W
W. L. K. Wu
Researcher at Stanford University
Publications - 110
Citations - 4936
W. L. K. Wu is an academic researcher from Stanford University. The author has contributed to research in topics: Cosmic microwave background & South Pole Telescope. The author has an hindex of 31, co-authored 100 publications receiving 4083 citations. Previous affiliations of W. L. K. Wu include SLAC National Accelerator Laboratory & University of Chicago.
Papers
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Journal ArticleDOI
Detection of CMB-Cluster Lensing using Polarization Data from SPTpol.
Srinivasan Raghunathan,Srinivasan Raghunathan,S. Patil,Eric J. Baxter,Bradford Benson,Bradford Benson,Lindsey Bleem,T. M. Crawford,G. P. Holder,G. P. Holder,T. McClintock,Christian L. Reichardt,T. N. Varga,T. N. Varga,Nathan Whitehorn,Peter A. R. Ade,S. Allam,Adam Anderson,Jason E. Austermann,Santiago Avila,Jessica Avva,David Bacon,J. A. Beall,Amy N. Bender,Federico Bianchini,Sebastian Bocquet,Sebastian Bocquet,David Brooks,D. L. Burke,John E. Carlstrom,John E. Carlstrom,J. Carretero,F. J. Castander,C. L. Chang,C. L. Chang,H. C. Chiang,Robert I. Citron,M. Costanzi,A. T. Crites,A. T. Crites,L. N. da Costa,Shantanu Desai,H. T. Diehl,J. P. Dietrich,Matt Dobbs,Matt Dobbs,Peter Doel,S. Everett,August E. Evrard,Chang Feng,B. Flaugher,Pablo Fosalba,Joshua A. Frieman,Jason Gallicchio,Juan Garcia-Bellido,Enrique Gaztanaga,Elizabeth George,Elizabeth George,Tommaso Giannantonio,A. J. Gilbert,Robert A. Gruendl,J. Gschwend,Nikhel Gupta,G. Gutierrez,T. de Haan,T. de Haan,N. W. Halverson,N. L. Harrington,Jason W. Henning,Gene C. Hilton,Devon L. Hollowood,W. L. Holzapfel,K. Honscheid,J. D. Hrubes,N. Huang,Johannes Hubmayr,Kent D. Irwin,Tesla E. Jeltema,M. Carrasco Kind,Lloyd Knox,N. Kuropatkin,Ofer Lahav,Adrian T. Lee,Adrian T. Lee,Dale Li,Dale Li,Marcos Lima,A. E. Lowitz,M. A. G. Maia,Jennifer L. Marshall,Jeff McMahon,Peter Melchior,Felipe Menanteau,S. S. Meyer,Ramon Miquel,L. M. Mocanu,Joseph J. Mohr,Joseph J. Mohr,Joshua Montgomery,C. Corbett Moran,Andrew Nadolski,T. Natoli,T. Natoli,John P. Nibarger,G. I. Noble,Valentine Novosad,R. L. C. Ogando,Stephen Padin,Stephen Padin,A. A. Plazas,C. Pryke,David Rapetti,David Rapetti,A. K. Romer,A. Roodman,A. Carnero Rosell,Eduardo Rozo,J. E. Ruhl,Eli S. Rykoff,Benjamin Saliwanchik,Benjamin Saliwanchik,E. J. Sanchez,J. T. Sayre,V. Scarpine,K. K. Schaffer,K. K. Schaffer,Michael Schubnell,S. Serrano,I. Sevilla-Noarbe,C. Sievers,Graeme Smecher,Mathew Smith,Marcelle Soares-Santos,Antony A. Stark,K. T. Story,E. Suchyta,M. E. C. Swanson,Gregory Tarle,Carole Tucker,K. Vanderlinde,T. Veach,J. De Vicente,Joaquin Vieira,Vinu Vikram,Gensheng Wang,W. L. K. Wu,V. G. Yefremenko,Yanxi Zhang +147 more
TL;DR: This detection of gravitational lensing due to galaxy clusters using only the polarization of the cosmic microwave background (CMB) is reported, a key first step for cluster cosmology with future low-noise CMB surveys, like CMB-S4, for which CMB polarization will be the primary channel for cluster lensing measurements.
Posted ContentDOI
The Latest Constraints on Inflationary B-modes from the BICEP/Keck Telescopes
BICEPKeck Collaboration P.A.R. Ade,Zeeshan Ahmed,Mandana Amiri,Denis Barkats,R. Basu Thakur,D. Beck,Colin A. Bischoff,James J. Bock,H. Boenish,E. Bullock,Victor Buza,IV J.R.Cheshire,Jake Connors,J. Cornelison,M. Crumrine,Ari Cukierman,E. V. Denison,Marion Dierickx,L. Duband,M. Eiben,S. Fatigoni,Jeffrey P. Filippini,S. Fliescher,Christos Giannakopoulos,Neil Goeckner-Wald,D. C. Goldfinger,J. A. Grayson,Paul K. Grimes,George Halal,G. Hall,Mark Halpern,E. Hand,S. A. Harrison,Stuart Henderson,S. R. Hildebrandt,Gene C. Hilton,Johannes Hubmayr,Howard Hui,Kent D. Irwin,J. Kang,Kirit Karkare,E. Karpel,S. Kefeli,S. A. Kernasovskiy,John M Kovac,Chao-Lin Kuo,K. Lau,E. M. Leitch,Amber Lennox,K. G. Megerian,L. Minutolo,Lorenzo Moncelsi,Y. Nakato,Toshiya Namikawa,H. T. Nguyen,Roger O'Brient,IV R.W.Ogburn,S. Palladino,Matthew Petroff,T. Prouve,C. Pryke,B. Racine,Carl D. Reintsema,S. Richter,Alessandro Schillaci,Benjamin L. Schmitt,R. Schwarz,C. D. Sheehy,Baibhav Singari,Ahmed Soliman,T. St. Germaine,Bryan Steinbach,R. V. Sudiwala,Grant Teply,K. L. Thompson,J. E. Tolan,Carole Tucker,A. D. Turner,C. Umilta,Clara Vergès,Abigail G. Vieregg,A. Wandui,A. C. Weber,D. V. Wiebe,J. Willmert,Chi Lam Wong,W. L. K. Wu,H. Yang,Ki Won Yoon,Edward D. Young,Lingzhen Zeng,C. Zhang,S. University,Kipacslac,U British Columbia,HarvardCfA,Caltech,U. Cincinnati,S. University,Nasa Jpl,M. I. O. Astrophysics,Universityof Chicago,U Minnesota,Nist,S. Grenoble,U. O. I. Urbana-Champaign,Harvard University,T. U. O. Tokyo,Aix-Marseille Universite,B. N. Laboratory +109 more
TL;DR: In this paper , the Bicep/Keck data were used to constrain the tensor-to-scalar ratio of the BK18 data to 0. 009.
Proceedings ArticleDOI
Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz
Ahmed Soliman,P. A. R. Ade,Z. Ahmed,Randol W. Aikin,Kate D. Alexander,Denis Barkats,S. J. Benton,Colin A. Bischoff,J. J. Bock,J. J. Bock,R. Bowens-Rubin,Justus A. Brevik,I. Buder,E. Bullock,Victor Buza,Jake Connors,J. Cornelison,B. P. Crill,M. Crumrine,Marion Dierickx,Lionel Duband,Cora Dvorkin,Jeffrey P. Filippini,S. Fliescher,J. A. Grayson,G. Hall,Mark Halpern,Sarah M. Harrison,S. R. Hildebrandt,S. R. Hildebrandt,Gene C. Hilton,Howard Hui,Kent D. Irwin,Kent D. Irwin,J. Kang,Kirit Karkare,Kirit Karkare,E. Karpel,J. P. Kaufman,Brian Keating,S. Kefeli,S. A. Kernasovskiy,John M Kovac,C. L. Kuo,Kei May Lau,N. A. Larsen,E. M. Leitch,M. Lueker,K. G. Megerian,Lorenzo Moncelsi,Toshiya Namikawa,Calvin B. Netterfield,Calvin B. Netterfield,H. T. Nguyen,Roger O'Brient,Roger O'Brient,R. W. Ogburn,S. Palladino,C. Pryke,B. Racine,S. Richter,R. Schwarz,Alessandro Schillaci,C. D. Sheehy,T. St. Germaine,Z. K. Staniszewski,Z. K. Staniszewski,Bryan Steinbach,R. V. Sudiwala,Grant Teply,Grant Teply,K. L. Thompson,J. E. Tolan,Carole Tucker,A. D. Turner,C. Umilta,J.J. van Zyl,Abigail G. Vieregg,A. Wandui,A. C. Weber,D. V. Wiebe,J. Willmert,C. L. Wong,W. L. K. Wu,Eui-Hyeok Yang,K. W. Yoon,C. Zhang +86 more
TL;DR: The BICEP Array is a degree-scale cosmic microwave background (CMB) experiment that will search for primordial B-mode polarization while constraining Galactic foregrounds.
Posted Content
Optimal CMB Lensing Reconstruction and Parameter Estimation with SPTpol Data
M. Millea,C. Daley,T.-L. Chou,Ethan Anderes,P. A. R. Ade,Adam Anderson,J. E. Austermann,Jessica Avva,J. A. Beall,Andreas Bender,Bradford Benson,Federico Bianchini,Lindsey Bleem,John E. Carlstrom,C. L. Chang,P. Chaubal,H. C. Chiang,Robert I. Citron,C. Corbett Moran,T. M. Crawford,A. T. Crites,T. de Haan,M. A. Dobbs,W. B. Everett,Jason Gallicchio,Elizabeth George,Neil Goeckner-Wald,S. Guns,Nikhel Gupta,N. W. Halverson,Jason W. Henning,Gene C. Hilton,Gilbert Holder,W. L. Holzapfel,J. D. Hrubes,N. Huang,J. Hubmayr,Kent D. Irwin,Lloyd Knox,A. T. Lee,Dale Li,A. Lowitz,Jeff McMahon,S. S. Meyer,L. M. Mocanu,Joshua Montgomery,T. Natoli,John P. Nibarger,G. I. Noble,V. Novosad,Y. Omori,S. Padin,S. Patil,C. Pryke,Christian L. Reichardt,J. E. Ruhl,Benjamin Saliwanchik,K. K. Schaffer,C. Sievers,Graeme Smecher,A. A. Stark,B. Thorne,C. Tucker,Todd J. Veach,J. D. Vieira,Gensheng Wang,Nathan Whitehorn,W. L. K. Wu,V. G. Yefremenko +68 more
TL;DR: In this article, the first simultaneous Bayesian parameter inference and optimal reconstruction of the gravitational lensing of the cosmic microwave background (CMB), using 100 deg$^2$ of polarization observations from the SPT-pol receiver on the South Pole Telescope, was performed.
Journal ArticleDOI
Design and Performance of the First BICEP Array Receiver
Alessandro Schillaci,Peter A. R. Ade,Zeeshan Ahmed,Mandana Amiri,Denis Barkats,R. Basu Thakur,Colin A. Bischoff,James J. Bock,H. Boenish,E. Bullock,Victor Buza,J. Cheshire,Jake Connors,J. Cornelison,M. Crumrine,A. Cukierman,Marion Dierickx,Lionel Duband,S. Fatigoni,Jeffrey P. Filippini,G. Hall,Mark Halpern,Sarah M. Harrison,S. Henderson,Sergi R. Hildebrandt,Gene C. Hilton,Howard Hui,Kent D. Irwin,J. Kang,Kirit Karkare,E. Karpel,S. Kefeli,John M Kovac,Chao-Lin Kuo,King Tong Lau,K. G. Megerian,Lorenzo Moncelsi,Toshiya Namikawa,H. T. Nguyen,Roger O'Brient,S. Palladino,N. Precup,T. Prouvé,C. Pryke,B. Racine,Carl D. Reintsema,S. Richter,Benjamin L. Schmitt,R. Schwarz,C. D. Sheehy,Ahmed Soliman,T. St. Germaine,Bryan Steinbach,Rashmikant V. Sudiwala,Keith L. Thompson,Carole Tucker,Anthony D. Turner,C. Umiltà,Abigail G. Vieregg,A. Wandui,A. C. Weber,Donald V. Wiebe,J. Willmert,W. L. K. Wu,Eui-Hyeok Yang,Ki Won Yoon,Edward D. Young,Che-Hang Yu,Chao Zhang +68 more
TL;DR: The BICEP/Keck (BK) experiment targets this primordial signature, the amplitude of which is parameterized by the tensor-to-scalar ratio r, by observing the polarized microwave sky through the exceptionally clean and stable atmosphere at the South Pole as discussed by the authors.