Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution

Abstract

We analyse cosmological hydrodynamical simulations of galaxy clusters to study the X-ray scaling relations between total masses and observable quantities such as X-ray luminosity, gas mass, X-ray temperature, and $Y_X$. Three sets of simulations are performed with an improved version of the smoothed particle hydrodynamics GADGET-3 code. These consider the following: non-radiative gas, star formation and stellar feedback, and the addition of feedback by active galactic nuclei (AGN). We select clusters with $M_{500}>10^{14}{M}_{\odot }E(z{)}^{-1}$, mimicking the typical selection of Sunyaev-Zeldovich samples. This permits to have a mass range large enough to enable robust fitting of the relations even at $z\sim 2$. The results of the analysis show a general agreement with observations. The values of the slope of the mass-gas mass and mass-temperature relations at $z=2$ are 10 per cent lower with respect to $z=0$ due to the applied mass selection, in the former case, and to the effect of early merger in the latter. We investigate the impact of the slope variation on the study of the evolution of the normalization. We conclude that cosmological studies through scaling relations should be limited to the redshift range $z=0-1$, where we find that the slope, the scatter, and the covariance matrix of the relations are stable. The scaling between mass and $Y_X$ is confirmed to be the most robust relation, being almost independent of the gas physics. At higher redshifts, the scaling relations are sensitive to the inclusion of AGNs which influences low-mass systems. The detailed study of these objects will be crucial to evaluate the AGN effect on the ICM.

arXiv comment24 pages, 11 figures, 5 tables, replaced to match accepted version

References in corpus (115)

• Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• The cosmological simulation code GADGET-2
• Statistical Properties of X-ray Clusters: Analytic and Numerical Comparisons
• Cosmological SPH simulations: A hybrid multi-phase model for star formation
• Modeling feedback from stars and black holes in galaxy mergers
• Collisional Plasma Models with APEC/APED: Emission Line Diagnostics of Hydrogen-like and Helium-like Ions
• Observational Probes of Cosmic Acceleration
• Some Aspects of Measurement Error in Linear Regression of Astronomical Data
• Cosmological Parameters from Observations of Galaxy Clusters
• Substructures in hydrodynamical cluster simulations
• Euclid Definition Study Report
• Tracing cosmic evolution with clusters of galaxies
• Chandra Cluster Cosmology Project II: Samples and X-ray Data Reduction
• Linear Regression for Astronomical Data with Measurement Errors and Intrinsic Scatter
• CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey
• Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
• Effects of Galaxy Formation on Thermodynamics of the Intracluster Medium
• Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
• Mechanical Feedback from Active Galactic Nuclei in Galaxies, Groups, and Clusters
• The Lx-T Relation and Temperature Function for Nearby Clusters Revisited
• Testing X-ray Measurements of Galaxy Clusters with Cosmological Simulations
• A New Robust Low-Scatter X-ray Mass Indicator for Clusters of Galaxies
• What is a Cool-Core Cluster? A Detailed Analysis of the Cores of the X-ray Flux-Limited HIFLUGCS Cluster Sample
• Comparing the temperatures of galaxy clusters from hydro-N-body simulations to Chandra and XMM-Newton observations
• Comparing the temperatures of galaxy clusters from hydro-N-body simulations to Chandra and XMM-Newton observations
• eROSITA Science Book: Mapping the Structure of the Energetic Universe
• CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey - Imaging Data and Catalogue Products
• The Canadian Cluster Comparison Project: detailed study of systematics and updated weak lensing masses
• Towards a realistic population of simulated galaxy groups and clusters
• Chemical enrichment of galaxy clusters from hydrodynamical simulations
• The Structure and Dynamical Evolution of Dark Matter Halos
• On the Accuracy of Weak Lensing Cluster Mass Reconstructions
• Weighing simulated galaxy clusters using lensing and X-ray
• The halo mass function through the cosmic ages
• Simulating the effect of AGN feedback on the metal enrichment of galaxy clusters
• A dynamical model for the distribution of dark matter and gas in galaxy clusters
• The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme
• Joint Analysis of Cluster Observations: II. Chandra/XMM-Newton X-ray and Weak Lensing Scaling Relations for a Sample of 50 Rich Clusters of Galaxies
• 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
• Robust Weak-lensing Mass Calibration of Planck Galaxy Clusters
• Lensing and X-ray mass estimates of clusters (SIMULATION)
• On the nature of hydrostatic equilibrium in galaxy clusters
• Gas expulsion by quasar-driven winds as a solution to the over-cooling problem in galaxy groups and clusters
• Raining on black holes and massive galaxies: the top-down multiphase condensation model
• SZ effects in the Magneticum Pathfinder Simulation: Comparison with the Planck, SPT, and ACT results
• Cool Core Clusters from Cosmological Simulations
• Simulations of AGN feedback in galaxy clusters and groups: impact on gas fractions and the Lx-T scaling relation
• The Growth of Cool Cores and Evolution of Cooling Properties in a Sample of 83 Galaxy Clusters at 0.3 < z < 1.2 Selected from the SPT-SZ Survey
• What are Protoclusters? -- Defining High Redshift Galaxy Clusters and Protoclusters
• A refined sub-grid model for black hole accretion and AGN feedback in large cosmological simulations
• Next Generation Cosmology: Constraints from the Euclid Galaxy Cluster Survey
• Cosmological simulations of galaxy clusters
• Self-similar scaling and evolution in the galaxy cluster X-ray Luminosity-Temperature relation
• Massive Halos in Millennium Gas Simulations: Multivariate Scaling Relations
• Baryon Census in Hydrodynamical Simulations of Galaxy Clusters
• Unifying the micro and macro properties of AGN feeding and feedback
• The X-Ray Luminosity--Mass Relation for Local Clusters of Galaxies
• Weighing the Giants V: Galaxy Cluster Scaling Relations
• On the role of AGN feedback on the thermal and chemodynamical properties of the hot intra-cluster medium
• Predicting Single-Temperature Fit to Multi-Component Thermal Plasma Spectra
• The impact of mergers on relaxed X-ray clusters - II. Effects on global X-ray and SZ properties and their scaling relations
• On the Baryon Fractions in Clusters and Groups of Galaxies
• A non-ideal MHD Gadget: Simulating massive galaxy clusters
• Scaling relations for galaxy clusters: properties and evolution
• Observational constraints on the redshift evolution of X-ray scaling relations of galaxy clusters out to z ~ 1.5
• The redshift evolution of massive galaxy clusters in the MACSIS simulations
• X-ray Clusters of Galaxies as Tracers of Structure in the Universe
• The MUSIC of Galaxy Clusters I: Baryon properties and Scaling Relations of the thermal Sunyaev-Zel'dovich Effect
• The XXL Survey. XIII. Baryon content of the bright cluster sample
• Witnessing the Growth of the Nearest Galaxy Cluster: Thermodynamics of the Virgo Cluster Outskirts
• The impact of cluster mergers on arc statistics
• On the Cluster Physics of Sunyaev-Zel'dovich and X-ray Surveys III: Measurement Biases and Cosmological Evolution of Gas and Stellar Mass Fractions
• X-ray mass proxies from hydrodynamic simulations of galaxy clusters (paper I)
• The XXL Survey III. Luminosity-temperature relation of the Bright Cluster Sample
• LoCuSS: The Sunyaev-Zel'dovich Effect and Weak Lensing Mass Scaling Relation
• Pressure of the hot gas in simulations of galaxy clusters
• Thermal SZ fluctuations in the ICM: probing turbulence and thermodynamics in Coma cluster with $Planck$
• The history of chemical enrichment in the intracluster medium from cosmological simulations
• Mock weak lensing analysis of simulated galaxy clusters: bias and scatter in mass and concentration
• The XXL Survey IV. Mass-temperature relation of the bright cluster sample
• Comparing Masses in Literature (CoMaLit)-I. Bias and scatter in weak lensing and X-ray mass estimates of clusters
• nIFTy galaxy cluster simulations I: dark matter & non-radiative models
• Sunyaev-Zel'dovich clusters in Millennium Gas simulations
• Can AGN feedback break the self-similarity of galaxies, groups, and clusters?
• Rhapsody-G simulations I: the cool cores, hot gas and stellar content of massive galaxy clusters
• A Model for Multi-property Galaxy Cluster Statistics
• The merger history of clusters and its effect on the X-ray properties of the intracluster medium
• The scatter and evolution of the global hot gas properties of simulated galaxy cluster populations
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• nIFTy galaxy cluster simulations II: radiative models
• Constraining galaxy cluster temperatures and redshifts with eROSITA survey data
• The Atacama Cosmology Telescope: Physical Properties of Sunyaev-Zel'dovich Effect Clusters on the Celestial Equator
• The evolution of galaxy cluster X-ray scaling relations
• The physics inside the scaling relations for X-ray galaxy clusters: gas clumpiness, gas mass fraction and slope of the pressure profile
• Cosmological simulations of galaxy clusters with feedback from active galactic nuclei: profiles and scaling relations
• Large-Scale Structure Formation: from the first non-linear objects to massive galaxy clusters
• The XMM-LSS survey: the Class 1 cluster sample over the extended 11 deg${}^2$ and its spatial distribution
• Chandra deep observation of XDCP J0044.0-2033, a massive galaxy cluster at z>1.5
• The MUSIC of Galaxy Clusters II: X-ray global properties and scaling relations
• Neutral hydrogen in galaxy clusters: impact of AGN feedback and implications for intensity mapping
• Hydrostatic and Caustic Mass Profiles of Galaxy Clusters
• Rhapsody-G simulations: galaxy clusters as baryonic closed boxes and the covariance between hot gas and galaxies
• The 2XMMi/SDSS Galaxy Cluster Survey. II. The optically confirmed cluster sample and the L_X-T relation
• IDCS J1426.5+3508: The Most Massive Galaxy Cluster at $z>1.5$
• Cluster X-ray luminosity-temperature relation at z>~1.5
• Chandra Measurements of a Complete Sample of X-ray Luminous Galaxy Clusters: The Luminosity-Mass Relation
• High redshift X-ray galaxy clusters. II. The L_X-T relationship revisited
• The generalized scaling relations for X-ray galaxy clusters: the most powerful mass proxy
• Scaling Rrelation in two situations of extreme mergers
• The XMM Cluster Survey: Evidence for energy injection at high redshift from evolution of the X-ray luminosity-temperature relation
• The MUSIC of Galaxy Clusters III: Properties, evolution and Y-M scaling relation of protoclusters of galaxies
• Combining Semi-analytic Models with Simulations of Galaxy Clusters: the Need for Heating from Active Galactic Nuclei
• Effects of Selection and Covariance on X-ray Scaling Relations of Galaxy Clusters
• II. Apples to apples $A^2$: cluster selection functions for next-generation surveys
• Pointing to the minimum scatter: the generalized scaling relations for galaxy clusters

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• The FABLE simulations: A feedback model for galaxies, groups and clusters
• Baryon Content in a Sample of 91 Galaxy Clusters Selected by the South Pole Telescope at 0.2 < z < 1.25
• X-ray scaling relations for a representative sample of Planck selected clusters observed with XMM-Newton
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• The DIANOGA simulations of galaxy clusters: characterizing star formation in proto-clusters
• Localized massive halo properties in Bahamas and Macsis simulations: scalings, log-normality, and covariance
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• Predictions for anisotropic X-ray signatures in the circumgalactic medium: imprints of supermassive black hole driven outflows
• Correlations between supermassive black holes and hot gas atmospheres in IllustrisTNG and X-ray observations
• Athena X-IFU synthetic observations of galaxy clusters to probe the chemical enrichment of the Universe
• XXL Survey groups and clusters in the Hyper Suprime-Cam Survey. Scaling relations between X-ray properties and weak lensing mass
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• Characterising the intra-cluster light in The Three Hundred simulations
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• Mass-Metallicity Relation from Cosmological Hydrodynamical Simulations and X-ray Observations of Galaxy Groups and Clusters
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• Mass Variance from Archival X-ray Properties of Dark Energy Survey Year-1 Galaxy Clusters
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• Black hole mass of central galaxies and cluster mass correlation in cosmological hydro-dynamical simulations
• Machine Learning methods to estimate observational properties of galaxy clusters in large volume cosmological N-body simulations
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• X-ray scaling relations from a complete sample of the richest maxBCG clusters
• The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray line emission
• Aging Halos: Implications of the Magnitude Gap on Conditional Statistics of Stellar and Gas Properties of Massive Halos
• A general framework to test gravity using galaxy clusters IV: Cluster and halo properties in DGP gravity
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• Voyage through the Hidden Physics of the Cosmic Web
• Chandra Observations of the Planck ESZ Sample: A Re-Examination of Masses and Mass Proxies
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• The XXL Survey: XXIII. The Mass Scale of XXL Clusters from Ensemble Spectroscopy
• A general framework to test gravity using galaxy clusters III: Observable-mass scaling relations in $f(R)$ gravity
• Ellipticity of Brightest Cluster Galaxies as tracer of halo orientation and weak-lensing mass bias
• Simulation view of galaxy clusters with low X-ray surface brightness
• High-redshift galaxy groups as seen by Athena/WFI
• 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${}_{\odot }$
• Cross Correlation between the Thermal Sunyaev-Zel'dovich Effect and Projected Galaxy Density Field
• A New Interpretation of the Mass-Temperature Relation and Mass Calibration of Galaxy Clusters Based on the Fundamental Plane
• Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- II. The X-ray Luminosity-Mass Relation
• The XXL Survey: XXXVIII. Scatters and correlations of X-ray proxies in the bright XXL cluster sample
• A Study of Gas Entropy Profiles of 47 Galaxy Clusters and Groups Out to the Virial Radius
• Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations
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• A general framework to test gravity using galaxy clusters VI: Realistic galaxy formation simulations to study clusters in modified gravity
• Suzaku Measurements of Hot Halo Emission at Outskirts for Two Poor Galaxy Groups: NGC 3402 and NGC 5129
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• On a possible cosmological evolution of galaxy cluster $Y_{\mathrm{X}}-Y_{\mathrm{SZE}}$ scaling relation
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