The SRG/eROSITA all-sky survey: The morphologies of clusters of galaxies: II. The intrinsic distributions of morphological parameters
arXiv:2601.00636 · doi:10.1051/0004-6361/202556830
Abstract
X-ray selected surveys of clusters of galaxies have been reported to contain more regular cool core clusters compared to samples selected using the Sunyaev-Zel'dovich (SZ) effect. Morphology population studies on X-ray selected clusters will be biased without taking into account selection, as cool cores are more easily detected at low redshifts, but can be mistaken for point sources at high redshift. eROSITA, aboard SRG, found over 12000 optically-identified clusters in its first survey, eRASS1. Taking account of the selection function obtained from simulations, we obtain using a Bayesian framework the intrinsic distribution of morphological parameters, including the concentration, central density, cuspiness, ellipticity and slosh. We construct scaling relations for the parameters as a function of redshift (z) and luminosity (LX), and study their distribution within z or LX bins. We find that the concentration in a scaled aperture evolves positively with LX, similarly to the central scaled density, and negatively with z. When using a fixed aperture, its evolution with LX is lower, but also dependent on the choice of cluster centre. The mean ellipticity does not significantly evolve with z or LX. eRASS1 clusters show indications of higher concentrations compared to SZ-selected objects, even after taking account the selection; this suggests that if our X-ray selection model is correct SZ-selected clusters may also suffer from morphological selection effects. We compare different parameter distribution models in bins of z and LX. The distribution of concentration and ellipticity is generally consistent with a normal one, but other parameters such as the central density and cuspiness strongly favour more complex distributions. However, modelling of all clusters as a single population generally prefers non-normal distributions. [abridged]
arXiv comment19 pages, 10 figures, accepted by A&A
References in corpus (50)
- Simulating the joint evolution of quasars, galaxies and their large-scale distribution
- Observational Evidence of AGN Feedback
- Toward a halo mass function for precision cosmology: the limits of universality
- The eROSITA X-ray telescope on SRG
- A New Non-Parametric Approach to Galaxy Morphological Classification
- Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
- Galaxy cluster X-ray luminosity scaling relations from a representative local sample (REXCESS)
- What is a Cool-Core Cluster? A Detailed Analysis of the Cores of the X-ray Flux-Limited HIFLUGCS Cluster Sample
- The SRG X-ray orbital observatory, its telescopes and first scientific results
- The SRG/eROSITA all-sky survey: First X-ray catalogues and data release of the western Galactic hemisphere
- The eROSITA Final Equatorial Depth Survey (eFEDS): The X-ray catalog
- Gas entropy in a representative sample of nearby X-ray galaxy clusters (REXCESS): relationship to gas mass fraction
- The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
- On the Cluster Physics of Sunyaev-Zel'dovich Surveys I: The Influence of Feedback, Non-thermal Pressure and Cluster Shapes on Y-M Scaling Relations
- The 400 square degrees ROSAT PSPC galaxy cluster survey: Catalog and statistical calibration
- On the nature of hydrostatic equilibrium in galaxy clusters
- Searching for Cool Core Clusters at High redshift
- Self-similar scaling and evolution in the galaxy cluster X-ray Luminosity-Temperature relation
- Quantifying the Morphologies and Dynamical Evolution of Galaxy Clusters. I. The Method
- The Remarkable Similarity of Massive Galaxy Clusters From z~0 to z~1.9
- Substructure of the galaxy clusters in the REXCESS sample: observed statistics and comparison to numerical simulations
- The fraction of cool-core clusters in X-ray vs. SZ samples using Chandra observations
- X-Ray morphological analysis of the Planck ESZ clusters
- The Prevalence of Cooling Cores in Clusters of Galaxies at z~0.15-0.4
- The cool core state of Planck SZ-selected clusters versus X-ray selected samples: evidence for cool core bias
- SIXTE -- The Generic X-ray Instrument Simulation Toolkit
- X-ray scaling relations for a representative sample of Planck selected clusters observed with XMM-Newton
- Lack of cooling flow clusters at z>0.5
- The evolution of cool-core clusters
- The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray Observable-to-Mass-and-Redshift Relations of Galaxy Clusters and Groups with Weak-Lensing Mass Calibration from the Hyper Suprime-Cam Subaru Strategic Program Survey
- The Non-Uniformity of Galaxy Cluster Metallicity Profiles
- A Morphology--Cosmology Connection for X--Ray Clusters
- Hydrostatic Chandra X-ray analysis of SPT-selected galaxy clusters - I. Evolution of profiles and core properties
- The Lx-Tvir relation in galaxy clusters: Effects of radiative cooling and AGN heating
- The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray Properties and Scaling Relations of Galaxy Clusters and Groups
- Full-sky photon simulation of clusters and active galactic nuclei in the soft X-rays for eROSITA
- Robust Quantification of Galaxy Cluster Morphology Using Asymmetry and Central Concentration
- Testing for X-ray-SZ Differences and Redshift Evolution in the X-ray Morphology of Galaxy Clusters
- Mass Estimation of Merging Galaxy Clusters
- What Do Dark Matter Properties Tell Us About Their Mass Assembly Histories?
- The eROSITA Final Equatorial-Depth Survey (eFEDS): Characterization of Morphological Properties of Galaxy Groups and Clusters
- The Selection Function of SZ Cluster Surveys
- The SRG/eROSITA All-Sky Survey: SRG/eROSITA cross-calibration with Chandra and XMM-Newton using galaxy cluster gas temperatures
- A study of cool core resiliency and entropy mixing in simulations of galaxy cluster mergers
- Projection effects in galaxy cluster samples: insights from X-ray redshifts
- The Observable Thermal and Kinetic Sunyaev-Zel'dovich Effect in Merging Galaxy Clusters
- The SRG/eROSITA all-sky survey: The morphologies of clusters of galaxies I: A catalogue of morphological parameters
- CHEX-MATE: the intracluster medium entropy distribution in the gravity-dominated regime
- Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
- XMM-Newton follow-up of a sample of apparent low surface brightness galaxy groups detected in the ROSAT All-Sky Survey