A Weak Lensing Study of X-ray Groups in the COSMOS survey: Form and Evolution of the Mass-Luminosity Relation

Abstract

Measurements of X-ray scaling laws are critical for improving cosmological constraints derived with the halo mass function and for understanding the physical processes that govern the heating and cooling of the intracluster medium. In this paper, we use a sample of 206 X-ray selected galaxy groups to investigate the scaling relation between X-ray luminosity (Lx) and halo mass (M00) where M200 is derived via stacked weak gravitational lensing. This work draws upon a broad array of multi-wavelength COSMOS observations including 1.64 square degrees of contiguous imaging with the Advanced Camera for Surveys (ACS) and deep XMM-Newton/Chandra imaging. The combined depth of these two data-sets allows us to probe the lensing signals of X-ray detected structures at both higher redshifts and lower masses than previously explored. Weak lensing profiles and halo masses are derived for nine sub-samples, narrowly binned in luminosity and redshift. The COSMOS data alone are well fit by a power law, M200 ~ Lx^a, with a slope of a=0.66+-0.14. These results significantly extend the dynamic range for which the halo masses of X-ray selected structures have been measured with weak gravitational lensing. As a result, tight constraints are obtained for the slope of the M-Lx relation. The combination of our group data with previously published cluster data demonstrates that the M-Lx relation is well described by a single power law, a=0.64+-0.03, over two decades in mass, 10^13.5-10^15.5 h72^-1 Msun. These results are inconsistent at the 3.7 level with the self-similar prediction of a=0.75. We examine the redshift dependence of the M-Lx relation and find little evidence for evolution beyond the rate predicted by self-similarity from z ~ 0.25 to z ~ 0.8.

20 pages, 9 figures, 1 table. Accepted to ApJ. V2: Typos corrected

References in corpus (97)

• Stellar population synthesis at the resolution of 2003
• A Universal Density Profile from Hierarchical Clustering
• Profiles of dark haloes: evolution, scatter, and environment
• The Cosmic Evolution Survey (COSMOS) -- Overview
• Toward a halo mass function for precision cosmology: the limits of universality
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
• Accurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey
• COSMOS Photometric Redshifts with 30-bands for 2-deg2
• Concentrations of Dark Halos from their Assembly Histories
• The Mass Function of an X-Ray Flux-Limited Sample of Galaxy Clusters
• zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field
• Cosmology with the Sunyaev-Zel'dovich Effect
• Response of dark matter halos to condensation of baryons: cosmological simulations and improved adiabatic contraction model
• Cluster Abundance Constraints on Quintessence Models
• Tracing cosmic evolution with clusters of galaxies
• The First Release COSMOS Optical and Near-IR Data and Catalog
• The COSMOS Survey: Hubble Space Telescope / Advanced Camera for Surveys (HST/ACS) Observations and Data Processing
• Chandra Cluster Cosmology Project II: Samples and X-ray Data Reduction
• Galaxy halo masses and satellite fractions from galaxy-galaxy lensing in the SDSS: stellar mass, luminosity, morphology, and environment dependencies
• Effects of Galaxy Formation on Thermodynamics of the Intracluster Medium
• Galaxy cluster X-ray luminosity scaling relations from a representative local sample (REXCESS)
• The ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy Cluster Survey. V. The cluster catalogue
• The Mass Assembly History of Field Galaxies: Detection of an Evolving Mass Limit for Star Forming Galaxies
• A MaxBCG Catalog of 13,823 Galaxy Clusters from the Sloan Digital Sky Survey
• The Lx-T Relation and Temperature Function for Nearby Clusters Revisited
• The Northern ROSAT All-Sky (NORAS) Galaxy Cluster Survey I: X-ray Properties of Clusters Detected as Extended X-ray Sources
• Concentration, Spin and Shape of Dark Matter Haloes: Scatter and the Dependence on Mass and Environment
• The Shear TEsting Programme 1: Weak lensing analysis of simulated ground-based observations
• A New Robust Low-Scatter X-ray Mass Indicator for Clusters of Galaxies
• Accurate universal models for the mass accretion histories and concentrations of dark matter halos
• Constraints on Cosmological Parameters from Future Galaxy Cluster Surveys
• The Chandra COSMOS Survey, I: Overview and Point Source Catalog
• Weak Gravitational Lensing with COSMOS: Galaxy Selection and Shape Measurements
• The structural and scaling properties of nearby galaxy clusters - II. The M-T relation
• The Shear TEsting Programme 2: Factors affecting high precision weak lensing analyses
• A Catalog of 200 Galaxy Clusters Serendipitously Detected in the ROSAT PSPC Pointed Observations
• The Red-Sequence Cluster Survey I: The Survey and Cluster Catalogs for Patches RCS0926+37 and RCS1327+29
• Dark matter maps reveal cosmic scaffolding
• XMM-Newton observation of the Lockman Hole; I. The X-ray Data
• The XMM-Newton wide-field survey in the COSMOS field: I. Survey description
• The XMM-Newton wide-field survey in the COSMOS field: VI. Statistical properties of clusters of galaxies
• The C4 Clustering Algorithm: Clusters of Galaxies in the Sloan Digital Sky Survey
• Galaxy clusters discovered with a Sunyaev-Zel'dovich effect survey
• The XMM-Newton wide-field survey in the COSMOS field. The point-like X-ray source catalogue
• Statistics of X-ray observables for the cooling-core and non-cooling core galaxy clusters
• Clusters of Galaxies in the First Half of the Universe from the IRAC Shallow Survey
• Non-linear Evolution of f(R) Cosmologies III: Halo Statistics
• Density profiles of galaxy groups and clusters from SDSS galaxy-galaxy weak lensing
• Self Calibration in Cluster Studies of Dark Energy: Combining the Cluster Redshift Distribution, the Power Spectrum and Mass Measurements
• How well can we determine cluster mass profiles from weak lensing?
• Self-Calibration of Cluster Dark Energy Studies: Observable-Mass Distribution
• The Integrated Sunyaev-Zeldovich Effect as the Superior Method for Measuring the Mass of Clusters of Galaxies
• Comparison of weak lensing masses and X-ray properties of galaxy clusters
• LoCuSS: Comparison of Observed X-ray and Lensing Galaxy Cluster Scaling Relations with Simulations
• The Impact of Galaxy Formation on the Sunyaev-Zeldovich Effect of Galaxy Clusters
• The XMM Cluster Survey: A Massive Galaxy Cluster at z=1.45
• Simulating the Sunyaev-Zel'dovich effect(s): including radiative cooling and energy injection by galactic winds
• Cosmological constraints from the local X-ray luminosity function of the most X-ray luminous galaxy clusters
• Evidence for Non-Hydrostatic Gas from the Cluster X-ray to Lensing Mass Ratio
• Weak Lensing Measurements: A Revisited Method and Application to HST Images
• Searching for massive clusters in weak lensing surveys
• The Compression of Dark Matter Halos by Baryonic Infall
• The Lx-Yx Relation: Using Galaxy Cluster X-Ray Luminosity as a Robust, Low Scatter Mass Proxy
• Constraining the Scatter in the Mass-Richness Relation of maxBCG Clusters With Weak Lensing and X-ray Data
• The X-Ray Luminosity--Mass Relation for Local Clusters of Galaxies
• Resurrecting the Red from the Dead: Optical Properties of BCGs in X-ray Luminous Clusters
• Precision photometric redshift calibration for galaxy-galaxy weak lensing
• The DEEP2 Galaxy Redshift Survey: First results on galaxy groups
• The Stability of the Point Spread Function of the Advanced Camera for Surveys on the Hubble Space Telescope and Implications for Weak Gravitational Lensing
• Galaxy-galaxy Lensing: Dissipationless Simulations Versus the Halo Model
• The RASS-SDSS Galaxy Cluster Survey. III. Scaling relations of galaxy clusters
• An optical group catalogue to z = 1 from the zCOSMOS 10k sample
• The Evolution of Structure in X-ray Clusters of Galaxies
• Cross-correlation Weak Lensing of SDSS Galaxy Clusters I: Measurements
• Measurements of Sunyaev-Zel'dovich Effect Scaling Relations for Clusters of Galaxies
• The L_X--M relation of Clusters of Galaxies
• Future Galaxy Cluster Surveys: The Effect of Theory Uncertainty on Constraining Cosmological Parameters
• Constraining the Evolution of Dark Energy with a Combination of Galaxy Cluster Observables
• Galaxy Halo Masses from Galaxy-Galaxy Lensing
• The Effect of the Cosmic Web on Cluster Weak Lensing Mass Estimates
• Self-Consistency and Calibration of Cluster Number Count Surveys for Dark Energy
• A Subaru Weak Lensing Survey I: Cluster Candidates and Spectroscopic Verification
• Lack of cooling flow clusters at z>0.5
• A Lensing Survey of X-ray Luminous Galaxy Clusters at Redshift z ~ 0.2: II: CFH12k Weak Lensing Analysis and Global Correlations
• From Galaxy-Galaxy Lensing to Cosmological Parameters
• XMM-Newton Observations of Evolution of Cluster X-Ray Scaling Relations at z=0.4-0.7
• Evolution at z>0.5 of the X-ray properties of simulated galaxy clusters: comparison with the observational constraints
• The XMM--NEWTON Omega Project: I. The X-ray Luminosity - Temperature Relation at z>0.4
• Combined analysis of weak lensing and X-ray blind surveys
• The Impact of Halo Properties, Energy Feedback and Projection Effects on the Mass-SZ Flux Relation
• Dark energy constraints from lensing-detected galaxy clusters
• Using Weak Lensing to find Halo Masses
• A robust lower limit on the amplitude of matter fluctuations in the universe from cluster abundance and weak lensing
• Finding Clusters in SZ Surveys
• Issues in joint SZ and optical cluster finding
• Evolution of the Cluster Correlation Function
• Halo Model Analysis of Cluster Statistics

Cited by in corpus (226)

• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• Cosmological Parameters from Observations of Galaxy Clusters
• 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
• Towards a realistic population of simulated galaxy groups and clusters
• Quantifying the effect of baryon physics on weak lensing tomography
• Dark energy two decades after: Observables, probes, consistency tests
• The dark matter of gravitational lensing
• CFHTLenS: Improving the quality of photometric redshifts with precision photometry
• Cluster Lenses
• Weighing the Giants - I. Weak-lensing masses for 51 massive galaxy clusters: project overview, data analysis methods and cluster images
• The first-year shear catalog of the Subaru Hyper Suprime-Cam SSP Survey
• Combined strong and weak lensing analysis of 28 clusters from the Sloan Giant Arcs Survey
• Discovery of a galaxy cluster with a violently starbursting core at z=2.506
• Origins of weak lensing systematics, and requirements on future instrumentation (or knowledge of instrumentation)
• A mature cluster with X-ray emission at z=2.07
• The Rise and Fall of Passive Disk Galaxies: Morphological Evolution Along the Red Sequence Revealed by COSMOS
• CFHTLenS: The relation between galaxy dark matter haloes and baryons from weak gravitational lensing
• Weak Lensing Measurement of the Mass--Richness Relation of SDSS redMaPPer Clusters
• Masses of galaxy clusters from gravitational lensing
• A cluster finding algorithm based on the multiband identification of red sequence galaxies
• The dependence of star formation activity on environment and stellar mass at z~1 from the HiZELS H-alpha survey
• A direct measurement of the baryonic mass function of galaxies & implications for the galactic baryon fraction
• Dark matter halo properties of GAMA galaxy groups from 100 square degrees of KiDS weak lensing data
• LoCuSS: A Comparison of Cluster Mass Measurements from XMM-Newton and Subaru - Testing Deviation from Hydrostatic Equilibrium and Non-Thermal Pressure Support
• The galaxy-halo connection from a joint lensing, clustering and abundance analysis in the CFHTLenS/VIPERS field
• Galaxies in X-ray Groups I: Robust Membership Assignment and the Impact of Group Environments on Quenching
• Weighing the Giants V: Galaxy Cluster Scaling Relations
• The Extended Chandra Deep Field-South Survey: Optical spectroscopy of faint X-ray sources with the VLT and Keck
• The FABLE simulations: A feedback model for galaxies, groups and clusters
• The evolution of the mass-size relation for early type galaxies from z~1 to the present: dependence on environment, mass-range and detailed morphology
• The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to $z\sim 5$
• Cluster-galaxy weak lensing
• Galaxies in X-ray Groups. II. A Weak Lensing Study of Halo Centering
• HIFLUGCS: Galaxy cluster scaling relations between X-ray luminosity, gas mass, cluster radius, and velocity dispersion
• Testing the Low-Mass End of X-Ray Scaling Relations with a Sample of Chandra Galaxy Groups
• A Weak-Lensing Mass Reconstruction of the Large-Scale Filament Feeding the Massive Galaxy Cluster MACSJ0717.5+3745
• A theoretical framework for combining techniques that probe the link between galaxies and dark matter
• Cluster Mass Calibration at High Redshift: HST Weak Lensing Analysis of 13 Distant Galaxy Clusters from the South Pole Telescope Sunyaev-Zel'dovich Survey
• The integrated stellar content of dark matter halos
• Observational constraints on the redshift evolution of X-ray scaling relations of galaxy clusters out to z ~ 1.5
• Galaxy Pairs in COSMOS -- Merger Rate Evolution Since z=1
• The spectroscopically confirmed X-ray cluster at z=1.62 with a possible companion in the Subaru/XMM-Newton deep field
• A Runaway Black Hole in COSMOS: Gravitational Wave or Slingshot Recoil?
• Size and velocity-dispersion evolution of early-type galaxies in a Lambda cold dark matter universe
• Hot Gas in Galaxy Groups: Recent Observations
• BUDHIES III: The fate of HI and the quenching of galaxies in evolving environments
• Direct observational evidence for a large transient galaxy population in groups at 0.85<z<1
• Physical properties underlying observed kinematics of satellite galaxies
• Cosmology and Astrophysics from Relaxed Galaxy Clusters III: Thermodynamic Profiles and Scaling Relations
• Scaling Properties of Galaxy Groups
• Galaxy-galaxy lensing constraints on the relation between baryons and dark matter in galaxies in the Red Sequence Cluster Survey 2
• The Complete Local Volume Groups Sample - I. Sample Selection and X-ray Properties of the High-Richness Subsample
• The XXL Survey IV. Mass-temperature relation of the bright cluster sample
• Chandra centres for COSMOS X-ray galaxy groups: Differences in stellar properties between central dominant and offset brightest group galaxies
• Three Lyman-alpha emitting filaments converging to a massive galaxy group at z=2.91: discussing the case for cold gas infall
• Environmental dependence of bulge-dominated galaxy sizes in hierarchical models of galaxy formation. Comparison with the local Universe
• The mass-richness relation of optically-selected clusters from weak gravitational lensing and abundance with Subaru HSC first-year data
• Weak lensing Analysis of X-Ray-selected XXL Galaxy Groups and Clusters with Subaru HSC Data
• Weak lensing, dark matter and dark energy
• Occupation of X-ray selected galaxy groups by X-ray AGN
• Probing the galaxy-halo connection in UltraVISTA to $z\sim 2$
• A Detection of Weak Lensing Magnification using Galaxy Sizes and Magnitudes
• Luminous Red Galaxies in Clusters: Central Occupation, Spatial Distributions, and Mis-centering
• LoCuSS: Pre-processing in galaxy groups falling into massive galaxy clusters at z=0.2
• GASP XXI. Star formation rates in the tails of galaxies undergoing ram-pressure stripping
• Where are the Luminous Red Galaxies (LRGs)? Using correlation measurements and lensing to relate LRGs to dark matter halos
• The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel
• Weak lensing measurement of galaxy clusters in the CFHTLS-Wide survey
• Weak lensing mass map and peak statistics in Canada-France-Hawaii Telescope Stripe 82 survey
• The Lx-Tvir relation in galaxy clusters: Effects of radiative cooling and AGN heating
• Measurement of the halo bias from stacked shear profiles of galaxy clusters
• Cluster abundance in chameleon $f(R)$ gravity I: toward an accurate halo mass function prediction
• Mock catalogs for the extragalactic X-ray sky: simulating AGN surveys with Athena and with the AXIS probe
• The pressure profiles of hot gas in local galaxy groups
• Weak-Lensing Mass Calibration of the Atacama Cosmology Telescope Equatorial Sunyaev-Zeldovich Cluster Sample with the Canada-France-Hawaii Telescope Stripe 82 Survey
• LoCuSS: The infall of X-ray groups onto massive clusters
• The GEEC2 spectroscopic survey of Galaxy Groups at $0.8<z<1$
• Line-of-sight effects in strong lensing: Putting theory into practice
• Measuring the X-ray luminosities of SDSS DR7 clusters from RASS
• Mining the gap: evolution of the magnitude gap in X-ray galaxy groups from the 3 square degree XMM coverage of CFHTLS
• The WIRCAM Deep Infrared Cluster Survey I: Groups and Clusters at z > 1.1
• Radio galaxy feedback in X-ray selected groups from COSMOS: the effect on the ICM
• Growing a `Cosmic Beast': Observations and Simulations of MACS J0717.5+3745
• Group connectivity in COSMOS: a tracer of mass assembly history
• Ultra-deep catalog of X-ray groups in the Extended Chandra Deep Field South
• Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties
• Measuring the Dark Matter Halo Mass of X-ray AGN at z~1 using photometric redshifts
• A simple model linking galaxy and dark matter evolution
• Exploring the Diversity of Groups at 0.1<z<0.8 with X-ray and Optically Selected Samples
• Comprehensive Gas Characterization of a $z=2.5$ Protocluster: A Cluster Core Caught in the Beginning of Virialization?
• Ultimate age-dating method for galaxy groups; clues from the Millennium Simulations
• The Growth and Enrichment of the Intragroup Gas
• The Galaxy Stellar Mass Function of X-ray detected groups: environmental dependence of galaxy evolution in the COSMOS survey
• CFHTLenS: The Environmental Dependence of Galaxy Halo Masses from Weak Lensing
• An X-ray Detected Group of Quiescent Early-type Galaxies at z=1.6 in the Chandra Deep Field South
• X-Ray Groups of Galaxies in the Aegis Deep and Wide Fields
• XMM-Newton (X-Ray Mulit-Mirror Mission) Observatory
• On stellar mass loss from galaxies in groups and clusters
• The eROSITA Final Equatorial-Depth Survey (eFEDS): Optical confirmation, redshifts, and properties of the cluster and group catalog
• Weak Lensing Calibrated M-T Scaling Relation of Galaxy Groups in the COSMOS Field
• The Halo Occupation Distribution of X-ray-Bright Active Galactic Nuclei: A Comparison with Luminous Quasars
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• An X-ray Selected Galaxy Cluster in the Lockman Hole at Redshift 1.753
• Magnification by Galaxy Group Dark Matter Halos
• The Mass-Concentration Relation and the Stellar-to-Halo Mass Ratio in the CFHT Stripe 82 Survey
• On the evolution of environmental and mass properties of strong lens galaxies in COSMOS
• The role of gas infall in the evolution of disc galaxies
• Stellar mass -- halo mass relation for the brightest central galaxies of X-ray clusters since z~0.65
• Cluster candidates around low power radio-galaxies at z~1-2 in COSMOS
• Stochastic bias of colour-selected BAO tracers by joint clustering-weak lensing analysis
• Velocity Dispersions of Brightest Cluster Galaxies and Their Host Clusters
• Massive Star-Forming Galaxies Have Converted Most of Their Halo Gas into Stars
• Statistics and implications of substructure detected in a representative sample of X-ray clusters
• Comparing Dense Galaxy Cluster Redshift Surveys with Weak Lensing Maps
• CFHTLenS: A Weak Lensing Shear Analysis of the 3D-Matched-Filter Galaxy Clusters
• MACSJ1423.8+2404: Gravitational Lensing by a Massive, Relaxed Cluster of Galaxies at z=0.54
• The Correlated Formation Histories of Massive Galaxies and Their Dark Matter Halos
• The lack of star formation gradients in galaxy groups up to z~1.6
• Cosmic Evolution of Star-Formation Enhancement in Close Major-Merger Galaxy Pairs Since z = 1
• A pan-chromatic view of the galaxy cluster XMMU J1230.3+1339 at z=0.975 - Observing the assembly of a massive system
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Chameleonic Generalized Brans--Dicke model and late-time acceleration
• Evolution of the cluster optical galaxy luminosity function in the CFHTLS : breaking the degeneracy between mass and redshift
• The dark matter distribution in z~0.5 clusters of galaxies. I : Determining scaling relations with weak lensing masses
• LoCuSS: A Herschel view of obscured star formation in Abell 1835
• The role of massive halos in the Star Formation History of the Universe
• A giant Ly$\alpha$ nebula in the core of an X-ray cluster at $z=1.99$: implications for early energy injection
• SPIDERS: An Overview of The Largest Catalogue of Spectroscopically Confirmed X-ray Galaxy Clusters
• The Megaparsec-scale Gas-sloshing Spiral in the Remnant Cool Core Cluster Abell 1763
• SARCS strong-lensing galaxy groups: II - mass-concentration relation and strong-lensing bias
• Stacked Weak Lensing Mass Calibration: Estimators, Systematics, and Impact on Cosmological Parameter Constraints
• The GOGREEN survey: Dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching
• 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
• Passive galaxies as tracers of cluster environments at z~2
• Radio galaxies in galaxy groups: kinematics, scaling relations and AGN feedback
• Detection of universality of dark matter profile from Subaru weak lensing measurements of 50 massive clusters
• The evolution of galaxy star formation activity in massive halos
• The Cosmic Web and galaxy evolution around the most luminous X-ray cluster: RXJ1347.5-1145
• Constraining AGN triggering mechanisms through the clustering analysis of active black holes
• Chandra Follow-Up of the SDSS DR8 redMaPPer Catalog Using the MATCha Pipeline
• A Gibbs Sampler for Multivariate Linear Regression
• Understanding the Unique Assembly History of Central Group Galaxies
• Galaxy clusters and groups in the ALHAMBRA Survey
• Galaxy-Mass Correlations on 10 Mpc Scales in the Deep Lens Survey
• Describing galaxy weak lensing measurements from tenths to tens of Mpc and up to z~0.6 with a single model
• The Cosmic Microwave Background and the Stellar Initial Mass Function
• Brightest X-ray clusters of galaxies in the CFHTLS wide fields: Catalog and optical mass estimator
• On the occupation of X-ray selected galaxy groups by radio AGN since z=1.3
• The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects
• Testing redMaPPer centring probabilities using galaxy clustering and galaxy-galaxy lensing
• The Massively Accreting Cluster A2029
• Sunyaev-Zel'dovich detection of the galaxy cluster Cl J1449+0856 at z = 1.99: the pressure profile in uv space
• A Direct Measurement of the Mean Occupation Function of Quasars: Breaking Degeneracies between Halo Occupation Distribution Models
• Cluster Lensing Profiles Derived from a Redshift Enhancement of Magnified BOSS-Survey Galaxies
• The relation between the diffuse X-ray luminosity and the radio power of the central AGN in galaxy groups
• HIFLUGCS: X-ray luminosity -- dynamical mass relation and its implications for mass calibrations with the SPIDERS and 4MOST surveys
• Galaxy stellar mass assembly: the difficulty matching observations and semi-analytical predictions
• X-ray Groups of Galaxies at 0.5<z<1 in zCOSMOS: Increased AGN Activities in High Redshift Groups
• Dark Matter Astrometry: Accuracy of sub-halo positions for the measurement of self-interaction cross sections
• Galaxies in X-ray Groups. III. Satellite Color and Morphology Transformations
• Exploring Relations Between BCG \& Cluster Properties in the SPectroscopic IDentification of eROSITA Sources Survey from $0.05<z<0.3$
• Measuring the Geometry of the Universe from Weak Gravitational Lensing behind Galaxy Groups in the HST COSMOS survey
• An empirical measurement of the Halo Mass Function from the combination of GAMA DR4, SDSS DR12, and REFLEX II data
• In the whirlpool's coils: tracing substructure from combined optical/X-ray data in the galaxy cluster A1300
• Probing cosmology and gastrophysics with fast radio bursts: Cross-correlations of dark matter haloes and cosmic dispersion measures
• The COSMOS Density Field: A Reconstruction Using Both Weak Lensing and Galaxy Distributions
• SARCS strong lensing galaxy groups: I - optical, weak lensing, and scaling laws
• The evolution of star formation activity in galaxy groups
• Low X-ray Luminosity Galaxy Clusters. III: Weak Lensing Mass Determination at 0.18 $<$ z $<$ 0.70
• The XXL Survey X: K-band luminosity - weak-lensing mass relation for groups and clusters of galaxies
• Kinematic unrest of low mass galaxy groups
• Brightest group galaxies-II: the relative contribution of BGGs to the total baryon content of groups at z<1.3
• Effect of richness on AGN and star formation activities in SDSS galaxy groups
• CODEX Weak Lensing Mass Catalogue and implications on the mass-richness relation
• Two fossil groups of galaxies at z~0.4 in the COSMOS: accelerated stellar-mass build-up, different progenitors
• The miniJPAS survey: clusters and galaxy groups detection with AMICO
• The Chandra COSMOS Legacy Survey: clustering dependence of Type 2 AGN on host galaxy properties
• An X-ray underluminous cluster of galaxies in the 4Ms CDFS observations
• The XXL Survey: XXII. The XXL-North spectrophotometric sample and galaxy stellar mass function in X-ray detected groups and clusters
• Next Generation Virgo Cluster Survey. XXI. The weak lensing masses of the CFHTLS and NGVS RedGOLD galaxy clusters and calibration of the optical richness
• Testing the accuracy of 3D-HST photometric redshift estimates as reference samples for deep weak lensing studies
• Galaxy luminosity function and Tully-Fisher relation: reconciled through rotation-curve studies
• The impact of cosmic variance on simulating weak lensing surveys
• Satellite content and quenching of star formation in galaxy groups at z~1.8
• A z=1.85 galaxy group in CEERS: evolved, dustless, massive intra-halo light and a brightest group galaxy in the making
• Close galaxy pairs with accurate photometric redshifts
• Weak lensing mass estimates of galaxy groups and the line-of-sight contamination
• AMICO-COSMOS galaxy cluster and group catalogue up to $z=2$: Sample properties and X-ray counterparts
• LoCuSS: exploring the connection between local environment, star formation and dust mass in Abell 1758
• A Spectroscopic Census of X-ray Systems in the COSMOS Field
• A new method to search for high redshift clusters using photometric redshifts
• A close-pair analysis of damp mergers at intermediate redshifts
• Can we use Weak Lensing to Measure Total Mass Profiles of Galaxies on 20 kiloparsec Scales?
• MaNGA DynPop -- IV. Stacked total density profile of galaxy groups and clusters from combining dynamical models of integral-field stellar kinematics and galaxy-galaxy lensing
• On the weak lensing masses of a new sample of galaxy groups
• Chemical and photometric evolution models for disk, irregular and low mass galaxies
• Weak lensing measurement of the mass-richness relation using the SDSS database
• Cluster-lensing: A Python Package for Galaxy Clusters & Miscentering
• The Stellar Mass - Halo Mass Relation for Low Mass X-ray Groups at 0.5<z<1 in the CDFS with CSI
• COSMOS Brightest Group Galaxies -- III: Evolution of stellar ages
• Assessing Mass Loss and Stellar-to-Halo Mass Ratio of Satellite Galaxies: A Galaxy-Galaxy Lensing Approach Utilizing DECaLS DR8 Data
• Stability analysis of agegraphic dark energy in Brans-Dicke cosmology
• The SDSS Coadd: Cross-Correlation Weak Lensing and Tomography of Galaxy Clusters
• Cluster candidates with massive quiescent galaxies at $z\sim 2$
• The BIG X-ray tail
• Extended X-ray emission from non-thermal sources in the COSMOS field: A detailed study of a large radio galaxy at z=1.168
• The PAU Survey: Close galaxy pairs identification and analysis
• Strong Lensing In The Inner Halo Of Galaxy Clusters
• The X-Ray Zurich Environmental Study (X-ZENS). II. X-ray Observations of the Diffuse Intragroup Medium in Galaxy Groups
• Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
• Stellar Mass and 3.4 $\mu$m M/L Ratio Evolution of Brightest Cluster Galaxies in COSMOS since z ~ 1.0
• Weak lensing analysis of galaxy pairs using CS82 data
• Compact Groups analysis using weak gravitational lensing
• Probing Satellite Halos with Weak Gravitational Lensing
• The mass distribution in an assembling super galaxy group at $z=0.37$
• Weak lensing constraints on the stellar-to-halo mass relation of galaxy groups with simulation-informed scatter
• The Jet Paths of Radio AGN and their Cluster Weather
• The evolution of the radio luminosity function of group galaxies in COSMOS
• Fraction of the X-ray selected AGNs with optical emission lines in galaxy groups
• Cosmic Dragons: A Two-Component Mixture Model of COSMOS Galaxies
• Dark matter halos of luminous AGNs from galaxy-galaxy lensing with the HSC Subaru Strategic Program
• Revisiting Agegraphic Dark Energy in Brans-Dicke Cosmology
• ALMA measures molecular gas reservoirs comparable to field galaxies in a low-mass galaxy cluster at z=1.3
• The XMM-BCS galaxy cluster survey: I. The X-ray selected cluster catalog from the initial 6 deg${}^2$
• Distinct radial acceleration relations of galaxies and galaxy clusters supports hyperconical modified gravity
• AMICO galaxy clusters in KiDS-DR3: the impact of estimator statistics on the luminosity-mass scaling relation