C
C. L. Chang
Researcher at Argonne National Laboratory
Publications - 298
Citations - 20619
C. L. Chang is an academic researcher from Argonne National Laboratory. The author has contributed to research in topics: South Pole Telescope & Cosmic microwave background. The author has an hindex of 74, co-authored 258 publications receiving 18558 citations. Previous affiliations of C. L. Chang include University of Chicago & University of California, Berkeley.
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CMB-S4 Science Book, First Edition
Kevork N. Abazajian,Peter Adshead,Zeeshan Ahmed,Steven W. Allen,David Alonso,Kam Arnold,Carlo Baccigalupi,James G. Bartlett,Nicholas Battaglia,Bradford Benson,Colin A. Bischoff,Julian Borrill,Victor Buza,Erminia Calabrese,Robert R. Caldwell,John E. Carlstrom,C. L. Chang,T. M. Crawford,Francis-Yan Cyr-Racine,Francesco De Bernardis,Tijmen de Haan,Sperello di Serego Alighieri,Joanna Dunkley,Cora Dvorkin,Josquin Errard,Giulio Fabbian,Stephen M. Feeney,Simone Ferraro,Jeffrey P. Filippini,Raphael Flauger,George M. Fuller,Vera Gluscevic,Daniel Green,Daniel Grin,Evan Grohs,Jason W. Henning,J. Colin Hill,Renée Hlozek,Gilbert Holder,W. L. Holzapfel,Wayne Hu,Kevin M. Huffenberger,Reijo Keskitalo,Lloyd Knox,Arthur Kosowsky,John M Kovac,Ely D. Kovetz,Chao-Lin Kuo,Akito Kusaka,Maude Le Jeune,Adrian T. Lee,M. Lilley,Marilena LoVerde,Mathew S. Madhavacheril,Adam Mantz,David J. E. Marsh,Jeff McMahon,P. D. Meerburg,Joel Meyers,Amber Miller,Julian B. Muñoz,Ho Nam Nguyen,Michael D. Niemack,Marco Peloso,J. Peloton,Levon Pogosian,C. Pryke,Marco Raveri,Christian L. Reichardt,Graca Rocha,Aditya Rotti,Emmanuel Schaan,Marcel Schmittfull,Douglas Scott,Neelima Sehgal,Sarah Shandera,Blake D. Sherwin,Tristan L. Smith,Lorenzo Sorbo,Glenn D. Starkman,K. T. Story,Alexander van Engelen,Joaquin Vieira,Scott Watson,Nathan Whitehorn,W. L. Kimmy Wu +85 more
TL;DR: The CMB-S4 project as mentioned in this paper is a ground-based cosmic microwave background (CMB) experiment with superconducting cameras, which will be used for the search for the B-mode polarization signature of primordial gravitational waves and the determination of the number and masses of neutrinos.
Journal ArticleDOI
The 10 Meter South Pole Telescope
John E. Carlstrom,Peter A. R. Ade,K. A. Aird,Bradford Benson,Lindsey Bleem,S. Busetti,C. L. Chang,E. Chauvin,Hsiao-Mei Cho,T. M. Crawford,A. T. Crites,Matt Dobbs,N. W. Halverson,S. Heimsath,W. L. Holzapfel,J. D. Hrubes,Marshall Joy,Ryan Keisler,Trevor Lanting,Adrian T. Lee,E. M. Leitch,J. Leong,W. Lu,M. Lueker,Daniel M. Luong-Van,Jeff McMahon,J. Mehl,S. S. Meyer,Joseph J. Mohr,T. E. Montroy,Stephen Padin,T. Plagge,C. Pryke,J. E. Ruhl,K. K. Schaffer,D. Schwan,Erik Shirokoff,Helmuth Spieler,Z. K. Staniszewski,Antony A. Stark,Carole Tucker,K. Vanderlinde,Joaquin Vieira,R. Williamson +43 more
TL;DR: The South Pole Telescope (SPT) as mentioned in this paper is a 10m diameter, wide-field, offset Gregorian telescope with a 966-pixel, multicolor, millimeter-wave, bolometer camera.
Journal ArticleDOI
Galaxy clusters discovered via the Sunyaev-Zel'dovich effect in the 2500-square-degree SPT-SZ survey
Lindsey Bleem,Lindsey Bleem,B. Stalder,T. de Haan,K. A. Aird,Steven W. Allen,Steven W. Allen,Douglas Applegate,Matthew L. N. Ashby,Mark W. Bautz,Matthew B. Bayliss,Bradford Benson,Bradford Benson,Sebastian Bocquet,Mark Brodwin,John E. Carlstrom,C. L. Chang,C. L. Chang,I-Non Chiu,Hsiao-Mei Cho,Alejandro Clocchiatti,T. M. Crawford,A. T. Crites,A. T. Crites,Shantanu Desai,J. P. Dietrich,Matt Dobbs,Matt Dobbs,R. J. Foley,R. J. Foley,William R. Forman,Elizabeth George,Michael D. Gladders,Anthony H. Gonzalez,N. W. Halverson,C. Hennig,Henk Hoekstra,Gilbert Holder,W. L. Holzapfel,J. D. Hrubes,Christine Jones,Ryan Keisler,Ryan Keisler,Lloyd Knox,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,Jiayi Liu,M. Lueker,M. Lueker,Daniel M. Luong-Van,Adam Mantz,Daniel P. Marrone,Michael McDonald,Jeff McMahon,S. S. Meyer,L. M. Mocanu,Joseph J. Mohr,S. S. Murray,Stephen Padin,Stephen Padin,C. Pryke,Christian L. Reichardt,Christian L. Reichardt,Armin Rest,Jonathan Ruel,J. E. Ruhl,Benjamin Saliwanchik,A. Saro,J. T. Sayre,K. K. Schaffer,K. K. Schaffer,Tim Schrabback,Erik Shirokoff,Erik Shirokoff,Jizhou Song,Jizhou Song,Helmuth Spieler,Spencer A. Stanford,Spencer A. Stanford,Z. K. Staniszewski,Z. K. Staniszewski,Antony A. Stark,K. T. Story,Christopher W. Stubbs,K. Vanderlinde,Joaquin Vieira,Alexey Vikhlinin,R. Williamson,R. Williamson,Oliver Zahn,Oliver Zahn,A. Zenteno +92 more
TL;DR: In this article, the authors presented a catalog of galaxy clusters selected via their Sunyaev-Zel'dovich (SZ) effect signature from 2500 deg^2 of South Pole Telescope (SPT) data.
Journal ArticleDOI
A measurement of the damping tail of the cosmic microwave background power spectrum with the south pole telescope
Ryan Keisler,Christian L. Reichardt,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,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,J. E. Ruhl,K. K. Schaffer,L. Shaw,Erik Shirokoff,Helmuth Spieler,Z. K. Staniszewski,Antony A. Stark,K. T. Story,A. van Engelen,K. Vanderlinde,Joaquin Vieira,R. Williamson,Oliver Zahn +52 more
TL;DR: In this article, the angular power spectrum of the cosmic microwave background (CMB) was measured using data from the South Pole Telescope (SPT) and the power spectrum was combined with the power spectra from the seven-year Wilkinson microwave anisotropy probe (WMAP) data release to constrain cosmological models.
Proceedings ArticleDOI
SPT-3G: A Next-Generation Cosmic Microwave Background Polarization Experiment on the South Pole Telescope
Bradford Benson,Peter A. R. Ade,Zeeshan Ahmed,Steven W. Allen,Kam Arnold,Jason E. Austermann,Jason E. Austermann,Amy N. Bender,Lindsey Bleem,John E. Carlstrom,John E. Carlstrom,C. L. Chang,C. L. Chang,Hsiao-Mei Cho,J. F. Cliche,T. M. Crawford,A. Cukierman,T. de Haan,Matt Dobbs,Matt Dobbs,D. Dutcher,W. B. Everett,A. J. Gilbert,N. W. Halverson,D. Hanson,N. L. Harrington,Kaori Hattori,Jason W. Henning,Gene C. Hilton,Gilbert Holder,Gilbert Holder,W. L. Holzapfel,Kent D. Irwin,Ryan Keisler,Lloyd Knox,Donna Kubik,Chao-Lin Kuo,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,Dale Li,Michael McDonald,S. S. Meyer,Joshua Montgomery,M. J. Myers,T. Natoli,H. Nguyen,Valentyn Novosad,Stephen Padin,Z. Pan,John E. Pearson,Christian L. Reichardt,Christian L. Reichardt,J. E. Ruhl,Benjamin Saliwanchik,G. Simard,Graeme Smecher,J. T. Sayre,Erik Shirokoff,Antony A. Stark,K. T. Story,Aritoki Suzuki,K. L. Thompson,Carole Tucker,K. Vanderlinde,Joaquin Vieira,Alexey Vikhlinin,Gensheng Wang,Volodymyr Yefremenko,Ki Won Yoon +69 more
TL;DR: SPT-3G as discussed by the authors is a new polarization sensitive receiver for the 10-meter South Pole Telescope (SPT), which will enable the advance from statistical detection of B-mode polarization anisotropy power to high signal-to-noise measurements of individual modes, i.e., maps.