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D

D. Santos

Researcher at University of Grenoble

Publications -  175
Citations -  67015

D. Santos is an academic researcher from University of Grenoble. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 85, co-authored 163 publications receiving 63310 citations. Previous affiliations of D. Santos include Joseph Fourier University & Centre national de la recherche scientifique.

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Planck intermediate results: XXXVIII. E- and B-modes of dust polarization from the magnetized filamentary structure of the interstellar medium

Peter A. R. Ade, +248 more
TL;DR: In this article, a statistical study of the filamentary structure of the Planck Stokes maps at high Galactic latitude is presented, relevant to the study of dust emission as a polarized foreground to the CMB.
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Planck 2013 results. III. LFI systematic uncertainties

Nabila Aghanim, +218 more
TL;DR: In this paper, the authors present the current estimate of instrumental and systematic effect uncertainties for the Planck-Low Frequency Instrument relevant to the first release of Planck cosmological results.

Overview of products and scientific results

R. Adam, +354 more
TL;DR: The European Space Agency's Planck satellite, dedicated to studying the early Universe and its subsequent evolution, was launched 14~May 2009 and scanned the microwave and submillimetre sky continuously between 12~August 2009 and 23~October 2013 as discussed by the authors.
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The CMB temperature power spectrum from an improved analysis of the Archeops data

TL;DR: In this paper, the angular power spectrum of the Cosmic Microwave Background (CMB) temperature anisotropies using the data from the last Archeops flight was improved by using the 6 most sensitive photometric pixels in the CMB bands centered at 143 and 217 GHz and 20% of the sky mostly clear of foregrounds.
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Planck 2013 results. III. LFI systematic uncertainties

P. A. R. Ade, +221 more
TL;DR: In this article, the authors present the current accounting of systematic effect uncertainties for the Low Frequency Instrument (LFI) that are relevant to the 2015 release of the Planck cosmological results, showing the robustness and consistency of our data set, especially for polarization analysis.