Fig. 2

All face-on, 5–5000 au simulated SEDs, and the stellar SED MARCS model (in black). The dust masses are 10−4 (blue), 10−5 (green), 10−6 (red), 10−7 (cyan), and 10−8 M⊙ (magenta). Top row: SEDs from CSE with 100% sphere, spiral and disc, respectively. Second row: combined sphere-spiral model SEDsand a comparison between the photometry listed in Table 2 (orange data points) and the MARCS model.
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