All 5–5000 au simulated dust SEDs – without the stellar SED model – of dust masses 10⁻⁴ (blue), 10⁻⁵ (green), 10⁻⁶ (red), 10⁻⁷ (cyan), and 10⁻⁸ M_⊙ (magenta). The dust cloud morphology and inclination are indicated in the top right courner of each panel. The long wavelength portion of the SEDs (> 2 μm) are primarily dust heat emission while the short wavelength portion (<2 μm) are scattered light on dust from the star.