Constraints on the relationship between stellar mass and halo mass at low and high redshift

Abstract

We use a statistical approach to determine the relationship between the stellar masses of galaxies and the masses of the dark matter halos in which they reside. We obtain a parameterized stellar-to-halo mass (SHM) relation by populating halos and subhalos in an N-body simulation with galaxies and requiring that the observed stellar mass function be reproduced. We find good agreement with constraints from galaxy-galaxy lensing and predictions of semi-analytic models. Using this mapping, and the positions of the halos and subhalos obtained from the simulation, we find that our model predictions for the galaxy two-point correlation function (CF) as a function of stellar mass are in excellent agreement with the observed clustering properties in the SDSS at z=0. We show that the clustering data do not provide additional strong constraints on the SHM function and conclude that our model can therefore predict clustering as a function of stellar mass. We compute the conditional mass function, which yields the average number of galaxies with stellar masses in the range [m, m+dm] that reside in a halo of mass M. We study the redshift dependence of the SHM relation and show that, for low mass halos, the SHM ratio is lower at higher redshift. The derived SHM relation is used to predict the stellar mass dependent galaxy CF and bias at high redshift. Our model predicts that not only are massive galaxies more biased than low mass ones at all redshifts, but the bias increases more rapidly with increasing redshift for massive galaxies than for low mass ones. We present convenient fitting functions for the SHM relation as a function of redshift, the conditional mass function, and the bias as a function of stellar mass and redshift.

21 pages, 17 figures, discussion enlarged, one more figure, updated references, accepted for publication in ApJ

References in corpus (21)

• Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
• A Semi-Analytic Model for the Co-evolution of Galaxies, Black Holes, and Active Galactic Nuclei
• Galaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties
• Connecting Galaxies, Halos, and Star Formation Rates Across Cosmic Time
• Dynamical Friction and Galaxy Merging Timescales
• The Galaxy Mass Function up to z=4 in the GOODS-MUSIC sample: into the epoch of formation of massive galaxies
• Galaxy Groups in the SDSS DR4: II. halo occupation statistics
• The star formation histories of galaxies in the Sloan Digital Sky Survey
• Towards a Concordant Model of Halo Occupation Statistics
• Satellite Kinematics II: The Halo Mass-Luminosity Relation of Central Galaxies in SDSS
• Red Galaxy Growth and the Halo Occupation Distribution
• Galaxy Clustering & Galaxy-Galaxy Lensing: A Promising Union to Constrain Cosmological Parameters
• Modelling galaxy clustering in a high resolution simulation of structure formation
• The Stellar Masses and Star Formation Histories of Galaxies at z ~ 6: Constraints from Spitzer Observations in the Great Observatories Origins Deep Survey
• The Stellar Mass Density at z~6 from Spitzer Imaging of i-drop Galaxies
• The zCOSMOS Survey. The dependence of clustering on luminosity and stellar mass at z=0.2-1
• Modelling and interpreting the dependence of clustering on the spectral energy distributions of galaxies
• The impact of Spitzer infrared data on stellar mass estimates - and a revised galaxy stellar mass function at 0 < z < 5
• Modeling the three-point correlation function
• Satellite Kinematics I: A New Method to Constrain the Halo Mass-Luminosity Relation of Central Galaxies
• Evidence for merging or disruption of red galaxies from the evolution of their clustering

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• GAMA/G10-COSMOS/3D-HST: Evolution of the galaxy stellar mass function over 12.5Gyrs
• A mass threshold for galactic gas discs by spin flips
• From Galaxy Clusters to Ultra-Faint Dwarf Spheroidals: A Fundamental Curve Connecting Dispersion-supported Galaxies to Their Dark Matter Halos
• PRIMUS: Galaxy Clustering as a Function of Luminosity and Color at 0.2<z<1
• On ths assembly history of stellar components in massive galaxies
• The VLT SINFONI Mg ii Program for Line Emitters (SIMPLE) II: background quasars probing z $\sim$ 1 galactic winds
• Evolution of galaxy size--stellar mass relation from the Kilo Degree Survey
• The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
• Where Do Galaxies End?
• Galaxy formation with L-GALAXIES: Modelling the environmental dependency of galaxy evolution and comparing with observations
• The Galaxy Clustering Crisis in Abundance Matching
• The origin of pseudobulges in cosmological simulations of galaxy formation
• Persistence of the Color-Density Relation and Efficient Environmental Quenching to $z\sim 1.4$
• The shapes of spiral arms in the S${}^4$G survey and their connection with stellar bars
• Wet Compaction to a Blue Nugget: a Critical Phase in Galaxy Evolution
• COMAP Early Science: I. Overview
• Large-scale clustering of Lyman-alpha emission intensity from SDSS/BOSS
• The metallicity evolution of low mass galaxies: New constraints at intermediate redshift
• How the super-Eddington regime regulates black hole growth in high-redshift galaxies
• The evolution of superluminous supernova LSQ14mo and its interacting host galaxy system
• The baryonic Tully-Fisher relation and galactic outflows
• 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
• Ambient Column Densities of Highly Ionized Oxygen in Precipitation-Limited Circumgalactic Media
• Enriched haloes at redshift $z=2$ with no star-formation: Implications for accretion and wind scenarios
• Constraints on the merging channel of massive galaxies since z~1
• Dark halo response and the stellar initial mass function in early-type and late-type galaxies
• SURFS: Riding the waves with Synthetic UniveRses For Surveys
• GLAMER Part II: Multiple Plane Gravitational Lensing
• Discovery of Multi-Phase Cold Accretion in a Massive Galaxy at z=0.7
• H0LiCOW II. Spectroscopic survey and galaxy-group identification of the strong gravitational lens system HE0435-1223
• The MUSE Ultra Deep Field (MUDF). II. Survey design and the gaseous properties of galaxy groups at 0.5 < z < 1.5
• Numerical resolution limits on subhalo abundance matching
• The Edge of the Galaxy
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• Galaxies flowing in the oriented saddle frame of the cosmic web
• Star Formation and Clumps in Cosmological Galaxy Simulations with Radiation Pressure Feedback
• Breaking degeneracies in the first galaxies with clustering
• Reconciling observed and simulated stellar halo masses
• Constraining the CO intensity mapping power spectrum at intermediate redshifts
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• The MaGICC volume: reproducing statistical properties of high redshift galaxies
• EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations
• Puffing up early-type galaxies by baryonic mass loss: numerical experiments
• The distribution of mass components in simulated disc galaxies
• The distribution and morphologies of Fornax Cluster dwarf galaxies suggest they lack dark matter
• NIHAO XII: galactic uniformity in a ΛCDM universe
• The Fornax Deep Survey (FDS) with the VST XI. The search for signs of preprocessing between the Fornax main cluster and Fornax A group
• Light breeze in the local Universe
• Quantifying the Stellar Halo's Response to the LMC's Infall with Spherical Harmonics
• Systematic variations of central mass density slopes in early-type galaxies
• Two-Face(s): ionized and neutral gas winds in the local Universe
• The massive relic galaxy NGC 1277 is dark matter deficient. From dynamical models of integral-field stellar kinematics out to five effective radii
• Connecting Dark Matter Halos with the Galaxy Center and the Supermassive Black Hole
• Constraining the HI-Halo Mass Relation From Galaxy Clustering
• Empirical constraints on the formation of early-type galaxies
• Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
• The SLUGGS Survey: Breaking degeneracies between dark matter, anisotropy and the IMF using globular cluster subpopulations in the giant elliptical NGC 5846
• An analytical model for the accretion of dark matter subhalos
• Testing Subhalo Abundance Matching in Cosmological Smoothed Particle Hydrodynamics Simulations
• WIMP searches with gamma rays in the Fermi era: challenges, methods and results
• Hot Extended Galaxy Halos Around Local L* Galaxies From Sunyaev-Zeldovich Measurements
• Constraining the Star Formation Histories in Dark Matter Halos: I. Central Galaxies
• From lenticulars to blue compact dwarfs: the stellar mass fraction is regulated by disc gravitational instability
• MRK 1216 & NGC 1277 - An orbit-based dynamical analysis of compact, high velocity dispersion galaxies
• An observer's guide to the (Local Group) dwarf galaxies: predictions for their own dwarf satellite populations
• Chemical evolution of Local Group dwarf galaxies in a cosmological context -- I. A new modelling approach and its application to the Sculptor dwarf spheroidal galaxy
• Slicing the cool circumgalactic medium along the major-axis of a star-forming galaxy at $z=0.7$
• Host galaxies of high-redshift quasars: supermassive black hole growth and feedback
• The Galaxy-Halo/Subhalo connection: Mass relations and implications for some satellite occupational distributions
• 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
• Galactic inflow and wind recycling rates in the EAGLE simulations
• Orbital masses of nearby luminous galaxies
• Dwarf Galaxy Formation with H2-Regulated Star Formation: II. Gas-Rich Dark Galaxies at Redshift 2.5
• Ultra-strong MgII Absorbers as a Signature of Cool Intragroup Gas
• Forming early-type galaxies without AGN feedback: a combination of merger-driven outflows and inefficient star formation
• The stability of stellar disks in Milky-Way sized dark matter halos
• The mass-concentration relation in lensing clusters: the role of statistical biases and selection effects
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• The universal rotation curve of low surface brightness galaxies IV: the interrelation between dark and luminous matter
• Virgo Cluster and field dwarf ellipticals in 3D - II. Internal dynamics points to tidal harassment?
• The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to $z\sim 5$
• The dependence of tidal stripping efficiency on the satellite and host galaxy morphology
• AGN feedback in the nucleus of M51
• PRIMUS+DEEP2: The Dependence of Galaxy Clustering on Stellar Mass and Specific Star Formation Rate at 0.2 < z < 1.2
• Cosmic rays and non-thermal emission in simulated galaxies. II. $\gamma$-ray maps, spectra and the far infrared-$\gamma$-ray relation
• Self-Interacting Dark Matter and the Origin of Ultra-Diffuse Galaxies NGC1052-DF2 and -DF4
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• Sub one percent mass fractions of young stars in red massive galaxies
• Strong Gravitational Lensing and the Stellar IMF of Early-type Galaxies
• Star Formation and Stellar Mass Assembly in Dark Matter Halos: From Giants to Dwarfs
• Properties of Dark Matter Haloes and their Correlations: the Lesson from Principal Component Analysis
• MOND Prediction for the Velocity Dispersion of the `Feeble Giant' Crater II
• The Mass Dependence of Dwarf Satellite Galaxy Quenching
• The Dark Matter Halos of Moderate Luminosity X-ray AGN as Determined from Weak Gravitational Lensing and Host Stellar Masses
• The Low Redshift Circumgalactic Medium in Simba
• UVUDF: UV Luminosity Functions at the cosmic high-noon
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• Machine Learning and Cosmological Simulations I: Semi-Analytical Models
• Stellar mass distribution of S${}^4$G disk galaxies and signatures of bar-induced secular evolution
• On the Random Motion of Nuclear Objects in a Fuzzy Dark Matter Halo
• The hot circumgalactic medium in the eROSITA All-Sky Survey I. X-ray surface brightness profiles
• Can winds driven by active galactic nuclei account for the extragalactic gamma-ray and neutrino backgrounds?
• How Do Supernovae Impact the Circumgalactic Medium? I. Large-Scale Fountains Around a Milky Way-Like Galaxy
• Direct Measurement of the HI-Halo Mass Relation through Stacking
• 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
• Near-Field Limits on the Role of Faint Galaxies in Cosmic Reionization
• On the intermediate-redshift central stellar mass-halo mass relation, and implications for the evolution of the most massive galaxies since z~1
• The Dwarfs Beyond: The Stellar-to-Halo Mass Relation for a New Sample of Intermediate Redshift Low Mass Galaxies
• The Strikingly Similar Relation between Satellite and Central Galaxies and Their Dark Matter Halos Since z=2
• A PCA-based automated finder for galaxy-scale strong lenses
• Fully cosmological virtual massive galaxies at z=0: kinematical, morphological, and stellar population characterisation
• Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• A modified star formation law as a solution to open problems in galaxy evolution
• The Mass Dependence of Star Formation Histories in Barred Spiral Galaxies
• The origin of the mass scales for maximal star formation efficiency and quenching: the critical role of Supernovae
• Galaxy properties and the cosmic web in simulations
• Bottom-heavy initial mass function in a nearby compact L*-galaxy
• Size matters: the non-universal density profile of subhaloes in SPH simulations and implications for the Milky Way's dSphs
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• Beyond halo mass: quenching galaxy mass assembly at the edge of filaments
• 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
• What Do Dark Matter Properties Tell Us About Their Mass Assembly Histories?
• Shallow Dark Matter Cusps in Galaxy Clusters
• Properties of simulated Milky Way-mass galaxies in loose group and field environments
• SDSS-IV MaNGA: Spatially resolved star-formation histories and the connection to galaxy physical properties
• Stellar orbits in cosmological galaxy simulations: the connection to formation history and line-of-sight kinematics
• The Faber-Jackson relation and Fundamental Plane from halo abundance matching
• Discovery of a massive supercluster system at $z\sim 0.47$
• The Accelerated Build-up of the Red Sequence in High Redshift Galaxy Clusters
• The evolution of the stellar mass versus halo mass relationship
• A tale of two populations: the stellar mass of central and satellite galaxies
• Molecular hydrogen regulated star formation in cosmological SPH simulations
• The Unchanging Circumgalactic Medium Over the Past 11 Billion Years
• Reconstructing the gravitational field of the local universe
• Supernovae and AGN driven galactic outflows
• Quenched Cold Accretion of a Large Scale Metal-Poor Filament due to Virial Shocking in the Halo of a Massive z=0.7 Galaxy
• The effect of Warm Dark Matter on galaxy properties: constraints from the stellar mass function and the Tully-Fisher relation
• Adaptive Mesh Refinement Simulations of Galaxy Formation: Exploring Numerical and Physical Parameters
• Properties of Submillimeter Galaxies in a Semi-analytic Model using the "Count Matching" Approach: Application to the ECDF-S
• Modeling color-dependent galaxy clustering in cosmological simulations
• Modelling Galaxy Merger Timescales and Tidal Destruction
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe I. - The Effect of the Group Environment on Star Formation in Spiral Galaxies
• Halo Histories vs. Galaxy Properties at z=0, I: The Quenching of Star Formation
• The Relationship Between Galaxy ISM and Circumgalactic Gas Metallicities
• Galaxy cluster mass estimation with deep learning and hydrodynamical simulations
• The impact of global environment on galaxy mass functions at low redshift
• Constraining Satellite Galaxy Stellar Mass Loss and Predicting Intrahalo Light I: Framework and Results at Low Redshift
• The Morphology-Density-Relation: Impact on the Satellite Fraction
• The Q Continuum Simulation: Harnessing the Power of GPU Accelerated Supercomputers
• Sloan Great Wall as a complex of superclusters with collapsing cores
• Stellar Velocity Dispersion: Linking Quiescent Galaxies to their Dark Matter Halos
• Evidence for Early Filamentary Accretion from the Andromeda Galaxy's Thin Plane of Satellites
• The extent of the MgII absorbing circum-galactic medium of quasars
• Hierarchical Galaxy Growth and Scatter in the Stellar Mass - Halo Mass Relation
• Baryon effects on void statistics in the EAGLE simulation
• The central dark matter content of early-type galaxies: scaling relations and connections with star formation histories
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• Time Evolution of Galaxy Scaling Relations in Cosmological Simulations
• Exploring the halo occupation of AGN using dark-matter cosmological simulations
• Evolution of central dark matter of early-type galaxies up to z ~ 0.8
• Internal kinematics of groups of galaxies in the Sloan Digital Sky Survey data release 7
• The Molecular Gas in the NGC 6240 Merging Galaxy System at the Highest Spatial Resolution
• Evolution of LMC/M33-mass dwarf galaxies in the EAGLE simulation
• The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS
• Stellar splashback: the edge of the intracluster light
• Cosmic variance of $z>7$ galaxies: Prediction from BlueTides
• The Incomplete Conditional Stellar Mass Function: Unveiling the Stellar Mass Functions of Galaxies at 0.1 < Z < 0.8 from BOSS Observations
• Stellar mass-gap as a probe of halo assembly history and concentration: youth hidden among old fossils
• Impact of Supernova feedback on the Tully-Fisher relation
• The specific star formation rate and stellar mass fraction of low-mass central galaxies in cosmological simulations
• Clearing the hurdle: The mass of globular cluster systems as a function of host galaxy mass
• Measuring subhalo mass in redMaPPer clusters with CFHT Stripe 82 Survey
• Dependence of GAMA galaxy halo masses on the cosmic web environment from 100 square degrees of KiDS weak lensing data
• Where stars form and live at high redshift: clues from the infrared
• The Relative Role of Galaxy Mergers and Cosmic Flows in Feeding Black Holes
• Star Formation and Quenching of Central Galaxies from Stacked HI Measurements
• The Mass-Concentration Relation and the Stellar-to-Halo Mass Ratio in the CFHT Stripe 82 Survey
• The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?
• The growth of galactic bulges through mergers in LCDM haloes revisited. I. Present-day properties
• The Main Sequence and the Fundamental Metallicity Relation in MaGICC Galaxies: Evolution and Scatter
• Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
• The emergence of dark matter-deficient ultra-diffuse galaxies driven by scatter in the stellar mass-halo mass relation and feedback from globular clusters
• Central galaxies in different environments: Do they have similar properties?
• Galaxy downsizing evidenced by hybrid evolutionary tracks
• The role of gas infall in the evolution of disc galaxies
• Observed trend in the star formation history and the dark matter fraction of galaxies at redshift $z\approx 0.8$
• A weak gravitational lensing recalibration of the scaling relations linking the gas properties of dark halos to their mass
• A Statistical Semi-Empirical Model: Satellite galaxies in Groups and Clusters
• HectoMAP and Horizon Run 4: Dense Structures and Voids in the Real and Simulated Universe
• Tidal-induced lopsidedness in Magellanic-type galaxies
• Constraints on the evolution of the relationship between HI mass and halo mass in the last 12 Gyr
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• Degeneracies Between Self-interacting Dark Matter and Supernova Feedback as cusp-core transformation mechanisms
• Sussing Merger Trees : The Impact of Halo Merger Trees on Galaxy Properties in a Semi-Analytic Model
• Cross-correlation of cosmic far-infrared background anisotropies with large scale structures
• Stellar mass -- halo mass relation for the brightest central galaxies of X-ray clusters since z~0.65
• The Violent Youth of Bright and Massive Cluster Galaxies and their Maturation over 7 Billion Years
• Velocity Dispersions of Brightest Cluster Galaxies and Their Host Clusters
• Brightest Cluster Galaxies in Cosmological Simulations with Adaptive Mesh Refinement: Successes and Failures
• Modeling the JWST high-redshift galaxies with a general formation scenario and the consistency with the $\Lambda$CDM model
• The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
• A scaling relation between merger rate of galaxies and their close pair count
• The Impact of Environment on the Stellar Mass - Halo Mass Relation
• Investigating evidence for different black hole accretion modes since redshift z~1
• Herschel reveals a molecular outflow in a z = 2.3 ULIRG
• A dwarf-dwarf merger and dark matter core as a solution to the Globular Cluster problems in the Fornax dSph
• SHELS: Complete Redshift Surveys of Two Widely Separated Fields
• Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
• The Most Bound Halo Particle-Galaxy Correspondence Model: Comparison between Models with Different Merger Timescales
• Telltale signs of metal recycling in the circumgalactic medium of a $z\sim 0.77$ galaxy
• A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The $(v_{\max },M_{\mathrm{DM}})$-$({\sigma }_0,M_{\mathrm{BH}},\varphi )$ Relations
• No evidence for modifications of gravity from galaxy motions on cosmological scales
• A Galaxy Redshift Survey near HST/COS AGN Sight Lines
• On the effect of galactic outflows in cosmological simulations of disc galaxies
• The Milky Way system in LCDM cosmological simulations
• Circumgalactic Pressure Profiles Indicate Precipitation-Limited Atmospheres for $M_{\ast }\sim 10^9$$-$$10^{11.5}{M}_{\odot }$
• Specific Frequencies and Luminosity Profiles of Cluster Galaxies and Intracluster Light in Abell 1689
• ELUCID. VI: Cosmic variance of galaxy distribution in the local Universe
• The effects of a hot gaseous halo on disc thickening in galaxy minor mergers
• The Brightest Galaxies at Cosmic Dawn from Scatter in the Galaxy Luminosity versus Halo Mass Relation
• Halo Mass Dependence of HI and OVI Absorption: Evidence for Differential Kinematics
• COMAP Early Science: VII. Prospects for CO Intensity Mapping at Reionization
• Compaction-Driven Black Hole Growth
• The Molecular Gas Content of z<0.1 Radio Galaxies: Linking the AGN Accretion Mode to Host Galaxy Properties
• Dark satellites and the morphology of dwarf galaxies
• On the Orbital Decay of Globular Clusters in NGC1052-DF2: Testing a Baryon-Only Mass Model
• The last 6 Gyr of dark matter assembly in massive galaxies from the Kilo Degree Survey
• Galaxy And Mass Assembly (GAMA): The Consistency of GAMA and WISE Derived Mass-to-Light Ratios
• Rapid Filamentary Accretion as the Origin of Extended Thin Discs
• A low pre-infall mass for the Carina dwarf galaxy from disequilibrium modelling
• Regulation of Star Formation by a Hot Circumgalactic Medium
• Strong Lensing by Galaxies
• MaGICC-WDM: the effects of warm dark matter in hydrodynamical simulations of disc galaxy formation
• The scatter in the galaxy-halo connection: a machine learning analysis
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Signatures of Dark Matter Halo Expansion in Galaxy Populations
• Herschel-ATLAS/GAMA: SDSS cross-correlation induced by weak lensing
• Confronting fuzzy dark matter with the rotation curves of nearby dwarf irregular galaxies
• Improved strong lensing modelling of galaxy clusters using the Fundamental Plane: Detailed mapping of the baryonic and dark matter mass distribution of Abell S1063
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• Cosmic CARNage I: on the calibration of galaxy formation models
• A cosmological context for compact massive galaxies
• The physical drivers of the atomic hydrogen-halo mass relation
• DEMNUni: comparing nonlinear power spectra prescriptions in the presence of massive neutrinos and dynamical dark energy
• What drives galaxy quenching? A deep connection between galaxy kinematics and quenching in the local Universe
• The accreted stellar halo as a window on halo assembly in L* galaxies
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• A measurement of circumgalactic gas around nearby galaxies using fast radio bursts
• Linking haloes to galaxies: how many halo properties are needed?
• On the relation between sSFR and metallicity
• The Mass Dependance of Satellite Quenching in Milky Way-like Halos
• The Effect of Coupled Dark Energy on the Alignment between Dark Matter and Galaxy Distributions in Clusters
• The PCA Lens-Finder: application to CFHTLS
• Resolving the baryon-fraction profile in lensing galaxies
• The effects of LMC-mass environments on their dwarf satellite galaxies in the FIRE simulations
• The PEP survey: clustering of infrared-selected galaxies and structure formation at z~2 in the GOODS South
• The quest for cradles of life: using the fundamental metallicity relation to hunt for the most habitable type of galaxy
• Galaxy Pairs in the Local Group
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• On the (Lack of) Evolution of the Stellar Mass Function of Massive Galaxies from $z$=1.5 to 0.4
• Are the halo occupation predictions consistent with large scale galaxy clustering?
• Density modulated star formation efficiency: implications for the observed abundance of ultra-violet luminous galaxies at z>10
• SatGen -- II. Assessing the impact of a disc potential on subhalo populations
• The Fundamental Relation between Halo Mass and Galaxy Group Properties
• An HST/COS legacy survey of intervening SiIII absorption in the extended gaseous halos of low-redshift galaxies
• MOND and IMF variations in early-type galaxies from $ATLA{S}^{3D}$
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
• Still at Odds with Conventional Galaxy Evolution: The Star Formation History of Ultra-Diffuse Galaxy Dragonfly 44
• ELUCID V. Lighting dark matter halos with galaxies
• The importance of galaxy formation histories in models of reionization
• Supercluster A2142 and collapse in action - infalling and merging groups and galaxy transformations
• The Intrinsic Scatter of Galaxy Scaling Relations
• DESI Peculiar Velocity Survey -- Fundamental Plane
• What do simulations predict for the galaxy stellar mass function and its evolution in different environments?
• Infalling groups and galaxy transformations in the cluster A2142
• Using Velocity Dispersion to Estimate Halo Mass: Is the Local Group in Tension with $\Lambda$CDM?
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• Galactic rotation curves in brane world models
• The Corona Borealis supercluster: connectivity, collapse, and evolution
• Compact Starburst Galaxies with Fast Outflows: Central Escape Velocities and Stellar Mass Surface Densities from Multi-band Hubble Space Telescope Imaging
• Characterizing dark interactions with the halo mass accretion history and structural properties
• Dissecting the roles of mass and environment quenching in galaxy evolution with EAGLE
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• High resolution near-infrared imaging of submillimeter galaxies
• An accurate method to determine the systematics due to the peculiar velocities of galaxies in measuring the Hubble constant from gravitational wave standard sirens
• A matter of measurement: rotation velocities and the velocity function of dwarf galaxies
• ECO and RESOLVE: Galaxy Disk Growth in Environmental Context
• The miniJPAS survey: The role of group environment in quenching the star formation
• Unveiling the atomic hydrogen-halo mass relation via spectral stacking
• RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions
• The dichotomy of dark matter fraction and total mass density slope of galaxies over five dex in mass
• The COS-AGN survey: Revealing the nature of circum-galactic gas around hosts of active galactic nuclei
• Constraining Cosmic-ray Transport with Observations of the Circumgalactic Medium
• The halo light cone catalogues of \Abacus{AbacusSummit}
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• On the scatter in the relation between stellar mass and halo mass: random or halo formation time dependent?
• Real- and redshift-space halo clustering in $f(R)$ cosmologies
• Interaction between dark matter sub-halos & galactic gaseous disk
• Scaling relations and baryonic cycling in local star-forming galaxies. III. Outflows, effective yields and metal loading factors
• Radio galaxies in ZFOURGE/NMBS: no difference in the properties of massive galaxies with and without radio-AGN out to z = 2.25
• Constraining the Tail-End of Reionization Using Lyman-$\alpha$ Transmission Spikes
• Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering
• A first estimate of the Milky Way dark matter halo spin
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• The Missing Satellite Problem Outside of the Local Group: I -- Pilot Observation
• Stellar mass versus stellar velocity dispersion: which is better for linking galaxies to their dark matter halos?
• Hosts and triggers of AGNs in the Local Universe
• Galaxy Formation in Sterile Neutrino Dark Matter Models
• Describing galaxy weak lensing measurements from tenths to tens of Mpc and up to z~0.6 with a single model
• The Influence of Galaxy Environment on the Stellar Initial Mass Function of Early-Type Galaxies
• Edge-on HI-bearing ultra diffuse galaxy candidates in the 40% ALFALFA catalog
• Discovery of a transparent sightline at ρ < 20 kpc from an interacting pair of galaxies
• A New Approach to Identifying the Most Powerful Gravitational Lensing Telescopes
• Magnitude Gap Statistics and the Conditional Luminosity Function
• Multi-frequency studies of galaxies and groups: I. Environmental effect on galaxy stellar mass and morphology
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Don't Forget the Forest for the Trees: The Stellar-Mass Halo-Mass Relation in Different Environments
• Generating Synthetic Cosmological Data with GalSampler
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Cosmic Galaxy-IGM HI Relation at $z\sim 2-3$ Probed in the COSMOS/UltraVISTA $1.6$ deg${}^2$ Field
• Simulations of isolated dwarf galaxies formed in dark matter halos with different mass assembly histories
• Numerical hydrodynamic simulations based on semi-analytic galaxy merger trees: method and Milky-Way like galaxies
• The Warm Circum-Galactic Medium: 10^5-6 K Gas Associated with a Single Galaxy Halo or with an Entire Group of Galaxies?
• Astrophysical Tests of Dark Matter Self-Interactions
• Constraints on the HI Mass of NGC 1052-DF2
• Testing Verlinde's emergent gravity in early-type galaxies
• Scaling relations for globular cluster systems in early-type galaxies
• Inferring galaxy dark halo properties from visible matter with Machine Learning
• SH$\alpha$DE: Survey description and mass-kinematics scaling relations for dwarf galaxies
• The Fate of Supernova-Heated Gas in Star-Forming Regions of the LMC: Lessons for Galaxy Formation?
• A Bayesian Hierarchical Approach to Galaxy-Galaxy Lensing
• Cosmic Near-infrared Background Tomography with SPHEREx Using Galaxy Cross-correlations
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• Galaxy stellar mass assembly: the difficulty matching observations and semi-analytical predictions
• Star Formation History in Barred Spiral Galaxies. AGN Feedback
• What galaxy masses perturb the local cosmic expansion?
• The Missing Satellite Problem Outside of the Local Group. II. Statistical Properties of Satellites of Milky Way-like Galaxies
• 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 neutral hydrogen distribution in large-scale haloes from 21-cm intensity maps
• The environment and host haloes of the brightest z~6 Lyman-break galaxies
• On the Prevalence of Super-Massive Black Holes over Cosmic Time
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• The distribution of faint satellites around central galaxies in the CFHT Legacy Survey
• From dwarf galaxies to galaxy clusters: Self-Interacting Dark Matter over 7 orders of magnitude in halo mass
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• Luminosity bias: from haloes to galaxies
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Estimating the Milky Way's Mass via Hierarchical Bayes: A Blind Test on MUGS2 Simulated Galaxies
• Galaxy Ecosystems: gas contents, inflows and outflows
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• The dependence of subhalo abundance matching on galaxy photometry and selection criteria
• Effects of Baryon Mass Loss on Profiles of Large Galactic Dark Matter Haloes
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• The massive dark halo of the compact, early-type galaxy NGC 1281
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• Main Sequence Scatter is Real: The Joint Dependence of Galaxy Clustering on Star Formation and Stellar Mass
• Observed versus modelled u,g,r,i,z-band photometry of local galaxies - Evaluation of model performance
• The effect of Large Magellanic Cloud on the satellite galaxy population in Milky Way analogous Galaxies
• MUSE-ALMA Halos VI: Coupling Atomic, Ionised & Molecular Gas Kinematics of Galaxies
• Dark Matter and IMF normalization in Virgo dwarf early-type galaxies
• Tidal stirring of satellites with shallow density profiles prevents them from being too big to fail
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• A unified scenario for the origin of spiral and elliptical galaxy structural scaling laws
• Zooming into the Cosmic Horseshoe: new insights on the lens profile and the source shape
• The galaxy-halo connection of disc galaxies over six orders of magnitude in stellar mass
• The Clustering Of Galaxies Around Radio-Loud AGNs
• Mass-to-Light Ratios of Spatially Resolved Stellar Populations in M31
• The abundance of satellites depends strongly on the morphology of the host galaxy
• Evolution of the baryon fraction in the Local Group: accretion versus feedback at low and high z
• A Census of the Extended Neutral Hydrogen Around 18 MHONGOOSE Galaxies
• Navarro-Frenk-White dark matter profile and the dark halos around disk systems
• Evolution of the Gas Mass Fraction of Progenitors to Today's Massive Galaxies: ALMA Observations in the CANDELS GOODS-S Field
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• Mass and size growth of early-type galaxies by dry mergers in cluster environments
• SN-driven mechanism of cusp-core transformation: an appraisal
• Hierarchical structure of the cosmic web and galaxy properties
• Constraints on the Evolution of the Galaxy Stellar Mass Function I: Role of Star Formation, Mergers and Stellar Stripping
• Direct-collapse black hole formation induced by internal radiation of host halos
• Effects of self-consistent rest-ultraviolet colours in semi-empirical galaxy formation models
• The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
• Gas Accretion and Galactic Chemical Evolution: Theory and Observations
• Observational Aspects of Galactic Accretion at Redshift 3.3
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• Predicting fully self-consistent satellite richness, galaxy growth and starformation rates from the STastical sEmi-Empirical modeL STEEL
• Characterizing the Circumgalactic Medium of the Lowest-Mass Galaxies: A Case Study of IC 1613
• The Molecular Baryon Cycle of M82
• Clustering dependence on Lyman-$\alpha$ luminosity from MUSE surveys at $3<z<6$
• Relative distribution of dark matter and stellar mass in three massive galaxy clusters
• Connections between galaxy properties and halo formation time in the cosmic web
• Stellar mass versus velocity dispersion as tracer of the lensing signal around bulge-dominated galaxies
• Fingerprints of the hierarchical building up of the structure on the gas kinematics of galaxies
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z<1.3
• Autocorrelations of stellar light and mass at z~0 and ~1: From SDSS to DEEP2
• The Effects of X-Ray and UV Background Radiation on the Low-Mass Slope of the Galaxy Mass Function
• The role of gas kinematics in setting metallicity gradients at high redshift
• Central velocity dispersion catalog of LAMOST-DR7 galaxies
• Measuring the total infrared light from galaxy clusters at z=0.5-1.6: connecting stellar populations to dusty star formation
• Euclid preparation. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields
• The XXL Survey: XXII. The XXL-North spectrophotometric sample and galaxy stellar mass function in X-ray detected groups and clusters
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• A 1-dimensional hydrodynamic model for accretion, cooling and heating of gas in dark matter halos from $z=6$ to $z=0$
• Momentum and energy injection by a supernova remnant into an inhomogeneous medium
• Joint Gas and Stellar Dynamical Models of WLM: An isolated dwarf galaxy within a cored, prolate DM halo
• Galaxy Three-Point Correlation Functions and Halo/Subhalo Models
• How feedback shapes galaxies: an analytic model
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• The strong environmental dependence of black hole scaling relations
• Modeling Reionization in a Bursty Universe
• Dynamical modelling and origin of gas turbulence in z $\sim$ 4.5 galaxies
• Probing the gaseous halo of galaxies through non-thermal emission from AGN-driven outflows
• The influence of the void environment on the ratio of dark matter halo mass to stellar mass in SDSS MaNGA galaxies
• Gamma-ray emission from spectrally resolved cosmic rays in galaxies
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• Bent Radio Jets Reveal a Stripped Interstellar Medium in NGC 1272
• Centrally Concentrated H I Distribution Enhances Star Formation in Galaxies
• Investigating the impact of quasar-driven outflows on galaxies at redshift 0.3-0.4
• How the super-Eddington regime affects black hole spin evolution in high-redshift galaxies
• The Luminosity Functions and Redshift Evolution of Satellites of Low-Mass Galaxies in the COSMOS Survey
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
• An improved prescription for merger time-scales from controlled simulations
• The Cosmic Evolution of Halo Pairs: I. Global Trends
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• Disentangling the multi-phase circumgalactic medium shared between a dwarf and a massive star-forming galaxy at z~0.4
• Compensated Isocurvature Perturbations in the Galaxy Power Spectrum
• The evolution of high-density cores of the BOSS Great Wall superclusters
• Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys
• Constraining Scatter in the Stellar Mass--Halo Mass Relation for Haloes Less Massive than the Milky Way
• Testing galaxy formation models with galaxy stellar mass functions
• Models of gravitational lens candidates from Space Warps CFHTLS
• Differentiable Predictions for Large Scale Structure with SHAMNet
• A VLT/MUSE galaxy survey towards QSO Q1410: looking for a WHIM traced by BLAs in inter-cluster filaments
• Testing baryon-induced core formation in $\Lambda$CDM: A comparison of the DC14 and coreNFW dark matter halo models on galaxy rotation curves
• Investigating the $M_{GCS}-M_h$ Relation in the Most Massive Galaxies
• Tentative Detection of the Circumgalactic Medium of the Isolated Low-Mass Dwarf Galaxy WLM
• Degeneracies between baryons and dark matter: the challenge of constraining the nature of dark matter with JWST
• BOSS Great Wall: morphology, luminosity, and mass
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• Cosmic Ray-Driven Galactic Winds with Resolved ISM and Ion-Neutral Damping
• SHALOS: Statistical Herschel-ATLAS Lensed Objects Selection
• Gas accretion in Milky Way-like galaxies: temporal and radial dependencies
• Impact of H${}_2$-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
• ΛCDM is still not broken: empirical constraints on the star formation efficiency at z ~ 12-30
• A possible signature of the influence of tidal perturbations in dwarf galaxy scaling relations
• A census of dwarf galaxy satellites around LMC-mass galaxy NGC 2403
• Proof of CMB-driven X-ray brightening of high-z radio galaxies
• The Velocity Dispersion Function for Quiescent Galaxies in Nine Strong-Lensing Clusters
• Resolved Stellar Mass Maps of Galaxies in the Hubble Frontier Fields: Evidence for Mass Dependency in Environmental Quenching
• Diagnostics of Baryonic Cooling in Lensing Galaxies
• Simulating Deep Hubble Images With Semi-empirical Models of Galaxy Formation
• Disk galaxy scaling relations at intermediate redshifts - I. The Tully-Fisher and velocity-size relations
• Gas around galaxy haloes: methodology comparisons using hydrodynamical simulations of the intergalactic medium
• Over-density of SMGs in fields containing z~0.3 galaxies: magnification bias and the implications for studies of galaxy evolution
• Probing the Diffuse Lyman-alpha Emission on Cosmological Scales: Lyα Emission Intensity Mapping Using the Complete SDSS-IV eBOSS Survey
• Chemical enrichment in isolated barred spiral galaxies
• Tracking the orbit of unresolved subhalos for semi-analytic models
• AGN and Star-Formation Properties of Inside-out Assembled Galaxy Candidates at z<0.1
• The weak dependence of velocity dispersion on disk fractions, mass-to-light ratio and redshift: Implications for galaxy and black hole evolution
• Distinctive GWBs from eccentric inspiraling SMBH binaries with a DM spike
• CLUES about M33: the reversed radial stellar age gradient in the outskirts of Triangulum galaxy
• Star formation in high redshift galaxies including Supernova feedback: effect on stellar mass and luminosity functions
• Cosmological feedback from a halo assembly perspective
• Relating galaxies across different redshift to study galaxy evolution
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• The Circumgalactic Medium in Massive Halos
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• Revisiting the clustering of narrow-line AGN in the local Universe: Joint dependence on stellar mass and color
• Star Formation of Merging Disk Galaxies with AGN Feedback Effects
• Revealing the Galaxy-Halo Connection Through Machine Learning
• Abundance matching for low mass galaxies in the CDM and FDM models
• Census of Gaseous Satellites around Local Spiral Galaxies
• Galaxy luminosity functions at redshifts 0.6 to 1.2 in the Chandra Deep Field South
• First results from SMAUG: Insights into star formation conditions from spatially-resolved ISM properties in TNG50
• Inferring dark matter halo properties for HI-selected galaxies
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• Stellar angular momentum distribution linked to galaxy morphology
• Towards an accurate model of small-scale redshift-space distortions in modified gravity
• Dark matter halos and the M-σrelation for supermassive black holes
• Weak lensing measurement of the mass-richness relation using the SDSS database
• The very wide-field $gzK$ galaxy survey -- II. The relationship between star-forming galaxies at $z\sim 2$ and their host haloes based upon HOD modelling
• Hot gas in galaxy halos traced by coronal broad Lyman alpha absorbers
• On merger bias and the clustering of quasars
• Can a conditioning on stellar mass explain the mutual information between morphology and environment?
• Disk galaxies are self-similar: the universality of the HI-to-Halo mass ratio for isolated disks
• The coevolution of the velocity and mass functions of galaxies and dark haloes
• Cosmic evolution of the incidence of Active Galactic Nuclei in massive clusters: Simulations versus observations
• A joint microlensing analysis of lensing mass and accretion disc models
• The central dark matter fraction of massive early-type galaxies
• Probing the Mpc-scale environment of hyperluminous infrared galaxies at 2<z<4
• An Eddington ratio-driven origin for the ${\mathrm{L}}_{\mathrm{X}}-{\mathrm{M}}_{\ast }$ relation in quiescent and star forming active galaxies
• Extreme circumgalactic HI and CIII absorption around the most massive, quenched galaxies
• Understanding the Fundamental Plane and the Tully Fisher Relation
• Color dependence of clustering of massive galaxies at 0.5$\le z\le$2.5: similar spatial distributions between green valley galaxies and AGNs
• Characterizing simulated galaxy stellar mass histories
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• A Hyperactive FRB Pinpointed in an SMC-Like Satellite Host Galaxy
• Oxygen Loss from Simulated Galaxies and the Metal Flow Main Sequence: Predicting the Dependence on Mass and Environment
• The stellar mass function and efficiency of galaxy formation with a varying initial mass function
• Predictions on the stellar-to-halo mass relation in the dwarf regime using the empirical model for galaxy formation EMERGE
• The THESAN-ZOOM project: Star-formation efficiencies in high-redshift galaxies
• Close Galaxy Pairs at z = 3: A Challenge to UV Luminosity Abundance Matching
• DEMNUni: cross-correlating the nonlinear ISWRS effect with CMB-lensing and galaxies in the presence of massive neutrinos
• Circumgalactic Environments around Distant Quasars 3C 9 and 4C 05.84
• Explaining JWST star formation history at $z\sim 17$ by modifying $\Lambda$CDM
• The Space Density of Intermediate Redshift, Extremely Compact, Massive Starburst Galaxies
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Abundance matching tested on small scales with galaxy dynamics
• Polytropic dark halos of elliptical galaxies
• IllustrisTNG Snapshots for 10 Gyr of Dynamical Evolution of Brightest Cluster Galaxies and Their Host Clusters
• Impact of star formation models on the growth of simulated galaxies at high redshifts
• Measuring the Total Ultraviolet Light from Galaxy Clusters at z=0.5-1.6: The Balance of Obscured and Unobscured Star-Formation
• EMERGE: Constraining merging probabilities and timescales of close galaxy pairs
• Semi-empirical catalog of early-type galaxy-halo systems: dark matter density profiles, halo contraction and dark matter annihilation strength
• Investigating the Dark Matter Halo of NGC 5128 using a Discrete Dynamical Model
• MaNGA AGN dwarf galaxies (MAD) -- II. AGN outflows in dwarf galaxies
• PRIMUS: The Effect of Physical Scale on the Luminosity-Dependence of Galaxy Clustering via Cross-Correlations
• MAMBO -- An empirical galaxy and AGN mock catalogue for the exploitation of future surveys
• The significant effects of stellar mass estimation on galaxy pair fractions
• Insights on Metal Enrichment and Environmental Effect at $z\approx 5-7$ with JWST ASPIRE/EIGER and Chemical Evolution Model
• Subhalo abundance matching in $f(R)$ gravity
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• The dependence of cluster galaxy properties on the central entropy of their host cluster
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• Mass Modeling the Andromeda Dwarf Galaxies: Andromeda VI and Andromeda XXIII
• The Halo Masses of Galaxies to $z\sim 3$: A Hybrid Observational and Theoretical Approach
• The dust and cold gas content of local star forming galaxies
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• Age-dating the Tully-Fisher relation at moderate redshift
• High accuracy power spectra including baryonic physics in dynamical Dark Energy models
• X-ray Surface Brightness Profiles of Optically Selected Active Galactic Nuclei: Comparison with X-ray AGN
• Shape noise and dispersion in precision weak lensing
• The quantity of dark matter in early-type galaxies and its relation to the environment
• Supernova-Neutrino-Boosted Dark Matter from All Galaxies
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• The galaxy counterpart of the high-metallicity and 16 kpc impact parameter DLA towards Q0918+1636 - a challenge to galaxy formation models?
• The spin of late-type galaxies at redshifts z < 1.2
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• Galaxy-galaxy lensing in the VOICE deep survey
• Measuring the Hubble constant through the galaxy pairwise peculiar velocity
• Physical Models for the Clustering of Obscured and Unobscured Quasars
• HST Hα grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation
• The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies
• Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS
• The Circular Velocity Function of Group Galaxies
• The role of scatter and satellites in shaping the large-scale clustering of X-ray AGN as a function of host galaxy stellar mass
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• A correlation between accreted stellar kinematics and dark matter halo spin in the ARTEMIS simulations
• Kinematic scaling relations of disc galaxies from ionised gas at $z\sim 1$ and their connection with dark matter haloes
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Star formation drivers across the M33 disk
• Clustering properties and halo masses for central galaxies in the local Universe
• Galaxy Superclusters and Their Complexes in the Cosmic Web
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• A new way to measure the distance to NGC1052-DF2
• Impact of the turnover in the high-z galaxy luminosity function on the 21-cm signal during Cosmic Dawn and Epoch of Reionization
• An Empirical Mass Function Distribution
• Reconciling PTA and JWST and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• Dependence of the ratio of total to visible mass on observable properties of SDSS MaNGA galaxies
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Transforming galaxies with EASE: widespread structural changes enabled by short-lived spirals
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• The AGORA High-resolution Galaxy Simulations Comparison Project. X: Formation and Evolution of Galaxies at the High-redshift Frontier
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Ionized gas kinematics of massive elliptical galaxies in CALIFA and in cosmological zoom-in simulations
• Cosmological parameters from lenses distance ratio
• Direct Shear Mapping: Prospects for weak lensing studies of individual galaxy-galaxy lensing systems
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• The Diversity of Environments Around Luminous Quasars at Redshift $z\sim 6$
• A Full Accounting of the Visible Mass in SDSS MaNGA Disk Galaxies
• On the Origin of the Variety of Velocity Dispersion Profiles of Galaxies
• Quantitatively rating galaxy simulations against real observations with anomaly detection
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• SHAM-OT: Rapid Subhalo Abundance Matching with Optimal Transport
• The Formation of M101-alike Galaxies in the Cold Dark Matter Model
• Modified Gravity and Large Scale Flows, a Review
• Revealing the formation histories of the first stars with the cosmic near-infrared background
• JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations
• Renzo's rule revisited: A statistical study of galaxies' baryon - dark matter coupling
• The Effect of Impact Parameters on the Formation of Massive Black Hole Binaries in Galactic Mergers
• Dark matter in ALFALFA galaxies: Investigating galaxy-halo connection
• How far have metals reached? Reconciling statistical constraints and enrichment models at reionization
• Kinematic analysis of an Ultra-Strong MgII absorber at z~1.13 linking to Circumgalactic Gas Structures
• Dynamical Mass Determinations and Scaling Relations of Early-Type Galaxies
• What triggers type Ia supernovae: Prompt detonations from primordial black holes or companion stars?
• The Lowest Metallicity Stars in the LMC: Clues from MaGICC Simulations
• Gravitational potential drives the concentration dependence of the stellar mass-halo mass relation
• Extended Hernquist-Springel formalism for cosmic star formation
• The mass profile of NGC 3377 from a Bayesian approach
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• High precision spectra at large redshift for dynamical DE cosmologies
• A positive correlation between broad HI Ly$\alpha$ absorptions and local overdensities of galaxies
• 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
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG
• The stellar population of a $z\sim 3.25$ Ly$\alpha$ emitting group associated with a damped Ly$\alpha$ absorber
• The tidal features of the classical Milky Way satellites: Expected in MOND but inconsistent with cold dark matter models
• Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment
• Morphological Transformation and Star Formation Quenching of Massive Galaxies at 0.5 < z < 2.5 in 3D-HST/CANDELS
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• The lens SW05 J143454.4+522850: a fossil group at redshift 0.6?
• The orbital dynamics of the LMC and SMC about the Milky Way
• Massive black holes and their galaxies
• The Baryon Budget of Galaxies across the First Billion Years
• Testing subhalo abundance matching with galaxy kinematics
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations IV. Testing warm dark matter cosmologies with galaxy scaling relations: A joint simulation-observation study using DREAMS simulations
• Substructures in Minor Mergers' Tidal Streams
• Systematic variation of central mass density slope in early-type galaxies
• A z$\sim$1 galactic-scale outflow transversally mapped to $\sim$50 kpc through gravitational-arc tomography
• An empirical model of the extragalactic radio background