The Connection between Galaxies and their Dark Matter Halos

Abstract

In our modern understanding of galaxy formation, every galaxy forms within a dark matter halo. The formation and growth of galaxies over time is connected to the growth of the halos in which they form. The advent of large galaxy surveys as well as high-resolution cosmological simulations has provided a new window into the statistical relationship between galaxies and halos and its evolution. Here we define this galaxy-halo connection as the multi-variate distribution of galaxy and halo properties that can be derived from observations and simulations. This connection provides a key test of physical galaxy formation models; it also plays an essential role in constraints of cosmological models using galaxy surveys and in elucidating the properties of dark matter using galaxies. We review techniques for inferring the galaxy-halo connection and the insights that have arisen from these approaches. Some things we have learned are that galaxy formation efficiency is a strong function of halo mass; at its peak in halos around a pivot halo mass of 10^12 Msun, less than 20% of the available baryons have turned into stars by the present day; the intrinsic scatter in galaxy stellar mass is small, less than 0.2 dex at a given halo mass above this pivot mass; below this pivot mass galaxy stellar mass is a strong function of halo mass; the majority of stars over cosmic time were formed in a narrow region around this pivot mass. We also highlight key open questions about how galaxies and halos are connected, including understanding the correlations with secondary properties and the connection of these properties to galaxy clustering.

arXiv comment56 pages, 13 figures. Invited review, submitted to Annual Reviews of Astronomy & Astrophysics, Vol 56

References in corpus (271)

• Planck 2015 results. XIII. Cosmological parameters
• The Sloan Digital Sky Survey: Technical Summary
• A Universal Density Profile from Hierarchical Clustering
• The Seventh Data Release of the Sloan Digital Sky Survey
• The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• Large scale bias and the peak background split
• Populating a cluster of galaxies - I. Results at z=0
• The broken hierarchy of galaxy formation
• The 2dF Galaxy Redshift Survey: Spectra and redshifts
• The Optical and Near-Infrared Properties of Galaxies: I. Luminosity and Stellar Mass Functions
• Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
• The Formation of Galactic Disks
• Stable clustering, the halo model and nonlinear cosmological power spectra
• Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
• Halo Models of Large Scale Structure
• Simulating Galaxy Formation with the IllustrisTNG Model
• Hierarchical Galaxy Formation
• Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
• The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
• The observed properties of dwarf galaxies in and around the Local Group
• Toward a halo mass function for precision cosmology: the limits of universality
• Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
• Small-Scale Challenges to the $\Lambda$CDM Paradigm
• An analytic model for the spatial clustering of dark matter haloes
• The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
• The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores
• Galactic star formation and accretion histories from matching galaxies to dark matter haloes
• Physical Models of Galaxy Formation in a Cosmological Framework
• Observational Probes of Cosmic Acceleration
• 3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since $z=3$
• The Environmental Dependence of the Relations between Stellar Mass, Structure, Star Formation and Nuclear Activity in Galaxies
• Concentrations of Dark Halos from their Assembly Histories
• Constraints on the relationship between stellar mass and halo mass at low and high redshift
• A Semi-Analytic Model for the Co-evolution of Galaxies, Black Holes, and Active Galactic Nuclei
• Analytic model for galaxy and dark matter clustering
• Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi-LAT Data
• Semi-Analytic Modelling of Galaxy Formation: The Local Universe
• Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
• A Comprehensive Analysis of Uncertainties Affecting the Stellar Mass - Halo Mass Relation for 0<z<4
• Halo occupation numbers and galaxy bias
• Galaxy Groups in the SDSS DR4: I. The Catalogue and Basic Properties
• The Large Scale Bias of Dark Matter Halos: Numerical Calibration and Model Tests
• MultiDark simulations: the story of dark matter halo concentrations and density profiles
• The Dark Side of the Halo Occupation Distribution
• The Halo Occupation Distribution: Towards an Empirical Determination of the Relation Between Galaxies and Mass
• Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies
• Reionization and the abundance of galactic satellites
• Morphological Transformation from Galaxy Harassment
• Formation of Galaxy Clusters
• The Baryonic Tully-Fisher Relation
• The Luminosity and Color Dependence of the Galaxy Correlation Function
• Galaxy Clustering in the Completed SDSS Redshift Survey: The Dependence on Color and Luminosity
• Modeling Luminosity-Dependent Galaxy Clustering Through Cosmic Time
• redMaPPer I: Algorithm and SDSS DR8 Catalog
• Theoretical Challenges in Galaxy Formation
• Properties of Galaxy Groups in the SDSS: I.-- The Dependence of Colour, Star Formation, and Morphology on Halo Mass
• The Atlas3D project - XX. Mass-size and mass-sigma distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function
• The age dependence of halo clustering
• Galaxy formation in the Planck Cosmology - I. Matching the observed evolution of star formation rates, colours and stellar masses
• How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering
• Constraining Galaxy Formation and Cosmology with the Conditional Luminosity Function of Galaxies
• Linking halo mass to galaxy luminosity
• Galaxy evolution in groups and clusters: satellite star formation histories and quenching timescales in a hierarchical Universe
• Galaxy Evolution from Halo Occupation Distribution Modeling of DEEP2 and SDSS Galaxy Clustering
• Forming Disk Galaxies in Lambda CDM Simulations
• Stellar Feedback in Galaxies and the Origin of Galaxy-scale Winds
• The Dependence of Halo Clustering on Halo Formation History, Concentration, and Occupation
• Evolution of structure in cold dark matter universes
• PRIMUS: Constraints on Star Formation Quenching and Galaxy Merging, and the Evolution of the Stellar Mass Function From z=0-1
• Density profiles and substructure of dark matter halos: converging results at ultra-high numerical resolution
• New constraints on the evolution of the stellar-to-dark matter connection: a combined analysis of galaxy-galaxy lensing, clustering, and stellar mass functions from z=0.2 to z=1
• Galaxies in N-body simulations: overcoming the overmerging problem
• Connecting Galaxies, Halos, and Star Formation Rates Across Cosmic Time
• A hierarchy of voids: Much ado about nothing
• Spitzer view on the evolution of star-forming galaxies from z=0 to z~3
• Galaxy evolution in groups and clusters: star formation rates, red sequence fractions, and the persistent bimodality
• Galaxy ecology: groups and low-density environments in the SDSS and 2dFGRS
• K-band Properties of Galaxy Clusters and Groups: Brightest Cluster Galaxies and Intracluster Light
• The Nature of Galaxy Bias and Clustering
• The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues
• The spin and shape of dark matter haloes in the Millennium simulation of a LambdaCDM universe
• The effects of galaxy formation on the matter power spectrum: A challenge for precision cosmology
• A Halo-Based Galaxy Group Finder: Calibration and Application to the 2dFGRS
• A Stellar Mass Threshold for Quenching of Field Galaxies
• Making Galaxies in a Cosmological Context: The Need for Early Stellar Feedback
• Rotation-Dependent Catastrophic Disruption of Gravitational Aggregates
• Dependence of the outer density profiles of halos on their mass accretion rate
• EMERGE - An empirical model for the formation of galaxies since $z\sim 10$
• The haloes of bright satellite galaxies in a warm dark matter universe
• Dark matter and cosmic structure
• The properties and luminosity function of extremely low luminosity galaxies
• The Halo Occupation Distribution and the Physics of Galaxy Formation
• The distribution of stellar mass in the low-redshift Universe
• Weak lensing for precision cosmology
• On the Mass-to-Light Ratio of Large Scale Structure
• Gravitational detection of a low-mass dark satellite at cosmological distance
• Effects of Baryons and Dissipation on the Matter Power Spectrum
• The Connection between Galaxies and Dark Matter Structures in the Local Universe
• K-band Properties of Galaxy Clusters and Groups: Luminosity Function, Radial Distribution and Halo Occupation Number
• CFHTLenS: Combined probe cosmological model comparison using 2D weak gravitational lensing
• The redMaPPer Galaxy Cluster Catalog From DES Science Verification Data
• The MassiveBlack-II Simulation: The Evolution of Halos and Galaxies to z~0
• Evolution of the Galaxy - Dark Matter Connection and the Assembly of Galaxies in Dark Matter Halos
• Halo assembly bias and its effects on galaxy clustering
• Galaxy Groups in the SDSS DR4: II. halo occupation statistics
• Galaxy Groups in the SDSS DR4: III. the luminosity and stellar mass functions
• Detection of lensing substructure using ALMA observations of the dusty galaxy SDP.81
• Quantifying the effect of baryon physics on weak lensing tomography
• The Coyote Universe I: Precision Determination of the Nonlinear Matter Power Spectrum
• Disruption of Dark Matter Substructure: Fact or Fiction?
• On Departures From a Power Law in the Galaxy Correlation Function
• The splashback radius as a physical halo boundary and the growth of halo mass
• Stellar mass -- halo mass relation and star formation efficiency in high-mass halos
• Satellite Kinematics III: Halo Masses of Central Galaxies in SDSS
• Dark Matter Substructure in Numerical Simulations: A Tale of Discreteness Noise, Runaway Instabilities, and Artificial Disruption
• The clustering of massive galaxies at z~0.5 from the first semester of BOSS data
• Halo Assembly Bias in Hierarchical Structure Formation
• The Radial Distribution of Galaxies in LCDM clusters
• CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys
• Shredded Galaxies as the Source of Diffuse Intrahalo Light On Varying Scales
• Galactic Searches for Dark Matter
• The SAGA Survey: I. Satellite Galaxy Populations Around Eight Milky Way Analogs
• The Galaxy Content of SDSS Clusters and Groups
• KiDS+GAMA: Cosmology constraints from a joint analysis of cosmic shear, galaxy-galaxy lensing and angular clustering
• Time Delay Cosmography
• Galaxy Properties from the Ultra-violet to the Far-Infrared: Lambda-CDM models confront observations
• A Counts-in-Cells Analysis of Lyman-break Galaxies at z~3
• Cosmological Constraints from a Combination of Galaxy Clustering and Lensing -- I. Theoretical Framework
• The DEEP2 Galaxy Redshift Survey: Color and Luminosity Dependence of Galaxy Clustering at z~1
• The Hierarchical Build-Up of Massive Galaxies and the Intracluster Light since z=1
• A critical look at cosmological perturbation theory techniques
• Halo Occupation Distribution Modeling of Clustering of Luminous Red Galaxies
• Lensing is Low: Cosmology, Galaxy Formation, or New Physics?
• A new method to quantify the effects of baryons on the matter power spectrum
• Galaxy Assembly Bias: A Significant Source of Systematic Error in the Galaxy-Halo Relationship
• Dark Energy Survey Year 1 Results: Redshift distributions of the weak lensing source galaxies
• The pseudo-evolution of halo mass
• Evolution of the atomic and molecular gas content of galaxies
• The Dark Side of Galaxy Color
• Mapping stellar content to dark matter halos using galaxy clustering and galaxy-galaxy lensing in the SDSS DR7
• SubHaloes going Notts: The SubHalo-Finder Comparison Project
• Measurement of Galaxy Cluster Sizes, Radial Profiles, and Luminosity Functions from SDSS Photometric Data
• Modeling Galaxy-Mass Correlations in Dissipationless Simulations
• Galaxy Clustering & Galaxy-Galaxy Lensing: A Promising Union to Constrain Cosmological Parameters
• Reproducing the Stellar Mass/Halo Mass Relation in Simulated LCDM Galaxies: Theory vs Observational Estimates
• Cosmological Constraints from a Combination of Galaxy Clustering and Lensing -- III. Application to SDSS Data
• Galaxy clustering in the NEWFIRM Medium Band Survey: the relationship between stellar mass and dark matter halo mass at 1 < z < 2
• What aspects of galaxy environment matter?
• Tidal Effects and the Environment Dependence of Halo Assembly
• On Halo Formation Times and Assembly Bias
• Introducing Decorated HODs: modeling assembly bias in the galaxy-halo connection
• CFHTLenS: Co-evolution of galaxies and their dark matter haloes
• A Halo Model of Galaxy Colors and Clustering in the SDSS
• Halo Model at Its Best: Constraints on Conditional Luminosity Functions from Measured Galaxy Statistics
• Subhalo abundance matching and assembly bias in the EAGLE simulation
• The abundance of (not just) dark matter haloes
• A Re-examination of Galactic Conformity and a Comparison with Semi-analytic Models of Galaxy Formation
• A halo model for intrinsic alignments of galaxy ellipticities
• The Effective Number Density of Galaxies for Weak Lensing Measurements in the LSST Project
• The Kinematic Connection Between Galaxies and Dark Matter Haloes
• Evolution of bias in different cosmological models
• The Warm DM halo mass function below the cut-off scale
• The SL2S Galaxy-scale Lens Sample. V. Dark Matter Halos and Stellar IMF of Massive Early-type Galaxies out to Redshift 0.8
• Galaxy Halo Occupation at High Redshift
• A Critical Assessment of Stellar Mass Measurement Methods
• Star formation quenching in simulated group and cluster galaxies: When, how, and why?
• The Weak Lensing Signal and the Clustering of BOSS Galaxies II: Astrophysical and Cosmological Constraints
• Origin and evolution of halo bias in linear and non-linear regimes
• Tidal alignment of galaxies
• Cosmological Constraints from Galaxy Clustering and the Mass-to-Number Ratio of Galaxy Clusters
• The origin of scatter in the stellar mass - halo mass relation of central galaxies in the EAGLE simulation
• Towards Cosmological Concordance on Galactic Scales
• Satellite abundances around bright isolated galaxies
• Galaxy Mergers and Dark Matter Halo Mergers in LCDM: Mass, Redshift, and Mass-Ratio Dependence
• Mapping stellar content to dark matter halos. II. Halo mass is the main driver of galaxy quenching
• The Relationship between Galaxy and Dark Matter Halo Size from z~3 to the present
• Probing Dark Matter Haloes with Satellite Kinematics
• The Concentration Dependence of the Galaxy-Halo Connection: Modeling Assembly Bias with Abundance Matching
• Beyond Assembly Bias: Exploring Secondary Halo Biases for Cluster-size Haloes
• A theoretical framework for combining techniques that probe the link between galaxies and dark matter
• The 2dF-SDSS LRG and QSO survey: evolution of the clustering of luminous red galaxies since z = 0.6
• Sussing Merger Trees: The Merger Trees Comparison Project
• What Does Clustering Tell Us About the Buildup of the Red Sequence?
• Beyond Halo Mass: Galactic Conformity as a Smoking Gun of Central Galaxy Assembly Bias
• Statistics of Satellite Galaxies Around Milky Way-Like Hosts
• The stellar-to-halo mass relations of local galaxies segregates by color
• Individual Stellar Halos of Massive Galaxies Measured to 100 kpc at $0.3<z<0.5$ using Hyper Suprime-Cam
• A Comparison between Semi-Analytic Model Predictions for the CANDELS Survey
• A Bayesian approach to the semi-analytic model of galaxy formation: methodology
• The Dependence of Subhalo Abundance on Halo Concentration
• Halo-to-Halo Similarity and Scatter in the Velocity Distribution of Dark Matter
• Redshift-Space Distortions with the Halo Occupation Distribution II: Analytic Model
• On Detecting Halo Assembly Bias with Galaxy Populations
• Void Statistics in Large Galaxy Redshift Surveys: Does Halo Occupation of Field Galaxies Depend on Environment?
• A Study in Blue: The Baryon Content of Isolated Low Mass Galaxies
• The stellar-to-halo mass relation of GAMA galaxies from 100 square degrees of KiDS weak lensing data
• An analytic model for redshift-space distortions
• The Dark Side of Galaxy Color: evidence from new SDSS measurements of galaxy clustering and lensing
• Is Main Sequence Galaxy Star Formation Controlled by Halo Mass Accretion?
• The halo model and numerical simulations
• Quenching of Star Formation in SDSS Groups: Centrals, Satellites, and Galactic Conformity
• The Evidence of Absence: Galaxy Voids in the Excursion Set Formalism
• Assessing Colour-dependent Occupation Statistics Inferred from Galaxy Group Catalogues
• Simulations of galaxy formation in a cosmological volume
• Constraints on the mass-richness relation from the abundance and weak lensing of SDSS clusters
• The Accuracy of Subhalo Detection
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: modeling of the luminosity and colour dependence in the Data Release 10
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Luminosity and Color Dependence and Redshift Evolution
• Splashback Shells of Cold Dark Matter Halos
• The scale-dependence of relative galaxy bias: encouragement for the halo model description
• Observational Evidence for an Age Dependence of Halo Bias
• Evolution of the atomic and molecular gas content of galaxies in dark matter haloes
• Spatial Clustering of Dark Matter Halos: Secondary Bias, Neighbor Bias, and the Influence of Massive Neighbors on Halo Properties
• Which galaxies dominate the neutral gas content of the Universe?
• Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain Dark Energy
• The Real Space Correlation Function Measured from the APM Galaxy Survey
• Monte Carlo Markov Chain Parameter Estimation in Semi-Analytic Models of Galaxy Formation
• The Masses, Ancestors and Descendents of Extremely Red Objects: Constraints from Spatial Clustering
• Dark Energy Survey Year 1 Results: Cross-Correlation Redshifts - Methods and Systematics Characterization
• Reconstructing the Lensing Mass in the Universe from Photometric Catalogue Data
• From Galaxy-Galaxy Lensing to Cosmological Parameters
• The Tully-Fisher and mass-size relations from halo abundance matching
• Galaxy Formation at z~3: Constraints from Spatial Clustering
• ELUCID IV: Galaxy Quenching and its Relation to Halo Mass, Environment, and Assembly Bias
• Dissecting the Evolution of Dark Matter Subhaloes in the Bolshoi Simulation
• The clustering of luminous red galaxies at z $\sim$ 0.7 from eBOSS and BOSS data
• Modelling galaxy stellar mass evolution from z~0.8 to today
• Statistics of Dark Matter Substructure: III. Halo-to-Halo Variance
• Galaxy and Mass Assembly (GAMA): halo formation times and halo assembly bias on the cosmic web
• The clustering of SDSS galaxy groups: mass and color dependence
• Future constraints on halo thermodynamics from combined Sunyaev-Zel'dovich measurements
• A Search for Dark Matter Annihilation in Galaxy Groups
• The Redshift Evolution of the Mass Function of Cold Gas in Hierarchical Galaxy Formation Models
• Satellite Quenching and Galactic Conformity at 0.3 < z < 2.5
• Implications of Spikes in the Redshift Distribution of $z\sim 3$ Galaxies
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• Predicting Galaxy Star Formation Rates via the Co-evolution of Galaxies and Halos
• The Extreme Small Scales: Do Satellite Galaxies Trace Dark Matter?
• The Correlation Between Halo Mass and Stellar Mass for the Most Massive Galaxies in the Universe
• Modeling the three-point correlation function
• Testing Subhalo Abundance Matching in Cosmological Smoothed Particle Hydrodynamics Simulations
• Constraining the HI-Halo Mass Relation From Galaxy Clustering
• Halo Histories vs. Galaxy Properties at z=0 II: Large-Scale Galactic Conformity
• Mapping stellar content to dark matter halos - III.Environmental dependence and conformity of galaxy colours
• Connecting Direct Dark Matter Detection Experiments to Cosmologically Motivated Halo Models
• The Strikingly Similar Relation between Satellite and Central Galaxies and Their Dark Matter Halos Since z=2
• Rhapsody. II. Subhalo Properties and the Impact of Tidal Stripping From a Statistical Sample of Cluster-Size Halos
• Modelling The Redshift-Space Three-Point Correlation Function in SDSS-III
• Mapping Extragalactic Dark Matter Annihilation with Galaxy Surveys: A Systematic Study of Stacked Group Searches
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• On the galaxy-halo connection in the EAGLE simulation
• On the evidence for large-scale galactic conformity in the local Universe
• The Faber-Jackson relation and Fundamental Plane from halo abundance matching
• Halo Histories vs. Galaxy Properties at z=0, I: The Quenching of Star Formation
• PRIMUS: One- and Two-Halo Galactic Conformity at $0.2<z<1$
• The nature of assembly bias - III. Observational properties
• Cosmological Constraints from Galaxy Clustering and the Mass-to-Number Ratio of Galaxy Clusters: Marginalizing over the Physics of Galaxy Formation
• nIFTy Cosmology: the clustering consistency of galaxy formation models
• Towards Accurate Modelling of Galaxy Clustering on Small Scales: Testing the Standard $\Lambda \mathrm{CDM}$ + Halo Model
• Does the Milky Way Obey Spiral Galaxy Scaling Relations?
• Cosmic Shear as a Probe of Galaxy Formation Physics
• The Dependence of Halo Mass on Galaxy Size at Fixed Stellar Mass Using Weak Lensing
• Counts-in-Cylinders in the Sloan Digital Sky Survey with Comparisons to N-body Simulations
• Some observational tests of a minimal galaxy formation model
• Halo Histories vs. Galaxy Properties at z=0, III: The Properties of Star-Forming Galaxies
• The Clustering of Extremely Red Objects
• Group galaxy number density profiles far out: is the 'one-halo' term NFW out to $>10$ virial radii?

Cited by in corpus (562)

• UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10
• CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Data Calibration
• The distribution of dark matter in galaxies
• First measurement of the Hubble constant from a dark standard siren using the Dark Energy Survey galaxies and the LIGO/Virgo binary-black-hole merger GW170814
• A redshift-independent efficiency model: star formation and stellar masses in dark matter halos at z>4
• Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions
• Galaxy Formation and Reionization: Key Unknowns and Expected Breakthroughs by the James Webb Space Telescope
• The brightest galaxies at Cosmic Dawn
• Beyond linear galaxy alignments
• The LoTSS view of radio AGN in the local Universe. The most massive galaxies are always switched on
• The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation
• Corrfunc --- A Suite of Blazing Fast Correlation Functions on the CPU
• Milky Way Satellite Census. II. Galaxy--Halo Connection Constraints Including the Impact of the Large Magellanic Cloud
• COSMOS2020: The Galaxy Stellar Mass Function: the assembly and star formation cessation of galaxies at $0.2<z\le 7.5$
• The Clustering of DESI-like Luminous Red Galaxies Using Photometric Redshifts
• The SAGA Survey. II. Building a Statistical Sample of Satellite Systems around Milky Way-like Galaxies
• The stellar-to-halo mass relation over the past 12 Gyr
• Large-scale dark matter simulations
• Galaxy Stellar Mass Functions from z~10 to z~6 using the Deepest Spitzer/IRAC Data: No Significant Evolution in the Stellar-to-Halo Mass Ratio of Galaxies in the First Gyr of Cosmic Time
• Still Missing Dark Matter: KCWI High-Resolution Stellar Kinematics of NGC1052-DF2
• Dark Energy Survey Year 1 Results: Methods for Cluster Cosmology and Application to the SDSS
• The Universe at z>10: Predictions for JWST from the UniverseMachine DR1
• Stochastic modelling of star-formation histories II: star-formation variability from molecular clouds and gas inflow
• CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST
• Baryon Cycles in the Biggest Galaxies
• Semi-analytic forecasts for JWST -- II. physical properties and scaling relations for galaxies at z = 4-10
• The Diversity and Variability of Star Formation Histories in Models of Galaxy Evolution
• Galaxy formation in the Planck Millennium: the atomic hydrogen content of dark matter halos
• Shadows in the Dark: Low-Surface-Brightness Galaxies Discovered in the Dark Energy Survey
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• Quenching as a Contest between Galaxy Halos and their Central Black Holes
• Peak star formation efficiency and no missing baryons in massive spirals
• Cosmological Constraints on Dark Matter Interactions with Ordinary Matter
• CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
• Revealing the galaxy-halo connection in IllustrisTNG
• The specific angular momentum of disc galaxies and its connection with galaxy morphology, bar structure and disc gravitational instability
• Instability of Supersonic Cold Streams Feeding Galaxies IV: Survival of Radiatively Cooling Streams
• NuSTAR Tests of Sterile-Neutrino Dark Matter: New Galactic Bulge Observations and Combined Impact
• The cosmology dependence of galaxy clustering and lensing from a hybrid $N$-body-perturbation theory model
• COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5
• Quantifying scatter in galaxy formation at the lowest masses
• Consistent lensing and clustering in a low-$S_8$ Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000
• Going, going, gone dark: Quantifying the scatter in the faintest dwarf galaxies
• Hyper Suprime-Cam Subaru Strategic Program: A Mass-Dependent Slope of the Galaxy Size-Mass Relation at $z<1$
• Dissecting and Modelling Galaxy Assembly Bias
• Simulations and symmetries
• The Effect of Environment on Type Ia Supernovae in the Dark Energy Survey Three-Year Cosmological Sample
• Hydrodynamical Backflow in X-shaped Radio Galaxy PKS 2014-55
• The Three Causes of Low-Mass Assembly Bias
• The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics
• HI-MaNGA: HI Followup for the MaNGA Survey
• Mining for Dark Matter Substructure: Inferring subhalo population properties from strong lenses with machine learning
• Modeling the Connection Between Subhalos and Satellites in Milky Way-like Systems
• Predictions and Outcomes for the Dynamics of Rotating Galaxies
• CLASSY III: The Properties of Starburst-Driven Warm Ionized Outflows
• Trinity I: Self-Consistently Modeling the Dark Matter Halo-Galaxy-Supermassive Black Hole Connection from $z=0-10$
• Galactic Archaeology with Gaia
• EDGE: The origin of scatter in ultra-faint dwarf stellar masses and surface brightnesses
• Concentrations of Dark Haloes Emerge from Their Merger Histories
• Stringent ${\sigma }_8$ constraints from small-scale galaxy clustering using a hybrid MCMC+emulator framework
• Five-percent measurements of the growth rate from simulation-based modelling of redshift-space clustering in BOSS LOWZ
• Evidence for galaxy assembly bias in BOSS CMASS redshift-space galaxy correlation function
• CHIME/FRB Catalog 1 results: statistical cross-correlations with large-scale structure
• Warm Dark Matter Constraints Using Milky-Way Satellite Observations and Subhalo Evolution Modeling
• Tomographic measurement of the intergalactic gas pressure through galaxy-tSZ cross-correlations
• Semi-analytic forecasts for JWST -- VI. Simulated lightcones and galaxy clustering predictions
• The baryonic specific angular momentum of disc galaxies
• The Edge of the Galaxy
• COSMOS-Web: stellar mass assembly in relation to dark matter halos across $0.2<z<12$ of cosmic history
• Breaking degeneracies in the first galaxies with clustering
• The mass of our Galaxy from satellite proper motions in the Gaia era
• The galaxy-halo connection of emission-line galaxies in IllustrisTNG
• The Aemulus Project V: Cosmological constraint from small-scale clustering of BOSS galaxies
• Dynamical evidence for a morphology-dependent relation between the stellar and halo masses of galaxies
• Bright galaxy sample in the Kilo-Degree Survey Data Release 4: selection, photometric redshifts, and physical properties
• Empirical constraints on the formation of early-type galaxies
• New Roads to the Small-Scale Universe: Measurements of the Clustering of Matter with the High-Redshift UV Galaxy Luminosity Function
• Extensions to models of the galaxy-halo connection
• From lenticulars to blue compact dwarfs: the stellar mass fraction is regulated by disc gravitational instability
• SDSS-IV MaNGA: The kinematic-morphology of galaxies on the mass vs star-formation relation in different environments
• A Self-Calibrating Halo-Based Group Finder: Application to SDSS
• Mock Lightcones and Theory Friendly Catalogs for the CANDELS Survey
• The impact of gas disc flaring on rotation curve decomposition and revisiting baryonic and dark-matter relations for nearby galaxies
• Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies
• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• KiDS-1000: Combined halo-model cosmology constraints from galaxy abundance, galaxy clustering and galaxy-galaxy lensing
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for the eBOSS Emission Line Galaxy Sample
• The dependence of the galaxy stellar-to-halo mass relation on galaxy morphology
• Quasinormal modes of black holes embedded in halos of matter
• Constraining the Cosmic Baryon Distribution with Fast Radio Burst Foreground Mapping
• Galaxy disc scaling relations: A tight linear galaxy -- halo connection challenges abundance matching
• The manifestation of secondary halo bias on the galaxy population from IllustrisTNG300
• Baryonic Imprints on DM Halos: Population Statistics from Dwarf Galaxies to Galaxy Clusters
• The hot circumgalactic medium in the eROSITA All-Sky Survey I. X-ray surface brightness profiles
• Elucidating Galaxy Assembly Bias in SDSS
• Analytical models of supermassive black holes in galaxies surrounded by dark matter halos
• On the influence of halo mass accretion history on galaxy properties and assembly bias
• Evolution of Star-forming Galaxies from z = 0.7 to 1.2 with eBOSS Emission-line Galaxies
• Probing galaxy evolution in massive clusters using ACT and DES: splashback as a cosmic clock
• A machine learning approach to galaxy properties: joint redshift-stellar mass probability distributions with Random Forest
• Stellar Property Statistics of Massive Halos from Cosmological Hydrodynamics Simulations: Common Kernel Shapes
• The SRG/eROSITA All-Sky Survey: Dark Energy Survey Year 3 Weak Gravitational Lensing by eRASS1 selected Galaxy Clusters
• A machine learning approach to mapping baryons onto dark matter haloes using the EAGLE and C-EAGLE simulations
• GRUMPY: a simple framework for realistic forward-modelling of dwarf galaxies
• Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
• The Progenitors of Calcium-Strong Transients
• Bayesian field-level inference of primordial non-Gaussianity using next-generation galaxy surveys
• Rotation curves and scaling relations of extremely massive spiral galaxies
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• The evolution of the size-mass relation at $z$=1-3 derived from the complete Hubble Frontier Fields data set
• Baryons in the CosmicWeb of IllustrisTNG -- II: the Connection among Galaxies, Halos, their Formation Time and their Location in the Cosmic Web
• The LBT Satellites of Nearby Galaxies Survey (LBT-SONG): The Satellite Population of NGC 628
• Stellar mass as a galaxy cluster mass proxy: application to the Dark Energy Survey redMaPPer clusters
• The splashback radius of optically selected clusters with Subaru HSC Second Public Data Release
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• The first Super Massive Black Holes: indications from models for future observations
• A persistent excess of galaxy-galaxy strong lensing observed in galaxy clusters
• GALLUMI: A Galaxy Luminosity Function Pipeline for Cosmology and Astrophysics
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• The role of the cosmic web in the scatter of the galaxy stellar mass - gas metallicity relation
• Imaging Systematics and Clustering of DESI Main Targets
• On the halo-mass and radial scale dependence of the lensing is low effect
• ERGO-ML I: Inferring the assembly histories of IllustrisTNG galaxies from integral observable properties via invertible neural networks
• Updated Results on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Detection of anisotropic galaxy assembly bias in BOSS DR12
• NIHAO XXII: Introducing black hole formation, accretion and feedback into the NIHAO simulation suite
• Cross-Correlation of Planck CMB Lensing with DESI-Like LRGs
• Priors on red galaxy stochasticity from hybrid effective field theory
• Quenching and morphological evolution due to circumgalactic gas expulsion in a simulated galaxy with a controlled assembly history
• Spectral signatures of axionlike dark matter
• Constraints on $S_8$ from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS
• Controlling and leveraging small-scale information in tomographic galaxy-galaxy lensing
• New physics of strong interaction and Dark Universe
• The Red Dead Redemption Survey of Circumgalactic Gas About Massive Galaxies. I. Mass and Metallicity of the Cool Phase
• Galaxy sizes and the galaxy-halo connection -- I: the remarkable tightness of the size distributions
• RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• Forecasting [C II] line-intensity mapping measurements between the end of reionization and the epoch of galaxy assembly
• Stellar mass -- halo mass relation for the brightest central galaxies of X-ray clusters since z~0.65
• AGN Selection Methods Have Profound Impacts on the Distributions of Host Galaxy Properties
• Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
• Massive disc galaxies in cosmological hydrodynamical simulations are too dark matter-dominated
• Hubble Space Telescope Observations of Two Faint Dwarf Satellites of Nearby LMC Analogs from MADCASH
• Predicting dark matter halo formation in N-body simulations with deep regression networks
• Forecasts for Galaxy Formation and Dark Matter Constraints from Dwarf Galaxy Surveys
• Does Concentration Drive the Scatter in the Stellar-to-Halo Mass Relation of Galaxy Clusters?
• Dark matter halos and scaling relations of extremely massive spiral galaxies from extended HI rotation curves
• Probing Galaxy Assembly Bias in BOSS Galaxies Using Void Probabilities
• A High-Resolution Investigation of the Multi-Phase ISM in a Galaxy during the First Two Billion Years
• The DESI $N$-body Simulation Project I: Testing the Robustness of Simulations for the DESI Dark Time Survey
• [CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST
• First Constraints on Small-Scale Non-Gaussianity from UV Galaxy Luminosity Functions
• Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
• Probing gravity and growth of structure with gravitational waves and galaxies' peculiar velocity
• Extensions to the halo occupation distribution model for more accurate clustering predictions
• Superradiance of charged black holes embedded in dark matter halos
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• The physical origins of low-mass spin bias
• A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics
• The physical drivers of the atomic hydrogen-halo mass relation
• Shattering of Cosmic Sheets due to Thermal Instabilities: a Formation Channel for Metal-Free Lyman Limit Systems
• A dynamics-based density profile for dark haloes -- II. Fitting function
• Measurement of the B-band Galaxy Luminosity Function with Approximate Bayesian Computation
• On the prospect of using the maximum circular velocity of halos to encapsulate assembly bias in the galaxy-halo connection
• The cosmic web of X-ray active galactic nuclei seen through the eROSITA Final Equatorial Depth Survey (eFEDS)
• Thermal Instabilities and Shattering in the High-Redshift WHIM: Convergence Criteria and Implications for Low-Metallicity Strong HI Absorbers
• The Fundamental Relation between Halo Mass and Galaxy Group Properties
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• Hyper Suprime-Cam Low Surface Brightness Galaxies II: A Hubble Space Telescope Study of the Globular Cluster Systems of Ultra-Diffuse Galaxies in Groups
• Augmenting astrophysical scaling relations with machine learning: application to reducing the Sunyaev-Zeldovich flux-mass scatter
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• The SZ flux-mass ($Y$-$M$) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback
• Modeling Nearest Neighbor distributions of biased tracers using Hybrid Effective Field Theory
• Still at Odds with Conventional Galaxy Evolution: The Star Formation History of Ultra-Diffuse Galaxy Dragonfly 44
• Forecast of Neutrino Cosmology from the CSST Photometric Galaxy Clustering and Cosmic Shear Surveys
• SHAPing the Gas: Understanding Gas Shapes in Dark Matter Haloes with Interpretable Machine Learning
• From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
• Responses of Halo Occupation Distributions: a new ingredient in the halo model & the impact on galaxy bias
• Combination of cluster number counts and two-point correlations: Validation on Mock Dark Energy Survey
• The binary-host connection: astrophysics of gravitational wave binaries from their host galaxy properties
• Probing the galaxy-halo connection with total satellite luminosity
• The MillenniumTNG Project: The large-scale clustering of galaxies
• Clustering with JWST: Constraining Galaxy Host Halo Masses, Satellite Quenching Efficiencies, and Merger Rates at z=4-10
• Anisotropic halo assembly bias and redshift-space distortions
• The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
• Sensitivity of dark matter haloes to their accretion histories
• Relating the Diverse Merger Histories and Satellite Populations of Nearby Galaxies
• Diffstar: A Fully Parametric Physical Model for Galaxy Assembly History
• Imprints of Supermassive Black Hole Evolution on the Spectral and Spatial Anisotropy of Nano-Hertz Stochastic Gravitational-Wave Background
• Unveiling the atomic hydrogen-halo mass relation via spectral stacking
• The MillenniumTNG Project: Semi-analytic galaxy formation models on the past lightcone
• Flat Rotation Curves of $z\sim 1$ Star-Forming Galaxies and Evidence of Disk-Scale Length Evolution
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
• Evidence of Galaxy Assembly Bias in SDSS DR7 Galaxy Samples from Count Statistics
• The size-luminosity relation of lensed galaxies at $z=6-9$ in the Hubble Frontier Fields
• Suppressing cosmic variance with paired-and-fixed cosmological simulations: average properties and covariances of dark matter clustering statistics
• The galaxy-halo size relation of low-mass galaxies in FIRE
• SHAM through the lens of a hydrodynamical simulation
• First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
• Constructing high-fidelity halo merger trees in AbacusSummit
• Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• Missing Giants: Predictions on Dust-Obscured Galaxy Stellar Mass Assembly Throughout Cosmic Time
• Linear bias and halo occupation distribution of emission line galaxies from Nancy Grace Roman Space Telescope
• Observational Measures of Halo Properties Beyond Mass
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Aging Halos: Implications of the Magnitude Gap on Conditional Statistics of Stellar and Gas Properties of Massive Halos
• How Cosmic Rays Mediate the Evolution of the Interstellar Medium
• Hosts and triggers of AGNs in the Local Universe
• Dark Matter Density Profiles in Dwarf Galaxies: Linking Jeans Modeling Systematics and Observation
• What is Important? Morphological Asymmetries are Useful Predictors of Star Formation Rates of Star-forming Galaxies in SDSS Stripe 82
• Generating Synthetic Cosmological Data with GalSampler
• Photometric Mass Estimation and the Stellar Mass-Halo Mass Relation for Low Mass Galaxies
• Construct the emission line galaxy-host halo connection through auto and cross correlations
• Conditional HI mass functions and the HI-to-halo mass relation in the local Universe
• The oblateness of the Milky Way dark matter halo from the stellar streams of NGC 3201, M68, and Palomar 5
• From rest-frame luminosity functions to observer-frame colour distributions: tackling the next challenge in cosmological simulations
• Astrophysical Tests of Dark Matter Self-Interactions
• Stochastic Modelling of Star Formation Histories III. Constraints from Physically-Motivated Gaussian Processes
• The Last Journey. I. An Extreme-Scale Simulation on the Mira Supercomputer
• The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects
• The Aemulus Project VI: Emulation of beyond-standard galaxy clustering statistics to improve cosmological constraints
• pop-cosmos: A comprehensive picture of the galaxy population from COSMOS data
• RedMaPPer: Evolution and Mass Dependence of the Conditional Luminosity Functions of Red Galaxies in Galaxy Clusters
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• Taming assembly bias for primordial non-Gaussianity
• Galaxy and Mass Assembly: luminosity and stellar mass functions in GAMA groups
• AGN-driven quenching of satellite galaxies
• WEAVE-StePS. A stellar population survey using WEAVE at WHT
• The importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization
• A Review of Stable, Traversable Wormholes in f (R) Gravity Theories
• Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes
• Multiple Beads-on-a-string: Dark Matter-Deficient Galaxy Formation in a Mini-bullet Satellite-satellite Galaxy Collision
• Probing massive neutrinos with the Minkowski functionals of the galaxy distribution
• Tracer-Field Cross-Correlations with $k$-Nearest Neighbor Distributions
• The Bimodal Absorption System Imaging Campaign (BASIC) I. A Dual Population of Low-metallicity Absorbers at z $<1$
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• The dependence of subhalo abundance matching on galaxy photometry and selection criteria
• The assembly bias of emission line galaxies
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• Multiwavelength cluster mass estimates and machine learning
• An empirical measurement of the Halo Mass Function from the combination of GAMA DR4, SDSS DR12, and REFLEX II data
• Cosmology from weak lensing alone and implications for the Hubble tension
• Main Sequence Scatter is Real: The Joint Dependence of Galaxy Clustering on Star Formation and Stellar Mass
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• Maturing Satellite Kinematics into a Competitive Probe of the Galaxy-Halo Connection
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• The high-ionization IR fine-structure lines as bolometric indicators of the AGN power: study of the complete 12 micron AGN sample
• Constraining the mass density of free-floating black holes using razor-thin lensing arcs
• Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
• Tracing the Local Volume galaxy halo-to-stellar mass ratio with satellite kinematics
• Groups and protocluster candidates in the CLAUDS and HSC-SSP joint deep surveys
• Simulation view of galaxy clusters with low X-ray surface brightness
• The galaxy HI-(sub)halo connection and the HI spatial clustering of local galaxies
• Finding closure: approximating Vlasov-Poisson using finitely generated cumulants
• Machine-learning recovery of foreground wedge-removed 21-cm light cones for high-$z$ galaxy mapping
• The Dispersion Measure Contributions of the Cosmic Web
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• The evolution of compact massive quiescent and starforming galaxies derived from the $R_e-R_h$ and $M_{\mathrm{star}}-M_h$ relations
• The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine
• Cosmic Reionization On Computers: The Galaxy-Halo Connection between $5\le z\le 10$
• CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
• Generating mock galaxy catalogues for flux-limited samples like the DESI Bright Galaxy Survey
• Halo-model analysis of the clustering of photometric luminous red galaxies at $0.10\le z\le 1.05$ from the Subaru Hyper Suprime-Cam Survey
• Virial halo mass function in the $Planck$ cosmology
• An analytic model for the sub-galactic matter power spectrum in fuzzy dark matter halos
• The LEGA-C of nature and nurture in stellar populations of galaxies at z~0.6-1.0: D4000 and H-delta reveal different assembly histories for quiescent galaxies in different environments
• Baryonic properties of nearby galaxies across the stellar-to-total dynamical mass relation
• The galaxy - halo connection in low mass halos
• PANORAMIC: Discovery of an Ultra-Massive Grand-Design Spiral Galaxy at $z\sim 5.2$
• Explaining dark matter halo density profiles with neural networks
• HOD-Dependent Systematics for Luminous Red Galaxies in the DESI 2024 BAO Analysis
• Clustering dependence on Lyman-$\alpha$ luminosity from MUSE surveys at $3<z<6$
• Low-Surface-Brightness Galaxies are missing in the observed Stellar Mass Function
• A Versatile and Accurate Method for Halo Mass Determination from Phase-Space Distribution of Satellite Galaxies
• On the kinetic Sunyaev-Zel'dovich effect as an observational probe for halo spin bias
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. IV. High Precision Constraints on the Evolution of Stellar-Halo Mass Relation at Redshift $z<0.7$
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• Constraining the galaxy-halo connection of infrared-selected unWISE galaxies with galaxy clustering and galaxy-CMB lensing power spectra
• Do galaxy mergers prefer under-dense environments?
• The impact of environment on size: Galaxies are 50% smaller in the Fornax Cluster compared to the field
• How feedback shapes galaxies: an analytic model
• Detection of spatial clustering in the 1000 richest SDSS DR8 redMaPPer clusters with Nearest Neighbor distributions
• Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
• The High-Redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Radio Source Properties
• Revisiting the Extreme Clustering of $z\approx 4$ Quasars with Large Volume Cosmological Simulations
• 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
• Connecting SDSS central galaxies to their host halos using total satellite luminosity
• A multi-tracer empirically-driven approach to line-intensity mapping lightcones
• The First Billion Years in Seconds: An Effective Model for the 21-cm Signal with Population III Stars
• Constraining the scatter in the galaxy-halo connection at Milky Way masses
• Farpoint: A High-Resolution Cosmology Simulation at the Gigaparsec Scale
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• The Origin of the Relation Between Stellar Angular Momentum and Stellar Mass in Nearby Disk-dominated galaxies
• Signatures of dark and baryonic structures on weakly lensed gravitational waves
• Correlation function: biasing and fractal properties of the cosmic web
• Connecting galaxy structure and star formation: the role of environment in formation of S0 galaxies
• Biased tracer reconstruction with halo mass information
• Good and Proper: Self-similarity of N-body Simulations with Proper Force Softening
• Modelling the galaxy-halo connection with semi-recurrent neural networks
• Tracing the galaxy-halo connection with galaxy clustering in COSMOS-Web from z = 0.1 to z ~ 12
• The bright end of the galaxy luminosity function at $z\simeq 7$ from the VISTA VIDEO survey
• Constraining Dark Energy With Stacked Concave Lenses
• The influence of the void environment on the ratio of dark matter halo mass to stellar mass in SDSS MaNGA galaxies
• On the accuracy of dark matter halo merger trees and the consequences for semi-analytic models of galaxy formation
• Galaxy clustering from the bottom up: A Streaming Model emulator I
• The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years
• How the Galaxy-Halo Connection Depends on Large-Scale Environment
• The CGM-GRB Study. I. Uncovering The CircumGalactic Medium around GRB hosts at redshifts 2-6
• Mass-Velocity Dispersion Relation in HIFLUGCS Galaxy Clusters
• Galaxies and Halos on Graph Neural Networks: Deep Generative Modeling Scalar and Vector Quantities for Intrinsic Alignment
• ${\mu }_{\star }$ Masses: Weak Lensing Calibration of the Dark Energy Survey Year 1 redMaPPer Clusters using Stellar Masses
• 2D k-th nearest neighbor statistics: a highly informative probe of galaxy clustering
• SIDM Concerto: Compilation and Data Release of Self-interacting Dark Matter Zoom-in Simulations
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: I. Recent Star Formation Activity in Isolated Milky Way-Mass Galaxies
• Around the Spindle galaxy: the dark halo mass of NGC3115
• The Velocity Dispersion Function for Quiescent Galaxies in Nine Strong-Lensing Clusters
• Robust Clustering of the Local Milky Way Stellar Kinematic Substructures with Gaia eDR3
• Denser Environments Cultivate Larger Galaxies: A Comprehensive Study beyond the Local Universe with 3 Million Hyper Suprime-Cam Galaxies
• Growing the First Galaxies' Merger Trees
• High-fidelity reproduction of central galaxy joint distributions with Neural Networks
• The Beyond-Halo Mass Effects of the Cosmic Web Environment on Galaxies
• Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
• Galaxy populations in groups and clusters: evidence for a characteristic stellar mass scale at $M_{\ast }\sim 10^{9.5}{M}_{\odot }$
• Feedback and dynamical masses in high-$z$ galaxies: the advent of high-resolution NIRSpec spectroscopy
• Evolution of CIV Absorbers. II. Where does CIV live?
• Tracking the orbit of unresolved subhalos for semi-analytic models
• A Stochastic Theory of the Hierarchical Clustering I. Halo Mass Function
• Evolution of superclusters and supercluster cocoons in various cosmologies
• How dark are filaments in the cosmic web?
• Anisotropic Satellite Galaxy Quenching: A Unique Signature of Energetic Feedback by Supermassive Black Holes?
• Late-formed halos prefer to host quiescent central galaxies. I. Observational results
• Exploration of 3D wavelet scattering transform coefficients for line-intensity mapping measurements
• When Leaving the Solar System: Dark Matter Makes a Difference
• MAHGIC: A Model Adapter for the Halo-Galaxy Inter-Connection
• Tracing Dark Matter Halos with Satellite Kinematics and the Central Stellar Velocity Dispersion of Galaxies
• Revealing the Galaxy-Halo Connection Through Machine Learning
• Cosmological feedback from a halo assembly perspective
• Using the Modified Nearest Neighbor Method to Correct Fiber-collision Effects on Galaxy Clustering
• Quenching in the Right Place at the Right Time: Tracing the Shared History of Starbursts, AGNs, and Post-starburst Galaxies Using Their Structures and Multiscale Environments
• Orbital pericenters and the inferred dark matter halo structure of satellite galaxies
• PROBES-I: A Compendium of Deep Rotation Curves and Matched multiband Photometry
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Cold Gas in Massive Galaxies as A Critical Test of Black Hole Feedback Models
• Quantifying the effect of black hole feedback from the central galaxy on the satellite populations of groups and clusters
• The DESI One-Percent Survey: Modelling the clustering and halo occupation of all four DESI tracers with Uchuu
• Primordial monopolium as dark matter
• The dark side of galaxy stellar populations II: The dependence of star formation histories on halo mass and on the scatter of the main sequence
• Can Early Dark Energy be Probed by the High-Redshift Galaxy Abundance?
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic survey. II. Morphology, Color and Size Dependences of the Stellar-halo Mass Relation for Massive Galaxies
• Relating galaxies across different redshift to study galaxy evolution
• The biasing phenomenon
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Galaxy and Mass Assembly (GAMA): Tracing galaxy environment using the marked correlation function
• Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF
• Rapid Simulations of Halo and Subhalo Clustering
• The relationship between galaxy and halo sizes in the Illustris and IllustrisTNG simulations
• Inferring dark matter halo properties for HI-selected galaxies
• Characterizing the Conditional Galaxy Property Distribution using Gaussian Mixture Models
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• The Supersonic Project: The eccentricity and rotational support of SIGOs and DM GHOSts
• SDSS-IV MaNGA: The effect of stellar mass and halo mass on the assembly histories of satellite galaxies
• Exploring the Intrinsic Scatter of the Star-Forming Galaxy Main Sequence at redshift 0.5 to 3.0
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• From Halos to Galaxies. VI. Improved halo mass estimation for SDSS groups and measurement of the halo mass function
• Quantifying Observational Projection Effects with a Simulation-based hot CGM model
• Cosmology with Galaxy Cluster Properties using Machine Learning
• Constraining quenching timescales in galaxy clusters by forward-modelling stellar ages and quiescent fractions in projected phase space
• Stellar velocity dispersion and initial mass function gradients in dissipationless galaxy mergers
• The impact of the halo spin-concentration relation on disc scaling laws
• The Last Journey. II. SMACC -- Subhalo Mass-loss Analysis using Core Catalogs
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• A New Stellar Mass Proxy for Subhalo Abundance Matching
• Galaxy assembly bias in the stellar-to-halo mass relation for red central galaxies from SDSS
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• Hitting the mark: Optimising Marked Power Spectra for Cosmology
• Multiresolution angular momentum measurements of z~1.5-2 star-forming galaxies
• Accurate Modeling of the Projected Galaxy Clustering in Photometric Surveys: I. Tests with Mock Catalogs
• Fast Forward Modelling of Galaxy Spatial and Statistical Distributions
• The THESAN-ZOOM project: Star formation efficiency from giant molecular clouds to galactic scale in high-redshift starbursts
• Probing Reionization-Era Galaxies with JWST UV Luminosity Functions and Large-Scale Clustering
• SCONCE: A cosmic web finder for spherical and conic geometries
• The kinematic bimodality: Efficient feedback and cold gas deficiency in slow-rotating galaxies
• Investigating the Dark Matter Halo of NGC 5128 using a Discrete Dynamical Model
• The feasibility of constraining DM interactions with high-redshift observations by JWST
• MAMBO -- An empirical galaxy and AGN mock catalogue for the exploitation of future surveys
• Abundance matching tested on small scales with galaxy dynamics
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Probing modified Newtonian dynamics with hypervelocity stars
• Galaxy-halo size relation from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• Mid-IR cosmological spectrophotometric surveys from space: Measuring AGN and star formation at the Cosmic Noon with a SPICA-like mission
• An efficient and robust method to estimate halo concentration
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• Multi-wavelength consensus of large-scale linear bias
• Assembly bias evidence in close galaxy pairs
• A Pair of Early- and Late-Forming Galaxy Cluster Samples: a Novel Way of Studying Halo Assembly Bias Assisted by a Constrained Simulation
• MultiCAM: A multivariable framework for connecting the mass accretion history of haloes with their properties
• ScamPy -- A sub-halo clustering & abundance matching based Python interface for painting galaxies on the dark matter halo/sub-halo hierarchy
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• Time delay in the strong field limit for null and timelike signals and its simple interpretation
• Emission Line Predictions for Mock Galaxy Catalogues: a New Differentiable and Empirical Mapping from DESI
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• The dark matter halo masses of elliptical galaxies as a function of observationally robust quantities
• DarkAI: Reconstructing the density, velocity and tidal field of dark matter from a DESI-like bright galaxy sample
• Satellite galaxy abundance dependency on cosmology in Magneticum simulations
• Compact Binary Merger Rate with Modified Gravity in Dark-Matter Spikes
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Evaluating the variance of individual halo properties in constrained cosmological simulations
• Predictions for Detecting a Turndown in the Baryonic Tully Fisher Relation
• Measuring the growth of structure by matching dark matter haloes to galaxies with VIPERS and SDSS
• Total and dark mass from observations of galaxy centers with Machine Learning
• Intrinsic mass-richness relation of clusters from THE THREE HUNDRED hydrodynamic simulations
• The galaxy bias profile of cosmic voids
• Central galaxy alignments. Dependence on the mass and the large-scale environment
• Anisotropic effective redshift and evolving clustering amplitude
• On the Constraints of Galaxy Assembly Bias in Velocity Space
• Evaluating the origins of the secondary bias based on the correlation of halo properties with the linear density field
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• STRRINGS: STReams in Residual Images of Nearby GalaxieS
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• Can Dark Stars account for the star formation efficiency excess at very high redshifts?
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• Unexpected clustering pattern in dwarf galaxies challenges formation models
• Galaxy and halo properties around cosmic filaments from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• Baryon Pasting the Uchuu Lightcone Simulation
• Inferring Cosmological Parameters on SDSS via Domain-Generalized Neural Networks and Lightcone Simulations
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• Testing galaxy formation models with the stellar mass-halo mass relations for star-forming and quiescent galaxies
• Globular Cluster Systems and X-Ray Atmospheres in Galaxies
• The cosmological constant and scale hierarchies with emergent gauge symmetries
• The information on halo properties contained in spectroscopic observations of late-type galaxies
• Effect of some modified models of gravity on the radial velocity of binary systems
• Galaxy-galaxy lensing in the VOICE deep survey
• Impact of the turnover in the high-z galaxy luminosity function on the 21-cm signal during Cosmic Dawn and Epoch of Reionization
• Retrieving the hot circumgalactic medium physics from the X-ray radial profile from eROSITA with an IlustrisTNG-based forward model
• The THREEHUNDRED project: the effect of baryon processes at galaxy cluster scale
• Galaxy assembly bias and large-scale distribution: a comparison between IllustrisTNG and a semi-analytic model
• Dependence of the ratio of total to visible mass on observable properties of SDSS MaNGA galaxies
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Galaxy and Mass Assembly (GAMA): Probing galaxy-group correlations in redshift space with the halo streaming model
• The circular velocity and halo mass functions of galaxies in the nearby Universe
• Applying unsupervised learning to resolve evolutionary histories and explore the galaxy-halo connection in IllustrisTNG
• How do uncertainties in galaxy formation physics impact field-level galaxy bias?
• Tiny galaxies and dark substructures: exploring the "dark" subhaloes in TNG50
• The multi-wavelength Tully-Fisher relation in the TNG50 cosmological simulation
• A giant central red disk galaxy at redshift $z=0.76$: challenge to theories of galaxy formation
• Exploring HOD-dependent systematics for the DESI 2024 Full-Shape galaxy clustering analysis
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations
• An ultra-high-resolution map of (dark) matter
• Why the mean anomaly at epoch is not used in tests of non-Newtonian gravity?
• Galaxy Superclusters and Their Complexes in the Cosmic Web
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation
• Memoirs of mass accretion: probing the edges of intracluster light in simulated galaxy clusters
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Galaxy and Mass Assembly (GAMA): Mid-infrared properties as tracers of galaxy environment
• Galaxy Correlation Function and Local Density from Photometric Redshifts Using the Stochastic Order Redshift Technique (SORT)
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Hubble Space Telescope Captures UGC~12591: Bulge/Disc Properties, Star Formation and `Missing Baryons' Census in a Very Massive and Fast Spinning Hybrid Galaxy
• Cosmological prior for the $J$-factor estimation of dwarf spheroidal galaxies
• On the Dark Matter Halos of Optical and IR-selected AGN in the Local Universe
• Observing Correlations Between Dark Matter Accretion and Galaxy Growth: II. Testing the Impact of Galaxy Mass, Star Formation Indicator, and Neighbour Colours
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• The Gravitational Wave Bias Parameter from Angular Power Spectra: Bridging Between Galaxies and Binary Black Holes
• Hidden Figures in the Sky: Evolution of low-surface brightness galaxies from a hydro-dynamical perspective
• Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Low-density star cluster formation: discovery of a young faint fuzzy on the outskirts of the low-mass spiral galaxy NGC 247
• Deep Learning for direct Dark Matter search with nuclear emulsions
• Weak Gravitational Lensing
• Phenomenological power spectrum models for H$\alpha$ emission line galaxies from the Nancy Grace Roman Space Telescope
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• Supermassive black hole in NGC 4649 (M60) with a dark matter halo: Impact on shadow measurements and thermodynamic properties
• Probing the rapid formation of black holes and their galaxy hosts in QSOs
• Relativistic structure of a supermassive black hole embedded in the dark matter halo of NGC 4649 (M60)
• Cosmological nanolensing by dense gas clouds
• Assessing the connection between galactic conformity and assembly-type bias
• DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [OII] Luminosity
• DELVE Milky Way Satellite Galaxy Census I: Satellite Population and Survey Selection Function in DES, DELVE, and Pan-STARRS
• Bounds on galaxy stochasticity from halo occupation distribution modeling
• The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
• Extreme Galaxy-scale Outflows Are Frequent among Luminous Early Quasars
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
• Model Independent Dark Matter Properties from Cosmic Growth
• Relativistic positioning and Sagnac-like measurements for fundamental physics in space
• SHAM-OT: Rapid Subhalo Abundance Matching with Optimal Transport
• Searching for Particle Dark Matter with eROSITA Early Data
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Is cosmic dynamics self-regulating?
• On Dark Matter As A Geometric Effect in the Galactic Halo
• Exploring the halo-galaxy connection with probabilistic approaches
• On the origin of transient features in cosmological N-Body Simulations
• COUGS-DESI: A Catalog of Unusual Galaxies with Polar Structures in the DESI Legacy Imaging Surveys
• A stellar stream around the spiral galaxy Messier 61 in Rubin First Look imaging
• Inferring halo masses with Graph Neural Networks
• On the radial acceleration of disk galaxies
• Pair Counting without Binning -- A New Approach to Correlation Functions in Clustering Statistics
• Modes of the Dark Ages 21cm field accessible to a lunar radio interferometer
• Distinguishing Orbiting and Infalling Dark Matter Particles with Machine Learning
• Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies
• A Redshift Survey of the Coma Cluster (A1656): Understanding the Nature of Subhalos in the Weak-lensing Map
• Abundance and phase-space distribution of subhalos in cosmological N-body simulations: testing numerical convergence and correction methods
• Towards characterizing dark matter subhalo perturbations in stellar streams with graph neural networks
• The Origin of the Gas and Its Low Star Formation Efficiency in Quiescent Galaxies
• Cluster optical depth and pairwise velocity estimation using machine learning
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• Simultaneous Estimation of Large-Scale Structure and Milky Way Dust Extinction from Galaxy Surveys
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Investigation of mass substructure in gravitational lens system SDP.81 with ALMA long-baseline observations
• The invariance of group occupation across the cosmic web
• Simulation budgeting for hybrid effective field theories
• Galaxy assembly bias in cosmological hydrodynamical simulations: a comparison between SIMBA and IllustrisTNG
• Game Theory in Cosmology
• Gravitational potential drives the concentration dependence of the stellar mass-halo mass relation
• Pattern dark matter and galaxy scaling relations
• The S-PLUS Fornax Project (S+FP): An extragalactic catalog covering $\sim$ 5 virial radii around NGC 1399 with galaxy properties
• A systematic study of AGN feedback in a disk galaxy using MACER II: predictions of X-ray surface brightness profiles and comparison with eROSITA observations
• Probabilistic Inference of the Structure and Orbit of Milky Way Satellites with Semi-Analytic Modeling
• Galaxy clustering in modified gravity from full-physics simulations. I: two-point correlation functions
• Disk galaxies and their dark halos as self-organized patterns
• Toward accurate measurement of property-dependent galaxy clustering: II. Tests of the smoothed density-corrected $V_{\max }$ method
• A galaxy cluster in the innermost Zone of Avoidance, close to the radio phoenix VLSSJ2217.5+594
• Impact of a Rapid Diluted Energy Density on the halo mass function
• The catalogue of virtual early-type galaxies from IllustrisTNG: validation and real observation consistency
• Measuring the Stellar-to-Halo Mass Relation at $\sim 10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses
• Examining Baryonic Faber-Jackson Relation in Galaxy Groups
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• Luminosity Function of Galaxies in Voids: A Modification Inspired by Excursion Set Theory
• Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
• Tidal Grinding of Dwarf Galaxies in Cluster Environments
• Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging
• A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10
• Environmental Sculpting of Galaxy Structure at Fixed Stellar Mass: A Multi-Scale Analysis Across Cosmic Time using 3 Million HSC Galaxies
• Bound or blown: the fate of hot gas in galaxy groups
• Controlled Experiments on Dark-Matter Halo Structure and Galaxy Morphology I: What Sets Galaxy Sizes?
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• Cylindrical cosmological simulations with StePS
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
• Testing subhalo abundance matching with galaxy kinematics
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• Clustering analysis of medium-band selected high-redshift galaxies
• Mimicking the halo-galaxy connection using machine learning
• An Optimal In-Situ Multipole Algorithm for the Isotropic Three-Point Correlation Functions
• IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust
• The impact of the redshift-dependent selection effect of halos on the redshift-space power spectrum
• Correlation between Outlying Halo Abundance and Host Halo Properties
• Where's Swimmy?: Mining unique color features buried in galaxies by deep anomaly detection using Subaru Hyper Suprime-Cam data
• From the Fire: A Deeper Look at the Phoenix Stream
• The Delegate Survey: KOALA/AAOmega-IFU spectroscopy of three nearby dwarf galaxies
• Predicting Halo Formation Time Using Machine Learning
• The Baryonic Tully-Fisher Relation in the Local Group and the Equivalent Circular Velocity of Pressure Supported Dwarfs
• Extending the SAGA Survey (xSAGA) I: Satellite Radial Profiles as a Function of Host Galaxy Properties