S
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.
Papers
More filters
Journal ArticleDOI
A measurement of secondary cosmic microwave background anisotropies with two years of South Pole Telescope observations
Christian L. Reichardt,L. Shaw,Oliver Zahn,K. A. Aird,Bradford Benson,Lindsey Bleem,John E. Carlstrom,John E. Carlstrom,C. L. Chang,C. L. Chang,Hsiao-Mei Cho,T. M. Crawford,A. T. Crites,T. de Haan,Matt Dobbs,J. P. Dudley,Elizabeth George,N. W. Halverson,Gilbert Holder,W. L. Holzapfel,S. Hoover,Zhen Hou,J. D. Hrubes,Marshall Joy,Ryan Keisler,Lloyd Knox,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,M. Lueker,Daniel M. Luong-Van,Jeff McMahon,J. Mehl,S. S. Meyer,Marius Millea,Joseph J. Mohr,T. E. Montroy,T. Natoli,Stephen Padin,Stephen Padin,T. Plagge,C. Pryke,C. Pryke,J. E. Ruhl,K. K. Schaffer,K. K. Schaffer,Erik Shirokoff,Helmuth Spieler,Z. K. Staniszewski,Antony A. Stark,K. T. Story,A. van Engelen,K. Vanderlinde,Joaquin Vieira,R. Williamson +54 more
TL;DR: In this paper, the authors present the first three-frequency South Pole Telescope (SPT) cosmic microwave background (CMB) power spectra, and find strong evidence for nonlinear clustering.
Journal ArticleDOI
Galaxy clusters discovered with a Sunyaev-Zel'dovich effect survey
Z. K. Staniszewski,Peter A. R. Ade,K. A. Aird,Bradford Benson,Lindsey Bleem,John E. Carlstrom,C. L. Chang,Hsiao-Mei Cho,T. M. Crawford,A. T. Crites,T. de Haan,Matt Dobbs,N. W. Halverson,Gilbert Holder,W. L. Holzapfel,J. D. Hrubes,Marshall Joy,Ryan Keisler,Trevor Lanting,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,A. Loehr,M. Lueker,Jeff McMahon,J. Mehl,S. S. Meyer,Joseph J. Mohr,T. E. Montroy,Chow-Choong Ngeow,Stephen Padin,T. Plagge,C. Pryke,Christian L. Reichardt,J. E. Ruhl,K. K. Schaffer,L. Shaw,Erik Shirokoff,Helmuth Spieler,B. Stalder,Antony A. Stark,K. Vanderlinde,Joaquin Vieira,Oliver Zahn,A. Zenteno +44 more
TL;DR: In this article, the South Pole Telescope (SPT) is conducting a Sunyaev-Zel'dovich (SZ) effect survey over large areas of the southern sky, searching for massive galaxy clusters to high redshift.
Journal ArticleDOI
Cosmological constraints from Sunyaev-Zel'dovich-selected clusters with X-ray observations in the first 178 deg2 of the South Pole Telescope survey
Bradford Benson,T. de Haan,J. P. Dudley,Christian L. Reichardt,K. A. Aird,K. Andersson,K. Andersson,R. Armstrong,M. L. N. Ashby,Marshall W. Bautz,Matthew B. Bayliss,G. Bazin,Lindsey Bleem,Mark Brodwin,John E. Carlstrom,John E. Carlstrom,John E. Carlstrom,C. L. Chang,C. L. Chang,Hsiao-Mei Cho,Alejandro Clocchiatti,T. M. Crawford,A. T. Crites,Shantanu Desai,M. A. Dobbs,Ryan J. Foley,William R. Forman,Elizabeth George,Michael D. Gladders,Anthony H. Gonzalez,N. W. Halverson,N. L. Harrington,F. W. High,Gilbert Holder,W. L. Holzapfel,S. Hoover,J. D. Hrubes,C. Jones,Marshall Joy,Ryan Keisler,Lloyd Knox,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,Jiayi Liu,M. Lueker,M. Lueker,D. Luong-Van,Adam Mantz,Daniel P. Marrone,Michael McDonald,Jeff McMahon,Jeff McMahon,J. Mehl,S. S. Meyer,S. S. Meyer,L. M. Mocanu,L. M. Mocanu,Joseph J. Mohr,T. E. Montroy,S. S. Murray,T. Natoli,Stephen Padin,Stephen Padin,T. Plagge,C. Pryke,Armin Rest,Jonathan Ruel,J. E. Ruhl,Benjamin Saliwanchik,A. Saro,J. T. Sayre,K. K. Schaffer,K. K. Schaffer,L. Shaw,L. Shaw,Erik Shirokoff,Erik Shirokoff,J. Song,Helmuth Spieler,B. Stalder,Z. K. Staniszewski,Antony A. Stark,K. T. Story,Christopher W. Stubbs,R. Šuhada,A. van Engelen,K. Vanderlinde,Joaquin Vieira,Joaquin Vieira,Alexey Vikhlinin,R. Williamson,Oliver Zahn,A. Zenteno +93 more
TL;DR: In this article, the authors use measurements from the South Pole Telescope (SPT) Sunyaev-Zel'dovich (SZ) cluster survey in combination with X-ray measurements to constrain cosmological parameters.
Journal ArticleDOI
CONSTRAINTS ON COSMOLOGY FROM THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM OF THE 2500 deg2 SPT-SZ SURVEY
Zhen Hou,Christian L. Reichardt,K. T. Story,B. Follin,Ryan Keisler,K. A. Aird,Bradford Benson,Lindsey Bleem,John E. Carlstrom,John E. Carlstrom,C. L. Chang,C. L. Chang,H. M. Cho,T. M. Crawford,A. T. Crites,T. de Haan,R. de Putter,M. A. Dobbs,Scott Dodelson,Scott Dodelson,J. P. Dudley,Elizabeth George,N. W. Halverson,Gilbert Holder,W. L. Holzapfel,S. Hoover,J. D. Hrubes,Marshall Joy,Lloyd Knox,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,M. Lueker,D. Luong-Van,Jeff McMahon,J. Mehl,J. Mehl,S. S. Meyer,Marius Millea,Joseph J. Mohr,T. E. Montroy,Stephen Padin,Stephen Padin,T. Plagge,C. Pryke,J. E. Ruhl,J. T. Sayre,K. K. Schaffer,K. K. Schaffer,L. Shaw,Erik Shirokoff,Helmuth Spieler,Z. K. Staniszewski,Antony A. Stark,A. van Engelen,K. Vanderlinde,J. D. Vieira,R. Williamson,Oliver Zahn +58 more
TL;DR: The authors explored extensions to the ΛCDM cosmology using measurements of the cosmic microwave background (CMB) from the recent SPT-SZ survey, along with data from WMAP7 and measurements of H_0 and baryon acoustic oscillation (BAO).
Journal ArticleDOI
First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Interpretation of the TT and TE Angular Power Spectrum Peaks
Lyman A. Page,M. R. Nolta,Cris W. Barnes,Charles L. Bennett,Mark Halpern,Gary Hinshaw,N. Jarosik,Alan J. Kogut,Michele Limon,Michele Limon,S. S. Meyer,Hiranya V. Peiris,David N. Spergel,Gregory S. Tucker,Gregory S. Tucker,Edward J. Wollack,Edward L. Wright +16 more
TL;DR: In this paper, a scaling relation for the temperature angular power spectrum (TT) and temperature-polarization cross-power spectrum (TE) was introduced, and a new scaling relation was introduced for the TE amplitude ratio, which is based on a flat adiabatic LambdaCDM model with the goal of showing how the cosmic baryon density, Omega-b h^2, matter density, and Omega-m istg^2 were encoded in their positions and amplitudes.