Cosmology with the Sunyaev-Zel'dovich Effect

Abstract

The Sunyaev-Zel'dovich effect (SZE) provides a unique way to map the large-scale structure of the universe as traced by massive clusters of galaxies. As a spectral distortion of the cosmic microwave background, the SZE is insensitive to the redshift of the galaxy cluster, making it well-suited for studies of clusters at all redshifts, and especially at reasonably high redshifts (z > 1) where the abundance of clusters is critically dependent on the underlying cosmology. Recent high signal-to-noise detections of the SZE have enabled interesting constraints on the Hubble constant and the matter density of the universe using small samples of galaxy clusters. Upcoming SZE surveys are expected to find hundreds to thousands of new galaxy clusters, with a mass selection function that is remarkably uniform with redshift. In this review we provide an overview of the SZE and its use for cosmological studies with emphasis on the cosmology that can, in principle, be extracted from SZE survey yields. We discuss the observational and theoretical challenges that must be met before precise cosmological constraints can be extracted from the survey yields.

submitted to ARAA Oct 2001, to appear ARAA, 2002, V40

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• Galaxy Cluster Pressure Profiles as Determined by Sunyaev Zel'dovich Effect Observations with MUSTANG and Bolocam I: Joint Analysis Technique
• Pilot-WINGS: An extended MUSE view of the structure of Abell 370
• Exploiting NIKA2/XMM-Newton imaging synergy for intermediate mass, high-$z$ galaxy clusters within the NIKA2 SZ Large Program
• SZ polarisation as a probe of the intracluster medium
• A simple parametric model for spherical galaxy clusters
• Galaxy clusters and a possible variation of the fine structure constant
• The Atacama Cosmology Telescope: the stellar content of galaxy clusters selected using the Sunyaev-Zel'dovich effect
• RAY-RAMSES: a code for ray tracing on the fly in N-body simulations
• Constrained Cluster Parameters from Sunyaev-Zel'dovich Observations
• Imprints of primordial non-Gaussianities in X-ray and SZ signals from galaxy clusters
• Galaxy Clusters at z>=1: Gas Constraints from the Sunyaev-Zel'dovich Array
• The Shape of Galaxy Cluster Dark Matter Haloes: Systematics of Its Imprint on Cluster Gas, and Comparison to Observations
• Spectroscopic confirmation and velocity dispersions for twenty Planck galaxy clusters at 0.16<z<0.78
• A method to search for bulk motions in the ICM with {\sl Chandra} CCD spectra: application to the Bullet cluster
• Quasar Host Environments: The view from Planck
• Galaxy cluster Sunyaev-Zel'dovich effect scaling-relation and type Ia supernova observations as a test for the cosmic distance duality relation
• The estimation of the SZ effects with unbiased multifilters
• Galaxy Clusters as a probe of early dark energy
• A 3% Determination of $H_0$ at Intermediate Redshifts
• Cluster temperature profiles and Sunyaev-Zeldovich observations
• Physical Properties of Four SZE-Selected Galaxy Clusters in the Southern Cosmology Survey
• Finding Clusters in SZ Surveys
• Patchy Kinetic Sunyaev-Zel'dovich Effect with Controlled Reionization History and Morphology
• Planck Intermediate Results II: Comparison of Sunyaev-Zeldovich measurements from Planck and from the Arcminute Microkelvin Imager for 11 galaxy clusters
• Extracting Galaxy Cluster Gas Inhomogeneity from X-ray Surface Brightness: A Statistical Approach and Application to Abell 3667
• A measurement of the mean central optical depth of galaxy clusters via the pairwise kinematic Sunyaev-Zel'dovich effect with SPT-3G and DES
• Impact of Systematic Errors in Sunyaev-Zel'dovich Surveys of Galaxy Clusters
• Bayesian analysis of weak gravitational lensing and Sunyaev-Zel'dovich data for six galaxy clusters
• Prospects for ACT: simulations, power spectrum, and non-Gaussian analysis
• MultiDark-Clusters: Galaxy Cluster Mock Light-Cones, eROSITA and the Cluster Power Spectrum
• Issues in joint SZ and optical cluster finding
• Searching for High-Energy Neutrino Emission from Galaxy Clusters with IceCube
• AMiBA Wideband Analog Correlator
• High-significance Sunyaev-Zel'dovich measurement: Abell 1914 seen with the Arcminute Microkelvin Imager
• Baryon content and dynamic state of galaxy clusters: XMM-Newton observations of A1095 and A1926
• Unveiling the merger dynamics of the most massive MaDCoWS cluster at $z=1.2$ from a multi-wavelength mapping of its intracluster medium properties
• CMB Polarization due to Scattering in Clusters
• DeepSZ: Identification of Sunyaev-Zel'dovich Galaxy Clusters using Deep Learning
• Dissecting the Compton scattering kernel I: Isotropic media
• SARCS strong lensing galaxy groups: I - optical, weak lensing, and scaling laws
• Observations of the Corona Borealis supercluster with the superextended Very Small Array: further constraints on the nature of the non-Gaussian CMB cold spot
• Analytical Study on the Sunyaev-Zeldovich Effect for Clusters of Galaxies
• Impact of ICM disturbances on the mean pressure profile of galaxy clusters: a prospective study of the NIKA2 SZ large program with MUSIC synthetic clusters
• Optical Characterization of the SPT-3G Focal Plane
• The Santa Fe Light Cone Simulation Project: II. The Prospects for Direct Detection of the WHIM with SZE Surveys
• CENN: A fully convolutional neural network for CMB recovery in realistic microwave sky simulations
• Atacama Cosmology Telescope measurements of a large sample of candidates from the Massive and Distant Clusters of WISE Survey: Sunyaev-Zeldovich effect confirmation of MaDCoWS candidates using ACT
• The distribution of two-dimensional eccentricity of Sunyaev-Zeldovich Effect and X-ray surface brightness profiles
• Tangential Velocity of the Dark Matter in the Bullet Cluster from Precise Lensed Image Redshifts
• Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: I. Evidence for thermal energy anisotropy using oriented stacking
• Cosmology from weak lensing, galaxy clustering, CMB lensing and tSZ: I. 10x2pt Modelling Methodology
• Galaxy Clusters at 0.9<z<1.7 in the AKARI NEP deep field
• Multi-wavelength mock observations of the WHIM in a simulated galaxy cluster
• Probability Friends-of-Friends (PFOF) Group Finder: Performance Study and Observational Data Applications on Photometric Surveys
• Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs
• Mass Selection Bias in Galaxy Cluster Peculiar Velocities from the Kinetic Sunyaev-Zel'dovich Effect
• Relativistic Corrections to the Sunyaev-Zeldovich Effect for Clusters of Galaxies. V. Effect of the Motion of the Observer
• Superclusters with thermal SZ effect surveys
• Beyond the Standard Lore of the SZ effect
• The thermal and non-thermal components within and between galaxy clusters Abell 399 and Abell 401
• Planck/SDSS Cluster Mass and Gas Scaling Relations for a Volume-Complete redMaPPer Sample
• Efficient Differential Fourier-Transform Spectrometer for precision Sunyaev-Zel'dovich effect measurements
• WMAP Observations of Planck ESZ Clusters
• Neutrino Mass Inference from SZ Surveys
• Sunyaev-Zel'dovich observations of galaxy clusters out to the virial radius with the Arcminute Microkelvin Imager
• High angular resolution observation of the Sunyaev-Zel'dovich effect in the massive z=0.83 cluster ClJ0152-1357
• The Science Case for PILOT I: Summary and Overview
• Probing the cosmic microwave background temperature using the Sunyaev-Zeldovich effect
• Sunyaev-Zel'dovich Cluster Survey Simulations for Planck
• Measuring the Mach number of the Universe via the Sunyaev-Zeldovich effect
• SALT spectroscopic observations of galaxy clusters detected by ACT and a Type II quasar hosted by a brightest cluster galaxy
• Preliminary Sunyaev Zel'dovich Observations of Galaxy Clusters with OCRA-p
• Extraction of cluster parameters with future Sunyaev-Zel'dovich observations
• The Clusters Hiding in Plain Sight (CHiPS) survey: Complete sample of extreme BCG clusters
• Percent-level constraints on baryonic feedback with spectral distortion measurements
• Refined modelling of the radio SZ signal: kinematic terms, relativistic temperature corrections and anisotropies in the radio background
• X-ray mapping the outer regions of galaxy clusters at z= 0.23 and 0.45
• Reconstructing three-dimensional parameters of galaxy clusters via multifrequency SZ observations
• Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
• The Evolution and Mass Dependence of Galaxy Cluster Pressure Profiles at 0.05 $\le z\le$ 0.60 and $4\times 10^{14}$ M${}_{\odot }$ $\le {\text{M}}_{500}\le 30\times 10^{14}$ M${}_{\odot }$
• Constraining H0 in General Dark Energy Models from Sunyaev-Zeldovich/X-ray Technique and Complementary Probes
• Millimetric observation of the SZ effect in the Corona Borealis supercluster
• Extraction of cluster parameters from Sunyaev-Zeldovich effect observations with simulated annealing optimization
• Super-sample covariance of the thermal Sunyaev-Zel'dovich effect
• Mass and pressure constraints on galaxy clusters from interferometric SZ observations
• A multifrequency method based on the Matched Multifilter for the detection of point sources in CMB maps
• Synthesizing Stellar Populations in South Pole Telescope Galaxy Clusters: I. Ages of Quiescent Member Galaxies at 0.3 < z < 1.4
• Observational Cosmology
• The Sunyaev-Zeldovich Signal of the maxBCG SDSS Galaxy Clusters in WMAP
• Statistical properties of SZ and X-ray cluster detections
• 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
• Calibrating the Planck Cluster Mass Scale with Cluster Velocity Dispersions
• Measurement of the Sunyaev-Zel'dovich Increment in Massive Galaxy Clusters
• GBT/MUSTANG-2 9" resolution imaging of the SZ effect in MS0735.6+7421: Confirmation of the SZ Cavities through direct imaging
• Modifications to the Cosmic 21-cm Background Frequency Spectrum by Scattering via electrons in Galaxy Clusters
• Systematic Errors in the Hubble Constant Measurement from the Sunyaev-Zel'dovich effect
• Small scale contributions to CMB: A coherent analysis
• Cosmography with the Sunyaev-Zeldovich effect and X-ray data
• Inference of gravitational lensing and patchy reionization with future CMB data
• Clusters of galaxies: setting the stage
• Further Sunyaev-Zel'dovich observations of two Planck ERCSC clusters with the Arcminute Microkelvin Imager
• The Observable Thermal and Kinetic Sunyaev-Zel'dovich Effect in Merging Galaxy Clusters
• AMI SZ observations and Bayesian analysis of a sample of six redshift-one clusters of galaxies
• Cluster-Cluster Lensing and the Case of Abell 383
• Measurements of the Sunyaev-Zel'dovich Effect in MACS J0647.7+7015 and MACS J1206.2-0847 at High Angular Resolution with MUSTANG
• Dynamical quintessence fields Press-Schechter mass function: detectability and effect on dark haloes
• Constraints on the Hubble Parameter from galaxy clusters and the Validity of the Cosmic Distance Duality Relation
• Search for GeV Gamma-Ray Emission from SPT-SZ selected Galaxy Clusters with 15 years of Fermi-LAT data
• Subdegree Sunyaev-Zel'dovich Signal from Multifrequency BOOMERanG observations
• Mitigating the impact of the CIB on galaxy cluster SZ detection with spectrally constrained matched filters
• Intracluster Entropy from Joint X-ray and Sunyaev-Zel'dovich Observations
• Cosmology with the Planck cluster sample
• Impact of a non-Gaussian density field on Sunyaev-Zeldovich observables
• An Optical Observational Cluster Mass Function at $z\sim 1$ with the ORELSE Survey
• Impact of thermal diffusion and other abundance anomalies on cosmological uses of galaxy clusters
• Order statistics applied to the most massive and most distant galaxy clusters
• Free-form modelling of galaxy clusters: a Bayesian and data-driven approach
• Weak lensing mass estimates of galaxy groups and the line-of-sight contamination
• Limits on evolution of the fine-structure constant in runaway dilaton models from Sunyaev-Zeldovich Observations
• Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope
• Real space tomography of the primordial Universe with cluster polarization
• Magnetic Sunyaev-Zel'dovich effect in galaxy clusters
• Observing the Sunyaev-Zel'dovich Effect Closer to Home
• Optical follow-up study of 32 high-redshift galaxy cluster candidates from Planck with the William Herschel Telescope
• Emulating Sunyaev-Zeldovich Images of Galaxy Clusters using Auto-Encoders
• Joint cosmology and mass calibration from tSZ cluster counts and cosmic shear
• CARMA follow-up of the northern unconfirmed PLANCK galaxy cluster candidates
• Probing the cluster pressure profile with thermal Sunyaev-Zeldovich effect and weak lensing cross-correlation
• Sunyaev-Zel'dovich Signal from Quasar Hosts: Implications for Detection of Quasar Feedback
• Angular diameter distance estimates from the Sunyaev-Zel'dovich effect in hydrodynamical cluster simulations
• The Atacama Cosmology Telescope: The LABOCA/ACT Survey of Clusters at All Redshifts
• Lensed CMB power spectrum biases from masking extragalactic sources
• Imaging Simulations of the Sunyaev-Zel'dovich Effect for ALMA
• A joint analysis of AMI and CARMA observations of the recently discovered SZ galaxy cluster system AMI-CL J0300+2613
• A blind detection of a large, complex, Sunyaev--Zel'dovich structure
• Parameterization Effects in the analysis of AMI Sunyaev-Zel'dovich Observations
• MILCANN : A neural network assessed tSZ map for galaxy cluster detection
• X-ray Clusters of Galaxies as Cosmological Tools
• CMB Comptonization in Clusters: Spectral and Angular Power from Evolving Polytropic Gas
• New Horizons in Cosmology with Spectral Distortions of the Cosmic Microwave Background
• Systematic errors in the determination of Hubble constant due to the asphericity and non-isothermality of clusters of galaxies
• Sunyaev-Zel'dovich power spectrum with decaying cold dark matter
• The thermal SZ tomography
• Relativistic inverse Compton scattering of photons from the early universe
• Breaking the baryon-dark matter degeneracy in a model-independent way through the Sunyaev-Zeldovich effect
• Uncertainties in the S-Z selected cluster angular power spectrum
• Separating the kinetic SZ effect from primary CMB fluctuations
• Signature of cool cores in SZ clusters: a multiwavelength approach
• Introducing constrained matched filters for improved separation of point sources from galaxy clusters
• Sunyaev-Zel'dovich scaling relations from a simple phenomenological model for galaxy clusters
• Revisiting GeV-scale annihilating dark matter with the AMS-02 positron fraction
• Relativistic corrections to the Kompaneets equation
• A potentially pure test of cosmic geometry: galaxy clusters and the real space Alcock-Paczynski test
• Joint signal extraction from galaxy clusters in X-ray and SZ surveys: A matched-filter approach
• Pairwise kSZ signal extraction efficacy and optical depth estimation
• The kinetic Sunyaev-Zel'dovich tomography II: probing the circumgalactic medium
• SZ observations with AMI of the hottest galaxy clusters detected in the XMM-Newton Cluster Survey
• Fundamental Plane of Sunyaev-Zeldovich clusters
• Detection of Hot Gas in Galaxy Groups via the Sunyaev-Zel'dovich Effect
• Cosmological constraints from a 2D SZ catalog
• Constraining Intra-cluster Gas Models with AMiBA13
• Joint analysis of X-ray and Sunyaev Zel'dovich observations of galaxy clusters using an analytic model of the intra-cluster medium
• Testing the SZ-based tomographic approach to the thermal history of the universe with pressure-density cross-correlations: Insights from the Magneticum simulation
• Decrease in the Brightness of the Cosmic X-ray and Soft Gamma-ray Background toward Clusters of Galaxies
• A model-independent test of the evolution of gas depletion factor for SPT-SZ and Planck ESZ clusters
• Galaxy cluster SZ detection with unbiased noise estimation: an iterative approach
• Inverse-Compton Scattering of the Cosmic Infrared Background
• Probing Cosmology and Galaxy Cluster Structure with the Sunyaev-Zel'dovich Decrement vs. X-ray Temperature Scaling Relation
• Determining Distances to Clusters of Galaxies using Resonant X-ray Emission Lines
• Compact source detection in multi-channel microwave surveys: from SZ clusters to polarized sources
• Model-Independent Limits on the Line-of-Sight Depth of Clusters of Galaxies Using X-ray and Sunyaev-Zel'dovich Data
• Study on the Solutions of the Sunyaev-Zeldovich Effect for Clusters of Galaxies
• Is the non-isothermal double $\beta$-model incompatible with no time evolution of galaxy cluster gas mass fraction ?
• The XXL survey: XLII. Detection and characterization of the galaxy population of distant galaxy clusters in the XXL-N/VIDEO field: A tale of variety
• Comparison of numerical methods for computing the repeated Compton scattering of photons in isotropic media
• The Evolution of Cluster Early-Type Galaxies over the Past 8 Gyr
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• Lyman-alpha forest-CMB cross-correlation and the search for the ionized baryons at high redshift
• Estimating Power Spectrum of Sunyaev-Zeldovich Effect from the Cross-Correlation between WMAP and 2MASS
• Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps
• Optical validation and characterisation of Planck PSZ1 sources at the Canary Islands observatories. II. Second year of ITP13 observations
• Some astrophysical implications of dark matter and gas profiles in a new galaxy clusters model
• Stokes parameters spectral distortions due to the Sunyaev-Zel'dovich effect and an independent estimation of the CMB low multipoles
• Radio source contamination of the Sunyaev-Zeldovich effect in galaxy clusters
• A Method for Mapping the Temperature Profile of X-ray Clusters Through Radio Observations
• On the modelling of the excesses of galaxy clusters over high-mass thresholds
• Cosmological Implications of the BIMA 30 Ghz Sunyaev-Zel'dovich Effect Galaxy Cluster Survey
• The NIKA2 Sunyaev-Zeldovich Large Program
• Galaxy clusters as probes for cosmology and dark matter
• The Ups and Downs of the Hubble Constant
• Mapping the temperature of the intra-cluster medium with the tSZ effect
• New constraints on H_0 and Omega_M from SZE/X-RAY data and Baryon Acoustic Oscillations
• A Diffused Background from Axion-like Particles in the Microwave Sky
• Polarization of Sunyaev-Zeldovich signal due to electron pressure anisotropy in galaxy clusters
• Probing galaxy cluster and intra-cluster gas with luminous red galaxies
• KISS: a spectrometric imager for millimetre cosmology
• Weak Lensing analysis of Abell 2390 using short exposures
• Analytical studies on the Sunyaev Zeldovich effect in the cluster of galaxies for three Lorentz frames
• Constraints on the SZ Power Spectrum on Degree Angular Scales in WMAP Data
• The Growth of Baryonic Structure in the Presence of Cosmological Magnetic Pressure
• Analysis of the Amplitude of the Sunyaev-Zel'dovich Effect out to Redshift z=0.8
• The Effects of Relativistic Corrections on Cosmological Parameter Estimations from SZE Cluster Surveys
• Total power horn-coupled 150 GHz LEKID array for space applications
• The Gaussian cell two-point "energy-like" equation: Application to large scale galaxy redshift and peculiar motion surveys
• Identification of galaxy clusters in cosmic microwave background maps using the Sunyaev-Zel'dovich effect
• A large thermal energy reservoir in the nascent intracluster medium at a redshift of 4.3
• Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect
• A measurement of cluster masses using Planck and SPT-SZ CMB lensing
• The Impact of Non-Equipartition on Cosmological Parameter Estimation from Sunyaev-Zel'dovich Surveys
• A Search for Neutron Star Precession and Interstellar Magnetic Field Variations via Multiepoch Pulsar Polarimetry
• Redshift estimation of clusters by wavelet decomposition of their Sunyaev-Zel'dovich morphology
• The XMM Cluster Survey: Predicted overlap with the Planck Cluster Catalogue
• Observing the Epoch of Reionization with the Cosmic Microwave Background
• Observability of the virialization phase of spheroidal galaxies with radio arrays
• Point Source Confusion in SZ Cluster Surveys
• Analytical Study on the Sunyaev-Zeldovich Effect for Clusters of Galaxies. II. comparison of covariant formalisms
• The Kinetic Sunyaev-Zel'dovich effect of the Milky Way Halo
• Observing the Evolution of the Universe
• Revealing the Warm and Hot Halo Baryons via Thomson Scattering of Quasar Light
• Galaxy clusters in the CFHTLS. First matched filter candidate catalogue of the Deep fields
• The Atacama Cosmology Telescope: SZ-based masses and dust emission from IR-selected cluster candidates in the SHELA survey
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Linearized Kompaneetz equation as a relativistic diffusion
• Empirical test for relativistic kinetic theories based on the Sunyaev-Zel'dovich effect
• Analytical studies on the Sunyaev-Zeldovich effect in the cluster of galaxies for three Lorentz frames II: single integral formula
• Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs
• Probing the Cosmic Distance Duality Relation via Non-Parametric Reconstruction for High Redshifts
• On the accuracy of the high redshift cluster luminosity function
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• An SZ-Like Effect on Cosmological Gravitational Wave Backgrounds
• SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
• CARMA observations of massive Planck-discovered cluster candidates at z>0.5 associated with WISE overdensities: strategy, observations and validation
• Prospects for studying the mass and gas in protoclusters with future CMB observations
• Cosmological parameters from Galaxy Clusters: an Introduction
• Considering light-matter interactions in the Friedmann equations
• Multiple component decomposition from millimeter single-channel data
• The Sunyaev-Zel'dovich effect due to hyper-starburst galaxy winds
• The imprints of galaxy cluster internal dynamics on the Sunyaev-Zeldovich effect
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• kSZ Pairwise Velocity Reconstruction with Machine Learning
• Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations
• VST ATLAS Galaxy Cluster Catalogue I: cluster detection and mass calibration
• Optical Confirmation of X-ray selected Galaxy clusters from the Swift AGN and Cluster survey with MDM and Pan-STARRS Data (Paper III)
• An Optimal and Model-Independent Measurement of the Intracluster Pressure Profile I: Methodology and First Applications
• Cosmological Implications of a Neutrino Mass Detection
• Physical modelling of galaxy clusters and Bayesian inference in astrophysics
• Estimators for the cross-pairwise kSZ effect: forecasts for the dark energy and modified gravity parameters with Simons Observatory and CMB-S4
• Turbulence Induced Non-Gaussian Spectral Distortion in the Microwave Sky from Photon-Axion Conversion in Galaxy Clusters
• HI Intensity Mapping cross-correlation with thermal SZ fluctuations: forecasted cosmological parameters estimation for FAST and Planck
• Galaxy Cluster Science with the Sunyaev-Zel'dovich Effect
• Sunyaev-Zeldovich Cluster Counts as a Probe of Intra-Supercluster Gas
• Simulated differential observations of the Sunyaev-Zel'dovich Effect: Probing the Dark Ages and Epoch of Reionization
• Enabling Discoveries: Thirty Years of Advanced Technologies and Instrumentation at the National Science Foundation
• Increase in the Brightness of the Cosmic Radio Background toward Galaxy Clusters
• Dissecting the Thermal SZ Power Spectrum by Halo Mass and Redshift in SPT-SZ Data and Simulations
• AMiBA: Cluster Sunyaev-Zel'dovich Effect Observations with the Expanded 13-Element Array
• The gas distribution in the high-redshift cluster MS 1054-0321
• Elastic Scattering of Cosmological Gravitational Wave Backgrounds: Primordial Black Holes and Stellar Objects
• Halo detection via large-scale Bayesian inference
• Large Scale Distribution of Galaxies in The Field HS 47.5-22. I. Data Analysis Technique
• The Swift AGN and Cluster Survey. II. Cluster Confirmation with SDSS Data
• Delensing CMB B-modes using galaxy surveys: the effect of galaxy bias and matter clustering non-linearities
• Thermal Sunyaev-Zel'dovich effect at the core of CL J1226.9+3332 revealed by NOEMA
• A halo approach to the evaluation of the cross-correlation between the SZ sky and galaxy survey
• Optimizing Observational Strategy for Future Fgas Constraints
• "SZ spectroscopy" in the coming decade: Galaxy cluster cosmology and astrophysics in the submillimeter
• Intracluster Medium through three years of WMAP
• On the radiative and thermodynamic properties of the cosmic radiations using Cobe Firas instrumental data: Sunyaev-Zeldovich distortion effect
• Fully Relativistic Derivation of the Thermal Sunyaev-Zel'dovich Effect
• AutoEnRichness: A hybrid empirical and analytical approach for estimating the richness of galaxy clusters
• SZ effect or Not? - Detecting most galaxy clusters' main foreground effect
• Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
• A comparative test of different pressure profile models in clusters of galaxies using recent ACT data
• Built-in precision: Improving cluster cosmology through the self-calibration of a galaxy cluster sample
• Modeling Integrated Properties and the Polarization of the Sunyaev-Zeldovich Effect
• Fast Baryonic Field Painting for Sunyaev-Zel'dovich Analyses: Transfer Function vs. Hybrid Effective Field Theory
• Observational tests of the galaxy formation process