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Frédéric Schmidt

Researcher at Université Paris-Saclay

Publications -  84
Citations -  1570

Frédéric Schmidt is an academic researcher from Université Paris-Saclay. The author has contributed to research in topics: Mars Exploration Program & CRISM. The author has an hindex of 21, co-authored 78 publications receiving 1218 citations. Previous affiliations of Frédéric Schmidt include ASTRON & University of Grenoble.

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On the decomposition of Mars hyperspectral data by ICA and Bayesian positive source separation

TL;DR: A combination of spatial ICA with spectral Bayesian positive source (BPSS) with a rough classification of pixels is proposed, which allows selection of small, but relevant, number of pixels for the component extraction and consequently the endmember classification.
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Martian dust storm impact on atmospheric H2O and D/H observed by ExoMars Trace Gas Orbiter

Ann Carine Vandaele, +65 more
- 25 Apr 2019 - 
TL;DR: The observed changes in H2O and HDO abundance occurred within a few days during the development of the dust storm, suggesting a fast impact of dust storms on the Martian atmosphere.
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Climatic control of sediment transport from the Himalayas to the proximal NE Bengal Fan during the last glacial-interglacial cycle

TL;DR: In this paper, the authors used deep-sea sediments cored in the north-eastern Bay of Bengal are used to reconstruct evolution of detrital sources and sediment transport to the proximal part of the Bengal deepsea fan during the last climatic cycle.
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Implementation Strategies for Hyperspectral Unmixing Using Bayesian Source Separation

TL;DR: In this paper, the effects of pixel selection and the impact of sampling on the relevance of the estimated component spectra and abundance maps, as well as on the computation times are discussed.
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Formation of recurring slope lineae on Mars by rarefied gas-triggered granular flows.

TL;DR: In this paper, the authors present numerical simulations to demonstrate that such a dry process involving the pumping of rarefied gas in the Martian soil due to temperature contrasts can explain the formation of the recurring slope lineae.