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S. S. Meyer

Researcher at University of Chicago

Publications -  503
Citations -  111128

S. S. Meyer is an academic researcher from University of Chicago. The author has contributed to research in topics: Cosmic microwave background & South Pole Telescope. The author has an hindex of 116, co-authored 474 publications receiving 105142 citations. Previous affiliations of S. S. Meyer include Massachusetts Institute of Technology & University of Arizona.

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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

TL;DR: In this article, the authors derived cosmological constraints using a galaxy cluster sample selected from the 2500~deg$^2$ SPT-SZ survey, which is supplemented with optical weak gravitational lensing measurements of 32 clusters with $0.29
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First Year Wilkinson Microwave Anisotropy Probe Observations: Dark Energy Induced Correlation with Radio Sources

TL;DR: In this paper, the first-year Wilkinson Microwave Anisotropy Probe (WMAP) data, in combination with any one of a number of other cosmic probes, show that we live in a flat Λ-dominated cold dark matter (CDM) universe with Ωm ≈ 0.28, h = 0.33, and no dark energy component (ΩΛ = 0) would produce an anticorrelation between the matter distribution and the CMB.
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X-ray properties of the first sunyaev-zel'dovich effect selected galaxy cluster sample from the south pole telescope

K. Andersson, +68 more
TL;DR: In this paper, the authors present results of X-ray observations of a sample of 15 clusters selected via their imprint on the cosmic microwave background from the thermal Sunyaev-Zel'dovich (SZ) effect.
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Preliminary separation of galactic and cosmic microwave emission for the COBE Differential Microwave Radiometer

TL;DR: In this article, preliminary models of microwave emission from the Milky Way Galaxy based on COBE and other data are constructed for the purpose of distinguishing cosmic and Galactic signals, with the modeled Galactic emission removed, with a quadrupole distribution.