K
K. L. Thompson
Researcher at Stanford University
Publications - 146
Citations - 8444
K. L. Thompson is an academic researcher from Stanford University. The author has contributed to research in topics: Cosmic microwave background & Telescope. The author has an hindex of 42, co-authored 116 publications receiving 7371 citations. Previous affiliations of K. L. Thompson include California Institute of Technology & SLAC National Accelerator Laboratory.
Papers
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Searching for axion-like time-dependent cosmic birefringence with SPT-3G Probing axionlike
K. R. Ferguson,A. Jay Anderson,Nathan Whitehorn,P. A. R. Ade,M. Archipley,Jessica Avva,L. Balkenhol,K. Benabed,Amy N. Bender,Bradford Benson,Federico Bianchini,Lindsey Bleem,François R. Bouchet,E. Camphuis,John E. Carlstrom,Thomas Cecil,C. L. Chang,P. Chaubal,Paul M. Chichura,T.-L. Chou,T. M. Crawford,Ari Cukierman,Cail Daley,T. de Haan,K. Dibert,M. A. Dobbs,D. Dutcher,A. Everett,Chang Feng,A. Foster,S. Galli,A. E. Gambrel,Richard Wayne Gardner,Neil Goeckner-Wald,R. Gualtieri,S. Guns,N. W. Halverson,E. Hivon,Gilbert Holder,W. L. Holzapfel,J. Hood,N. Huang,Lloyd Knox,M. Korman,Chao-Lin Kuo,A. T. Lee,A. E. Lowitz,C. Lu,Marius Millea,Joshua Montgomery,T. Natoli,G. I. Noble,Valentyn Novosad,Y. Omori,Stephen Padin,Z. Pan,K. H. Prabhu,W. Quan,Alexandra S. Rahlin,Christian L. Reichardt,Maclean Rouble,J. E. Ruhl,E. Schiappucci,Graeme Smecher,J. A. Sobrin,A. Suzuki,Caterina Tandoi,K. L. Thompson,B. Thorne,Carole Tucker,C. Umilta,Joaquin Vieira,G. Wang,W. L. K. Wu,Volodymyr Yefremenko,M. R. Young +75 more
TL;DR: Observations of the cosmic microwave background from SPT-3G, the current receiver on the South Pole Telescope, are used to set upper limits on the value of the axion-photon coupling constant g φγ over the approximate mass range, corresponding to oscillation periods from 12 hours to 100 days.
Posted Content
BICEP / Keck XV: The BICEP3 CMB Polarimeter and the First Three Year Data Set
P. A. R. Ade,Z. Ahmed,M. Amiri,Denis Barkats,R. Basu Thakur,D. Beck,C. Bischoff,C. Bischoff,J. J. Bock,H. Boenish,E. Bullock,Victor Buza,J. R. Cheshire,Jake Connors,J. Cornelison,M. Crumrine,A. Cukierman,E. V. Denison,Marion Dierickx,L. Duband,M. Eiben,S. Fatigoni,Jeffrey P. Filippini,S. Fliescher,N. Goeckner-Wald,D. C. Goldfinger,J. Grayson,P. Grimes,G. Halal,G. Hall,Mark Halpern,E. Hand,Sarah M. Harrison,S. Henderson,S. Henderson,S. R. Hildebrandt,Gene C. Hilton,J. Hubmayr,H. Hui,H. Hui,Kent D. Irwin,Kent D. Irwin,J. Kang,J. Kang,K. S. Karkare,E. Karpel,S. Kefeli,S. A. Kernasovskiy,J. M. Kovac,Chao-Lin Kuo,K. Lau,E. M. Leitch,A. Lennox,K. G. Megerian,L. Minutolo,L. Moncelsi,Y. Nakato,T. Namikawa,H. T. Nguyen,H. T. Nguyen,R. O'Brient,R. W. Ogburn,S. Palladino,T. Prouve,C. Pryke,C. Pryke,B. Racine,C. D. Reintsema,S. Richter,A. Schillaci,B. L. Schmitt,R. Schwarz,C. D. Sheehy,A. Soliman,T. St. Germaine,B. Steinbach,R. V. Sudiwala,G. P. Teply,K. L. Thompson,J. E. Tolan,C. Tucker,A. Turner,A. Turner,C. Umilta,C. Verges,Abigail G. Vieregg,A. Wandui,A. C. Weber,D. V. Wiebe,J. Willmert,C. L. Wong,W. L. K. Wu,Haijun Yang,K. W. Yoon,E. Young,Che-Hang Yu,L. Zeng,Chao Zhang,Shengyu Zhang +98 more
TL;DR: The BICEP3 as discussed by the authors is a 52cm aperture, refracting telescope designed to observe the polarization of the cosmic microwave background (CMB) on degree angular scales at 95GHz.
Journal ArticleDOI
A non-isothermal approach to evaluate the impact of the cooling stage on the startup flow of waxy crude oils
TL;DR: In this article , the authors investigate how the cooling process after a shutdown impacts the flow assurance problem and show that higher values of Pl and higher waiting times in the cooling after the shutdown stage lead to conditions less prone to restart.
Proceedings ArticleDOI
Analysis of Carbopol And Triethanolamine Concentration in The Viscoplastic Properties of Aqueous Solution
Daiane Mieko Iceri,Jorge Luiz Biazussi,Charlie van der Geest,K. L. Thompson,Marcelo Souza de Castro +4 more
TL;DR: In this article , the authors measured the yield stress from flow curve tests, performed in a rheometer, were made for different combinations of Carbopol and Triethanolamine (neutralizing agent) concentrations.
Journal ArticleDOI
Tensor-to-scalar ratio forecasts for extended LiteBIRD frequency configurations
Unni Irene Fuskeland,J. Aumont,R. Aurlien,Carlo Baccigalupi,A. J. Banday,H. K. Eriksen,Josquin Errard,R. T. G'enova-Santos,T. Hasebe,Johannes Hubmayr,H. Imada,Nicoletta Krachmalnicoff,Luca Lamagna,Giampaolo Pisano,Davide Poletti,Mathieu Remazeilles,K. L. Thompson,L. Vacher,Ingunn Kathrine Wehus,S. Azzoni,Mario Ballardini,R. B. Barreiro,N. Bartolo,A. Y. Basyrov,D. Beck,Marco Bersanelli,Marco Bortolami,M. Brilenkov,Erminia Calabrese,Alessandro V Carones,F. J. Casas,K. Cheung,Jens Chluba,Susan E. Clark,Lionel Clermont,F. Columbro,Alessandro Coppolecchia,Giuseppe D'Alessandro,P. de Bernardis,T. de Haan,E. D. L. Hoz,Marco De Petris,S. Della Torre,P. Diego-Palazuelos,Fabio Finelli,Cristian Franceschet,G. Galloni,Matt Galloway,Martina Gerbino,Massimo Gervasi,T. Ghigna,Serena Giardiello,E. Gjerløw,Alessandro Gruppuso,P. Hargrave,M. Hattori,Masashi Hazumi,L. T. Hergt,Daniel Herman,D. Herranz,E. Hivon,Thuong D. Hoang,Kumiko Kohri,Massimiliano Lattanzi,A. T. Lee,Christophe Leloup,François Levrier,Anto. I. Lonappan,Gemma Luzzi,Bruno Maffei,E. Mart'inez-Gonz'alez,Silvia Masi,Sabino Matarrese,T. Matsumura,M. Migliaccio,L. Montier,Gianluca Morgante,B. Mot,L. Mousset,Ryo Nagata,Tadahiro Namikawa,Federico Nati,Paolo Natoli,S. Nerval,Antonella Novelli,L. Pagano,Alessandro Paiella,Daniela Paoletti,G. Pascual-Cisneros,G. Patanchon,Vincent Pelgrims,F. Piacentini,Giulia Piccirilli,G. Polenta,Giuseppe Puglisi,N. Raffuzzi,A. Ritacco,Jose Alberto Rubino-Martin,Giorgio Savini,Doran Scott,Yusuke Sekimoto,Maresuke Shiraishi,Giulia Signorelli,S. Stever,N. Stutzer,Raelyn M. Sullivan,S. Takakura,Luca Terenzi,H. Thommesen,M. Tristram,Masanobu Tsuji,P. Vielva,John Weller,Benjamin Westbrook,G. Weymann-Despres,Edward J. Wollack,Mario Zannoni +116 more
TL;DR: In this paper , the authors compare the baseline design with five extended configurations, while varying the underlying dust modeling, in each of which the HFT (High-Frequency Telescope) frequency range is shifted logarithmically towards higher frequencies, with an upper cutoff ranging between 400 and 600 GHz.