Comparison of the SEDs of some of the RADMC models in Table B.1. Unless otherwise specified, the models assume well-mixed gas and dust, a disk mass of 0.001 M_⊙ and a standard grain distribution with grain sizes 0.1−10 000 μm and power-law exponent p = −3.5. For examples changing the flaring, thickness, and some of the TD/PTD cases, we show both well-mixed (“Mixed”) and decoupled dust/gas distributions (given by various H/R relations and outer disk thickness (H/R)_out).