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.
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Journal ArticleDOI
DISCOVERY AND COSMOLOGICAL IMPLICATIONS OF SPT-CL J2106-5844, THE MOST MASSIVE KNOWN CLUSTER AT z > 1
Ryan J. Foley,K. Andersson,K. Andersson,G. Bazin,T. de Haan,Jonathan Ruel,Peter A. R. Ade,K. A. Aird,Robert Armstrong,M. L. N. Ashby,Mark W. Bautz,Bradford Benson,Lindsey Bleem,Massimiliano Bonamente,M. Brodwin,John E. Carlstrom,C. L. Chang,Alejandro Clocchiatti,T. M. Crawford,A. T. Crites,Shantanu Desai,M. A. Dobbs,J. P. Dudley,Giovanni G. Fazio,William R. Forman,Gordon P. Garmire,Elizabeth George,Michael D. Gladders,Anthony H. Gonzalez,N. W. Halverson,F. W. High,Gilbert Holder,W. L. Holzapfel,S. Hoover,J. D. Hrubes,Christine Jones,Marshall Joy,Ryan Keisler,Lloyd Knox,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,M. Lueker,Daniel M. Luong-Van,Daniel P. Marrone,Jeff McMahon,J. Mehl,S. S. Meyer,Joseph J. Mohr,T. E. Montroy,S. S. Murray,Stephen Padin,Stephen Padin,T. Plagge,C. Pryke,Christian L. Reichardt,Armin Rest,Armin Rest,J. E. Ruhl,Benjamin Saliwanchik,A. Saro,K. K. Schaffer,L. Shaw,L. Shaw,Erik Shirokoff,Jizhou Song,Helmuth Spieler,B. Stalder,Spencer A. Stanford,Z. K. Staniszewski,Antony A. Stark,K. T. Story,Christopher W. Stubbs,K. Vanderlinde,Joaquin Vieira,Joaquin Vieira,Alexey Vikhlinin,R. Williamson,A. Zenteno +78 more
TL;DR: The most massive known galaxy cluster at z>1, SPT-CL J2106-5844, was discovered using the South Pole Telescope (SPT) and Magellan spectroscopy of 18 member galaxies as discussed by the authors.
Journal ArticleDOI
High angular resolution Sunyaev-Zel’dovich observations of MACS J1423.8+2404 with NIKA: Multiwavelength analysis
R. Adam,R. Adam,Barbara Comis,I. Bartalucci,A. Adane,Peter A. R. Ade,Ph. André,Monique Arnaud,Alexandre Beelen,Benoit Belier,Alain Benoit,Aurelien Bideaud,N. Billot,O. Bourrion,Martino Calvo,A. Catalano,Gregoire Coiffard,A. D'Addabbo,A. D'Addabbo,F.-X. Désert,Simon Doyle,Johannes Goupy,B. Hasnoun,Israel Hermelo,Carsten Kramer,Guilaine Lagache,Samuel Leclercq,J. F. Macías-Pérez,J. Martino,Philip Daniel Mauskopf,Philip Daniel Mauskopf,F. Mayet,Alessandro Monfardini,F. Pajot,Enzo Pascale,L. Perotto,Etienne Pointecouteau,Etienne Pointecouteau,Nicolas Ponthieu,G. W. Pratt,V. Revéret,A. Ritacco,L. Rodriguez,Giorgio Savini,Karl Schuster,A. Sievers,Sébastien Triqueneaux,Carole Tucker,R. Zylka +48 more
TL;DR: In this article, the NIKA data were combined with Herschel satellite data to study the SZ effect of the submm point source contaminants, and a joint reconstruction of the ICM electronic pressure and density was performed by combining NIKa, Planck, XMM-Newton and Chandra data, focussing on the impact of the radio and submm sources on the reconstructed pressure profile.
Journal ArticleDOI
Planck 2013 results. XIX. The integrated Sachs-Wolfe effect
Peter A. R. Ade,Nabila Aghanim,C. Armitage-Caplan,Monique Arnaud,M. Ashdown,Fernando Atrio-Barandela,J. Aumont,Carlo Baccigalupi,A. J. Banday,A. J. Banday,R. B. Barreiro,James G. Bartlett,James G. Bartlett,Nicola Bartolo,E. Battaner,K. Benabed,Alain Benoit,A. Benoit-Lévy,A. Benoit-Lévy,J.-P. Bernard,J.-P. Bernard,Marco Bersanelli,Marco Bersanelli,P. Bielewicz,P. Bielewicz,P. Bielewicz,Jérôme Bobin,J. J. Bock,Anna Bonaldi,Laura Bonavera,J. R. Bond,Julian Borrill,Julian Borrill,François R. Bouchet,M. Bridges,M. Bucher,Carlo Burigana,Carlo Burigana,R. C. Butler,Jean-François Cardoso,Jean-François Cardoso,Jean-François Cardoso,A. Catalano,A. Catalano,Anthony Challinor,A. Chamballu,A. Chamballu,A. Chamballu,H. C. Chiang,H. C. Chiang,Lung-Yih Chiang,P. R. Christensen,Sarah E. Church,David L. Clements,S. Colombi,L. P. L. Colombo,L. P. L. Colombo,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,J.-M. Delouis,F.-X. Désert,Clive Dickinson,Jose M. Diego,Klaus Dolag,Klaus Dolag,H. Dole,H. Dole,S. Donzelli,Olivier Doré,Marian Douspis,X. Dupac,George Efstathiou,Torsten A. Enßlin,H. K. Eriksen,James R. Fergusson,Fabio Finelli,Olivier Forni,Olivier Forni,Pablo Fosalba,M. Frailis,E. Franceschi,M. Frommert,S. Galeotta,K. Ganga,Ricardo Génova-Santos,M. Giard,M. Giard,G. Giardino,Y. Giraud-Héraud,J. González-Nuevo,J. González-Nuevo,Krzysztof M. Gorski,Krzysztof M. Gorski,Serge Gratton,A. Gregorio,A. Gregorio,Alessandro Gruppuso,F. K. Hansen,Duncan Hanson,Duncan Hanson,Duncan Hanson,D. L. Harrison,Sophie Henrot-Versille,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Shirley Ho,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,S. Ilić,Andrew H. Jaffe,T. R. Jaffe,T. R. Jaffe,Jens Jasche,W. C. Jones,Mika Juvela,E. Keihänen,Reijo Keskitalo,Reijo Keskitalo,Theodore Kisner,J. Knoche,Lloyd Knox,Martin Kunz,Martin Kunz,Martin Kunz,Hannu Kurki-Suonio,Hannu Kurki-Suonio,Guilaine Lagache,Anne Lähteenmäki,Anne Lähteenmäki,J.-M. Lamarre,Mathieu Langer,Anthony Lasenby,René J. Laureijs,Charles R. Lawrence,J. P. Leahy,R. Leonardi,Julien Lesgourgues,Julien Lesgourgues,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Bruno Maffei,Davide Maino,Davide Maino,N. Mandolesi,N. Mandolesi,N. Mandolesi,Anna Mangilli,A. Marcos-Caballero,M. Maris,D. J. Marshall,Peter G. Martin,E. Martínez-González,Silvia Masi,Marcella Massardi,Sabino Matarrese,F. Matthai,Pasquale Mazzotta,Peter Meinhold,Alessandro Melchiorri,L. Mendes,A. Mennella,A. Mennella,M. Migliaccio,Subhabrata Mitra,Subhabrata Mitra,M.-A. Miville-Deschênes,M.-A. Miville-Deschênes,A. Moneti,L. Montier,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Adam Moss,Dipak Munshi,Pavel Naselsky,Federico Nati,Paolo Natoli,Paolo Natoli,Paolo Natoli,Calvin B. Netterfield,Hans Ulrik Nørgaard-Nielsen,F. Noviello,Dmitry Novikov,I. D. Novikov,S. Osborne,C. A. Oxborrow,F. Paci,L. Pagano,F. Pajot,Daniela Paoletti,Bruce Partridge,F. Pasian,G. Patanchon,O. Perdereau,L. Perotto,Francesca Perrotta,F. Piacentini,M. Piat,E. Pierpaoli,Davide Pietrobon,Stéphane Plaszczynski,Etienne Pointecouteau,Etienne Pointecouteau,G. Polenta,G. Polenta,N. Ponthieu,N. Ponthieu,L. Popa,T. Poutanen,T. Poutanen,T. Poutanen,G. W. Pratt,G. Prézeau,Simon Prunet,J.-L. Puget,Jörg P. Rachen,Jörg P. Rachen,B. Racine,Rafael Rebolo,Rafael Rebolo,M. Reinecke,Mathieu Remazeilles,Mathieu Remazeilles,Mathieu Remazeilles,C. Renault,A. Renzi,S. Ricciardi,T. Riller,I. Ristorcelli,I. Ristorcelli,Graca Rocha,C. Rosset,G. Roudier,G. Roudier,G. Roudier,Michael Rowan-Robinson,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,D. Santos,Giorgio Savini,B. M. Schaefer,F. Schiavon,Douglas Scott,Michael Seiffert,E. P. S. Shellard,Locke D. Spencer,Jean-Luc Starck,V. Stolyarov,V. Stolyarov,Radek Stompor,R. V. Sudiwala,R. A. Sunyaev,R. A. Sunyaev,F. Sureau,Paul M. Sutter,D. Sutton,A.-S. Suur-Uski,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,D. Tavagnacco,D. Tavagnacco,Luca Terenzi,L. Toffolatti,L. Toffolatti,M. Tomasi,M. Tristram,M. Tucci,M. Tucci,Jussi Tuovinen,G. Umana,Luca Valenziano,Jussi-Pekka Väliviita,Jussi-Pekka Väliviita,Jussi-Pekka Väliviita,B. Van Tent,Jussi Varis,Matteo Viel,P. Vielva,Fabrizio Villa,Nicola Vittorio,L. A. Wade,Benjamin D. Wandelt,Benjamin D. Wandelt,Martin White,Jun-Qing Xia,D. Yvon,Andrea Zacchei,Andrea Zonca +311 more
TL;DR: In this paper, the authors presented the detection of the integrated Sachs-Wolfe (ISW) effect, that is, the correlation between the CMB and large-scale evolving gravitational potentials.
Journal ArticleDOI
SPT-CL J0546-5345: A massive z > 1 galaxy cluster selected via the Sunyaev-Zel'dovich Effect with the South Pole Telescope
M. Brodwin,Jonathan Ruel,Peter A. R. Ade,K. A. Aird,K. Andersson,M. L. N. Ashby,Mark W. Bautz,G. Bazin,Bradford Benson,Lindsey Bleem,John E. Carlstrom,C. L. Chang,T. M. Crawford,A. T. Crites,T. de Haan,Shantanu Desai,Matt Dobbs,J. P. Dudley,Giovanni G. Fazio,Ryan J. Foley,William R. Forman,Gordon P. Garmire,Elizabeth George,Michael D. Gladders,Anthony H. Gonzalez,N. W. Halverson,F. W. High,Gilbert Holder,W. L. Holzapfel,J. D. Hrubes,Christine Jones,Marshall Joy,Ryan Keisler,Lloyd Knox,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,M. Lueker,Daniel P. Marrone,Jeff McMahon,Jeff McMahon,J. Mehl,S. S. Meyer,Joseph J. Mohr,T. E. Montroy,S. S. Murray,Stephen Padin,T. Plagge,T. Plagge,C. Pryke,Christian L. Reichardt,Armin Rest,J. E. Ruhl,K. K. Schaffer,L. Shaw,L. Shaw,Erik Shirokoff,Jizhou Song,Helmuth Spieler,B. Stalder,Spencer A. Stanford,Z. K. Staniszewski,Antony A. Stark,Christopher W. Stubbs,K. Vanderlinde,Joaquin Vieira,Alexey Vikhlinin,R. Williamson,Yi Yang,Oliver Zahn,A. Zenteno +70 more
TL;DR: In this article, the authors reported the spectroscopic confirmation of SPT-CL J0546-5345 at z = 1.067, which is the first z>1 cluster discovered by the Sunyaev-Zel'dovich Effect (SZE).
Proceedings ArticleDOI
EBEX: A balloon-borne CMB polarization experiment
Britt Reichborn-Kjennerud,Asad M. Aboobaker,Peter A. R. Ade,François Aubin,Carlo Baccigalupi,Chaoyun Bao,Julian Borrill,Christopher Cantalupo,Daniel Chapman,Joy Didier,Matt Dobbs,Julien Grain,William F. Grainger,Shaul Hanany,Seth Hillbrand,Johannes Hubmayr,Andrew H. Jaffe,Bradley R. Johnson,Terry J. Jones,Theodore Kisner,Jacob Klein,Andrei Korotkov,S. Leach,Adrian T. Lee,L. J. Levinson,Michele Limon,Kevin MacDermid,Tomotake Matsumura,X. Meng,Amber Miller,Michael Milligan,Enzo Pascale,Daniel Polsgrove,Nicolas Ponthieu,Kate Raach,Ilan Sagiv,Graeme Smecher,F. Stivoli,Radek Stompor,Huan Tran,Matthieu Tristram,Gregory S. Tucker,Yury Vinokurov,Amit P. S. Yadav,Matias Zaldarriaga,Kyle Zilic +45 more
TL;DR: The EBEX experiment as mentioned in this paper is a NASA-funded balloon-borne experiment designed to measure the polarization of the cosmic microwave background (CMB) using 1432 transition edge sensor (TES) bolometric detectors read out with frequency multiplexed SQuIDs.