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arxiv: 1112.1527 · v1 · pith:JWY6AH73new · submitted 2011-12-07 · 🌌 astro-ph.IM · astro-ph.EP· physics.space-ph· stat.AP

On the unmixing of MEx/OMEGA hyperspectral data

classification 🌌 astro-ph.IM astro-ph.EPphysics.space-phstat.AP
keywords hyperspectralabundanceestimatoromegaunmixingaccountalgorithmalgorithms
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This article presents a comparative study of three different types of estimators used for supervised linear unmixing of two MEx/OMEGA hyperspectral cubes. The algorithms take into account the constraints of the abundance fractions, in order to get physically interpretable results. Abundance maps show that the Bayesian maximum a posteriori probability (MAP) estimator proposed in Themelis and Rontogiannis (2008) outperforms the other two schemes, offering a compromise between complexity and estimation performance. Thus, the MAP estimator is a candidate algorithm to perform ice and minerals detection on large hyperspectral datasets.

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