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
More filters
Journal ArticleDOI
Improved Constraints on Cosmology and Foregrounds from BICEP2 and Keck Array Cosmic Microwave Background Data with Inclusion of 95 GHz Band
Peter A. R. Ade,Zeeshan Ahmed,Randol W. Aikin,Kate D. Alexander,Denis Barkats,S. J. Benton,Colin A. Bischoff,J. J. Bock,R. Bowens-Rubin,Justus A. Brevik,I. Buder,E. Bullock,Victor Buza,Jake Connors,B. P. Crill,L. Duband,Cora Dvorkin,Jeffrey P. Filippini,S. Fliescher,J. A. Grayson,Mark Halpern,Sarah M. Harrison,Gene C. Hilton,Howard Hui,Kent D. Irwin,Kirit Karkare,E. Karpel,J. P. Kaufman,Brian Keating,S. Kefeli,S. A. Kernasovskiy,John M Kovac,Chao-Lin Kuo,E. M. Leitch,M. Lueker,K. G. Megerian,Calvin B. Netterfield,H. T. Nguyen,Roger O'Brient,R. W. Ogburn,A. Orlando,C. Pryke,S. Richter,R. Schwarz,C. D. Sheehy,Z. K. Staniszewski,Bryan Steinbach,R. V. Sudiwala,Grant Teply,K. L. Thompson,J. E. Tolan,Carole Tucker,A. D. Turner,Abigail G. Vieregg,A. C. Weber,D. V. Wiebe,J. Willmert,C. L. Wong,W. L. K. Wu,Ki Won Yoon +59 more
TL;DR: An analysis of all data taken by the BICEP2 and Keck Array cosmic microwave background (CMB) polarization experiments up to and including the 2014 observing season yields an upper limit r_{0.05}<0.09 at 95% confidence, which is robust to variations explored in analysis and priors.
Journal ArticleDOI
Constraints on Primordial Gravitational Waves Using Planck, WMAP, and New BICEP2/Keck Observations through the 2015 Season.
Peter A. R. Ade,Z. Ahmed,Randol W. Aikin,Kate D. Alexander,Denis Barkats,Steven 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,L. 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,E. Karpel,J. P. Kaufman,Brian Keating,S. Kefeli,S. A. Kernasovskiy,John M Kovac,Chao-Lin Kuo,N. A. Larsen,King Tong Lau,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,Stefan Richter,Alessandro Schillaci,R. Schwarz,C. D. Sheehy,Ahmed Soliman,T. St. Germaine,Z. K. Staniszewski,Z. K. Staniszewski,Bryan Steinbach,R. V. Sudiwala,Grant Teply,Grant Teply,K. L. Thompson,J. E. Tolan,C. Tucker,A. D. Turner,C. Umilta,Abigail G. Vieregg,A. Wandui,A. C. Weber,D. V. Wiebe,J. Willmert,C. L. Wong,W. L. K. Wu,Hyunsoo Yang,Ki Won Yoon,Chao Zhang +84 more
TL;DR: Results from an analysis of all data taken by the bicep2/Keck CMB polarization experiments up to and including the 2015 observing season are presented, showing the strongest constraints to date on primordial gravitational waves.
Book
Inflation Physics from the Cosmic Microwave Background and Large Scale Structure.
K. N. Abazajian,Kam Arnold,Jason E. Austermann,Bradford Benson,Colin A. Bischoff,J. Bock,J. R. Bond,J. Borrill,I. Buder,D. L. Burke,Erminia Calabrese,John E. Carlstrom,C. S. Carvalho,C. L. Chang,H. C. Chiang,S. Church,Asantha Cooray,T. M. Crawford,B. P. Crill,Kyle S. Dawson,S. Das,M. J. Devlin,M. Dobbs,Scott Dodelson,O. Doré,Joanna Dunkley,Jonathan L. Feng,A. Fraisse,Jason Gallicchio,Steven B. Giddings,D. Green,N. W. Halverson,S. Hanany,D. Hanson,S. R. Hildebrandt,A. Hincks,R. Hlozek,Gilbert Holder,W. L. Holzapfel,K. Honscheid,G. Horowitz,Wayne Hu,Johannes Hubmayr,K. Irwin,M. Jackson,W. C. Jones,R. Kallosh,Marc Kamionkowski,Brian Keating,Ryan Keisler,William H. Kinney,Lloyd Knox,Eiichiro Komatsu,John M Kovac,Chao-Lin Kuo,Akito Kusaka,C. Lawrence,A. T. Lee,E. M. Leitch,A. Linde,Eric V. Linder,P. Lubin,J. Maldacena,Emil J. Martinec,Jeff McMahon,Amber Miller,Viatcheslav Mukhanov,Laura Newburgh,M. D. Niemack,H. Nguyen,H. T. Nguyen,L. A. Page,C. Pryke,Christian L. Reichardt,J. E. Ruhl,N. Sehgal,U. Seljak,Leonardo Senatore,Jon Sievers,Eva Silverstein,A. Slosar,Kendrick M. Smith,David N. Spergel,Suzanne T. Staggs,Antony A. Stark,R. Stompor,Abigail G. Vieregg,G. Wang,Scott Watson,Edward J. Wollack,W. L. K. Wu,Ki Won Yoon,O. Zahn,M. Zaldarriaga +93 more
TL;DR: For example, a future CMB and large-scale structure (LSS) experiments are poised to test the leading paradigm for these earliest moments and to detect the imprints of the inflationary epoch, thereby dramatically increasing our understanding of fundamental physics and the early universe.
Journal ArticleDOI
Dark Energy Survey year 1 results: a precise H0 estimate from DES Y1, BAO, and D/H data
T. M. C. Abbott,F. B. Abdalla,F. B. Abdalla,J. Annis,Keith Bechtol,Jonathan Blazek,Jonathan Blazek,Bradford Benson,Bradford Benson,R. A. Bernstein,Gary Bernstein,E. Bertin,David J. Brooks,D. L. Burke,D. L. Burke,A. Carnero Rosell,M. Carrasco Kind,M. Carrasco Kind,J. Carretero,F. J. Castander,Chihway Chang,Chihway Chang,T. M. Crawford,Carlos E. Cunha,C. B. D'Andrea,L. N. da Costa,C. Davis,J. DeRose,Shantanu Desai,H. T. Diehl,J. P. Dietrich,Peter Doel,Alex Drlica-Wagner,August E. Evrard,Enrique J. Fernández,B. Flaugher,Pablo Fosalba,Joshua A. Frieman,Joshua A. Frieman,Juan Garcia-Bellido,Enrique Gaztanaga,D. W. Gerdes,Tommaso Giannantonio,Tommaso Giannantonio,Daniel Gruen,Daniel Gruen,Robert A. Gruendl,Robert A. Gruendl,J. Gschwend,G. Gutierrez,W. G. Hartley,W. G. Hartley,Jason W. Henning,K. Honscheid,Ben Hoyle,Ben Hoyle,Dragan Huterer,Bhuvnesh Jain,David J. James,Matt J. Jarvis,Tesla E. Jeltema,M. D. Johnson,Marvin Johnson,Elisabeth Krause,Kyler Kuehn,S. E. Kuhlmann,N. Kuropatkin,Ofer Lahav,Andrew R. Liddle,Marcos Lima,Huan Lin,Niall MacCrann,M. A. G. Maia,A. Manzotti,M. March,Jennifer L. Marshall,Ramon Miquel,Ramon Miquel,Joseph J. Mohr,Joseph J. Mohr,T. Natoli,Peter Nugent,Ricardo L. C. Ogando,Youngsoo Park,A. A. Plazas,Christian L. Reichardt,Kevin Reil,A. Roodman,A. Roodman,Ashley J. Ross,Eduardo Rozo,Eli S. Rykoff,Eli S. Rykoff,E. J. Sanchez,V. Scarpine,Michael Schubnell,Daniel Scolnic,I. Sevilla-Noarbe,Erin Sheldon,Mathew Smith,R. C. Smith,Marcelle Soares-Santos,Flavia Sobreira,E. Suchyta,G. Tarle,Daniel Thomas,Michael Troxel,Alistair R. Walker,Risa H. Wechsler,Risa H. Wechsler,Jochen Weller,Jochen Weller,W. C. Wester,W. L. K. Wu,Joe Zuntz +114 more
TL;DR: In this article, the authors combine Dark Energy Survey Year 1 clustering and weak lensing data with baryon acoustic oscillations and Big Bang nucleosynthesis experiments to constrain the Hubble constant.
Journal ArticleDOI
Measurements of the temperature and E-mode polarization of the CMB from 500 square degrees of SPTpol data
Jason W. Henning,J. T. Sayre,Christian L. Reichardt,Peter A. R. Ade,Adam Anderson,Jason E. Austermann,James A. Beall,Amy N. Bender,Amy N. Bender,Bradford Benson,Bradford Benson,Lindsey Bleem,Lindsey Bleem,John E. Carlstrom,C. L. Chang,C. L. Chang,H. C. Chiang,H-M. Cho,Robert I. Citron,C. Corbett Moran,T. M. Crawford,A. T. Crites,A. T. Crites,T. de Haan,Matt Dobbs,Matt Dobbs,W. B. Everett,Jason Gallicchio,Jason Gallicchio,Elizabeth George,Elizabeth George,A. J. Gilbert,N. W. Halverson,N. L. Harrington,Gene C. Hilton,Gilbert Holder,Gilbert Holder,W. L. Holzapfel,S. Hoover,Zhen Hou,J. D. Hrubes,N. Huang,Johannes Hubmayr,Kent D. Irwin,Ryan Keisler,Lloyd Knox,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,Dale Li,Dale Li,A. E. Lowitz,A. Manzotti,Jeff McMahon,S. S. Meyer,L. M. Mocanu,Joshua Montgomery,Joshua Montgomery,Andrew Nadolski,T. Natoli,John P. Nibarger,V. Novosad,Stephen Padin,Stephen Padin,C. Pryke,J. E. Ruhl,Benjamin Saliwanchik,K. K. Schaffer,K. K. Schaffer,C. Sievers,Graeme Smecher,Antony A. Stark,K. T. Story,Carole Tucker,K. Vanderlinde,T. Veach,Joaquin Vieira,Gensheng Wang,Nathan Whitehorn,Nathan Whitehorn,W. L. K. Wu,Volodymyr Yefremenko +81 more
TL;DR: Henning et al. as discussed by the authors measured the E-mode polarization angular power spectrum (EE) and temperature-E-mode cross-power spectrum (TE) of the cosmic microwave background (CMB) using 150 GHz data from three seasons of SPTpol observations.