Fig. D.1

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RSM detection maps generated using the Auto-RSM with the bottom-up (left) and top-down (middle left) approaches to select the optimal set of likelihoods cubes (each likelihood cube corresponds to a PSF-subtraction technique), S/N maps generated using the Auto-SNR to select the optimal set of S/N maps (middle right) and S/N maps obtained by averaging the S/N map generated with APCA, NMF, LLSG, and LOCI (right). The expected position of the planetary signal as estimated via the RSM based planetary signal characterisation algorithm is indicated by a yellow circle.
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