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Lloyd Knox

Researcher at University of California, Davis

Publications -  394
Citations -  87991

Lloyd Knox is an academic researcher from University of California, Davis. The author has contributed to research in topics: Cosmic microwave background & Planck. The author has an hindex of 139, co-authored 375 publications receiving 78589 citations. Previous affiliations of Lloyd Knox include University of Toronto & Institut d'Astrophysique de Paris.

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A Measurement of the Cosmic Microwave Background Gravitational Lensing Potential from 100 Square Degrees of SPTpol Data

K. T. Story, +78 more
TL;DR: In this article, a measurement of the cosmic microwave background (CMB) gravitational lensing potential using data from the first two seasons of observations with SPTpol, the polarization-sensitive receiver currently installed on the South Pole Telescope (SPT).
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Planck 2013 results. II. Low Frequency Instrument data processing

Peter A. R. Ade, +298 more
TL;DR: In this article, the processing of the 531 billion raw data samples from the High Frequency Instrument (hereafter HFI), which performed to produce six temperature maps from the first 473 days of Planck-HFI survey data, was described.
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A re-analysis of the three-year WMAP temperature power spectrum and likelihood

TL;DR: In this article, the power spectrum and likelihoods of WMAP were confirmed by applying five independent implementations of four algorithms to power spectrum estimation and two implementations to parameter estimation, and the results showed that most parameters are affected by a few tenths of a sigma.
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Planck 2013 results. X. HFI energetic particle effects: characterization, removal, and simulation

Peter A. R. Ade, +276 more
TL;DR: In this paper, the authors describe the detection, interpretation, and removal of the signal resulting from interactions of high energy particles with the Planck High Frequency Instrument (HFI) using a joint fit of population templates.
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Cosmic Microwave Background Anisotropy Induced by Cosmic Strings on Angular Scales ≳15′

TL;DR: In this article, the angular power spectrum of the cosmic microwave background (CMB) induced by cosmic strings on angular scales was estimated using a numerical simulation of a cosmic string network; and decomposed this pattern into scalar, vector, and tensor parts.