Fig. 6
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Modeled SED of debris disks with a narrow belt (ΔR/R ~ 0.17) around an A-type star depending on the underabundance of medium grains (color dot lines). Total emissions (i.e., net SED including the emission from the star and dust) are indicated with solid lines of the same color for the underabundance of medium grains. See Table 5 for details.
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