Galaxy halo masses and satellite fractions from galaxy-galaxy lensing in the SDSS: stellar mass, luminosity, morphology, and environment dependencies

Abstract

The relationship between galaxies and dark matter can be characterized by the halo mass of the central galaxy and the fraction of galaxies that are satellites. Here we present observational constraints from the SDSS on these quantities as a function of r-band luminosity and stellar mass using galaxy-galaxy weak lensing, with a total of 351,507 lenses. We use stellar masses derived from spectroscopy and virial halo masses derived from weak gravitational lensing to determine the efficiency with which baryons in the halo of the central galaxy have been converted into stars. We find that an L* galaxy with a stellar mass of 6x10^{10} M_{sun} is hosted by a halo with mass of 1.4x10^{12} M_{sun}/h, independent of morphology, yielding baryon conversion efficiencies of 17_{-5}^{+10} (early types) and 16_{-6}^{+15} (late types) per cent at the 95 per cent CL (statistical, not including systematic uncertainty due to assumption of a universal initial mass function, or IMF). We find that for a given stellar mass, the halo mass is independent of morphology below M_{stellar}=10^{11} M_{sun}, in contrast to typically a factor of two difference in halo mass between ellipticals and spirals at a fixed luminosity. This suggests that stellar mass is a good proxy for halo mass in this range and should be used preferentially whenever a halo mass selected sample is needed. For higher stellar masses, the conversion efficiency is a declining function of stellar mass, and the differences in halo mass between early and late types become larger, reflecting the fact that most group and cluster halos with masses above 10^{13} M_{sun} host ellipticals at the center, while even the brightest central spirals are hosted by halos of mass below 10^{13} M_{sun}. (Abridged)

arXiv comment19 pages, matches MNRAS accepted version

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• The Accretion of Gas onto Galaxies as Traced by their Satellites
• Satellite Kinematics I: A New Method to Constrain the Halo Mass-Luminosity Relation of Central Galaxies
• Calcium H & K Induced by Galaxy Halos
• Cosmic Evolution of Virial and Stellar Mass in Massive Early-Type Galaxies
• Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies
• Limits on the power-law mass and luminosity density profiles of elliptical galaxies from gravitational lensing systems
• TheHaloMod: An online calculator for the halo model
• Mapping stellar content to dark matter halos - III.Environmental dependence and conformity of galaxy colours
• Impact of the non-Gaussian covariance of the weak lensing power spectrum and bispectrum on cosmological parameter estimation
• Robust covariance estimation of galaxy-galaxy weak lensing: validation and limitation of jackknife covariance
• Rotation rates, sizes, and star formation efficiencies of a representative population of simulated disc galaxies
• Cosmic web dependence of galaxy clustering and quenching in SDSS
• The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation
• The Dark Matter Halos of Moderate Luminosity X-ray AGN as Determined from Weak Gravitational Lensing and Host Stellar Masses
• First measurement of the bulk flow of nearby galaxies using the cosmic microwave background
• Galaxy disc scaling relations: A tight linear galaxy -- halo connection challenges abundance matching
• The discovery of a significant sample of massive galaxies at redshifts 5 < z < 6 in the UKIDSS Ultra Deep Survey Early Data Release
• Probing the star formation history using the redshift evolution of luminosity functions
• Constraints on the merging timescale of luminous red galaxies, or, where do all the halos go?
• On the surface density of dark matter haloes
• The Dwarfs Beyond: The Stellar-to-Halo Mass Relation for a New Sample of Intermediate Redshift Low Mass Galaxies
• Elucidating Galaxy Assembly Bias in SDSS
• Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties
• 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
• COLD GASS, an IRAM Legacy Survey of Molecular Gas in Massive Galaxies: III. Comparison with semi-analytic models of galaxy formation
• Mapping the allowed parameter space for decaying dark matter models
• Galaxy and Mass Assembly (GAMA): galaxy radial alignments in GAMA groups
• Near-Infrared Properties of Moderate-Redshift Galaxy Clusters: Halo Occupation Number, Mass-to-Light Ratios and Omega_m
• Properties of simulated Milky Way-mass galaxies in loose group and field environments
• Galaxy density profiles and shapes -- II. selection biases in strong lensing surveys
• A tale of two populations: the stellar mass of central and satellite galaxies
• The evolution of the stellar mass versus halo mass relationship
• SHARP - I. A high-resolution multi-band view of the infra-red Einstein ring of JVAS B1938+666
• Supernovae and AGN driven galactic outflows
• CFHTLenS: The Environmental Dependence of Galaxy Halo Masses from Weak Lensing
• The Galaxy Stellar Mass Function of X-ray detected groups: environmental dependence of galaxy evolution in the COSMOS survey
• Probing Galaxy Dark Matter Haloes in COSMOS with Weak Lensing Flexion
• Major Cluster Mergers and the Location of the Brightest Cluster Galaxy
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• Modeling color-dependent galaxy clustering in cosmological simulations
• The effect of Warm Dark Matter on galaxy properties: constraints from the stellar mass function and the Tully-Fisher relation
• First Galaxy-Galaxy Lensing Measurement of Satellite Halo Mass in the CFHT Stripe-82 Survey
• Galaxy-galaxy weak-lensing measurement from SDSS: II. host halo properties of galaxy groups
• Revisiting the bulge-halo conspiracy I: Dependence on galaxy properties and halo mass
• The Morphology-Density-Relation: Impact on the Satellite Fraction
• A universal relation between the properties of supermassive black holes, galaxies, and dark matter halos
• Exploring the halo occupation of AGN using dark-matter cosmological simulations
• Internal kinematics of groups of galaxies in the Sloan Digital Sky Survey data release 7
• The Dark Matter Distributions in Low-Mass Disk Galaxies. II. The Inner Density Profiles
• The minor role of gas-rich major mergers in the rise of intermediate-mass early types at z <~ 1
• Evolution of central dark matter of early-type galaxies up to z ~ 0.8
• A List of Groups of Dwarf Galaxies in the Local Supercluster
• Halo stochasticity in global clustering analysis
• Dependence of GAMA galaxy halo masses on the cosmic web environment from 100 square degrees of KiDS weak lensing data
• Where stars form and live at high redshift: clues from the infrared
• Missing Dark Matter in the Local Universe
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• The galaxy-subhalo connection in low-redshift galaxy clusters from weak gravitational lensing
• Observations of dark and luminous matter: the radial distribution of satellite galaxies around massive red galaxies
• Simulating Supersonic Turbulence in Galaxy Outflows
• The Mass-Concentration Relation and the Stellar-to-Halo Mass Ratio in the CFHT Stripe 82 Survey
• Galaxy density profiles and shapes -- I. simulation pipeline for lensing by realistic galaxy models
• Strong orientation dependence of surface mass density profiles of dark haloes at large scales
• Central galaxies in different environments: Do they have similar properties?
• A weak gravitational lensing recalibration of the scaling relations linking the gas properties of dark halos to their mass
• Halo Concentration, Galaxy Red Fraction, and Gas Properties of Optically-defined Merging Clusters
• A weak lensing estimate from GEMS of the virial to stellar mass ratio in massive galaxies to z~0.8
• Modelling mass distribution in elliptical galaxies: mass profiles and their correlation with velocity dispersion profiles
• Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
• Dark matter dynamics in Abell 3827: new data consistent with standard Cold Dark Matter
• Evidence of Environmental Quenching at Redshift z ~ 2
• 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
• A scaling relation between merger rate of galaxies and their close pair count
• The 6dF Galaxy Survey: Dependence of halo occupation on stellar mass
• Cosmological Constraints from Galaxy Clustering and the Mass-to-Number Ratio of Galaxy Clusters: Marginalizing over the Physics of Galaxy Formation
• A measurement of galaxy halo mass from the surrounding HI Lyα absorption
• Gravitational lensing in the Supernova Legacy Survey (SNLS)
• The Correlated Formation Histories of Massive Galaxies and Their Dark Matter Halos
• The relation between stellar mass and weak lensing signal around galaxies: Implications for MOND
• The Milky Way system in LCDM cosmological simulations
• The Conditional Colour-Magnitude Distribution: I. A Comprehensive Model of the Colour-Magnitude-Halo Mass Distribution of Present-Day Galaxies
• First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. II. Faint end color-magnitude diagrams and radial profiles of red and blue galaxies at $0.1<z<1.1$
• PICS: Simulations of Strong Gravitational Lensing in Galaxy Clusters
• Specific Frequencies and Luminosity Profiles of Cluster Galaxies and Intracluster Light in Abell 1689
• Early-type galaxy density profiles from IllustrisTNG: II. Evolutionary trend of the total density profile
• Galaxy environments over cosmic time: the non-evolving radial galaxy distributions around massive galaxies since z=1.6
• On the Determination of Rotation Velocity and Dynamical Mass of Galaxies Based on Integrated H I Spectra
• The Spectroscopy and H-band Imaging of Virgo cluster galaxies (SHIVir) Survey: Scaling Relations and the Stellar-to-Total Mass Relation
• KiDS-i-800: Comparing weak gravitational lensing measurements in same-sky surveys
• The last 6 Gyr of dark matter assembly in massive galaxies from the Kilo Degree Survey
• The angular momentum of disc galaxies: implications for gas accretion, outflows, and dynamical friction
• Shapes of Stellar Systems and Dark Halos from Simulations of Galaxy Major Mergers
• The stellar mass - halo mass relation from galaxy clustering in VUDS: a high star formation efficiency at z~3
• CFHTLenS: Higher-order galaxy-mass correlations probed by galaxy-galaxy-galaxy lensing
• How to Optimally Constrain Galaxy Assembly Bias: Supplement Projected Correlation Functions with Count-in-cells Statistics
• Modeling Galaxy-Galaxy Weak Lensing with SDSS Groups
• Resolving the baryon-fraction profile in lensing galaxies
• $\Lambda$CDM Predictions for the Satellite Population of M33
• Linking haloes to galaxies: how many halo properties are needed?
• Dissecting the Red Sequence. IV. The Role of Truncation in the Two-Dimensional Family of Early-Type Galaxy Star Formation Histories
• The Mass Dependance of Satellite Quenching in Milky Way-like Halos
• Weak lensing in the Horizon-AGN simulation lightcone. Small scale baryonic effects
• Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• Improving PSF modelling for weak gravitational lensing using new methods in model selection
• 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
• The galaxy size - halo mass scaling relations and clustering properties of central and satellite galaxies
• Constraining the substructure of dark matter haloes with galaxy-galaxy lensing
• CFHTLenS: Weak lensing constraints on the ellipticity of galaxy-scale matter haloes and the galaxy-halo misalignment
• Weak-lensing-inferred scaling relations of galaxy clusters in the RCS2: mass-richness, mass-concentration, mass-bias, and more
• Bivariate Luminosity Function of Galaxy Pairs
• ZOMG II: Does the halo assembly history influence central galaxies and gas accretion?
• A Subhalo-Galaxy Correspondence Model of Galaxy Formation
• First detection of galaxy-galaxy-galaxy lensing in RCS. A new tool for studying the matter environment of galaxy pairs
• Probing the dark-matter halos of cluster galaxies with weak lensing
• Cross-correlation cosmic shear with the SDSS and VLA FIRST surveys
• Intergalactic Dust Extinction in Hydrodynamic Cosmological Simulations
• Mass-concentration relation of clusters of galaxies from CFHTLenS
• Gravitational lens candidates in the E-CDFS
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• The Galaxy Cross-Correlation Function as a Probe of the Spatial Distribution of Galactic Satellites
• Stellar mass versus stellar velocity dispersion: which is better for linking galaxies to their dark matter halos?
• Exploring Galaxy Formation Models and Cosmologies with Galaxy Clustering
• Real- and redshift-space halo clustering in $f(R)$ cosmologies
• Cosmological dependence of the measurements of luminosity function, projected clustering and galaxy-galaxy lensing signal
• On the scatter in the relation between stellar mass and halo mass: random or halo formation time dependent?
• The galaxy-halo size relation of low-mass galaxies in FIRE
• Can galaxy outflows and re-accretion produce the downsizing in specific star formation rate of late-type galaxies?
• Large Scale Structures in COSMOS2020: Evolution of Star Formation Activity in Different Environments at 0.4 < z < 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
• Measuring Dark Matter Substructure with Galaxy-Galaxy Flexion Statistics
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• TRGB distances to galaxies in front of the Virgo cluster
• Hosts and triggers of AGNs in the Local Universe
• Galaxy-Mass Correlations on 10 Mpc Scales in the Deep Lens Survey
• Magnitude Gap Statistics and the Conditional Luminosity Function
• Galaxy-galaxy weak gravitational lensing in $f(R)$ gravity
• Lyman-α Emitters in the context of hierarchical galaxy formation: predictions for VLT/MUSE surveys
• Dark Matter in Elliptical Galaxies
• Halo Properties and Mass Functions of Groups/Clusters from the DESI Legacy Imaging Surveys DR9
• Seeing in the dark -- I. Multi-epoch alchemy
• Stacked lensing estimators and their covariance matrices: Excess surface mass density vs. Lensing shear
• The degeneracy between star-formation parameters in dwarf galaxy simulations and the Mstar-Mhalo relation
• A deep Chandra observation of the hot gaseous halo around a rare, extremely massive and relativistic jet launching spiral galaxy
• On the occupation of X-ray selected galaxy groups by radio AGN since z=1.3
• The Dependence of Halo Mass on Galaxy Size at Fixed Stellar Mass Using Weak Lensing
• Testing redMaPPer centring probabilities using galaxy clustering and galaxy-galaxy lensing
• The Effect of Adiabatic Compression on Dark Matter Halos and the Radial Acceleration Relation
• Hydrostatic equilibrium profiles for gas in elliptical galaxies
• The Formation History of Subhalos and the Evolution of Satellite Galaxies
• DESCQA: An Automated Validation Framework for Synthetic Sky Catalogs
• A Bayesian Hierarchical Approach to Galaxy-Galaxy Lensing
• Dark acoustic oscillations: Imprints on the matter power spectrum and the halo mass function
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• The PAU Survey: Intrinsic alignments and clustering of narrow-band photometric galaxies
• Cosmological Studies from HSC-SSP Tomographic Weak Lensing Peak Abundances
• Tracer-Field Cross-Correlations with $k$-Nearest Neighbor Distributions
• The distribution of faint satellites around central galaxies in the CFHT Legacy Survey
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• What to expect from dynamical modelling of galactic haloes
• The massive dark halo of the compact, early-type galaxy NGC 1281
• The hot circumgalactic medium in the eROSITA All-Sky Survey III. Star-forming and quiescent galaxies
• What to expect from dynamical modelling of cluster haloes I. The information content of different dynamical tracers
• Constraining quasar host halo masses with the strength of nearby Lyman-alpha forest absorption
• Effects of center offset and noise on weak-lensing derived concentration-mass relation of dark matter halos
• The abundance of satellites depends strongly on the morphology of the host galaxy
• Tully-Fisher Distances and Dynamical Mass Constraints for 24 Host Galaxies of Reverberation-Mapped AGN
• The galaxy HI-(sub)halo connection and the HI spatial clustering of local galaxies
• Galaxy-Galaxy Weak Lensing Measurements from SDSS: I. Image Processing and Lensing signals
• Frequent Spin Reorientation of Galaxies due to Local Interactions
• Dark Matter Halo Mergers I: Dependence on Environment & Redshift Evolution
• Halo-Galaxy Lensing: A Full Sky Approach
• Biases on cosmological parameters by general relativity effects
• Stellar mass versus velocity dispersion as tracer of the lensing signal around bulge-dominated galaxies
• Towards an understanding of third-order galaxy-galaxy lensing
• Constraints on the velocity profiles of galaxies from strong lensing statistics and semi-analytical modelling of galaxy formation
• Connections between galaxy properties and halo formation time in the cosmic web
• Observational signatures of a static $f(R)$ black hole with thin accretion disk
• The strong environmental dependence of black hole scaling relations
• The Stellar-to-Halo Mass Ratios of Passive and Star-Forming Galaxies at z~2-3 from the SMUVS survey
• Not-so-little Red Dots: Two massive and dusty starbursts at z~5-7 pushing the limits of star formation discovered by JWST in the COSMOS-Web survey
• The importance of secondary halos for strong lensing in massive galaxy clusters across redshift
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• Galaxy-Galaxy Lensing by Non-Spherical Haloes I:Theoretical Considerations
• Galaxy luminosity function and Tully-Fisher relation: reconciled through rotation-curve studies
• Linear Systematics Mitigation in Galaxy Clustering in the Dark Energy Survey Year 1 Data
• How accurate is our knowledge of galaxy bias?
• Local Group Analogs in $\Lambda$CDM cosmological simulations
• Constraining warm dark matter mass with cosmic reionization and gravitational wave
• The Origin of the Relation Between Stellar Angular Momentum and Stellar Mass in Nearby Disk-dominated galaxies
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• Multiwavelength study of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A field
• Simulating the Anisotropic Clustering of Luminous Red Galaxies with Subhalos: A Direct Confrontation with Observation and Cosmological Implications
• Galaxy-Galaxy Lensing in EAGLE: comparison with data from 180 square degrees of the KiDS and GAMA surveys
• Testing a simple recipe for estimating galaxy masses from minimal observational data
• Confronting semi-analytic galaxy models with galaxy-matter correlations observed by CFHTLenS
• The bias of weighted dark matter halos from peak theory
• Constraining Halo Occupation Distribution and Cosmic Growth Rate using Multipole Power Spectrum
• Quiescent luminous red galaxies (LRGs) as cosmic chronometers: on the significance of mass and environmental dependence
• AGN and Star-Formation Properties of Inside-out Assembled Galaxy Candidates at z<0.1
• Evolution of CIV Absorbers. II. Where does CIV live?
• Velocity Dispersions of Massive Quiescent Galaxies from Weak Lensing and Spectroscopy
• Probing Hot Gas in Galaxy Groups through the Sunyaev-Zeldovich Effect
• Astrophysics in 2006
• RCSLenS: A new estimator for large-scale galaxy-matter correlations
• Studying Large and Small Scale Environments of Ultraviolet Luminous Galaxies
• Galaxy Halo Masses from Weak Gravitational Lensing
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• A close-pair analysis of damp mergers at intermediate redshifts
• A Universal Profile for Stacked Filaments from Cold Dark Matter Simulations
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• Multiple Weak Deflections in Galaxy-Galaxy Lensing
• From Halos to Galaxies. VI. Improved halo mass estimation for SDSS groups and measurement of the halo mass function
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• Testing modified gravity with motion of satellites around galaxies
• Galaxy And Mass Assembly (GAMA): Gas Fuelling of Spiral Galaxies in the Local Universe II. -- Direct Measurement of the Dependencies on Redshift and Host Halo Mass of Stellar Mass Growth in Central Disk Galaxies
• The central dark matter fraction of massive early-type galaxies
• Semi-empirical catalog of early-type galaxy-halo systems: dark matter density profiles, halo contraction and dark matter annihilation strength
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Weighing the Light Gravitino Mass with Weak Lensing Surveys
• Measurement of halo properties with weak lensing shear and flexion
• A pseudo-spectrum analysis of galaxy-galaxy lensing
• Dynamical cluster masses from photometric surveys
• The PAU Survey: Close galaxy pairs identification and analysis
• The quantity of dark matter in early-type galaxies and its relation to the environment
• Dark matter in massive galaxies
• COSMOS2020: Disentangling the Role of Mass and Environment in Star Formation Activity of Galaxies at $0.4<z<4$
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• Fitting functions for a disk-galaxy model with different LCDM-halo profiles
• Subaru HSC weak lensing of SDSS redMaPPer cluster satellite galaxies: Empirical upper limit on orphan fractions
• 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
• Galaxy-galaxy lensing in the VOICE deep survey
• Weak gravitational lensing as a probe of physical properties of substructures in dark matter halos
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• A multi-wavelength study of the gravitational lens COSMOS J095930+023427
• A comparison of the excess mass around CFHTLenS galaxy-pairs to predictions from a semi-analytic model using galaxy-galaxy-galaxy lensing
• The circular velocity and halo mass functions of galaxies in the nearby Universe
• A Framework for Measuring Weak-Lensing Magnification Using the Fundamental Plane
• Probing Satellite Halos with Weak Gravitational Lensing
• Unified dark matter: constraints from galaxies and clusters
• Clustering properties and halo masses for central galaxies in the local Universe
• A new way to measure the distance to NGC1052-DF2
• Testing Cotton gravity as dark matter substitute with weak lensing
• Measuring the gravitomagnetic distortion from rotating halos I: methods
• Dark haloes as seen with gravitational lensing
• BASILISK II. Improved Constraints on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Probing the shape and internal structure of dark matter halos with the halo-shear-shear three-point correlation function
• Inferring Host Dark Matter Halo Masses of Individual Galaxies from Neighboring Galaxy Counts
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• Direct Shear Mapping: Prospects for weak lensing studies of individual galaxy-galaxy lensing systems
• FPFS Shear Estimator: Systematic Tests on the Hyper Suprime-Cam Survey First Year Data
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• Impact of cosmic web on galaxy properties and their correlations: Insights from Principal Component Analysis
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Implications for the missing low-mass galaxies (satellites) problem from cosmic shear
• The Intergalactic Stellar Population from Mergers of Elliptical Galaxies with Dark Matter halos
• Examining early-type galaxy scaling relations using simple dynamical models
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Gravitational potential drives the concentration dependence of the stellar mass-halo mass relation
• Dark matter in ALFALFA galaxies: Investigating galaxy-halo connection
• Towards characterizing dark matter subhalo perturbations in stellar streams with graph neural networks
• Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red-Sequence Galaxy Luminosity Function
• Clustering Property of Wolf-Rayet Galaxies in the SDSS
• Hyper Suprime-Cam Y3 results: photo-$z$ bias calibration with lensing shear ratios and cosmological constraints from cosmic shear
• Game Theory in Cosmology
• Most Strong Lensing Deflectors in the AGEL Survey Are in Group and Cluster Environments
• The life and times of dark matter haloes: what will I be when I grow up?
• The Slow Growth of Massive Galaxies in Rapidly Growing Dark Matter Halos
• Characteristic Scales of Initial Density and Velocity Fields
• Morphological diversity of spiral galaxies originating in the cold gas inflow from cosmic webs
• Spikes in the SED and Ripples in the Outskirts of Galaxies
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
• Breaking down the link between luminous and dark matter in massive galaxies
• Effect of dust in circumgalactic haloes on the cosmic shear power spectrum
• Spacetime of rotating black holes surrounded by massive scalar charges