Chandra Cluster Cosmology Project II: Samples and X-ray Data Reduction

Abstract

We discuss the measurements of the galaxy cluster mass functions at z=~0.05 and z=~0.5 using high-quality Chandra observations of samples derived from the ROSAT PSPC All-Sky and 400deg^2 surveys. We provide a full reference for the data analysis procedures, present updated calibration of relations between the total cluster mass and its X-ray indicators (T_X, Mgas, and Y_X) based on a subsample of low-z relaxed clusters, and present a first measurement of the evolving L_X-Mtot relation (with Mtot estimated from Y_X) obtained from a well-defined statistically complete cluster sample and with appropriate corrections for the Malmquist bias applied. Finally, we present the derived cluster mass functions, estimate the systematic uncertainties in this measurement, and discuss the calculation of the likelihood function. We confidently measure the evolution in the cluster comoving number density at a fixed mass threshold, e.g., by a factor of 5.0 +- 1.2 at M_500=2.5e14 h^-1 Msun between z=0 and 0.5. This evolution reflects the growth of density perturbations and can be used for the cosmological constraints complementing those from the distance-redshift relation.

ApJ in press (Feb 10, 2009 issue); replacement to match accepted version, includes revisions in response to referee's and community comments

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• Weak-lensing mass calibration of the Sunyaev-Zel'dovich effect using APEX-SZ galaxy clusters
• Optical identifications of high-redshift galaxy clusters from Planck Sunyaev-Zeldovich survey
• Exact Extreme Value Statistics and the Halo Mass Function
• The X-ray luminosity-temperature relation of a complete sample of low-mass galaxy clusters
• The 400d Galaxy Cluster Survey Weak Lensing Programme: I: MMT/Megacam Analysis of CL0030+2618 at z=0.50
• Abell 611. II. X-ray and strong lensing analyses
• A New Class of X-Ray Tails of Early-Type Galaxies and Subclusters in Galaxy Clusters - Slingshot Tails vs Ram Pressure Stripped Tails
• Extending the $L_{\mathrm{X}}-T$ relation from clusters to groups-Impact of cool core nature, AGN feedback, and selection effects
• An extension of the Planck galaxy cluster catalogue
• The Ysz--Yx Scaling Relation as Determined from Planck and Chandra
• Candidate Clusters of Galaxies at $z>1.3$ Identified in the Spitzer SPT Deep Field Survey
• Offsets between the X-ray and the Sunyaev-Zel'dovich-effect peaks in merging galaxy clusters and their cosmological implications
• Constraining the masses of high-redshift clusters with weak lensing: Revised shape calibration testing for the impact of stronger shears and increased blending
• (No) dimming of X-ray clusters beyond z~1 at fixed mass: crude redhshifts and masses from raw X-ray and SZ data
• The polytropic approximation and X-ray scaling relations: constraints on gas and dark matter profiles for galaxy groups and clusters
• A fitting formula for the non-Gaussian contribution to the lensing power spectrum covariance
• Stacked Weak Lensing Mass Calibration: Estimators, Systematics, and Impact on Cosmological Parameter Constraints
• Recovering galaxy cluster gas density profiles with XMM-Newton and Chandra
• The Impact of Baryons on Cosmological Inference from Weak Lensing Statistics
• Spectroscopic confirmation of a galaxy cluster associated with 7C1756+6520 at z=1.416
• Including massive neutrinos in thermal Sunyaev Zeldovich power spectrum and cluster counts analyses
• Reconciling Planck cluster counts and cosmology? Chandra/XMM instrumental calibration and hydrostatic mass bias
• X-ray calibration of SZ scaling relations with the ACCEPT catalogue of galaxy clusters observed by Chandra
• A multi-simulation study of relativistic SZ temperature scalings in galaxy clusters and groups
• Shape of Clusters as a Probe of Screening Mechanisms in Modified Gravity
• Yet another test of Radial Acceleration Relation for galaxy clusters
• Constraining the dark matter contribution of $\gamma$ rays in Cluster of galaxies using Fermi-LAT data
• Stellar Mass to Halo Mass Scaling Relation for X-ray Selected Low Mass Galaxy Clusters and Groups out to Redshift $z\approx 1$
• Are fossil groups a challenge of the Cold Dark Matter paradigm?
• One Thousand and One Clusters: Measuring the Bulk Flow with the Planck ESZ and X-Ray Selected Galaxy Cluster Catalogs
• Cosmological evidence for leptonic asymmetry after Planck
• Testing flatness of the universe with probes of cosmic distances and growth
• Metal Production in Galaxy Clusters: The Non-Galactic Component
• High significance detection of the tSZ effect relativistic corrections
• On the evolution of cluster scaling relations
• Model-independent X-ray mass determinations
• The Galaxy Luminosity Functions down to M_R=-10 in the Coma Cluster
• The 400d Galaxy Cluster Survey weak lensing programme: II: Weak lensing study of seven clusters with MMT/Megacam
• Possible indication for non-zero neutrino mass and additional neutrino species from cosmological observations
• RXJ0848.6+4453: The Evolution of Galaxy Sizes and Stellar Populations in a z=1.27 Cluster
• Nonlinear Effects in the Amplitude of Cosmological Density Fluctuations
• GalWeight Application: A publicly-available catalog of dynamical parameters of 1,800 galaxy clusters from SDSS-DR13, ($GalWCat19$)
• Impact of Weak Lensing Mass Calibration on eROSITA Galaxy Cluster Cosmological Studies -- a Forecast
• K-mouflage effects on clusters of galaxies
• Measuring galaxy cluster mass profiles into the low acceleration regime with galaxy kinematics
• Gravitationally Bound Bose Condensates with Rotation
• A Gibbs Sampler for Multivariate Linear Regression
• Aging Halos: Implications of the Magnitude Gap on Conditional Statistics of Stellar and Gas Properties of Massive Halos
• X-ray scaling relations from a complete sample of the richest maxBCG clusters
• Gas rotation in galaxy clusters: signatures and detectability in X-rays
• A New Approach to Identifying the Most Powerful Gravitational Lensing Telescopes
• Suzaku Observations of the Outskirts of the Galaxy Cluster Abell 3395 including a Filament toward Abell 3391
• Cosmology with the largest galaxy cluster surveys: Going beyond Fisher matrix forecasts
• XMMU J100750.5+125818: A strong lensing cluster at z=1.082
• The Atacama Cosmology Telescope: the stellar content of galaxy clusters selected using the Sunyaev-Zel'dovich effect
• Constraints on shear and rotation with massive galaxy clusters
• 7.1 keV sterile neutrino constraints from X-ray observations of 33 clusters of galaxies with Chandra ACIS
• 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 $z\gtrsim 1$
• Evidence for the Fifth Element Astrophysical status of Dark Energy
• Testing cosmic acceleration for $w(z)$ parameterizations using $f_{gas}$ measurements in galaxy clusters
• Galaxy populations in the most distant SPT-SZ clusters - I. Environmental quenching in massive clusters at $1.4\lesssim z\lesssim 1.7$
• Coping with Selection Effects: A Primer on Regression with Truncated Data
• The Effect of Galactic Feedback on Gas Accretion and Wind Recycling
• Constructing mock catalogues for the REFLEX II galaxy cluster sample
• Ophiuchus: an optical view of a very massive cluster of galaxies hidden behind the Milky Way
• A Massive Cluster at z = 0.288 Caught in the Process of Formation: The Case of Abell 959
• Cluster Lensing Profiles Derived from a Redshift Enhancement of Magnified BOSS-Survey Galaxies
• Velocity dispersion and dynamical mass for 270 galaxy clusters in the Planck PSZ1 catalogue
• A Detailed Study of the Most Relaxed SPT-Selected Galaxy Clusters: Cool Core and Central Galaxy Properties
• HIFLUGCS: X-ray luminosity -- dynamical mass relation and its implications for mass calibrations with the SPIDERS and 4MOST surveys
• Probing modified gravity via the mass-temperature relation of galaxy clusters
• A Multi-Wavelength Mass Analysis of RCS2 J232727.6-020437, a ~3x10${}^{15}$M${}_{\odot }$ Galaxy Cluster at z=0.7
• A Parameter Space Exploration of Galaxy Cluster Mergers II: Effects of Magnetic Fields
• eROSITA cluster cosmology forecasts: cluster temperature substructure bias
• High Frequency Cluster Radio Galaxies: Luminosity Functions and Implications for SZE Selected Cluster Samples
• Scientific Objectives of the Hot Universe Baryon Surveyor (HUBS) Mission
• X-ray surface brightness and gas density profiles of galaxy clusters up to 3*R500c with SRG/eROSITA
• MultiDark-Clusters: Galaxy Cluster Mock Light-Cones, eROSITA and the Cluster Power Spectrum
• Chandra Observations of the Planck ESZ Sample: A Re-Examination of Masses and Mass Proxies
• Unveiling the merger dynamics of the most massive MaDCoWS cluster at $z=1.2$ from a multi-wavelength mapping of its intracluster medium properties
• Galaxy Formation with Local Photoionization Feedback -II. Effect of X-Ray Emission from Binaries and Hot Gas
• The thermalisation of massive galaxy clusters
• Analysis of Sunyaev-Zel'dovich Effect Mass-Observable Relations using South Pole Telescope Observations of an X-ray Selected Sample of Low Mass Galaxy Clusters and Groups
• Suzaku X-ray Observations of the Nearest Non-Cool Core Cluster, Antlia: Dynamically Young but with Remarkably Relaxed Outskirts
• Bulge formation inside quiescent lopsided stellar disks: connecting accretion, star formation and morphological transformation in a z ~ 3 galaxy group
• The X-ray Properties of Weak Lensing Selected Galaxy Clusters
• Cosmological parameter estimation from CMB and X-ray clusters after Planck
• Low X-ray Luminosity Galaxy Clusters. III: Weak Lensing Mass Determination at 0.18 $<$ z $<$ 0.70
• Average Heating Rate of Hot Atmospheres in Distant Clusters by Radio AGN: Evidence for Continuous AGN Heating
• A general framework to test gravity using galaxy clusters III: Observable-mass scaling relations in $f(R)$ gravity
• VLT/Magellan spectroscopy of 29 strong lensing selected galaxy clusters
• KLLR: A scale-dependent, multivariate model class for regression analysis
• Galaxy and Mass Assembly (GAMA): Witnessing the assembly of the cluster Abell 1882
• How typical is the Coma cluster?
• The Three Hundred Project: the evolution of physical baryon profiles
• An accurate method of modeling cluster scaling relations in modified gravity
• Brightest Cluster Galaxies Trace Weak Lensing Mass Bias and Halo Triaxiality in The Three Hundred Project
• Scaling Relations and X-ray Properties of Moderate-Luminosity Galaxy Clusters from 0.3 < z < 0.6 with XMM-Newton
• Validation of Selection Function, Sample Contamination and Mass Calibration in Galaxy Cluster Samples
• Stringent Restriction from the Growth of Large-Scale Structure on Apparent Acceleration in Inhomogeneous Cosmological Models
• Chandra and XMM-Newton Observations of the Bimodal Planck SZ-detected Cluster PLCKG345.40-39.34 (A3716) with High and Low Entropy Subcluster Cores
• Fossil Groups in the Millennium Simulation: Their environment and its evolution
• Evaluating Tests of Virialization and Substructure Using Galaxy Clusters in the ORELSE Survey
• The SRG-eROSITA All-Sky Survey : Constraints on f(R) Gravity from Cluster Abundance
• X-Ray Emitting Active Galactic Nuclei from z = 0.6-1.3 in the Intermediate and High-Density Environments of the ORELSE Survey
• Merger Hydrodynamics of the Luminous Cluster RXJ1347.5-1145
• Probing dark energy with the next generation X-ray surveys of galaxy clusters
• Intrinsic scatter of caustic masses and hydrostatic bias: An observational study
• Constraints on ${\Omega }_{\mathrm{m}}$ and ${\sigma }_8$ from the potential-based cluster temperature function
• The X-ray-Optical Relations for Nine Clusters at z = 0.7-1.1
• Temperature and Entropy Profiles to the Virial Radius of Abell 1246 Cluster Observed with Suzaku
• A Simple Physical Model for the Gas Distribution in Galaxy Clusters
• Planck/SDSS Cluster Mass and Gas Scaling Relations for a Volume-Complete redMaPPer Sample
• Detection of spatial clustering in the 1000 richest SDSS DR8 redMaPPer clusters with Nearest Neighbor distributions
• Pointing to the minimum scatter: the generalized scaling relations for galaxy clusters
• The Clusters Hiding in Plain Sight (CHiPS) survey: Complete sample of extreme BCG clusters
• Cosmology based on $f(R)$ gravity with $\mathcal{O}(1)$ eV sterile neutrino
• X-ray Signatures of Non-Equilibrium Ionization Effects in Galaxy Cluster Accretion Shock Regions
• Unveiling the internal structure of Hercules supercluster
• Galaxy Luminosity Function of Dynamically Young Abell 119 Cluster: Probing the Cluster Assembly
• Multiwavelength study of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A field
• Galaxy cluster scaling relations measured with APEX-SZ
• Biases on cosmological parameter estimators from galaxy cluster number counts
• AMI observations of ten CLASH galaxy clusters: SZ and X-ray data used together to determine cluster dynamical states
• Sunyaev Zel'dovich observations of a statistically complete sample of galaxy clusters with OCRA-p
• Primordial magnetic fields with X-ray and S-Z cluster survey
• Hydrostatic Mass Profiles of Galaxy Clusters in the eROSITA Survey
• Revised Mass-to-Light Ratios For Nearby Galaxy Groups and Clusters
• The gas depletion factor in galaxy clusters: implication from Atacama Cosmology Telescope Polarization experiment measurements
• Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- II. The X-ray Luminosity-Mass Relation
• Discovery of large-scale diffuse radio emission and of a new galaxy cluster in the surroundings of MACSJ0520.7-1328
• Pulsar-wind-nebula-powered Galactic center X-ray filament G0.13-0.11: Proof of the synchrotron nature by IXPE
• The Universal Gas Mass Fraction in Clusters of Galaxies
• IDCS J1426.5+3508: Weak Lensing Analysis of a Massive Galaxy Cluster at $z=1.75$
• XLSSC 122 caught in the act of growing up: Spatially resolved SZ observations of a z=1.98 galaxy cluster
• The XXL Survey: XXXVIII. Scatters and correlations of X-ray proxies in the bright XXL cluster sample
• The Importance of Being Interpretable: Toward An Understandable Machine Learning Encoder for Galaxy Cluster Cosmology
• Measurement of Galaxy Cluster Integrated Comptonization and Mass Scaling Relations with the South Pole Telescope
• Exploring the galaxy cluster-group transition regime at high redshifts: Physical properties of two newly detected z > 1 systems
• Using clusters in SZE + x-ray surveys as an ensemble of rulers to constrain cosmology
• Constraining Cosmological Parameters using the Cluster Mass-Richness Relation
• Do cluster properties affect the quenching rate?
• Chandra Observations of the Spectacular A3411-12 Merger Event
• Suzaku Observations of the Cluster Outskirts and Intercluster Filament in the Triple Merger Cluster Abell 98
• Limits on evolution of the fine-structure constant in runaway dilaton models from Sunyaev-Zeldovich Observations
• X-ray galaxy clusters abundance and mass temperature scaling
• Observation of a very massive galaxy cluster at z=0.76 in SRG/eROSITA all-sky survey
• The SRG/eROSITA all-sky survey: The morphologies of clusters of galaxies I: A catalogue of morphological parameters
• The three-dimensional geometry and merger history of the massive galaxy cluster MACS J0358.8-2955
• Average Dark Matter Halo Sparsity Relations as Consistency Check of Mass Estimates in Galaxy Cluster Samples
• SZ Scaling Relations of Galaxy Groups and Clusters Near the North Ecliptic Pole
• Bound on the graviton mass from Chandra X-ray cluster sample
• Limits and challenges of the detection of cluster-scale diffuse radio emission at high redshift: The Massive and Distant Clusters of WISE Survey (MaDCoWS) in LoTSS-DR2
• Multi-wavelength Observations of the Dissociative Merger in the Galaxy Cluster CIZA J0107.7+5408
• The Halo Mass-Temperature Relation for Clusters, Groups, and Galaxies
• Galaxy cluster hydrostatic masses using Tolman-Oppenheimer-Volkoff equation
• Upper Limit on Dimming of Cosmological Sources by Intergalactic Grey Dust from the Soft X-ray Background
• An Empirical Determination of the Dependence of the Circumgalactic Mass Cooling Rate and Feedback Mass Loading Factor on Galactic Stellar Mass
• Probing Cosmology and Galaxy Cluster Structure with the Sunyaev-Zel'dovich Decrement vs. X-ray Temperature Scaling Relation
• Efficient Mass Estimate at the Core of Strong Lensing Galaxy Clusters Using the Einstein Radius
• Signature of cool cores in SZ clusters: a multiwavelength approach
• A model-independent test of the evolution of gas depletion factor for SPT-SZ and Planck ESZ clusters
• Sunyaev-Zel'dovich scaling relations from a simple phenomenological model for galaxy clusters
• Cosmology with Galaxy Cluster Properties using Machine Learning
• The Clusters Hiding in Plain Sight (CHiPS) survey: A first discovery of a massive nearby cluster around PKS1353-341
• Suzaku X-ray Follow-up Observation of Weak-lensing-detected Halos in the Field around ZwCl0823.2+0425
• Suzaku Measurements of Hot Halo Emission at Outskirts for Two Poor Galaxy Groups: NGC 3402 and NGC 5129
• The influence of mergers on the cluster temperature function and cosmological parameters derived from it
• Mass-Richness relations for X-ray and SZE-selected clusters at $0.4<z<2.0$ as seen by $Spitzer$ at 4.5$\mu$m
• Exploring the mass and redshift dependence of the cluster pressure profile with stacks on thermal SZ maps
• SZ/X-ray scaling relations using X-ray data and Planck Nominal maps
• The Velocity Distribution Function of Galaxy Clusters as a Cosmological Probe
• Measuring the X-ray luminosities of DESI groups from eROSITA Final Equatorial-Depth Survey: I. X-ray luminosity -- halo mass scaling relation
• Physical modelling of galaxy clusters using Einasto dark matter profiles
• The Gemini/HST Galaxy Cluster Project: Stellar Populations in the Low Redshift Reference Cluster Galaxies
• The Planck SZ Cluster Catalog: Expected X-ray Properties
• On the canonical formalism of $f(R)$-type gravity using Lie derivatives
• Testing Emergent Gravity with Optical, X-ray, and Weak Lensing Measurements in Massive, Relaxed Galaxy Clusters
• A Multi-wavelength Study of the Host Environment of SMBHB 4C+37.11
• X-ray properties of X-CLASS-redMaPPer galaxy cluster sample: The luminosity-temperature relation
• An excursion into the core of the cluster lens Abell 1689
• The NuSTAR and Chandra view of CL 0217+70 and Its Tell-Tale Radio Halo
• Classification of gamma-ray targets for velocity-dependent and subhalo-boosted dark-matter annihilation
• Scaling relations of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program Field
• The measurements of matter density perturbations amplitude from cosmological data
• The velocity field of the Lyra complex
• Imaging results from the legacy GMRT Galaxy Cluster Key Project
• Concentrating the Dark Matter in Galaxy Clusters through Tidal Stripping of Baryonically-Compressed Galactic Halos
• Studying galaxy cluster morphological metrics with Mock-X
• AMI SZ observation of galaxy-cluster merger CIZA J2242+5301: perpendicular flows of gas and dark matter
• Improvements in the X-ray luminosity function and constraints on the Cosmological parameters from X-ray luminous clusters
• Diffuse radio source candidate in CIZA J1358.9-4750
• A direct measurement of hierarchical growth in galaxy groups since z~1
• Follow-up of eROSITA and Euclid Galaxy Clusters with XMM-Newton
• The XXL Survey: XLVIII; X-ray follow-up of distant XXL clusters: Masses, scaling relations and AGN contamination
• Suppressing the thermal SZ-induced variance in CMB-cluster lensing estimators
• An expanded merger-tree description of cluster evolution
• Cosmological Simulation of Galaxy Groups and Clusters-II: Studying Different Modes of Feedback through X-ray Observations
• Substructure analysis of the RXCJ0232.2-4420 galaxy cluster
• Testing the Reliability of Cluster Mass Indicators with a Systematics Limited Dataset
• The Effect of Interacting Dark Energy on Mass-Temperature Relation in Galaxy Clusters
• The Fates of Merging Supermassive Black Holes and a Proposal for a New Class of X-Ray Sources
• Bayesian recalibration of Planck galaxy cluster scaling relations including relativistic Sunyaev-Zel'dovich corrections
• 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
• A Search for Neutron Star Precession and Interstellar Magnetic Field Variations via Multiepoch Pulsar Polarimetry
• Distant galaxy clusters in a deep XMM-Newton field within the CFTHLS D4
• Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect
• The Impact of Non-Equipartition on Cosmological Parameter Estimation from Sunyaev-Zel'dovich Surveys
• 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
• A high-resolution view of the filament of gas between Abell 399 and Abell 401 from the Atacama Cosmology Telescope and MUSTANG-2
• Jet interaction with galaxy cluster mergers
• A study of the galaxy redshift distribution toward the cosmic microwave background cold spot in the Corona Borealis supercluster
• 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
• Spectroscopic characterization of the protocluster of galaxies around 7C 1756+6520 at z ~ 1.4
• Tidal virialization of dark matter haloes with clustering dark energy
• Can decaying sterile neutrinos account for all dark matter?
• Semi analytical description of formation of galaxies and clusters of galaxies
• A Pre-Merger Stage Galaxy Cluster: Abell 3733
• SuperModel Analysis of Abell 1246 and J255: on the Evolution of Galaxy Clusters from High to Low Entropy States
• Constraints on the Neutrino Mass from SZ Surveys
• The eROSITA view on the halo mass-temperature relation: From low-mass groups to massive clusters
• Tracing the assembly histories of galaxy clusters in the nearby universe
• A rare case of FR I interaction with a hot X-ray bridge in the A2384 galaxy cluster
• Chandra observations of the Abell S0295 cluster
• X-ray Temperatures, Luminosities, and Masses From XMM-Newton Follow-up of the First Shear-selected Galaxy Cluster Sample
• Testing for evolution in scaling relations of galaxy clusters: Cross analysis between X-ray and SZ observations
• Average energy of the X-ray spectrum as a model-independent proxy for the mass of galaxy clusters
• Predicting the Non-Thermal Pressure in Galaxy Clusters
• X-ray and optical analysis of the distant, merging double cluster SPT-CLJ2228-5828, its gas bridge, and shock front
• Suzaku Observation of Abell 1555 and Abell 1558: Searching for Non-thermal Emission from Large Scale Structure Formation
• The stellar and hot gas content of low-mass galaxy clusters
• Spectroscopic confirmation of the galaxy clusters CARLA J0950+2743 at z=2.363, and CARLA-Ser J0950+2743 at z=2.243
• Sunyaev-Zel'dovich galaxy clusters number counts : consequences of cluster scaling laws evolution
• Differences in baryonic and dark matter scaling relations of galaxy clusters: A comparison between IllustrisTNG simulations and observations
• Forecasts for cosmological measurements based on the angular power spectra of AGN and clusters of galaxies in the SRG/eROSITA all-sky survey
• SZ power spectrum and cluster numbers from an extended merger-tree model
• Predicting the Scaling Relations between the Dark Matter Halo Mass and Observables from Generalised Profiles II: Intracluster Gas Emission
• Optical Identification of Galaxy Clusters among SRG/eROSITA X-ray Sources Based on Photometric Redshift Estimates for Galaxies
• Mapping the gas thermodynamic properties of the massive cluster merger MOO J1142$+$1527 at z = 1.2
• XMM-Newton follow-up of a sample of apparent low surface brightness galaxy groups detected in the ROSAT All-Sky Survey
• The Swift AGN and Cluster Survey. II. Cluster Confirmation with SDSS Data
• Deriving accurate galaxy cluster masses using X-ray thermodynamic profiles and graph neural networks
• Perseus cluster in its X-ray entirety with SRG/eROSITA. Merger and Radio-Uroboroses
• HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters
• Chandra Studies of the X-ray Gas Properties of Fossil Systems
• X-ray flux -- mass relation for $z\gtrsim 0.7$ galaxy clusters
• ALMA measures molecular gas reservoirs comparable to field galaxies in a low-mass galaxy cluster at z=1.3
• What halts the growth of galaxies?
• SRG/ART-XC all-sky X-ray survey: Catalog of sources detected during the first year
• Merger of massive galaxy cluster CL0238.3+2005 at z~0.4: just after pericenter passage?
• Estimating Cluster Masses from SDSS Multi-band Images with Transfer Learning
• Revisiting Galaxy Cluster Scaling Relations through Dark Matter-Gas Coherence: Scatter Dependence on Dynamical State
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray stacking analysis of Subaru's optically selected clusters spanning low richness regime
• 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
• X-ray characterisation of the massive galaxy clusterClG-J104803.7+313843 at z=0.76 with XMM-Newton
• Dynamical Properties and Velocity Dispersion-Mass Relation of $z\sim 1$ Galaxy Clusters from the GOGREEN and GCLASS Surveys
• A Spectroscopic View of the JWST/GTO Strong Lensing Cluster A1489
• The XMM-BCS galaxy cluster survey: I. The X-ray selected cluster catalog from the initial 6 deg${}^2$
• Discovery of Galaxy Clusters and a Head-Tail Radio Galaxy in the Direction of Globular Cluster NGC 6752
• Sunyaev-Zel'dovich Effect Observations of the Bullet Cluster (1E 0657-56) with APEX-SZ
• A comparative test of different pressure profile models in clusters of galaxies using recent ACT data