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François Levrier

Researcher at École Normale Supérieure

Publications -  238
Citations -  69458

François Levrier is an academic researcher from École Normale Supérieure. The author has contributed to research in topics: Planck & Cosmic microwave background. The author has an hindex of 89, co-authored 230 publications receiving 58842 citations. Previous affiliations of François Levrier include Centre national de la recherche scientifique & Max Planck Society.

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Journal Article

French SKA White Book - The French Community towards the Square Kilometre Array

Fabio Acero, +177 more
TL;DR: The publication of this French SKA white paper illustrates the strong involvement in the SKA project of the French astronomical community and of a rapidly growing number of major scientific and technological players in the fields of Big Data, high performance computing, energy production and storage, as well as system integration.
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Velocity centroids and the structure of interstellar turbulence. I. Analytical study

TL;DR: In this article, the authors present an analytical study of the statistical properties of integrated emission and velocity centroids for a slightly compressible turbulent slab model, to retrieve the underlying statistics of three-dimensional density and velocity fluctuations.
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A new approach for the statistical denoising of Planck interstellar dust polarization data

TL;DR: Bregaldo et al. as mentioned in this paper proposed a statistical denoising method based on wavelet phase harmonics (WPH) statistics, which characterized the coherent structures in non-Gaussian random fields and defined a generative model of the data.
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Quantitative inference of the H2 column densities from 3 mm molecular emission: case study towards Orion B

TL;DR: In this paper, a data-driven approach was proposed to determine the H2 gas column densities from radio molecular line observations, which is based on the finding that molecular hydrogen is unobservable in cold molecular clouds, but the relationship between the emission of one molecular line and the column density is non-linear and sensitive to excitation conditions, optical depths, and abundance variations.