The stellar-to-halo mass relation over the past 12 Gyr

Abstract

Understanding how galaxy properties are linked to the dark matter halos they reside in, and how they co-evolve is a powerful tool to constrain the processes related to galaxy formation. The stellar-to-halo mass relation (SHMR) and its evolution over the history of the Universe provides insights on galaxy formation models and allows to assign galaxy masses to halos in N-body dark matter simulations. We use a statistical approach to link the observed galaxy stellar mass functions on the COSMOS field to dark matter halo mass functions from the DUSTGRAIN simulation and from a theoretical parametrization from z=0 to z=4. We also propose an empirical model to describe the evolution of the stellar-to-halo mass relation as a function of redshift. We calculate the star-formation efficiency (SFE) of galaxies and compare results with previous works and semi-analytical models.

arXiv commentaccepted for publication in A&A, matching version in press

References in corpus (142)

• emcee: The MCMC Hammer
• Stellar population synthesis at the resolution of 2003
• A Universal Density Profile from Hierarchical Clustering
• Galactic Stellar and Substellar Initial Mass Function
• The Dust Content and Opacity of Actively Star-Forming Galaxies
• The Seventh Data Release of the Sloan Digital Sky Survey
• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• Efficient Computation of CMB anisotropies in closed FRW models
• Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• Populating a cluster of galaxies - I. Results at z=0
• The UKIRT Infrared Deep Sky Survey (UKIDSS)
• Stellar Masses and Star Formation Histories for 10^5 Galaxies from the Sloan Digital Sky Survey
• Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons
• Cosmological SPH simulations: A hybrid multi-phase model for star formation
• The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
• Stable clustering, the halo model and nonlinear cosmological power spectra
• The Cosmic Evolution Survey (COSMOS) -- Overview
• Accurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey
• The hierarchical formation of the brightest cluster galaxies
• New Insight on Galaxy Formation and Evolution from Keck Spectroscopy of the Hawaii Deep Fields
• Galactic star formation and accretion histories from matching galaxies to dark matter haloes
• Physical Models of Galaxy Formation in a Cosmological Framework
• Revisiting the Scaling Relations of Black Hole Masses and Host Galaxy Properties
• UniverseMachine: The Correlation between Galaxy Growth and Dark Matter Halo Assembly from z=0-10
• NYU-VAGC: a galaxy catalog based on new public surveys
• The ages and metallicities of galaxies in the local universe
• Constraints on the relationship between stellar mass and halo mass at low and high redshift
• The COSMOS2015 Catalog: Exploring the 1<z<6 Universe with half a million galaxies
• The Galaxy Luminosity Function and Luminosity Density at Redshift z=0.1
• Mass assembly in quiescent and star-forming galaxies since z=4 from UltraVISTA
• zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field
• A Comprehensive Analysis of Uncertainties Affecting the Stellar Mass - Halo Mass Relation for 0<z<4
• The Evolution of the Stellar Mass Functions of Star-Forming and Quiescent Galaxies to z = 4 from the COSMOS/UltraVISTA Survey
• What Shapes the Luminosity Function of Galaxies?
• UltraVISTA: a new ultra-deep near-infrared survey in COSMOS
• The Connection between Galaxies and their Dark Matter Halos
• Modeling Luminosity-Dependent Galaxy Clustering Through Cosmic Time
• Galaxy halo masses and satellite fractions from galaxy-galaxy lensing in the SDSS: stellar mass, luminosity, morphology, and environment dependencies
• Theoretical Challenges in Galaxy Formation
• Galaxy formation in the Planck Cosmology - I. Matching the observed evolution of star formation rates, colours and stellar masses
• The subhalo populations of LCDM dark haloes
• The Illustris simulation: the evolving population of black holes across cosmic time
• The stellar mass assembly of galaxies from z=0 to z=4. Analysis of a sample selected in the rest-frame near-infrared with Spitzer
• The Chandra Deep Field South: the 1 Million Second
• Galaxy Evolution from Halo Occupation Distribution Modeling of DEEP2 and SDSS Galaxy Clustering
• PRIMUS: Constraints on Star Formation Quenching and Galaxy Merging, and the Evolution of the Stellar Mass Function From z=0-1
• Mass, Metal, and Energy Feedback in Cosmological Simulations
• The Illustris Simulation: Public Data Release
• The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues
• zCOSMOS - 10k-bright spectroscopic sample. The bimodality in the Galaxy Stellar Mass Function: exploring its evolution with redshift
• Galaxy Stellar Mass Functions from ZFOURGE/CANDELS: An Excess of Low-Mass Galaxies Since z=2 and the Rapid Buildup of Quiescent Galaxies
• EMERGE - An empirical model for the formation of galaxies since $z\sim 10$
• Haloes gone MAD: The Halo-Finder Comparison Project
• The Galaxy Mass Function up to z=4 in the GOODS-MUSIC sample: into the epoch of formation of massive galaxies
• The distribution of stellar mass in the low-redshift Universe
• Statistical Analysis of Galaxy Surveys - I. Robust error estimation for 2-point clustering statistics
• The Evolutionary History of Lyman Break Galaxies Between Redshift 4 and 6: Observing Successive Generations of Massive Galaxies in Formation
• The Connection between Galaxies and Dark Matter Structures in the Local Universe
• The Many Manifestations of Downsizing: Hierarchical Galaxy Formation Models confront Observations
• K-band Properties of Galaxy Clusters and Groups: Luminosity Function, Radial Distribution and Halo Occupation Number
• The halo mass function from the dark ages through the present day
• Homogeneous Velocity-Distance Data for Peculiar Velocity Analysis. III. The Mark III Catalog of Galaxy Peculiar Velocities
• Evolution of the Galaxy - Dark Matter Connection and the Assembly of Galaxies in Dark Matter Halos
• The Evolution of the Galaxy Stellar Mass Function at z= 4-8: A Steepening Low-mass-end Slope with Increasing Redshift
• Stellar and total baryon mass fractions in groups and clusters since redshift 1
• Galaxy Cluster Baryon Fractions Revisited
• Stellar mass -- halo mass relation and star formation efficiency in high-mass halos
• The star formation histories of galaxies in the Sloan Digital Sky Survey
• Near-IR Properties of Galaxy Clusters: Luminosity as a Binding Mass Predictor and the State of Cluster Baryons
• The massive end of the luminosity and stellar mass functions: Dependence on the fit to the light profile
• Satellite Kinematics III: Halo Masses of Central Galaxies in SDSS
• The galaxy stellar mass function at 3.5<z<7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields
• Measuring the Redshift Evolution of Clustering: the Hubble Deep Field South
• The high redshift galaxy population in hierarchical galaxy formation models
• The universality of the virial halo mass function and models for non-universality of other halo definitions
• Semi-Analytic Galaxy Evolution (SAGE): Model Calibration and Basic Results
• Linking Early and Late Type Galaxies to their Dark Matter Haloes
• The Galaxy-Halo Connection Over The Last 13.3 Gyrs
• The MORGANA model for the rise of galaxies and active nuclei
• The stellar mass function of galaxies to z ~ 5 in the Fors Deep and GOODS-S fields
• The FourStar Galaxy Evolution Survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z~3.5
• Simulations of the galaxy population constrained by observations from z=3 to the present day: implications for galactic winds and the fate of their ejecta
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Full spectroscopic data and auxiliary information release (PDR-2)
• The VIMOS Public Extragalactic Redshift Survey (VIPERS): The growth of structures at $0.5<z<1.2$ from redshift-space distortions in the clustering of the PDR-2 final sample
• The mass of a halo
• CFHTLenS: The relation between galaxy dark matter haloes and baryons from weak gravitational lensing
• Satellite Kinematics II: The Halo Mass-Luminosity Relation of Central Galaxies in SDSS
• Galaxy assembly, stellar feedback and metal enrichment: the view from the GAEA model
• The Population of Dark Matter Subhaloes: Mass Functions and Average Mass Loss Rates
• A new model of galaxy formation: How sensitive are predicted galaxy luminosities to the choice of SPS model?
• Modified Gravity-GADGET: A new code for cosmological hydrodynamical simulations of modified gravity models
• An algorithm to build mock galaxy catalogues using MICE simulations
• Modelling galaxy clustering in a high resolution simulation of structure formation
• The onion universe: all sky lightcone simulations in spherical shells
• Cold gas properties of the Herschel Reference Survey. I. 12CO(1-0) and HI data
• The stellar mass fraction and baryon content of galaxy clusters and groups
• The origin of scatter in the stellar mass - halo mass relation of central galaxies in the EAGLE simulation
• Evolution in the Halo Masses of Isolated Galaxies between z~1 and z~0: From DEEP2 to SDSS
• Galaxy-galaxy Lensing: Dissipationless Simulations Versus the Halo Model
• The evolving slope of the stellar mass function at 0.6 <= z < 4.5 from deep WFC3 data
• The stellar mass function of the most massive galaxies at 3<=z<5 in the UKIDSS Ultra Deep Survey
• The intergalactic medium over the last 10 billion years I: Lyman alpha absorption and physical conditions
• Semi-Analytic Galaxies - I. Synthesis of environmental and star-forming regulation mechanisms
• The DEEP2 Galaxy Redshift Survey: Clustering of Quasars and Galaxies at z=1
• The DEEP2 Galaxy Redshift Survey: Clustering of Galaxies as a Function of Luminosity at z=1
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). A precise measurement of the galaxy stellar mass function and the abundance of massive galaxies at redshifts 0.5<z<1.3
• Rest-frame Ultraviolet-to-Optical Properties of Galaxies at z ~ 6 and 5 in the Hubble Ultra Deep Field: from Hubble to Spitzer
• The XXL Survey. XIII. Baryon content of the bright cluster sample
• The stellar-to-halo mass relations of local galaxies segregates by color
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Luminosity and stellar mass dependence of galaxy clustering at 0.5<z<1.1
• Peak star formation efficiency and no missing baryons in massive spirals
• The impact of baryonic physics on the subhalo mass function and implications for gravitational lensing
• A Deep Probe of the Galaxy Stellar Mass Functions at z~1-3 with the GOODS NICMOS Survey
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). Gravity test from the combination of redshift-space distortions and galaxy-galaxy lensing at $0.5<z<1.2$
• The subhalo - satellite connection and the fate of disrupted satellite galaxies
• The Hubble Space Telescope GOODS NICMOS Survey: Overview and the Evolution of Massive Galaxies at 1.5 < z < 3
• Galaxy formation in the Planck cosmology - IV. Mass and environmental quenching, conformity and clustering
• CosmoBolognaLib: C++ libraries for cosmological calculations
• Probing the galaxy-halo connection in UltraVISTA to $z\sim 2$
• Modelling galaxy stellar mass evolution from z~0.8 to today
• Weak Lensing Light-Cones in Modified Gravity simulations with and without Massive Neutrinos
• On ths assembly history of stellar components in massive galaxies
• The dynamics of tidal tails from massive satellites
• The evolution of quiescent galaxies at high redshift (z > 1.4)
• An analytical model for the accretion of dark matter subhalos
• Mass and Concentration estimates from Weak and Strong Gravitational Lensing: a Systematic Study
• Satellite Kinematics I: A New Method to Constrain the Halo Mass-Luminosity Relation of Central Galaxies
• EGG: hatching a mock Universe from empirical prescriptions
• The COSMOS-UltraVISTA stellar-to-halo mass relationship: new insights on galaxy formation efficiency out to $z\sim 5$
• Dark matter stripping in galaxy clusters: a look at the Stellar to Halo Mass relation in the Illustris simulation
• Internal kinematics of groups of galaxies in the Sloan Digital Sky Survey data release 7
• A Statistical Semi-Empirical Model: Satellite galaxies in Groups and Clusters
• The Impact of Gas Stripping and Stellar Mass Loss on Satellite Galaxy Evolution
• Estimating the galaxy two-point correlation function using a split random catalog
• Stellar mass -- halo mass relation for the brightest central galaxies of X-ray clusters since z~0.65
• Semi-Analytic Galaxies - II. Revealing the role of environmental and mass quenching in galaxy formation
• Cosmic CARNage I: on the calibration of galaxy formation models
• AGN feedback and the origin of the $\alpha$ enhancement in early type galaxies - insights from the GAEA model
• Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models
• Redshift-space distortions of galaxies, clusters and AGN: testing how the accuracy of growth rate measurements depends on scales and sample selections
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution

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• Dark matter halos of massive elliptical galaxies at $z\sim 0.2$ are well described by the Navarro-Frenk-White profile
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