Physical Models of Galaxy Formation in a Cosmological Framework

Abstract

Modeling galaxy formation in a cosmological context presents one of the greatest challenges in astrophysics today, due to the vast range of scales and numerous physical processes involved. Here we review the current status of models that employ two leading techniques to simulate the physics of galaxy formation: semi-analytic models and numerical hydrodynamic simulations. We focus on a set of observational targets that describe the evolution of the global and structural properties of galaxies from roughly Cosmic High Noon ($z\sim 2-3$) to the present. Although minor discrepancies remain, overall, models show remarkable convergence between different methods and make predictions that are in qualitative agreement with observations. Modelers seem to have converged on a core set of physical processes that are critical for shaping galaxy properties. This core set includes cosmological accretion, strong stellar-driven winds that are more efficient at low masses, black hole feedback that preferentially suppresses star formation at high masses, and structural and morphological evolution through merging and environmental processes. However, all cosmological models currently adopt phenomenological implementations of many of these core processes, which must be tuned to observations. Many details of how these diverse processes interact within a hierarchical structure formation setting remain poorly understood. Emerging multi-scale simulations are helping to bridge the gap between stellar and cosmological scales, placing models on a firmer, more physically grounded footing. Concurrently, upcoming telescope facilities will provide new challenges and constraints for models, particularly by directly constraining inflows and outflows through observations of gas in and around galaxies.

Submitted version of review article to appear in Vol. 53 of Annual Reviews of Astronomy and Astrophysics. 67 pages, 8 figures

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• Molecular gas in z~6 quasar host galaxies
• Learning the Relationship between Galaxies Spectra and their Star Formation Histories using Convolutional Neural Networks and Cosmological Simulations
• Simple Yet Powerful: Hot Galactic Outflows Driven by Supernovae
• The molecular gas content in obscured AGN at z > 1
• A natural boundary of dark matter haloes revealed around the minimum bias and maximum infall locations
• MUFASA: The assembly of the red sequence
• Semi-analytic forecasts for JWST -- III. Intrinsic production efficiency of Lyman-continuum radiation
• O VI Emission Imaging of a Galaxy with the Hubble Space Telescope: a Warm Gas Halo Surrounding the Intense Starburst SDSS J115630.63+500822.1
• The Low Redshift Circumgalactic Medium in Simba
• 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
• The impact of stellar and AGN feedback on halo-scale baryonic and dark matter accretion in the EAGLE simulations
• Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
• Machine Learning and Cosmological Simulations I: Semi-Analytical Models
• How Do Supernovae Impact the Circumgalactic Medium? I. Large-Scale Fountains Around a Milky Way-Like Galaxy
• Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7
• Integral field spectroscopy of nearby QSOs II. The molecular gas content and condition for star formation
• Galactic angular momentum in the IllustrisTNG simulation -- I. Connection to morphology, halo spin, and black hole mass
• The impact of magnetic fields on cold streams feeding galaxies
• On the influence of halo mass accretion history on galaxy properties and assembly bias
• Disk settling and dynamical heating: histories of Milky Way-mass stellar disks across cosmic time in the FIRE simulations
• Hot phase generation by supernovae: resolution, chemistry and thermal conduction
• AGN feedback, quiescence and CGM metal enrichment in early-type galaxies
• Origin of the galaxy HI size-mass relation
• Ubiquitous Molecular Outflows in z > 4 Massive, Dusty Galaxies II. Momentum-Driven Winds Powered by Star Formation in the Early Universe
• Galactic Chemical Evolution of Radioactive Isotopes
• A Giant Intragroup Nebula Hosting a Damped Lya Absorber at z=0.313
• Probing galaxy evolution in massive clusters using ACT and DES: splashback as a cosmic clock
• Cosmic Ballet III: halo spin evolution in the cosmic web
• An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift $1\le z\le 9$
• Cosmological baryon transfer in the SIMBA simulations
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• AGN All the Way Down? AGN-like Line Ratios are Common In the Lowest-Mass Isolated Quiescent Galaxies
• The Physics of Galactic Winds Driven by Cosmic Rays I: Diffusion
• Evolution of Galactic Outflows at $z\sim 0$-$2$ Revealed with SDSS, DEEP2, and Keck spectra
• The KLEVER survey: Nitrogen abundances at $z\sim$2 and probing the existence of a fundamental nitrogen relation
• How runaway stars boost galactic outflows
• Star Formation Stochasticity Measured from the Distribution of Burst Indicators
• INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars
• The Physics of Galactic Winds Driven by Cosmic Rays II: Isothermal Streaming Solutions
• The HIX galaxy survey II: HI kinematics of HI eXtreme galaxies
• Are star formation rates of galaxies bimodal?
• GRUMPY: a simple framework for realistic forward-modelling of dwarf galaxies
• Dual Stellar Halos in the Standard Elliptical Galaxy M105 and Formation of Massive Early-Type Galaxies
• ALMA hints at the presence of turbulent disk galaxies at z > 5
• The emergence of passive galaxies in the early Universe
• Comparing galaxy formation in the L-GALAXIES semi-analytical model and the IllustrisTNG simulations
• Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations
• A machine learning approach to mapping baryons onto dark matter haloes using the EAGLE and C-EAGLE simulations
• Photometric properties of reionization-epoch galaxies in the Simba simulations
• 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
• Does black-hole growth depend on the cosmic environment?
• The many lives of active galactic nuclei-II: The formation and evolution of radio jets and their impact on galaxy evolution
• The Stellar Mass, Star Formation Rate and Dark Matter Halo Properties of LAEs at $z\sim 2$
• Black Hole Growth and Feedback in Isolated Romulus25 Dwarf Galaxies
• Efficacy of early stellar feedback in low gas surface density environments
• The evolution of the stellar mass versus halo mass relationship
• Momentum-driven Winds from Radiatively Efficient Black Hole Accretion and Their Impact on Galaxies
• Cross-correlation of DES Y3 lensing and ACT/$Planck$ thermal Sunyaev Zel'dovich Effect II: Modeling and constraints on halo pressure profiles
• A New Method to Quantify Environment and Model Ram-Pressure Stripping in N-Body Simulations
• Baryons in the CosmicWeb of IllustrisTNG -- II: the Connection among Galaxies, Halos, their Formation Time and their Location in the Cosmic Web
• Equilibrium model prediction for the scatter in the star-forming main sequence
• From Stellar Halos to Intracluster Light: the physics of the Intra-Halo Stellar Component in cosmological hydrodynamical simulations
• X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
• Recent Progress in Modeling the Macro- and Micro-Physics of Radio Jet Feedback in Galaxy Clusters
• Interacting galaxies in the IllustrisTNG simulations -- III: (the rarity of) quenching in post-merger galaxies
• The challenge of simulating the star cluster population of dwarf galaxies with resolved interstellar medium
• Characterizing Dust Attenuation in Local Star-Forming Galaxies: Near-Infrared Reddening and Normalization
• Evolution of the galaxy stellar mass function: evidence for an increasing $M^{\ast }$ from $z=2$ to the present day
• $\text{Mangrove}$: Learning Galaxy Properties from Merger Trees
• Chasing Lyman alpha-emitting galaxies at z = 8.8
• Creating a galaxy lacking dark matter in a dark matter dominated universe
• The inner mass power spectrum of galaxies using strong gravitational lensing: beyond linear approximation
• The first Super Massive Black Holes: indications from models for future observations
• The mass-metallicity relation at z~1-2 and its dependence on star formation rate
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• Galaxies in the Illustris simulation as seen by the Sloan Digital Sky Survey - I: Bulge+disc decompositions, methods, and biases
• The Radio Galaxy Population in the SIMBA SImulations
• Evolution of galactic magnetic fields
• The sensitivity of stellar feedback to IMF averaging versus IMF sampling in galaxy formation simulations
• Voronoi volume function: A new probe of cosmology and galaxy evolution
• The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS
• $\kappa$TNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations
• Local positive feedback in the overall negative: the impact of quasar winds on star formation in the FIRE cosmological simulations
• Early chemo-dynamical evolution of dwarf galaxies deduced from enrichment of r-process elements
• Multitracer cosmological line intensity mapping mock lightcone simulation
• Jet Feedback and the Photon Underproduction Crisis in Simba
• Kinematics and Dynamics of Multiphase Outflows in Simulations of the Star-Forming Galactic ISM
• The rocky road to quiescence: compaction and quenching of quasar host galaxies at z~2
• Connecting and dissecting galaxies' angular momenta and neutral gas in a hierarchical universe: cue DARK SAGE
• The Three-Phase Evolution of the Milky Way
• Co-evolution of black hole accretion and star formation in galaxies up to z=3.5
• Cosmic variance of $z>7$ galaxies: Prediction from BlueTides
• Multi-phase outflows in Mkn 848 observed with SDSS-MaNGA Integral Field Spectroscopy
• Simulating and interpreting deep observations in the Hubble Ultra Deep Field with the JWST/NIRSpec low-resolution 'prism'
• The DUVET Survey: Direct $T_e$-based metallicity mapping of metal-enriched outflows and metal-poor inflows in Mrk 1486
• Constraints on galaxy formation models from the galaxy stellar mass function and its evolution
• The clustering of typical Ly$\alpha$ emitters from $z\sim 2.5-6$: host halo masses depend on Ly$\alpha$ and UV luminosities
• A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
• Do model emission line galaxies live in filaments at z~1?
• A Comprehensive Bayesian Discrimination of the Simple Stellar Population Model, Star Formation History and Dust Attenuation Law in the Spectral Energy Distribution Modeling of Galaxies
• The IRX-$\beta$ relation of high-redshift galaxies
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• Properties of the ionized CGM and IGM: a comparison of galaxy formation models via the Sunyaev-Zel'dovich effect
• A multi-wavelength de-blended Herschel view of the statistical properties of dusty star-forming galaxies across cosmic time
• Modeling for Stellar Feedback in Galaxy Formation Simulations
• Dynamic Localised Turbulent Diffusion and its Impact on the Galactic Ecosystem
• Active galactic nucleus jet feedback in hydrostatic halos
• Code Comparison in Galaxy Scale Simulations with Resolved Supernova Feedback: Lagrangian vs. Eulerian Methods
• SYGMA: Stellar Yields for Galactic Modeling Applications
• Can magnetized turbulence set the mass scale of stars?
• Does the Galaxy-Halo Connection Vary with Environment?
• A Multi-wavelength Study of the Turbulent Central Engine of the Low-mass AGN hosted by NGC404
• The First Large Absorption Survey in HI (FLASH): I. Science Goals and Survey Design
• The Galaxy Activity, Torus, and Outflow Survey (GATOS). (IV): Exploring Ionized Gas Outflows in Central Kiloparsec Regions of GATOS Seyferts
• Pre-supernova feedback sets the star cluster mass function to a power law and reduces the cluster formation efficiency
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• The Extreme Low-mass End of the Mass-Metallicity Relation at $z\sim 7$
• The New Numerical Galaxy Catalog (${\nu }^2$GC): An Updated Semi-analytic Model of Galaxy and AGN with Large Cosmological N-body Simulation
• Constraints on the evolution of the relationship between HI mass and halo mass in the last 12 Gyr
• Dust properties and star formation of approximately a thousand local galaxies
• Lyman-αabsorption beyond the disk of simulated spiral galaxies
• Quiescent galaxies at $z\gtrsim 2.5$: observations vs. models
• AGN Selection Methods Have Profound Impacts on the Distributions of Host Galaxy Properties
• From Nuclear to Circumgalactic: Zooming in on AGN-Driven Outflows at z~2.2 with SINFONI
• Formation of Galactic Disks I: Why Did the Milky Way's Disk Form Unusually Early?
• Finding universal relations in subhalo properties with artificial intelligence
• On the CGM Fundamental Plane: The Halo Mass Dependency of Circumgalactic HI
• A Global Inventory of Feedback
• Exploring the astrophysics of dark atoms
• Machine Learning for Observational Cosmology
• Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations
• Spatially resolved dust properties and quasar-galaxy decomposition of a HyLIRG at z = 4.4
• The cosmic abundance of cold gas in the local Universe
• nIFTy Cosmology: the clustering consistency of galaxy formation models
• A combined VANDELS and LEGA-C study: the evolution of quiescent galaxy size, stellar mass and age from $\text{z}=0.6$ to $\text{z}=1.3$
• Gas accretion regulates the scatter of the mass-metallicity relation
• Close-up view of a luminous star-forming galaxy at z=2.95
• EDGE: What shapes the relationship between HI and stellar observables in faint dwarf galaxies?
• High-resolution synthetic UV-submm images for simulated Milky Way-type galaxies from the Auriga project
• The formation of low surface brightness galaxies in the IllustrisTNG simulation
• The Next Generation Virgo Cluster Survey (NGVS). XXXV. First Kinematical Clues of Overly-Massive Dark Matter Halos in Several Ultra-Diffuse Galaxies in the Virgo Cluster
• Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
• Physics of ULIRGs with MUSE and ALMA: The PUMA project I. Properties of the survey and first MUSE data results
• Breaking baryon-cosmology degeneracy with the electron density power spectrum
• North Ecliptic Pole merging galaxy catalogue
• 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
• Figuring Out Gas & Galaxies in Enzo (FOGGIE). III. The Mocky Way: Investigating Biases in Observing the Milky Way's Circumgalactic Medium
• Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
• Rapid Filamentary Accretion as the Origin of Extended Thin Discs
• $\mathrm{S}\mathrm{IM}\mathrm{BIG}$: Mock Challenge for a Forward Modeling Approach to Galaxy Clustering
• On the origin of magnetic driven winds and the structure of the galactic dynamo in isolated galaxies
• Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales
• Regulation of Star Formation by a Hot Circumgalactic Medium
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• $R_{\mathrm{e}}$. I. Understanding galaxy sizes, associated luminosity densities, and the artificial division of the early-type galaxy population
• A population of galaxy-scale jets discovered using LOFAR
• IQ-Collaboratory 1.1: the Star-Forming Sequence of Simulated Central Galaxies
• Cosmic CARNage I: on the calibration of galaxy formation models
• BIRTH of the COSMOS Field: Primordial and Evolved Density Reconstructions During Cosmic High Noon
• Do AGN triggering mechanisms vary with radio power? II. The importance of mergers as a function of radio power and optical luminosity
• 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
• The physical drivers of the atomic hydrogen-halo mass relation
• The evolution of the galaxy content of dark matter haloes
• On the formation of massive quiescent galaxies with diverse morphologies in the TNG50 simulation
• The abundance of compact quiescent galaxies since z ~ 0.6
• FLUKA cross sections for cosmic-ray interactions with the DRAGON2 code
• The twisted dark matter halo of the Milky Way
• Prediction of H$\alpha$ and [OIII] Emission Line Galaxy Number Counts for Future Galaxy Redshift Surveys
• Figuring Out Gas & Galaxies In Enzo (FOGGIE) VI: The Circumgalactic Medium of $L^{\ast }$ Galaxies is Supported in an Emergent, Non-Hydrostatic Equilibrium
• The evolution of the mass-metallicity relations from the VANDELS survey and the GAEA Semi-Analytic model
• SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies
• Evolution of CIV Absorbers I. The Cosmic Incidence
• EDGE: The sensitivity of ultra-faint dwarfs to a metallicity-dependent initial mass function
• The evolution of barred galaxies in the EAGLE simulations
• Observability of Low-Luminosity AGN in the Early Universe with JWST
• Halo assembly bias from Separate Universe simulations
• Probing the Circum-Galactic Medium with Fast Radio Bursts: Insights from the CAMELS Simulations
• The importance of preventive feedback: inference from observations of the stellar masses and metallicities of Milky Way dwarf galaxies
• GA-NIFS: Multi-phase analysis of a star-forming galaxy at $z\sim 5.5$
• The contribution of HI-bearing ultra-diffuse galaxies to the cosmic number density of galaxies
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• Red quasars blow out molecular gas from galaxies during the peak of cosmic star formation
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• VINTERGATAN-GM: The cosmological imprints of early mergers on Milky-Way-mass galaxies
• The evolution of the SFR and Sigma-SFR of galaxies in cosmic morning (4 < z < 10)
• Dark Matter in Galaxies: evidences and challenges
• Evaluating Lya Emission as a Tracer of the Largest Cosmic Structure at z~2.47
• The importance of galaxy formation histories in models of reionization
• The impact of AGN on stellar kinematics and orbits in simulated massive galaxies
• The Star-forming Main Sequence of the Host Galaxies of Low-redshift Quasars
• The SZ flux-mass ($Y$-$M$) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback
• Local stellar formation history from the 40 pc white dwarf sample
• How cosmological merger histories shape the diversity of stellar haloes
• Gas outflows in two recently quenched galaxies at z = 4 and 7
• SHAPing the Gas: Understanding Gas Shapes in Dark Matter Haloes with Interpretable Machine Learning
• The Faint Host Galaxies of C IV Absorbers at z > 5
• SMART: A new implementation of Schwarzschild's Orbit Superposition technique for triaxial galaxies and its application to an N-body merger simulation
• The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
• The Intrinsic Scatter of the Radial Acceleration Relation
• Star-formation driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel
• Boosting galactic outflows with enhanced resolution
• The Origin of the Dust Extinction Curve in Milky Way-like Galaxies
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• The Evolution of Gas-Phase Metallicity and Resolved Abundances in Star-forming Galaxies at $z\approx 0.6-1.8$
• Simba: The average properties of the circumgalactic medium of $2\le z\le 3$ quasars are determined primarily by stellar feedback
• Investigating The Growing Population of Massive Quiescent Galaxies at Cosmic Noon
• Quasars Probing Quasars IX. The Kinematics of the Circumgalactic Medium Surrounding z ~ 2 Quasars
• A CO molecular gas wind 340 pc away from the Seyfert 2 nucleus in ESO 420-G13 probes an elusive radio jet
• Uncertainties in Galaxy Rotation Curves
• Compact Starburst Galaxies with Fast Outflows: Central Escape Velocities and Stellar Mass Surface Densities from Multi-band Hubble Space Telescope Imaging
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the SIMBA and TNG simulations
• Submillimetre galaxies in two massive protoclusters at z = 2.24: witnessing the enrichment of extreme starbursts in the outskirts of HAE density peaks
• A unified accretion disc model for supermassive black holes in galaxy formation simulations: method and implementation
• Spatially Resolved Metal Loss from M31
• UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
• The two phases of core formation -- orbital evolution in the centres of ellipticals with supermassive black hole binaries
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• Multi-phase black-hole feedback and a bright [CII] halo in a Lo-BAL quasar at $z\sim 6.6$
• Cool outflows in MaNGA: a systematic study and comparison to the warm phase
• The THESAN-ZOOM project: Burst, quench, repeat -- unveiling the evolution of high-redshift galaxies along the star-forming main sequence
• Galaxy Formation in the Santa Cruz semi-analytic model compared with IllustrisTNG -- I. Galaxy scaling relations, dispersions, and residuals at z=0
• Co-evolution of Dust and Chemistry in Galaxy Simulations with a Resolved Interstellar Medium
• IR SED and Dust Masses of Sub-solar Metallicity Galaxies at z~2.3
• The orbital phase space of contracted dark matter halos
• Faint LAEs near z>4.7 CIV absorbers revealed by MUSE
• Suppressing cosmic variance with paired-and-fixed cosmological simulations: average properties and covariances of dark matter clustering statistics
• Missing Giants: Predictions on Dust-Obscured Galaxy Stellar Mass Assembly Throughout Cosmic Time
• The segregation of baryons and dark matter during halo assembly
• Cosmological simulations of Milky Way-sized galaxies
• The DESI PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) Mock Challenge
• Double-peak emission line galaxies in the SDSS catalogue. A minor merger sequence
• Canceling out intensity mapping foregrounds
• First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
• The Spitzer Matching Survey of the UltraVISTA Ultra-deep Stripes (SMUVS): the Evolution of Dusty and Non-Dusty Galaxies with Stellar Mass at z=2-6
• MACER improved: AGN feedback computed in rotating early-type galaxies at high resolution
• A Fundamental Test for Galaxy Formation Models: Matching the Lyman-$\alpha$ Absorption Profiles of Galactic Halos over Three Decades in Distance
• Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
• The bivariate gas-stellar mass distributions and the mass functions of early- and late-type galaxies at $z\sim 0$
• Better Together: The Complex Interplay Between Radiative Cooling and Magnetic Draping
• The galaxy-halo size relation of low-mass galaxies in FIRE
• The cosmic evolution of the stellar mass$-$velocity dispersion relation of early-type galaxies
• Constraining interacting dark energy models with the halo concentration-mass relation
• The interplay between feedback, accretion, transport and winds in setting gas-phase metal distribution in galaxies
• Generating Synthetic Cosmological Data with GalSampler
• The $I\kappa \epsilon \alpha$ model of feedback-regulated galaxy formation
• The Morphology of Reionization in a Dynamically Clumpy Universe
• Observational Measures of Halo Properties Beyond Mass
• Predicting the Neutral Hydrogen Content of Galaxies From Optical Data Using Machine Learning
• Galaxy Formation in Sterile Neutrino Dark Matter Models
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• A hidden population of massive black holes in simulated dwarf galaxies
• Predicting sub-millimeter flux densities from global galaxy properties
• Evidence for the Accretion of Gas in Star-Forming Galaxies: High N/O Abundances in Regions of Anomalously-Low Metallicity
• Exploring the Milky Way Circumgalactic Medium in a Cosmological Context with a Semi-Analytic Model
• Redshift evolution of stellar mass versus gas fraction relation in 0<z<2 regime: observational constraint for galaxy formation models
• Gauging Metallicity of Diffuse Gas Under An Uncertain Ionizing Radiation Field
• What is Important? Morphological Asymmetries are Useful Predictors of Star Formation Rates of Star-forming Galaxies in SDSS Stripe 82
• Tracing star formation with non-thermal radio emission
• Observational Evidence of Evolving Dark Matter Profiles at $z\le 1$
• The SATIN project I: Turbulent multi-phase ISM in Milky Way simulations with SNe feedback from stellar clusters
• Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models
• The Cosmic Microwave Background and the Stellar Initial Mass Function
• Stochastic Modelling of Star Formation Histories III. Constraints from Physically-Motivated Gaussian Processes
• The global and radial stellar mass assembly of Milky Way-sized galaxies
• The complementary roles of feedback and mergers in building the gaseous halo and the X-ray corona of Milky Way-sized galaxies
• ZFIRE: Similar Stellar Growth in H$\alpha$-emitting Cluster and Field Galaxies at z~2
• Infrared luminosity functions and dust mass functions in the EAGLE simulation
• Exploring over 700 massive quiescent galaxies at z = 2-7: Demographics and stellar mass functions
• [OII] emitters in MultiDark-Galaxies and DEEP2
• Diagnostics of a Nuclear Starburst: Water and Methanol Masers
• Modeling multi-phase gases in cosmological simulations using compressible multi-fluid hydrodynamics
• The NEWFIRM HETDEX Survey: Photometric Catalog and a Conservative Sample of Massive Quiescent Galaxies at z=3-5 over 17.5 deg^2 in the SHELA Field
• 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
• CHANG-ES XXV: HI Imaging of Nearby Edge-on Galaxies -- Data Release 4
• Gas phase metallicity determinations in nearby AGNs with SDSS-IV MaNGA: evidence of metal poor accretion
• On the Significance of Rare Objects at High Redshift: The Impact of Cosmic Variance
• pop-cosmos: A comprehensive picture of the galaxy population from COSMOS data
• Effects of Spatial Discretization in Lyman-alpha Line Radiation Transfer Simulations
• The interconnection between galaxy mergers, AGN activity and rapid quenching of star formation in simulated post-merger galaxies
• The AGN contribution to the UV-FIR luminosities of interacting galaxies and its role in identifying the Main Sequence
• New Analytic Solutions for Galaxy Evolution II: Wind Recycling, Galactic Fountains and Late-Type Galaxies
• The galaxy morphology-density relation in the EAGLE simulation
• Photometric Objects around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. I. Methods
• SIMBA-C: An updated chemical enrichment model for galactic chemical evolution in the SIMBA simulation
• Galaxy Formation Efficiency and the Multiverse Explanation of the Cosmological Constant with EAGLE Simulations
• EDGE: A new approach to suppressing numerical diffusion in adaptive mesh simulations of galaxy formation
• Mass Distribution and Bar Formation in Growing Disk Galaxy Models
• HI galaxies with little star formation: an abundance of LIERs
• Connecting cosmological accretion to strong Lyman-alpha absorbers
• Kinematics, Structure, and Mass Outflow Rates of Extreme Starburst Galactic Outflows
• Multi-wavelength mock galaxy catalogs of the low-redshift Universe
• AGN-driven quenching of satellite galaxies
• Assembly of the Intracluster Light in the Horizon-AGN Simulation
• Formation and spatial distribution of hypervelocity stars in AGN outflows
• Observing Merger Trees in a New Light
• Evidence of extended cold molecular gas and dust halos around $\mathbf{z}\sim 2.3$ Extremely Red Quasars with ALMA
• Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables
• The Launching of Cosmic Ray Driven Outflows
• Euclid: Early Release Observations -- Overview of the Perseus cluster and analysis of its luminosity and stellar mass functions
• The Impact of Outflows driven by Active Galactic Nuclei on Metals in and around Galaxies
• Massive galaxy formation caught in action at z~5 with JWST
• On the Prevalence of Super-Massive Black Holes over Cosmic Time
• A Comparison of the Baryonic Tully-Fisher Relation in MaNGA and IllustrisTNG
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• The Response of Dark Matter Haloes to Gas Ejection: CuspCore II
• Far-Ultraviolet Spectra of Main-Sequence O Stars at Extremely Low Metallicity
• The Star Formation Reference Survey-V: the effect of extinction, stellar mass, metallicity, and nuclear activity on star-formation rates based on H$\alpha$ emission
• Discovery and origins of giant optical nebulae surrounding quasar PKS 0454-22
• Oxygen abundances in the narrow line regions of Seyfert galaxies and the metallicity-luminosity relation
• The MUSE Ultra Deep Field (MUDF). III. Hubble Space Telescope WFC3 Grism Spectroscopy and Imaging
• Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• Dust and Power: Unravelling the merger - active galactic nucleus connection in the second half of cosmic history
• The low redshift Lyman-$\alpha$ Forest as a constraint for models of AGN feedback
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• The effect of environment on star formation activity and morphology at 0.5 < z < 2.5 in CANDELS
• The Connection between Mergers and AGN Activity in Simulated and Observed Massive Galaxies
• An Amusing Look at the Host of the Periodic Nuclear Transient ASASSN-14ko Reveals a Second AGN
• Cosmological simulations of quasar fueling to sub-parsec scales using Lagrangian hyper-refinement
• Does jackknife scale really matter for accurate large-scale structure covariances?
• Sub-damped Lyman alpha systems in the XQ-100 survey I -- Identification and contribution to the cosmological HI budget
• Halo models of HI selected galaxies
• The nuclear activity and central structure of the elliptical galaxy NGC 5322
• Data Compression and Inference in Cosmology with Self-Supervised Machine Learning
• Mass-to-Light Ratios of Spatially Resolved Stellar Populations in M31
• Accretion History of AGN III: Radiative Efficiency and AGN Contribution to Reionization
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• Bulge formation inside quiescent lopsided stellar disks: connecting accretion, star formation and morphological transformation in a z ~ 3 galaxy group
• An emission map of the disk-circumgalactic medium transition in starburst IRAS 08339+6517
• Effects of galaxy environment on merger fraction
• NIKA2 Cosmological Legacy Survey: Survey Description and Galaxy Number Counts
• The galaxy-halo connection of disc galaxies over six orders of magnitude in stellar mass
• Dark matter substructures affect dark matter-electron scattering in xenon-based direct detection experiments
• Classifying the full SDSS-IV MaNGA Survey using optical diagnostic diagrams: presentation of AGN catalogs in flexible apertures
• The dearth of difference between central and satellite galaxies II. Comparison of observations with L-GALAXIES and EAGLE in star formation quenching
• The Obsidian model: Three regimes of black hole feedback
• Push it to the limit: Local Group constraints on high-redshift stellar mass functions for Mstar > 10^5 Msun
• Gas Accretion and Galactic Chemical Evolution: Theory and Observations
• QSOs sigposting cluster size halos as gravitational lenses: halo mass, projected mass density profile and concentration at $z\sim 0.7$
• What Is Inside Matters: Simulated Green Valley Galaxies Have Centrally Concentrated Star Formation
• Strongly Time-Variable Ultra-Violet Metal Line Emission from the Circum-Galactic Medium of High-Redshift Galaxies
• DUVET: Spatially Resolved Observations of Star Formation Regulation via Galactic Outflows in a Starbursting Disk Galaxy
• One-Two Quench: A Double Minor Merger Scenario
• There and back again: understanding the critical properties of backsplash galaxies
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• Virial halo mass function in the $Planck$ cosmology
• TODDLERS: A new UV-mm emission library for star-forming regions. 1. Integration with SKIRT and public release
• Analytical halo model of galactic conformity
• The evolution of compact massive quiescent and starforming galaxies derived from the $R_e-R_h$ and $M_{\mathrm{star}}-M_h$ relations
• New empirical constraints on the cosmological evolution of gas and stars in galaxies
• The Complete Local Volume Groups Sample -- IV. Star formation and gas content in group-dominant galaxies
• On the connection between galactic downsizing and the most fundamental galactic scaling relations
• The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
• Mufasa:The strength and evolution of galaxy conformity in various tracers
• A 30 kpc Spatially Extended Clumpy and Asymmetric Galactic Outflow at z $\sim$ 1.7
• Rapid formation of black holes in galaxies: a self-limiting growth mechanism
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• The evolutionary pathways of disk galaxies with different sizes
• The Relative Growth of Black Holes and of the Stellar Components of Galaxies
• SPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust
• Towards precise galaxy evolution: a comparison between spectral indices of $z\sim 1$ galaxies in the IllustrisTNG simulation and the LEGA-C survey
• Two interacting galaxies hiding as one, revealed by MaNGA
• Hybrid analytic and machine-learned baryonic property insertion into galactic dark matter haloes
• A $\sim$15 kpc outflow cone piercing through the halo of the blue compact metal-poor galaxy SBS0335-052
• The Horizon of the McVittie Black Hole: On the Role of the Cosmic Fluid Modeling
• Measuring the cosmic expansion rate using 21-cm velocity acoustic oscillations
• How feedback shapes galaxies: an analytic model
• Witnessing the star-formation quenching in $L_{\ast }$ ellipticals
• The role of AGN on the structure, kinematics and evolution of ETGs in the Horizon simulations
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• Accuracy and precision of triaxial orbit models I: SMBH mass, stellar mass and dark-matter halo
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• The Physical Origin of the Mass-Size Relation and Its Scatter of Disk Galaxies
• The origin of double-peak emission-line galaxies: rotating discs, bars or galaxy mergers?
• Modelling the star-formation activity and ionizing properties of high-redshift galaxies
• Detection of spatial clustering in the 1000 richest SDSS DR8 redMaPPer clusters with Nearest Neighbor distributions
• FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group
• Galaxies decomposition with spiral arms -- II: A multiwavelength case study of M 51
• The diversity of spiral galaxies explained
• The Role of Inner HI Mass in Regulating the Scatter of the Mass-Metallicity Relation
• 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
• The Activation of Galactic Nuclei and Their Accretion Rates are Linked to the Star Formation Rates and Bulge-types of Their Host Galaxies
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. IV. High Precision Constraints on the Evolution of Stellar-Halo Mass Relation at Redshift $z<0.7$
• Deep Chandra observations of diffuse hot plasma in M83
• The hyperluminous, dust-obscured quasar W2246-0526 at z=4.6: detection of parsec-scale radio activity
• A multi-tracer empirically-driven approach to line-intensity mapping lightcones
• Cosmological 3D HI Gas Map with HETDEX Ly$\alpha$ Emitters and eBOSS QSOs at $z=2$: IGM-Galaxy/QSO Connection and a $\sim$ 40-Mpc Scale Giant HII Bubble Candidate
• Modelling the galaxy-halo connection with semi-recurrent neural networks
• AGN must be very efficient at powering outflows
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
• The Shape and Scatter of The Galaxy Main Sequence for Massive Galaxies at Cosmic Noon
• iMaNGA: mock MaNGA galaxies based on IllustrisTNG and MaStar SSPs -- II. The catalogue
• Centrally Concentrated H I Distribution Enhances Star Formation in Galaxies
• ERGO-ML: Towards a robust machine learning model for inferring the fraction of accreted stars in galaxies from integral-field spectroscopic maps
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Galaxies and Halos on Graph Neural Networks: Deep Generative Modeling Scalar and Vector Quantities for Intrinsic Alignment
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• The role of stochastic and smooth processes in regulating galaxy quenching
• PHANGS-ALMA: Arcsecond CO(2-1) Imaging of Nearby Star-Forming Galaxies
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• Timescales for Hi consumption and SFR depletion of satellite galaxies in groups
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• Gas Accretion and Star Formation Rates
• Spatially Resolved Gas Flows Around the Milky Way
• Cosmic-Ray Driven Galactic Winds from the Warm Interstellar Medium
• Quasars at intermediate redshift are not special; but they are often satellites
• Subaru Hyper Suprime-Cam revisits the large-scale environmental dependence on galaxy morphology over 360 deg${}^2$ at z=0.3-0.6
• Cosmic Ray-Driven Galactic Winds with Resolved ISM and Ion-Neutral Damping
• A systematic study of galactic outflows via fluorescence emission: implications for their size and structure
• Broad-line region configuration of the supermassive binary black hole candidate PG1302-102 in the relativistic Doppler boosting scenario
• The size--mass and other structural parameter ($n,{\mu }_z,R_z$) relations for local bulges/spheroids from multicomponent decompositions
• A Semi-Analytical Line Transfer (SALT) Model III: Galactic Inflows
• MusE GAs FLOw and Wind (MEGAFLOW) IX. The impact of gas flows on the relations between the mass, star formation rate and metallicity of galaxies
• Recent progress in simulating galaxy formation from the largest to the smallest scales
• SDSS-IV MaNGA: The MaNGA Dwarf Galaxy Sample
• A search for candidate strongly-lensed dusty galaxies in the Planck satellite catalogues
• Recoiling Supermassive Black Hole Escape Velocities from Dark Matter Halos
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: I. Recent Star Formation Activity in Isolated Milky Way-Mass Galaxies
• The quenched mass portion of star-forming galaxies and the origin of the star formation sequence slope
• Unveiling the inner morphology and gas kinematics of NGC 5135 with ALMA
• Mock halo catalogs: assigning unresolved halo properties using correlations with local halo environment
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE) XV. The Halpha luminosity function of the Virgo cluster
• Morphology-assisted galaxy mass-to-light predictions using deep learning
• The ultra-diffuse galaxy AGC 114905 needs dark matter
• Detection of an ionized gas outflow in the extreme UV-luminous star-forming galaxy BOSS-EUVLG1 at z=2.47
• Growing the First Galaxies' Merger Trees
• Physical properties of hyperluminous, dust-obscured quasars at $z\sim 3$: multiwavelength Spectral Energy Distribution analysis and cold gas content revealed by ALMA
• Flexible Models for Galaxy Star Formation Histories Both Shift and Scramble the Optical Color-M/L Relationship
• Evolution of CIV Absorbers. II. Where does CIV live?
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• Ages and metallicities of quiescent galaxies: confronting broadband ($UVJ$) colours with stellar absorption lines
• The VIRUS-P Exploration of Nearby Galaxies (VENGA): The stellar populations and assembly of NGC 2903's bulge, bar, and outer disc
• The redshift evolution of the S0 fraction for $z<1$ in COSMOS
• Calibration of mid- to far-infrared spectral lines in galaxies
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Age and metal gradients in massive quiescent galaxies at $0.6\lesssim z\lesssim 1.0$: implications for quenching and assembly histories
• AGEL: Is the Conflict Real? Investigating Galaxy Evolution Models using Strong Lensing at 0.3 < z < 0.9
• The Nature and Evolution of Early Massive Quenched Galaxies in the Simba-C Simulation
• Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
• Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
• The molecular gas in the central region of NGC 7213
• The Subtle Effects of Mergers on Star Formation in Nearby Galaxies
• Running Late: Testing Delayed Supermassive Black Hole Growth Models Against the Quasar Luminosity Function
• Galaxy luminosity functions at redshifts 0.6 to 1.2 in the Chandra Deep Field South
• Field spheroid-dominated galaxies in a Λ-CDM Universe
• The detection of ultra-faint low surface brightness dwarf galaxies in the Virgo Cluster: a Probe of Dark Matter and Baryonic Physics
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Revealing the Galaxy-Halo Connection Through Machine Learning
• A new analytic ram pressure profile for satellite galaxies
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• Spatially-resolved UV diagnostics of AGN feedback: radiation pressure dominates in a prototypical quasar-driven superwind
• Thermal and Reionisation History within a Large-Volume Semi-Analytic Galaxy Formation Simulation
• Mesh-free hydrodynamics in PKDGRAV3 for galaxy formation simulations
• The Molecular Mass function of the Local Universe
• Lightning: An X-ray to Submillimeter Galaxy SED-Fitting Code With Physically-Motivated Stellar, Dust, and AGN Models
• A Global Semi-Analytic Model of the First Stars and Galaxies Including Dark Matter Halo Merger Histories
• Overdensity of VVV galaxies behind the Galactic bulge
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• JWST/NIRSpec spectroscopy of intermediate-mass quiescent galaxies at $z\sim 3-4$
• Testing core creation in hydrodynamical simulations using the HI kinematics of field dwarfs
• AGN and Star Formation at Cosmic Noon: Comparison of Data to Theoretical Models
• The Circumgalactic Medium in Massive Halos
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• 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
• Abundance matching for low mass galaxies in the CDM and FDM models
• Modelling Dark Matter Halo Spin using Observations and Simulations: application to UGC 5288
• Probing the fluctuating Ultra-violet background using the Hubble Frontier Fields
• The connection between stellar mass, age and quenching timescale in massive quiescent galaxies at $z\simeq 1$
• Reconciling Mass Functions with the Star-Forming Main Sequence Via Mergers
• Warm ionized gas in the blue compact galaxy Haro 14 viewed by MUSE. The diverse ionization mechanisms acting in low-mass starbursts
• Damped Lyman-$\alpha$ absorbers and atomic hydrogen in galaxies: the view of the GAEA model
• Global analysis of luminosity- and colour-dependent galaxy clustering in the Sloan Digital Sky Survey
• Probing galaxy evolution from $z=0$ to $z\simeq 10$ through galaxy scaling relations in three L-Galaxies flavours
• Euclid: Early Release Observations of diffuse stellar structures and globular clusters as probes of the mass assembly of galaxies in the Dorado group
• Tidal features and disc thicknesses of edge-on galaxies in the SDSS Stripe 82
• A quantitative demonstration that stellar feedback locally regulates galaxy growth
• Characterizing the Conditional Galaxy Property Distribution using Gaussian Mixture Models
• Mapping AGN winds: a connection between radio-mode AGN and the AGN feedback cycle
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• Cross Correlation of the Extragalactic Gamma-ray Background with Thermal Sunyaev-Zel'dovich Effect in the Cosmic Microwave Background
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• $Herschel$/PACS OH Spectroscopy of Seyfert, LINER, and Starburst Galaxies
• Probabilistic model for dynamic galaxy decomposition
• Early-Type Galaxies: Elliptical and S0 Galaxies, or Fast and Slow Rotators
• Constraints on galactic outflows from the metallicity-stellar mass-SFR relation of EAGLE simulation and SDSS galaxies
• First results from SMAUG: Insights into star formation conditions from spatially-resolved ISM properties in TNG50
• Boundless baryons: how diffuse gas contributes to anisotropic tSZ signal around simulated Three Hundred clusters
• The Supersonic Project: The eccentricity and rotational support of SIGOs and DM GHOSts
• Infrared fine-structure lines at high redshift
• The Star-Forming Interstellar Medium of Lyman Break Galaxy Analogs
• BreakBRD Galaxies I: Global Properties of Spiral Galaxies with Central Star Formation in Red Disks
• Testing SALT Approximations with Numerical Radiation Transfer Code Part 1: Validity and Applicability
• Can a conditioning on stellar mass explain the mutual information between morphology and environment?
• Outflows in the Gaseous Discs of Active Galaxies and their impact on Black Hole Scaling Relations
• Exploring the Intrinsic Scatter of the Star-Forming Galaxy Main Sequence at redshift 0.5 to 3.0
• Learning the Universe: Cosmological and Astrophysical Parameter Inference with Galaxy Luminosity Functions and Colours
• KiDS-Legacy: Covariance validation and the unified OneCovariance framework for projected large-scale structure observables
• The Baltimore Oriole's Nest: Cool Winds from the Inner and Outer Parts of a Star-Forming Galaxy at z=1.3
• Searching for HI around MHONGOOSE Galaxies via Spectral Stacking
• Simulations of the merging cluster of galaxies Cygnus A
• Extended neutral hydrogen filamentary network in NGC 2403
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Merger identification through photometric bands, colours, and their errors
• Chemical abundances and deviations from the solar S/O ratio in the gas-phase ISM of galaxies based on infrared emission lines
• LBT/ARGOS adaptive optics observations of z$\sim 2$ lensed galaxies
• The JWST Emission Line Survey (JELS): Extending rest-optical narrow-band emission line selection into the Epoch of Reionization
• Hyenas: X-ray Bubbles and Cavities in the Intra-Group Medium
• The Last Journey. II. SMACC -- Subhalo Mass-loss Analysis using Core Catalogs
• The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations
• NGDEEP: The Star Formation and Ionization Properties of Galaxies at $1.7<z<3.4$
• The Dark Matter Halos of HI Selected Galaxies
• HSC-CLAUDS survey: The star formation rate functions since z ~ 2 and comparison with hydrodynamical simulations
• Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations
• Probing the link between quenching and morphological evolution
• SDSS-IV MaNGA: Unveiling Galaxy Interaction by Merger Stages with Machine Learning
• Accelerating Galaxy Winds During the Big Bang of Starbursts
• Modeling Dust Production, Growth, and Destruction in Reionization-Era Galaxies with the CROC Simulations: Methods and Parameter Exploration
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• Field-level simulation-based inference with galaxy catalogs: the impact of systematic effects
• Catching galaxies in the act of quenching star formation
• From haloes to galaxies. III. The gas cycle of local galaxy populations
• Active galactic nuclei feedback in an elliptical galaxy (III): the impacts and fate of cosmological inflow
• Impact of star formation models on the growth of simulated galaxies at high redshifts
• Inferring redshift and galaxy properties via a multi-task neural net with probabilistic outputs: An application to simulated MOONS spectra
• An efficient hybrid method to produce high resolution large volume dark matter simulations for semi-analytic models of reionisation
• On The Role of Supermassive Black Holes in Quenching Star Formation in Local Central Galaxies
• DIISC-I: The Discovery of Kinematically Anomalous HI Clouds in M 100
• Thermal Regulation and the Star-Forming Main Sequence
• Physical Origins of Outflowing Cold Clouds in Local Star-forming Dwarf Galaxies
• Escaping the maze: a statistical sub-grid model for cloud-scale density structures in the interstellar medium
• Insights on Metal Enrichment and Environmental Effect at $z\approx 5-7$ with JWST ASPIRE/EIGER and Chemical Evolution Model
• Chromium Nucleosynthesis and Silicon-Carbon Shell Mergers in Massive Stars
• When relics were made: vigorous stellar rotation and low dark matter content in the massive ultra-compact galaxy GS-9209 at z=4.66
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• The impact of the cosmological constant on past and future star formation
• Observational Diagnostics of Gas Flows: Insights from Cosmological Simulations
• Halo mass function in scale invariant models
• The bimodality in the mass-metallicity relation in SDSS-MaNGA galaxy pairs
• Baryonic Post-Processing of N-body Simulations, with Application to Fast Radio Bursts
• Cosmic evolution of grain size distribution in galaxies using the ${\nu }^2$GC semi-analytic model
• RUBIES spectroscopically confirms the high number density of quiescent galaxies from $2<\mathbf{z}<5$
• Seeking Self-Regulating Simulations of Idealized Milky Way-Like Galaxies
• Re-assessing the stellar population scaling relations of the galaxies in the Local Universe
• The Space Density of Intermediate Redshift, Extremely Compact, Massive Starburst Galaxies
• Clustering of emission line galaxies with IllustrisTNG I.: fundamental properties and halo occupation distribution
• A stochastic model to reproduce the star-formation history of individual galaxies in hydrodynamic simulations
• Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the Cosmic Noon with a SPICA-like mission
• The formation of compact massive relic galaxies in MOND
• Universal bimodality in kinematic morphology and the divergent pathways to galaxy quenching
• Measuring Stellar Masses of Emission Line Galaxies at 1.2<z<1.9
• Enhanced spectrum of primordial perturbations, galaxy formation and small scale structure
• The ALMA-CRISTAL survey: Extended [CII] emission in an interacting galaxy system at z ~ 5.5
• Radio AGN jet alignment: Radio and Optical Position Angle of Radio Galaxies
• Astraeus VII: The environmental-dependent assembly of galaxies in the Epoch of Reionization
• Gas-Phase metallicity for the Seyfert galaxy NGC 7130
• CosmoDRAGoN simulations -- I. Dynamics and observable signatures of radio jets in cosmological environments
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• RadioSED I: Bayesian inference of radio SEDs from inhomogeneous surveys
• Spatially Resolved Circumgalactic Medium around a Star-Forming Galaxy Driving a Galactic Outflow at $z\approx 0.8$
• Evolution of Gas Flows along the Starburst to Post-Starburst to Quiescent Galaxy Sequence
• How are Lyman $\alpha$ absorbers in the cosmic web related to gas-rich galaxies?
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• The quantity of dark matter in early-type galaxies and its relation to the environment
• Determining the time before or after a galaxy merger event
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• A Bayesian chemical evolution model of the DustPedia Galaxy M74
• The spatial distribution deviation and the power suppression of baryons from dark matter
• The environments of the radio galaxy population in SIMBA
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• Multi-Epoch Machine Learning 2: Identifying physical drivers of galaxy properties in simulations
• The miniJPAS survey. Evolution of the luminosity and stellar mass functions of galaxies up to $z\sim 0.7$
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Fading Light, Fierce Winds: JWST Snapshot of a Sub-Eddington Quasar at Cosmic Dawn
• Can Dark Stars account for the star formation efficiency excess at very high redshifts?
• ALMACAL XIII. Evolution of the CO luminosity function and the molecular gas mass density out to $z$ ~ 6
• The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies
• STRRINGS: STReams in Residual Images of Nearby GalaxieS
• A Simulated Galaxy Laboratory: Exploring the Observational Effects on UV Spectral Absorption Line Measurements
• Degeneracies between Modified Gravity and Baryonic Physics
• Metal line emission around z<1 galaxies
• Galaxy formation from a timescale perspective
• Bimodal Formation Time Distribution for Infall Dark Matter Halos
• Galaxy-galaxy lensing in the VOICE deep survey
• Using Artificial Intelligence and real galaxy images to constrain parameters in galaxy formation simulations
• Milliarcsecond X-ray astrometry to resolve inner regions of AGN at $z>1$ using gravitational lensing
• Low-redshift quasars in the SDSS Stripe 82 II: associated companion galaxies and signature of star formation
• Detecting episodes of star formation using Bayesian model selection
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• Dark Matter Annihilation Feedback in Cosmological Simulations II: The Influence on Gas and Halo Structure
• How do uncertainties in galaxy formation physics impact field-level galaxy bias?
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• VALES VIII: Weak ionized gas outflows in star-forming galaxies at $z\sim 0.15$ traced with VLT/MUSE
• A Global Census of Metals in the Universe
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• The THREEHUNDRED project: the effect of baryon processes at galaxy cluster scale
• COMAP Pathfinder -- Season 2 results III. Implications for cosmic molecular gas content at "Cosmic Half-past Eleven"
• TODDLERS: A New UV to Millimeter Emission Library for Star-Forming Regions. II. Star Formation Rate Indicators Using Auriga Zoom Simulations
• A giant central red disk galaxy at redshift $z=0.76$: challenge to theories of galaxy formation
• Gaseous Dynamical Friction: a Numerical Study of Extended Perturbers
• Inferences on relations between distant supermassive black holes and their hosts complemented by the galaxy fundamental plane
• A non cool-core 4.6-keV cluster around the bright nearby radio galaxy PKS B1416-493
• Massive dusty multiphase outflow in local merger shows no sign of slowing on kiloparsec scales
• An Improved and Physically-Motivated Scheme for Matching Galaxies with Dark Matter Halos
• Hierarchical Bayesian inference of the Initial Mass Function in Composite Stellar Populations
• Large-scale geometry and topology of gas fields: Effects of AGN and stellar feedback
• The Chemodynamical Nature of the Triangulum-Andromeda Overdensity
• Dark-ages Reionization and Galaxy Formation Simulation - XIV. Gas accretion, cooling and star formation in dwarf galaxies at high redshift
• Cold-mode and hot-mode accretion in galaxy formation: an entropy approach
• Extracting Galaxy Merger Timescales II: A new fitting formula
• syren-baryon: Analytic emulators for the impact of baryons on the matter power spectrum
• Galaxy Manifold: Characterizing and understanding galaxies with two parameters
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• The hot gas distribution, X-ray luminosity and baryon budget in the L-Galaxies semi-analytic model of galaxy formation
• Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
• Sensitivity analysis of a galaxy formation model
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• Bringing manifold learning and dimensionality reduction to SED fitters
• Extreme Neutral Outflow in a non-AGN Quiescent Galaxy at z~1.3
• Not so-dark: High resolution HI imaging of J0139+4328 and identification of an optical counterpart
• Born to be Starless: Revisiting the Missing Satellite Problem
• Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn
• Growth and Feedback from the First Black Holes
• Hubble Space Telescope Captures UGC~12591: Bulge/Disc Properties, Star Formation and `Missing Baryons' Census in a Very Massive and Fast Spinning Hybrid Galaxy
• Properties beyond mass for unresolved haloes across redshift and cosmology using correlations with local halo environment
• Is there a need for dark matter in galaxies?
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: II. Testing the Impact of Galaxy Mass, Star Formation Indicator, and Neighbour Colours
• MUSE observations of the blue compact dwarf galaxy Haro 14. Data analysis and first results on morphology and stellar populations
• A Fast, Hot Wind from a Nuclear Starburst
• Radial Dependence of the Proto-Globular Cluster Contribution to the Milky Way Formation
• Fisher matrix forecasts on the astrophysics of galaxies during the epoch of reionisation from the 21-cm power spectra
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• The spatially-resolved effect of mergers on the stellar mass assembly of MaNGA galaxies
• Stellar mass measurements in Abell 133 with Magellan / IMACS
• The RINGS Survey III: Medium-Resolution Halpha Fabry-Perot Kinematic Dataset
• Time-average properties of $z\sim 0.6$ major mergers: mergers significantly scatter high-z scaling relations
• Is the stellar mass-stellar metallicity relation universal in the Milky Way satellites and beyond?
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Galaxy Correlation Function and Local Density from Photometric Redshifts Using the Stochastic Order Redshift Technique (SORT)
• Core to Cosmic Edge: SIMBA-C's New Take on Abundance Profiles in the Intragroup Medium at z = 0
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• COSMOS2025: Machine Learning Classification of Early- and Late-type Galaxies at 0 < z < 3
• On the origin of transient features in cosmological N-Body Simulations
• The Nature of LoBAL QSOs: II. HST/WFC3 Observations Reveal Host Galaxies Dominated by Mergers
• LEGA-C stellar populations scaling relations. I: Chemo-archaeological downsizing trends at z~0.7
• Mock X-ray observations of hot gas with L-Galaxies semi-analytic models of galaxy formation
• Machine Learning vs. Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation
• Galactic bars and active galactic nucleus fuelling in the second half of cosmic history
• The Cosmic Evolution of CIV Absorbers at $1.4<z<4.5$: Insights from $100,000$ Systems in DESI Quasars
• Inferring halo masses with Graph Neural Networks
• Aeos: The Impact of Population III Initial Mass Function and Star-by-Star Models in Galaxy Simulations
• An Order Statistics Approach to the Halo Model for Galaxies
• Mock catalogues of emission line galaxies based on the local mass density in dark-matter only simulations
• Estimating the evolution of gas in the Fornax dwarf spheroidal galaxy from its star formation history: an illustrative example
• Co-interacting dark matter and conformally coupled light scalars
• Shocked, Heated, and Now Resolved: H${}_2$ excitation in the low-luminosity AGN at M58 core with JWST
• Pre-heating of the intergalactic medium by gravitational collapse and ultraviolet background
• The GECKOS Survey: Resolved, multiphase observations of mass-loading and gas density in the galactic wind of NGC 4666
• A theoretical investigation of far-infrared fine structure lines at $z>6$ and of the origin of the [OIII]88/[CII]158 enhancement
• The signature of galaxy formation models in the power spectrum of the hydrogen 21cm line during reionization
• A Model For Intergalactic Filaments and Galaxy Formation During the First Gigayear
• The multi-component fitting to the star formation histories in the TNG simulation
• Tracing black hole and galaxy growth across environments since cosmic noon
• Halo Merger Tree Comparison: Impact on Galaxy Formation Models
• The major merger-active galactic nucleus connection up to the cosmic noon
• Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
• ARCHITECTS I: Impact of subgrid physics on the simulated properties of the circumgalactic medium
• Modelling gas around galaxy pairs and groups using the Q0107 quasar triplet
• Black hole merger rates for LISA and LGWA from semi-analytical modelling of light seeds
• Effects of Varied Cosmic Ray Feedback from AGN on Massive Galaxy Properties
• The Eddington Ratio Distribution of Narrow Line Active Galactic Nuclei
• SHAPE. I. A SOM-SED hybrid approach for efficient galaxy parameter estimation leveraging JWST
• Extended Hernquist-Springel formalism for cosmic star formation
• The invariance of group occupation across the cosmic web
• Investigation of mass substructure in gravitational lens system SDP.81 with ALMA long-baseline observations
• Investigating Galactic Fountains in M101: Insights from Ionized, UV emissions and Neutral Gas
• The Effect of Impact Parameters on the Formation of Massive Black Hole Binaries in Galactic Mergers
• Multi-cloud crushing -- the collective survival of cold clouds in galactic outflows
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• Massive Star Clusters in the Semi-Analytical Galaxy Formation Model L-Galaxies 2020
• Baryon-driven decontraction in Milky Way mass haloes
• How Many Bursts Does it Take to Form a Core at the Center of a Galaxy?
• Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
• DESI Mg II Absorbers: Extinction Characteristics & Quasar Redshift Accuracy
• How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
• One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies
• Lyman-alpha at Cosmic Noon II: The relationship between kinematics and Lyman-alpha in z~2-3 Lyman Break Galaxies
• Cosmic Dragons: A Two-Component Mixture Model of COSMOS Galaxies
• Origin of Weak MgII and Higher Ionization Absorption Lines in an Outflow from an Intermediate-Redshift Dwarf Satellite Galaxy
• The Three Hundred Project: A fast semi-analytic model emulator of hydrodynamical galaxy cluster simulations
• A search for cold molecular outflows in cosmic noon galaxies
• Probing baryonic feedback with fast radio bursts: joint analyses with cosmic shear and galaxy clustering
• Radio Galaxies in SIMBA: A MIGHTEE Comparison
• Evaluating quenching in cosmological simulations of galaxy formation with spectral covariance in the optical window
• Recent Developments on the HI Gas of Low-Redshift Galaxies Seen by the 21cm Emission Lines
• Astrophysical Black holes: An Explanation for the Galaxy Quenching
• The ALMA View of High-Redshift Galaxy Formation
• Extending the SAGA Survey (xSAGA) I: Satellite Radial Profiles as a Function of Host Galaxy Properties
• Semi-empirical constraints on the HI mass function of star-forming galaxies and ${\Omega }_{\mathrm{HI}}$ at $z\sim 0.37$ from interferometric surveys
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• Forward-modelling the Luminosity, Distance, and Size distributions of the Milky Way Satellites
• The cosmic environment overtakes the local density in shaping galaxy star formation
• Modeling Emission-Line Surface Brightness in a Multiphase Galactic Wind: An O VI Case Study
• Observational constraints on the origin of the elements. X. Combining NLTE and machine learning for chemical diagnostics of 4 million stars in the 4MIDABLE-HR survey
• The contribution of stars, dust, neutral gas and supermassive black holes in galaxies to the cosmic baryon inventory
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• Finding High-Redshift Galaxies with JWST
• Dynamic Zoom Simulations of structure formation beyond standard cosmology
• Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
• Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations
• Imladris: a detailed and flexible model for galaxy simulations with individual stars
• Hydromagnetic waves in an expanding universe -- cosmological MHD code tests using analytic solutions
• Cold vs. Hot Gas Accretion and Angular Momentum in FIRE Simulations: From Halo to Galaxy Scales
• ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations
• The Panchromatic Hubble Andromeda Southern Treasury (PHAST). II. The Spatially Resolved Recent Star Formation History in M31
• HI Observations of Baryon-Dominated Dwarf Galaxy Candidates
• Mimicking the halo-galaxy connection using machine learning
• A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10
• Testing the CCC+TL cosmology with cosmic-chronometer measurements of the Hubble parameter
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Multi-Object Spectroscopy of Galaxy Clusters at $z\sim 0.95$ in Ultra Deep Survey Field with Different Star-formation Properties and Large-scale Environments
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• How non-thermal pressure impacts the modelling of star formation in galaxy formation simulations
• Populating Galaxies Into Halos Via Machine Learning on the Simba Simulation
• Epicyclic Density Variations in the Indus Stellar Stream
• Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• Modelling intergalactic low ionisation metal absorption line systems near the epoch of reionization
• Gas flows in galaxy mergers: supersonic turbulence in bridges, accretion from the circumgalactic medium, and metallicity dilution