W
William F. Grainger
Researcher at Rutherford Appleton Laboratory
Publications - 74
Citations - 2833
William F. Grainger is an academic researcher from Rutherford Appleton Laboratory. The author has contributed to research in topics: Cosmic microwave background & Polarization (waves). The author has an hindex of 24, co-authored 74 publications receiving 2703 citations. Previous affiliations of William F. Grainger include Science and Technology Facilities Council & Cardiff University.
Papers
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Journal ArticleDOI
A Measurement of the Cosmic Microwave Background B-Mode Polarization Power Spectrum at Sub-Degree Scales with POLARBEAR
P. A. R. Ade,Y. Akiba,A. E. Anthony,Kam Arnold,M. Atlas,Darcy Barron,D. Boettger,Julian Borrill,Scott Chapman,Yuji Chinone,M. A. Dobbs,Tucker Elleflot,Josquin Errard,Giulio Fabbian,Chang Feng,Daniel Flanigan,A. J. Gilbert,William F. Grainger,N. W. Halverson,Masaya Hasegawa,Kaori Hattori,Masashi Hazumi,W. L. Holzapfel,Y. Hori,Jonathon Howard,P. Hyland,Yuki Inoue,G. Jaehnig,Andrew H. Jaffe,Brian Keating,Zigmund Kermish,R. Keskitalo,Theodore Kisner,M. Le Jeune,Adrian T. Lee,E. M. Leitch,Eric V. Linder,Marius Lungu,Frederick Matsuda,Tomotake Matsumura,X. Meng,Nathan Miller,H. Morii,S. Moyerman,M. J. Myers,M. Navaroli,H. Nishino,Hans P. Paar,J. Peloton,D. Poletti,E. Quealy,Gabriel M. Rebeiz,Christian L. Reichardt,Paul L. Richards,Colin Ross,I. Schanning,D. E. Schenck,B. D. Sherwin,A. Shimizu,Chase Owen Shimmin,Meir Shimon,Praween Siritanasak,Graeme Smecher,Helmuth Spieler,Nathan Stebor,Bryan Steinbach,R. Stompor,Aritoki Suzuki,S. Takakura,Takayuki Tomaru,B. Wilson,Amit Yadav,Oliver Zahn +72 more
TL;DR: In this article, a measurement of the B-mode polarization power spectrum in the cosmic microwave background (CMB) using the POLARBEAR experiment in Chile is reported, including both systematic and statistical uncertainties.
Journal ArticleDOI
A measurement of the cosmic microwave background b-mode polarization power spectrum at sub-degree scales with polarbear
Y. Akiba,A. E. Anthony,Kam Arnold,M. Atlas,Darcy Barron,D. Boettger,Julian Borrill,Julian Borrill,Scott Chapman,Yuji Chinone,Yuji Chinone,M. A. Dobbs,Tucker Elleflot,Josquin Errard,Josquin Errard,Giulio Fabbian,Giulio Fabbian,Chang Feng,Daniel Flanigan,Daniel Flanigan,A. J. Gilbert,William F. Grainger,N. W. Halverson,Masaya Hasegawa,Masaya Hasegawa,Kaori Hattori,Masashi Hazumi,Masashi Hazumi,Masashi Hazumi,W. L. Holzapfel,Y. Hori,J. Howard,J. Howard,P. Hyland,Yuki Inoue,G. Jaehnig,Andrew H. Jaffe,Brian Keating,Zigmund Kermish,Reijo Keskitalo,Theodore Kisner,Theodore Kisner,M. Le Jeune,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,Eric V. Linder,Marius Lungu,Marius Lungu,Frederick Matsuda,Tomotake Matsumura,X. Meng,Nathan J. Miller,H. Morii,S. Moyerman,M. J. Myers,M. Navaroli,H. Nishino,A. Orlando,Hans P. Paar,J. Peloton,D. Poletti,E. Quealy,E. Quealy,Gabriel M. Rebeiz,Christian L. Reichardt,Paul L. Richards,Colin Ross,I. Schanning,D. E. Schenck,Blake D. Sherwin,A. Shimizu,Chase Owen Shimmin,Chase Owen Shimmin,Meir Shimon,Meir Shimon,Praween Siritanasak,Graeme Smecher,Helmuth Spieler,Nathan Stebor,Bryan Steinbach,Radek Stompor,Aritoki Suzuki,S. Takakura,S. Takakura,Takayuki Tomaru,B. Wilson,Amit P. S. Yadav,Oliver Zahn +88 more
TL;DR: In this paper, a measurement of the B-mode polarization power spectrum in the cosmic microwave background (CMB) using the POLARBEAR experiment in Chile is reported, which is based on observations of an effective sky area of 25? with 3.'5 resolution at 150?GHz.
Journal ArticleDOI
The Arcminute Microkelvin Imager
Jonathan T. L. Zwart,R. W. Barker,P. Biddulph,D. Bly,Roger C. Boysen,A. R. Brown,C. Clementson,M. Crofts,T. Culverhouse,J. Czeres,Roger Dace,M. L. Davies,R. D'Alessandro,P. Doherty,K. Duggan,John Ely,M. Felvus,Farhan Feroz,W. Flynn,Thomas M. O. Franzen,J. Geisbüsch,Ricardo Génova-Santos,Keith Grainge,William F. Grainger,D. Hammett,Richard Hills,Michael P. Hobson,C. M. Holler,Natasha Hurley-Walker,R. Jilley,M. Jones,T. Kaneko,Rüdiger Kneissl,Katy Lancaster,Anthony Lasenby,Phil Marshall,F. Newton,O. Norris,I. Northrop,D. M. Odell,G. Petencin,Jonathan C. Pober,Guy G. Pooley,Marian Pospieszalski,V. Quy,Carmen Rodríguez-Gonzálvez,Richard D. E. Saunders,Anna M. M. Scaife,J. Schofield,Paul F. Scott,C. Shaw,Timothy W. Shimwell,H. Smith,Angela C. Taylor,David Titterington,M. Velić,E. M. Waldram,S. West,B. A. Wood,Ghassan Yassin +59 more
TL;DR: The Arcminute Microkelvin Imager as discussed by the authors is a pair of interferometer arrays operating with six frequency channels spanning 13.9-18.2 GHz for observations on angular scales of 30 arcsec-10 arcmin and for declinations greater than 15°.
Journal ArticleDOI
Measurement of the Cosmic Microwave Background Polarization Lensing Power Spectrum with the POLARBEAR Experiment
Peter A. R. Ade,Y. Akiba,A. E. Anthony,Kam Arnold,M. Atlas,Darcy Barron,D. Boettger,Julian Borrill,Scott Chapman,Yuji Chinone,M. A. Dobbs,Tucker Elleflot,Josquin Errard,Giulio Fabbian,Chang Feng,Daniel Flanigan,A. J. Gilbert,William F. Grainger,N. W. Halverson,Masaya Hasegawa,Kaori Hattori,Masashi Hazumi,W. L. Holzapfel,Y. Hori,Jonathon Howard,P. Hyland,Yuki Inoue,G. Jaehnig,Andrew H. Jaffe,Brian Keating,Zigmund Kermish,Reijo Keskitalo,Theodore Kisner,M. Le Jeune,Adrian T. Lee,Eric V. Linder,E. M. Leitch,Marius Lungu,Frederick Matsuda,Tomotake Matsumura,X. Meng,Nathan J. Miller,H. Morii,S. Moyerman,M. J. Myers,M. Navaroli,H. Nishino,Hans P. Paar,J. Peloton,E. Quealy,Gabriel M. Rebeiz,Christian L. Reichardt,Paul L. Richards,Colin Ross,I. Schanning,D. E. Schenck,Blake D. Sherwin,Atsushi Shimizu,Chase Owen Shimmin,Meir Shimon,Praween Siritanasak,Graeme Smecher,Helmuth Spieler,Nathan Stebor,Bryan Steinbach,R. Stompor,Aritoki Suzuki,S. Takakura,Takayuki Tomaru,B. Wilson,Amit P. S. Yadav,Oliver Zahn +71 more
TL;DR: The first direct evidence for polarization lensing based on purely CMB information is reported, from using the four-point correlations of even- and odd-parity E- and B-mode polarization mapped over ∼30 square degrees of the sky measured by the POLARBEAR experiment.
Journal ArticleDOI
The Arcminute Microkelvin Imager
Jonathan T. L. Zwart,R. W. Barker,P. Biddulph,D. Bly,Roger C. Boysen,A. R. Brown,C. Clementson,M. Crofts,T. Culverhouse,J. Czeres,Roger Dace,M. L. Davies,R. D'Alessandro,P. Doherty,K. Duggan,John Ely,M. Felvus,Farhan Feroz,W. Flynn,T. M. O. Franzen,J. Geisbüsch,Ricardo Génova-Santos,Keith Grainge,William F. Grainger,D. Hammett,Richard Hills,Michael P. Hobson,C. M. Holler,Natasha Hurley-Walker,R. Jilley,M. Jones,T. Kaneko,R. Kneissl,Katy Lancaster,Anthony Lasenby,Philip J. Marshall,F. Newton,O. Norris,I. Northrop,D. M. Odell,Jonathan C. Pober,Guy G. Pooley,V. Quy,C. Rodriguez-Gonzalvez,Richard D. E. Saunders,Anna M. M. Scaife,J. Schofield,Paul F. Scott,C. Shaw,Timothy W. Shimwell,Harry Smith,Angela C. Taylor,David Titterington,M. Velić,E. M. Waldram,S. West,B. A. Wood,Ghassan Yassin +57 more
TL;DR: The Arcminute Microkelvin Imager as mentioned in this paper is a pair of interferometer arrays operating with six frequency channels spanning 13.9-18.2 GHz with very high sensitivity to angular scales 30''-10'.