Galactic star formation and accretion histories from matching galaxies to dark matter haloes

Abstract

We present a new statistical method to determine the relationship between the stellar masses of galaxies and the masses of their host dark matter haloes over the entire cosmic history from z~4 to the present. This multi-epoch abundance matching (MEAM) model self-consistently takes into account that satellite galaxies first become satellites at times earlier than they are observed. We employ a redshift-dependent parameterization of the stellar-to-halo mass relation to populate haloes and subhaloes in the Millennium simulations with galaxies, requiring that the observed stellar mass functions at several redshifts be reproduced simultaneously. Using merger trees extracted from the dark matter simulations in combination with MEAM, we predict the average assembly histories of galaxies, separating into star formation within the galaxies (in-situ) and accretion of stars (ex-situ). The peak star formation efficiency decreases with redshift from 23% at z=0 to 9% at z=4 while the corresponding halo mass increases from 10^11.8M\odot to 10^12.5M\odot. The star formation rate of central galaxies peaks at a redshift which depends on halo mass; for massive haloes this peak is at early cosmic times while for low-mass galaxies the peak has not been reached yet. In haloes similar to that of the Milky-Way about half of the central stellar mass is assembled after z=0.7. In low-mass haloes, the accretion of satellites contributes little to the assembly of their central galaxies, while in massive haloes more than half of the central stellar mass is formed ex-situ with significant accretion of satellites at z<2. We find that our method implies a cosmic star formation history and an evolution of specific star formation rates which are consistent with those inferred directly. We present convenient fitting functions for stellar masses, star formation rates, and accretion rates as functions of halo mass and redshift.

20 pages, 12 figures, 1 table, submitted to MNRAS

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• Characterizing the Circumgalactic Medium of Nearby Galaxies with HST/COS and HST/STIS Absorption-Line Spectroscopy: II. Methods and Models
• Fuzzy Dark Matter and Dark Matter Halo Cores
• Environmental dependence of bulge-dominated galaxy sizes in hierarchical models of galaxy formation. Comparison with the local Universe
• Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation
• The Molecular and Ionized Gas Phases of an AGN-driven Outflow in a Typical Massive Galaxy at z=2
• Expanded haloes, abundance matching and too-big-to-fail in the Local Group
• JADES: The incidence rate and properties of galactic outflows in low-mass galaxies across 3 < z < 9
• Equilibrium Model Constraints on Baryon Cycling Across Cosmic Time
• The Impact of Scatter in the Galaxy UV Luminosity to Halo Mass Relation on Ly$\alpha$ Visibility During the Epoch of Reionization
• The Fates of the Circumgalactic Medium in the FIRE Simulations
• Understanding black hole mass assembly via accretion and mergers at late times in cosmological simulations
• A hypervelocity star with a Magellanic origin
• Origins and Demographics of Wandering Black Holes
• MAGIICAT III. Interpreting Self-Similarity of the Circumgalactic Medium with Virial Mass using MgII Absorption
• Avoiding progenitor bias: The structural and mass evolution of Brightest Group and Cluster Galaxies in Hierarchical models since z~1
• Post-Newtonian dynamical modeling of supermassive black holes in galactic-scale simulations
• The physics of gas phase metallicity gradients in galaxies
• VINTERGATAN II: the history of the Milky Way told by its mergers
• The Dramatic Size and Kinematic Evolution of Massive Early-Type Galaxies
• X-ray Scaling Relation in Early-Type Galaxies: Dark Matter as a Primary Factor in Retaining Hot Gas
• The host dark matter halos of [OII] emitters at 0.5< z< 1.5
• Enhanced tidal stripping of satellites in the galactic halo from dark matter self-interactions
• CLEAR: The Gas-Phase Metallicity Gradients of Star-Forming Galaxies at 0.6 < z < 2.6
• Feedback from supermassive black holes transforms centrals into passive galaxies by ejecting circumgalactic gas
• The COS Absorption Survey of Baryon Harbors (CASBaH): Warm-hot Circumgalactic Gas Reservoirs Traced by Ne VIII Absorption
• The properties of "dark" ΛCDM halos in the Local Group
• Orbital Decay of Supermassive Black Hole Binaries in Clumpy Multiphase Merger Remnants
• The evolving relation between star-formation rate and stellar mass in the VIDEO Survey since $z=3$
• Dynamical signatures of a LCDM-halo and the distribution of the baryons in M33
• Disruption of satellite galaxies in simulated groups and clusters: the roles of accretion time, baryons, and pre-processing
• The formation of extremely diffuse galaxy cores by merging supermassive black holes
• Major Mergers Going Notts: Challenges for Modern Halo Finders
• A Census of Stellar Mass in 10 Massive Haloes at z~1 from the GCLASS Survey
• Circumgalactic Mg II Emission from an Isotropic Starburst Galaxy Outflow Mapped by KCWI
• Preparing for low surface brightness science with the Vera C. Rubin Observatory: characterisation of tidal features from mock images
• The evolution of the star formation rate function in the EAGLE simulations: A comparison with UV, IR and H$\alpha$ observations from z ~ 8 to z ~ 0
• Galactic Archaeology with Gaia
• The MaGICC Baryon Cycle: The Enrichment History of Simulated Disc Galaxies
• A tale of two populations: surviving and destroyed dwarf galaxies and the build up of the Milky Way's stellar halo
• Dissecting the Local Environment of FRB 190608 in the Spiral Arm of its Host Galaxy
• The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
• Brightest cluster galaxies in cosmological simulations: achievements and limitations of AGN feedback models
• Shaken, not blown: the gentle baryonic feedback of nearby starburst dwarf galaxies
• GASTRO library I: the simulated chemodynamical properties of several GSE-like stellar halos
• The clustering of luminous red galaxies at z $\sim$ 0.7 from eBOSS and BOSS data
• Scale-dependent bias in the BAO-scale intergalactic neutral hydrogen
• The Dynamics of Galaxy Pairs in a Cosmological Setting
• A deep survey of short GRB host galaxies over $z\sim 0-2$: implications for offsets, redshifts, and environments
• An Empirical Model for the Star Formation History in Dark Matter Halos
• The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles
• The effect of the LMC on the Milky Way system
• On the Physical Origin of Galactic Conformity
• NIHAO XIII: Clumpy discs or clumpy light in high redshift galaxies?
• NIHAO XX: The impact of the star formation threshold on the cusp-core transformation of cold dark matter haloes
• MUSEQuBES: Calibrating the redshifts of Ly α emitters using stacked circumgalactic medium absorption profiles
• Mass Transport and Turbulence in Gravitationally Unstable Disk Galaxies. I: The Case of Pure Self-Gravity
• Cosmological Galaxy Evolution with Superbubble Feedback I: Realistic Galaxies with Moderate Feedback
• Equilibrium models of the Milky Way mass are biased high by the LMC
• Baryonic and dark matter distribution in cosmological simulations of spiral galaxies
• Precision Scaling Relations for Disk Galaxies in the Local Universe
• A small-scale dynamo in feedback-dominated galaxies - II. The saturation phase and the final magnetic configuration
• Low-mass galaxy assembly in simulations: regulation of early star formation by radiation from massive stars
• NIHAO VI. The hidden discs of simulated galaxies
• NIHAO VIII: Circum-galactic medium and outflows - The puzzles of HI and OVI gas distributions
• Modelling the Tucana III stream - a close passage with the LMC
• Quiescent Ultra-diffuse galaxies in the field originating from backsplash orbits
• Active Galactic Nuclei and their Large-scale Structure: an eROSITA mock catalogue
• An assessment of the "too big to fail" problem for field dwarf galaxies in view of baryonic feedback effects
• Hidden depths in the local Universe: The Stellar Stream Legacy Survey
• Ionized and molecular gas kinematics in a z=1.4 star-forming galaxy
• The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
• Statistics of Dark Matter Substructure: III. Halo-to-Halo Variance
• No Assembly Required: Mergers are Mostly Irrelevant for the Growth of Low-mass Dwarf Galaxies
• Where Do Galaxies End?
• Absorption-Line Detections of $10^{5-6}$ K Gas in Spiral-Rich Groups of Galaxies
• The Galaxy Clustering Crisis in Abundance Matching
• The Massive End of the Stellar Mass Function
• Knocking on giants' doors: I. The evolution of the dust-to-stellar mass ratio in distant dusty galaxies
• Dissecting the Gaseous Halos of z~2 Damped Ly$\alpha$ Systems with Close Quasar Pairs
• Persistence of the Color-Density Relation and Efficient Environmental Quenching to $z\sim 1.4$
• Wet Compaction to a Blue Nugget: a Critical Phase in Galaxy Evolution
• The effect of the deforming dark matter haloes of the Milky Way and the Large Magellanic Cloud on the Orphan-Chenab stream
• The Argo Simulation: II. The Early Build-up of the Hubble Sequence
• Reignition of Star Formation in Dwarf Galaxies
• How to Reconcile the Observed Velocity Function of Galaxies with Theory
• A Lightcone Catalogue from the Millennium-XXL Simulation
• The effects of metallicity, UV radiation and non-equilibrium chemistry in high-resolution simulations of galaxies
• Connecting Transitions in Galaxy Properties to Refueling
• A Dichotomy in Satellite Quenching Around L* Galaxies
• The evolution of superluminous supernova LSQ14mo and its interacting host galaxy system
• The rest-frame optical (900nm) galaxy luminosity function at z~4-7: abundance matching points to limited evolution in the Mstar/Mhalo ratio at z>4
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): Downsizing of the blue cloud and the influence of galaxy size on mass quenching over the last eight billion years
• Galactic disk winds driven by cosmic ray pressure
• Physics of Galactic Metals: Evolutionary Effects due to Production, Distribution, Feedback & Interaction with Black Holes
• CGM${}^2$ I: The Extent of the Circumgalactic Medium Traced by Neutral Hydrogen
• Numerical resolution limits on subhalo abundance matching
• H0LiCOW II. Spectroscopic survey and galaxy-group identification of the strong gravitational lens system HE0435-1223
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
• On the mass of the Local Group
• Constraining the CO intensity mapping power spectrum at intermediate redshifts
• The quiescent phase of galactic disc growth
• Galaxies flowing in the oriented saddle frame of the cosmic web
• Constraining the evolution of CII intensity through the end stages of reionization
• The bias of the submillimetre galaxy population: SMGs are poor tracers of the most massive structures in the z ~ 2 Universe
• Breaking degeneracies in the first galaxies with clustering
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• The eROSITA Final Equatorial Depth Survey (eFEDS): X-ray emission around star-forming and quiescent galaxies at $0.05<z<0.3$
• Star Formation and Clumps in Cosmological Galaxy Simulations with Radiation Pressure Feedback
• The MaGICC volume: reproducing statistical properties of high redshift galaxies
• The distribution of mass components in simulated disc galaxies
• Search for Gamma-ray Emission from Dark Matter Annihilation in the Large Magellanic Cloud with the Fermi Large Area Telescope
• Predicting Galaxy Star Formation Rates via the Co-evolution of Galaxies and Halos
• The galaxy-halo connection of emission-line galaxies in IllustrisTNG
• Machine Learning and Cosmological Simulations II: Hydrodynamical Simulations
• Glimpsing the Imprint of Local Environment on the Galaxy Stellar Mass Function
• Impact of Lyman alpha pressure on metal-poor dwarf galaxies
• The Dekel-Zhao profile: A mass-dependent dark-matter density profile with flexible inner slope and analytic potential, velocity dispersion, and lensing properties
• The evolution of the star forming sequence in hierarchical galaxy formation models
• EMERGE: Empirical predictions of galaxy merger rates since $z\sim 6$
• The Correlation Between Halo Mass and Stellar Mass for the Most Massive Galaxies in the Universe
• Complex AGN feedback in the Teacup galaxy. A powerful ionised galactic outflow, jet-ISM interaction, and evidence for AGN-triggered star formation in a giant bubble
• Size matters: abundance matching, galaxy sizes, and the Tully-Fisher relation in EAGLE
• Light breeze in the local Universe
• Two-Face(s): ionized and neutral gas winds in the local Universe
• Direct Insights into Observational Absorption Line Analysis Methods of the Circumgalactic Medium Using Cosmological Simulations
• The Frequency of Dwarf Galaxy Multiples at Low Redshift in SDSS vs. Cosmological Expectations
• Quantifying the Stellar Halo's Response to the LMC's Infall with Spherical Harmonics
• Dynamical evidence for a morphology-dependent relation between the stellar and halo masses of galaxies
• A flexible subhalo abundance matching model for galaxy clustering in redshift space
• The cumulative star-formation histories of dwarf galaxies with TNG50. I: Environment-driven diversity and connection to quenching
• Disentangling the Cosmic Web Towards FRB 190608
• NIHAO XIX: How supernova feedback shapes the galaxy baryon cycle
• Interpreting Short Gamma Ray Burst Progenitor Kicks and Time Delays Using the Host Galaxy-Dark Matter Halo Connection
• NIHAO XXI: The emergence of Low Surface Brightness galaxies
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• Empirical constraints on the formation of early-type galaxies
• Exploring SMBH Assembly with Semi-analytic Modelling
• From lenticulars to blue compact dwarfs: the stellar mass fraction is regulated by disc gravitational instability
• Luminosity Functions and Host-to-Host Scatter of Dwarf Satellite Systems in the Local Volume
• Constraining the Star Formation Histories in Dark Matter Halos: I. Central Galaxies
• Formation of elongated galaxies with low masses at high redshift
• Tracing Black Hole and Galaxy Co-evolution in the Romulus Simulations
• CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping
• HST Proper Motions of NGC 147 and NGC 185: Orbital Histories and Test of Dynamically Coherent Andromeda Satellite Plane
• Multi-tracer intensity mapping: Cross-correlations, Line noise & Decorrelation
• Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
• Galaxy And Mass Assembly (GAMA): Testing galaxy formation models through the most massive galaxies in the Universe
• An observer's guide to the (Local Group) dwarf galaxies: predictions for their own dwarf satellite populations
• High resolution study of the cluster complexes in a lensed spiral at redshift ~1.5; constraints on the bulge formation and disk evolution
• A fresh look into the interacting dark matter scenario
• The edge of galaxy formation I: formation and evolution of MW-satellites analogues before accretion
• From massive spirals to dwarf irregulars: a new set of tight scaling relations for cold gas and stars driven by disc gravitational instability
• Metal-enriched halo gas across galaxy overdensities over the last 10 billion years
• Vast planes of satellites in a high resolution simulation of the Local Group: comparison to Andromeda
• Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data I: Stellar Mass Growth of Bright Central Galaxies Since z~1.2
• The impact of gas disc flaring on rotation curve decomposition and revisiting baryonic and dark-matter relations for nearby galaxies
• Structure Formation Models Weaken Limits on WIMP Dark Matter from Dwarf Spheroidal Galaxies
• Estimating the Mass of the Milky Way Using the Ensemble of Classical Satellite Galaxies
• Hunting Faint Dwarf Galaxies in the Field Using Integrated Light Surveys
• Cosmological Galaxy Evolution with Superbubble Feedback II: The Limits of Supernovae
• Does circumgalactic OVI trace low-pressure gas beyond the accretion shock? Clues from HI and low-ion absorption, line kinematics, and dust extinction
• The Quest for Dusty Star-forming Galaxies at High Redshift z>4
• Galactic ionising photon budget during the Epoch of Reionisation in the Cosmic Dawn II simulation
• The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to $z\sim 5$
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• MaNGA DynPop -- I. Quality-assessed stellar dynamical modelling from integral-field spectroscopy of 10K nearby galaxies: a catalogue of masses, mass-to-light ratios, density profiles and dark matter
• The Structural Evolution of Milky Way-like Star Forming Galaxies since z~1.3
• Orbits of massive satellite galaxies: II. Bayesian Estimates of the Milky Way and Andromeda masses using high precision astrometry and cosmological simulations
• Detecting clusters of galaxies and active galactic nuclei in an eROSITA all-sky survey digital twin
• Self-Interacting Dark Matter and Small-Scale Gravitational Lenses in Galaxy Clusters
• Galaxy spin as a formation probe: the stellar-to-halo specific angular momentum relation
• Constraining baryonic feedback and cosmology with weak-lensing, X-ray, and kinematic Sunyaev-Zeldovich observations
• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• PRIMUS+DEEP2: The Dependence of Galaxy Clustering on Stellar Mass and Specific Star Formation Rate at 0.2 < z < 1.2
• Self-Interacting Dark Matter and the Origin of Ultra-Diffuse Galaxies NGC1052-DF2 and -DF4
• Reionization inference from the CMB optical depth and E-mode polarization power spectra
• Star Formation and Stellar Mass Assembly in Dark Matter Halos: From Giants to Dwarfs
• Origin and evolution of ultra-diffuse galaxies in different environments
• Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
• KiDS-1000: Combined halo-model cosmology constraints from galaxy abundance, galaxy clustering and galaxy-galaxy lensing
• Incidence, scaling relations and physical conditions of ionised gas outflows in MaNGA
• Galaxy disc scaling relations: A tight linear galaxy -- halo connection challenges abundance matching
• 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 Cusp/Core problem: supernovae feedback versus the baryonic clumps and dynamical friction model
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• Search for 511 keV Emission in Satellite Galaxies of the Milky Way with INTEGRAL/SPI
• Osaka Feedback Model: Isolated Disk Galaxy Simulations
• The hot circumgalactic medium in the eROSITA All-Sky Survey I. X-ray surface brightness profiles
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• AGN feedback, quiescence and CGM metal enrichment in early-type galaxies
• Scaling relations and baryonic cycling in local star-forming galaxies: II. Gas content and star-formation efficiency
• The simplest model of galaxy formation I: A formation history model of galaxy stellar mass growth
• An analytical model for galaxy metallicity: What do metallicity relations tell us about star formation and outflow?
• The New Galaxy Evolution Paradigm Revealed by the Herschel Surveys
• Two Growing Modes and the Morphology-Quiescence Relation in Galaxies
• The Strikingly Similar Relation between Satellite and Central Galaxies and Their Dark Matter Halos Since z=2
• The evolution of clustering length, large-scale bias and host halo mass at 2<z<5 in the VIMOS Ultra Deep Survey (VUDS)
• Hot phase generation by supernovae: resolution, chemistry and thermal conduction
• The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type: A tracer of globular cluster formation and evolution
• On the intermediate-redshift central stellar mass-halo mass relation, and implications for the evolution of the most massive galaxies since z~1
• An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift $1\le z\le 9$
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• Deep MUSE observations in the HDFS. Morpho-kinematics of distant star-forming galaxies down to $10^8$M${}_{\odot }$
• Constraints on the circumburst environments of short gamma-ray bursts
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• Cosmological baryon transfer in the SIMBA simulations
• Evolution of Star-forming Galaxies from z = 0.7 to 1.2 with eBOSS Emission-line Galaxies
• On the origin of the mass-metallicity gradient relation in the local Universe
• A Preferential Growth Channel for Supermassive Black Holes in Elliptical Galaxies at z<2
• First results from the VIRIAL survey: the stellar content of $UVJ$-selected quiescent galaxies at $1.5<z<2$ from KMOS
• MHONGOOSE -- A MeerKAT Nearby Galaxy HI Survey
• Signatures of stellar accretion in MaNGA early-type galaxies
• A constant characteristic volume density of dark matter haloes from SPARC rotation curve fits
• The origin of the mass scales for maximal star formation efficiency and quenching: the critical role of Supernovae
• Millimeter mapping at z~1: dust-obscured bulge building and disk growth
• The bias of DLAs at z ~ 2.3: contraining stellar feedback in shallow potential wells
• Beyond halo mass: quenching galaxy mass assembly at the edge of filaments
• Modeling the Baryon Cycle in Low Mass Galaxy Encounters: the Case of NGC 4490 & NGC 4485
• Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations
• The combined effect of AGN and supernovae feedback in launching massive molecular outflows in high-redshift galaxies
• A tale of two sites -- II: Inferring the properties of minihalo-hosted galaxies with upcoming 21-cm interferometers
• A machine learning approach to mapping baryons onto dark matter haloes using the EAGLE and C-EAGLE simulations
• Stellar orbits in cosmological galaxy simulations: the connection to formation history and line-of-sight kinematics
• Black Hole Growth and Feedback in Isolated Romulus25 Dwarf Galaxies
• The highest-speed local dark matter particles come from the Large Magellanic Cloud
• The Stellar Mass, Star Formation Rate and Dark Matter Halo Properties of LAEs at $z\sim 2$
• New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
• Momentum-driven Winds from Radiatively Efficient Black Hole Accretion and Their Impact on Galaxies
• The evolution of the stellar mass versus halo mass relationship
• From Diversity to Dichotomy, and Quenching: Milky-Way-Like and Massive-Galaxy Progenitors at 0.5<z<3.0
• Timing the evolution of quiescent and star-forming local galaxies
• The Origin of r-process Enhanced Metal-Poor Halo Stars In Now-Destroyed Ultra-Faint Dwarf Galaxies
• The Immitigable Nature of Assembly Bias: The Impact of Halo Definition on Assembly Bias
• Evidences against cuspy dark matter halos in large galaxies
• A Break in Spiral Galaxy Scaling Relations at the Upper Limit of Galaxy Mass
• Formation of disk galaxies in preheated media: a preventative feedback model
• Rotation Curve Decomposition for Size-Mass Relations of Bulge, Disk, and Dark Halo in Spiral Galaxies
• Integral-Field Spectroscopy of Fast Outflows in Dwarf Galaxies with AGN
• Equilibrium model prediction for the scatter in the star-forming main sequence
• The LBT Satellites of Nearby Galaxies Survey (LBT-SONG): The Satellite Population of NGC 628
• Simple halo model formalism for the cosmic infrared background and its correlation with the thermal Sunyaev Zel'dovich effect
• A Deficit of Dark Matter from Jeans Modeling of the Ultra-diffuse Galaxy NGC 1052-DF2
• The Cluster-EAGLE project: velocity bias and the velocity dispersion - mass relation of cluster galaxies
• Warm FIRE: Simulating Galaxy Formation with Resonant Sterile Neutrino Dark Matter
• Halo Histories vs. Galaxy Properties at z=0, I: The Quenching of Star Formation
• Formation of the largest galactic cores through binary scouring and gravitational wave recoil
• Magellanic satellites in $\Lambda$CDM cosmological hydrodynamical simulations of the Local Group
• NIHAO -- XXV. Convergence in the cusp-core transformation of cold dark matter haloes at high star formation thresholds
• X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
• A semi-analytic study of self-interacting dark-matter haloes with baryons
• Baryon effects on void statistics in the EAGLE simulation
• Cold or Warm? Constraining Dark Matter with Primeval Galaxies and Cosmic Reionization after Planck
• Revisiting the bulge-halo conspiracy I: Dependence on galaxy properties and halo mass
• Dark matter stripping in galaxy clusters: a look at the Stellar to Halo Mass relation in the Illustris simulation
• On stellar mass loss from galaxies in groups and clusters
• Introducing galactic structure finder: the multiple stellar kinematic structures of a simulated Milky Way mass galaxy
• Creating a galaxy lacking dark matter in a dark matter dominated universe
• The Morphology-Density-Relation: Impact on the Satellite Fraction
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• The FRB20190520B Sightline Intersects Foreground Galaxy Clusters
• Simulating disc galaxy bulges that are consistent with observed scaling relations
• The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS
• The diverse formation histories of simulated disc galaxies
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• Where did the globular clusters of the Milky Way form? Insights from the E-MOSAICS simulations
• The Mass Profile of the Milky Way to the Virial Radius from the Illustris Simulation
• The Role of Cold Flows and Reservoirs in Galaxy Formation With Strong Feedback
• Search for Gamma-ray Emission from Dark Matter Annihilation in the Small Magellanic Cloud with the Fermi Large Area Telescope
• Is there enough star formation in simulated protoclusters?
• Constraining the last 7 billion years of galaxy evolution in semi-analytic models
• Matching the Evolution of the Stellar Mass Function Using Log-normal Star Formation Histories
• Constraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison
• NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite
• The clustering of radio galaxies: biasing and evolution versus stellar mass
• The Incomplete Conditional Stellar Mass Function: Unveiling the Stellar Mass Functions of Galaxies at 0.1 < Z < 0.8 from BOSS Observations
• MUSEQuBES: Characterizing the circumgalactic medium of redshift $\approx 3.3$ Ly$\alpha$ emitters
• Thermal Instability of Halo Gas Heated by Streaming Cosmic Rays
• The star formation history of Eridanus II: on the role of SNe feedback in the quenching of ultra-faint dwarf galaxies
• NIHAO XVI: The properties and evolution of kinematically selected discs, bulges and stellar haloes
• Jet-driven AGN feedback on molecular gas and low star-formation efficiency in a massive local spiral galaxy with bright X-ray halo
• The kinematics of massive quiescent galaxies at $1.4<z<2.1$: dark matter fractions, IMF variation, and the relation to local early-type galaxies
• Galaxies Probing Galaxies in PRIMUS - II. The Coherence Scale of the Cool Circumgalactic Medium
• The Main Sequence and the Fundamental Metallicity Relation in MaGICC Galaxies: Evolution and Scatter
• A new astrophysical solution to the Too Big To Fail problem - Insights from the MoRIA simulations
• Overdensity of submillimeter galaxies around the $z\simeq 2.3$ MAMMOTH-1 nebula
• The emergence of dark matter-deficient ultra-diffuse galaxies driven by scatter in the stellar mass-halo mass relation and feedback from globular clusters
• The edge of galaxy formation II: evolution of Milky Way satellite analogues after infall
• Central galaxies in different environments: Do they have similar properties?
• The radial acceleration relation in galaxy clusters
• A parametric study of possible solutions to the high-redshift overproduction of stars in modeled dwarf galaxies
• A Statistical Semi-Empirical Model: Satellite galaxies in Groups and Clusters
• Observed trend in the star formation history and the dark matter fraction of galaxies at redshift $z\approx 0.8$
• Modeling for Stellar Feedback in Galaxy Formation Simulations
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• FLIMFLAM DR1: The First Constraints on the Cosmic Baryon Distribution from 8 FRB sightlines
• HectoMAP and Horizon Run 4: Dense Structures and Voids in the Real and Simulated Universe
• Constraints on the evolution of the relationship between HI mass and halo mass in the last 12 Gyr
• Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
• Statistics of galaxy mergers: bridging the gap between theory and observation
• Does the Galaxy-Halo Connection Vary with Environment?
• Intensity mapping with neutral hydrogen and the Hidden Valley simulations
• Dust in the Wind: Composition and Kinematics of Galaxy Outflows at the Peak Epoch of Star Formation
• The New Numerical Galaxy Catalog (${\nu }^2$GC): An Updated Semi-analytic Model of Galaxy and AGN with Large Cosmological N-body Simulation
• Gaia-DR2 extended kinematical maps. Part II: Dynamics in the Galactic disk explaining radial and vertical velocities
• RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars
• Dark Matter Trapping by Stellar Bars: The Shadow Bar
• Brightest Cluster Galaxies in Cosmological Simulations with Adaptive Mesh Refinement: Successes and Failures
• The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
• Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
• Formation channels of slowly rotating early-type galaxies
• Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
• Lyman-αabsorption beyond the disk of simulated spiral galaxies
• Stellar Mass-to-light Ratios: Composite Bulge+Disk Models and the Baryonic Tully-Fisher Relation
• The Impact of Environment on the Stellar Mass - Halo Mass Relation
• Metal line emission from galaxy haloes at z~1
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• Discovery of a Quadruple Lens in CANDELS with a Record Lens Redshift z=1.53
• A Galaxy Redshift Survey near HST/COS AGN Sight Lines
• The impact of baryonic potentials on the gravothermal evolution of self-interacting dark matter haloes
• Dark MaGICC: the effect of Dark Energy on galaxy formation. Cosmology does matter
• A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The $(v_{\max },M_{\mathrm{DM}})$-$({\sigma }_0,M_{\mathrm{BH}},\varphi )$ Relations
• Globular Clusters Formed within Dark Halos I: present-day abundance, distribution and kinematics
• Hubble Space Telescope Observations of Two Faint Dwarf Satellites of Nearby LMC Analogs from MADCASH
• Dark matter halos and scaling relations of extremely massive spiral galaxies from extended HI rotation curves
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• Tidal Stripping in the Adiabatic Limit
• The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
• 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
• Compaction-Driven Black Hole Growth
• Origins of Scatter in the Relationship Between HCN 1-0 and Dense Gas Mass in the Galactic Center
• The stellar mass - halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z~3
• The VIMOS Ultra Deep Survey. Luminosity and stellar mass dependence of galaxy clustering at z~3
• The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields
• The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
• Formation and settling of a disc galaxy during the last 8 billion years in a cosmological simulation
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Tidal destruction in a low mass galaxy environment: the discovery of tidal tails around DDO 44
• Stellar-to-halo mass relation of cluster galaxies
• Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations
• Constraining the Warm Dark Matter Particle Mass through Ultra-Deep UV Luminosity Functions at z=2
• What's in a name? Quantifying the interplay between the Definition, Orientation, and Shape of Ultra-diffuse Galaxies Using the Romulus Simulations
• MaGICC-WDM: the effects of warm dark matter in hydrodynamical simulations of disc galaxy formation
• Evaporation of planetary atmospheres due to XUV illumination by quasars
• Supernovae feedback propagation: the role of turbulence
• Cosmic CARNage I: on the calibration of galaxy formation models
• Constraints on Chameleon f(R)-Gravity from Galaxy Rotation Curves of the SPARC Sample
• The central spheroids of Milky Way mass-sized galaxies
• The Pandora project. I: the impact of radiation and cosmic rays on baryonic and dark matter properties of dwarf galaxies
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Simulating the Spatial Distribution and Kinematics of Globular Clusters within Galaxy Clusters in Illustris
• Cross-calibration of CO- vs dust-based gas masses and assessment of the dynamical mass budget in Herschel-SDSS Stripe82 galaxies
• The angular momentum of disc galaxies at z=1
• Cool circumgalactic gas of passive galaxies from cosmological inflow
• Powerful quasar outflow in a massive disc galaxy at $z\sim 5$
• Gas flows in the circumgalactic medium around simulated high-redshift galaxies
• MaNGA DynPop -- III. Stellar dynamics versus stellar population relations in 6000 early-type and spiral galaxies: Fundamental Plane, mass-to-light ratios, total density slopes, and dark matter fractions
• Simulating the H2 content of high-redshift galaxies
• Modelling of Lyman-alpha Emitting Galaxies and Ionized Bubbles at the Era of Reionization
• $\Lambda$CDM Predictions for the Satellite Population of M33
• Using Galaxy Pairs to Probe Star Formation During Major Halo Mergers
• Stars behind bars II: A cosmological formation scenario for the Milky Way's central stellar structure
• The role of massive halos in the Star Formation History of the Universe
• The Mass Dependance of Satellite Quenching in Milky Way-like Halos
• NIHAO III: The constant disc gas mass conspiracy
• GA-NIFS: Multi-phase analysis of a star-forming galaxy at $z\sim 5.5$
• On the (Lack of) Evolution of the Stellar Mass Function of Massive Galaxies from $z$=1.5 to 0.4
• The cosmic web of X-ray active galactic nuclei seen through the eROSITA Final Equatorial Depth Survey (eFEDS)
• The Observed Evolution of the Stellar Mass - Halo Mass Relation for Brightest Central Galaxies
• Distribution of streaming rates into high-redshift galaxies
• Gas Accretion Can Drive Turbulence in Galaxies
• The mass accretion rate of galaxy clusters: a measurable quantity
• The impact of the Large Magellanic Cloud on dark matter direct detection signals
• Forward Modeling of Double Neutron Stars: Insights from Highly-Offset Short Gamma-Ray Bursts
• How AGN feedback drives the size growth of the first quasars
• ELUCID V. Lighting dark matter halos with galaxies
• An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
• The distribution of satellites around massive galaxies at 1<z<3 in ZFOURGE/CANDELS: dependence on star formation activity
• On Physical Scales of Dark Matter Halos
• Stellar feedback from HMXBs in cosmological hydrodynamical simulations
• Sensitivity of dark matter haloes to their accretion histories
• Discovery of a Strong Lensing Galaxy Embedded in a Cluster at z = 1.62
• The MillenniumTNG Project: The large-scale clustering of galaxies
• NIHAO XXIV: Rotation or pressure supported systems? Simulated Ultra Diffuse Galaxies show a broad distribution in their stellar kinematics
• The imprint of dark matter haloes on the size and velocity dispersion evolution of early-type galaxies
• ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
• The missing dwarf galaxies of the Local Group
• Orbital dynamics and histories of satellite galaxies around Milky Way-mass galaxies in the FIRE simulations
• Revisiting the Size-Luminosity Relation in the Era of Ultra Diffuse Galaxies
• Entropy Driven Winds: Outflows and Fountains Lifted Gently by Buoyancy
• The growth of galactic bulges through mergers in LCDM haloes revisited. II. Morphological mix evolution
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Simba: The average properties of the circumgalactic medium of $2\le z\le 3$ quasars are determined primarily by stellar feedback
• Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE
• High resolution near-infrared imaging of submillimeter galaxies
• A unified model for the clustering of quasars and galaxies at $z\approx 6$
• Cosmic evolution of bars in simulations of galaxy formation
• The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
• Characterising the Intracluster Light over the Redshift Range $0.2<z<0.8$ in the DES-ACT Overlap
• The Next Generation Virgo Cluster Survey. IX. Estimating the Efficiency of Galaxy Formation on the Lowest-Mass Scales
• Compact Starburst Galaxies with Fast Outflows: Central Escape Velocities and Stellar Mass Surface Densities from Multi-band Hubble Space Telescope Imaging
• From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• Constraining AGN triggering mechanisms through the clustering analysis of active black holes
• Growth of Supermassive Black Hole Seeds in ETG Star-Forming Progenitors: Multiple Merging of Stellar Compact Remnants via Gaseous Dynamical Friction and Gravitational Wave Emission
• On the early evolution of Local Group dwarf galaxy types: star formation and supernova feedback
• The phantom dark matter halos of the Local Volume in the context of modified Newtonian dynamics
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• Effects of the environment on galaxies in the Catalogue of Isolated Galaxies: physical satellites and large scale structure
• UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
• Constraining the Milky Way halo kinematics via its Linear Response to the Large Magellanic Cloud
• A Deep Search for Faint Galaxies Associated with Very Low-Redshift C IV Absorbers: A Case with Cold-Accretion Characteristics
• Scaling relations and baryonic cycling in local star-forming galaxies. III. Outflows, effective yields and metal loading factors
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• A first estimate of the Milky Way dark matter halo spin
• Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation
• Dark influences III. Structural characterization of minor mergers of dwarf galaxies with dark satellites
• A Fundamental Test for Galaxy Formation Models: Matching the Lyman-$\alpha$ Absorption Profiles of Galactic Halos over Three Decades in Distance
• Cosmological simulations of Milky Way-sized galaxies
• Testing the Relationship Between Bursty Star Formation and Size Fluctuations of Local Dwarf Galaxies
• Evidence for a Massive Andromeda Galaxy Using Satellite Galaxy Proper Motions
• SHAM through the lens of a hydrodynamical simulation
• A Search for Satellite Galaxies of Nearby Star-Forming Galaxies with Resolved Stars in LBT-SONG
• ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System
• Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
• Construct the emission line galaxy-host halo connection through auto and cross correlations
• Galaxy Flybys: Evolution of the Bulge, Disk, and Spiral Arms
• Measuring the delay time distribution of binary neutron stars. I. Through Scaling Relations of the Host Galaxies of Gravitational Wave Events
• Generating Synthetic Cosmological Data with GalSampler
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Brightest Group Galaxies: Stellar Mass and Star Formation Rate (paper I)
• Charting the main sequence of star-forming galaxies out to redshifts z<5.7
• The halo mass function of late-type galaxies from HI kinematics
• A hidden population of massive black holes in simulated dwarf galaxies
• The interplay between feedback, accretion, transport and winds in setting gas-phase metal distribution in galaxies
• Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Orbital decay of Globular Clusters in the galaxy with little dark matter
• Simulations of isolated dwarf galaxies formed in dark matter halos with different mass assembly histories
• Beyond Ultra-diffuse Galaxies. I. Mass--Size Outliers among the Satellites of Milky Way Analogs
• Testing Galaxy Quenching Theories with Scatter in the Stellar to Halo Mass Relation
• 21cmfish: Fisher-matrix framework for fast parameter forecasts from the cosmic 21-cm signal
• Systematic uncertainties from halo asphericity in dark matter searches
• The Thermal Sunyaev-Zel'dovich Effect from Massive, Quiescent 0.5 $\le$ z $\le$ 1.5 Galaxies
• Building robust AGN mock catalogs to unveil black hole evolution and for survey planning
• Photometric Objects around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. I. Methods
• The neutral hydrogen distribution in large-scale haloes from 21-cm intensity maps
• The origin of X-ray coronae around simulated disc galaxies
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• A scenario for ultra-diffuse satellite galaxies with low velocity dispersions: the case of [KKS 2000]04
• Towards a higher mass for NGC1052-DF2: an analysis based on full distribution functions
• Formation of globular clusters with multiple stellar populations from massive gas clumps in high-z gas-rich dwarf galaxies
• Galaxy Evolution at High Redshift: Obscured Star Formation, GRB Rates, Cosmic Reionization, and Missing Satellites
• Chemical evolution of giant molecular clouds in simulations of galaxies
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Exploring the dependence of the three-point correlation function on stellar mass and luminosity at 0.5<z<1.1
• On the Kinematics of Cold, Metal-enriched Galactic Fountain Flows in Nearby Star-forming Galaxies
• Keck Spectroscopy of the Coma Cluster Ultra-Diffuse Galaxy Y358: Dynamical Mass in a Wider Context
• How the first stars shaped the faintest gas-dominated dwarf galaxies
• The Effect of Adiabatic Compression on Dark Matter Halos and the Radial Acceleration Relation
• SH$\alpha$DE: Survey description and mass-kinematics scaling relations for dwarf galaxies
• Galaxy properties in the cosmic web of EAGLE simulation
• A high baryon fraction in massive haloes at z~3
• The stellar mass in and around isolated central galaxies: connections to the total mass distribution through galaxy-galaxy lensing in the Hyper Suprime-Cam survey
• The survival of globular clusters in a cuspy Fornax
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Dark influences II: gas and star formation in minor mergers of dwarf galaxies with dark satellites
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• Strong lensing with superfluid dark matter
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• Cosmology with velocity dispersion counts: an alternative to measuring cluster halo masses
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• AGN and Dwarf Galaxy Gas Kinematics
• Discovery of a red backsplash galaxy candidate near M81
• LoCuSS: The Near-Infrared Luminosity and Weak-Lensing Mass Scaling Relation of Galaxy Clusters
• The buildup of galaxies and their spheroids: the contributions of mergers, disc instabilities and star formation
• Galaxy size trends as a consequence of cosmology
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• Incorporating baryon-driven contraction of dark matter halos in rotation curve fits
• Circumnuclear Media of Quiescent Supermassive Black Holes
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• TRINITY II: The Luminosity-dependent Bias of the Supermassive Black Hole Mass--Galaxy Mass Relation for Bright Quasars at $z=6$
• Unraveling the interplay between SIDM and baryons in MW halos: defining where baryons dictate heat transfer
• The dominant origin of diffuse Ly$\alpha$ halos around LAEs explored by SED fitting and clustering analysis
• Galaxy morphoto-Z with neural Networks (GaZNets). I. Optimized accuracy and outlier fraction from Imaging and Photometry
• CAVITY, Calar Alto Void Integral-field Treasury surveY and project extension
• BASS. XXXVI. Constraining the Local Supermassive Black Hole - Halo Connection with BASS DR2 AGN
• From spirals to lenticulars: evidence from the rotation curves and mass models of three early-type galaxies
• Local photoionization feedback effects on galaxies
• The Case for Strangulation in Low-Mass Hosts: DDO 113
• Effects of feedback on galaxies in the VELA simulations: elongation, clumps and compaction
• Dark influences: imprints of dark satellites on dwarf galaxies
• The present-day gas content of simulated field dwarf galaxies
• The baryon cycle of Seven Dwarfs with superbubble feedback
• Navarro-Frenk-White dark matter profile and the dark halos around disk systems
• Galactic winds - How to launch galactic outflows in typical Lyman-break galaxies
• Some observational tests of a minimal galaxy formation model
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Hierarchical scaling and biasing
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• The evolution of star formation activity in galaxy groups
• Similarities and uniqueness of Ly$\alpha$ emitters among star-forming galaxies at z=2.5
• The changing circumgalactic medium over the last 10 Gyr I: physical and dynamical properties
• Evolution of the Gas Mass Fraction of Progenitors to Today's Massive Galaxies: ALMA Observations in the CANDELS GOODS-S Field
• Mass and size growth of early-type galaxies by dry mergers in cluster environments
• Reignited star formation in dwarf galaxies quenched during reionization
• Tracing the Local Volume galaxy halo-to-stellar mass ratio with satellite kinematics
• Halo Histories vs. Galaxy Properties at z=0, III: The Properties of Star-Forming Galaxies
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• Morphology of galaxies with quiescent recent assembly history in a Lambda-CDM universe
• Magnetogenesis at Cosmic Dawn: Tracing the Origins of Cosmic Magnetic Fields
• Measuring Dark Matter in Galaxies: The Mass Fraction Within 5 Effective Radii
• Stars on the edge: Galactic tides and the outskirts of the Sculptor dwarf spheroidal
• Bar ages derived for the first time in nearby galaxies: Insights on secular evolution from the TIMER sample
• EDGE: Dark matter core creation depends on the timing of star formation
• Setting firmer constraints on the evolution of the most massive, central galaxies from their local abundances and ages
• Cosmic Outliers: Low-Spin Halos Explain the Abundance, Compactness, and Redshift Evolution of the Little Red Dots
• Mufasa:The strength and evolution of galaxy conformity in various tracers
• Quantifying the Origin and Distribution of Intracluster Light in a Fornax-like Cluster
• The Black Hole Mass Function Across Cosmic Times II. Heavy Seeds and (Super)Massive Black Holes
• Revisiting the bulge-halo conspiracy II: Towards explaining its puzzling dependence on redshift
• 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
• Predicting fully self-consistent satellite richness, galaxy growth and starformation rates from the STastical sEmi-Empirical modeL STEEL
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• A new class of dark matter-free dwarf galaxies? I. Clues from FCC 224, NGC 1052-DF2 and NGC 1052-DF4
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• The edge of galaxy formation III: The effects of warm dark matter on Milky Way satellites and field dwarfs
• The Impact of Environment on Late Time Evolution of the Stellar Mass - Halo Mass Relation
• The Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties
• Dependence of galaxy clustering on UV-luminosity and stellar mass at $z\sim 4-7$
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• The Robustness of Cosmological Hydrodynamic Simulation Predictions to Changes in Numerics and Cooling Physics
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z<1.3
• A Study of Central Galaxy Rotation with Stellar Mass and Environment
• PANORAMIC: Discovery of an Ultra-Massive Grand-Design Spiral Galaxy at $z\sim 5.2$
• The Differing Relationships Between Size, Mass, Metallicity and Core Velocity Dispersion of Central and Satellite Galaxies
• Energy transfer from baryons to dark matter as a unified solution to small-scale structure issues of the $\Lambda$CDM model
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. III. Accurate Measurement of Galaxy Stellar Mass Function with the Aid of Cosmological Redshift Surveys
• On the Impact of Neutron Star Binaries Natal-Kick Distribution on the Galactic r-process Enrichment
• Late Bloomer Galaxies: Growing Up in Cosmic Autumn
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• Normalized additional velocity distribution: testing the radial profile of dark matter halos and MOND
• MUSEQuBES: The relation between Ly$\alpha$ emitters and C IV absorbers at $z\approx 3.3$
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
• The tidal evolution of the Fornax dwarf spheroidal and its globular clusters
• Kinematics and Mass Distributions for Non-Spherical Deprojected Sérsic Density Profiles and Applications to Multi-Component Galactic Systems
• WISDOM Project -- XIII. Feeding molecular gas to the supermassive black hole in the starburst AGN-host galaxy Fairall 49
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
• A shallow dark matter halo in Ultra Diffuse Galaxy AGC 242019: are UDGs structurally similar to low surface brightness galaxies?
• Not-so-little Red Dots: Two massive and dusty starbursts at z~5-7 pushing the limits of star formation discovered by JWST in the COSMOS-Web survey
• The frequency of very young galaxies in the local Universe: II. The view from SDSS spectra
• Stellar Kinematics and Environment at z~0.8 in the LEGA-C Survey: Massive, Slow-Rotators are Built First in Overdense Environments
• 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 $z<0.7$
• How feedback shapes galaxies: an analytic model
• A Precise Benchmark for Cluster Scaling Relations: Fundamental Plane, Mass Plane and IMF in the Coma Cluster from Dynamical Models
• The Properties of Radio and Mid-infrared Detected Galaxies and the Effect of Environment on the Co-evolution of AGN and Star Formation at $z\sim 1$
• Bulge formation through disc instability -- I
• A minimal empirical model for the cosmic far-infrared background anisotropies
• Star formation in mergers with cosmologically motivated initial conditions
• Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys
• AGN must be very efficient at powering outflows
• Differentiable Predictions for Large Scale Structure with SHAMNet
• The Luminosity Functions and Redshift Evolution of Satellites of Low-Mass Galaxies in the COSMOS Survey
• Constraining Scatter in the Stellar Mass--Halo Mass Relation for Haloes Less Massive than the Milky Way
• Constraining warm dark matter mass with cosmic reionization and gravitational wave
• Dwarf galaxies as a probe of a primordially magnetized Universe
• Testing galaxy formation models with galaxy stellar mass functions
• Effect of primordial non-Gaussianities on the far-UV luminosity function of high-redshift galaxies: implications for cosmic reionization
• A Holistic Review of a Galactic Interaction
• Modelling the formation of today's massive ellipticals
• The Origin of the Relation Between Stellar Angular Momentum and Stellar Mass in Nearby Disk-dominated galaxies
• Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation
• Mechanical feedback from stellar winds with an application to galaxy formation at high redshift
• The Galaxy Replacement Technique (GRT): a New Approach to Study Tidal Stripping and Formation of Intracluster Light in a Cosmological Context
• On the dark matter haloes inner structure and galaxy morphology
• Cosmic evolution of the H2 mass density and the epoch of molecular gas
• Spatially Resolved Gas-phase Metallicity in FIRE-2 Dwarfs: Late-Time Evolution of Metallicity Relations in Simulations with Feedback and Mergers
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• A systematic study of the inner rotation curves of galaxies observed as part of the GASS and COLD GASS surveys
• On the Edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies
• What has quenched the massive spiral galaxies?
• MHONGOOSE discovery of a gas-rich low-surface brightness galaxy in the Dorado Group
• Satellite content and quenching of star formation in galaxy groups at z~1.8
• Self-gravitating Equilibria of Non-minimally Coupled Dark Matter Halos
• The Clustering of Undetected High-redshift Black Holes and Their Signatures in Cosmic Backgrounds
• Light or heavy supermassive black hole seeds: the role of internal rotation in the fate of supermassive stars
• The CGM-GRB Study. I. Uncovering The CircumGalactic Medium around GRB hosts at redshifts 2-6
• Constraining the subgrid physics in simulations of isolated dwarf galaxies
• HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy
• Accurate Computation of the Screening of Scalar Fifth Forces in Galaxies
• Dark Matter in Fractional Gravity I: Astrophysical Tests on Galactic Scales
• The XMM-Newton Wide Field Survey in the COSMOS Field: Clustering Dependence of X-ray Selected AGN on Host Galaxy Properties
• A universal angular momentum profile for dark matter haloes
• A new gas cooling model for semi-analytical galaxy formation models
• HI within and around observed and simulated galaxy discs -- Comparing MeerKAT observations with mock data from TNG50 and FIRE-2
• Recent progress in simulating galaxy formation from the largest to the smallest scales
• The quenched mass portion of star-forming galaxies and the origin of the star formation sequence slope
• Selecting ultra-faint dwarf candidate progenitors in cosmological N-body simulations at high redshifts
• Simulating Deep Hubble Images With Semi-empirical Models of Galaxy Formation
• Around the Spindle galaxy: the dark halo mass of NGC3115
• Dark matter fraction of low-mass cluster members probed by galaxy-scale strong lensing
• A too-many dwarf galaxy satellites problem in the M83 group
• Ironing the folds: The phase space chevrons of a GSE-like merger as a dark matter subhalo detector
• Exploring Self-Interacting Dark Matter Halos with Diverse Baryonic Distributions: A Parametric Approach
• Applying Noether's theorem to matter in the Milky Way: evidence for external perturbations and non-steady-state effects from Gaia Data Release 2
• Shutting down or powering up a (U)LIRG? Merger components in distinctly different evolutionary states in IRAS 19115-2124 (The Bird)
• Galaxy growth from redshift 5 to 0 at fixed comoving number density
• Probing the Diffuse Lyman-alpha Emission on Cosmological Scales: Lyα Emission Intensity Mapping Using the Complete SDSS-IV eBOSS Survey
• The weak dependence of velocity dispersion on disk fractions, mass-to-light ratio and redshift: Implications for galaxy and black hole evolution
• Evolution of CIV Absorbers. II. Where does CIV live?
• Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies
• CGM${}^2$ $+$ CASBaH: The Mass Dependence of H~I Ly$\alpha$-Galaxy Clustering and the Extent of the CGM
• An empirical model to form and evolve galaxies in dark matter halos
• Age and metal gradients in massive quiescent galaxies at $0.6\lesssim z\lesssim 1.0$: implications for quenching and assembly histories
• Ages and metallicities of quiescent galaxies: confronting broadband ($UVJ$) colours with stellar absorption lines
• A Comparison of Outflow Properties in AGN Dwarfs vs. Star Forming Dwarfs
• Tracing the co-evolution path of super massive black holes and spheroids with AKARI-selected ultra-luminous IR galaxies at intermediate redshifts
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• The detection of ultra-faint low surface brightness dwarf galaxies in the Virgo Cluster: a Probe of Dark Matter and Baryonic Physics
• The Tail of Late-forming Dwarf Galaxies in $\Lambda$CDM
• A Two-Parameter Matching Scheme for Massive Galaxies and Dark Matter Haloes
• Abundance matching for low mass galaxies in the CDM and FDM models
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic survey. II. Morphology, Color and Size Dependences of the Stellar-halo Mass Relation for Massive Galaxies
• EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
• Empirical estimation of host galaxy dispersion measure towards well localized fast radio bursts
• The Fundamental Plane Relation of Early-Type Galaxies: Environmental Dependence
• Galaxy mass-size segregation in the cosmic web from the CAVITY parent sample
• Bursty Star Formation in Dwarfs is Sensitive to Numerical Choices in Supernova Feedback Models
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• The signal of decaying dark matter with hydrodynamical simulations
• Connection between galaxy morphology and dark-matter halo structure I: a running threshold for thin discs and size predictors from the dark sector
• The abundance and colours of galaxies in high redshift clusters in the cold dark matter cosmology
• Auriga Streams I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• A galactic outflow traced by its extended Mg II emission out to a $\sim 30$ kpc radius in the Hubble Ultra Deep Field with MUSE
• The Magellanic Clouds are very rare in the IllustrisTNG simulations
• The GMRT archive atomic gas survey -- II. Mass modelling and dark matter halo properties across late-type spirals
• Using KCWI to Explore the Chemical Inhomogeneities and Evolution of J1044+0353
• Disk galaxies are self-similar: the universality of the HI-to-Halo mass ratio for isolated disks
• Growth of Massive Black Hole Seeds by Migration of Stellar and Primordial Black Holes: Gravitational Waves and Stochastic Background
• GABE: Galaxy Assembly with Binary Evolution
• Gravity and the Nonlinear Growth of Structure in the Carnegie-Spitzer-IMACS Redshift Survey
• Damped Lyman-$\alpha$ absorbers and atomic hydrogen in galaxies: the view of the GAEA model
• Using large galaxy surveys to distinguish z~0.5 quiescent galaxy models
• Properties of the circumgalactic medium in simulations compared to observations
• The Stellar Mass - Halo Mass Relation for Low Mass X-ray Groups at 0.5<z<1 in the CDFS with CSI
• Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• 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
• Type Ia Supernova Magnitude Step from the local Dark Matter Environment
• MusE GAs FLOw and Wind (MEGAFLOW) XI. Scaling relations between outflows and host galaxy properties
• The Dark Matter Halos of HI Selected Galaxies
• Constraints on galaxy formation from the cosmic-far-infrared-background\,$-$\,optical-imaging cross-correlation using \textit{Herschel} and UNIONS
• Characterizing simulated galaxy stellar mass histories
• Search for Missing Links Between Two Extreme Wind Speed Profiles : Dark Energy Accretion and Adiabatic Fluid Accretion
• The impact of the halo spin-concentration relation on disc scaling laws
• Exploring galaxy dark matter halos across redshifts with strong quasar absorbers
• The Formation of a Milky Way-sized Disk Galaxy 1. A Comparison of Numerical Methods
• Mass-morphology relation of TNG50 galaxies
• A physically motivated galaxy size definition across different state-of-the-art hydrodynamical simulations
• Co-Evolution vs. Co-existence: The Effect of Accretion Modelling on the Evolution of Black Holes and Host Galaxies
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Accreting Black Holes in Dark Matter Halos
• Constraining dark matter annihilation with HSC Low Surface Brightness Galaxies
• NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
• From Gas to Stars Over Cosmic Time
• Early-type galaxy density profiles from IllustrisTNG: III. Effects on outer kinematic structure
• Globular Cluster Counts around 700 Nearby Galaxies
• MaNGA AGN dwarf galaxies (MAD) -- II. AGN outflows in dwarf galaxies
• A partial Lyman limit system tracing intragroup gas at $z\approx 0.8$ towards HE1003+0149
• A break in the high-redshift stellar mass Tully-Fisher relation
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
• Probing gaseous halos of galaxies with radio jets
• Abundance matching tested on small scales with galaxy dynamics
• The significant effects of stellar mass estimation on galaxy pair fractions
• Modeling the Cosmic Dispersion Measure in the D < 120 Mpc Local Universe
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• The Isophotal Structure of Star-forming Galaxies at $0.5<z<1.8$ in CANDELS: Implications for the Evolution of Galaxy Structure
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• The variation of the gas content of galaxy groups and pairs compared to isolated galaxies
• A physical model for the redshift evolution of high-z Lyman-Break Galaxies
• Toward a stellar population catalog in the Kilo Degree Survey: the impact of stellar recipes on stellar masses and star formation rates
• Dynamical Properties of Molecular-forming Gas Clumps in Galaxies at the Epoch of Reionization
• No Evolution in the Half-mass Radius of Milky Way-type Galaxies over the Last 10 Gyr
• An Escaping Outflow in a Galaxy with an Intermediate-mass Black Hole
• Shape noise and dispersion in precision weak lensing
• The properties and environment of very young galaxies in the local Universe
• The velocity function of dark matter halos at r=20 kpc: Remarkably little evolution since z ~ 4
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Predictions for Detecting a Turndown in the Baryonic Tully Fisher Relation
• AGN lifetimes in UV-selected galaxies: a clue to supermassive black hole-host galaxy coevolution
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies
• Decoupled Black Hole Accretion and Quenching: The Relationship Between BHAR, SFR, and Quenching in Milky Way and Andromeda-mass Progenitors Since z = 2.5
• MaNGA AGN dwarf galaxies (MAD). III. The role of mergers and environment in active galactic nucleus activity in dwarf galaxies
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• The dynamical impact of cosmic rays in the Rhea magnetohydrodynamics simulations
• Flattening of dark matter cusps during mergers: model of M31
• Globular Cluster Systems and X-Ray Atmospheres in Galaxies
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• Intertwined Formation of ${\mathrm{H}}_2$, Dust, and Stars in Cosmological Simulations
• The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data
• The galaxy counterpart of the high-metallicity and 16 kpc impact parameter DLA towards Q0918+1636 - a challenge to galaxy formation models?
• Galaxy-galaxy lensing in the VOICE deep survey
• Star formation and stellar & AGN feedback in the absence of accretion, not gas stripping, set the quenching timescale in satellite galaxies
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• An H$\alpha$ kinematic survey of the $Herschel$ Reference Survey -- I. Fabry-Perot observations with the 1.93m telescope at OHP
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Massive dusty multiphase outflow in local merger shows no sign of slowing on kiloparsec scales
• Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra-I cluster IV. A study of the Globular Cluster population in four UDGs
• The inflow and outflow rate evolution of local Milky Way-mass star-forming galaxies since z=1.3
• Clues to the nature of dark matter from first galaxies
• Galaxy kinematics across different environments in the RXJ1347-1145 cluster complex
• Modelling the selection of galaxy groups with end to end simulations
• Fundamental properties of the dark and the luminous matter from Low Surface Brightness discs
• The Milky Way in context: The formation of galactic discs and chemical sequences from a cosmological perspective
• Diving into dangerous tides: The impact of galaxy cluster tidal environments on satellite galaxy mass densities
• Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
• The SRG/eROSITA All-Sky Survey. The Weak-Lensing Mass Calibration and the Stellar Mass-to-Halo Mass Relation from the Hyper Suprime-Cam Subaru Strategic Program
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• Quenching vs. Quiescence: forming realistic massive ellipticals with a simple starvation model
• Spatial Distribution of OVI Covering Fractions in the Simulated Circumgalactic Medium
• Predicting HCN, HCO${}^{+}$, multi-transition CO, and dust emission of star-forming galaxies -- Extension to luminous infrared galaxies and the role of cosmic ray ionization
• MaNGA DynPop. VII. A Unified Bulge-Disk-Halo Model for Explaining Diversity in Circular Velocity Curves of 6000 Spiral and Early-Type Galaxies
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn
• IllustrisTNG + Cosmic Rays with a Simple Transport Model: From Dwarfs to L${}^{\star }$ Galaxies
• Modelling the Evolution of Ly$\alpha$ Blobs and Ly$\alpha$ Emitters
• Hubble Space Telescope Captures UGC~12591: Bulge/Disc Properties, Star Formation and `Missing Baryons' Census in a Very Massive and Fast Spinning Hybrid Galaxy
• Cosmological prior for the $J$-factor estimation of dwarf spheroidal galaxies
• Improving photometric redshifts with Ly$\alpha$ tomography
• A path towards constraining the evolution of the interstellar medium and outflows in the Milky Way using APOGEE
• LATIS: Comparing Galaxy and IGM Tomography Maps as Tracers of Large-scale Structure and Protoclusters at $z\sim 2.5$
• Associations of dwarf galaxies in a $\Lambda$CDM Universe
• Impact of supermassive black hole growth on star formation
• The "Little Dark Dot": Evidence for Self-interacting Dark Matter in the Strong Lens SDSS J0946+1006?
• Deciphering Baryonic Feedback from ACT tSZ Galaxy Clusters
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations -- II. Constraining cosmology and astrophysical processes with early- and late-type galaxies
• Neutral hydrogen in the post-reionization universe
• How do the dynamics of the Milky Way -- Large Magellanic Cloud system affect gamma-ray constraints on particle dark matter?
• Improved SED-Fitting Assumptions Result in Inside-Out Quenching at $z\sim 0.5$ and Quenching at All Radii Simultaneously at $z\sim 1$
• A Shallow Slope for the Stellar Mass--Angular Momentum Relation of Star-Forming Galaxies at $1.5<z<2.5$
• Tracing the cosmological origin of gas that fuels in situ star formation in TNG50 galaxies
• A Recent Starbust in the Low Surface Brightness Galaxy UGC 628
• Barions and $\Lambda$CDM Model Problems
• The origin of galaxy colour bimodality in the scatter of the Stellar-to-Halo Mass Relation
• SEMPER I. Radio Predictions for Star-Forming Galaxies at $0<z<5$
• Mapping luminous and dark matter in the Universe
• The environmental dependence of the stellar mass fundamental plane of early-type galaxies
• HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
• Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies
• Exploring Milky Way rotation curves with Gaia DR3: a comparison between $\Lambda$CDM, MOND, and General Relativistic approaches
• A Bending in the Size-mass Relation of Star-forming Galaxies across $0.5<z<6.0$ at a Critical Stellar Mass of $10^{10}{M}_{\odot }$ Revealed by JWST
• The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
• Updated Models for the Creation of a Low-z QSO Absorber by a Dwarf Galaxy Wind
• Estimating the contribution of foreground halos to the FRB 180924 dispersion measure
• Measuring the Stellar-to-Halo Mass Relation at $\sim 10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses
• Magnetic fields in galactic environments probed by Fast Radio Bursts
• AGN with massive black holes have closer galactic neighbors: k-Nearest-Neighbor statistics of an unbiased sample of AGN at z~0.03
• An Enhanced Isothermal Jeans Approach to Constraining Dark Matter Self-Interactions from Galactic Kinematics
• Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses
• Bridging Simulations and Observations: New Insights into Galaxy Formation Simulations via Out-of-Distribution Detection and Bayesian Model Comparison
• The Role of Mass and Environment on Satellite distributions around Milky Way analogs in the Romulus25 simulation
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• Probing baryonic feedback with fast radio bursts: joint analyses with cosmic shear and galaxy clustering
• The Origin of the Gas and Its Low Star Formation Efficiency in Quiescent Galaxies
• The Lowest Metallicity Stars in the LMC: Clues from MaGICC Simulations
• Reconstructing the mass accretion histories of nearby Red Nuggets with their globular cluster systems
• Gas thermodynamics meets galaxy kinematics: Joint mass measurements for eROSITA galaxy clusters
• Extended Hernquist-Springel formalism for cosmic star formation
• Recoiling supermassive black holes in analytical and numerical galaxy potential
• JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations
• Photometric Objects Around Cosmic Webs (PAC). VI. High Satellite Fraction of Quasars
• How Many Bursts Does it Take to Form a Core at the Center of a Galaxy?
• Baryon-driven decontraction in Milky Way mass haloes
• Mapping the Distorted Dark Matter Distribution of the LMC-SMC System Prior to Milky Way Infall with Basis Function Expansions
• Probabilistic Inference of the Structure and Orbit of Milky Way Satellites with Semi-Analytic Modeling
• The odd primordial halo of the Milky Way implied by Gaia. A shallow core, but a steep decline
• Clustering properties of TGSS radio sources
• The satellite population around luminous red galaxies in the 25 square degree DESI Legacy Imaging Surveys Early Data Release
• On the Tidal Formation of Dark Matter Deficient Galaxies
• Cross-checking SMBH mass estimates in NGC 6958 -- I: Stellar dynamics from adaptive optics-assisted MUSE observations
• The tidal evolution of satellite galaxies in cosmological simulations: insights from COLIBRE
• The NIKA2 cosmological legacy survey at 2 mm: catalogs, colors, redshift distributions, and implications for deep surveys
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• Challenges of standard halo models in constraining galaxy properties from CIB anisotropies
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• Testing the key role of the stellar mass-halo mass relation in galaxy merger rates and morphologies via DECODE, a novel Discrete statistical sEmi-empiriCal mODEl
• Estimating major merger rates and spin parameters ab initio via the clustering of critical events
• Controlled Experiments on Dark-Matter Halo Structure and Galaxy Morphology I: What Sets Galaxy Sizes?
• Bridging Galaxy Dynamics and Baryon Efficiency of 40 EDGE-CALIFA galaxies
• Initial Mass Function for Massive Galaxies at z$\sim$1
• Hierarchal formation and growth of galaxies through dynamical friction
• The Cen A galaxy group: dynamical mass and missing baryons
• Resolved molecular gas and star-formation in massive unquenched spirals : I. UGC 8179
• Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies
• Tracing the evolution of brightest galaxies and diffuse light in galaxy groups
• A Mass Dependent Density Profile from Dwarfs to Clusters
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
• A Near-Infrared look at AGN Feedback in Bulgeless Galaxies
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• SF-R You Sure? The Conflicting Role of Star Formation Rates in Constraining the Evolution of Milky Way Analogues in Cosmological Simulations
• LYRA II: Cosmological dwarf galaxy formation with inhomogeneous Population III enrichment
• Large Molecular Gas Reservoirs in Ancestors of Milky Way-Mass Galaxies 9 Billion Years Ago
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• The vertical structure of the stellar disk in NGC 551
• The orbital dynamics of the LMC and SMC about the Milky Way
• The effects of self-interacting dark matter on the stripping of galaxies that fall into clusters