Open Access

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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