The FABLE simulations: A feedback model for galaxies, groups and clusters

Abstract

We present the Feedback Acting on Baryons in Large-scale Environments (FABLE) suite of cosmological hydrodynamical simulations of galaxies, groups and clusters. The simulations use the AREPO moving-mesh code with a set of physical models for galaxy formation based on the successful Illustris simulation, but with updated AGN and supernovae feedback models. This allows us to simultaneously reproduce the observed redshift evolution of the galaxy stellar mass function together with the stellar and gas mass fractions of local groups and clusters across a wide range of halo masses. Focusing on the properties of groups and clusters, we find very good agreement with a range of observed scaling relations, including the X-ray luminosity--total mass and gas mass relations as well as the total mass--temperature and Sunyaev-Zel'dovich flux--mass relations. Careful comparison of our results with scaling relations based on X-ray hydrostatic masses as opposed to weak lensing-derived masses reveals some discrepancies, which hint towards a non-negligible X-ray mass bias in observed samples. We further show that radial profiles of density, pressure and temperature of the simulated intracluster medium are in very good agreement with observations, in particular for $r>0.3r_{500}$. In the innermost regions however we find too large entropy cores, which indicates that a more sophisticated modelling of the physics of AGN feedback may be required to accurately reproduce the observed populations of cool-core and non-cool-core clusters.

arXiv comment31 pages, 20 figures, 2 appendices; MNRAS accepted

References in corpus (180)

• Planck 2015 results. XIII. Cosmological parameters
• A Universal Density Profile from Hierarchical Clustering
• Galactic Stellar and Substellar Initial Mass Function
• On the variation of the Initial Mass Function
• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• Energy input from quasars regulates the growth and activity of black holes and their host galaxies
• Populating a cluster of galaxies - I. Results at z=0
• E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
• Cosmological SPH simulations: A hybrid multi-phase model for star formation
• Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
• 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
• Simulating Galaxy Formation with the IllustrisTNG Model
• Toward a halo mass function for precision cosmology: the limits of universality
• First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
• Chandra sample of nearby relaxed galaxy clusters: mass, gas fraction, and mass-temperature relation
• Simulating galaxy formation with black hole driven thermal and kinetic feedback
• From dwarf spheroidals to cDs: Simulating the galaxy population in a LCDM cosmology
• Cosmological Parameters from Observations of Galaxy Clusters
• Introducing the Illustris Project: the evolution of galaxy populations across cosmic time
• Mass assembly in quiescent and star-forming galaxies since z=4 from UltraVISTA
• Substructures in hydrodynamical cluster simulations
• The Inner Structure of LambdaCDM Halos I: A Numerical Convergence Study
• The Evolution of the Stellar Mass Functions of Star-Forming and Quiescent Galaxies to z = 4 from the COSMOS/UltraVISTA Survey
• Cosmological Simulations with TreeSPH
• A model for cosmological simulations of galaxy formation physics
• Cosmology with the Sunyaev-Zel'dovich Effect
• The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the Y_SZ-M_500 relation
• The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas
• Euclid Definition Study Report
• A unified model for AGN feedback in cosmological simulations of structure formation
• Dancing in the dark: galactic properties trace spin swings along the cosmic web
• Formation of Galaxy Clusters
• Cosmological simulations of the growth of supermassive black holes and feedback from active galactic nuclei: method and tests
• Tracing cosmic evolution with clusters of galaxies
• The Sunyaev-Zel'dovich Effect
• CFHTLenS: The Canada-France-Hawaii Telescope Lensing Survey
• Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
• The Luminosity Function of Galaxies in SDSS Commissioning Data
• Galaxy cluster X-ray luminosity scaling relations from a representative local sample (REXCESS)
• The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time
• Testing X-ray Measurements of Galaxy Clusters with Cosmological Simulations
• The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology
• Scaling relations for galaxy clusters in the Millennium-XXL simulation
• Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts
• Galaxy Stellar Mass Functions from ZFOURGE/CANDELS: An Excess of Low-Mass Galaxies Since z=2 and the Rapid Buildup of Quiescent Galaxies
• The effects of galaxy formation on the matter power spectrum: A challenge for precision cosmology
• 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
• The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission
• The distribution of stellar mass in the low-redshift Universe
• Weak lensing for precision cosmology
• A Census of Baryons in Galaxy Clusters and Groups
• Effects of Baryons and Dissipation on the Matter Power Spectrum
• Towards a realistic population of simulated galaxy groups and clusters
• Galaxy And Mass Assembly (GAMA): The galaxy stellar mass function at z < 0.06
• The formation of disc galaxies in high resolution moving-mesh cosmological simulations
• The GEMS project: X-ray analysis and statistical properties of the group sample
• Gas entropy in a representative sample of nearby X-ray galaxy clusters (REXCESS): relationship to gas mass fraction
• The MassiveBlack-II Simulation: The Evolution of Halos and Galaxies to z~0
• Advanced ACTPol Cryogenic Detector Arrays and Readout
• A physical model for cosmological simulations of galaxy formation: multi-epoch validation
• Stellar and total baryon mass fractions in groups and clusters since redshift 1
• SPT-3G: A Next-Generation Cosmic Microwave Background Polarization Experiment on the South Pole Telescope
• Quantifying the effect of baryon physics on weak lensing tomography
• Galaxy Cluster Baryon Fractions Revisited
• The baseline intracluster entropy profile from gravitational structure formation
• Stellar mass -- halo mass relation and star formation efficiency in high-mass halos
• On the Accuracy of Weak Lensing Cluster Mass Reconstructions
• The massive end of the luminosity and stellar mass functions: Dependence on the fit to the light profile
• Weighing simulated galaxy clusters using lensing and X-ray
• A Weak Lensing Study of X-ray Groups in the COSMOS survey: Form and Evolution of the Mass-Luminosity Relation
• The halo mass function through the cosmic ages
• The case for AGN feedback in galaxy groups
• Images, structural properties and metal abundances of galaxy clusters observed with Chandra ACIS-I at 0.1<z<1.3
• Simulating the effect of AGN feedback on the metal enrichment of galaxy clusters
• Weighing the Giants - I. Weak-lensing masses for 51 massive galaxy clusters: project overview, data analysis methods and cluster images
• Weighing the Giants - III. Methods and Measurements of Accurate Galaxy Cluster Weak-Lensing Masses
• The Representative XMM-Newton Cluster Structure Survey (REXCESS) of an X-ray Luminosity Selected Galaxy Cluster Sample
• Scaling Properties of a Complete X-ray Selected Galaxy Group Sample
• 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
• The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies
• Robust Weak-lensing Mass Calibration of Planck Galaxy Clusters
• Lensing and X-ray mass estimates of clusters (SIMULATION)
• The Hydrangea simulations: galaxy formation in and around massive clusters
• The 400 square degrees ROSAT PSPC galaxy cluster survey: Catalog and statistical calibration
• Planck Early Results XI: Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations
• Gas expulsion by quasar-driven winds as a solution to the over-cooling problem in galaxy groups and clusters
• SZ effects in the Magneticum Pathfinder Simulation: Comparison with the Planck, SPT, and ACT results
• Cool Core Clusters from Cosmological Simulations
• Calibration of the galaxy cluster M_500-Y_X relation with XMM-Newton
• Simulations of AGN feedback in galaxy clusters and groups: impact on gas fractions and the Lx-T scaling relation
• Galaxy-cluster gas-density distributions of the Representative XMM-Newton Cluster Structure Survey (REXCESS)
• Total Galaxy Magnitudes and Effective Radii from Petrosian Magnitudes and Radii
• Simulating the Universe with MICE: The abundance of massive clusters
• Simulating cosmic ray physics on a moving mesh
• The X-ray cluster survey with eROSITA: forecasts for cosmology, cluster physics and primordial non-Gaussianity
• Mass Function Predictions Beyond LCDM
• The impact of baryons on the matter power spectrum from the Horizon-AGN cosmological hydrodynamical simulation
• Probing the Dark Matter and Gas Fraction in Relaxed Galaxy Groups with X-ray observations from Chandra and XMM
• Masses of galaxy clusters from gravitational lensing
• Four Measures of the Intracluster Medium Temperature and Their Relation to a Cluster's Dynamical State
• The impact of galaxy formation on the total mass, mass profile and abundance of haloes
• Cosmological simulations of galaxy clusters
• Self-similar scaling and evolution in the galaxy cluster X-ray Luminosity-Temperature relation
• Intracluster stars in simulations with AGN feedback
• Evidence for Non-Hydrostatic Gas from the Cluster X-ray to Lensing Mass Ratio
• Galaxy luminosities, stellar masses, sizes, velocity dispersions as a function of morphological type
• LoCuSS: A Comparison of Cluster Mass Measurements from XMM-Newton and Subaru - Testing Deviation from Hydrostatic Equilibrium and Non-Thermal Pressure Support
• The ASTRO-H Mission
• Constraining the Scatter in the Mass-Richness Relation of maxBCG Clusters With Weak Lensing and X-ray Data
• LoCuSS: First Results from Strong-lensing Analysis of 20 Massive Galaxy Clusters at z~0.2
• Weighing the Giants V: Galaxy Cluster Scaling Relations
• Gravitational Lensing in Clusters of Galaxies: New Clues Regarding the Dynamics of Intracluster Gas
• On the role of AGN feedback on the thermal and chemodynamical properties of the hot intra-cluster medium
• The XXL Survey. II. The bright cluster sample: catalogue and luminosity function
• HIFLUGCS: Galaxy cluster scaling relations between X-ray luminosity, gas mass, cluster radius, and velocity dispersion
• Imprints of dark energy on cosmic structure formation: II) Non-Universality of the halo mass function
• The fraction of cool-core clusters in X-ray vs. SZ samples using Chandra observations
• Testing the Low-Mass End of X-Ray Scaling Relations with a Sample of Chandra Galaxy Groups
• CLASH-X: A Comparison of Lensing and X-ray Techniques for Measuring the Mass Profiles of Galaxy Clusters
• Quenching star formation with quasar outflows launched by trapped IR radiation
• The cool core state of Planck SZ-selected clusters versus X-ray selected samples: evidence for cool core bias
• A Statistical Study of Weak Lensing by Triaxial Dark Matter Halos: Consequences for Parameter Estimation
• LoCuSS: Testing hydrostatic equilibrium in galaxy clusters
• The redshift evolution of massive galaxy clusters in the MACSIS simulations
• Weak lensing analysis of SZ-selected clusters of galaxies from the SPT and Planck surveys
• The XXL Survey. XIII. Baryon content of the bright cluster sample
• AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence
• Hot Gas in Galaxy Groups: Recent Observations
• Mismatch between X-ray and emission-weighted temperatures in galaxy clusters: cosmological implications
• Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution
• X-ray mass proxies from hydrodynamic simulations of galaxy clusters (paper I)
• The effect of AGN feedback on the halo mass function
• Simulating the interaction of jets with the intra-cluster medium
• The impact of baryons on massive galaxy clusters: halo structure and cluster mass estimates
• A census of cool core galaxy clusters in IllustrisTNG
• The XXL Survey III. Luminosity-temperature relation of the Bright Cluster Sample
• Driving gas shells with radiation pressure on dust in radiation-hydrodynamic simulations
• Cosmology and astrophysics from relaxed galaxy clusters - IV: Robustly calibrating hydrostatic masses with weak lensing
• Planck Intermediate Results. XI: The gas content of dark matter halos: the Sunyaev-Zeldovich-stellar mass relation for locally brightest galaxies
• HeCS-SZ: The Hectospec Survey of Sunyaev-Zeldovich Selected Clusters
• The Stacked Thermal SZ Signal of Locally Brightest Galaxies in Planck Full Mission Data: Evidence for Galaxy Feedback?
• The XXL Survey IV. Mass-temperature relation of the bright cluster sample
• Characterizing Intra-cluster light in the Hubble Frontier Fields
• Testing Sunyaev-Zel'dovich measurements of the hot gas content of dark matter haloes using synthetic skies
• Can AGN feedback break the self-similarity of galaxies, groups, and clusters?
• Weighing the Giants II: Improved Calibration of Photometry from Stellar Colors and Accurate Photometric Redshifts
• Rhapsody-G simulations I: the cool cores, hot gas and stellar content of massive galaxy clusters
• The high mass end of the stellar mass function: Dependence on stellar population models and agreement between fits to the light profile
• Gamma-ray Blazars Within the First 2 Billion Years
• Dark matter halo abundances, clustering and assembly histories at high redshift
• Baryon Content of Massive Galaxy Clusters (0.57 < z < 1.33)
• The Massive End of the Stellar Mass Function
• A Statistical Comparison of Cluster Mass Estimates from Optical/X-ray Observations and Gravitational Lensing
• The scatter and evolution of the global hot gas properties of simulated galaxy cluster populations
• The energetics of AGN radiation pressure-driven outflows
• Cosmic ray heating in cool core clusters - II. Self-regulation cycle and non-thermal emission
• 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 baryon budget on the galaxy group/cluster boundary
• The 400d Galaxy Cluster Survey weak lensing programme: III: Evidence for consistent WL and X-ray masses at $z\approx 0.5$
• Increasing blackhole feedback induced quenching with anisotropic thermal conduction
• How well do we know the Halo Mass Function?
• Impact of baryons on the cluster mass function and cosmological parameter determination
• The MUSIC of Galaxy Clusters II: X-ray global properties and scaling relations
• Hydrostatic and Caustic Mass Profiles of Galaxy Clusters
• Weak Lensing Calibrated M-T Scaling Relation of Galaxy Groups in the COSMOS Field
• Bias from gas inhomogeneities in the pressure profiles as measured from X-ray and SZ observations
• A weak gravitational lensing recalibration of the scaling relations linking the gas properties of dark halos to their mass
• Accurately simulating anisotropic thermal conduction on a moving mesh
• The impact of correlated projections on weak lensing cluster counts
• Chandra Measurements of a Complete Sample of X-ray Luminous Galaxy Clusters: The Luminosity-Mass Relation
• The X-ray luminosity-temperature relation of a complete sample of low-mass galaxy clusters
• Weak lensing calibration of mass bias in the REFLEX+BCS X-ray galaxy cluster catalogue
• Comparison of hydrostatic and dynamical masses of distant X-ray luminous galaxy clusters
• Intrinsic scatter of caustic masses and hydrostatic bias: An observational study

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