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
Kinetic inductance detectors for the OLIMPO experiment: in-flight operation and performance
Silvia Masi,P. de Bernardis,Alessandro Paiella,F. Piacentini,Luca Lamagna,Alessandro Coppolecchia,Peter A. R. Ade,Elia S. Battistelli,Maria Gabriella Castellano,I. Colantoni,F. Columbro,Giuseppe D'Alessandro,M. De Petris,S. Gordon,C. Magneville,P. Mauskopf,Giorgio Pettinari,Giampaolo Pisano,G. Polenta,G. Presta,E. Tommasi,Carole Tucker,Vyacheslav Vdovin,A. Volpe,D. Yvon +24 more
TL;DR: In this paper, the performance of lumped-elements Kinetic Inductance Detector (KID) arrays for mm and sub-mm wavelengths, operated at 0.3 K during the stratospheric flight of the OLIMPO payload, at an altitude of 37.8 km.
Proceedings ArticleDOI
Herschel-SPIRE: Design, Performance, and Scientific Capabilities
Matthew Joseph Griffin,Alain Abergel,Peter A. R. Ade,Philippe André,Jean-Paul Baluteau,James J. Bock,Alberto Franceschini,Walter Kieran Gear,Jason Glenn,Douglas Griffin,K. J. King,Emmanuel Lellouch,David A. Naylor,Göran Olofsson,Ismael Perez-Fournon,M. Rowan-Robinson,Paolo Saraceno,Eric Sawyer,Alan Smith,Bruce Swinyard,L. Vigroux,Gillian S. Wright +21 more
TL;DR: SPIRE, the Spectral and Photometric Imaging Receiver, is a submillimetre camera and spectrometer for the European Space Agency's Herschel Space Observatory as mentioned in this paper, which comprises a three-band imaging photometer operating at 250, 360 and 520.
Journal ArticleDOI
Imaging the environment of a z = 6.3 submillimeter galaxy with SCUBA-2.
E. I. Robson,Rob Ivison,Ian Smail,Wayne S. Holland,Wayne S. Holland,James E. Geach,Andy Gibb,Dominik A. Riechers,Peter A. R. Ade,Dan Bintley,James J. Bock,E. Chapin,Scott Chapman,David L. Clements,A. Conley,A. Cooray,James Dunlop,Duncan Farrah,M. Fich,Hai Fu,Tim Jenness,Nicolas Laporte,Seb Oliver,Alain Omont,Ismael Perez-Fournon,Ismael Perez-Fournon,Douglas Scott,A. M. Swinbank,Julie Wardlow +28 more
TL;DR: In this article, a search for submillimeter emission in the vicinity of one of the most distant, luminous galaxies known, HerMES FLS3, at z = 6.34, exploiting it as a signpost to a potentially biased region of the early universe.
Proceedings ArticleDOI
The performance of the bolometer array and readout system during the 2012/2013 flight of the E and B experiment (EBEX)
Kevin MacDermid,Asad M. Aboobaker,Peter A. R. Ade,François Aubin,Carlo Baccigalupi,Kevin Bandura,Chaoyun Bao,Julian Borrill,Daniel Chapman,Joy Didier,Matt Dobbs,Matt Dobbs,Julien Grain,William F. Grainger,Shaul Hanany,Kyle Helson,Seth Hillbrand,Gene C. Hilton,Hannes Hubmayr,Kent D. Irwin,Bradley R. Johnson,Andrew H. Jaffe,Terry Jay Jones,Ted Kisner,Jeff Klein,Andrei Korotkov,Adrian T. Lee,L. J. Levinson,Michele Limon,Amber Miller,Michael Milligan,Enzo Pascale,Kate Raach,Britt Reichborn-Kjennerud,Carl D. Reintsema,Ilan Sagiv,Graeme Smecher,Radek Stompor,Matthieu Tristram,Gregory S. Tucker,Ben Westbrook,Kyle Zilic +41 more
TL;DR: EBEX as discussed by the authors is a balloon-borne telescope designed to measure the polarization of the cosmic microwave background radiation (CMBR) using 955 spider-web transition edge sensor (TES) separated into bands at 150, 250 and 410 GHz.
Journal ArticleDOI
Measurement of Cosmic Microwave Background Polarization Power Spectra from Two Years of BICEP Data
H. C. Chiang,H. C. Chiang,Peter A. R. Ade,Denis Barkats,Denis Barkats,J. Battle,E. M. Bierman,James J. Bock,James J. Bock,C. D. Dowell,L. Duband,Eric Hivon,W. L. Holzapfel,Viktor Hristov,W. C. Jones,W. C. Jones,Brian Keating,John M Kovac,Chao-Lin Kuo,Andrew E. Lange,Andrew E. Lange,E. M. Leitch,P. V. Mason,Tomotake Matsumura,H. T. Nguyen,Nicolas Ponthieu,C. Pryke,S. Richter,G. Rocha,G. Rocha,C. D. Sheehy,Y. D. Takahashi,J. E. Tolan,Ki Won Yoon +33 more
TL;DR: In this article, the E-mode angular power spectrum was measured with high precision at 21 < ell < 335, detecting for the first time the peak expected at ell ~ 140.