Fig. A.2
Simulated surface brightness with debris disks composed of the icy dust mixture from near-IR to submm wavelengths at λobs = 2.2, 3.5, 10, 44, and 1000 μm. Different fractional ratios of ice 
are considered (indicated in each row). Ice (a), ice (c), and astrosil indicate amorphous ice, crystalline ice, and astrosilicate, respectively.
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