P
Peter A. R. Ade
Researcher at Cardiff University
Publications - 1402
Citations - 147299
Peter A. R. Ade is an academic researcher from Cardiff University. The author has contributed to research in topics: Cosmic microwave background & Telescope. The author has an hindex of 162, co-authored 1387 publications receiving 138051 citations. Previous affiliations of Peter A. R. Ade include Queen Mary's College & Max Planck Society.
Papers
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Proceedings ArticleDOI
BICEP3 focal plane design and detector performance
Howard Hui,Peter A. R. Ade,Zeeshan Ahmed,Kate D. Alexander,Mandana Amiri,Denis Barkats,Steven J. Benton,Steven J. Benton,Colin A. Bischoff,James J. Bock,H. Boenish,R. Bowens-Rubin,I. Buder,E. Bullock,Victor Buza,Jake Connors,Jeffrey P. Filippini,S. Fliescher,J. A. Grayson,Mark Halpern,Sarah M. Harrison,Gene C. Hilton,Viktor Hristov,Kent D. Irwin,Kent D. Irwin,J. Kang,Kirit Karkare,E. Karpel,S. Kefeli,S. A. Kernasovskiy,John M Kovac,Chao-Lin Kuo,E. M. Leitch,M. Lueker,K. G. Megerian,V. Monticue,Toshiya Namikawa,Calvin B. Netterfield,Calvin B. Netterfield,H. T. Nguyen,Roger O'Brient,R. W. Ogburn,C. Pryke,Carl D. Reintsema,S. Richter,R. Schwarz,C. Sorensen,C. D. Sheehy,Z. K. Staniszewski,Bryan Steinbach,G. P. Teply,G. P. Teply,Keith L. Thompson,J. E. Tolan,Carole Tucker,Anthony D. Turner,Abigail G. Vieregg,A. Wandui,A. C. Weber,Donald V. Wiebe,J. Willmert,W. L. K. Wu,W. L. K. Wu,Ki Won Yoon +63 more
TL;DR: In this article, the authors show the focal plane design and detector performance of BICEP3, including spectral response, optical efficiency, and preliminary sensitivity of the upgraded BiceP3 receiver.
Journal ArticleDOI
Fabrication of Detector Arrays for the SPT-3G Receiver
C. M. Posada,Peter A. R. Ade,Zeeshan Ahmed,Zeeshan Ahmed,Adam Anderson,Adam Anderson,Jason E. Austermann,Jessica Avva,R. Basu Thakur,Amy N. Bender,Amy N. Bender,Bradford Benson,Bradford Benson,John E. Carlstrom,Faustin Carter,Faustin Carter,Thomas Cecil,Chihway Chang,Chihway Chang,J. F. Cliche,A. Cukierman,E. V. Denison,T. de Haan,Junjia Ding,Ralu Divan,M. A. Dobbs,M. A. Dobbs,D. Dutcher,W. B. Everett,A. Foster,R. N. Gannon,A. J. Gilbert,John Groh,N. W. Halverson,A. H. Harke-Hosemann,A. H. Harke-Hosemann,N. L. Harrington,Jason W. Henning,Gene C. Hilton,W. L. Holzapfel,N. Huang,Kent D. Irwin,Kent D. Irwin,Oliver Jeong,M. Jonas,Trupti Khaire,A. M. Kofman,M. Korman,Donna Kubik,S. E. Kuhlmann,C. L. Kuo,C. L. Kuo,Aaron Lee,Aaron Lee,A. E. Lowitz,S. S. Meyer,Daniel Michalik,C. S. Miller,Joshua Montgomery,Andrew Nadolski,T. Natoli,H. Nguyen,G. I. Noble,Valentine Novosad,Stephen Padin,Z. Pan,John E. Pearson,Alexandra S. Rahlin,Alexandra S. Rahlin,J. E. Ruhl,L. J. Saunders,L. J. Saunders,J. T. Sayre,I. Shirley,Erik Shirokoff,Graeme Smecher,J. A. Sobrin,Liliana Stan,A. A. Stark,K. T. Story,Aritoki Suzuki,Aritoki Suzuki,Q. Y. Tang,K. L. Thompson,K. L. Thompson,Carole Tucker,Leila R. Vale,K. Vanderlinde,Joaquin Vieira,Gensheng Wang,Nathan Whitehorn,Nathan Whitehorn,V. G. Yefremenko,K. W. Yoon,K. W. Yoon,M. R. Young +95 more
TL;DR: The South Pole Telescope third-generation (SPT-3G) receiver was installed during the austral summer of 2016-2017 as mentioned in this paper, which is designed to measure the cosmic microwave background across three frequency bands centered at 95, 150, and 220 GHz.
Proceedings ArticleDOI
Attitude determination for balloon-borne experiments
Natalie N. Gandilo,Peter A. R. Ade,Mandana Amiri,Francesco E. Angilè,S. J. Benton,James J. Bock,John Bond,John Bond,Sean Bryan,H. C. Chiang,Carlo R. Contaldi,B. P. Crill,Mark J. Devlin,Bradley Dober,O. Doré,Marzieh Farhang,Jeffrey P. Filippini,Laura M. Fissel,Laura M. Fissel,A. A. Fraisse,Yasuo Fukui,Nicholas Galitzki,A. E. Gambrel,Sunil Golwala,Jon E. Gudmundsson,Mark Halpern,Mark Halpern,Matthew Hasselfield,Gene C. Hilton,W. Holmes,Viktor Hristov,Kent D. Irwin,Kent D. Irwin,W. C. Jones,Zigmund Kermish,Jeff Klein,A. L. Korotkov,Chao-Lin Kuo,C. J. MacTavish,P. V. Mason,Tristan G. Matthews,K. G. Megerian,Lorenzo Moncelsi,T. A. Morford,Tony Mroczkowski,Johanna Nagy,Calvin B. Netterfield,Calvin B. Netterfield,Giles Novak,D. Nutter,Roger O'Brient,Enzo Pascale,Frédérick Poidevin,Frédérick Poidevin,Alexandra S. Rahlin,Carl D. Reintsema,J. E. Ruhl,Marcus Runyan,Giorgio Savini,Douglas Scott,Jamil A. Shariff,Juan D. Soler,Juan D. Soler,Nicholas Thomas,Amy Trangsrud,Matthew D. P. Truch,Carole Tucker,Gregory S. Tucker,R. S. Tucker,Anthony D. Turner,Derek Ward-Thompson,A. C. Weber,Donald V. Wiebe,E. Y. Young +73 more
TL;DR: In this article, an attitude determination system for balloon-borne experiments is presented, which provides pointing information in azimuth and elevation for instruments flying on stratospheric balloons over Antarctica.
Posted Content
The Origin of the Universe as Revealed Through the Polarization of the Cosmic Microwave Background
Scott Dodelson,Richard Easther,Shaul Hanany,Liam McAllister,S. S. Meyer,L. A. Page,Peter A. R. Ade,A. Amblard,Amjad Ashoorioon,C. Baccigalupi,Amedeo Balbi,James G. Bartlett,Nicola Bartolo,Daniel Baumann,Maria T. Beltrán,Dominic Benford,Mark Birkinshaw,J. J. Bock,Dick Bond,J. Borrill,F. Bouchet,M. Bridges,E. Bunn,Erminia Calabrese,Christopher Cantalupo,A. Caramete,Carmelita Carbone,Sean M. Carroll,Suchetana Chatterjee,X. Chen,Sarah E. Church,David T. Chuss,Carlo R. Contaldi,Asantha Cooray,Paolo Creminelli,Sudeep Das,F. De Bernardis,P. de Bernardis,J. Delabrouille,F.-X. Désert,M. J. Devlin,Clive Dickinson,Simon Dicker,M. DiPirro,M. A. Dobbs,O. Doré,Jessie L. Dotson,Jo Dunkley,Cora Dvorkin,H. K. Eriksen,M. Cristina Falvella,D. Finley,D. P. Finkbeiner,D. J. Fixsen,Raphael Flauger,P. Fosalba,Joseph W. Fowler,Silvia Galli,Evalyn Gates,Walter Kieran Gear,Y. Giraud-Héraud,K. M. Górski,B. Greene,A. Gruppuso +63 more
TL;DR: In this article, the authors focus on the pattern of polarization in the Cosmic Microwave Background (CMB), which is uniquely sensitive to primordial gravity waves and propose a method to map CMB polarization over the next decade.
Journal ArticleDOI
Submillimeter Polarization Spectrum in the Vela C Molecular Cloud
Natalie N. Gandilo,Natalie N. Gandilo,Peter A. R. Ade,Francesco E. Angilè,Peter Ashton,Steven J. Benton,Steven J. Benton,Mark J. Devlin,Bradley Dober,Laura M. Fissel,Yasuo Fukui,Nicholas Galitzki,Jeff Klein,Andrei Korotkov,Zhi-Yun Li,Peter G. Martin,Tristan G. Matthews,Lorenzo Moncelsi,Fumitaka Nakamura,Calvin B. Netterfield,Calvin B. Netterfield,Giles Novak,Enzo Pascale,Frédérick Poidevin,Frédérick Poidevin,Fabio P. Santos,Giorgio Savini,Douglas Scott,Jamil A. Shariff,Jamil A. Shariff,Juan D. Soler,Nicholas Thomas,Carole Tucker,Gregory S. Tucker,Derek Ward-Thompson +34 more
TL;DR: Polarization maps of the Vela C molecular cloud were obtained at 250, 350, and 500um during the 2012 flight of the balloon-borne telescope BLASTPol.