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Cosmological Parameters from Observations of Galaxy Clusters

Journal Article · · Annual Review of Astronomy and Astrophysics
 [1];  [2];  [3]
  1. Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology, Dept. of Physics
  2. Univ. of Michigan, Ann Arbor, MI (United States). Dept. of Physics and Astronomy and Michigan Center for Theoretical Physics
  3. NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)

Studies of galaxy clusters have proved crucial in helping to establish the standard model of cosmology, with a universe dominated by dark matter and dark energy. A theoretical basis that describes clusters as massive, multi-component, quasi-equilibrium systems is growing in its capability to interpret multi-wavelength observations of expanding scope and sensitivity. We review current cosmological results, including contributions to fundamental physics, obtained from observations of galaxy clusters. These results are consistent with and complementary to those from other methods. We highlight several areas of opportunity for the next few years, and emphasize the need for accurate modeling of survey selection and sources of systematic error. Capitalizing on these opportunities will require a multi-wavelength approach and the application of rigorous statistical frameworks, utilizing the combined strengths of observers, simulators and theorists.

Research Organization:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC02-76SF00515
OSTI ID:
1502963
Report Number(s):
SLAC-PUB--17063
Journal Information:
Annual Review of Astronomy and Astrophysics, Journal Name: Annual Review of Astronomy and Astrophysics Journal Issue: 1 Vol. 49; ISSN 0066-4146
Country of Publication:
United States
Language:
English

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The gas distribution in the outer regions of galaxy clusters journal April 2012
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The gas distribution in the outer regions of galaxy clusters text January 2011
Galaxy clusters discovered via the Sunyaev-Zel'dovich effect in the first 720 square degrees of the South Pole Telescope survey text January 2012
Chandra and optical/IR observations of CXOJ1415.2+3610, a massive, newly discovered galaxy cluster at z~1.5 text January 2012
The Atacama Cosmology Telescope: Sunyaev-Zel'dovich Selected Galaxy Clusters at 148 GHz from Three Seasons of Data text January 2013
The relation between velocity dispersion and mass in simulated clusters of galaxies: dependence on the tracer and the baryonic physics text January 2013
Masses of galaxy clusters from gravitational lensing text January 2013
Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources text January 2013
How well do we know the Halo Mass Function? text January 2013
The 2XMMi/SDSS Galaxy Cluster Survey. II. The optically confirmed cluster sample and the L_X-T relation text January 2013
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Cosmology with massive neutrinos III: the halo mass function and an application to galaxy clusters text January 2013
Constraining thawing and freezing models with cluster number counts text January 2014
The Swift X-ray Telescope Cluster Survey II. X-ray spectral analysis text January 2014
Weighing the Giants IV: Cosmology and Neutrino Mass text January 2014
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Galaxy clusters in the SDSS Stripe 82 based on galaxy photometric redshifts text January 2015
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Prospects for high-z cluster detections with Planck, based on a follow-up of 28 candidates using MegaCam@CFHT text January 2015
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Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe text January 2017
The fraction of cool-core clusters in X-ray vs. SZ samples using Chandra observations text January 2017
Comparison of hydrostatic and dynamical masses of distant X-ray luminous galaxy clusters text January 2017
Constraints from thermal Sunyaev-Zeldovich cluster counts and power spectrum combined with CMB text January 2017
A General Precipitation-Limited L_X-T-R Relation Among Early-Type Galaxies text January 2017
Optimizing measurements of cluster velocities and temperatures for CCAT-prime and future surveys text January 2017
Dark energy two decades after: Observables, probes, consistency tests text January 2017
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Weak lensing magnification of SpARCS galaxy clusters text January 2017
Localized massive halo properties in Bahamas and Macsis simulations: scalings, log-normality, and covariance text January 2017
Sub-structure and merger detection in resolved NIKA Sunyaev-Zel'dovich images of distant clusters text January 2017
Optical Substructure and BCG Offsets of Sunyaev-Zel'dovich and X-ray Selected Galaxy Clusters text January 2018
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Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra text January 2018
An application of machine learning techniques to galaxy cluster mass estimation using the MACSIS simulations text January 2018
Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data text January 2018
Cluster Cosmology Constraints from the 2500 deg$^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope text January 2018
Dark Energy Survey Year 1 results: Validation of weak lensing cluster member contamination estimates from P(z) decomposition text January 2018
Coping with Selection Effects: A Primer on Regression with Truncated Data text January 2019
LoCuSS: Scaling relations between galaxy cluster mass, gas, and stellar content text January 2019
Tests of Gravity with Galaxy Clusters text January 2019
The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population text January 2019
The mass-richness relation of optically-selected clusters from weak gravitational lensing and abundance with Subaru HSC first-year data text January 2019
A Massive Cluster at z = 0.288 Caught in the Process of Formation: The Case of Abell 959 text January 2019
Covariance matrices for galaxy cluster weak lensing: from virial regime to uncorrelated large-scale structure text January 2019
Optical validation and characterization of Planck PSZ2 sources at the Canary Islands observatories. II. Second year of LP15 observations text January 2019
Ellipticity of Brightest Cluster Galaxies as tracer of halo orientation and weak-lensing mass bias text January 2019
Hydrostatic mass estimates of massive galaxy clusters: a study with varying hydrodynamics flavours and non-thermal pressure support text January 2019
Precision cosmology with baryons: non-radiative hydrodynamics of galaxy groups text January 2017
Optimal weighting in galaxy surveys: Application to redshift-space distortions text January 2012

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