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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Journal ArticleDOI
Mass Calibration of Optically Selected des Clusters Using a Measurement of CMB-cluster Lensing with SPTpol Data
Srinivasan Raghunathan,Srinivasan Raghunathan,S. Patil,Eric J. Baxter,Bradford Benson,Bradford Benson,Lindsey Bleem,T. L. Chou,T. M. Crawford,Gilbert Holder,Gilbert Holder,T. McClintock,Christian L. Reichardt,Eduardo Rozo,T. N. Varga,T. N. Varga,T. M. C. Abbott,Peter A. R. Ade,S. Allam,Adam Anderson,J. Annis,Jason E. Austermann,Santiago Avila,J. A. Beall,K. Bechtol,Amy N. Bender,Gary Bernstein,E. Bertin,Federico Bianchini,David Brooks,D. L. Burke,John E. Carlstrom,John E. Carlstrom,J. Carretero,C. L. Chang,C. L. Chang,H. C. Chiang,H. M. Cho,Robert I. Citron,A. T. Crites,A. T. Crites,Carlos E. Cunha,L. N. da Costa,C. Davis,Shantanu Desai,H. T. Diehl,J. P. Dietrich,M. A. Dobbs,M. A. Dobbs,P. Doel,Tim Eifler,Tim Eifler,W. B. Everett,A. E. Evrard,B. Flaugher,Pablo Fosalba,Joshua A. Frieman,Jason Gallicchio,Juan Garcia-Bellido,Enrique Gaztanaga,Elizabeth George,Elizabeth George,A. J. Gilbert,Daniel Gruen,Robert A. Gruendl,J. Gschwend,Nikhel Gupta,G. Gutierrez,T. de Haan,T. de Haan,N. W. Halverson,N. L. Harrington,W. G. Hartley,W. G. Hartley,Jason W. Henning,Gene C. Hilton,D. L. Hollowood,W. L. Holzapfel,K. Honscheid,Z. Hou,Ben Hoyle,Ben Hoyle,J. D. Hrubes,N. Huang,Johannes Hubmayr,Kent D. Irwin,David J. James,Tesla E. Jeltema,A. G. Kim,M. Carrasco Kind,Lloyd Knox,Attila Kovács,Kyler Kuehn,N. Kuropatkin,Adrian T. Lee,Adrian T. Lee,Tenglin Li,Marcos Lima,M. A. G. Maia,Jennifer L. Marshall,Jeff McMahon,Peter Melchior,Felipe Menanteau,S. S. Meyer,C. J. Miller,Ramon Miquel,L. M. Mocanu,Joshua Montgomery,Andrew Nadolski,T. Natoli,T. Natoli,John P. Nibarger,Valentine Novosad,Stephen Padin,Stephen Padin,A. A. Plazas,C. Pryke,David Rapetti,David Rapetti,A. K. Romer,A. Carnero Rosell,J. E. Ruhl,Benjamin Saliwanchik,E. J. Sanchez,J. T. Sayre,V. Scarpine,K. K. Schaffer,K. K. Schaffer,Michael Schubnell,S. Serrano,I. Sevilla-Noarbe,Graeme Smecher,R. C. Smith,Marcelle Soares-Santos,Flavia Sobreira,Antony A. Stark,K. T. Story,E. Suchyta,M. E.C. Swanson,Gregory Tarle,Daniel Thomas,Carole Tucker,K. Vanderlinde,J. De Vicente,Joaquin Vieira,Gensheng Wang,Nathan Whitehorn,W. L. K. Wu,Yanxi Zhang +148 more
TL;DR: In this paper, a modified quadratic estimator designed to be unbiased by the thermal Sunyaev-Zel{'dovich (tSZ) effect was used to estimate the background CMB gradient.
Journal ArticleDOI
MAXIMA: A balloon-borne cosmic microwave background anisotropy experiment
Bahman Rabii,C. D. Winant,J. Collins,Aaron Lee,Aaron Lee,Paul L. Richards,M. E. Abroe,Shaul Hanany,Bradley R. Johnson,Peter A. R. Ade,Amedeo Balbi,J. J. Bock,Julian Borrill,Julian Borrill,Radek Stompor,Radek Stompor,A. Boscaleri,Enzo Pascale,P. de Bernardis,Pedro G. Ferreira,Pedro G. Ferreira,Viktor Hristov,Andrew E. Lange,Andrew H. Jaffe,Andrew H. Jaffe,Calvin B. Netterfield,George F. Smoot,George F. Smoot,Jiun-Huei Proty Wu,Jiun-Huei Proty Wu +29 more
TL;DR: MAXIMA as mentioned in this paper is a balloon-borne experiment which measured the temperature anisotropy of the cosmic microwave background (CMB) on angular scales of 10′ to 5°.
The new generation CMB B-mode polarization experiment: POLARBEAR
Josquin Errard,Peter A. R. Ade,A. E. Anthony,Kam Arnold,François Aubin,D. Boettger,Julian Borrill,C. M. Cantalupo,M. A. Dobbs,Daniel Flanigan,A. Ghribi,N. W. Halverson,Masashi Hazumi,W. L. Holzapfel,J. Howard,P. Hyland,A. H. Jaffe,Brian Keating,Ted Kisner,Zigmund Kermish,A. T. Lee,Eric V. Linder,Marius Lungu,Tomotake Matsumura,Nathan Miller,X. Meng,Michael J. Myers,Haruki Nishino,Roger O'Brient,D. O'Dea,Christian L. Reichardt,I. Schanning,A. Shimizu,Chase Owen Shimmin,Meir Shimon,Helmuth Spieler,Bryan Steinbach,R. Stompor,Aritoki Suzuki,Takayuki Tomaru,Huan Tran,Carole Tucker,E. Quealy,Paul L. Richards,Oliver Zahn +44 more
TL;DR: The Polarbear experiment as mentioned in this paper used the Huan Tran Telescope equipped with a powerful 1,200-bolometer array receiver to map the CMB polarization with unprecedented accuracy, achieving state-of-the-art results.
Journal ArticleDOI
Exploring cosmic origins with CORE: Effects of observer peculiar motion
Carlo Burigana,Carlo Burigana,C. S. Carvalho,Tiziana Trombetti,Tiziana Trombetti,Alessio Notari,Miguel Quartin,G. De Gasperis,Alessandro Buzzelli,Nicola Vittorio,G. de Zotti,P. de Bernardis,Jens Chluba,Maciej Bilicki,Luigi Danese,Jacques Delabrouille,L. Toffolatti,Andrea Lapi,Mattia Negrello,Pasquale Mazzotta,Douglas Scott,D. Contreras,Ana Achúcarro,Peter A. R. Ade,R. Allison,M. Ashdown,Mario Ballardini,A. J. Banday,R. Banerji,James G. Bartlett,Nicola Bartolo,S. Basak,Marco Bersanelli,A. Bonaldi,M. Bonato,J. Borrill,François R. Bouchet,Francois Boulanger,Thejs Brinckmann,Martin Bucher,P. Cabella,Zhen-Yi Cai,Martino Calvo,Marco Castellano,Anthony Challinor,Sebastien Clesse,I. Colantoni,Alessandro Coppolecchia,Martin Crook,Giuseppe D'Alessandro,Jose M. Diego,A. Di Marco,E. Di Valentino,Josquin Errard,Stephen M. Feeney,R. Fernandez-Cobos,Simone Ferraro,Fabio Finelli,Francesco Forastieri,Silvia Galli,Ricardo Genova-Santos,Martina Gerbino,J. González-Nuevo,Sebastian Grandis,J. Greenslade,S. Hagstotz,Shaul Hanany,Will Handley,Carlos Hernández-Monteagudo,C. Hervias-Caimapo,Matthew Hills,Eric Hivon,K. Kiiveri,Ted Kisner,Thomas Kitching,M. Kunz,Hannu Kurki-Suonio,Luca Lamagna,Anthony Lasenby,Massimiliano Lattanzi,Julien Lesgourgues,Michele Liguori,V. Lindholm,M. López-Caniego,Gemma Luzzi,Bruno Maffei,N. Mandolesi,N. Mandolesi,Enrique Martinez-Gonzalez,C. J. A. P. Martins,Silvia Masi,Sabino Matarrese,D. McCarthy,Alessandro Melchiorri,Jean-Baptiste Melin,Diego Molinari,Diego Molinari,Alessandro Monfardini,Paolo Natoli,Paolo Natoli,Alessandro Paiella,Daniela Paoletti,Guillaume Patanchon,M. Piat,Giampaolo Pisano,L. Polastri,G. Polenta,Agnieszka Pollo,Vivian Poulin,Mathieu Remazeilles,M. Roman,Jose Alberto Rubino-Martin,Laura Salvati,A. Tartari,M. Tomasi,D. Tramonte,Neil Trappe,Carole Tucker,Jussi Valiviita,R. Van de Weijgaert,B. Van Tent,Vincent Vennin,P. Vielva,Karl Young,Mario Zannoni +124 more
TL;DR: In this article, the effects on the CMB, CIB, and thermal SZ effect due to the peculiar motion of an observer with respect to CMB rest frame, which induces boosting effects, are discussed.
Journal ArticleDOI
Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence
Peter A. R. Ade,Nabila Aghanim,D. Alina,M. I. R. Alves,G. Aniano,C. Armitage-Caplan,Monique Arnaud,Doris Arzoumanian,M. Ashdown,F. Atrio-Barandela,J. Aumont,Carlo Baccigalupi,A. J. Banday,R. B. Barreiro,E. Battaner,Karim Benabed,A. Benoit-Lévy,A. Benoit-Lévy,J.-P. Bernard,Marco Bersanelli,Marco Bersanelli,P. Bielewicz,P. Bielewicz,John Bond,Julian Borrill,Julian Borrill,François R. Bouchet,F. Boulanger,Andrea Bracco,Carlo Burigana,Carlo Burigana,J.-F. Cardoso,J.-F. Cardoso,J.-F. Cardoso,A. Catalano,A. Catalano,A. Chamballu,A. Chamballu,A. Chamballu,H. C. Chiang,H. C. Chiang,P. R. Christensen,Stephane Colombi,L. P. L. Colombo,L. P. L. Colombo,C. Combet,F. Couchot,A. Coulais,B. P. Crill,A. Curto,A. Curto,F. Cuttaia,Luigi Danese,R. D. Davies,R. J. Davis,P. de Bernardis,A. De Rosa,G. de Zotti,G. de Zotti,Jacques Delabrouille,Clive Dickinson,Jose M. Diego,S. Donzelli,O. Doré,Marian Douspis,X. Dupac,George Efstathiou,Torsten A. Enßlin,H. K. Eriksen,Edith Falgarone,L. Fanciullo,Katia Ferrière,Fabio Finelli,Olivier Forni,M. Frailis,A. A. Fraisse,E. Franceschi,S. Galeotta,Ken Ganga,Tuhin Ghosh,M. Giard,Y. Giraud-Héraud,J. González-Nuevo,J. González-Nuevo,Krzysztof M. Gorski,Krzysztof M. Gorski,Anna Gregorio,Anna Gregorio,Alessandro Gruppuso,Vincent Guillet,F. K. Hansen,D. L. Harrison,George Helou,C. Hernández-Monteagudo,Sergi R. Hildebrandt,Eric Hivon,Michael P. Hobson,W. Holmes,Allan Hornstrup,Kevin M. Huffenberger,Andrew H. Jaffe,T. R. Jaffe,W. C. Jones,Mika Juvela,E. Keihänen,Reijo Keskitalo,Ted Kisner,R. Kneissl,R. Kneissl,J. Knoche,Martin Kunz,Martin Kunz,Martin Kunz,Hannu Kurki-Suonio,Hannu Kurki-Suonio,Guilaine Lagache,J.-M. Lamarre,Anthony Lasenby,Charles R. Lawrence,R. Leonardi,François Levrier,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Davide Maino,Davide Maino,N. Mandolesi,N. Mandolesi,N. Mandolesi,M. Maris,Douglas J. Marshall,Peter G. Martin,Enrique Martínez-González,Silvia Masi,Sabino Matarrese,Pasquale Mazzotta,Alessandro Melchiorri,L. Mendes,A. Mennella,A. Mennella,M. Migliaccio,Marc-Antoine Miville-Deschênes,Marc-Antoine Miville-Deschênes,A. Moneti,L. A. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Pavel Naselsky,Federico Nati,Paolo Natoli,Paolo Natoli,Paolo Natoli,Calvin B. Netterfield,F. Noviello,Dmitry Novikov,Igor D. Novikov,C. A. Oxborrow,L. Pagano,F. Pajot,Daniela Paoletti,F. Pasian,V.-M. Pelkonen,O. Perdereau,L. Perotto,Francesca Perrotta,F. Piacentini,M. Piat,Davide Pietrobon,Stéphane Plaszczynski,Etienne Pointecouteau,G. Polenta,G. Polenta,L. Popa,G. W. Pratt,Simon Prunet,Jean-Loup Puget,Jörg P. Rachen,M. Reinecke,Mathieu Remazeilles,Mathieu Remazeilles,Mathieu Remazeilles,C. Renault,S. Ricciardi,T. Riller,I. Ristorcelli,Graca Rocha,C. Rosset,G. Roudier,G. Roudier,G. Roudier,Ben Rusholme,M. Sandri,Douglas Scott,Juan D. Soler,Locke D. Spencer,V. Stolyarov,V. Stolyarov,Radek Stompor,Rashmikant V. Sudiwala,D. Sutton,A.-S. Suur-Uski,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,L. Toffolatti,L. Toffolatti,M. Tomasi,M. Tomasi,Matthieu Tristram,M. Tucci,M. Tucci,G. Umana,Luca Valenziano,Jussi Valiviita,Jussi Valiviita,B. Van Tent,P. Vielva,Fabrizio Villa,L. A. Wade,Benjamin D. Wandelt,Benjamin D. Wandelt,Andrea Zonca +227 more
TL;DR: In this paper, the authors compared Planck HFI observations with simulations of anisotropic magnetohydrodynamical (MHD) turbulence in which they assume a uniform intrinsic polarization fraction of the dust grains.