Formation of Galaxy Clusters

Abstract

In this review, we describe our current understanding of cluster formation: from the general picture of collapse from initial density fluctuations in an expanding Universe to detailed simulations of cluster formation including the effects of galaxy formation. We outline both the areas in which highly accurate predictions of theoretical models can be obtained and areas where predictions are uncertain due to uncertain physics of galaxy formation and feedback. The former includes the description of the structural properties of the dark matter halos hosting cluster, their mass function and clustering properties. Their study provides a foundation for cosmological applications of clusters and for testing the fundamental assumptions of the standard model of structure formation. The latter includes the description of the total gas and stellar fractions, the thermodynamical and non-thermal processes in the intracluster plasma. Their study serves as a testing ground for galaxy formation models and plasma physics. In this context, we identify a suitable radial range where the observed thermal properties of the intra-cluster plasma exhibit the most regular behavior and thus can be used to define robust observational proxies for the total cluster mass. We put particular emphasis on examining assumptions and limitations of the widely used self-similar model of clusters. Finally, we discuss the formation of clusters in non-standard cosmological models, such as non-Gaussian models for the initial density field and models with modified gravity, along with prospects for testing these alternative scenarios with large cluster surveys in the near future.

66 pages, 17 figures, review to be published in 2012 Annual Reviews of Astronomy & Astrophysics

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• N-Body Simulations of DGP and Degravitation Theories
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• Signature of Primordial Non-Gaussianity on Matter Power Spectrum
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• A generalized local ansatz and its effect on halo bias
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• The impact of gas physics on strong cluster lensing
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• The Effect of Gas Physics on the Halo Mass Function
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• Reconstructing mass profiles of simulated galaxy clusters by combining Sunyaev-Zeldovich and X-ray images
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• Evidence for the Universality of Properties of Red-Sequence Galaxies in X-ray- and Red-Sequence-Selected Clusters at z ~ 1
• Towards mapping turbulence in the intra-cluster medium -- II. Measurement uncertainties in the estimation of structure functions
• Simulations of the Galaxy Cluster CIZA J2242.8+5301 I: Thermal Model and Shock Properties
• Scatter in Sunyaev--Zel'dovich effect scaling relations explained by inter-cluster variance in mass accretion histories
• The Gravitational Instability of Adiabatic Filaments
• Weak lensing clusters from HSC survey first-year data: Mitigating the dilution effect of foreground and cluster member galaxies
• A Massive Cluster at z = 0.288 Caught in the Process of Formation: The Case of Abell 959
• Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters
• AGN Feedback in Groups and Clusters of Galaxies
• How Much Can We Learn From A Merging Cold Front Cluster? : Insights From X-ray Temperature and Radio Maps of Abell 3667
• The Three Hundred project: A Machine Learning method to infer clusters of galaxies mass radial profiles from mock Sunyaev-Zel'dovich maps
• The Astrophysics of the Intracluster Plasma
• The role of the artificial conductivity in SPH simulations of galaxy clusters: effects on the ICM properties
• eROSITA cluster cosmology forecasts: cluster temperature substructure bias
• Ultraviolet Signatures of the Multiphase Intracluster and Circumgalactic Media in the RomulusC Simulation
• S-PLUS DR1 galaxy clusters and groups catalogue using PzWav
• Warm Gas in and Around Simulated Galaxy Clusters as Probed by Absorption Lines
• Cosmology with galaxy cluster weak lensing: statistical limits and experimental design
• Chandra Observations of the Planck ESZ Sample: A Re-Examination of Masses and Mass Proxies
• Evolution of Splashback Boundaries and Gaseous Outskirts: Insights from Mergers of Self-similar Galaxy Clusters
• The XXL Survey: XXIII. The Mass Scale of XXL Clusters from Ensemble Spectroscopy
• Constraining the Rotational Kinematic Sunyaev-Zel'dovich Effect in Massive Galaxy Clusters
• X-ray surface brightness and gas density profiles of galaxy clusters up to 3*R500c with SRG/eROSITA
• Studying the late evolution of a radio-loud AGN in a galaxy group with LOFAR
• Galaxy cluster luminosities and colours, and their dependence on cluster mass and merger state
• Stirred, not Clumped: Evolution of Temperature Profiles in the Outskirts of Galaxy Clusters
• A Baryonic Effect on the Merger Timescale of Galaxy Clusters
• MINOT: Modeling the intracluster medium (non-)thermal content and observable prediction tools
• Comparing different mass estimators for a large subsample of the {\it Planck}-ESZ clusters
• Photon-ALP oscillations inducing modifications to photon polarization
• Thermodynamic evolution of the $z=1.75$ galaxy cluster IDCS J1426.5+3508
• SPT-CL J2032-5627: a new Southern double relic cluster observed with ASKAP
• Cluster cosmology with anisotropic boosts: Validation of a novel forward modeling analysis and application on SDSS redMaPPer clusters
• Fast and realistic large-scale structure from machine-learning-augmented random field simulations
• The History of Metal Enrichment Traced by X-ray Observations of High Redshift Galaxy Clusters
• Groups and protocluster candidates in the CLAUDS and HSC-SSP joint deep surveys
• X-ray Observations of Complex Temperature Structure in the Cool-core cluster Abell 85
• On Mass Concentrations & Magnitude Gaps of Galaxy Systems in the CS82 Survey
• Low X-ray Luminosity Galaxy Clusters. III: Weak Lensing Mass Determination at 0.18 $<$ z $<$ 0.70
• Simulation view of galaxy clusters with low X-ray surface brightness
• Some observational tests of a minimal galaxy formation model
• Spatial Distribution of Metals in the ICM: Evolution of the Iron Excess in Relaxed Galaxy Clusters
• The Three Hundred Project: the evolution of physical baryon profiles
• A High-Caliber View of the Bullet Cluster Through JWST Strong and Weak Lensing Analyses
• Shattering and growth of cold clouds in galaxy clusters: the role of radiative cooling, magnetic fields and thermal conduction
• AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
• Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z=3.95
• Building a Better Understanding of the High Redshift BOSS Galaxies as Tools for Cosmology
• The XXL Survey X: K-band luminosity - weak-lensing mass relation for groups and clusters of galaxies
• A Redshift Survey of the Nearby Galaxy Cluster Abell 2199: Comparison of the Spatial and Kinematic Distributions of Galaxies with the Intracluster Medium
• A Newly-Discovered Radio Halo in Merging Cluster MACS J2243.3-0935
• A heuristic wave equation parameterizing BEC dark matter halos with a quantum core and an isothermal atmosphere
• Multi-wavelength mock observations of the WHIM in a simulated galaxy cluster
• The XMM Cluster Survey analysis of the SDSS DR8 redMaPPer Catalogue: Implications for scatter, selection bias, and isotropy in cluster scaling relations
• Simulating the LOcal Web (SLOW) II: Properties of local galaxy clusters
• Hydrodynamical simulations of coupled and uncoupled quintessence models II: Galaxy clusters
• Planck/SDSS Cluster Mass and Gas Scaling Relations for a Volume-Complete redMaPPer Sample
• The Differing Relationships Between Size, Mass, Metallicity and Core Velocity Dispersion of Central and Satellite Galaxies
• A Simple Physical Model for the Gas Distribution in Galaxy Clusters
• The Cluster-EAGLE project: a comparison of dynamical mass estimators using simulated clusters
• Multi-probe analysis of the galaxy cluster CL J1226.9+3332: Hydrostatic mass and hydrostatic-to-lensing bias
• The Manhattan Suite: Accelerated galaxy evolution in the early Universe
• A Spectacular Bow Shock in the 11 keV Galaxy Cluster Around 3C 438
• On the choice of the most suitable indicator for the assembly state of dark matter haloes through cosmic time
• 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${}_{\odot }$
• Detection of spatial clustering in the 1000 richest SDSS DR8 redMaPPer clusters with Nearest Neighbor distributions
• A Chandra Study of Radial Temperature Profiles of the Intra-Cluster Medium in 50 Galaxy Clusters
• XRISM Observation of the Ophiuchus Galaxy Cluster: Quiescent Velocity Structure in the Dynamically Disturbed Core
• Impact of substructure on local dark matter searches
• Reconsidering the dynamical states of galaxy clusters using PCA and UMAP
• Non-virialised clusters for detection of Dark Energy-Dark Matter interaction
• Unveiling the internal structure of Hercules supercluster
• Synthesizing Stellar Populations in South Pole Telescope Galaxy Clusters: I. Ages of Quiescent Member Galaxies at 0.3 < z < 1.4
• Chandra and optical/IR observations of CXOJ1415.2+3610, a massive, newly discovered galaxy cluster at z~1.5
• On the complexity and the information content of cosmic structures
• Galaxy clusters and structure formation in quintessence versus phantom dark energy universe
• K-CLASH: Strangulation and Ram Pressure Stripping in Galaxy Cluster Members at 0.3 < z < 0.6
• The Massive and Distant Clusters of WISE Survey VI: Stellar Mass Fractions of a Sample of High-Redshift Infrared-selected Clusters
• Low redshift calibration of the Amati relation using galaxy clusters
• Can AGN and galaxy clusters explain the surface brightness fluctuations of the cosmic X-ray background?
• Measuring the surface mass density ellipticity of redMaPPer galaxy clusters using weak-lensing
• Baryonic Imprints on DM Halos: The concentration-mass relation in the CAMELS simulations
• ${\mu }_{\star }$ Masses: Weak Lensing Calibration of the Dark Energy Survey Year 1 redMaPPer Clusters using Stellar Masses
• Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption
• Mass-Velocity Dispersion Relation in HIFLUGCS Galaxy Clusters
• Detection of anisotropic satellite quenching in galaxy clusters up to $z\sim 1$
• Pairs of Giant Shock Waves (N-Waves) in Merging Galaxy Clusters
• Starbursts with suppressed velocity dispersion revealed in a forming cluster at z=2.51
• The Observable Thermal and Kinetic Sunyaev-Zel'dovich Effect in Merging Galaxy Clusters
• The XMM Cluster Survey: evolution of the velocity dispersion -- temperature relation over half a Hubble time
• Search for GeV Gamma-Ray Emission from SPT-SZ selected Galaxy Clusters with 15 years of Fermi-LAT data
• Probing dark energy via galaxy cluster outskirts
• Halo Scaling Relations and Hydrostatic Mass Bias in the Simba Simulation From Realistic Mock X-ray Catalogues
• CHEX-MATE: CLUster Multi-Probes in Three Dimensions (CLUMP-3D), I. Gas Analysis Method using X-ray and Sunyaev-Zel'dovich Effect Data
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
• The eROSITA Final Equatorial-Depth Survey (eFEDS) -- Splashback radius of X-ray galaxy clusters using galaxies from HSC survey
• Abell 315: reconciling cluster mass estimates from kinematics, X-ray, and lensing
• Galaxy cluster outskirts: a universal entropy profile for relaxed clusters?
• Precision cosmology with baryons: non-radiative hydrodynamics of galaxy groups
• The binding of cosmological structures by massless topological defects
• Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope
• A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
• Emulating Sunyaev-Zeldovich Images of Galaxy Clusters using Auto-Encoders
• A new method to search for high redshift clusters using photometric redshifts
• What can the spatial distribution of galaxy clusters tell about their scaling relations?
• The abundance and colours of galaxies in high redshift clusters in the cold dark matter cosmology
• The Circumgalactic Medium in Massive Halos
• On the weak lensing masses of a new sample of galaxy groups
• Probing Saraswati's heart: evaluating the dynamical state of the massive galaxy cluster A2631 through a comprehensive weak-lensing and dynamical analysis
• Faraday Rotation Measure Dependence on Galaxy Clusters Dynamics
• The Galaxy Cluster 'Pypeline' for X-ray Temperature Maps: ClusterPyXT
• Cosmological interpretation of the color-magnitude diagrams of galaxy clusters
• Average Dark Matter Halo Sparsity Relations as Consistency Check of Mass Estimates in Galaxy Cluster Samples
• Can the splashback radius be an observable boundary of galaxy clusters?
• An Optical Analysis of the Merging Cluster Abell 3888
• SZ Scaling Relations of Galaxy Groups and Clusters Near the North Ecliptic Pole
• On Escaping a Galaxy Cluster in an Accelerating Universe
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• Environmental dependence of X-ray and optical properties of galaxy clusters
• On the phase-space structure of galaxy clusters from cosmological simulations
• Constraining the Milky Way Mass with Its Hot Gaseous Halo
• An exploration of the properties of cluster profiles for the thermal and kinetic Sunyaev-Zel'dovich effects
• The Entire Virial Radius of the Fossil Cluster RXJ1159+5531: II. Dark Matter and Baryon Fraction
• Revisiting GeV-scale annihilating dark matter with the AMS-02 positron fraction
• Off-centre supermassive black holes in bright central galaxies
• Cross Correlation of the Extragalactic Gamma-ray Background with Thermal Sunyaev-Zel'dovich Effect in the Cosmic Microwave Background
• Suzaku Measurements of Hot Halo Emission at Outskirts for Two Poor Galaxy Groups: NGC 3402 and NGC 5129
• Cosmology with Galaxy Cluster Properties using Machine Learning
• Compact Groups analysis using weak gravitational lensing II: CFHT Stripe 82 data
• Galaxy cluster hydrostatic masses using Tolman-Oppenheimer-Volkoff equation
• Suzaku Observations of Low Surface Brightness Cluster Abell 1631
• The effect of pressure-anisotropy-driven kinetic instabilities on magnetic field amplification in galaxy clusters
• Prospects for $\gamma$-ray observations of the Perseus galaxy cluster with the Cherenkov Telescope Array
• Nonthermal Pressure in the Outskirts of Abell 2142
• Miscentering of Optical Galaxy Clusters Based on Sunyaev-Zeldovich Counterparts
• The Merger Dynamics of the Galaxy Cluster Abell 1775: New Insights from Chandra and XMM-Newton for a Cluster Simultaneously Hosting a WAT and a NAT Radio Sources
• Studying the ICM in clusters of galaxies via surface brightness fluctuations of the cosmic X-ray background
• CHEX-MATE: pressure profiles of 6 galaxy clusters as seen by SPT and Planck
• SZ/X-ray scaling relations using X-ray data and Planck Nominal maps
• Turbulent Pressure Support in Galaxy Clusters -- Impact of the Hydrodynamical Solver
• The Three Hundred project: Estimating the dependence of gas filaments on the mass of galaxy clusters
• Optical and X-ray profiles in the REXCESS sample of galaxy clusters
• Deriving galaxy cluster velocity anisotropy profiles from a joint analysis of dynamical and weak lensing data
• Testing generalized scalar-tensor theories of gravity with clusters of galaxies
• Extreme circumgalactic HI and CIII absorption around the most massive, quenched galaxies
• The Hercules cluster in X-rays with $XMM$-$Newton$ and $Chandra$
• CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation
• The effect of dynamical states on galaxy clusters populations. I. Classification of dynamical states
• Identification of 4876 Bent-Tail Radio Galaxies in the FIRST Survey Using Deep Learning Combined with Visual Inspection
• Constraints on dark energy from the CSST galaxy clusters
• Magnetic dynamos in galaxy clusters: the crucial role of galaxy formation physics at high redshifts
• Haloes at the ragged edge: The importance of the splashback radius
• Testing the rotation versus merger scenario in the galaxy cluster Abell 2107
• Scatter in the satellite galaxy SHMR: fitting functions, scaling relations & physical processes from the IllustrisTNG simulation
• Studying galaxy cluster morphological metrics with Mock-X
• IllustrisTNG Snapshots for 10 Gyr of Dynamical Evolution of Brightest Cluster Galaxies and Their Host Clusters
• The effect of AGN feedback on the X-ray morphologies of clusters -- simulations vs. observations
• Dynamical analysis of the cluster pair: A3407 + A3408
• Galaxy populations in protoclusters at cosmic noon
• The XMM Cluster Survey: Exploring scaling relations and completeness of the Dark Energy Survey Year 3 redMaPPer cluster catalogue
• From "universal" profiles to "universal" scaling laws in X-ray galaxy clusters
• X-ray cluster cosmology
• Morphology, color-magnitude and scaling relations of galaxies in Abell 426
• BUFFALO Wild Wings: A High Precision Free-Form Lens Model of MACSJ0416 with Constraints on Dark Matter from Substructure and Highly Magnified Arcs
• Deep learning insights into non-universality in the halo mass function
• The Three Hundred Project: Mapping The Matter Distribution in Galaxy Clusters Via Deep Learning from Multiview Simulated Observations
• relensing: Reconstructing the mass profile of galaxy clusters from gravitational lensing
• COSMOS-Web galaxy groups: Evolution of red sequence and quiescent galaxy fraction
• Searching for cold gas traced by MgII quasar absorbers in massive X-ray-selected galaxy clusters
• Degradation analysis in the estimation of photometric redshifts from non-representative training sets
• Dissociation of dark matter and gas in cosmic large-scale structure
• Galaxy pairs in The Three Hundred simulations: a study on the performance of observational pair-finding techniques
• Comparison of hydrostatic and lensing cluster mass estimates:a pilot study in MACS J0647.7+7015
• How complex is the cosmic web?
• The Swift X-ray Telescope Cluster Survey II. X-ray spectral analysis
• Weak Lensing analysis of Abell 2390 using short exposures
• 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
• Growth and disruption in the Lyra complex
• PITSZI: Probing Intra-cluster medium Turbulence with Sunyaev-Zel'dovich Imaging -- Application to the triple merging cluster MACS J0717.5+3745
• Cosmic accretion shocks as a tool to measure the dark matter mass of galaxy clusters
• Search for Dark Matter Annihilation to gamma-rays from SPT-SZ selected Galaxy Clusters
• Resilience of Sloshing Cold Fronts against Subsequent Minor Mergers
• The Rotational Profiles of Cluster Galaxies
• Interplay of periodic dynamics and noise: insights from a simple adaptive system
• Chandra view of Abell 407: the central compact group of galaxies and the interaction between the radio AGN and the ICM
• A pilot search for MeV gamma-ray emission from five galaxy clusters using archival COMPTEL data
• Identifying Galaxy Cluster Mergers with Deep Neural Networks using Idealized Compton-y and X-ray maps
• Protoclusters at z=5.7: A view from the MultiDark galaxies
• Dynamics of the galactic component of Abell S1063 and MACS J1206.2$-$0847
• Galaxy pairs in The Three Hundred simulations II: studying bound ones and identifying them via machine learning
• Clash of Titans: The Impact of Cluster Mergers in the Galaxy Cluster Red Sequence
• A Machine Learning Approach to Enhancing eROSITA Observations
• Intrinsic mass-richness relation of clusters from THE THREE HUNDRED hydrodynamic simulations
• Galaxy cluster virial quantities from extrapolating strong lensing mass profiles
• Effect of Priomordial non-Gaussianities on Galaxy Clusters Scaling Relations
• Joint cluster reconstructions: Combining free-form lensing and X-rays
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• The eventful life journey of galaxy clusters. I. Impact of DM halo and ICM properties on their full assembly histories
• Constraining the average magnetic field in galaxy clusters with current and upcoming CMB surveys
• Evolution of X-ray galaxy Cluster Properties in a Representative Sample (EXCPReS). Optimal binning for temperature profile extraction
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
• SuperModel Analysis of Abell 1246 and J255: on the Evolution of Galaxy Clusters from High to Low Entropy States
• C2-GaMe: Classification of Cluster Galaxy Membership with Machine Learning
• A Dynamically Driven, Universal Thermal Profile of Galaxy Groups and Clusters
• CHEX-MATE: Multi-probe analysis of Abell 1689
• The SRG/eROSITA All-Sky Survey. The Weak-Lensing Mass Calibration and the Stellar Mass-to-Halo Mass Relation from the Hyper Suprime-Cam Subaru Strategic Program
• Millimeter-wave observations of Euclid Deep Field South using the South Pole Telescope: A data release of temperature maps and catalogs
• Density Fluctuations in the Intracluster Medium: An Attempt to Constrain Viscosity with Cosmological Simulations
• Simulation-based marginal likelihood for cluster strong lensing cosmology
• Deep Chandra observations of PLCKG287.0+32.9: a clear detection of a shock front in a heated former cool core
• Search for GeV gamma-ray emission from SPT-CL J2012-5649 with six years of DAMPE data
• Average energy of the X-ray spectrum as a model-independent proxy for the mass of galaxy clusters
• The non-Gaussian distribution of galaxies gravitational fields
• Galaxy cluster hydrostatic bias in Kottler spacetime
• Stellar mass measurements in Abell 133 with Magellan / IMACS
• Turbulence in Simulated Local Cluster Analogs: One-to-one comparisons between SLOW and XRISM/Hitomi
• SLICE: SPT-CL J0546-5345 -- A prominent strong-lensing cluster at $z=1.07$
• Chandra observations of the Abell S0295 cluster
• The Correlation Function and Detection of Baryon Acoustic Oscillation Peak from the Spectroscopic SDSS GalWCat Galaxy Cluster Catalogue
• Results from the SuperModel Analysis of the X-COP Galaxy Clusters Sample
• Improving Galaxy Cluster Selection with the Outskirt Stellar Mass of Galaxies
• Boosting the evolutionary picture of Cl 0024+17 and MS 0451-03: A case study at intermediate-redshift
• Hydrostatic mass of galaxy clusters within some theories of gravity
• The Three Hundred Project: deducing the stellar splashback structure of galaxy clusters from their orbiting profiles
• Testing Cotton gravity as dark matter substitute with weak lensing
• An empirical method for mitigating an excess up-scattering mass bias on the weak lensing mass estimates for shear-selected cluster samples
• GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
• Synthetic Galaxy Clusters and Observations Based on Dark Energy Survey Year 3 Data
• Splashback radius and the mass accretion rate of RASS MCMF galaxy clusters
• VST ATLAS Galaxy Cluster Catalogue I: cluster detection and mass calibration
• The Intracluster Light of Abell 3667: Unveiling an Optical Bridge in LSST Precursor Data
• Mock X-ray observations of hot gas with L-Galaxies semi-analytic models of galaxy formation
• On the Robustness of Cluster Clustering Covariance Calibration
• The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
• Imaging-spectroscopy diagnosis of the giant sloshing spiral in the Virgo cluster with the Einstein Probe Follow-up X-ray Telescope
• A test of galaxy cluster fundamental plane for the X-COP sample
• Star formation activity in a young galaxy cluster at z=0.866
• The Intragroup versus the Intracluster Medium
• On the Alignment of Galaxies in Clusters
• Observations of compact sources in galaxy clusters using MUSTANG2
• The Complexity and Information Content of Simulated Universes
• On the Origin of Intracluster Light based on the High-resolution Simulation, NewCluster
• The environment of QSO triplets at 1 $\lesssim$ z $\lesssim$ 1.5
• Bright [CII]158$\mu$m Streamers as a Beacon for Giant Galaxy Formation in SPT2349$-$56 at $z=4.3$
• Z-Sequence: Photometric redshift predictions for galaxy clusters with sequential random k-nearest neighbours
• Galaxy Cluster Mass Estimation Through The Splashback Radius
• Confirmation of NIKA2 investigation of the Sunyaev-Zel'dovich effect by using synthetic clusters of galaxies
• Optical Confirmation of X-ray selected Galaxy clusters from the Swift AGN and Cluster survey with MDM and Pan-STARRS Data (Paper III)
• A Stacked Analysis of GeV Gamma-Ray Emission from SPT-SZ Galaxy Clusters with 16 Years of Fermi-LAT Data
• Statistical analysis of bound companions in the Coma cluster
• Cluster Formation and Relaxation in Particle Rafts under Uniform Radial Expansion
• Exploiting the high-resolution NIKA2 data to study the intracluster medium and dynamical state of ACT-CL J0240.0+0116
• Comparison of $\Lambda$CDM and $R_h=ct$ with updated galaxy cluster $f_{gas}$ measurements using Bayesian inference
• An Optimal and Model-Independent Measurement of the Intracluster Pressure Profile I: Methodology and First Applications
• Chandra and XMM-Newton observations of the merging cluster of galaxies PLCK G036.7+14.9
• Observing gravitational redshift with X-Ray emission in galaxy clusters with Athena X-IFU
• A test of linearity of the ratio of dark matter to baryonic matter in galaxy clusters
• Spectroscopic Confirmation of Two X-ray Diffuse and Massive Galaxy Clusters at Low Redshift
• Euclid preparation. L. Calibration of the linear halo bias in $\Lambda (\nu )$CDM cosmologies
• Selecting Clusters and Protoclusters via Stellar Mass Density: I. Method and tests on Mock HSC-SSP catalogs
• The ${\mathrm{Y}}_{\mathrm{SZ},\mathrm{Planck}}-{\mathrm{Y}}_{\mathrm{SZ},\mathrm{XMM}}$ scaling relation and its difference between cool-core and non-cool-core clusters
• Inference of morphology and dynamical state of nearby $Planck$-SZ galaxy clusters with Zernike polynomials
• Intracluster globular clusters as tracers of the mass assembly of the Hydra I galaxy cluster
• Halo detection via large-scale Bayesian inference
• DUCA: Dynamic Universe Cosmological Analysis. I. The halo mass function in dynamical dark energy cosmologies
• An X-ray-Emitting Proto-Cluster at $z\approx 5.7$ Reveals Rapid Structure Growth
• Radio Halo Detection in MWA Data using Deep Neural Networks and Generative Data Augmentation
• Dark Energy Survey Year 3 Results: Mis-centering calibration and X-ray-richness scaling relations in redMaPPer clusters
• X-ray flux -- mass relation for $z\gtrsim 0.7$ galaxy clusters
• A Model For Intergalactic Filaments and Galaxy Formation During the First Gigayear
• Euclid: Exploring observational systematics in cluster cosmology -- a comprehensive analysis of cluster counts and clustering
• Merger of massive galaxy cluster CL0238.3+2005 at z~0.4: just after pericenter passage?
• Deriving accurate galaxy cluster masses using X-ray thermodynamic profiles and graph neural networks
• MIGHTEE: The dark matter haloes, duty cycle and mechanical feedback from radio-AGN up to $z\sim 2.5$
• The Swift AGN and Cluster Survey. II. Cluster Confirmation with SDSS Data
• Robustness of Neural Ratio and Posterior Estimators to Distributional Shifts for Population-Level Dark Matter Analysis in Strong Gravitational Lensing
• Impact of a Rapid Diluted Energy Density on the halo mass function
• X-ray analysis of the Planck-detected triplet-cluster system PLCK G334.8-38
• Dissecting the Strong-lensing Galaxy Cluster MS 0440.5+0204. I. The Mass Density Profile
• Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium
• ComPACT: ACT+Planck galaxy cluster catalogue
• VENUS: Strong-lensing model of MACS J1931.8-2635 -- revealing the farthest multiply imaged supernova
• Towards an optimal extraction of cosmological parameters from galaxy cluster surveys using convolutional neural networks
• The velocity dispersion function of red galaxies in four Hubble Frontier Fields galaxy clusters
• Tidal Limit of Stellar Systems in Two-Power Density Models
• A Chandra view of SPT-CL J0217-5014: a massive galaxy cluster at a cosmic intersection at z=0.53
• AutoEnRichness: A hybrid empirical and analytical approach for estimating the richness of galaxy clusters
• The eventful life journey of galaxy clusters. II. Impact of mass accretion on the thermodynamical structure of the ICM
• Probing the evolution of galaxy clusters with the SZ Effect
• Deep Learning generated observations of galaxy clusters from dark-matter-only simulations
• Braginskii Viscosity in Cosmological Simulations of Galaxy Clusters: Implementation, Validation, and First Application
• Generating Galaxy Clusters Mass Density Maps from Mock Multiview Images via Deep Learning
• Impact of the calibration of the Halo Mass Function on galaxy cluster number count cosmology
• Catalogs of optically-selected clusters and photometric luminous red galaxies from the Hyper Suprime-Cam Subaru Strategic Program final year dataset
• Estimating the heterogeneity of pressure profiles within a complete sample of 55 galaxy clusters: a Bayesian Hierarchical Model
• Forecasting Galaxy Cluster HI Mass Recovery with CHIME at Redshifts z = 1 and 2 via the IllustrisTNG Simulations
• Impact of Rastall gravity on hydrostatic mass of galaxy clusters
• The Filament Rift: $\Lambda$CDM's Structural Challenge Against Observation
• Multiwavelength Characterization of a Dynamically Relaxed Cool Core Galaxy Cluster at $z=1.5$
• Discovery of Galaxy Clusters and a Head-Tail Radio Galaxy in the Direction of Globular Cluster NGC 6752
• Multi-scale weak lensing detection of galaxy clusters with source redshift tomography
• A MINOT-based Study of Gamma-ray emission from SPT-CL J2012-5649/Abell 3667
• The Splashback Mass Function of Galaxy Clusters from Photometric Data
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• SuperModel Predictions in the Outskirts of the Galaxy Cluster Zwicky 3146
• Dynamical Properties and Velocity Dispersion-Mass Relation of $z\sim 1$ Galaxy Clusters from the GOGREEN and GCLASS Surveys
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG
• The mass-dependent interplay of active galacitc nuclei and supernova feedback in shaping the $L_{\mathrm{X}}$--$T$ relation of early-type galaxies
• DUCA: Dynamic Universe Cosmological Analysis. II. The impact of clustering dark energy on the halo mass function
• Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
• GLTCAM: Concept of Multi-color Millimeter and Submillimeter Camera for the Greenland Telescope
• ESO 137-002: a large spiral undergoing edge-on ram-pressure stripping with little star formation in the tail
• Pressure profiles of distant Galaxy clusters with Planck-SPT data
• The hydrostatic mass bias in The Three Hundred clusters
• Luminosity-Temperature Relation as a Probe for Modified Gravity
• Cosmologia com aglomerados de galáxias
• The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
• Galaxies in the central regions of simulated galaxy clusters
• A new shock in the pre-merging cluster pair 1E2215-2216
• Timing the last major merger of galaxy clusters with large halo sparsity
• Universality of the halo mass function in modified gravity cosmologies
• CLASH-VLT: The Fifth Force in Chameleon Gravity from Joint Lensing and Kinematics Cluster Mass Profiles
• Assembly History and Internal Structure of Cluster Cold Dark Matter Haloes
• The richest clusters in the Coma and Leo superclusters: Properties and evolution
• The signature of major mergers on the hydrostatic mass bias of galaxy clusters