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Kevin M. Huffenberger

Researcher at Florida State University

Publications -  415
Citations -  100443

Kevin M. Huffenberger is an academic researcher from Florida State University. The author has contributed to research in topics: Cosmic microwave background & Planck. The author has an hindex of 138, co-authored 402 publications receiving 93452 citations. Previous affiliations of Kevin M. Huffenberger include University of Central Florida & Jet Propulsion Laboratory.

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The Power Spectra of Polarized, Dusty Filaments

TL;DR: In this paper, an analytic model for the power spectra of polarized filamentary structures is developed to study the Galactic polarization foreground to the Cosmic Microwave Background, which is analogous to the cosmological halo-model framework.
Posted Content

CMB-S4 Decadal Survey APC White Paper

Kevork N. Abazajian, +224 more
TL;DR: An overview of the science case, instrument configuration and project plan for the next-generation ground-based cosmic microwave background experiment CMB-S4, for consideration by the 2020 Decadal Survey is provided in this article.
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Planck 2013 results. XIV. Zodiacal emission

Peter A. R. Ade, +292 more
TL;DR: In this article, the authors used the Planck data to investigate the behaviour of zodiacal emission over the whole sky at sub-millimetre and millimetre wavelengths, finding the emissivities of the various components of the COBE zodiacAL model -- a diffuse cloud, three asteroidal dust bands, a circumsolar ring, and an Earth-trailing feature.
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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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Prospects for ACT: Simulations, power spectrum, and non-Gaussian analysis

TL;DR: The Atacama Cosmology Telescope as discussed by the authors was the first to reveal the microwave sky at high resolution using a new generation of high-resolution instruments. But it is not suitable for high-dimensional observations.