A Comprehensive Analysis of Uncertainties Affecting the Stellar Mass - Halo Mass Relation for 0<z<4

Abstract

We conduct a comprehensive analysis of the relationship between central galaxies and their host dark matter halos, as characterized by the stellar mass-halo mass (SM-HM) relation, with rigorous consideration of uncertainties. Our analysis focuses on results from the abundance matching technique, which assumes that every dark matter halo or subhalo above a specific mass threshold hosts one galaxy. We discuss the quantitative effects of uncertainties in observed galaxy stellar mass functions (GSMFs) (including stellar mass estimates and counting uncertainties), halo mass functions (including cosmology and uncertainties from substructure), and the abundance matching technique used to link galaxies to halos (including scatter in this connection). Our analysis results in a robust estimate of the SM-HM relation and its evolution from z=0 to z=4. The shape and evolution are well constrained for z < 1. The largest uncertainties at these redshifts are due to stellar mass estimates; however, failure to account for scatter in stellar masses at fixed halo mass can lead to errors of similar magnitude in the SM-HM relation for central galaxies in massive halos. We also investigate the SM-HM relation to z=4, although the shape of the relation at higher redshifts remains fairly unconstrained when uncertainties are taken into account. These results will provide a powerful tool to inform galaxy evolution models. [Abridged]

27 pages, 12 figures, updated to match ApJ accepted version.

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• Machine Learning and Cosmological Simulations I: Semi-Analytical Models
• Hot phase generation by supernovae: resolution, chemistry and thermal conduction
• 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
• Sample variance in photometric redshift calibration: cosmological biases and survey requirements
• Luminous and High Stellar Mass Candidate Galaxies at z ~ 8 Discovered in CANDELS
• An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift $1\le z\le 9$
• Early-type galaxy density profiles from IllustrisTNG: I. Galaxy correlations and the impact of baryons
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• Mapping Extragalactic Dark Matter Annihilation with Galaxy Surveys: A Systematic Study of Stacked Group Searches
• Evolution of Star-forming Galaxies from z = 0.7 to 1.2 with eBOSS Emission-line Galaxies
• Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties
• Modelling the Transfer Function for the Dark Energy Survey
• On the galaxy-halo connection in the EAGLE simulation
• Iron in X-COP: tracing enrichment in cluster outskirts with high accuracy abundance profiles
• Clustering of quasars in the First Year of the SDSS-IV eBOSS survey: Interpretation and halo occupation distribution
• Stars, Dust, and the Growth of UV-Selected Sub-L* Galaxies at Redshift z~2
• Shallow Dark Matter Cusps in Galaxy Clusters
• A machine learning approach to mapping baryons onto dark matter haloes using the EAGLE and C-EAGLE simulations
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• What Do Dark Matter Properties Tell Us About Their Mass Assembly Histories?
• Beyond halo mass: quenching galaxy mass assembly at the edge of filaments
• SDSS-IV MaNGA: Spatially resolved star-formation histories and the connection to galaxy physical properties
• Building a Predictive Model of Galaxy Formation - I: Phenomenological Model Constrained to the $z=0$ Stellar Mass Function
• Comprehensive Gas Characterization of a $z=2.5$ Protocluster: A Cluster Core Caught in the Beginning of Virialization?
• The evolution of the stellar mass versus halo mass relationship
• Molecular hydrogen regulated star formation in cosmological SPH simulations
• The H-alpha luminosity-dependent clustering of star-forming galaxies from z~0.8 to z~2.2 with HiZELS
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• Metal-poor, Strongly Star-Forming Galaxies in the DEEP2 Survey: The Relationship between Stellar Mass, Temperature-based Metallicity, and Star Formation Rate
• A tale of two populations: the stellar mass of central and satellite galaxies
• The Faber-Jackson relation and Fundamental Plane from halo abundance matching
• The Progenitors of Calcium-Strong Transients
• The Cosmic Evolution of Faint Satellite Galaxies as a Test of Galaxy Formation and the Nature of Dark Matter
• SHARP - I. A high-resolution multi-band view of the infra-red Einstein ring of JVAS B1938+666
• The LBT Satellites of Nearby Galaxies Survey (LBT-SONG): The Satellite Population of NGC 628
• The Unchanging Circumgalactic Medium Over the Past 11 Billion Years
• Quenched Cold Accretion of a Large Scale Metal-Poor Filament due to Virial Shocking in the Halo of a Massive z=0.7 Galaxy
• Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
• Missing baryons traced by the galaxy luminosity density in the large-scale WHIM filaments
• Reconstructing the gravitational field of the local universe
• Supernovae and AGN driven galactic outflows
• The MillenniumTNG Project: An improved two-halo model for the galaxy-halo connection of red and blue galaxies
• Formation of disk galaxies in preheated media: a preventative feedback model
• The ACS Fornax Cluster Survey. III. Globular Cluster Specific Frequencies of Early-Type Galaxies
• 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
• Major Cluster Mergers and the Location of the Brightest Cluster Galaxy
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• Hierarchical Galaxy Growth and Scatter in the Stellar Mass - Halo Mass Relation
• The Morphology-Density-Relation: Impact on the Satellite Fraction
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• Stellar Velocity Dispersion: Linking Quiescent Galaxies to their Dark Matter Halos
• Connecting the Milky Way potential profile to the orbital timescales and spatial structure of the Sagittarius Stream
• On stellar mass loss from galaxies in groups and clusters
• Constraining Satellite Galaxy Stellar Mass Loss and Predicting Intrahalo Light I: Framework and Results at Low Redshift
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for Galaxy Clustering Measurements
• Upper Limit on the Milky Way Mass from the Orbit of the Sagittarius Dwarf Satellite
• The dependence of galaxy clustering on stellar mass, star-formation rate and redshift at z = 0.8-2.2, with HiZELS
• Spectroscopic failures in photometric redshift calibration: cosmological biases and survey requirements
• Internal kinematics of groups of galaxies in the Sloan Digital Sky Survey data release 7
• Exploring the halo occupation of AGN using dark-matter cosmological simulations
• Time Evolution of Galaxy Scaling Relations in Cosmological Simulations
• Physical Correlations of the Scatter between Galaxy Mass, Stellar Content, and Halo Mass
• The specific star formation rate and stellar mass fraction of low-mass central galaxies in cosmological simulations
• Stellar mass-gap as a probe of halo assembly history and concentration: youth hidden among old fossils
• Chandra Survey of Nearby Highly Inclined Disc Galaxies - III: Comparison with Hydrodynamical Simulations of Circumgalactic Coronae
• A 16 deg${}^2$ survey of emission-line galaxies at z<1.5 in HSC-SSP PDR1
• The Incomplete Conditional Stellar Mass Function: Unveiling the Stellar Mass Functions of Galaxies at 0.1 < Z < 0.8 from BOSS Observations
• BAM: Bias Assignment Method to generate mock catalogs
• Where stars form and live at high redshift: clues from the infrared
• Combining FOF and halo-based algorithms for the identification of galaxy groups
• 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
• The Mass-Concentration Relation and the Stellar-to-Halo Mass Ratio in the CFHT Stripe 82 Survey
• The growth of galactic bulges through mergers in LCDM haloes revisited. I. Present-day properties
• The clustering of X-ray selected AGN at z=0.1
• Central galaxies in different environments: Do they have similar properties?
• The galaxy - dark matter halo connection: which galaxy properties are correlated with the host halo mass?
• Massive black holes in central cluster galaxies
• A Statistical Semi-Empirical Model: Satellite galaxies in Groups and Clusters
• The role of gas infall in the evolution of disc galaxies
• HectoMAP and Horizon Run 4: Dense Structures and Voids in the Real and Simulated Universe
• A parametric study of possible solutions to the high-redshift overproduction of stars in modeled dwarf galaxies
• Galaxy downsizing evidenced by hybrid evolutionary tracks
• Revealing the Milky Way's Hidden Circumgalactic Medium with the Cosmic Origins Spectrograph Quasar Database for Galactic Absorption Lines
• The Red Dead Redemption Survey of Circumgalactic Gas About Massive Galaxies. I. Mass and Metallicity of the Cool Phase
• Does the Galaxy-Halo Connection Vary with Environment?
• Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
• The metallicity of galactic winds
• The Violent Youth of Bright and Massive Cluster Galaxies and their Maturation over 7 Billion Years
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• On the Angular Momentum History of Galactic Disks
• Cross-correlation of cosmic far-infrared background anisotropies with large scale structures
• Constraints on the evolution of the relationship between HI mass and halo mass in the last 12 Gyr
• Stellar mass -- halo mass relation for the brightest central galaxies of X-ray clusters since z~0.65
• Velocity Dispersions of Brightest Cluster Galaxies and Their Host Clusters
• The SLUGGS Survey: globular clusters and the dark matter content of early-type galaxies
• Beyond UVJ: Color Selection of Galaxies in the JWST Era
• The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
• Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
• The MillenniumTNG Project: Refining the one-halo model of red and blue galaxies at different redshifts
• The Impact of Environment on the Stellar Mass - Halo Mass Relation
• The effects of baryonic cooling on the concentration-mass relation
• A Comparison of Circumgalactic MgII Absorption between the TNG50 Simulation and the MEGAFLOW Survey
• The Milky Way system in LCDM cosmological simulations
• On the CGM Fundamental Plane: The Halo Mass Dependency of Circumgalactic HI
• A Galaxy Redshift Survey near HST/COS AGN Sight Lines
• Exploring the astrophysics of dark atoms
• A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The $(v_{\max },M_{\mathrm{DM}})$-$({\sigma }_0,M_{\mathrm{BH}},\varphi )$ Relations
• Precise Cosmological Constraints from BOSS Galaxy Clustering with a Simulation-Based Emulator of the Wavelet Scattering Transform
• Void Galaxies Follow a Distinct Evolutionary Path in the Environmental COntext Catalog
• The Brightest Galaxies at Cosmic Dawn from Scatter in the Galaxy Luminosity versus Halo Mass Relation
• Galaxy assembly bias of central galaxies in the Illustris simulation
• Reproducing cosmic evolution of galaxy population from $z=4$ to $0$
• Halo Mass Dependence of HI and OVI Absorption: Evidence for Differential Kinematics
• Mapping Dark Matter with Extragalactic Stellar Streams: the Case of Centaurus A
• FEASTS: IGM cooling triggered by tidal interactions through the diffuse HI phase around NGC 4631
• The Spectroscopy and H-band Imaging of Virgo cluster galaxies (SHIVir) Survey: Scaling Relations and the Stellar-to-Total Mass Relation
• 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
• [CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST
• 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
• A low pre-infall mass for the Carina dwarf galaxy from disequilibrium modelling
• The Molecular Gas Content of z<0.1 Radio Galaxies: Linking the AGN Accretion Mode to Host Galaxy Properties
• The scatter in the galaxy-halo connection: a machine learning analysis
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Stellar-to-halo mass relation of cluster galaxies
• The Missing Satellite Problem in 3D
• ZFIRE: The Evolution of the Stellar Mass Tully-Fisher Relation to Redshift 2.0 < Z < 2.5 with MOSFIRE
• The evolution of the galaxy content of dark matter haloes
• Simulating the H2 content of high-redshift galaxies
• A cosmological context for compact massive galaxies
• How gas flows shape the stellar-halo mass relation in the EAGLE simulation
• Linking haloes to galaxies: how many halo properties are needed?
• $\Lambda$CDM Predictions for the Satellite Population of M33
• The role of massive halos in the Star Formation History of the Universe
• Figuring Out Gas & Galaxies In Enzo (FOGGIE) VI: The Circumgalactic Medium of $L^{\ast }$ Galaxies is Supported in an Emergent, Non-Hydrostatic Equilibrium
• A Spatially-Resolved Survey of Distant Quasar Host Galaxies: I. Dynamics of galactic outflows
• The physical drivers of the atomic hydrogen-halo mass relation
• Probing hot gas around luminous red galaxies through the Sunyaev-Zel'dovich effect
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• Galaxy Pairs in the Local Group
• MusE GAs FLOw and Wind (MEGAFLOW) IV: A two sightline tomography of a galactic wind
• An ALMA survey of the SCUBA-2 Cosmology Legacy SurveyUKIDSS/UDS Field: Halo Masses for Submillimetre Galaxies
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• The distribution of satellites around massive galaxies at 1<z<3 in ZFOURGE/CANDELS: dependence on star formation activity
• ELUCID V. Lighting dark matter halos with galaxies
• Galaxy groups in the 2MASS Redshift Survey
• The ALPINE-ALMA [CII] Survey: On the nature of an extremely obscured serendipitous galaxy
• Halo Occupation Distribution Modeling of Green Valley Galaxies
• Probing high-redshift galaxies with Ly$\alpha$ intensity mapping
• Using Velocity Dispersion to Estimate Halo Mass: Is the Local Group in Tension with $\Lambda$CDM?
• The imprint of dark matter haloes on the size and velocity dispersion evolution of early-type galaxies
• What do simulations predict for the galaxy stellar mass function and its evolution in different environments?
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Constraining galactic structures of mirror dark matter
• Damped Lyα Absorption Systems in Semi-Analytic Models with Multiphase Gas
• Star-formation driven outflows in local dwarf galaxies as revealed from [CII] observations by Herschel
• Gravitational lens candidates in the E-CDFS
• The Next Generation Virgo Cluster Survey. IX. Estimating the Efficiency of Galaxy Formation on the Lowest-Mass Scales
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Implications of a variable IMF for the interpretation of observations of galaxy populations
• The growth of galactic bulges through mergers in LCDM haloes revisited. II. Morphological mix evolution
• High resolution near-infrared imaging of submillimeter galaxies
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• Are Some Milky Way Globular Clusters Hosted by Undiscovered Galaxies?
• Evidence of Galaxy Assembly Bias in SDSS DR7 Galaxy Samples from Count Statistics
• A question of separation: disentangling tracer bias and gravitational nonlinearity with counts-in-cells statistics
• The Circum-Galactic Medium of MASsive Spirals I: Overview and a Case Study of NGC 5908
• COSMOS2020: Identification of High-z Protocluster Candidates in COSMOS
• Unveiling the atomic hydrogen-halo mass relation via spectral stacking
• The Stripe 82 Massive Galaxy Project III: A Lack of Growth Among Massive Galaxies
• SDSS-IV MaNGA: Evidence for enriched accretion onto satellite galaxies in dense environments
• Stellar mass versus stellar velocity dispersion: which is better for linking galaxies to their dark matter halos?
• SHAM through the lens of a hydrodynamical simulation
• Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era
• Cosmological simulations of the same spiral galaxy: the impact of baryonic physics
• The bivariate gas-stellar mass distributions and the mass functions of early- and late-type galaxies at $z\sim 0$
• Merging galaxies produce outliers from the Fundamental Metallicity Relation
• The galaxy-halo size relation of low-mass galaxies in FIRE
• Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering
• CO($J$=1-0) mapping survey of 64 galaxies in the Fornax cluster with the ALMA Morita array
• Early Science with the Large Millimeter Telescope: Constraining the Gas Fraction of a Compact Quiescent Galaxy at z=1.883
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmic Flows and Cosmic Web from Luminous Red Galaxies
• Observational Measures of Halo Properties Beyond Mass
• Emission from the Ionized Gaseous Halos of Low Redshift Galaxies and Their Neighbors
• A Lyman limit system associated with galactic winds
• Construct the emission line galaxy-host halo connection through auto and cross correlations
• The halo mass function of late-type galaxies from HI kinematics
• Photometric Mass Estimation and the Stellar Mass-Halo Mass Relation for Low Mass Galaxies
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Generating Synthetic Cosmological Data with GalSampler
• Magnitude Gap Statistics and the Conditional Luminosity Function
• Detection of thermal Sunyaev-Zel'dovich Effect in the circumgalactic medium of low-mass galaxies -- a surprising pattern in self-similarity and baryon sufficiency
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Describing galaxy weak lensing measurements from tenths to tens of Mpc and up to z~0.6 with a single model
• A New Approach to Identifying the Most Powerful Gravitational Lensing Telescopes
• Beyond Ultra-diffuse Galaxies. I. Mass--Size Outliers among the Satellites of Milky Way Analogs
• Lyα emitters in a cosmological volume I: the impact of radiative transfer
• The Warm Circum-Galactic Medium: 10^5-6 K Gas Associated with a Single Galaxy Halo or with an Entire Group of Galaxies?
• Orbital decay of Globular Clusters in the galaxy with little dark matter
• Scaling relations for globular cluster systems in early-type galaxies
• Simulations of isolated dwarf galaxies formed in dark matter halos with different mass assembly histories
• The Clustering of X-ray Luminous Quasars
• Characterizing the local gamma-ray Universe via angular cross-correlations
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• A Bayesian Hierarchical Approach to Galaxy-Galaxy Lensing
• [OII] emitters in MultiDark-Galaxies and DEEP2
• Dark acoustic oscillations: Imprints on the matter power spectrum and the halo mass function
• Towards a higher mass for NGC1052-DF2: an analysis based on full distribution functions
• What galaxy masses perturb the local cosmic expansion?
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• The Thermal Sunyaev-Zel'dovich Effect from Massive, Quiescent 0.5 $\le$ z $\le$ 1.5 Galaxies
• Extended and Filamentary Lyman Alpha Emission from the Formation of a Protogalactic Halo at z=2.63
• Cosmic Near-infrared Background Tomography with SPHEREx Using Galaxy Cross-correlations
• Galaxy stellar mass assembly: the difficulty matching observations and semi-analytical predictions
• A scenario for ultra-diffuse satellite galaxies with low velocity dispersions: the case of [KKS 2000]04
• Constructing mock catalogues for the REFLEX II galaxy cluster sample
• Star Formation History in Barred Spiral Galaxies. AGN Feedback
• The Dynamics and Distribution of Angular Momentum in HiZELS Star-Forming Galaxies at z = 0.8 - 3.3
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Galaxy Ecosystems: gas contents, inflows and outflows
• The clustering of baryonic matter. I: a halo-model approach
• Subhaloes gone Notts: the clustering properties of subhaloes
• The dependence of subhalo abundance matching on galaxy photometry and selection criteria
• Quantifying Baryonic Feedback on Warm-Hot Circumgalactic Medium in CAMELS Simulations
• The SAMI -- Fornax Dwarfs Survey II: The Stellar Mass Fundamental Plane and the Dark Matter fraction of Dwarf Galaxies
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• Tracing stars in Milky Way satellites with A-SLOTH
• Main Sequence Scatter is Real: The Joint Dependence of Galaxy Clustering on Star Formation and Stellar Mass
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• Systematic uncertainties in models of the cosmic dawn
• MUSE-ALMA Halos VI: Coupling Atomic, Ionised & Molecular Gas Kinematics of Galaxies
• Formation and assembly history of stellar components in galaxies as a function of stellar and halo mass
• ELUCID -- Exploring the Local Universe with the reConstructed Initial Density field. II: Reconstruction diagnostics, applied to numerical halo catalogs
• Evolution of the Gas Mass Fraction of Progenitors to Today's Massive Galaxies: ALMA Observations in the CANDELS GOODS-S Field
• The trajectories of galaxies in groups: mass loss and preprocessing
• Metal enrichment in a semi-analytical model, fundamental scaling relations, and the case of Milky Way galaxies
• Cold and Hot gas distribution around the Milky-Way-M31 system in the HESTIA simulations
• BASS. XXXVI. Constraining the Local Supermassive Black Hole - Halo Connection with BASS DR2 AGN
• Improved Mock Galaxy Catalogs for the DEEP2 Galaxy Redshift Survey from Subhalo Abundance and Environment Matching
• Mass-to-Light Ratios of Spatially Resolved Stellar Populations in M31
• Mass and size growth of early-type galaxies by dry mergers in cluster environments
• How do galaxies populate halos in extreme density environments? An analysis of the Halo Occupation Distribution in SDSS
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• Modeling Redshift-Space Clustering with Abundance Matching
• New empirical constraints on the cosmological evolution of gas and stars in galaxies
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• The evolution of compact massive quiescent and starforming galaxies derived from the $R_e-R_h$ and $M_{\mathrm{star}}-M_h$ relations
• Constraints on the Evolution of the Galaxy Stellar Mass Function I: Role of Star Formation, Mergers and Stellar Stripping
• Effects of self-consistent rest-ultraviolet colours in semi-empirical galaxy formation models
• The Cosmological Constant in the Quantum Multiverse
• Phase spirals in cosmological simulations of Milky Way-size galaxies
• EDGE: Dark matter core creation depends on the timing of star formation
• Calibration of a star formation and feedback model for cosmological simulations with Enzo
• Stellar mass versus velocity dispersion as tracer of the lensing signal around bulge-dominated galaxies
• Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z<1.3
• Topology of Luminous Red Galaxies from the Sloan Digital Sky Survey
• A discrete chemo-dynamical model of M87's globular clusters: Kinematics extending to ~ 400 kpc
• Baryonic properties of nearby galaxies across the stellar-to-total dynamical mass relation
• Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
• A hot gaseous galaxy halo candidate with Mg X absorption
• A Study of Central Galaxy Rotation with Stellar Mass and Environment
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• Cosmic Web Dissection in Fuzzy Dark Matter Cosmologies
• 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
• 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
• Evidence for galaxy quenching in the green valley caused by a lack of a circumgalactic medium
• Momentum and energy injection by a supernova remnant into an inhomogeneous medium
• Galaxy Three-Point Correlation Functions and Halo/Subhalo Models
• The Circumgalactic Medium of Submillimeter Galaxies. I. First Results from a Radio-Identified Sample
• A minimal empirical model for the cosmic far-infrared background anisotropies
• Understanding the progenitor formation galaxies of merging binary black holes
• Testing galaxy formation models with galaxy stellar mass functions
• The Halo Occupation Distribution of Black Holes: Dependence on Mass
• Differentiable Predictions for Large Scale Structure with SHAMNet
• Investigating the $M_{GCS}-M_h$ Relation in the Most Massive Galaxies
• Estimates for the impact of Ultraviolet Background fluctuations on galaxy clustering measurements
• Galaxy And Mass Assembly (GAMA): The absence of stellar mass segregation in galaxy groups and consistent predictions from GALFORM and EAGLE simulations
• Constraining Dark Energy With Stacked Concave Lenses
• Constraining Scatter in the Stellar Mass--Halo Mass Relation for Haloes Less Massive than the Milky Way
• Tentative Detection of the Circumgalactic Medium of the Isolated Low-Mass Dwarf Galaxy WLM
• Detecting clusters and groups of galaxies populating the local Universe in large optical spectroscopic surveys
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• Constraining the scatter in the galaxy-halo connection at Milky Way masses
• An improved prescription for merger time-scales from controlled simulations
• Observational challenges in Ly-alpha intensity mapping
• Stochastic Processes as the Origin of the Double-Power Law Shape of the Quasar Luminosity Function
• Revised Mass-to-Light Ratios For Nearby Galaxy Groups and Clusters
• The relationship between gas and galaxies at z<1 using the Q0107 quasar triplet
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• PdBI Cold Dust Imaging of Two Extremely Red H-[4.5]>4 Galaxies Discovered with SEDS and CANDELS
• Dwarf Galaxy Discoveries from the KMTNet Supernova Program II. The NGC 3585 Group and Its Dynamical State
• Extremely Massive Quasars are not Good Proxies for Dense Environments Compared to Massive Galaxies: Environments of Extremely Massive Quasars and Galaxies
• ${\mu }_{\star }$ Masses: Weak Lensing Calibration of the Dark Energy Survey Year 1 redMaPPer Clusters using Stellar Masses
• Performance study of Lagrangian methods: reconstruction of large scale peculiar velocities and baryonic acoustic oscillations
• Constraining the subgrid physics in simulations of isolated dwarf galaxies
• Compatibility of the Large Quasar Groups with the Concordance Cosmological Model
• The Anisotropic Circumgalactic Medium of Massive Early-Type Galaxies
• Cuspy dark matter density profiles in massive dwarf galaxies
• Inferring the 3-D shapes of extremely metal-poor galaxies from sets of projected shapes
• Simulating Deep Hubble Images With Semi-empirical Models of Galaxy Formation
• Resolved Stellar Mass Maps of Galaxies in the Hubble Frontier Fields: Evidence for Mass Dependency in Environmental Quenching
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Evolution of CIV Absorbers. II. Where does CIV live?
• Distribution of Dust around Galaxies: An Analytic Model
• AGN and Star-Formation Properties of Inside-out Assembled Galaxy Candidates at z<0.1
• Explaining ultra-massive quiescent galaxies at $3<z<5$ in the context of their environments
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• The Uchuu-GLAM BOSS and eBOSS LRG lightcones: Exploring clustering and covariance errors
• Simulated stellar kinematics studies of high-redshift galaxies with the HARMONI Integral Field Spectrograph
• Chemical enrichment in isolated barred spiral galaxies
• How dark are filaments in the cosmic web?
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• Star formation histories of Coma Cluster galaxies matched to simulated orbits hint at quenching around first pericenter
• The Circumgalactic Medium in Massive Halos
• Cosmological feedback from a halo assembly perspective
• On the weak lensing masses of a new sample of galaxy groups
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• Abundance matching for low mass galaxies in the CDM and FDM models
• A Spatially-Resolved Survey of Distant Quasar Host Galaxies: II. Photoionization and Kinematics of the ISM
• $\text{PineTree}$: A generative, fast, and differentiable halo model for wide-field galaxy surveys
• A Two-Parameter Matching Scheme for Massive Galaxies and Dark Matter Haloes
• Galaxy luminosity functions at redshifts 0.6 to 1.2 in the Chandra Deep Field South
• Relating galaxies across different redshift to study galaxy evolution
• Can we use Weak Lensing to Measure Total Mass Profiles of Galaxies on 20 kiloparsec Scales?
• Rapid Simulations of Halo and Subhalo Clustering
• Linking galaxies to dark matter haloes at $z\sim 1$ : dependence of galaxy clustering on stellar mass and specific star formation rate
• The coevolution of the velocity and mass functions of galaxies and dark haloes
• Beyond Ultra-diffuse Galaxies. II. Environmental Quenching of Mass-Size Outliers among the Satellites of Milky Way Analogs
• Using large galaxy surveys to distinguish z~0.5 quiescent galaxy models
• Disk galaxies are self-similar: the universality of the HI-to-Halo mass ratio for isolated disks
• Inferring dark matter halo properties for HI-selected galaxies
• Using Strong Gravitational Lensing to Identify Fossil Group Progenitors
• A joint microlensing analysis of lensing mass and accretion disc models
• A quantitative demonstration that stellar feedback locally regulates galaxy growth
• Damped Lyman-$\alpha$ absorbers and atomic hydrogen in galaxies: the view of the GAEA model
• Exploring the Intrinsic Scatter of the Star-Forming Galaxy Main Sequence at redshift 0.5 to 3.0
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• Spritz is sparkling: simulated CO and [CII] luminosities
• 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
• The Population of Galaxies that Contribute to The HI Mass Function
• Cosmic evolution of the incidence of Active Galactic Nuclei in massive clusters: Simulations versus observations
• Galactic Outflows and Evolution of the Interstellar Medium
• The Dark Matter Halos of HI Selected Galaxies
• JWST + ALMA ubiquitously discover companion systems within $\lesssim 18$kpc around four $z$$\approx$3.5 luminous radio-loud AGN
• Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations
• Oxygen Loss from Simulated Galaxies and the Metal Flow Main Sequence: Predicting the Dependence on Mass and Environment
• Understanding the Fundamental Plane and the Tully Fisher Relation
• Molecular Gas of the Most Massive Spiral Galaxies I: a Case Study of NGC 5908
• The Close AGN Reference Survey (CARS): No evidence of galaxy-scale hot outflows in two nearby AGN
• Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
• FEASTS Combined with Interferometry. III. The Low Column Density HI Around M51 and Possibility of Turbulent-mixing Gas Accretion
• Constraining galaxy-halo connection with high-order statistics
• Galaxy populations in haloes in high-density environments
• The fundamental plane of evolving red nuggets
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• Semi-empirical catalog of early-type galaxy-halo systems: dark matter density profiles, halo contraction and dark matter annihilation strength
• Globular Cluster Counts around 700 Nearby Galaxies
• The dependence of cluster galaxy properties on the central entropy of their host cluster
• PRIMUS: The Effect of Physical Scale on the Luminosity-Dependence of Galaxy Clustering via Cross-Correlations
• Dynamics of Molecular Gas in the Central Region of the Quasar IZwicky1
• The evolution of galaxy scaling relations in clusters at 0.5<z<1.5
• Fast Forward Modelling of Galaxy Spatial and Statistical Distributions
• Baryonic Post-Processing of N-body Simulations, with Application to Fast Radio Bursts
• Correlations of the feedback energy and BCG radio luminosity in galaxy clusters
• The variation of the gas content of galaxy groups and pairs compared to isolated galaxies
• LARgE Survey -- II. The Dark Matter Halos and the Progenitors and Descendants of Ultra-Massive Passive Galaxies at Cosmic Noon
• Explaining JWST star formation history at $z\sim 17$ by modifying $\Lambda$CDM
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• NeutralUniverseMachine: How Filaments and Dark Matter Halo Influence the Galaxy Cold Gas Content
• Following the tidal trail: a history of modeling the Magellanic Stream
• Challenges in modeling the dark matter halo of NGC 1052-DF2: Cored versus cuspy halo models
• Do gravitational lens galaxies have an excess of luminous substructure?
• IMF-induced intrinsic uncertainties on measuring galaxy distances based on the number of giant stars: the case of the ultra-diffuse galaxy NGC 1052-DF2
• A Multi-messenger view of Cosmic Dawn: Conquering the Final Frontier
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Shape noise and dispersion in precision weak lensing
• Pair Lines of Sight Observations of Multiphase Gas Bearing O VI in a Galaxy Environment
• Galaxy-galaxy lensing in the VOICE deep survey
• Detecting episodes of star formation using Bayesian model selection
• Physical Models for the Clustering of Obscured and Unobscured Quasars
• Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS
• Void Lensing in Cubic Galileon Gravity
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• Does Gravity Fall Down? Evidence for Gravitational Wave Deflection Along the Line of Sight to GW 170817
• The spin of late-type galaxies at redshifts z < 1.2
• The galaxy counterpart of the high-metallicity and 16 kpc impact parameter DLA towards Q0918+1636 - a challenge to galaxy formation models?
• Central galaxy alignments. Dependence on the mass and the large-scale environment
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• Flattening of dark matter cusps during mergers: model of M31
• HST Hα grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation
• Searching for [CII] Emission from the First Sample of $z\sim 6$ OI Absorption-Associated Galaxies with ALMA
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• The impact of AGN X-ray selection on the AGN halo occupation distribution
• Evolving beyond z=0: insights about the future of stars and the intergalactic medium
• Spatial Distribution of OVI Covering Fractions in the Simulated Circumgalactic Medium
• Kinematics of Circumgalactic O VI Gas and Disk Rotation of $z\approx 0.2$ Star-forming Galaxies
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Clustering properties and halo masses for central galaxies in the local Universe
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• Modeling Strong Lenses from Wide-Field Ground-Based Observations in KiDS and GAMA
• A Galaxy-Halo Model for Multiple Cosmological Tracers
• An Empirical Mass Function Distribution
• Cosmic ray heating of intergalactic medium: patchy or uniform?
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Non-gaussianity of optical emission lines in SDSS star-forming galaxies and its implications on galactic outflows
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Not so-dark: High resolution HI imaging of J0139+4328 and identification of an optical counterpart
• ELG$\times$LRG distribution through dark matter halo dynamics
• Transforming galaxies with EASE: widespread structural changes enabled by short-lived spirals
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Effect of lensing magnification on type Ia supernova cosmology
• The Assembly of the Virgo Cluster, Traced by its Galaxy Halos
• MUSE observations of dwarf galaxies and a stellar stream in the M83 group
• Machine-guided Exploration and Calibration of Astrophysical Simulations
• The "Little Dark Dot": Evidence for Self-interacting Dark Matter in the Strong Lens SDSS J0946+1006?
• Fundamental relation in isolated galaxies, pairs, and triplets in the local universe
• Direct Shear Mapping: Prospects for weak lensing studies of individual galaxy-galaxy lensing systems
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Understanding Stellar Mass-Metallicity and Size Relations in Simulated Ultra-Faint Dwarf Galaxies
• Hubble Space Telescope Captures UGC~12591: Bulge/Disc Properties, Star Formation and `Missing Baryons' Census in a Very Massive and Fast Spinning Hybrid Galaxy
• The Diversity of Environments Around Luminous Quasars at Redshift $z\sim 6$
• SHAM-OT: Rapid Subhalo Abundance Matching with Optimal Transport
• Inferring halo masses with Graph Neural Networks
• Estimating the contribution of foreground halos to the FRB 180924 dispersion measure
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).III. Star formation in the stripped gas of NGC 4254
• Mapping luminous and dark matter in the Universe
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• CO-CHANGES II: spatially resolved IRAM 30M CO line observations of 23 nearby edge-on spiral galaxies
• Updated Models for the Creation of a Low-z QSO Absorber by a Dwarf Galaxy Wind
• Environmental Quenching of Low Surface Brightness Galaxies near Milky Way mass Hosts
• A sparse regression approach for populating dark matter halos and subhalos with galaxies
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• AGN with massive black holes have closer galactic neighbors: k-Nearest-Neighbor statistics of an unbiased sample of AGN at z~0.03
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• Probabilistic Inference of the Structure and Orbit of Milky Way Satellites with Semi-Analytic Modeling
• Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters
• Covariances of Galaxy Stellar Mass Functions and Correlation Functions
• JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations
• Measuring the Stellar-to-Halo Mass Relation at $\sim 10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses
• Modelling gas around galaxy pairs and groups using the Q0107 quasar triplet
• Angular momentum and morphological sequence of massive galaxies through Dark Sage
• The multi-component fitting to the star formation histories in the TNG simulation
• Dark matter in ALFALFA galaxies: Investigating galaxy-halo connection
• Predicting halo occupation and galaxy assembly bias with machine learning
• The invariance of group occupation across the cosmic web
• Renzo's rule revisited: A statistical study of galaxies' baryon - dark matter coupling
• Fuzzy dark matter dynamical friction: stalling of globular clusters induced by dynamical heatings
• Extragalactic Searches for Dark Matter Annihilation
• Higher resolution optical spectra of $M_{\ast }<10^{10}{M}_{\odot }$ galaxies reveal outflow signatures unresolved by the SDSS
• Resonant optical gating of suspended carbon nanotube transistor
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG
• Mimicking the halo-galaxy connection using machine learning
• The kinematic imprinting of environmental quenching in $z<0.2$ galaxies
• The orbital dynamics of the LMC and SMC about the Milky Way
• 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
• Testing subhalo abundance matching with galaxy kinematics
• Massive Neutrinos Promote the Size Growth of Early-Type Galaxies
• The NIKA2 cosmological legacy survey at 2 mm: catalogs, colors, redshift distributions, and implications for deep surveys