaging versus IMF sampling in galaxy formation simulations
• Survey of Water and Ammonia in Nearby galaxies (SWAN): Resolved Ammonia Thermometry, Water and Methanol Masers in the Nuclear Starburst of NGC 253
• The impact of Stellar feedback from velocity-dependent ionised gas maps. -- A MUSE view of Haro 11
• The first Super Massive Black Holes: indications from models for future observations
• Quantifying the energetics of molecular superbubbles in PHANGS galaxies
• Multitracer cosmological line intensity mapping mock lightcone simulation
• Early chemo-dynamical evolution of dwarf galaxies deduced from enrichment of r-process elements
• Galactic angular momentum in cosmological zoom-in simulations. I. Disk and bulge components and the galaxy--halo connection
• Stellar and AGN feedback in isolated early-type galaxies: the role in regulating star formation and ISM properties
• The Dark Matter Distributions in Low-Mass Disk Galaxies. II. The Inner Density Profiles
• Measuring dynamical masses from gas kinematics in simulated high-redshift galaxies
• Is there enough star formation in simulated protoclusters?
• Where did the globular clusters of the Milky Way form? Insights from the E-MOSAICS simulations
• Testing Feedback Regulated Star Formation in Gas Rich, Turbulent Disk Galaxies
• Local positive feedback in the overall negative: the impact of quasar winds on star formation in the FIRE cosmological simulations
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
• Growth of First Galaxies: Impacts of Star Formation and Stellar Feedback
• Empirically Constrained Predictions for Metal-Line Emission from the Circumgalactic Medium
• Structural and Dynamical Properties of Galaxies in a Hierarchical Universe: Sizes and Specific Angular Momenta
• The Grism Lens-Amplified Survey from Space (GLASS). IX. The dual origin of low-mass cluster galaxies as revealed by new structural analyses
• Bursting Bubbles: Feedback from Clustered SNe and the Trade-off Between Turbulence and Outflows
• The Resonant Drag Instability (RDI): Acoustic Modes
• NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite
• Neutral CGM as damped Lyα absorbers at high redshift
• The Dust Attenuation Curve versus Stellar Mass for Emission Line Galaxies at z ~ 2
• A new astrophysical solution to the Too Big To Fail problem - Insights from the MoRIA simulations
• The IRX-$\beta$ relation of high-redshift galaxies
• The edge of galaxy formation II: evolution of Milky Way satellite analogues after infall
• Dirt-cheap Gas Scaling Relations: Using Dust Absorption, Metallicity and Galaxy Size to Predict Gas Masses for Large Samples of Galaxies
• The LOFAR Two-metre Sky Survey: the radio view of the cosmic star formation history
• The history of the dark and luminous side of Milky Way-like progenitors
• Ring Galaxies in the EAGLE Hydrodynamical Simulations
• X-ray Twinkles and Pop III Stars
• Galaxies Probing Galaxies in PRIMUS - II. The Coherence Scale of the Cool Circumgalactic Medium
• MUSE integral-field spectroscopy towards the Frontier Fields cluster Abell S1063: II. Properties of low luminosity Lyman alpha emitters at z>3
• Code Comparison in Galaxy Scale Simulations with Resolved Supernova Feedback: Lagrangian vs. Eulerian Methods
• Great Balls of FIRE II: The evolution and destruction of star clusters across cosmic time in a Milky Way-mass galaxy
• Simulations of galaxies formed in warm dark matter halos of masses at the filtering scale
• Dynamic Localised Turbulent Diffusion and its Impact on the Galactic Ecosystem
• NIHAO-XXIII: Dark Matter density shaped by Black Hole feedback
• Can magnetized turbulence set the mass scale of stars?
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• Modeling for Stellar Feedback in Galaxy Formation Simulations
• Quenching and the UVJ diagram in the SIMBA cosmological simulation
• On the Dynamics of Supermassive Black Holes in Gas-Rich, Star-Forming Galaxies: the Case for Nuclear Star Cluster Coevolution
• The DUVET Survey: Resolved Maps of Star Formation Driven Outflows in a Compact, Starbursting Disk Galaxy
• Spatial Decorrelation of Young Stars and Dense Gas as a Probe of the Star Formation-Feedback Cycle in Galaxies
• A new census of dust and polycyclic aromatic hydrocarbons at z=0.7-2 with JWST MIRI
• The impact of magnetic fields on cosmological galaxy mergers. I: Reshaping gas and stellar discs
• The vertical structure of gaseous galaxy discs in cold dark matter halos
• 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
• An evolving and mass dependent ${\sigma }_{\text{sSFR}}$-${\mathrm{M}}_{\star }$ relation for galaxies
• Gas contents of galaxy groups from thermal Sunyaev-Zel'dovich effects
• Radiation hydrodynamics models of Active Galactic Nuclei: Beyond the central parsec
• Clumpy high-z galaxies as a testbed for feedback-regulated galaxy formation
• The role of gas fraction and feedback in the stability and evolution of galactic discs: implications for cosmological galaxy formation models
• Merger Signatures in the Dynamics of Star-forming Gas
• A simple model for molecular hydrogen chemistry coupled to radiation hydrodynamics
• Radiative properties of the first galaxies: rapid transition between blue and red
• Feeding the fire: Tracing the mass-loading of 10^7 K galactic outflows with O VI absorption
• The Star Formation Histories of Disk Galaxies: the Live, the Dead, and the Undead
• The impact of environment and mergers on the HI content of galaxies in hydrodynamic simulations
• Formation of Galactic Disks I: Why Did the Milky Way's Disk Form Unusually Early?
• The IRX-$\beta$ relation: Insights from simulations
• The impact of cosmic rays on dynamical balance and disk-halo interaction in Lstar disk galaxies
• The Grism lens-amplified survey from space (GLASS). VII. The diversity of the distribution of star formation in cluster and field galaxies at 0.3<z<0.7
• The relation between atomic gas and star formation rate densities in faint irregular galaxies
• Evolution of the Stellar Mass--Metallicity Relation - I: Galaxies in the z~0.4 Cluster Cl0024
• Dwarf Galaxy Mass Estimators vs. Cosmological Simulations
• From large-scale environment to CGM angular momentum to star forming activities -- I: star-forming galaxies
• Chandra survey of nearby highly inclined disk galaxies -- IV: New insights into the working of stellar feedback
• Cosmic Ray Acceleration by a Versatile Family of Galactic Wind Termination Shocks
• Figuring Out Gas & Galaxies in Enzo (FOGGIE). III. The Mocky Way: Investigating Biases in Observing the Milky Way's Circumgalactic Medium
• Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales
• Chemical Evolution with Radial Mixing Redux: Extending beyond the Solar Neighborhood
• Formation and settling of a disc galaxy during the last 8 billion years in a cosmological simulation
• Rapid Filamentary Accretion as the Origin of Extended Thin Discs
• Star Formation Suppresion by Tidal Removal of Cold Molecular Gas from an Intermediate-Redshift Massive Post-Starburst Galaxy
• Fifth force constraints from the separation of galaxy mass components
• Galaxy Zoo: star-formation versus spiral arm number
• The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
• Semi-Analytic Galaxies - II. Revealing the role of environmental and mass quenching in galaxy formation
• Simulating the effect of photoheating feedback during reionization
• A dearth of young and bright massive stars in the Small Magellanic Cloud
• Supernovae feedback propagation: the role of turbulence
• Strong Lensing by Galaxies
• The Star Formation Rate Efficiency of Neutral Atomic-dominated Hydrogen Gas in the Outskirts of Star Forming Galaxies from z~1 to z~3
• IQ Collaboratory II: The Quiescent Fraction of Isolated, Low Mass Galaxies Across Simulations and Observations
• Constraining the Warm Dark Matter Particle Mass through Ultra-Deep UV Luminosity Functions at z=2
• Direct Detection of Mirror Matter in Twin Higgs Models
• The Detection of [O III]$\lambda$4363 in a Lensed, Dwarf Galaxy at $z$ = 2.59: Testing Metallicity Indicators and Scaling Relations at High Redshift and Low Mass
• Is it possible to reconcile extragalactic IMF variations with a universal Milky Way IMF?
• Mixing matters
• Modelling of Lyman-alpha Emitting Galaxies and Ionized Bubbles at the Era of Reionization
• Gas flows in the circumgalactic medium around simulated high-redshift galaxies
• A Massive Star is Born: How Feedback from Stellar Winds, Radiation Pressure, and Collimated Outflows Limits Accretion onto Massive Stars
• Origin of highly $r$-process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy
• Zapped then Napped? A rapidly quenched remnant leaker candidate with a steep spectroscopic ${\beta }_{UV}$ slope at z=8.5
• Uncertainties in supernova input rates drive qualitative differences in simulations of galaxy evolution
• Spectral shifting strongly constrains molecular cloud disruption by radiation pressure on dust
• The impact of AGN-driven winds on physical and observable galaxy sizes
• Characterising the intra-cluster light in The Three Hundred simulations
• SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies
• Global Simulations of Galactic Discs: Violent Feedback from Clustered Supernovae during Bursts of Star Formation
• Strong stellar-driven outflows shape the evolution of galaxies at cosmic dawn
• A New Model For Including Galactic Winds in Simulations of Galaxy Formation I: Introducing the Physically Evolved Winds (PhEW) Model
• VINTERGATAN IV: Cosmic phases of star formation in Milky Way-like galaxies
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• The response of dark matter haloes to elliptical galaxy formation: a new test for quenching scenarios
• The Properties of Radio Galaxies and the Effect of Environment in Large Scale Structures at $z\sim 1$
• Virial shocks are suppressed in cosmic ray-dominated galaxy halos
• The effect of gas accretion on the radial gas metallicity profile of simulated galaxies
• NIHAO III: The constant disc gas mass conspiracy
• Stellar feedback strongly alters the amplification and morphology of galactic magnetic fields
• The importance of galaxy formation histories in models of reionization
• Evaluating Lya Emission as a Tracer of the Largest Cosmic Structure at z~2.47
• [CII] halos in ALPINE galaxies: smoking-gun of galactic outflows?
• Dust temperature uncertainties hamper the inference of dust and molecular gas masses from the dust continuum emission of quiescent high-redshift galaxies
• FEEDBACK from the NGC7538 HII region
• Radiative Supernova Remnants and Supernova Feedback
• From HI to Stars: HI Depletion in Starbursts and Star-Forming Galaxies in the ALFALFA H-alpha Survey
• The Effects of Protostellar Jet Feedback on Turbulent Collapse
• The Milky Way Project and ATLASGAL: The distribution and physical properties of cold clumps near infrared bubbles
• Star-formation driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel
• Super-Eddington growth of black holes in the early Universe: effects of disk radiation spectra
• Data-driven spectroscopic estimates of absolute magnitude, distance and binarity -- method and catalog of 16,002 O- and B-type stars from LAMOST
• Negative and Positive Feedback from a Supernova Remnant with SHREC: A detailed Study of the Shocked Gas in IC443
• The Global Star-Formation Law by Supernova Feedback
• Modelling the M*-SFR relation at high redshift: untangling factors driving biases in the intrinsic scatter measurement
• A tight relation between the age distributions of stellar clusters and the properties of the interstellar medium in the host galaxy
• Stellar feedback from HMXBs in cosmological hydrodynamical simulations
• NIHAO XXIV: Rotation or pressure supported systems? Simulated Ultra Diffuse Galaxies show a broad distribution in their stellar kinematics
• Survival of molecular gas in a stellar feedback-driven outflow witnessed with the MUSE TIMER project and ALMA
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• The Origin of the Dust Extinction Curve in Milky Way-like Galaxies
• Relating the Diverse Merger Histories and Satellite Populations of Nearby Galaxies
• Implications of a variable IMF for the interpretation of observations of galaxy populations
• Survey of Water and Ammonia in Nearby galaxies (SWAN): Resolved Ammonia Thermometry, and Water and Methanol Masers in IC 342, NGC 6946 and NGC 2146
• Compact Starburst Galaxies with Fast Outflows: Central Escape Velocities and Stellar Mass Surface Densities from Multi-band Hubble Space Telescope Imaging
• Entropy Driven Winds: Outflows and Fountains Lifted Gently by Buoyancy
• The origin of the relation between metallicity and size in star-forming galaxies
• The VLT LBG Redshift Survey - VI. Mapping HI in the proximity of $z\sim 3$ LBGs with X-Shooter
• Simba: The average properties of the circumgalactic medium of $2\le z\le 3$ quasars are determined primarily by stellar feedback
• Cosmological Simulations of Dwarf Galaxies with Cosmic Ray Feedback
• How galactic environment regulates star formation
• The nature of damped HI absorbers probed by cosmological simulations: satellite accretion and outflows
• Stellar associations powering HII regions $\unicode{x2013}$ I. Defining an evolutionary sequence
• Stacked star formation rate profiles of bursty galaxies exhibit 'coherent' star formation
• Project AMIGA: A Minimal Covering Factor for Optically Thick Circumgalactic Gas Around the Andromeda Galaxy
• Radiative feedback and cosmic molecular gas: the role of different radiative sources
• On the Interpretation of Far-infrared Spectral Energy Distributions. I: The 850 $\mu$m Molecular Mass Estimator
• Cool outflows in MaNGA: a systematic study and comparison to the warm phase
• The Role of Star-Formation and AGN in Dust Heating of z=0.3-2.8 Galaxies - II. Informing IR AGN fraction estimates through simulations
• Empirically-motivated early feedback: momentum input by stellar feedback in galaxy simulations inferred through observations
• Empirical Constraints on the Nucleosynthesis of Nitrogen
• The THESAN-ZOOM project: Burst, quench, repeat -- unveiling the evolution of high-redshift galaxies along the star-forming main sequence
• A highly-ionized region surrounding SN Refsdal revealed by MUSE
• Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
• Cosmological simulations of Milky Way-sized galaxies
• The galaxy-halo size relation of low-mass galaxies in FIRE
• Nonparametric galaxy morphology from UV to submm wavelengths
• Quenching or Bursting: the Role of Stellar Mass, Environment, and Specific Star Formation Rate to $z$ $\sim$ 1
• Testing the Relationship Between Bursty Star Formation and Size Fluctuations of Local Dwarf Galaxies
• The Early-type Stars from LAMOST survey: Atmospheric parameters
• Signature of the first galaxies in JWST deep field observations
• A Dusty Locale: Evolution of Galactic Dust Populations from Milky Way to Dwarf-Mass Galaxies
• Dark Molecular Gas in Simulations of z~0 Disc Galaxies
• A New Discrete Dynamical Friction Estimator Based on $N$-body Simulations
• Faint LAEs near z>4.7 CIV absorbers revealed by MUSE
• A General Precipitation-Limited L_X-T-R Relation Among Early-Type Galaxies
• A Fundamental Test for Galaxy Formation Models: Matching the Lyman-$\alpha$ Absorption Profiles of Galactic Halos over Three Decades in Distance
• CLEAR: Paschen-$\beta$ Star Formation Rates and Dust Attenuation of Low Redshift Galaxies
• Predicting sub-millimeter flux densities from global galaxy properties
• The $I\kappa \epsilon \alpha$ model of feedback-regulated galaxy formation
• Black hole -- galaxy scaling relations in FIRE: the importance of black hole location and mergers
• Exact relations for energy transfer in self-gravitating isothermal turbulence
• Gas-phase metallicity break radii of star-forming galaxies in IllustrisTNG
• The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray line emission
• Comparing Models for IMF Variation Across Cosmological Time in Milky Way-like Galaxies
• Modelling the Milky Way. I -- Method and first results fitting the thick disk and halo with DES-Y3 data
• The observability of galaxy merger signatures in nearby gas-rich spirals
• nIFTy galaxy cluster simulations V: Investigation of the Cluster Infall Region
• A high fraction of close massive binary stars at low metallicity
• Astrophysical Tests of Dark Matter Self-Interactions
• SIRIUS project II: a new tree-direct hybrid code for smoothed particle hydrodynamics/N-body simulations of star clusters
• The Interstellar Medium and Star Formation of Galactic Disks. I. ISM and GMC properties with Diffuse FUV and Cosmic Ray Backgrounds
• Constraints on the HI Mass of NGC 1052-DF2
• The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
• SH$\alpha$DE: Survey description and mass-kinematics scaling relations for dwarf galaxies
• The Fate of Supernova-Heated Gas in Star-Forming Regions of the LMC: Lessons for Galaxy Formation?
• Reproducing the CO-to-H${}_2$ conversion factor in cosmological simulations of Milky Way-mass galaxies
• The density-bounded twilight of starbursts in the early Universe
• Ultra-Diffuse Galaxies as Extreme Star-forming Environments I: Mapping Star Formation in HI-Rich UDGs
• What shapes the far-infrared spectral energy distributions of galaxies?
• Testing Hydrodynamics Schemes in Galaxy Disc Simulations
• How the first stars shaped the faintest gas-dominated dwarf galaxies
• A spatially resolved analysis of star-formation burstiness by comparing UV and H$\alpha$ in galaxies at z$\sim$1 with UVCANDELS
• A Local Leaky-box Model for the Local Stellar Surface Density - Gas Surface Density - Gas Phase Metallicity Relation
• Spatially Resolved Dust, Gas, and Star Formation in the Dwarf Magellanic Irregular NGC4449
• Evidence of extended cold molecular gas and dust halos around $\mathbf{z}\sim 2.3$ Extremely Red Quasars with ALMA
• The Milky Way and Andromeda galaxies in a constrained hydrodynamical simulation: morphological evolution
• Delayed Photons from Binary Evolution Help Reionize the Universe
• From Peculiar Morphologies to Hubble-type Spirals: The relation between galaxy dynamics and morphology in star-forming galaxies at z~1.5
• The galaxy correlation function as a constraint on galaxy formation physics
• Significant enhancement of ${\mathrm{H}}_2$ formation in disk galaxies under strong ram pressure
• The mass-metallicity relation as a ruler for galaxy evolution: insights from the James Webb Space Telescope
• The Characteristic Momentum of Radiatively Cooling Energy-Driven Galactic Winds
• Extended Schmidt law holds for faint dwarf irregular galaxies
• Red Misfits in the Sloan Digital Sky Survey: Properties of Star-forming Red Galaxies
• Hydrodynamic simulations of the central molecular zone with realistic Galactic potential
• Estimating the Milky Way's Mass via Hierarchical Bayes: A Blind Test on MUGS2 Simulated Galaxies
• High-redshift Galaxy Formation with Self-consistently Modeled Stars and Massive Black Holes: Stellar Feedback and Quasar Growth
• The Bimodal Absorption System Imaging Campaign (BASIC) I. A Dual Population of Low-metallicity Absorbers at z $<1$
• Kinematics, Structure, and Mass Outflow Rates of Extreme Starburst Galactic Outflows
• Hydrodynamical structure formation in Milgromian cosmology
• A new model framework for circumgalactic Ly$\alpha$ radiative transfer constrained by galaxy-Ly$\alpha$ forest clustering
• Realistic HI scale heights of Milky Way-mass galaxies in the FIREbox cosmological volume
• The miniJPAS survey: Identification and characterization of the emission line galaxies down to $z<0.35$ in the AEGIS field
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• The history of stellar metallicity in a simulated disc galaxy
• The Elephant in the Bathtub: when the physics of star formation regulate the baryon cycle of galaxies
• Tracing stars in Milky Way satellites with A-SLOTH
• Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
• The small and the beautiful: How the star formation law affects galactic disk structure
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• Galaxy Formation with Local Photoionization Feedback -II. Effect of X-Ray Emission from Binaries and Hot Gas
• SIEGE III: The formation of dense stellar clusters in sub-parsec resolution cosmological simulations with individual star feedback
• Dark-ages Reionization and Galaxy Formation Simulation -- XIX: Predictions of infrared excess and cosmic star formation rate density from UV observations
• Evolution of the Gas Mass Fraction of Progenitors to Today's Massive Galaxies: ALMA Observations in the CANDELS GOODS-S Field
• The Bolocam Galactic Plane Survey. XIII. Physical Properties and Mass Functions of Dense Molecular Cloud Structures
• The baryon cycle of Seven Dwarfs with superbubble feedback
• The diversity of assembly histories leading to disc galaxy formation in a LambdaCDM model
• The Case for Strangulation in Low-Mass Hosts: DDO 113
• The morphology and kinematics of neutral hydrogen in the vicinity of z=0 galaxies with Milky Way masses -- a study with the Illustris simulation
• Quasi-equilibrium models of high-redshift disc galaxy evolution
• Effects of feedback on galaxies in the VELA simulations: elongation, clumps and compaction
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• Properties of the interstellar medium in star-forming galaxies at redshifts 2 < z < 5 from the VANDELS survey
• Gas Accretion and Galactic Chemical Evolution: Theory and Observations
• A 30 kpc Spatially Extended Clumpy and Asymmetric Galactic Outflow at z $\sim$ 1.7
• The Obsidian model: Three regimes of black hole feedback
• The MOSDEF-LRIS Survey: Connection between Galactic-scale Outflows and the Properties of $z$~2 star-forming Galaxies
• X-ray Emission from the Taffy (VV254) Galaxies and Bridge
• The Clustering and Halo Masses of Star Forming Galaxies at z<1
• Strongly Time-Variable Ultra-Violet Metal Line Emission from the Circum-Galactic Medium of High-Redshift Galaxies
• The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
• Clumpy galaxies in cosmological simulations: The effect of ISM model
• The Complete Local Volume Groups Sample -- IV. Star formation and gas content in group-dominant galaxies
• A Search for correlations between turbulence and star formation in LITTLE THINGS dwarf irregular galaxies
• External gas accretion provides a fresh gas supply to the active S0 galaxy NGC 5077
• Probing the CGM of Low-redshift Dwarf Galaxies Using FIRE Simulations
• Filamentary structures of ionized gas in Cygnus X
• Gas clump formation via thermal instability in high-redshift dwarf galaxy mergers
• Galactic Chemical Evolution Models Favor an Extended Type Ia Supernova Delay-Time Distribution
• Dependence of galaxy clustering on UV-luminosity and stellar mass at $z\sim 4-7$
• Local models of two-temperature accretion disc coronae. I. Structure, outflows, and energetics
• The Cloud Factory II: Gravoturbulent Kinematics of Resolved Molecular Clouds in a Galactic Potential
• The LEGA-C of nature and nurture in stellar populations of galaxies at z~0.6-1.0: D4000 and H-delta reveal different assembly histories for quiescent galaxies in different environments
• The role of gas kinematics in setting metallicity gradients at high redshift
• The Origin and Evolution of Lyman-alpha Blobs in Cosmological Galaxy Formation Simulations
• Star Formation in Simulated Galaxies: Understanding the Transition to Quiescence at $3\times 10^{10}$ M${}_{\odot }$
• Smoothed Particle Radiation Hydrodynamics: Two-Moment method with Local Eddington Tensor Closure
• The Robustness of Cosmological Hydrodynamic Simulation Predictions to Changes in Numerics and Cooling Physics
• Gas around galaxy haloes - III: hydrogen absorption signatures around galaxies and QSOs in the Sherwood simulation suite
• The galaxy - halo connection in low mass halos
• Barlenses in the CALIFA survey: combining the photometric and stellar population analysis
• From Seeds to Supermassive Black Holes: Capture, Growth, Migration, and Pairing in Dense Proto-Bulge Environments
• The radial acceleration relation is a natural consequence of the baryonic Tully-Fisher relation
• Simplified galaxy formation with mesh-less hydrodynamics
• Momentum and energy injection by a supernova remnant into an inhomogeneous medium
• LEO-Py: Estimating likelihoods for correlated, censored, and uncertain data with given marginal distributions
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• Giant Star Forming Complexes in High-z Main Sequence Galaxy Analogues: The Internal Structure of Clumps in DYNAMO Galaxies
• Observation and calibration strategies for large-scale multi-beam velocity-resolved mapping of the [CII] emission in the Orion molecular cloud
• Testing Feedback from Star Clusters in Simulations of the Milky Way Formation
• Clumps as multiscale structures in cosmic noon galaxies
• The Manhattan Suite: Accelerated galaxy evolution in the early Universe
• Dynamical modelling and origin of gas turbulence in z $\sim$ 4.5 galaxies
• Near-IR clumps and their properties in high-z galaxies with JWST/NIRCam
• A geostatistical analysis of multiscale metallicity variations in galaxies [II]: Predicting the metallicities of Hii and diffuse ionised gas regions via universal kriging
• Formation of proto-globular cluster candidates in cosmological simulations of dwarf galaxies at $z>4$
• Galactic Winds across the Gas-Rich Merger Sequence: I. Highly Ionized N V and O VI Outflows in the QUEST Quasars
• Excitation and acceleration of molecular outflows in LIRGs: The extended ESO 320-G030 outflow on 200-pc scales
• The Effects of Metallicity and Abundance Pattern of the ISM on Supernova Feedback
• The Duration of Star Formation in Galactic Giant Molecular Clouds. I. The Great Nebula in Carina
• The Implications of Local Fluctuations in the Galactic Midplane for Dynamical Analysis in the Gaia Era
• The Mass and Absorption Columns of Galactic Gaseous Halos II -- The High Ionization State Ions
• On the deuterium abundance and the importance of stellar mass loss in the interstellar and intergalactic medium
• Probing Hot Gas Components of Circumgalactic Medium in Cosmological Simulations with the Thermal Sunyaev-Zel'dovich Effect
• Deep Chandra observations of diffuse hot plasma in M83
• Correlations between H$\alpha$ Equivalent Width and Galaxy Properties at $z=0.47$: Physical or Selection-driven?
• X-ray morphology of cluster-mass haloes in self-interacting dark matter
• Early Results from GLASS-JWST. XXV. Electron Density in the Interstellar Medium at $0.7\lesssim z\lesssim 9.3$ with NIRSpec High-resolution Spectroscopy
• Investigating 39 Galactic Wolf-Rayet stars with VLTI/GRAVITY: Uncovering A Long Period Binary Desert
• Detection of the self-regulation of star formation in galaxy discs
• Electron Densities and Nitrogen Abundances in Ionized Gas Derived Using [NII] Fine-structure and Hydrogen Recombination lines
• Understanding the progenitor formation galaxies of merging binary black holes
• A multi-tracer empirically-driven approach to line-intensity mapping lightcones
• Local and global gas metallicity versus stellar age relation in MaNGA galaxies
• On the likelihoods of finding very metal-poor (and old) stars in the Milky Way's disc, bulge, and halo
• Investigating Clumpy Galaxies in the Sloan Digital Sky Survey Stripe 82 using the Galaxy Zoo
• Determining the Timescale over Which Stellar Feedback Drives Turbulence in the ISM: A Study of four Nearby Dwarf Irregular Galaxies
• ELUCID VII: Using Constrained Hydro Simulations to Explore the Gas Component of the Cosmic Web
• Simulations of black hole fueling in isolated and merging galaxies with an explicit, multiphase ISM
• GalICS 2.1: a new semianalytic model for cold accretion, cooling, feedback and their roles in galaxy formation
• Active galactic nuclei jets simulated with smoothed particle hydrodynamics
• AI-assisted super-resolution cosmological simulations III: Time evolution
• Fiery Cores: Bursty and Smooth Star Formation Distributions across Galaxy Centers in Cosmological Zoom-in Simulations
• Degeneracies between baryons and dark matter: the challenge of constraining the nature of dark matter with JWST
• Simulating Globular Clusters in Dark Matter Sub-Halos
• Robust profile decomposition for large extragalactic spectral-line surveys
• Timescales for Hi consumption and SFR depletion of satellite galaxies in groups
• Gas accretion in Milky Way-like galaxies: temporal and radial dependencies
• 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
• Accurate mass estimates from the proper motions of dispersion-supported galaxies
• The complete census of molecular hydrogen in a simulated disc galaxy
• The MURALES survey. I. A dual AGN in the radio galaxy 3C459?
• Accelerated quenching and chemical enhancement of massive galaxies in a $z\sim 4$ gas-rich halo
• Cosmic Voids in Evolving Dark Sector Cosmologies: the Low Redshift Universe
• Dwarf galaxy formation with and without dark matter-baryon streaming velocities
• The Rest-frame $H$-band Luminosity Function of Red Sequence Galaxies in Clusters at $1.0<z<1.3$
• The CGM-GRB Study. I. Uncovering The CircumGalactic Medium around GRB hosts at redshifts 2-6
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• A Dusty Dawn: Galactic Dust Buildup at $z\gtrsim 5$
• Is the molecular KS relationship universal down to low metallicities?
• The Physical Nature of Circumgalactic Medium Absorbers in Simba
• The quenched mass portion of star-forming galaxies and the origin of the star formation sequence slope
• The Gas Mass Reservoir of Quiescent Galaxies at Cosmic Noon
• The Timescales of Star Cluster Emergence: The Case of NGC 4449
• Novel Conservative Methods for Adaptive Force Softening in Collisionless and Multi-Species N-Body Simulations
• A Semi-Analytical Line Transfer (SALT) Model III: Galactic Inflows
• SDSS-IV MaNGA: A serendipitous observation of a potential gas accretion event
• The Strong Gravitationally Lensed Herschel Galaxy HLock01: Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas
• Quenching, bursting and galaxy shapes: colour transformation as a function of morphology
• Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants
• Recent progress in simulating galaxy formation from the largest to the smallest scales
• Cosmic Voids in Evolving Dark Sector Cosmologies: the High Redshift Universe
• Gas dynamics and star formation in NGC 6822
• Critical Metallicity of Cool Supergiant Formation. I. Effects on Stellar Mass Loss and Feedback
• Populations of evolved massive binary stars in the Small Magellanic Cloud II: Predictions from rapid binary evolution
• Testing the Breathing Mode in Intermediate Mass Galaxies and its Predicted Star Formation Rate-Size Anti-Correlation
• The Hot Gas Exhaust of Starburst Engines in Mergers: Testing Models of Stellar Feedback and Star Formation Regulation
• Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies
• G.A.S. I: A prescription for turbulence-regulated star formation and its impact on galaxy properties
• Running Late: Testing Delayed Supermassive Black Hole Growth Models Against the Quasar Luminosity Function
• Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
• Ionised gas kinematics in bipolar H II regions
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• Effects of Stellar Feedback on Stellar and Gas Kinematics of Star-Forming Galaxies at 0.6<z<1.0
• Where are the extremely metal-poor stars in the Milky Way and Andromeda? Expectations from TNG50
• Probing Feedback in Galaxy Formation with Millimeter-wave Observations
• The physical properties of massive green valley galaxies as a function of environments at $0.5<z<2.5$ in 3D-\textit{HST}/CANDELS fields
• Extending Semi-numeric Reionisation Models to the First Stars and Galaxies
• Dust Buried Compact Sources in the Dwarf Galaxy NGC 4449
• Non-Parametric Spherical Jeans Mass Estimation with B-splines
• Galaxy luminosity functions at redshifts 0.6 to 1.2 in the Chandra Deep Field South
• 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
• Abundance matching for low mass galaxies in the CDM and FDM models
• A VLT/FORS2 Narrowband Imaging Search for MgII Emission Around z ~ 0.7 Galaxies
• Exploring the Correlation between $\mathrm{H}\alpha$-to-UV Ratio and Burstiness for Typical Star-forming Galaxies at $z\sim 2$
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• A selection of Hα emitters at z = 2.1-2.5 using the Ks-band photometry of ZFOURGE
• An Empirical Determination of the Dependence of the Circumgalactic Mass Cooling Rate and Feedback Mass Loading Factor on Galactic Stellar Mass
• A quantitative demonstration that stellar feedback locally regulates galaxy growth
• First results from SMAUG: Insights into star formation conditions from spatially-resolved ISM properties in TNG50
• Positive feedback at the disc-halo interface
• On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn
• A Search for H I Lyman $\alpha$ Counterparts to Ultra-Fast X-ray Outflows
• Measuring Star-Formation Histories, Distances, and Metallicities with Pixel Color-Magnitude Diagrams I: Model Definition and Mock Tests
• Sliding into DM: Determining the local dark matter density and speed distribution using only the local circular speed of the Galaxy
• NGC 6822 as a probe of dwarf galactic evolution
• The Grism Lens-Amplified Survey from Space (GLASS). XII. Spatially Resolved Galaxy Star Formation Histories and True Evolutionary Paths at z > 1
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• The Direct-Method Oxygen Abundance of Typical Dwarf Galaxies at Cosmic High-Noon
• Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization
• The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
• Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift $z=0$
• HYACINTH: HYdrogen And Carbon chemistry in the INTerstellar medium in Hydro simulations
• SDSS-IV MaNGA: Constraints on the Conditions for Star Formation in Galaxy Discs
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• Measuring Star Formation Histories, Distances, and Metallicities with Pixel Color-Magnitude Diagrams II: Applications to Nearby Elliptical Galaxies
• Explaining the Weak Evolution of the High-Redshift Mass-Metallicity Relation with Galaxy Burst Cycles
• Implementing Dust Shielding as a Criteria for Star Formation
• Another X-ray UFO without a momentum-boosted molecular outflow. ALMA CO(1-0) observations of the galaxy pair IRAS 05054+1718
• Entropy-Conserving Scheme for Modeling Nonthermal Energies in Fluid Dynamics Simulations
• On the Origin of High-velocity Clouds in the Galaxy
• Oxygen Loss from Simulated Galaxies and the Metal Flow Main Sequence: Predicting the Dependence on Mass and Environment
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe II. -- Direct Measurement of the Dependencies on Redshift and Host Halo Mass of Stellar Mass Growth in Central Disk Galaxies
• The Formation of a Milky Way-sized Disk Galaxy 1. A Comparison of Numerical Methods
• High-Resolution Chemical Abundances of the Nyx Stream
• Physical Properties and Scaling Relations of Molecular Clouds: the Impact of Star Formation
• Bursty star formation feedback and cooling outflows
• Diverse dark matter profiles in FIRE dwarfs: black holes, cosmic rays and the cusp-core enigma
• Recovering Injected Astrophysics from the LISA Galactic Double White Dwarf Binaries
• Improved Measurements of Galaxy Star Formation Stochasticity from the Intrinsic Scatter of Burst Indicators
• Impact of star formation models on the growth of simulated galaxies at high redshifts
• Non-explosive pre-supernova feedback in the COLIBRE model of galaxy formation
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• Modelling H${}_2$ and its effects on star formation using a joint implementation of GADGET-3 and KROME
• Abundance matching tested on small scales with galaxy dynamics
• Where Did the Outskirts Go? Outer Stellar Haloes as a Sensitive Probe of Supernova Feedback
• Gusts in the Headwind: Uncertainties in Direct Dark Matter Detection
• Effects of secular growth and mergers on the evolution of metallicity gradients and azimuthal variations in a Milky Way-like galaxy
• Observational Diagnostics of Gas Flows: Insights from Cosmological Simulations
• Pre-supernova stellar feedback in nearby starburst dwarf galaxies
• The physical origin of positive metallicity radial gradients in high-redshift galaxies: insights from the FIRE-2 cosmological hydrodynamic simulations
• Bidimensional Exploration of the warm-Temperature Ionised gaS (BETIS) II. Revisiting the ionisation mechanism of the extraplanar diffuse ionised gas
• Braving the Storm: Quantifying Disk-wide Ionized Outflows in the Large Magellanic Cloud with ULLYSES
• A comparison of ${\text{H}}_2$ formation models at high redshift
• The impact of the cosmological constant on past and future star formation
• Identifying the possible ex-situ origin of the globular clusters of the Milky Way: A kinematic study
• A Novel Scheme for Dark Matter Annihilation Feedback in Cosmological Simulations
• Chandra survey of nearby highly inclined disk galaxies -- V: emission structure and origin of galactic coronae
• Astrophysics with the Laser Interferometer Space Antenna
• ATLASGAL-selected massive clumps in the inner Galaxy. X. Observations of atomic carbon at 492 GHz
• A Simple Sub-Grid Model For Cosmic Ray Effects on Galactic Scales
• Dark Matter-Induced Baryonic Feedback in Galaxies
• Evolution of Gas Flows along the Starburst to Post-Starburst to Quiescent Galaxy Sequence
• A public grid of radiative transfer simulations for Lyman-alpha and metal lines in idealised galactic outflows
• Spatially Resolved Circumgalactic Medium around a Star-Forming Galaxy Driving a Galactic Outflow at $z\approx 0.8$
• The life cycle of giant molecular clouds in simulated Milky Way-mass galaxies
• Measurements of the angular momentum-mass relations in the Simba simulation
• Substructure in the Globular Cluster Populations of the Virgo Cluster Elliptical Galaxies M84 and M86
• Evidence for Non-smooth Quenching in Massive Galaxies at $z\sim 1$
• Galaxy luminosity function and its cosmological evolution: Testing a new feedback model depending on galaxy-scale dust opacity
• Central densities of dark matter halos in FIRE-2 simulations of low-mass galaxies with cold dark matter and self-interacting dark matter
• The fate of the interstellar medium in early-type galaxies. IV. The impact of stellar feedback, mergers, and black holes on the cold ISM in simulated galaxies
• Red riding on hood: Exploring how galaxy colour depends on environment
• The drastic impact of Eddington-limit induced mass ejections on massive star populations
• Dark-ages Reionization and Galaxy Formation Simulation - XV. Stellar evolution and feedback in dwarf galaxies at high redshift
• Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
• Dust around massive stars is agnostic to galactic environment: New insights from PHAT/BEAST
• Intertwined Formation of ${\mathrm{H}}_2$, Dust, and Stars in Cosmological Simulations
• Delayed Stellar Mass Assembly in the Low Surface Brightness Dwarf Galaxy KDG215
• Searching for compact objects in the single-lined spectroscopic binaries of the young Galactic cluster NGC 6231
• A-priori Validation of Subgrid-scale Models for Astrophysical Turbulence
• Using Artificial Intelligence and real galaxy images to constrain parameters in galaxy formation simulations
• NIHAO-RiNG: A Comparison of Simulated Disc Galaxies from GASOLINE and GIZMO
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• Bidimensional Exploration of the warm-Temperature Ionised gaS (BETIS) I. Showcase sample and first results
• The emergence of globular clusters and globular-cluster-like dwarfs
• The Evolution of Magellanic-like Galaxy Pairs and The Production of Magellanic Stream Analogues in Simulations with Tides, Ram Pressure, and Stellar Feedback
• H$\alpha$-based Star Formation Rates in and around z $\sim$ 0.5 EDisCS clusters
• The galaxy counterpart of the high-metallicity and 16 kpc impact parameter DLA towards Q0918+1636 - a challenge to galaxy formation models?
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• Multiple gas phases in supernova remnant IC 443: mapping shocked H${}_2$ with VLT/KMOS
• Does radiative feedback make faint z>6 galaxies look small?
• Beyond the stars: Linking H$\alpha$ sizes, kinematics, and star formation in galaxies at $z\approx 4-6$ with JWST grism surveys and $\text{geko}$
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• Great Balls of FIRE IV. The contribution of massive star clusters to the astrophysical population of merging binary black holes
• SDSS-V Local Volume Mapper (LVM): Revealing the Structure of the Rosette Nebula
• 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
• Local variations of the Stellar Velocity Ellipsoid-II: the effect of the bar in the inner regions of Auriga galaxies
• Extreme Neutral Outflow in a non-AGN Quiescent Galaxy at z~1.3
• Improving Performance of Zoom-In Cosmological Simulations using Initial Conditions with Customized Grids
• The outskirts of M33: Tidally induced distortions versus signatures of gas accretion
• Searching for Conformity Across Cosmic Time with Local Group and Local Volume Star Formation Histories
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• Galaxy Manifold: Characterizing and understanding galaxies with two parameters
• SEURAT: SPH scheme extended with ultraviolet line radiative transfer
• Ionization Modeling Astrophysical Gaseous Structures. I. The Optically Thin Regime
• The Impact of Baryons on the Large-Scale Structure of the Universe
• The effects of Galactic model uncertainties on LISA observations of double neutron stars
• Testing the Momentum-driven Supernova Feedback Paradigm in M31
• A${}^3$COSMOS: The dust content of massive quiescent galaxies and its evolution with cosmic time
• Constraining gas metal mixing strength in simulations using observations of the Milky Way's disc
• Stellar-gas kinematic misalignments in EAGLE: lifetimes and longevity of misaligned galaxies
• The Color Gradients of the Globular Cluster Systems in M87 and M49
• A Galactic Molecular Cloud Clump Catalog from Hi-GAL Data: Method and Initial Results Comparison to BGPS
• Formation of Substructure in Luminous Submillimeter Galaxies (FOSSILS): Evidence of Multiple Pathways to Trigger Starbursts in Luminous Submillimeter Galaxies
• The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
• Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn
• Northern Galactic Molecular Cloud Clumps in Hi-GAL: Dense Gas Map and Environmental Trends
• Refracting into Ultra Diffuse Galaxy NGC 1052-DF2 by Passing near the Center of NGC 1052
• Exploring effects of IMF sampling and SN feedback injection on star formation and metallicity in ultra-faint dwarf galaxies
• Understanding Stellar Mass-Metallicity and Size Relations in Simulated Ultra-Faint Dwarf Galaxies
• Galactic chimney sweeping: the effect of 'gradual' stellar feedback mechanisms on the evolution of dwarf galaxies
• Exploring the evolution of a dwarf spheroidal galaxy with SPH simulations: II. AGN feedback
• A new strategy for matching observed and simulated lensing galaxies
• Applying a star formation model calibrated on high-resolution interstellar medium simulations to cosmological simulations of galaxy formation
• Impact of radiation feedback on the assembly of star clusters in galactic context
• Stirring the cosmic pot: how black hole feedback shapes the matter power spectrum in the Fable simulations
• Comparing population synthesis models of compact double white dwarfs to electromagnetic observations
• ALMA survey of a massive node of the Cosmic Web at $z\sim 3$. II. A dynamically cold and massive disk galaxy in the proximity of a hyperluminous quasar
• Wind of Change: Faraday Rotation in a Simulated Large Magellanic Cloud
• MIGHTEE-HI: The star-forming properties of HI selected galaxies
• ATLASGAL-selected high-mass clumps in the inner Galaxy: XI. Morphology and kinematics of warm inner envelopes
• Dark-Matter-Deficient Galaxies from Collisions: A New Probe of Bursty Feedback and Dark Matter Physics
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• An analytical model to kinematically identify thin discs in MaNGA galaxies
• The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations
• Dissecting stellar populations with manifold learning I. Validation of the method on a synthetic Milky Way-like galaxy
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Evidence for Coupling of Evolved Star Atmospheres and Spiral Arms of the Milky Way
• The observed multiplicity properties of B-type stars in the Galactic young open cluster NGC 6231
• The MOSDEF Survey: A New View of a Remarkable z=1.89 Merger
• Star Formation for Predictive Primordial Galaxy Formation
• Capture and Escape: The Dependence of Radiation Forces on Clumping in Dusty Envelopes
• How Many Bursts Does it Take to Form a Core at the Center of a Galaxy?
• Constraining cosmic ray transport models using circumgalactic medium properties and observables
• The PARADIGM project II: The lifetimes and quenching of satellites in Milky Way-mass haloes
• Nature of High Equivalent Width Emitters in the Epoch of Reionization Revealed by JWST Medium-band Imaging
• Gravitational wave energy spectral density properties from BPASS Galactic binary population in the Milky Way galaxy
• The Formation of Dwarf Galaxy Disks
• 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
• SUNRISE-3D: Sharp UNveiling of AGN feedback Regulation and its Impact on Star-formation at the cosmic noon Epoch
• First JWST/NIRSpec Spectroscopy of O Stars in the Small Magellanic Cloud
• Radial Transport in High-Redshift Disk Galaxies Dominated by Inflowing Streams
• Effect of cosmic rays and ionizing radiation on observational ultraviolet plasma diagnostics in the circumgalactic medium
• A fast algorithm for identifying Friends-of-Friends halos
• Simulating gravitational motion, gas dynamics, and structure in the cosmos
• Linking the Internal Properties of Infant Globular Clusters to their Formation Environments
• The Star Formation History of a Post-Starburst Galaxy Determined From Its Cluster Population
• Galactic chemical evolution revisited
• TULIPS: a Tool for Understanding the Lives, Interiors, and Physics of Stars
• Extended Hernquist-Springel formalism for cosmic star formation
• Star formation in cloud cores -- simulations and observations of dense molecular cores and the formation of solar mass stars
• Resolved Neutral Outflow from a Lensed Dusty Star Forming Galaxy at z=2.09
• Numerical Methods for Simulating Star Formation
• PHIBSS: Searching for Molecular Gas Outflows in Star-Forming Galaxies at $z=$ 0.5-2.6
• Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations
• From naked spheroids to disky galaxies: how do massive disk galaxies shape their morphology?
• How non-thermal pressure impacts the modelling of star formation in galaxy formation simulations
• Estimating the Atmospheric Parameters of Early-type Stars from the Chinese Space Station Telescope (CSST) Slitless Spectra Survey
• The lens SW05 J143454.4+522850: a fossil group at redshift 0.6?
• A Census of B[e] Supergiants
• Comparative internal kinematics of the HII regions in interacting and isolated galaxies: implications for massive star formation modes
• Stellar halos of bright central galaxies II: Scaling relations, colors and metallicity evolution with redshift
• The origin of the intra-cluster light in The Three Hundred simulations
• Using CSST and ejecta-wind interaction in type II-P supernovae to constrain the wind-mass loss of red supergiant stars
• Recent Developments on the HI Gas of Low-Redshift Galaxies Seen by the 21cm Emission Lines
• Research on the Interstellar Medium and Star Formation in the Galaxy: An Indian Perspective
• Astro2020: Hot Drivers of Stellar Feedback from 10 to 10,000 pc
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Mainly on the Plane: Observing the Extended, Ionized Disks of Milky Way Analogs in IllustrisTNG
• Binarity at LOw Metallicity (BLOeM): massive star variability revealed using a novel software tool for point-spread function fitting of TESS images
• Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
• The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES
• Cold vs. Hot Gas Accretion and Angular Momentum in FIRE Simulations: From Halo to Galaxy Scales
• Imladris: a detailed and flexible model for galaxy simulations with individual stars
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• Born in the Dark: The Catastrophic Collapse of Fuzzy Dark Matter Solitons as the Origin of Little Red Dots
• Merging massive black holes: the right place and the right time
• Determining the Dark Matter distribution in galaxies with Deep Learning
• Forward-modelling the Luminosity, Distance, and Size distributions of the Milky Way Satellites
• The link between star formation and gas in nearby galaxies
• The MACH HI absorption survey I: Physical conditions of cold atomic gas outside of the Galactic plane
• EDGE-INFERNO: How chemical enrichment assumptions impact the individual stars of a simulated ultra-faint dwarf galaxy