The Sunyaev-Zel'dovich Effect

Abstract

The Sunyaev-Zel'dovich effect causes a change in the apparent brightness of the Cosmic Microwave Background Radiation towards a cluster of galaxies or any other reservoir of hot plasma. Measurements of the effect provide distinctly different information about cluster properties than X-ray imaging data, while combining X-ray and Sunyaev-Zel'dovich effect data leads to new insights into the structures of cluster atmospheres. The effect is redshift-independent, and so provides a unique probe of the structure of the Universe on the largest scales. The present review discusses the theory of the Sunyaev-Zel'dovich effect and collects published results for many clusters, presents the overall conclusions that may be drawn from the detections so far, and discusses the prospects for future research on the Sunyaev-Zel'dovich effects.

137 pages, 28 figures. LaTeX (aastex macros) plus encapsulated PostScript. To appear in Physics Reports

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• Constraining the Rotational Kinematic Sunyaev-Zel'dovich Effect in Massive Galaxy Clusters
• AMiBA Wideband Analog Correlator
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• The Mass-Richness Relation of MaxBCG Clusters from Quasar Lensing Magnification using Variability
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• Observations of the Corona Borealis supercluster with the superextended Very Small Array: further constraints on the nature of the non-Gaussian CMB cold spot
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• The Santa Fe Light Cone Simulation Project: II. The Prospects for Direct Detection of the WHIM with SZE Surveys
• The impact of relativistic corrections and component separation in the measurement of the SZ effect and on the small angular scale non-Gaussianity of the CMB
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• The distribution of two-dimensional eccentricity of Sunyaev-Zeldovich Effect and X-ray surface brightness profiles
• Optimizing measurements of cluster velocities and temperatures for CCAT-prime and future surveys
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• Exploring diffuse radio emission in galaxy clusters and groups with the uGMRT and the SKA
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• High angular resolution observation of the Sunyaev-Zel'dovich effect in the massive z=0.83 cluster ClJ0152-1357
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• Probing the cosmic microwave background temperature using the Sunyaev-Zeldovich effect
• Beyond the Standard Lore of the SZ effect
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• A comparison of central temperatures of the intracluster gas determined from X-ray and SZ measurements
• The thermal and non-thermal components within and between galaxy clusters Abell 399 and Abell 401
• Detecting the halo heating from AGN feedback with ALMA
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• The non-thermal emission of extended radio galaxy lobes with curved electron spectra
• Probing the Evolution of Gas Mass Fraction with Sunyaev-Zel'dovich Effect
• SALT spectroscopic observations of galaxy clusters detected by ACT and a Type II quasar hosted by a brightest cluster galaxy
• Millimetric observation of the SZ effect in the Corona Borealis supercluster
• Extraction of cluster parameters with future Sunyaev-Zel'dovich observations
• Preliminary Sunyaev Zel'dovich Observations of Galaxy Clusters with OCRA-p
• Reconstructing three-dimensional parameters of galaxy clusters via multifrequency SZ observations
• Constraining H0 in General Dark Energy Models from Sunyaev-Zeldovich/X-ray Technique and Complementary Probes
• Measurement of the Sunyaev-Zel'dovich Increment in Massive Galaxy Clusters
• Mass and pressure constraints on galaxy clusters from interferometric SZ observations
• Cosmological Parameters 2000
• A parametric physical model for the intracluster medium and its use in joint SZ/X-ray analyses of galaxy clusters
• The Sunyaev-Zeldovich Signal of the maxBCG SDSS Galaxy Clusters in WMAP
• The Morphology of the Thermal Sunyaev-Zel'dovich Sky
• Further Sunyaev-Zel'dovich observations of two Planck ERCSC clusters with the Arcminute Microkelvin Imager
• Primordial magnetic fields with X-ray and S-Z cluster survey
• Modifications to the Cosmic 21-cm Background Frequency Spectrum by Scattering via electrons in Galaxy Clusters
• An Assessment of Contamination in the thermal-SZ Map Using Cross Correlations
• Sunyaev--Zel'dovich profile fitting with joint AMI-Planck analysis
• AMI SZ observations and Bayesian analysis of a sample of six redshift-one clusters of galaxies
• Multi wavelength cross-correlation analysis of the simulated cosmic web
• Systematic Errors in the Hubble Constant Measurement from the Sunyaev-Zel'dovich effect
• Probing gaseous galactic halos through the rotational kSZ effect
• Predicted Constraints on Cosmic String Tension from Planck and Future CMB Polarization Measurements
• On cooling flows and the Sunyaev-Zel'dovich effect
• An Optical Observational Cluster Mass Function at $z\sim 1$ with the ORELSE Survey
• Simulating the galaxy cluster "El Gordo": gas motion, kinetic Sunyaev-Zel'dovich signal, and X-ray line features
• Search for GeV Gamma-Ray Emission from SPT-SZ selected Galaxy Clusters with 15 years of Fermi-LAT data
• Cosmology with the Planck cluster sample
• Statistical Properties of Thermal Sunyaev-Zel'dovich Maps
• Constraints on the Hubble Parameter from galaxy clusters and the Validity of the Cosmic Distance Duality Relation
• Intracluster Entropy from Joint X-ray and Sunyaev-Zel'dovich Observations
• Angular diameter distance estimates from the Sunyaev-Zel'dovich effect in hydrodynamical cluster simulations
• Magnetohydrodynamic relaxation of AGN ejecta: radio bubbles in the intracluster medium
• Probing Hot Gas in Galaxy Groups through the Sunyaev-Zeldovich Effect
• Magnetic Sunyaev-Zel'dovich effect in galaxy clusters
• CARMA follow-up of the northern unconfirmed PLANCK galaxy cluster candidates
• Real space tomography of the primordial Universe with cluster polarization
• Weak lensing mass estimates of galaxy groups and the line-of-sight contamination
• Probing the cluster pressure profile with thermal Sunyaev-Zeldovich effect and weak lensing cross-correlation
• On the Sunyaev-Zel'dovich effect from dark matter annihilation or decay in galaxy clusters
• Using clusters in SZE + x-ray surveys as an ensemble of rulers to constrain cosmology
• Limits on evolution of the fine-structure constant in runaway dilaton models from Sunyaev-Zeldovich Observations
• Studying the leptonic structure of galaxy cluster atmospheres from the spectral properties of the SZ effect
• The failure of testing for cosmic opacity via the distance-duality relation
• On the Detectability of the SZ Effect of Massive Young Galaxies
• The XXL Survey XLIV. Sunyaev-Zel'dovich mapping of a low-mass cluster at z~1: a multi-wavelength approach
• Simultaneous determination of ${\Omega }_{M0}$ and $H_0$ from joint Sunyaev-Zeldovich effect and X-ray observations with median statistics
• Cross-correlating Sunyaev-Zel'dovich and Weak Lensing Maps
• Parameterization Effects in the analysis of AMI Sunyaev-Zel'dovich Observations
• A Multiphase Model for the Intracluster Medium
• Relativistic inverse Compton scattering of photons from the early universe
• A blind detection of a large, complex, Sunyaev--Zel'dovich structure
• Can the splashback radius be an observable boundary of galaxy clusters?
• A joint analysis of AMI and CARMA observations of the recently discovered SZ galaxy cluster system AMI-CL J0300+2613
• MILCANN : A neural network assessed tSZ map for galaxy cluster detection
• An analysis of the temperature structure of galaxy clusters by means of the thermal Sunyaev-Zel'dovich effect
• The Chameleonic Contribution to the SZ Radial Profile of the Coma Cluster
• Imaging Simulations of the Sunyaev-Zel'dovich Effect for ALMA
• Lensed CMB power spectrum biases from masking extragalactic sources
• Simulating SZ intensity maps of giant AGN cocoons
• Uncertainties in the S-Z selected cluster angular power spectrum
• X-ray Clusters of Galaxies as Cosmological Tools
• The Sunyaev-Zeldovich effect in superclusters of galaxies using gasdynamical simulations: the case of Corona Borealis
• SZ observations with AMI of the hottest galaxy clusters detected in the XMM-Newton Cluster Survey
• Fundamental Plane of Sunyaev-Zeldovich clusters
• Probing Cosmology and Galaxy Cluster Structure with the Sunyaev-Zel'dovich Decrement vs. X-ray Temperature Scaling Relation
• Cosmological constraints from a 2D SZ catalog
• Bose-Einstein condensation of photons in microcavity plasmas
• Clarifying the covariant formalism for the SZ effect due to relativistic non-thermal electrons
• Joint signal extraction from galaxy clusters in X-ray and SZ surveys: A matched-filter approach
• Decrease in the Brightness of the Cosmic X-ray and Soft Gamma-ray Background toward Clusters of Galaxies
• A multi-frequency study of the SZE in giant radio galaxies
• A model-independent test of the evolution of gas depletion factor for SPT-SZ and Planck ESZ clusters
• Pairwise kSZ signal extraction efficacy and optical depth estimation
• Constraining Intra-cluster Gas Models with AMiBA13
• A potentially pure test of cosmic geometry: galaxy clusters and the real space Alcock-Paczynski test
• Introducing constrained matched filters for improved separation of point sources from galaxy clusters
• Separating the kinetic SZ effect from primary CMB fluctuations
• Sunyaev-Zel'dovich effect in the Virgo cluster from WMAP and ROSAT data
• Relativistic corrections to the Kompaneets equation
• Inverse-Compton Scattering of the Cosmic Infrared Background
• Determining Distances to Clusters of Galaxies using Resonant X-ray Emission Lines
• Prospects for Detection of Intracluster Gas Bulk Velocities Through the Sunyaev-Zel'dovich Effect
• The kinetic Sunyaev-Zel'dovich tomography II: probing the circumgalactic medium
• Joint analysis of X-ray and Sunyaev Zel'dovich observations of galaxy clusters using an analytic model of the intra-cluster medium
• The Planck SZ Cluster Catalog: Expected X-ray Properties
• CHEX-MATE: pressure profiles of 6 galaxy clusters as seen by SPT and Planck
• Improving Constraints on Inflation with CMB Delensing
• Physical modelling of galaxy clusters using Einasto dark matter profiles
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• Estimating Power Spectrum of Sunyaev-Zeldovich Effect from the Cross-Correlation between WMAP and 2MASS
• Model-Independent Limits on the Line-of-Sight Depth of Clusters of Galaxies Using X-ray and Sunyaev-Zel'dovich Data
• Constraints on structure formation models from Sunyaev-Zel'dovich Effect
• Statistics of the Sunyaev-Zel'dovich Effect power spectrum
• Study on the Solutions of the Sunyaev-Zeldovich Effect for Clusters of Galaxies
• The Atacama Cosmology Telescope: DR6 Power Spectrum Foreground Model and Validation
• Can electron distribution functions be derived through the Sunyaev-Zel'dovich effect?
• Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps
• MIGHTEE-HI: Discovery of an HI-rich galaxy group at z = 0.044 with MeerKAT
• Some astrophysical implications of dark matter and gas profiles in a new galaxy clusters model
• Characterizing galaxy clusters by their gravitational potential: systematics of cluster potential reconstruction
• Camouflaged galactic CMB foregrounds: total and polarized contributions of the kinetic Sunyaev Zeldovich effect
• The Sunyaev-Zel'dovich Effect: Results and Future Prospects
• A Diffused Background from Axion-like Particles in the Microwave Sky
• Determination of cosmological parameters: an introduction for non-specialists
• The rotational kinetic Sunyaev-Zeldovich contribution to the temperature asymmetry toward the M31 halo
• Galaxy clusters as probes for cosmology and dark matter
• Inverse Compton cooling of thermal plasma in colliding-wind binaries
• Redshift evolution of the 1.4 GHz volume averaged radio luminosity function in clusters of galaxies
• Probing photon decay with the Sunyaev-Zel'dovich effect
• Narrow Band X-ray Photometry as a Tool for Studying Galaxy and Cluster Mass Distributions
• Cosmological Implications of the BIMA 30 Ghz Sunyaev-Zel'dovich Effect Galaxy Cluster Survey
• New constraints on H_0 and Omega_M from SZE/X-RAY data and Baryon Acoustic Oscillations
• Mapping the temperature of the intra-cluster medium with the tSZ effect
• Constraints on the Sunyaev-Zel'dovich signal from the Warm Hot Intergalactic Medium from WMAP and SPT data
• The effect of bandpass uncertainties on component separation
• Dark matter annihilation and non-thermal Sunyaev-Zel'dovich effect: I. galaxy cluster
• Analytical studies on the Sunyaev Zeldovich effect in the cluster of galaxies for three Lorentz frames
• Polarization of the Sunyaev-Zel'dovich effect: relativistic imprint of thermal and non-thermal plasma
• Importance of intracluster scattering and relativistic corrections from tSZ effect with Cosmic Infrared Background
• Spectral imaging of the thermal Sunyaev-Zel'dovich effect in X-COP galaxy clusters: method and validation
• Milestones of general relativity: Hubble's law (1929) and the expansion of the universe
• Probing galaxy cluster and intra-cluster gas with luminous red galaxies
• The Effects of Relativistic Corrections on Cosmological Parameter Estimations from SZE Cluster Surveys
• Intracluster gas pressure, entropy injection and redshift evolution
• Magnetic fields and Sunyaev-Zel'dovich effect in galaxy clusters
• Identification of galaxy clusters in cosmic microwave background maps using the Sunyaev-Zel'dovich effect
• CMB Shadows: The Effect of Interstellar Extinction on Cosmic Microwave Background Polarization and Temperature Anisotropy
• Non-thermal Sunyaev-Zeldovich signal from radio galaxy lobes
• The impact of non-Planckian effects on cosmological radio backgrounds
• A Simple Gravitational Lens Model For Cosmic Voids
• Contamination of the Central Sunyaev--Zel'dovich Decrements in AMiBA Galaxy Cluster Observations
• The XXL Survey LI. Pressure profile and $Y_{\mathrm{SZ}}$-$M$ scaling relation in three low-mass galaxy clusters at $z\sim 1$ observed with NIKA2
• Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect
• A study of the galaxy redshift distribution toward the cosmic microwave background cold spot in the Corona Borealis supercluster
• PITSZI: Probing Intra-cluster medium Turbulence with Sunyaev-Zel'dovich Imaging -- Application to the triple merging cluster MACS J0717.5+3745
• The Hubble constant from galaxy cluster scaling-relation and SNe Ia observations: a consistency test
• Abell 370: A Cluster with a Pronounced Triaxial Morphology
• A Direct Method for Measuring Heat Conductivity in Intracluster Medium
• Simulation of a Combined SZE and Weak Lensing Cluster Survey for AMiBA Experiment
• Redshift estimation of clusters by wavelet decomposition of their Sunyaev-Zel'dovich morphology
• The correlation of high-redshift galaxies with the thermal Sunyaev-Zel'dovich effect traces reionization
• Constraining the optical depth of galaxies and velocity bias with cross-correlation between kinetic Sunyaev-Zeldovich effect and peculiar velocity field
• Unveiling the 3D temperature structure of galaxy clusters by means of the thermal SZ effect
• Using Galaxy Cluster Peculiar Velocities to Constrain Cosmological Parameters
• 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
• The Thermal Sunyaev-Zeldovich Effect of Primordial Recombination Radiation
• Observing the Epoch of Reionization with the Cosmic Microwave Background
• Limits on Hot Intracluster Gas Contributions to the Tenerife Temperature Anisotropy Map
• Search for the Sunyaev-Zel'dovich Effect in a Giant Radio Galaxy B1358+305
• The Atacama Cosmology Telescope: SZ-based masses and dust emission from IR-selected cluster candidates in the SHELA survey
• On a possible cosmological evolution of galaxy cluster $Y_{\mathrm{X}}-Y_{\mathrm{SZE}}$ scaling relation
• A high-frequency study of the Sunyaev-Zel'dovich effect morphology in galaxy clusters
• Hydrodynamical chemistry simulations of the SZ effect and the impacts from primordial non-Gaussianities
• Galaxy clusters, cosmic chronometers and the Einstein equivalence principle
• Empirical test for relativistic kinetic theories based on the Sunyaev-Zel'dovich effect
• A Search for CMB Decrements Towards Distant Cluster Candidates PC1643+4631 and VLA1312+4237 at 28.5 GHz
• Analytical studies on the Sunyaev-Zeldovich effect in the cluster of galaxies for three Lorentz frames II: single integral formula
• Reconstruction of Gas Temperature and Density Profiles of the Galaxy Cluster RX J1347.5-1145
• Kinetic inductance detectors for millimeter and submillimeter astronomy / Détecteurs à inductance cinétique pour l'astronomie millimétrique et sub-millimétrique
• On the Number Density of Sunyaev-Zel'dovich Clusters of Galaxies
• Probing the Cosmic Distance Duality Relation via Non-Parametric Reconstruction for High Redshifts
• Probing the physics and history of cosmic reionization with the Sunyaev-Zel'dovich Effect
• Analytical Study on the Sunyaev-Zeldovich Effect for Clusters of Galaxies. II. comparison of covariant formalisms
• The Standard Model, Dark Matter, and Dark Energy: From the Sublime to the Ridiculous
• An integrated Sachs-Wolfe effect vs redshift test for the cosmological parameters
• Linearized Kompaneetz equation as a relativistic diffusion
• The Herschel-SPIRE Legacy Survey (HSLS): the scientific goals of a shallow and wide submillimeter imaging survey with SPIRE
• kSZ Pairwise Velocity Reconstruction with Machine Learning
• Simulations of cm-wavelength Sunyaev-Zel'dovich galaxy cluster and point source blind sky surveys and predictions for the RT32/OCRA-f and the Hevelius 100-m radio telescope
• An SZ-Like Effect on Cosmological Gravitational Wave Backgrounds
• The imprints of galaxy cluster internal dynamics on the Sunyaev-Zeldovich effect
• SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
• Statistical evaluation of the observational information on ${\Omega }_m$ and ${\Omega }_{\Lambda }$
• A structure factor approach to the Sunyaev-Zel'dovich effect
• Gamma-ray detection toward the Coma cluster with Fermi-LAT: Implications for the cosmic ray content in the hadronic scenario
• Sensitivity and Insensitivity of Galaxy Cluster Surveys to New Physics
• Embedded Lensing Time Delays, the Fermat Potential, and the Integrated Sachs-Wolfe Effect
• Considering light-matter interactions in the Friedmann equations
• Cosmological constraints from Sunyaev-Zeldovich cluster counts: an approach to account for missing redshifts
• Simulations and Observations of the Microwave Universe
• Physical modelling of galaxy clusters and Bayesian inference in astrophysics
• Turbulence Induced Non-Gaussian Spectral Distortion in the Microwave Sky from Photon-Axion Conversion in Galaxy Clusters
• On a Boltzmann equation for Compton scattering, from non relativistic electrons at low density
• SZ effects from annihilating dark matter in the Milky Way: smooth halo, subhalos and intermediate-mass-black-holes
• A Stacked Analysis of GeV Gamma-Ray Emission from SPT-SZ Galaxy Clusters with 16 Years of Fermi-LAT Data
• An Optimal and Model-Independent Measurement of the Intracluster Pressure Profile I: Methodology and First Applications
• Cosmic backgrounds from the radio to the far-infrared: recent results and perspectives from cosmological and astrophysical surveys
• Extracting cosmological signals from foregrounds in deep mm maps of the sky
• Galaxy Cluster Science with the Sunyaev-Zel'dovich Effect
• A Semi-Parametric Approach to Fitting Gas Pressure Profiles of Galaxy Clusters
• An approach for the detection of point-sources in very high resolution microwave maps
• Effect of the non-thermal Sunyaev-Zel'dovich Effect on the temperature determination of galaxy clusters
• The gas distribution in the high-redshift cluster MS 1054-0321
• AMiBA: Cluster Sunyaev-Zel'dovich Effect Observations with the Expanded 13-Element Array
• Simulated differential observations of the Sunyaev-Zel'dovich Effect: Probing the Dark Ages and Epoch of Reionization
• High frequency radio imaging of 3CR 403.1 with the Sardinia Radio Telescope
• Increase in the Brightness of the Cosmic Radio Background toward Galaxy Clusters
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• Measuring the baryon fraction in cluster of galaxies with Kinematic Sunyaev Zeldovich and a Standard Candle
• The thermodynamic structure and large-scale structure filament in MACS J0717.5+3745
• Analysing the Effect on CMB in a Parity and Charge Parity Violating Varying Alpha Theory
• Fast Baryonic Field Painting for Sunyaev-Zel'dovich Analyses: Transfer Function vs. Hybrid Effective Field Theory
• Sunyaev-Zel'dovich Effect Observations of the Bullet Cluster (1E 0657-56) with APEX-SZ
• Supervised Extraction of the Thermal Sunyaev$-$Zel'dovich Effect with a Three-Dimensional Convolutional Neural Network
• A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
• On the radiative and thermodynamic properties of the cosmic radiations using Cobe Firas instrumental data: Sunyaev-Zeldovich distortion effect
• A comparative test of different pressure profile models in clusters of galaxies using recent ACT data
• Shadows of Giants: Constraints on Stupendously Large Black Holes from Negative Sources against the Cosmic Microwave Background
• Optimizing Observational Strategy for Future Fgas Constraints
• "SZ spectroscopy" in the coming decade: Galaxy cluster cosmology and astrophysics in the submillimeter
• Sunyaev-Zel'dovich Effect by Multiple Sctattering : Numerical Solution of the Transfer Equations