Fig. C.1

Photometry of HD 114082 showing excess flux (black dots) over the photosphere (red line). The blue solid line is the best-fit model SED corresponding to the MLOCI+ADI model in Table B.1 (disk inner radius of 27.6 au and γ = 3.9; see text for details) with a grain radius of 7.2 μm and grain size power-law index, q = 4.25. The dashed lines are the SED contributions of different grain diameters spaced evenly on a log scale (light green for 10 μm, blue for 19 μm, ..., purple for 1056 μm).
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