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C. Armitage-Caplan

Researcher at University of Oxford

Publications -  47
Citations -  22743

C. Armitage-Caplan is an academic researcher from University of Oxford. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 41, co-authored 47 publications receiving 21522 citations.

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Planck 2013 results. XXIX. Planck catalogue of Sunyaev-Zeldovich sources

P. A. R. Ade, +272 more
TL;DR: In this paper, the authors describe the all-sky Planck catalogue of clusters and cluster candidates derived from Sunyaev-Zeldovich (SZ) effect detections using the first 15.5 months of Planck satellite observations.
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Planck 2013 results. XV. CMB power spectra and likelihood

Peter A. R. Ade, +328 more
TL;DR: The Planck 2013 likelihood as mentioned in this paper is a complete statistical description of the two-point correlation function of the CMB temperature fluctuations that accounts for all known relevant uncertainties, both instrumental and astrophysical in nature.
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Planck 2013 results. XXIV. Constraints on primordial non-Gaussianity

Peter A. R. Ade, +302 more
TL;DR: The Planck nominal mission cosmic microwave background (CMB) maps yield unprecedented constraints on primordial non-Gaussianity (NG) using three optimal bispectrum estimators, separable template-fitting (KSW), binned, and modal as discussed by the authors.
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Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust

Peter A. R. Ade, +200 more
TL;DR: In this paper, a large-scale view of the Planck HFI at 353 GHz is presented, showing that the maximum observed dust polarization fraction is high in some of the intermediate dust column density (AV < 1mag) regions.
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Planck 2013 results. XVII. Gravitational lensing by large-scale structure

Peter A. R. Ade, +303 more
TL;DR: In this paper, the authors used the temperature-gradient correlations induced by lensing to reconstruct a (noisy) map of the CMB lensing potential, which provides an integrated measure of the mass distribution back to the last-scattering surface.