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Title: Cool core bias in Sunyaev–zel’dovich galaxy cluster surveys

Journal Article · · Astrophysical Journal
 [1]; ;  [2];  [3]
  1. Harvard University, Cambridge, MA 02138 (United States)
  2. Kavli Institute for Astrophysics and Space Research, MIT, Cambridge, MA 02139 (United States)
  3. Fermi National Accelerator Laboratory, Batavia, IL 60510-0500 (United States)

Sunyaev–Zel’dovich (SZ) surveys find massive clusters of galaxies by measuring the inverse Compton scattering of cosmic microwave background off of intra-cluster gas. The cluster selection function from such surveys is expected to be nearly independent of redshift and cluster astrophysics. In this work, we estimate the effect on the observed SZ signal of centrally peaked gas density profiles (cool cores) and radio emission from the brightest cluster galaxy by creating mock observations of a sample of clusters that span the observed range of classical cooling rates and radio luminosities. For each cluster, we make simulated SZ observations by the South Pole Telescope and characterize the cluster selection function, but note that our results are broadly applicable to other SZ surveys. We find that the inclusion of a cool core can cause a change in the measured SPT significance of a cluster between 0.01 and 10% at z>0.3, increasing with cuspiness of the cool core and angular size on the sky of the cluster (i.e., decreasing redshift, increasing mass). We provide quantitative estimates of the bias in the SZ signal as a function of a gas density cuspiness parameter, redshift, mass, and the 1.4 GHz radio luminosity of the central active galactic nuclei. Based on this work, we estimate that, for the Phoenix cluster (one of the strongest cool cores known), the presence of a cool core is biasing the SZ significance high by ∼6%. The ubiquity of radio galaxies at the centers of cool core clusters will offset the cool core bias to varying degrees.

OSTI ID:
22882613
Journal Information:
Astrophysical Journal, Vol. 802, Issue 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); Since 2009, the country of publication for this journal is the UK.; ISSN 0004-637X
Country of Publication:
United Kingdom
Language:
English

Cited By (11)

Toward a characterization of X-ray galaxy clusters for cosmology journal August 2019
A study of high-redshift AGN feedback in SZ cluster samples journal June 2017
The cool-core state of Planck SZ-selected clusters versus X-ray-selected samples: evidence for cool-core bias journal February 2017
A census of cool-core galaxy clusters in IllustrisTNG journal August 2018
THE EVOLUTION OF THE INTRACLUSTER MEDIUM METALLICITY IN SUNYAEV ZEL’DOVICH-SELECTED GALAXY CLUSTERS AT 0 < z < 1.5 journal July 2016
The Fraction of Cool-core Clusters in X-Ray versus SZ Samples Using Chandra Observations journal July 2017
X-Ray Morphological Analysis of the Planck ESZ Clusters journal August 2017
The cool core state of Planck SZ-selected clusters versus X-ray selected samples: evidence for cool core bias text January 2017
The fraction of cool-core clusters in X-ray vs. SZ samples using Chandra observations text January 2017
A Study of High-redshift AGN Feedback in SZ Cluster Samples text January 2017
Towards a characterization of X-ray galaxy clusters for cosmology text January 2019