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Fig. 3

image

SEDs obtained from the dust density distribution after 1 Myr (upper panel) and 5 Myr (lower panel) for the case of a 1, 5, or 15 MJup mass planet embedded at 20 AU. In the lower panel the dashed line corresponds to the SEDs obtained by assuming a planet mass of 1 MJup, but neglecting the effect of the snow line in the inner disk.

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