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Fig. 4


Vertically integrated dust density distribution after 5 Myr of evolution and the corresponding SEDs (after 1 and 5 Myr), considering a disk with higher temperature (hence rsnow = 1.2 AU), for a planet mass of 1 MJup (left) and 5 MJup (right). For comparison, we plot the SEDs of the reference models (referred to as “cold”).

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