Baryon Content of Massive Galaxy Clusters at z=0-0.6

Abstract

We study the relationship between two major baryonic components in galaxy clusters, namely the stars in galaxies, and the ionized gas in the intracluster medium (ICM), using 94 clusters that span the redshift range 0-0.6. Accurately measured total and ICM masses from Chandra observations, and stellar masses derived from the Wide-field Infrared Survey Explorer and the Two-Micron All-Sky Survey allow us to trace the evolution of cluster baryon content in a self-consistent fashion. We find that, within r_{500}, the evolution of the ICM mass--total mass relation is consistent with the expectation of self-similar model, while there is no evidence for redshift evolution in the stellar mass--total mass relation. This suggests that the stellar mass and ICM mass in the inner parts of clusters evolve differently.

5 pages, 4 figures; accepted for publication in ApJ Letters

References in corpus (7)

• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
• The UKIRT Infrared Deep Sky Survey (UKIDSS)
• Stellar and total baryon mass fractions in groups and clusters since redshift 1
• Images, structural properties and metal abundances of galaxy clusters observed with Chandra ACIS-I at 0.1<z<1.3
• The Galaxy Content of SDSS Clusters and Groups
• The Hierarchical Build-Up of Massive Galaxies and the Intracluster Light since z=1
• Exploring the Energetics of Intracluster Gas with a Simple and Accurate Model

Cited by in corpus (77)

• The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
• Formation of Galaxy Clusters
• Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources
• Towards a realistic population of simulated galaxy groups and clusters
• Galaxy Cluster Baryon Fractions Revisited
• Stellar mass -- halo mass relation and star formation efficiency in high-mass halos
• The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies
• The EAGLE simulations of galaxy formation: the importance of the hydrodynamics scheme
• The pseudo-evolution of halo mass
• The impact of galaxy formation on the total mass, mass profile and abundance of haloes
• The BAHAMAS project: the CMB--large-scale structure tension and the roles of massive neutrinos and galaxy formation
• Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra
• The quenching and morphological evolution of central galaxies is facilitated by the feedback-driven expulsion of circumgalactic gas
• Baryon Census in Hydrodynamical Simulations of Galaxy Clusters
• The MOG Weak Field approximation II. Observational test of Chandra X-ray Clusters
• redMaPPer IV: Photometric Membership Identification of Cluster Galaxies with 1% Precision
• The redshift evolution of massive galaxy clusters in the MACSIS simulations
• The quenching and survival of ultra-diffuse galaxies in the Coma cluster
• Baryon Content in a Sample of 91 Galaxy Clusters Selected by the South Pole Telescope at 0.2 < z < 1.25
• The effect of AGN feedback on the halo mass function
• The impact of baryons on massive galaxy clusters: halo structure and cluster mass estimates
• Interactions between multiple supermassive black holes in galactic nuclei: a solution to the final parsec problem
• The thermal Sunyaev Zel'dovich effect power spectrum in light of Planck
• Intra Cluster Light properties in the CLASH-VLT cluster MACS J1206.2-0847
• The Massive and Distant Clusters of WISE Survey. I: Survey Overview and a Catalog of >2000 Galaxy Clusters at z~1
• \textsc{The Three Hundred} project: The \textsc{Gizmo-Simba} run
• The impact of the observed baryon distribution in haloes on the total matter power spectrum
• Understanding black hole mass assembly via accretion and mergers at late times in cosmological simulations
• A Census of Stellar Mass in 10 Massive Haloes at z~1 from the GCLASS Survey
• Observational Tests of Nonlocal Gravity: Galaxy Rotation Curves and Clusters of Galaxies
• The Rich Globular Cluster System of Abell 1689 and the Radial Dependence of the Globular Cluster Formation Efficiency
• Chemical Evolution on the Scale of Clusters of Galaxies: A Conundrum?
• Baryon Content of Massive Galaxy Clusters (0.57 < z < 1.33)
• The similarity of the stellar mass fractions of galaxy groups and clusters
• The biasing of baryons on the cluster mass function and cosmological parameter estimation
• A large sample of shear selected clusters from the Hyper Suprime-Cam Subaru Strategic Program S16A wide field mass maps
• The baryon content of groups and clusters of galaxies in the FABLE simulations
• SP(k) -- A hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
• Weak Lensing Reveals a Tight Connection Between Dark Matter Halo Mass and the Distribution of Stellar Mass in Massive Galaxies
• Iron in X-COP: tracing enrichment in cluster outskirts with high accuracy abundance profiles
• A Comparative Study of Local Galaxy Clusters: I. Derived X-ray Observables
• First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. III. Brightest cluster galaxies, stellar mass distribution, and active galaxies
• An application of machine learning techniques to galaxy cluster mass estimation using the MACSIS simulations
• Dynamical effects of the scale invariance of the empty space: The fall of dark matter ?
• Rhapsody-G simulations: galaxy clusters as baryonic closed boxes and the covariance between hot gas and galaxies
• Physical Correlations of the Scatter between Galaxy Mass, Stellar Content, and Halo Mass
• The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the FABLE simulations
• The Chemical Evolution of Galaxy Clusters: Dissecting the Iron Mass Budget of the Intracluster Medium
• Scalar field dark matter in clusters of galaxies
• Perspectives on Intracluster Enrichment and the Stellar Initial Mass Function in Elliptical Galaxies
• Mass-Metallicity Relation from Cosmological Hydrodynamical Simulations and X-ray Observations of Galaxy Groups and Clusters
• Yet another test of Radial Acceleration Relation for galaxy clusters
• SHELS: Optical Spectral Properties of WISE 22 μm-selected Galaxies
• Stellar Mass to Halo Mass Scaling Relation for X-ray Selected Low Mass Galaxy Clusters and Groups out to Redshift $z\approx 1$
• On the evolution of cluster scaling relations
• The Atacama Cosmology Telescope: the stellar content of galaxy clusters selected using the Sunyaev-Zel'dovich effect
• The origin of X-ray coronae around simulated disc galaxies
• The Effect of Galactic Feedback on Gas Accretion and Wind Recycling
• Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters
• Importance of Mock Observations in Validating Galaxy Properties for Cosmological Simulations
• Counts of galaxy clusters as cosmological probes: the impact of baryonic physics
• Spatial Distribution of Metals in the ICM: Evolution of the Iron Excess in Relaxed Galaxy Clusters
• The complex interplay of AGN jet-inflated bubbles and the intracluster medium
• Multiwavelength study of X-ray Luminous Clusters in the Hyper Suprime-Cam Subaru Strategic Program S16A field
• The Massive and Distant Clusters of WISE Survey VI: Stellar Mass Fractions of a Sample of High-Redshift Infrared-selected Clusters
• Revised Mass-to-Light Ratios For Nearby Galaxy Groups and Clusters
• The transformation and quenching of simulated gas-rich dwarf satellites within a group environment
• Scaling relations for dark matter core density and radius from Chandra X-ray cluster sample
• A test of Radial Acceleration Relation for the {\it Giles et al Chandra} cluster sample
• SZ/X-ray scaling relations using X-ray data and Planck Nominal maps
• DARKSKIES: A suite of super-sampled zoom-in simulations of galaxy clusters with self-interacting dark matter
• Stellar mass measurements in Abell 133 with Magellan / IMACS
• Dynamics of clusters of galaxies with extended $f(\chi )$ gravity
• The environmental dependence of the stellar mass fundamental plane of early-type galaxies
• A test of linearity of the ratio of dark matter to baryonic matter in galaxy clusters
• HSC-XXL : Baryon budget of the 136 XXL Groups and Clusters
• Properties of the Intracluster Medium Assuming an Einasto Dark Matter Profile