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Fig. 3

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MiRA image reconstructions as a function of the assumed chromatic parameters: the stellar-to-total-flux ratio and the dust spectral index denv. The star is represented in red at the center of each image. The true values are and denv = 1. Top right: χ2 map of the reconstructions as a function of the chromatic parameters for reconstructions with the total variation regularization. All χ2sup3 are represented in black. The blue crosses represent the location of the images in the χ2 map. We can clearly see that this map is degenerated.

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