Spatial-spectral unmixing of hyperspectral data for detection and analysis of astrophysical sourceswith the muse instrument


Detection and analysis of astrophysical sources from the forthcoming MUSE instrument is of greatest challenge mainly due to the high noise level and the three-dimensional translation variant blur effect of MUSE data. In this work, we use some realistic hypotheses of MUSE to reformulate the data convolution model into a set of linear mixing models… (More)
DOI: 10.1109/WHISPERS.2012.6874266


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