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Supervised detection of exoplanets in high-contrast imaging sequences

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Academic year: 2021

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Fig. 1. The three stages of our supervised detection framework. Panel a: labeled data generation step
Fig. 2. Generation of a labeled dataset. Left panel: procedure for deter- deter-mining the approximation levels and shows the cumulative explained variance ratio as defined by Eq
Fig. 3. MLAR samples from the positive and negative classes obtained with up to 16 singular vectors
Fig. 4. SODIRF and SODINN outputs for the VLT/NACO β Pic dataset.
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