Stellar Mass Assembly of Brightest Cluster Galaxies at Late Times
arXiv:1409.4820 · doi:10.1093/mnras/stu2126
Abstract
Understanding the formation history of brightest cluster galaxies is an important topic in galaxy formation. Utilizing the Planck Sunyaev-Zel'dovich cluster catalog, and applying the Ansatz that the most massive halos at one redshift remain among the most massive ones at a slightly later cosmic epoch, we have constructed cluster samples at redshift z~0.4 and z~0.2 that can be statistically regarded as progenitor-descendant pairs. This allows us to study the stellar mass assembly history of BCGs in these massive clusters at late times, finding the degree of growth between the two epochs is likely at only few percent level, which is far lower compared to the prediction from a state-of-the-art semi-analytic galaxy formation model.
arXiv comment11 pages, 8 figures, 3 tables; resubmitted to MNRAS after addressing the referee report
References in corpus (28)
- Stellar population synthesis at the resolution of 2003
- The Sloan Digital Sky Survey: Technical Summary
- Galactic Stellar and Substellar Initial Mass Function
- The cosmological simulation code GADGET-2
- Simulating the joint evolution of quasars, galaxies and their large-scale distribution
- Planck 2013 results. I. Overview of products and scientific results
- GADGET: A code for collisionless and gasdynamical cosmological simulations
- K-corrections and filter transformations in the ultraviolet, optical, and near infrared
- The hierarchical formation of the brightest cluster galaxies
- From dwarf spheroidals to cDs: Simulating the galaxy population in a LCDM cosmology
- The formation history of elliptical galaxies
- The Tenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the SDSS-III Apache Point Observatory Galactic Evolution Experiment
- The Evolution of the Stellar Mass Functions of Star-Forming and Quiescent Galaxies to z = 4 from the COSMOS/UltraVISTA Survey
- The Growth of Massive Galaxies Since z=2
- Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts
- Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources
- K-band Properties of Galaxy Clusters and Groups: Brightest Cluster Galaxies and Intracluster Light
- Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts
- An Infrared Survey of Brightest Cluster Galaxies. II: Why are Some Brightest Cluster Galaxies Forming Stars?
- Total Galaxy Magnitudes and Effective Radii from Petrosian Magnitudes and Radii
- Evidence for Significant Growth in the Stellar Mass of Brightest Cluster Galaxies over the Past 10 Billion Years
- Early assembly of the most massive galaxies
- The Color-Magnitude Effect in Early-Type Cluster Galaxies
- The evolution of the brightest cluster galaxies since z~1 from the ESO Distant Cluster Survey (EDisCS)
- The XMM Cluster Survey: The build up of stellar mass in Brightest Cluster Galaxies at high redshift
- Early Formation and Late Merging of the Giant Galaxies
- The Stellar Mass Growth of Brightest Cluster Galaxies in the IRAC Shallow Cluster Survey
- Surface photometry of BCGs and intracluster stars in Lambda-CDM
Cited by in corpus (15)
- The realm of the galaxy protoclusters
- Avoiding progenitor bias: The structural and mass evolution of Brightest Group and Cluster Galaxies in Hierarchical models since z~1
- BCG Mass Evolution in Cosmological Hydro-Simulations
- The baryon content of groups and clusters of galaxies in the FABLE simulations
- Galaxies in X-ray Selected Clusters and Groups in Dark Energy Survey Data I: Stellar Mass Growth of Bright Central Galaxies Since z~1.2
- The early phases of galaxy clusters formation in IR: coupling hydrodynamical simulations with GRASIL3D
- First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. III. Brightest cluster galaxies, stellar mass distribution, and active galaxies
- Stellar Populations of BCGs, Close Companions and Intracluster Light in Abell 85, Abell 2457 and IIZw108
- The accretion histories of brightest cluster galaxies from their stellar population gradients
- The Relationship Between Brightest Cluster Galaxy Star Formation and the Intracluster Medium in CLASH
- Star Formation in Intermediate Redshift 0.2 < z < 0.7 Brightest Cluster Galaxies
- Stellar Mass and 3.4 m M/L Ratio Evolution of Brightest Cluster Galaxies in COSMOS since z ~ 1.0
- SDSS-IV MaNGA: Cannibalism Caught in the Act -- on the Frequency of Occurrence of Multiple Cores in Brightest Cluster Galaxies
- A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
- The Kormendy relation of cluster galaxies in PPS regions