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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: XLIII. Spectral energy distribution of dust in clusters of galaxies

R. Adam, +249 more
TL;DR: In this article, the spectral energy distribution (SED) of the infrared spectrum of thermal dust emission in clusters of galaxies was obtained by using a stacking approach for a sample of several hundred objects from the Planck cluster sample; this procedure averaged out fluctuations from the IR sky, allowing to reach a significant detection of the faint cluster contribution.
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Planck 2013 results. IX. HFI spectral response

Peter A. R. Ade, +273 more
TL;DR: In this article, the Planck High Frequency Instrument (HFI) spectral response was determined through a series of ground-based tests conducted with the HFI focal plane in a cryogenic environment prior to launch.
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Planck intermediate results. XLI. A map of lensing-induced B-modes

Peter A. R. Ade, +238 more
TL;DR: In this article, an all-sky template map of the lensing-induced B-modes using a real-space algorithm that minimizes the impact of sky masks is presented.
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Planck intermediate results - XXXIV. The magnetic field structure in the Rosette Nebula

Nabila Aghanim, +236 more
TL;DR: In this article, the magnetic field structure of the Rosette nebula was studied using the Planck intensity map and rotation measure (RM) data from a massive star-forming region in the Monoceros molecular cloud.
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Archeops in-flight performance, data processing, and map making

J. F. Macías-Pérez, +76 more
TL;DR: Archeops is a balloon-borne experiment inspired by the Planck satellite and its high frequency instrument (HFI) which is designed to measure the cosmic microwave background (CMB) temperature anisotropies at high angular resolution (~12 arcmin) over a large fraction of the sky (around 30%) at 143, 217, 353, and 545 GHz.