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
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Journal ArticleDOI
The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) Observatory
Angela V. Olinto,John F. Krizmanic,John F. Krizmanic,James H. Adams,Roberto Aloisio,Luis A. Anchordoqui,A. Anzalone,A. Anzalone,M. Bagheri,D. Barghini,M. Battisti,Douglas Bergman,M. E. Bertaina,P. Bertone,Francesca Bisconti,Mauricio Bustamante,F. Cafagna,Rossella Caruso,Rossella Caruso,Marco Casolino,K. Černý,Mark Christl,A. L. Cummings,I. De Mitri,R. Diesing,Ralph Engel,Johannes Eser,Ke Fang,Francesco Fenu,G. Filippatos,Eliza Gazda,C. Guepin,A. Haungs,E. Hays,E. G. Judd,Pavel Klimov,V. Kungel,E. Kuznetsov,S. Mackovjak,Dusan Mandat,L. Marcelli,Julie McEnery,G. Medina-Tanco,Kevin-Druis Merenda,S. S. Meyer,John Mitchell,H. Miyamoto,Jane Nachtman,Andrii Neronov,F. Oikonomou,Yasar Onel,G. Osteria,A. N. Otte,E. Parizot,T. Paul,Miroslav Pech,J. S. Perkins,P. Picozza,P. Picozza,Lech Wiktor Piotrowski,Z. Plebaniak,G. Prévôt,Patrick J. Reardon,Mary Hall Reno,M. Ricci,O. Romero Matamala,Fred Sarazin,Petr Schovanek,Valentina Scotti,K. Shinozaki,Jorge F. Soriano,Floyd W. Stecker,Y. Takizawa,Ralf Ulrich,M. Unger,Tonia M. Venters,L. R. Wiencke,D. Winn,R. Young,Mikhail Zotov +79 more
TL;DR: The Probe of Extreme Multi-Messenger Astrophysics (POEMMA) is designed to accurately observe ultra-high-energy cosmic rays (UHECRs) and cosmic neutrinos from space with sensitivity over the full celestial sky as discussed by the authors.
Journal ArticleDOI
Whole-Disk Observations of Jupiter, Saturn, and Mars in Millimeter/Submillimeter Bands
A. B. Goldin,M. S. Kowitt,Edward Cheng,D. A. Cottingham,D. J. Fixsen,C. A. Inman,S. S. Meyer,J. L. Puchalla,J. E. Ruhl,Robert F. Silverberg +9 more
TL;DR: In this paper, a balloon-borne observations of whole-disk brightness ratios for Jupiter, Saturn, and Mars are reported in four millimeter/submillimeter bands of bandwidth.
Proceedings ArticleDOI
Feedhorn‐Coupled TES Polarimeters for Next‐Generation CMB Instruments
Ki Won Yoon,J. W. Appel,Jason E. Austermann,J. A. Beall,Dan Becker,Bradford Benson,Lindsey Bleem,Joseph W. Britton,C. L. Chang,John E. Carlstrom,H. M. Cho,A. T. Crites,Thomas Essinger-Hileman,W. Everett,N. W. Halverson,Jason W. Henning,Gene C. Hilton,Kent D. Irwin,Jeff McMahon,J. Mehl,S. S. Meyer,Samuel J. Moseley,Michael D. Niemack,L. P. Parker,S. M. Simon,Suzanne T. Staggs,Kongpop U-Yen,C. Visnjic,Edward J. Wollack,Yue Zhao +29 more
TL;DR: In this article, the design and performance of planar orthomode transducer (OMT) coupled TES polarimeters and silicon micromachined platelet feedhorns optimized for scaling to large monolithic arrays are reported.
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 for the frequency bands centered at 95, 150, and 220 GHz.
Journal ArticleDOI
A measurement of the large-scale cosmic microwave background anisotropy at 1. 8 millimeter wavelength
TL;DR: In this article, the authors used a four-channel bolometric radiometer operating at 1.8, 1.1, 0.63, and 0.44 mm to map the diffuse sky brightness over half of the northern hemisphere with an angular resolution of 3.8 deg.