Constraints on Cosmological Parameters from Future Galaxy Cluster Surveys
arXiv:astro-ph/0002336 · doi:10.1086/320939
Abstract
We study the expected redshift evolution of galaxy cluster abundance between 0 < z < 3 in different cosmologies, including the effects of the cosmic equation of state parameter w=p/rho. Using the halo mass function obtained in recent large scale numerical simulations, we model the expected cluster yields in a 12 deg^2 Sunyaev-Zeldovich Effect (SZE) survey and a deep 10^4 deg^2 X-ray survey over a wide range of cosmological parameters. We quantify the statistical differences among cosmologies using both the total number and redshift distribution of clusters. Provided that the local cluster abundance is known to a few percent accuracy, we find only mild degeneracies between w and either Omega_m or h. As a result, both surveys will provide improved constraints on Omega_m and w. The Omega_m-w degeneracy from both surveys is complementary to those found either in studies of CMB anisotropies or of high-redshift Supernovae (SNe). As a result, combining these surveys together with either CMB or SNe studies can reduce the statistical uncertainty on both w and Omega_m to levels below what could be obtained by combining only the latter two data sets. Our results indicate a formal statistical uncertainty of about 3% (68% confidence) on both Omega_m and w when the SZE survey is combined with either the CMB or SN data; the large number of clusters in the X-ray survey further suppresses the degeneracy between w and both Omega_m and h. Systematics and internal evolution of cluster structure at the present pose uncertainties above these levels. We briefly discuss and quantify the relevant systematic errors. By focusing on clusters with measured temperatures in the X-ray survey, we reduce our sensitivity to systematics such as non-standard evolution of internal cluster structure.
ApJ, revised version. Expanded discussion of systematics; Press-Schechter mass function replaced by fit from simulations
References in corpus (4)
Cited by in corpus (367)
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
- Dark Energy and the Accelerating Universe
- Toward a halo mass function for precision cosmology: the limits of universality
- Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements
- Cosmology with the Sunyaev-Zel'dovich Effect
- Tracing cosmic evolution with clusters of galaxies
- The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
- Dark Energy
- Probing Dark Energy with Baryonic Acoustic Oscillations from Future Large Galaxy Redshift Surveys
- The large-scale structure of the Universe
- The DEEP2 Galaxy Redshift Survey: Design, Observations, Data Reduction, and Redshifts
- Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
- Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts
- Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope
- Precision Determination of the Mass Function of Dark Matter Halos
- Euclid. I. Overview of the Euclid mission
- Probing dark energy using baryonic oscillations in the galaxy power spectrum as a cosmological ruler
- Probing the dark energy: methods and strategies
- The Physics of Cosmic Acceleration
- Sample Variance Considerations for Cluster Surveys
- The Sunyaev-Zel'dovich angular power spectrum as a probe of cosmological parameters
- Planck Early Results VIII: The all-sky Early Sunyaev-Zeldovich cluster sample
- Cluster Cosmology Constraints from the 2500 deg SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
- Future Supernovae observations as a probe of dark energy
- Galaxy Clusters Selected with the Sunyaev-Zel'dovich Effect from 2008 South Pole Telescope Observations
- On the Accuracy of Weak Lensing Cluster Mass Reconstructions
- Near-IR Properties of Galaxy Clusters: Luminosity as a Binding Mass Predictor and the State of Cluster Baryons
- Galaxy clusters discovered with a Sunyaev-Zel'dovich effect survey
- The Atacama Cosmology Telescope: Sunyaev Zel'dovich Selected Galaxy Clusters at 148 GHz in the 2008 Survey
- A Weak Lensing Study of X-ray Groups in the COSMOS survey: Form and Evolution of the Mass-Luminosity Relation
- CLASH: Weak-Lensing Shear-and-Magnification Analysis of 20 Galaxy Clusters
- Galaxy clusters discovered via the Sunyaev-Zel'dovich effect in the first 720 square degrees of the South Pole Telescope survey
- A Spitzer-Selected Galaxy Cluster at z=1.62
- The South Pole Telescope
- LoCuSS: Subaru Weak Lensing Study of 30 Galaxy Clusters
- An SZ-selected sample of the most massive galaxy clusters in the 2500-square-degree South Pole Telescope survey
- Cosmological Constraints from Galaxy Clusters in the 2500 square-degree SPT-SZ Survey
- Cosmological Constraints from Sunyaev-Zel'dovich-Selected Clusters with X-ray Observations in the First 178 Square Degrees of the South Pole Telescope Survey
- Halo mass function: Baryon impact, fitting formulae and implications for cluster cosmology
- MaxBCG: A Red Sequence Galaxy Cluster Finder
- The Blanco Cosmology Survey: Data Acquisition, Processing, Calibration, Quality Diagnostics and Data Release
- Weak Lensing and Dark Energy
- Catalog Extraction in SZ Cluster Surveys: a matched filter approach
- The 400 square degrees ROSAT PSPC galaxy cluster survey: Catalog and statistical calibration
- Theoretical Models of Dark Energy
- Dark Synergy: Gravitational Lensing and the CMB
- Constraints on Omega_m, Omega_L, and Sigma_8, from Galaxy Cluster Redshift Distributions
- Self Calibration in Cluster Studies of Dark Energy: Combining the Cluster Redshift Distribution, the Power Spectrum and Mass Measurements
- CLASH: Joint Analysis of Strong-Lensing, Weak-Lensing Shear and Magnification Data for 20 Galaxy Clusters
- 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
- Total mass biases in X-ray galaxy clusters
- A mature cluster with X-ray emission at z=2.07
- Comparison of weak lensing masses and X-ray properties of galaxy clusters
- The Impact of Galaxy Formation on the Sunyaev-Zeldovich Effect of Galaxy Clusters
- Cosmology with the shear-peak statistics
- Mass Function Predictions Beyond LCDM
- The XMM-LSS survey. Survey design and first results
- X-ray Properties of the First SZE-selected Galaxy Cluster Sample from the South Pole Telescope
- New constraints on dark energy from the observed growth of the most X-ray luminous galaxy clusters
- Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion and X-ray Measurements
- Can the Steep Mass Profile of A1689 Be Explained by a Triaxial Dark Halo?
- IDCS J1426+3508: Discovery of a Massive, IR-Selected Galaxy Cluster at z = 1.75
- First Results On Shear-Selected Clusters From the Deep Lens Survey: Optical Imaging, Spectroscopy, and X-ray Followup
- 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
- Effects of Mergers and Core Structure on the Bulk Properties of Nearby Galaxy Clusters
- Importance of Cluster Structural Evolution in Using X-ray and SZE Galaxy Cluster Surveys to Study Dark Energy
- Predicting Single-Temperature Fit to Multi-Component Thermal Plasma Spectra
- The DEEP2 Galaxy Redshift Survey: First results on galaxy groups
- Constraining cosmological parameters using Sunyaev-Zel'dovich cluster surveys
- Cluster-galaxy weak lensing
- Why Do Only Some Galaxy Clusters Have Cool Cores?
- Probing Cosmology with Weak Lensing Peak Counts
- Self-Calibration of Cluster Dark Energy Studies: Counts in Cells
- Cosmological Constraints from the Red-Sequence Cluster Survey
- X-ray Properties of SPT Selected Galaxy Clusters at 0.2<z<1.5 Observed with XMM-Newton
- The Incidence of Strong-Lensing Clusters in the Red-Sequence Cluster Survey
- Cluster Mass Calibration at High Redshift: HST Weak Lensing Analysis of 13 Distant Galaxy Clusters from the South Pole Telescope Sunyaev-Zel'dovich Survey
- Cluster number counts dependence on dark energy inhomogeneities and coupling to dark matter
- Simultaneous Falsification of LCDM and Quintessence with Massive, Distant Clusters
- Discovery of a Rich Cluster at z = 1.63 using the Rest-Frame 1.6um "Stellar Bump Sequence" Method
- Observational Constraints on Quintessence: Thawing, Tracker, and Scaling models
- The FLAMINGOS Extragalactic Survey
- Quantifying properties of ICM inhomogeneities
- Redshifts, Sample Purity, and BCG Positions for the Galaxy Cluster Catalog from the first 720 Square Degrees of the South Pole Telescope Survey
- Probing dark energy with cluster counts and cosmic shear power spectra: including the full covariance
- The Cluster Mass Function from Weak Gravitational Lensing
- Observational Constraints on General Relativistic Energy Conditions, Cosmic Matter Density and Dark Energy from X-Ray Clusters of Galaxies and Type-Ia Supernovae
- Baryon Content in a Sample of 91 Galaxy Clusters Selected by the South Pole Telescope at 0.2 < z < 1.25
- Prospects for Determining the Equation of State of the Dark Energy: What can be Learned from Multiple Observables?
- Constraining dark energy with Sunyaev-Zel'dovich cluster surveys
- WMAPing the Universe: Supersymmetry, Dark Matter, Dark Energy, Proton Decay and Collider Physics
- Scaling Relations from Sunyaev-Zel'dovich Effect and Chandra X-ray measurements of high-redshift galaxy clusters
- The Angular Clustering of Distant Galaxy Clusters
- Measurements of Sunyaev-Zel'dovich Effect Scaling Relations for Clusters of Galaxies
- Completeness in Weak Lensing Searches for Clusters
- Future Galaxy Cluster Surveys: The Effect of Theory Uncertainty on Constraining Cosmological Parameters
- Cosmic Chronometers in the R_h=ct Universe
- Shear Selected Cluster Cosmology I: Tomography and Optimal Filtering
- Cosmological Information in Weak Lensing Peaks
- Constraining the Evolution of Dark Energy with a Combination of Galaxy Cluster Observables
- Statistics of Giant Arcs in Galaxy Clusters
- Self-Consistency and Calibration of Cluster Number Count Surveys for Dark Energy
- Dark Energy Survey Year 1 Results: Curved-Sky Weak Lensing Mass Map
- Constraints on the mass-richness relation from the abundance and weak lensing of SDSS clusters
- Using Galaxy Two-point Correlation Functions to Determine the Redshift Distributions of Galaxies Binned by Photometric Redshift
- The Correlation Function of Optically Selected Galaxy Clusters in the Sloan Digital Sky Survey
- Secondary anisotropies of the CMB
- Weak lensing survey of galaxy clusters in the CFHTLS Deep
- Application of a Self-Similar Pressure Profile to Sunyaev-Zel'dovich Effect Data from Galaxy Clusters
- The NGC 5846 Group: Dynamics and the Luminosity Function to M_R=-12
- Constraining the Dark Energy Equation of State with Cosmic Voids
- Evidence for Cold Accretion onto a Massive Galaxy at High Redshift?
- Detecting Neutrino Mass by Combining Matter Clustering, Halos, and Voids
- Cross-Correlation Lensing: Determining Galaxy and Cluster Mass Profiles from Statistical Weak Lensing Measurements
- Binned Cosmic Microwave Background Anisotropy Power Spectra: Peak Location
- 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
- The integrated Sachs-Wolfe Effect -- Large Scale Structure Correlation
- Probing dark energy with baryonic oscillations and future radio surveys of neutral Hydrogen
- Surveying the Sky with the Arcminute MicroKelvin Imager: Expected Constraints on Galaxy Cluster Evolution and Cosmology
- A New RASS Galaxy Cluster Catalog with Low Contamination Extending to in the DES Overlap Region
- The impact of Early Dark Energy on non-linear structure formation
- Gamma Rays from Clusters and Groups of Galaxies: Cosmic Rays versus Dark Matter
- SZE Observables, Pressure Profiles and Center Offsets in Magneticum Simulation Galaxy Clusters
- Spherical collapse model with shear and angular momentum in dark energy cosmologies
- The Santa Fe Light Cone Simulation Project: I. Confusion and the WHIM in Upcoming Sunyaev-Zel'dovich Effect Surveys
- The Evolution of Dusty Star Formation and Stellar Mass Assembly in Clusters: Results from the IRAC 3.6um, 4.5um, 5.8um and 8.0um Cluster Luminosity Functions
- Optical Redshift and Richness Estimates for Galaxy Clusters Selected with the Sunyaev-Zel'dovich Effect from 2008 South Pole Telescope Observations
- Cosmology with the Large Synoptic Survey Telescope: an Overview
- Three-dimensional Multi-probe Analysis of the Galaxy Cluster A1689
- Baryon Content of Massive Galaxy Clusters (0.57 < z < 1.33)
- High redshift X-ray cooling-core cluster associated with the luminous radio loud quasar 3C186
- A Multi-component Matched Filter Cluster Confirmation Tool for eROSITA: Initial Application to the RASS and DES-SV Datasets
- Combining clustering and abundances of galaxy clusters to test cosmology and primordial non-Gaussianity
- A measurement of the secondary-CMB and millimeter-wave-foreground bispectrum using 800 square degrees of South Pole Telescope data
- Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description
- A comparison of structure formation in minimally and non-minimally coupled quintessence models
- Effects of shear and rotation on the spherical collapse model for clustering dark energy
- Cosmological Constraints from Galaxy Clusters and Groups in the eROSITA Final Equatorial Depth Survey
- The Virial Mass Function of Nearby SDSS Galaxy Clusters
- The Voronoi Tessellation cluster finder in 2+1 dimensions
- Precision cosmology with a wide area XMM cluster survey
- Cluster morphologies and model-independent Y_SZ estimates from Bolocam Sunyaev-Zel'dovich images
- Bandpass Dependence of X-ray Temperatures in Galaxy Clusters
- Early structure formation in quintessence models and its implications for cosmic reionisation from first stars
- Toward an accurate mass function for precision cosmology
- Implications of multiple high-redshift galaxy clusters
- Photometric Redshift Requirements for Self-Calibration of Cluster Dark Energy Studies
- The value of the equation of state of dark energy
- Cosmic tomographies: baryon acoustic oscillations and weak lensing
- Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing
- The Atacama Cosmology Telescope: Relation Between Galaxy Cluster Optical Richness and Sunyaev-Zel'dovich Effect
- Structure formation in cosmologies with oscillating dark energy
- The Impact of Galaxy Cluster Mergers on Cosmological Parameter Estimation from Surveys of the Sunyaev-Zel'dovich Effect
- Constraining the expansion rate of the Universe using low-redshift ellipticals as cosmic chronometers
- Tracing the Gas to the Virial Radius (R100) in a Fossil Group
- The XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraints
- Growth Rate of Large Scale Structure as a Powerful Probe of Dark Energy
- A Systematic Search for High Surface Brightness Giant Arcs in a Sloan Digital Sky Survey Cluster Sample
- Reconstructing mass profiles of simulated galaxy clusters by combining Sunyaev-Zeldovich and X-ray images
- Cosmological Constraint on and from Cluster Abundances using the Optical-Spectroscopic SDSS Catalog
- Weak lensing analysis of RXC J2248.7-4431
- Quintessence Cosmology and the Cosmic Coincidence
- Baryon Oscillations and Consistency Tests for Photometrically-Determined Redshifts of Very Faint Galaxies
- Understanding Cluster Gas Evolution and Fine-Scale CMB Anisotropy with Deep Sunyaev-Zel'dovich Effect Surveys
- Weak-Lensing Mass Measurements of Five Galaxy Clusters in the South Pole Telescope Survey Using Magellan/Megacam
- The Impact of Halo Properties, Energy Feedback and Projection Effects on the Mass-SZ Flux Relation
- Weak Lensing Discovery and Tomography of a Cluster at z=0.68
- Quintessential Baryogenesis
- Dark energy constraints from lensing-detected galaxy clusters
- Three-Dimensional Mapping of the Dark Matter
- Improved optical mass tracer for galaxy clusters calibrated using weak lensing measurements
- Lensing Magnification: Implications for Counts of Submillimeter Galaxies and SZ Clusters
- Growth of Cosmic Structure
- Sensitivity of galaxy cluster dark energy constraints to halo modeling uncertainties
- WMAP constraints on the Intra-Cluster Medium
- The SRG/eROSITA All-Sky Survey: Dark Energy Survey Year 3 Weak Gravitational Lensing by eRASS1 selected Galaxy Clusters
- Redshift Accuracy Requirements for Future Supernova and Number Count Surveys
- Cluster Masses Accounting for Structure along the Line of Sight
- Cosmological Constraint Precision of the Photometric and Spectroscopic Multi-probe Surveys of China Space Station Telescope (CSST)
- A high precision semi-analytic mass function
- Likelihood Methods for Cluster Dark Energy Surveys
- The X-ray Properties of Optically-Selected Galaxy Clusters
- A new method to measure the mass of galaxy clusters
- Batch discovery of nine z~1 clusters using x-ray and K or R,z' images
- Accurate Realizations of the Ionized Gas in Galaxy Clusters: Calibrating Feedback
- Constraining Dark Energy with Clusters: Complementarity with Other Probes
- Primordial non-Gaussianity and Dark Energy constraints from Cluster Surveys
- Gravitational Lensing of the Microwave Background by Galaxy Clusters
- Cosmological parameters constraints from galaxy cluster mass function measurements in combination with other cosmological data
- Extrinsic Sources of Scatter in the Richness-Mass Relation of Galaxy Clusters
- Bias from gas inhomogeneities in the pressure profiles as measured from X-ray and SZ observations
- On the implementation of the spherical collapse model for dark energy models
- The signature of dark energy perturbations in galaxy cluster surveys
- Number counts in homogeneous and inhomogeneous dark energy models
- Microwave-Sky Simulations and Projections for Galaxy Cluster Detection with the Atacama Cosmology Telescope
- Implications for quintessence models from MAXIMA-1 and BOOMERANG-98
- The Effects of Halo Assembly Bias on Self-Calibration in Galaxy Cluster Surveys
- Morphological estimators on Sunyaev--Zel'dovich maps of MUSIC clusters of galaxies
- Constraining Dark Energy Evolution with Gravitational Lensing by Large Scale Structures
- The cosmological analysis of X-ray cluster surveys: I- A new method for interpreting number counts
- Non-linear Galaxy Power Spectrum and Cosmological Parameters
- Impact of Chandra calibration uncertainties on galaxy cluster temperatures: application to the Hubble Constant
- Are Clusters Standard Candles? Galaxy Cluster Scaling Relations With the Sunyaev-Zeldovich Effect
- The Mass, Baryonic Fraction, and X-ray Temperature of the Luminous, High Redshift Cluster of Galaxies, MS0451.6-0305
- Infrared and millimetre-wavelength evidence for cold accretion within a z = 2.83 Lyman-alpha blob
- Determining the equation of state of dark energy from angular size of compact radio sources and X-ray gas mass fraction of galaxy clusters
- The Selection Function of SZ Cluster Surveys
- Statistics of Sunyaev-Zel'dovich Cluster Surveys
- Constraining Cosmology with High Convergence Regions in Weak Lensing Surveys
- CMB-Cluster Lensing
- Completeness in Photometric and Spectroscopic Searches for Clusters
- First lensing measurements of SZ-discovered clusters
- Cosmological Simulations of the Preheating Scenario for Galaxy Cluster Formation: Comparison to Analytic Models and Observations
- Cluster scaling relations from cosmological hydrodynamic simulations in dark energy dominated universe
- CMB Polarization towards Clusters as a Probe of the Integrated Sachs-Wolfe Effect
- Galaxy Kinematics and Mass Calibration in Massive SZE Selected Galaxy Clusters to z=1.3
- Cosmology with clusters of galaxies
- The most massive objects in the Universe
- Merging Galaxy Clusters: Offset Between the Sunyaev-Zel'dovich Effect and X-ray Peaks
- SZE Signals in Cluster Models
- A Chandra Study of the Effects of a Major Merger on the Structure of Abell 2319
- A deep learning view of the census of galaxy clusters in IllustrisTNG
- The dark matter distribution in z~0.5 clusters of galaxies. I : Determining scaling relations with weak lensing masses
- Annealing a Follow-up Program: Improvement of the Dark Energy Figure of Merit for Optical Galaxy Cluster Surveys
- Mapping the Universe: The 2010 Russell Lecture
- Effects of the complex mass distribution of dark matter halos on weak lensing cluster surveys
- Shear-Selected Clusters From the Deep Lens Survey III: Masses from Weak Lensing
- The ROSAT-ESO Flux-Limited X-Ray (REFLEX) Galaxy Cluster Survey VI: Constraints on the cosmic matter density from the KL power spectrum
- Cosmology with Galaxy Clusters in the XMM Large-Scale Structure Survey
- Weak Lensing Analysis of SPT selected Galaxy Clusters using Dark Energy Survey Science Verification Data
- Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- I. The Richness-Mass Relation
- A Parametrized Galaxy Catalog Simulator For Testing Cluster Finding, Mass Estimation and Photometric Redshift Estimation in Optical and Near Infrared Surveys
- Apparent Clustering of Intermediate-redshift Galaxies as a Probe of Dark Energy
- Challenges for Precision Cosmology with X-ray and Sunyaev-Zeldovich Effect Gas Mass Measurements of Galaxy Clusters
- Constraining Dark Energy by Combining Cluster Counts and Shear-Shear Correlations in a Weak Lensing Survey
- Exploring Cosmic Origins with CORE: Cluster Science
- Dark Matter Structures In The Deep Lens Survey
- WMAP5 and the Cluster Mass Function
- Definitive Test of the R_h=ct Universe Using Redshift Drift
- Constraints on the solid dark universe model
- Dark energy parameterizations and their effect on dark halos
- Stellar Mass to Halo Mass Scaling Relation for X-ray Selected Low Mass Galaxy Clusters and Groups out to Redshift
- Optimizing weak lensing mass estimates for cluster profile uncertainty
- Can Virialization Shocks be Detected Around Galaxy Clusters Through the Sunyaev-Zel'dovich Effect?
- The SZ effect as a cosmological discriminator
- Constraining AGN triggering mechanisms through the clustering analysis of active black holes
- The Atacama Cosmology Telescope: High-Resolution Sunyaev-Zel'dovich Array Observations of ACT SZE-selected Clusters from the Equatorial Strip
- Friends-of-Friends Groups and Clusters in the 2SLAQ Catalogue
- Weak-lensing calibration of a stellar mass-based mass proxy for redMaPPer and Voronoi Tessellation clusters in SDSS Stripe 82
- Joint X-Ray and Optical Measurements of the Mass Distribution of the Distant Galaxy Cluster CLJ 0152.7-1357
- Gamma-ray probe of cosmic-ray pressure in galaxy clusters and cosmological implications
- Probing dark energy with the CMB: projected constraints from WMAP and Planck
- The Sloan Nearby Cluster Weak Lensing Survey
- Optical & Sunyaev-Zel'dovich Observations of a New Sample of Distant Rich Galaxy Clusters in the ROSAT All Sky Survey
- Measuring the Cosmic Equation of State with Galaxy Clusters in the DEEP2 Redshift Survey
- Constraints in Cosmological Parameter Space from the Sunyaev-Zel'dovich Effect and Thermal Bremsstrahlung
- Constraints on the Energy Content of the Universe from a Combination of Galaxy Cluster Observables
- Dynamical signatures of infall around galaxy clusters: a generalized Jeans equation
- Removing the giants and learning from the crowd: a new SZ power spectrum method and revised Compton -map analysis
- GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ()
- Covariance matrices for galaxy cluster weak lensing: from virial regime to uncorrelated large-scale structure
- Impact of Weak Lensing Mass Calibration on eROSITA Galaxy Cluster Cosmological Studies -- a Forecast
- Weak lensing peak count as a probe of f(R) theories
- Constrained Cluster Parameters from Sunyaev-Zel'dovich Observations
- Extending empirical constraints on the SZ-mass scaling relation to higher redshifts via HST weak lensing measurements of nine clusters from the SPT-SZ survey at
- Weak lensing mass modeling bias and the impact of miscentring
- The Outer Stellar Mass of Massive Galaxies: A Simple Tracer of Halo Mass with Scatter Comparable to Richness and Reduced Projection Effects
- On the Origin of Cool Core Galaxy Clusters: Comparing X-Ray Observations with Numerical Simulations
- A robust lower limit on the amplitude of matter fluctuations in the universe from cluster abundance and weak lensing
- Virialization of high redshift dark matter haloes
- Cosmological Acceleration Through Transition to Constant Scalar Curvature
- Non-Gaussian Scatter in Cluster Scaling Relations
- Galaxy Clusters as a probe of early dark energy
- Extracting Galaxy Cluster Gas Inhomogeneity from X-ray Surface Brightness: A Statistical Approach and Application to Abell 3667
- Impact of Systematic Errors in Sunyaev-Zel'dovich Surveys of Galaxy Clusters
- Cosmology with galaxy cluster weak lensing: statistical limits and experimental design
- Issues in joint SZ and optical cluster finding
- Improving cosmological constraints from galaxy cluster number counts with CMB-cluster-lensing data: Results from the SPT-SZ survey and forecasts for the future
- The KMOS Cluster Survey (KCS) III: fundamental plane of cluster galaxies at in JKCS 041
- SARCS strong lensing galaxy groups: I - optical, weak lensing, and scaling laws
- The Impact of Cluster Structure and Dynamical State on Scatter in the Sunyaev-Zel'dovich Flux-Mass Relation
- Tracing the Nature of Dark Energy with Galaxy Distribution
- Cluster cosmology with anisotropic boosts: Validation of a novel forward modeling analysis and application on SDSS redMaPPer clusters
- Raytracing simulations of coupled dark energy models
- Validation of Selection Function, Sample Contamination and Mass Calibration in Galaxy Cluster Samples
- Breaking Cosmological Degeneracies in Galaxy Cluster Surveys with a Physical Model of Cluster Structure
- Optimal Chandra/XMM-Newton Band-Passes for Detecting Low Temperature Groups and Clusters of Galaxies
- Superclusters with thermal SZ effect surveys
- WMAP Observations of Planck ESZ Clusters
- Cosmological Perturbations and the Running Cosmological Constant Model
- Cosmological Parameter Determination from Counts of Galaxies
- A low-redshift galaxy cluster X-ray Temperature Function incorporating Suzaku data
- Tomography of the Reionization Epoch with Multifrequency CMB Observations
- Super-sample covariance of the thermal Sunyaev-Zel'dovich effect
- On the Angular Correlation Function of SZ Clusters : Extracting cosmological information from a 2D catalog
- Cross-correlating the Thermal Sunyaev-Zel'dovich Effect and the Distribution of Galaxy Clusters
- Galaxy cluster scaling relations measured with APEX-SZ
- Biases on cosmological parameter estimators from galaxy cluster number counts
- Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- II. The X-ray Luminosity-Mass Relation
- Masses: Weak Lensing Calibration of the Dark Energy Survey Year 1 redMaPPer Clusters using Stellar Masses
- Likelihood-free Forward Modeling for Cluster Weak Lensing and Cosmology
- The ACT-DR5 MCMF Galaxy Cluster Catalog
- Evolution of Spherical Overdensity in Thawing Dark energy Models
- Bolocam Observations of Two Unconfirmed Galaxy Cluster Candidates from the Planck Early SZ Sample
- Cosmology with the Planck cluster sample
- Is the Universe Inflating? Dark Energy and the Future of the Universe
- Evolution of density perturbations in double exponential quintessence models
- Combining Weak Lensing Tomography with Halo Clustering to Probe Dark Energy
- The CluMPR Galaxy Cluster-Finding Algorithm and DESI Legacy Survey Galaxy Cluster Catalogue
- Covariance of dark energy parameters and sound speed constraints from large HI surveys
- Constraining Intra-cluster Gas Models with AMiBA13
- Why are we still using 3D masses for cluster cosmology?
- Probing interacting dark sector models with future weak lensing-informed galaxy cluster abundance constraints from SPT-3G and CMB-S4
- Probing Cosmology and Galaxy Cluster Structure with the Sunyaev-Zel'dovich Decrement vs. X-ray Temperature Scaling Relation
- XMM-Newton observation of the cluster ZW 1305.4+2941 in the field SA 57
- Determining Distances to Clusters of Galaxies using Resonant X-ray Emission Lines
- Studying Dark Energy with Galaxy Cluster Surveys
- Cosmological constraints from a 2D SZ catalog
- Galaxy cluster aperture masses are more robust to baryonic effects than 3D halo masses
- An Evolving Entropy Floor in the Intracluster Gas?
- Systematic Errors in Sunyaev-Zeldovich Surveys of Galaxy Cluster Velocities
- The Sunyaev-Zel'dovich Effect: Results and Future Prospects
- Optimizing the yield of Sunyaev-Zel'dovich cluster surveys
- Cosmological Implications of the BIMA 30 Ghz Sunyaev-Zel'dovich Effect Galaxy Cluster Survey
- Effects of tidal gravitational fields in clustering dark energy models
- Geometrical tests of cosmological models. I. Probing dark energy using the kinematics of high-redshift galaxies
- Beyond the Standard Model of Physics with Astronomical Observations
- Weak lensing in the blue: a counter-intuitive strategy for stratospheric observations
- Complementarity of Future Dark Energy Probes
- Structure formation and CMBR anisotropy spectrum in the inflessence model
- The Gaussian cell two-point "energy-like" equation: Application to large scale galaxy redshift and peculiar motion surveys
- The Effects of Relativistic Corrections on Cosmological Parameter Estimations from SZE Cluster Surveys
- A Search for Neutron Star Precession and Interstellar Magnetic Field Variations via Multiepoch Pulsar Polarimetry
- Evidence for Non-Linear Growth of Structure from an X-ray Selected Cluster Survey using a Novel Joint Analysis of the Chandra and XMM-Newton Archives
- Using Galaxy Cluster Peculiar Velocities to Constrain Cosmological Parameters
- The Impact of Non-Equipartition on Cosmological Parameter Estimation from Sunyaev-Zel'dovich Surveys
- Redshift estimation of clusters by wavelet decomposition of their Sunyaev-Zel'dovich morphology
- Morphological Redshift Estimates for Galaxy Clusters in a Sunyaev-Zel'dovich Effect Survey
- A Deep Chandra Observation of the Distant Galaxy Cluster MS1137.5+6625
- DUET - The Dark Universe Exploration Telescope
- Point Source Confusion in SZ Cluster Surveys
- The Standard Model, Dark Matter, and Dark Energy: From the Sublime to the Ridiculous
- Constraining cosmology with thermal Sunyaev-Zel'dovich maps: Minkowski functionals, peaks, minima, and moments
- Measuring the scatter of the mass-richness relation in galaxy clusters in photometric imaging surveys by means of their correlation function
- Cosmological constraints from Sunyaev-Zeldovich cluster counts: an approach to account for missing redshifts
- AMR Simulations of the Cosmological Light Cone: SZE Surveys of the Synthetic Universe
- The abundance of lensing protoclusters
- The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE
- Galaxy cluster count cosmology with simulation-based inference
- Distances and Cosmology From Galaxy Cluster CMB Data
- Directional miscentering dependence in weak lensing mass bias
- Aemulus : Precision halo mass functions in wCDM cosmologies
- Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations
- Impact of projection-induced optical selection bias on the weak lensing mass calibration of galaxy clusters
- Constraints on the normal branch of DGP gravity from SPT galaxy clusters with DES and HST weak-lensing mass calibration and from Planck PR4 CMB anisotropies
- Mining the Sky with Redshift Surveys
- Observed Smooth Energy Fitted by Parametrized Quintessence
- The impact of projection effects on cluster observables: stacked lensing and projected clustering
- Optical followup of galaxy clusters detected by the South Pole Telescope
- The XMM-BCS galaxy cluster survey: I. The X-ray selected cluster catalog from the initial 6 deg
- High-redshift clusters from NVSS: The TexOx Cluster (TOC) Survey
- Dynamical Properties and Velocity Dispersion-Mass Relation of Galaxy Clusters from the GOGREEN and GCLASS Surveys
- Optical Wavelength Guided Self-Supervised Feature Learning For Galaxy Cluster Richness Estimate