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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. XII. Full Focal Plane simulations

Peter A. R. Ade, +229 more
TL;DR: The 8th Full Focal Plane Simulation Set (FFP8) as mentioned in this paper was deployed in support of the Planck 2015 results and consists of 10 fiducial mission realizations reduced to 18144 maps, together with the most massive suite of Monte Carlo realizations of instrument noise and CMB ever generated.
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Planck 2013 results. XXI. Power spectrum and high-order statistics of the Planck all-sky Compton parameter map

Peter A. R. Ade, +304 more
TL;DR: In this article, the authors constructed the first all-sky map of the thermal Sunyaev-Zeldovich (tSZ) e ect by applying specifically tailored component separation algorithms to the 100 to 857 GHz frequency channel maps from the Planck survey.
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Planck 2013 results - VIII. HFI photometric calibration and mapmaking

Peter A. R. Ade, +284 more
TL;DR: In this paper, the authors describe the methods used to produce photometrically calibrated maps from the Planck High Frequency Instrument (HFI) cleaned, time-ordered information.
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A Measurement of the Polarization-Temperature Angular Cross-Power Spectrum of the Cosmic Microwave Background from the 2003 Flight of BOOMERANG

TL;DR: In this paper, a measurement of the polarization-temperature angular cross power spectra of the cosmic microwave background using bolometric detectors is presented, which is consistent with previous detections and with the "concordance model" that assumes adiabatic initial conditions.
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Planck early results. XXI. Properties of the interstellar medium in the Galactic plane

A. Abergel, +200 more
TL;DR: In this paper, the authors show that anomalous dust emission is present in the atomic, molecular and dark gas phases throughout the Galactocentricity of the Galactic disk, and the derived dust propeties associated with the dark gas phase are derived but do not allow us to reveal the nature of this phase.