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
QUaD: A High-Resolution Cosmic Microwave Background Polarimeter
J. Hinderks,J. Hinderks,Peter A. R. Ade,J. J. Bock,J. J. Bock,M. Bowden,Michael L. Brown,Michael L. Brown,G. Cahill,John E. Carlstrom,P. G. Castro,P. G. Castro,Sarah E. Church,Thomas Culverhouse,R. B. Friedman,K. Ganga,Walter Kieran Gear,S. Gupta,J. Harris,Victor Haynes,Victor Haynes,Brian Keating,John M Kovac,John M Kovac,Evan N. Kirby,Andrew E. Lange,E. M. Leitch,E. M. Leitch,O. E. Mallie,Simon J. Melhuish,Simon J. Melhuish,Y. Memari,J. A. Murphy,Angiola Orlando,Angiola Orlando,R. Schwarz,Créidhe O'Sullivan,Lucio Piccirillo,Lucio Piccirillo,C. Pryke,N. Rajguru,Ben Rusholme,Ben Rusholme,Andy Taylor,K. L. Thompson,Carole Tucker,A. H. Turner,E. Y. S. Wu,Michael Zemcov,Michael Zemcov +49 more
TL;DR: The QUaD experiment as mentioned in this paper is a millimeter-wavelength polarimeter designed to observe the Cosmic Microwave Background (CMB) from a site at the South Pole, which comprises a 2.64 m Cassegrain telescope equipped with a cryogenically cooled receiver containing an array of 62 polarization-sensitive bolometers.
Journal ArticleDOI
First Sunyaev–Zel’dovich mapping with the NIKA2 camera: Implication of cluster substructures for the pressure profile and mass estimate
Florian Ruppin,F. Mayet,G. W. Pratt,R. Adam,Peter A. R. Ade,Pascale Andre,M. Arnaud,H. Aussel,I. Bartalucci,A. Beelen,Alain Benoit,A. Bideaud,O. Bourrion,Manuel Calvo,A. Catalano,B. Comis,M. De Petris,F.-X. Désert,Simon Doyle,E. F. C. Driessen,J. Goupy,C. Kramer,G. Lagache,S. Leclercq,J.-F. Lestrade,J. F. Macías-Pérez,Philip Daniel Mauskopf,Philip Daniel Mauskopf,Alessandro Monfardini,L. Perotto,Giampaolo Pisano,E. Pointecouteau,Nicolas Ponthieu,V. Revéret,A. Ritacco,C. Romero,H. Roussel,K. F. Schuster,Albrecht Sievers,Carole Tucker,R. Zylka +40 more
TL;DR: In this article, the authors presented the first thermal Sunyaev-Zel-dovich (tSZ) mapping of a cluster from the sample of the New IRAM Kids Arrays (NIKA2) SZ large program that aims at constraining the redshift evolution of cluster pressure profiles and the tSZ-mass scaling relation.
Proceedings ArticleDOI
Pre-flight integration and characterization of the SPIDER balloon-borne telescope
Alexandra S. Rahlin,Peter A. R. Ade,Mandana Amiri,S. J. Benton,James J. Bock,J. R. Bond,Sean Bryan,H. C. Chiang,Carlo R. Contaldi,B. P. Crill,O. Doré,Marzieh Farhang,Jeffrey P. Filippini,Laura M. Fissel,Laura M. Fissel,A. A. Fraisse,A. E. Gambrel,Natalie N. Gandilo,Sunil Golwala,Jon E. Gudmundsson,Mark Halpern,Matthew Hasselfield,Matthew Hasselfield,Gene C. Hilton,Warren Holmes,Viktor Hristov,Kent D. Irwin,Kent D. Irwin,W. C. Jones,Zigmund Kermish,Chao-Lin Kuo,C. J. MacTavish,P. V. Mason,K. G. Megerian,Lorenzo Moncelsi,T. A. Morford,Johanna Nagy,Calvin B. Netterfield,Calvin B. Netterfield,Roger O'Brient,Carl D. Reintsema,J. E. Ruhl,Marcus Runyan,Jamil A. Shariff,Juan D. Soler,Juan D. Soler,Amy Trangsrud,Carole Tucker,R. S. Tucker,Anthony D. Turner,A. C. Weber,Donald V. Wiebe,E. Young +52 more
TL;DR: Spider as discussed by the authors is a balloon-borne polarimeter designed to probe the primordial gravitational wave signal in the degree-scale B-mode polarization of the cosmic microwave background, which is used to map 7.5% of the sky with a depth of 11 to 14 μK•arcmin at each frequency.
Journal ArticleDOI
Probing changes of dust properties along a chain of solar-type prestellar and protostellar cores in Taurus with NIKA
Andrea Bracco,P. Palmeirim,Ph. André,R. Adam,Peter A. R. Ade,Aurore Bacmann,Alexandre Beelen,Alain Benoit,Aurelien Bideaud,N. Billot,O. Bourrion,Martino Calvo,A. Catalano,Gregoire Coiffard,Barbara Comis,A. D'Addabbo,Francois-Xavier Désert,P. Didelon,Simon Doyle,Johannes Goupy,Vera Könyves,Carsten Kramer,Guilaine Lagache,Samuel Leclercq,J. F. Macías-Pérez,Anaëlle Maury,Philip Daniel Mauskopf,Philip Daniel Mauskopf,F. Mayet,Alessandro Monfardini,Frédérique Motte,F. Pajot,Enzo Pascale,Nicolas Peretto,L. Perotto,Giampaolo Pisano,Nicolas Ponthieu,V. Revéret,Andrew Rigby,A. Ritacco,L. Rodriguez,Charles Romero,A. Roy,Florian Ruppin,K. F. Schuster,A. Sievers,Sébastien Triqueneaux,Carole Tucker,R. Zylka +48 more
TL;DR: In this article, the authors present results of a new study of dust emissivity changes based on millimeter continuum data obtained with the NIKA camera at the IRAM-30 m telescope.
Journal ArticleDOI
Planck intermediate results - XXXIX. The Planck list of high-redshift source candidates
Peter A. R. Ade,Nabila Aghanim,M. Arnaud,J. Aumont,Carlo Baccigalupi,A. J. Banday,A. J. Banday,R. B. Barreiro,N. Bartolo,N. Bartolo,E. Battaner,K. Benabed,A. Benoit-Lévy,A. Benoit-Lévy,J.-P. Bernard,J.-P. Bernard,Marco Bersanelli,Marco Bersanelli,P. Bielewicz,P. Bielewicz,Anna Bonaldi,Laura Bonavera,J. R. Bond,Julian Borrill,Julian Borrill,F. R. Bouchet,Francois Boulanger,Carlo Burigana,Carlo Burigana,R. C. Butler,Erminia Calabrese,A. Catalano,A. Catalano,H. C. Chiang,H. C. Chiang,P. R. Christensen,David L. Clements,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,Clive Dickinson,Jose M. Diego,H. Dole,H. Dole,Olivier Doré,Marian Douspis,A. Ducout,A. Ducout,X. Dupac,F. Elsner,F. Elsner,Torsten A. Enßlin,H. K. Eriksen,E. Falgarone,Fabio Finelli,I. Flores-Cacho,I. Flores-Cacho,M. Frailis,Aurelien A. Fraisse,E. Franceschi,S. Galeotta,S. Galli,K. Ganga,M. Giard,M. Giard,Y. Giraud-Héraud,E. Gjerløw,J. González-Nuevo,J. González-Nuevo,Krzysztof M. Gorski,Krzysztof M. Gorski,A. Gregorio,A. Gregorio,Alessandro Gruppuso,Jon E. Gudmundsson,Jon E. Gudmundsson,Jon E. Gudmundsson,F. K. Hansen,D. L. Harrison,George Helou,C. Hernández-Monteagudo,D. Herranz,S. R. Hildebrandt,E. Hivon,Michael P. Hobson,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,G. Hurier,Andrew H. Jaffe,T. R. Jaffe,T. R. Jaffe,E. Keihänen,Reijo Keskitalo,Theodore Kisner,R. Kneissl,R. Kneissl,J. Knoche,Martin Kunz,Martin Kunz,Martin Kunz,Hannu Kurki-Suonio,Guilaine Lagache,Guilaine Lagache,J.-M. Lamarre,Anthony Lasenby,Massimiliano Lattanzi,Charles R. Lawrence,R. Leonardi,François Levrier,Michele Liguori,Michele Liguori,P. B. Lilje,M. Linden-Vørnle,M. López-Caniego,Philip Lubin,J. F. Macías-Pérez,Bruno Maffei,Gianmarco Maggio,Davide Maino,Davide Maino,N. Mandolesi,N. Mandolesi,A. Mangilli,A. Mangilli,Michele Maris,Peter G. Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,Sabino Matarrese,Alessandro Melchiorri,A. Mennella,A. Mennella,M. Migliaccio,Subhasish Mitra,Subhasish Mitra,Marc-Antoine Miville-Deschênes,Marc-Antoine Miville-Deschênes,A. Moneti,L. Montier,L. Montier,Gianluca Morgante,Daniel J. Mortlock,Dipak Munshi,J. A. Murphy,Federico Nati,Paolo Natoli,Paolo Natoli,Nicole P. H. Nesvadba,F. Noviello,Dmitry Novikov,I. D. Novikov,I. D. Novikov,Carol Anne Oxborrow,L. Pagano,F. Pajot,Daniela Paoletti,B. Partridge,Fabio Pasian,T. J. Pearson,O. Perdereau,L. Perotto,Valeria Pettorino,F. Piacentini,M. Piat,Stéphane Plaszczynski,Etienne Pointecouteau,Etienne Pointecouteau,G. Polenta,G. Polenta,G. W. Pratt,Simon Prunet,J.-L. Puget,Jörg P. Rachen,Jörg P. Rachen,M. Reinecke,Mathieu Remazeilles,Mathieu Remazeilles,Mathieu Remazeilles,C. Renault,A. Renzi,I. Ristorcelli,I. Ristorcelli,Graca Rocha,C. Rosset,M. Rossetti,M. Rossetti,G. Roudier,G. Roudier,G. Roudier,Jose Alberto Rubino-Martin,Jose Alberto Rubino-Martin,Ben Rusholme,M. Sandri,D. Santos,M. Savelainen,Giorgio Savini,Douglas Scott,Locke D. Spencer,V. Stolyarov,V. Stolyarov,V. Stolyarov,Radek Stompor,R. V. Sudiwala,R. A. Sunyaev,R. A. Sunyaev,A.-S. Suur-Uski,J.-F. Sygnet,J. A. Tauber,Luca Terenzi,Luca Terenzi,L. Toffolatti,L. Toffolatti,L. Toffolatti,M. Tomasi,M. Tomasi,M. Tristram,M. Tucci,Marc Türler,G. Umana,Luca Valenziano,Jussi-Pekka Väliviita,F. Van Tent,P. Vielva,Fabrizio Villa,Lawrence A. Wade,B. D. Wandelt,B. D. Wandelt,Ingunn Kathrine Wehus,Ingunn Kathrine Wehus,Niraj Welikala,D. Yvon,Andrea Zacchei,Andrea Zonca +247 more
TL;DR: In this paper, a combination of Planck and IRAS data was used to select the most luminous cold sub-millimetre sources with spectral energy distributions peaking between 353 and 857 GHz at 5′ resolution.