Fig. 11.
Images of the flux distribution reconstructed by REXPACO comparatively to the PACO, PCA and cADI algorithms. For REXPACO, both the deblurred reconstruction 
and its reblurred version 
are given for comparison with the other considered methods that do not produce deblurred images of the flux distribution. Data sets: HR 4796A, RY Lupi, SAO 206462 and PDS 70, see Sect. 3.3.1 for observing conditions.
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