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Fig. 13.

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Reconstructions of the polarized intensity Ip of the transition disks RY Lupus, T Chae, and RXJ 1615. From the left to the right, the reconstructions have been obtained with the Double Difference, RHAPSODIE without deconvolution and RHAPSODIE with deconvolution. The maps are displayed in logarithmic scale and normalized in contrast to the unpolarized stellar flux. The pixels lying underneath the coronograph are masked in black. North is up and east is to the left in all frames.

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