Cosmological Parameters from Observations of Galaxy Clusters
Abstract
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.
- Authors:
-
- Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology, Dept. of Physics
- Univ. of Michigan, Ann Arbor, MI (United States). Dept. of Physics and Astronomy and Michigan Center for Theoretical Physics
- NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- Publication Date:
- Research Org.:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1502963
- Report Number(s):
- SLAC-PUB-17063
Journal ID: ISSN 0066-4146
- Grant/Contract Number:
- AC02-76SF00515
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Annual Review of Astronomy and Astrophysics
- Additional Journal Information:
- Journal Volume: 49; Journal Issue: 1; Journal ID: ISSN 0066-4146
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; cosmology; dark energy; dark matter; galaxy clusters; intracluster medium; large-scale structure
Citation Formats
Allen, Steven W., Evrard, August E., and Mantz, Adam B. Cosmological Parameters from Observations of Galaxy Clusters. United States: N. p., 2011.
Web. doi:10.1146/annurev-astro-081710-102514.
Allen, Steven W., Evrard, August E., & Mantz, Adam B. Cosmological Parameters from Observations of Galaxy Clusters. United States. https://doi.org/10.1146/annurev-astro-081710-102514
Allen, Steven W., Evrard, August E., and Mantz, Adam B. Thu .
"Cosmological Parameters from Observations of Galaxy Clusters". United States. https://doi.org/10.1146/annurev-astro-081710-102514. https://www.osti.gov/servlets/purl/1502963.
@article{osti_1502963,
title = {Cosmological Parameters from Observations of Galaxy Clusters},
author = {Allen, Steven W. and Evrard, August E. and Mantz, Adam B.},
abstractNote = {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.},
doi = {10.1146/annurev-astro-081710-102514},
journal = {Annual Review of Astronomy and Astrophysics},
number = 1,
volume = 49,
place = {United States},
year = {Thu Sep 22 00:00:00 EDT 2011},
month = {Thu Sep 22 00:00:00 EDT 2011}
}
Web of Science
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WIMP searches with gamma rays in the Fermi era: challenges, methods and results
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Next Generation Cosmology: Constraints from the Euclid Galaxy Cluster Survey
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Chandra Measurements of a Complete Sample of X-ray Luminous Galaxy Clusters: The Luminosity-Mass Relation
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Cluster-Void Degeneracy Breaking: Dark Energy, Planck and the Largest Cluster & Void
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Confrontation of Top-Hat Spherical Collapse against Dark Halos from Cosmological N-Body Simulations
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Cosmology constraints from shear peak statistics in Dark Energy Survey Science Verification data
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Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
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The fraction of cool-core clusters in X-ray vs. SZ samples using Chandra observations
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Comparison of hydrostatic and dynamical masses of distant X-ray luminous galaxy clusters
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Constraints from thermal Sunyaev-Zeldovich cluster counts and power spectrum combined with CMB
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A General Precipitation-Limited L_X-T-R Relation Among Early-Type Galaxies
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Optimizing measurements of cluster velocities and temperatures for CCAT-prime and future surveys
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Dark energy two decades after: Observables, probes, consistency tests
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An extreme proto-cluster of luminous dusty starbursts in the early Universe
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Localized massive halo properties in Bahamas and Macsis simulations: scalings, log-normality, and covariance
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Sub-structure and merger detection in resolved NIKA Sunyaev-Zel'dovich images of distant clusters
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Optical Substructure and BCG Offsets of Sunyaev-Zel'dovich and X-ray Selected Galaxy Clusters
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The progeny of a Cosmic Titan: a massive multi-component proto-supercluster in formation at z=2.45 in VUDS
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Constraints on Cosmology and Baryonic Feedback with the Deep Lens Survey Using Galaxy-Galaxy and Galaxy-Mass Power Spectra
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An application of machine learning techniques to galaxy cluster mass estimation using the MACSIS simulations
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Mass Calibration of Optically Selected DES clusters using a Measurement of CMB-Cluster Lensing with SPTpol Data
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Cluster Cosmology Constraints from the 2500 deg$^2$ SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
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Dark Energy Survey Year 1 results: Validation of weak lensing cluster member contamination estimates from P(z) decomposition
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Coping with Selection Effects: A Primer on Regression with Truncated Data
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LoCuSS: Scaling relations between galaxy cluster mass, gas, and stellar content
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The galaxy cluster mass scale and its impact on cosmological constraints from the cluster population
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The mass-richness relation of optically-selected clusters from weak gravitational lensing and abundance with Subaru HSC first-year data
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A Massive Cluster at z = 0.288 Caught in the Process of Formation: The Case of Abell 959
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Covariance matrices for galaxy cluster weak lensing: from virial regime to uncorrelated large-scale structure
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Optical validation and characterization of Planck PSZ2 sources at the Canary Islands observatories. II. Second year of LP15 observations
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Ellipticity of Brightest Cluster Galaxies as tracer of halo orientation and weak-lensing mass bias
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Hydrostatic mass estimates of massive galaxy clusters: a study with varying hydrodynamics flavours and non-thermal pressure support
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