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
A review of metal mesh filters
TL;DR: The current state of the art with respect to quasi-optical components (low-pass, high-pass and band-pass filters, dichroics and beam-dividers) as developed for the FIR and sub-millimetre wavelength region are reviewed.
Book ChapterDOI
Exploring The Saturn System In The Thermal Infrared: The Composite Infrared Spectrometer
F. M. Flasar,V. G. Kunde,Mian M. Abbas,R. K. Achterberg,Peter A. R. Ade,Antonella Barucci,B. Bezard,Gordon L. Bjoraker,John C. Brasunas,S. B. Calcutt,R. W. Carlson,C. J. Cesarsky,Barney J. Conrath,Angioletta Coradini,Régis Courtin,Athena Coustenis,S. Edberg,Scott G. Edgington,Chiara Ferrari,Thierry Fouchet,D. Gautier,Peter J. Gierasch,K. Grossman,Patrick G. J. Irwin,D. E. Jennings,E. Lellouch,A. A. Mamoutkine,A. Marten,J. P. Meyer,Conor A. Nixon,Glenn S. Orton,T. C. Owen,John C. Pearl,Renée Prangé,François Raulin,Peter L. Read,Paul N. Romani,Robert E. Samuelson,M. E. Segura,Mark R. Showalter,Amy A. Simon-Miller,M. D. Smith,John R. Spencer,Linda Spilker,Fredric W. Taylor +44 more
TL;DR: The Composite Infrared Spectrometer (CIRS) is a remote-sensing Fourier transform spectrometer on the Cassini orbiter that measures thermal radiation over two decades in wavenumber, with a spectral resolution that can be set from 0.5 to 15.5 cm− 1.
Journal ArticleDOI
Planck 2013 results. XXV. Searches for cosmic strings and other topological defects
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,Richard A. Battye,K. Benabed,Alain Benoit,A. Benoit-Lévy,A. Benoit-Lévy,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,Lung-Yih Chiang,H. C. Chiang,H. C. 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,Jose M. Diego,H. Dole,H. Dole,S. Donzelli,Olivier Doré,Marian Douspis,A. Ducout,Joanna Dunkley,X. Dupac,George Efstathiou,Torsten A. Enßlin,H. K. Eriksen,James R. Fergusson,Fabio Finelli,Olivier Forni,Olivier Forni,M. Frailis,E. Franceschi,S. Galeotta,K. Ganga,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,Michael P. Hobson,W. A. Holmes,Allan Hornstrup,W. Hovest,Kevin M. Huffenberger,T. R. Jaffe,T. R. Jaffe,Andrew H. Jaffe,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,Anthony Lasenby,René J. Laureijs,Charles R. Lawrence,J. P. Leahy,R. Leonardi,J. Lesgourgues,J. 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,M. Maris,D. J. Marshall,Peter G. Martin,E. Martínez-González,Silvia Masi,Sabino Matarrese,F. Matthai,Pasquale Mazzotta,Jason D. McEwen,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,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,F. Pasian,G. Patanchon,Hiranya V. Peiris,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,Christoph Räth,Rafael Rebolo,Rafael Rebolo,Mathieu Remazeilles,Mathieu Remazeilles,C. Renault,S. Ricciardi,T. Riller,Christophe Ringeval,Christophe Ringeval,I. Ristorcelli,I. Ristorcelli,Graca Rocha,C. Rosset,G. Roudier,G. Roudier,G. Roudier,Michael Rowan-Robinson,Ben Rusholme,M. Sandri,D. Santos,Giorgio Savini,Douglas Scott,M. D. Seiffert,E. P. S. Shellard,Locke D. Spencer,Jean-Luc Starck,V. Stolyarov,V. Stolyarov,Radek Stompor,R. Sudiwala,F. Sureau,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,Luca Valenziano,Jussi-Pekka Väliviita,Jussi-Pekka Väliviita,Jussi-Pekka Väliviita,B. Van Tent,Jussi Varis,P. Vielva,Fabrizio Villa,Nicola Vittorio,L. A. Wade,Benjamin D. Wandelt,Benjamin D. Wandelt,D. Yvon,Andrea Zacchei,Andrea Zonca +287 more
TL;DR: In this article, the angular power spectrum from strings has been used to provide stringent new constraints on cosmic strings and other defects, such as the string tension, which can be improved to 1.015 at 95% confidence with the inclusion of high-ell$ CMB data.
Journal ArticleDOI
Extragalactic millimeter-wave sources in South Pole Telescope Survey data: source counts, catalog, and statistics for an 87 square-degree field
Joaquin Vieira,T. M. Crawford,Eric R. Switzer,Peter A. R. Ade,K. A. Aird,M. L. N. Ashby,Bradford Benson,Lindsey Bleem,Mark Brodwin,John E. Carlstrom,C. L. Chang,Hsiao-Mei Cho,A. T. Crites,T. de Haan,Matt Dobbs,W. Everett,Elizabeth George,Michael D. Gladders,Nicholas Hall,N. W. Halverson,F. W. High,Gilbert Holder,W. L. Holzapfel,J. D. Hrubes,Marshall Joy,Ryan Keisler,Lloyd Knox,Adrian T. Lee,Adrian T. Lee,E. M. Leitch,M. Lueker,Daniel P. Marrone,Vince McIntyre,Jeff McMahon,Jeff McMahon,J. Mehl,S. S. Meyer,Joseph J. Mohr,T. E. Montroy,Stephen Padin,T. Plagge,T. Plagge,C. Pryke,Christian L. Reichardt,J. E. Ruhl,K. K. Schaffer,L. Shaw,L. Shaw,Erik Shirokoff,Helmuth Spieler,B. Stalder,Z. K. Staniszewski,Antony A. Stark,K. Vanderlinde,Wilfred M. Walsh,R. Williamson,Yi Yang,Oliver Zahn,A. Zenteno +58 more
TL;DR: In this article, the authors report the results of an 87 deg(2) point-source survey centered at R.A. 5(h)30(m), decl. −55° taken with the South Pole Telescope at 1.4 and 2.0 mm wavelengths with arcminute resolution and milli-Jansky depth.
Journal ArticleDOI
Cosmological parameters from the first results of Boomerang
Andrew E. Lange,Peter A. R. Ade,James J. Bock,J. Bond,Julian Borrill,A. Boscaleri,K. Coble,B. P. Crill,P. de Bernardis,P. C. Farese,Pedro G. Ferreira,K. Ganga,M. Giacometti,E. Hivon,V. Hristov,A. Iacoangeli,Andrew H. Jaffe,L. Martinis,Silvia Masi,Philip Daniel Mauskopf,Alessandro Melchiorri,T. E. Montroy,Calvin B. Netterfield,Enzo Pascale,F. Piacentini,Dmitry Pogosyan,Simon Prunet,S. Rao,Giovanni Romeo,J. E. Ruhl,F. Scaramuzzi,D. Sforna +31 more
TL;DR: In this article, the angular power spectrum measured in the first Antarctic flight of the Boomerang experiment was used to estimate the anisotropy of the cosmic microwave background radiation.