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Simon Prunet

Researcher at Institut d'Astrophysique de Paris

Publications -  439
Citations -  102156

Simon Prunet is an academic researcher from Institut d'Astrophysique de Paris. The author has contributed to research in topics: Cosmic microwave background & Planck. The author has an hindex of 141, co-authored 434 publications receiving 96314 citations. Previous affiliations of Simon Prunet include University of Hawaii & University of Toronto.

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Planck intermediate results: VI. The dynamical structure of PLCKG214.6+37.0, a Planck discovered triple system of galaxy clusters

Peter A. R. Ade, +244 more
TL;DR: In this paper, the results from a deep XMM-Newton re-observation were used to build a template model to extract the total SZ signal of the PLCKG214.6+37.0 galaxy cluster.
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Planck intermediate results. XII: Diffuse Galactic components in the Gould Belt System

Peter A. R. Ade, +180 more
TL;DR: In this article, the authors performed an analysis of the diffuse low-frequency Galactic components in the Southern part of the Gould Belt system (130^\circ/leq l\leq 230^ √ √ and -50^√/l √ b √ -10^\Circ).
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Cylinders out of a top hat: counts-in-cells for projected densities

TL;DR: In this paper, large deviation statistics is implemented to predict the statistics of cosmic densities in cylinders applicable to photometric surveys, which yields few percent accurate analytical predictions for the one-point probability distribution function (PDF) of densities of concentric or compensated cylinders.
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Secular resonant dressed orbital diffusion I : method and WKB limit for tepid discs

TL;DR: In this article, the authors derived an equation describing the secular diffusion of a self-gravitating collisionless system induced by an exterior perturbation while assuming that the time-scale corresponding to secular evolution is much larger than that corresponding to the natural frequencies of the system.
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Planck 2013 results. IV. Low Frequency Instrument beams and window functions

Nabila Aghanim, +260 more
TL;DR: In this article, the authors presented the characterization of the in-flight beams, the beam window functions and the associated uncertainties for the Planck Low Frequency Instrument (LFI) for the purpose of determining the transfer function for determining the actual sky anisotropy power spectrum.