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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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Planck 2015 results. XV. Gravitational lensing

TL;DR: The most significant measurement of the cosmic microwave background (CMB) lensing potential at a level of 40 sigma using temperature and polarization data from the Planck 2015 full-mission release was presented in this article.
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Constraints on Cosmological Parameters from MAXIMA-1

TL;DR: In this article, the angular power spectrum of the cosmic microwave background measured over a wide range of l in the first flight of the MAXIMA balloon-borne experiment (MAXIMA-1) and the low-l results from the COBE Differential Microwave Radiometer experiment was used to set new constraints on a seven-dimensional space of cosmological parameters within the class of inflationary adiabatic models.
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Planck intermediate results - XXX. The angular power spectrum of polarized dust emission at intermediate and high Galactic latitudes

R. Adam, +301 more
TL;DR: In this article, the authors exploit the uniqueness of the Planck HFI polarization data from 100 to 353 GHz to measure the polarized dust angular power spectra C_l^(EE) and C_ l^(BB) over the multipole range 40
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The atacama cosmology telescope: cosmological parameters from the 2008 power spectrum

Jo Dunkley, +84 more
TL;DR: In this paper, the angular power spectrum of the cosmic microwave background (CMB) radiation observed at 148 GHz and 218 GHz over 296 deg(exp 2) with the Atacama Cosmology Telescope (ACT) during its 2008 season was analyzed.
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SPT-3G: A Next-Generation Cosmic Microwave Background Polarization Experiment on the South Pole Telescope

Bradford Benson, +69 more
- 23 Jul 2014 - 
TL;DR: SPT-3G as discussed by the authors is a new polarization sensitive receiver for the 10-meter South Pole Telescope (SPT), which will enable the advance from statistical detection of B-mode polarization anisotropy power to high signal-to-noise measurements of individual modes, i.e., maps.