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

Abstract

Using data from the COSMOS survey, we perform the first joint analysis of galaxy-galaxy weak lensing, galaxy spatial clustering, and galaxy number densities. Carefully accounting for sample variance and for scatter between stellar and halo mass, we model all three observables simultaneously using a novel and self-consistent theoretical framework. Our results provide strong constraints on the shape and redshift evolution of the stellar-to-halo mass relation (SHMR) from z=0.2 to z=1. At low stellar mass, we find that halo mass scales as Mh M*^0.46 and that this scaling does not evolve significantly with redshift to z=1. We show that the dark-to-stellar ratio, Mh/M*, varies from low to high masses, reaching a minimum of Mh/M*~27 at M*=4.5x10^10 Msun and Mh=1.2x10^12 Msun. This minimum is important for models of galaxy formation because it marks the mass at which the accumulated stellar growth of the central galaxy has been the most efficient. We describe the SHMR at this minimum in terms of the "pivot stellar mass", M*piv, the "pivot halo mass", Mhpiv, and the "pivot ratio", (Mh/M*)piv. Thanks to a homogeneous analysis of a single data set, we report the first detection of mass downsizing trends for both Mhpiv and M*piv. The pivot stellar mass decreases from M*piv=5.75+-0.13x10^10 Msun at z=0.88 to M*piv=3.55+-0.17x10^10 Msun at z=0.37. Intriguingly, however, the corresponding evolution of Mhpiv leaves the pivot ratio constant with redshift at (Mh/M*)piv~27. We use simple arguments to show how this result raises the possibility that star formation quenching may ultimately depend on Mh/M* and not simply Mh, as is commonly assumed. We show that simple models with such a dependence naturally lead to downsizing in the sites of star formation. Finally, we discuss the implications of our results in the context of popular quenching models, including disk instabilities and AGN feedback.

31 pages, 18 figures, 5 tables. Submitted to ApJ. Comments welcome

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• Precise weak lensing constraints from deep high-resolution $K_{\mathrm{s}}$ images: VLT/HAWK-I analysis of the super-massive galaxy cluster RCS2$J$232727.7$-$020437 at $z=0.70$
• RESOLVE and ECO: The Halo Mass-Dependent Shape of Galaxy Stellar and Baryonic Mass Functions
• The evolution of galaxy intrinsic alignments in the MassiveBlack II universe
• Cosmological dependence of the measurements of luminosity function, projected clustering and galaxy-galaxy lensing signal
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• First Identification of a CMB Lensing Signal Produced by $1.5$ Million Galaxies at $z\sim$4: Constraints on Matter Density Fluctuations at High Redshift
• Galaxy-Mass Correlations on 10 Mpc Scales in the Deep Lens Survey
• The clustering of H$\beta$+[OIII] and [OII] emitters since $z\sim 5$: dependencies with line luminosity and stellar mass
• Generating Synthetic Cosmological Data with GalSampler
• The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
• Hosts and triggers of AGNs in the Local Universe
• Understanding the Unique Assembly History of Central Group Galaxies
• A New Approach to Identifying the Most Powerful Gravitational Lensing Telescopes
• Optimal filters for the moving lens effect
• The Cosmic Microwave Background and the Stellar Initial Mass Function
• Testing Galaxy Quenching Theories with Scatter in the Stellar to Halo Mass Relation
• The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• Galaxy stellar mass assembly: the difficulty matching observations and semi-analytical predictions
• hybrid-Lenstool: A self-consistent algorithm to model galaxy clusters with strong- and weak-lensing simultaneously
• The stellar mass in and around isolated central galaxies: connections to the total mass distribution through galaxy-galaxy lensing in the Hyper Suprime-Cam survey
• RedMaPPer: Evolution and Mass Dependence of the Conditional Luminosity Functions of Red Galaxies in Galaxy Clusters
• First Systematic Search for Oxygen-Line Blobs at High Redshift: Uncovering AGN Feedback and Star-Formation Quenching
• The Effect of Adiabatic Compression on Dark Matter Halos and the Radial Acceleration Relation
• A Bayesian Hierarchical Approach to Galaxy-Galaxy Lensing
• Primordial trispectrum from kSZ tomography
• The Spitzer South Pole Telescope Deep Field Survey: Linking galaxies and halos at z=1.5
• Imprints of gravitational lensing in the Planck CMB data at the location of WISExSCOS galaxies
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• Star formation and AGN activity in the most luminous LINERs in the local universe
• (DarkAI) Mapping the large-scale density field of dark matter using artificial intelligence
• On the mass assembly of low-mass galaxies in hydrodynamical simulations of structure formation
• Joint Analysis of Galaxy-Galaxy Lensing and Galaxy Clustering: Methodology and Forecasts for DES
• The distribution of dark matter and gas spanning six megaparsecs around the post-merger galaxy cluster MS0451-03
• Main Sequence Scatter is Real: The Joint Dependence of Galaxy Clustering on Star Formation and Stellar Mass
• Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
• Clustering Constraints on the Relative Sizes of Central and Satellite Galaxies
• Galaxies in X-ray Groups. III. Satellite Color and Morphology Transformations
• Maturing Satellite Kinematics into a Competitive Probe of the Galaxy-Halo Connection
• Towards a new modelling of gas flows in a semi-analytical model of galaxy formation and evolution
• Measuring the Geometry of the Universe from Weak Gravitational Lensing behind Galaxy Groups in the HST COSMOS survey
• The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters
• The COSMOS Density Field: A Reconstruction Using Both Weak Lensing and Galaxy Distributions
• Scaling relations for globular cluster systems in early-type galaxies. II. Is there an environmental dependence?
• The low dark matter content of the lenticular galaxy NGC 3998
• The evolution of compact massive quiescent and starforming galaxies derived from the $R_e-R_h$ and $M_{\mathrm{star}}-M_h$ relations
• The Diversity of Growth Histories of Milky Way-mass Galaxies
• Joint galaxy-galaxy lensing and clustering constraints on galaxy formation
• The Impacts of Modeling Choices on the Inference of the Circumgalactic Medium Properties from Sunyaev-Zeldovich Observations
• CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys
• Measuring Dark Matter in Galaxies: The Mass Fraction Within 5 Effective Radii
• The clustering of X-ray AGN at 0.5 < z < 4.5: host galaxies dictate dark matter halo mass
• The Baryonic Collapse Efficiency of Galaxy Groups in the RESOLVE and ECO Surveys
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Stellar mass versus velocity dispersion as tracer of the lensing signal around bulge-dominated galaxies
• The FMOS-COSMOS survey of star-forming galaxies at $z\sim 1.6$. V: Properties of dark matter halos containing H$\alpha$ emitting galaxies
• Globular Clusters: DNA of Early-Type galaxies?
• Bulge formation through disc instability -- I
• Merger-driven evolution of the effective stellar initial mass function of massive early-type galaxies
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• The Merian Survey: Design, Construction, and Characterization of a Filter Set Optimized to Find Dwarf Galaxies and Measure their Dark Matter Halo Properties with Weak Lensing
• Using galaxy pairs to investigate the three-point correlation function in the squeezed limit
• Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological $N$-body simulations
• The Luminosity Functions and Redshift Evolution of Satellites of Low-Mass Galaxies in the COSMOS Survey
• Do satellite galaxies trace matter in galaxy clusters?
• Satellite content and quenching of star formation in galaxy groups at z~1.8
• Cosmology with the thermal-kinetic Sunyaev-Zel'dovich effect
• On the link between nuclear star cluster and globular cluster system mass, nucleation fraction and environment
• Extremely Massive Quasars are not Good Proxies for Dense Environments Compared to Massive Galaxies: Environments of Extremely Massive Quasars and Galaxies
• A Cosmological Solution to the Impossibly Early Galaxy Problem
• Quantifying the abundance of faint, low-redshift satellite galaxies in the COSMOS survey
• CMB distortion from circumgalactic gas
• Uncorrelated Compensated Isocurvature Perturbations from kSZ Tomography
• Confronting semi-analytic galaxy models with galaxy-matter correlations observed by CFHTLenS
• Searching for dark matter annihilation from individual halos: uncertainties, scatter and signal-to-noise ratios
• Devouring the Milky Way Satellites: Modeling Dwarf Galaxies with Galacticus
• MOSFIRE and LDSS3 Spectroscopy for an [OII] Blob at z=1.18: Gas Outflow and Energy Source
• Distribution of Dust around Galaxies: An Analytic Model
• Star formation in high redshift galaxies including Supernova feedback: effect on stellar mass and luminosity functions
• An empirical model to form and evolve galaxies in dark matter halos
• AGN and Star-Formation Properties of Inside-out Assembled Galaxy Candidates at z<0.1
• Faint Dwarfs in Nearby Groups
• Can we use Weak Lensing to Measure Total Mass Profiles of Galaxies on 20 kiloparsec Scales?
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• A comparison of the R_h=ct and LCDM cosmologies based on the observed halo mass function
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• A close-pair analysis of damp mergers at intermediate redshifts
• The impact of correlated noise on galaxy shape estimation for weak lensing
• Reconciling Mass Functions with the Star-Forming Main Sequence Via Mergers
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Constraining the Galaxy-Halo Connection with Optimal Statistics
• Galaxy Halo Masses from Weak Gravitational Lensing
• Toward Accurate Modeling of Galaxy Clustering on Small Scales: Halo Model Extensions and Lingering Tension
• The XMM Cluster Survey: The Halo Occupation Number of BOSS galaxies in X-ray clusters
• The very wide-field $gzK$ galaxy survey -- II. The relationship between star-forming galaxies at $z\sim 2$ and their host haloes based upon HOD modelling
• Searches for Population III Pair-Instability Supernovae: Impact of Gravitational Lensing Magnification
• The Color and Stellar Mass Dependence of Small-scale Galaxy Clustering in SDSS-III BOSS
• A semi-analytic model of pairwise velocity distribution between dark matter halos
• Probing the circumgalactic baryons through cross-correlations
• Resolving the problem of galaxy clustering on small scales: any new physics needed?
• A New Stellar Mass Proxy for Subhalo Abundance Matching
• The ASTRID Simulation at z=0: From Massive Black Holes to Large-scale Structure
• PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at $0.2<z<0.9$
• Exploring galaxy dark matter halos across redshifts with strong quasar absorbers
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• A pseudo-spectrum analysis of galaxy-galaxy lensing
• Measuring Stellar Masses of Emission Line Galaxies at 1.2<z<1.9
• Investigating the Dark Matter Halo of NGC 5128 using a Discrete Dynamical Model
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• AGN lifetimes in UV-selected galaxies: a clue to supermassive black hole-host galaxy coevolution
• Do gravitational lens galaxies have an excess of luminous substructure?
• Subaru HSC weak lensing of SDSS redMaPPer cluster satellite galaxies: Empirical upper limit on orphan fractions
• Observations of Ly$\alpha$ Emitters at High Redshift
• Large-scale clustering of buried X-ray AGN: Trends in AGN obscuration and redshift evolution
• Subhalo abundance matching using progenitor mass at varying redshift: Two modes of stellar mass growth imprinted into the Subaru HSC galaxy clustering
• The size function of massive satellites from the $R_e-R_h$ and $M_{star}-M_h$ relations: constraining the role of environment
• Non-Gaussian assembly bias from a semi-analytic galaxy formation model
• The role of scatter and satellites in shaping the large-scale clustering of X-ray AGN as a function of host galaxy stellar mass
• Globular Cluster Systems and X-Ray Atmospheres in Galaxies
• Weak gravitational lensing as a probe of physical properties of substructures in dark matter halos
• The H$\alpha$ luminosity and stellar mass dependent clustering of star-forming galaxies at $0.7<z<1.5$ with 3D-HST
• Isolated dark matter deprived galaxies in hydrodynamical simulations: real objects or artefacts?
• Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
• Estimating lifetimes of uv-selected massive galaxies at $0.5\le z\le 2.5$ in the cosmos/ultravista field through clustering analyses
• A new way to measure the distance to NGC1052-DF2
• Retrieving the hot circumgalactic medium physics from the X-ray radial profile from eROSITA with an IlustrisTNG-based forward model
• The SRG/eROSITA All-Sky Survey. The Weak-Lensing Mass Calibration and the Stellar Mass-to-Halo Mass Relation from the Hyper Suprime-Cam Subaru Strategic Program
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Inferring Host Dark Matter Halo Masses of Individual Galaxies from Neighboring Galaxy Counts
• CLIMBER: Galaxy-Halo Connection Constraints from Next-Generation Surveys
• Direct Shear Mapping: Prospects for weak lensing studies of individual galaxy-galaxy lensing systems
• The Assembly of the Virgo Cluster, Traced by its Galaxy Halos
• Effects of Environment on the Size Evolution of Quiescent Galaxies: Comparing Galaxies in Clusters and in the Field at Two Rest-frame Wavelengths
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• The Dependence of Dark Matter Halo Properties on the Morphology of Their Central Galaxies from Weak Lensing
• The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
• Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data II: Hierarchical Bayesian Modeling of the Red-Sequence Galaxy Luminosity Function
• Covariances of Galaxy Stellar Mass Functions and Correlation Functions
• Lensing Without Borders. I. A Blind Comparison of the Amplitude of Galaxy-Galaxy Lensing Between Independent Imaging Surveys
• Angular correlation functions of bright Lyman-break galaxies at $3\lesssim \mathbf{z}\lesssim 5$
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• Hyper Suprime-Cam Y3 results: photo-$z$ bias calibration with lensing shear ratios and cosmological constraints from cosmic shear
• Exploiting Non-linear Scales in Galaxy-Galaxy Lensing and Galaxy Clustering: A Forecast for the Dark Energy Survey
• Dark matter halos of luminous AGNs from galaxy-galaxy lensing with the HSC Subaru Strategic Program
• A hierarchical clustering method for quantifying satellite abundance
• Massive Neutrinos Promote the Size Growth of Early-Type Galaxies
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• Revisiting the Constancy of the Speed of Light: Galaxy Cluster Mass Bias Implications
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
• A Novel Framework for Modeling Weakly Lensing Shear Using Kinematics and Imaging at Moderate Redshift