CFHTLenS: Co-evolution of galaxies and their dark matter haloes

Abstract

Galaxy-galaxy weak lensing is a direct probe of the mean matter distribution around galaxies. The depth and sky coverage of the CFHT Legacy Survey yield statistically significant galaxy halo mass measurements over a much wider range of stellar masses ($10^{8.75}$ to $10^{11.3}{M}_{\odot }$) and redshifts ($0.2<z<0.8$) than previous weak lensing studies. At redshift $z\sim 0.5$, the stellar-to-halo mass ratio (SHMR) reaches a maximum of $4.0\pm 0.2$ percent as a function of halo mass at $\sim 10^{12.25}{M}_{\odot }$. We find, for the first time from weak lensing alone, evidence for significant evolution in the SHMR: the peak ratio falls as a function of cosmic time from $4.5\pm 0.3$ percent at $z\sim 0.7$ to $3.4\pm 0.2$ percent at $z\sim 0.3$, and shifts to lower stellar mass haloes. These evolutionary trends are dominated by red galaxies, and are consistent with a model in which the stellar mass above which star formation is quenched "downsizes" with cosmic time. In contrast, the SHMR of blue, star-forming galaxies is well-fit by a power law that does not evolve with time. This suggests that blue galaxies form stars at a rate that is balanced with their dark matter accretion in such a way that they evolve along the SHMR locus. The redshift dependence of the SHMR can be used to constrain the evolution of the galaxy population over cosmic time.

18 pages, MNRAS, in press

References in corpus (10)

• Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
• Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
• PRIMUS: Constraints on Star Formation Quenching and Galaxy Merging, and the Evolution of the Stellar Mass Function From z=0-1
• Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -I. Methodology and a Fast Fitting Algorithm
• Analytic models of plausible gravitational lens potentials
• Satellite abundances around bright isolated galaxies
• Evolution of the Stellar-to-Dark Matter Relation: Separating Star-Forming and Passive Galaxies from z=1 to 0
• Dark Matter Halos in Galaxies and Globular Cluster Populations
• Bayesian Galaxy Shape Measurement for Weak Lensing Surveys -II. Application to Simulations
• Truncation of galaxy dark matter halos in high density environments

Cited by in corpus (134)

• The Connection between Galaxies and their Dark Matter Halos
• EMERGE - An empirical model for the formation of galaxies since $z\sim 10$
• NIHAO project I: Reproducing the inefficiency of galaxy formation across cosmic time with a large sample of cosmological hydrodynamical simulations
• Weak lensing for precision cosmology
• Stellar mass -- halo mass relation and star formation efficiency in high-mass halos
• The distribution of dark matter in galaxies
• Mapping stellar content to dark matter halos using galaxy clustering and galaxy-galaxy lensing in the SDSS DR7
• Strong bimodality in the host halo mass of central galaxies from galaxy-galaxy lensing
• Dark matter halo properties of GAMA galaxy groups from 100 square degrees of KiDS weak lensing data
• Galactic Dark Matter Halos and Globular Cluster Populations. III: Extension to Extreme Environments
• The galaxy-halo connection from a joint lensing, clustering and abundance analysis in the CFHTLenS/VIPERS field
• Extending the Globular Cluster System-Halo Mass Relation to the Lowest Galaxy Masses
• The impact of stellar feedback on the structure, size and morphology of galaxies in Milky Way size dark matter haloes
• Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data
• Galaxy-galaxy lensing estimators and their covariance properties
• Dark Energy Survey Year 1 Results: Galaxy-Galaxy Lensing
• Satellite quenching timescales in clusters from projected phase space measurements matched to simulated orbits
• The Next Generation Virgo Cluster Survey (NGVS). XXX. Ultra-Diffuse Galaxies and their Globular Cluster Systems
• The Eating Habits of Milky Way Mass Halos: Destroyed Dwarf Satellites and the Metallicity Distribution of Accreted Stars
• The stellar-to-halo mass relation of GAMA galaxies from 100 square degrees of KiDS weak lensing data
• Dark Matter Halos in Galaxies and Globular Cluster Populations. II: Metallicity and Morphology
• Is Main Sequence Galaxy Star Formation Controlled by Halo Mass Accretion?
• NIHAO IX: the role of gas inflows and outflows in driving the contraction and expansion of cold dark matter haloes
• Galaxy and Mass Assembly (GAMA): The halo mass of galaxy groups from maximum-likelihood weak lensing
• Relations Between the Sizes of Galaxies and their Dark Matter Halos at Redshifts $0<z<3$
• The Dramatic Size and Kinematic Evolution of Massive Early-Type Galaxies
• Testing the theory of gravity with DESI: estimators, predictions and simulation requirements
• Intrinsic alignments of BOSS LOWZ galaxies II: Impact of shape measurement methods
• Cosmology from large scale galaxy clustering and galaxy-galaxy lensing with Dark Energy Survey Science Verification data
• Precision Scaling Relations for Disk Galaxies in the Local Universe
• Origins of scaling relations of globular cluster systems
• The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
• Cosmological constraints from galaxy-lensing cross correlations using BOSS galaxies with SDSS and CMB lensing
• GalaxyNet: Connecting galaxies and dark matter haloes with deep neural networks and reinforcement learning in large volumes
• The eROSITA Final Equatorial Depth Survey (eFEDS): X-ray emission around star-forming and quiescent galaxies at $0.05<z<0.3$
• Galaxy-Galaxy Lensing in the DES Science Verification Data
• The Weak Lensing Masses of Filaments between Luminous Red Galaxies
• NIHAO XII: galactic uniformity in a ΛCDM universe
• Dynamical evidence for a morphology-dependent relation between the stellar and halo masses of galaxies
• Quenching low-mass satellite galaxies: evidence for a threshold ICM density
• The physical nature of the cosmic accretion of baryons and dark matter into halos and their galaxies
• Cosmological Galaxy Evolution with Superbubble Feedback II: The Limits of Supernovae
• The correlation between the sizes of globular cluster systems and their host dark matter haloes
• Testing gravity on large scales by combining weak lensing with galaxy clustering using CFHTLenS and BOSS CMASS
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• Evolution of Star-forming Galaxies from z = 0.7 to 1.2 with eBOSS Emission-line Galaxies
• New constraints on ${\sigma }_8$ from a joint analysis of stacked gravitational lensing and clustering of galaxy clusters
• The evolution of the stellar mass versus halo mass relationship
• New Analytic Solutions for Galaxy Evolution: Gas, Stars, Metals and Dust in local Early-Type Galaxies and in their high-z Starforming Progenitors
• KROSS-SAMI: A Direct IFS Comparison of the Tully-Fisher Relation Across 8 Gyr Since $z\approx 1$
• The Morphology-Density-Relation: Impact on the Satellite Fraction
• Exploring the halo occupation of AGN using dark-matter cosmological simulations
• Where did the globular clusters of the Milky Way form? Insights from the E-MOSAICS simulations
• Clearing the hurdle: The mass of globular cluster systems as a function of host galaxy mass
• The Mass-Concentration Relation and the Stellar-to-Halo Mass Ratio in the CFHT Stripe 82 Survey
• Globular clusters as tracers of the dark matter halo: insights from the E-MOSAICS simulations
• Globular clusters as tracers of the dark matter content of dwarfs in galaxy clusters
• How are galaxies assigned to halos? Searching for assembly bias in the SDSS galaxy clustering
• Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
• Accreted or Not Accreted? The Fraction of Accreted Mass in Galaxies from Simulations and Observations
• Specific Frequencies and Luminosity Profiles of Cluster Galaxies and Intracluster Light in Abell 1689
• The Spectroscopy and H-band Imaging of Virgo cluster galaxies (SHIVir) Survey: Scaling Relations and the Stellar-to-Total Mass Relation
• The Galaxy--Halo Connection in High-Redshift Universe: Details and Evolution of Stellar-to-Halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields
• Stellar-to-halo mass relation of cluster galaxies
• Simulating the Spatial Distribution and Kinematics of Globular Clusters within Galaxy Clusters in Illustris
• Cosmic CARNage I: on the calibration of galaxy formation models
• CODEX Weak Lensing: Concentration of Galaxy Clusters at z ~ 0.5
• A Photometric Survey of Globular Cluster Systems in Brightest Cluster Galaxies
• Weak lensing in the Horizon-AGN simulation lightcone. Small scale baryonic effects
• GAMA+KiDS: Empirical correlations between halo mass and other galaxy properties near the knee of the stellar-to-halo mass relation
• CFHTLenS: Weak lensing constraints on the ellipticity of galaxy-scale matter haloes and the galaxy-halo misalignment
• The SLUGGS survey: Exploring the globular cluster systems of the Leo II group and their global relationships
• The Galaxy-Halo Connection for $1.5\lesssim z\lesssim 5$ as revealed by the \emph{Spitzer} Matching survey of the UltraVISTA ultra-deep Stripes
• Probing the galaxy-halo connection with total satellite luminosity
• The Impact of Interpixel Capacitance in CMOS Detectors on PSF shapes and Implications for WFIRST
• Entropy Driven Winds: Outflows and Fountains Lifted Gently by Buoyancy
• The Next Generation Virgo Cluster Survey. IX. Estimating the Efficiency of Galaxy Formation on the Lowest-Mass Scales
• Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82
• The dark side of galaxy stellar populations I: The stellar-to-halo mass relation and the velocity dispersion - halo mass relation
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• Stellar Mass Function of Active and Quiescent Galaxies via the Continuity Equation
• Preprocessing, mass loss and mass segregation of galaxies in DM simulations
• ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System
• The Dependence of Halo Mass on Galaxy Size at Fixed Stellar Mass Using Weak Lensing
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• The Effect of Adiabatic Compression on Dark Matter Halos and the Radial Acceleration Relation
• Dark acoustic oscillations: Imprints on the matter power spectrum and the halo mass function
• 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
• New Analytic Solutions for Galaxy Evolution II: Wind Recycling, Galactic Fountains and Late-Type Galaxies
• The Evolution of Sizes and Specific Angular Momenta in Hierarchical Models of Galaxy Formation and Evolution
• KiDS+GAMA: The weak lensing calibrated stellar-to-halo mass relation of central and satellite galaxies
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• Modeling globular clusters in the TNG50 simulation: predictions from dwarfs to giants
• The trajectories of galaxies in groups: mass loss and preprocessing
• Measuring Dark Matter in Galaxies: The Mass Fraction Within 5 Effective Radii
• On the environment of Low Surface Brightness galaxies at different scales
• Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z<1.3
• Relative distribution of dark matter and stellar mass in three massive galaxy clusters
• The Dearth of Difference between Central and Satellite Galaxies III. Environmental Dependence of Mass-Size and Mass-Structure Relations
• Galaxy bias from galaxy-galaxy lensing in the DES Science Verification Data
• How feedback shapes galaxies: an analytic model
• 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
• Investigating the $M_{GCS}-M_h$ Relation in the Most Massive Galaxies
• Measuring the surface mass density ellipticity of redMaPPer galaxy clusters using weak-lensing
• Impact of H${}_2$-driven star formation and stellar feedback from low-enrichment environments on the formation of spiral galaxies
• Uncovering Mass Segregation with Galaxy Analogues in Dark Matter Simulations
• How dark are filaments in the cosmic web?
• Quiescent luminous red galaxies (LRGs) as cosmic chronometers: on the significance of mass and environmental dependence
• Searching for dark matter annihilation from individual halos: uncertainties, scatter and signal-to-noise ratios
• The impact of correlated noise on galaxy shape estimation for weak lensing
• Compact Groups analysis using weak gravitational lensing II: CFHT Stripe 82 data
• A Universal Profile for Stacked Filaments from Cold Dark Matter Simulations
• Characterizing simulated galaxy stellar mass histories
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• The Next Generation Virgo Cluster Survey. XXXIII. Stellar Population Gradients in the Virgo Cluster Core Globular Cluster System
• Kinematics and dynamics of the luminous infrared galaxy pair NGC 5257/58 (Arp 240)
• Why do semi-analytic models predict higher scatter in the stellar mass-halo mass relation than cosmological hydrodynamic simulations?
• Major Mergers Mean Major Offset: Drivers of Intrinsic Scatter in The $M_{GCS}-M_h$ Scaling Relation for Massive Elliptical Galaxies
• The dark matter halo masses of elliptical galaxies as a function of observationally robust quantities
• The PAU Survey: Close galaxy pairs identification and analysis
• Weak lensing analysis of galaxy pairs using CS82 data
• Globular Cluster Systems and X-Ray Atmospheres in Galaxies
• "Observing" Unrelaxed Clusters in Dark Matter Simulations
• Galaxy-galaxy lensing in the VOICE deep survey
• Properties of Globular Clusters in Galaxy Clusters: Sensitivity from the Formation and Evolution of Globular Clusters
• The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
• Dark Energy Survey Year 3 results: Galaxy-halo connection from galaxy-galaxy lensing
• CFHTLenS: Weak lensing calibrated scaling relations for low mass clusters of galaxies
• Impact of a Rapid Diluted Energy Density on the halo mass function
• Towards model-free stellar chemical abundances. Potential applications in the search for chemically peculiar stars in large spectroscopic surveys
• Constraining cosmological parameters using density split lensing and the conditional stellar mass function
• The effect of spiral arms on the Sérsic photometry of galaxies
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations