Notes. All models are constructed for M_∗ = 1.0 M_⊙, R_∗ = 1.7 R_⊙ (typical of low-mass stars in Cep OB2) and outer disk radius R_out=200 AU. Models with well-mixed dust and gas in hydrostatic equilibrium are marked in the disk structure parameters with “v”. Otherwise, we give the vertical scale height at the outer radius [(H/R)_out] and the power-law exponent of the disk surface (H/R ∝ R^q). The ID names of the models include some information about the disk mass (massive [M], intermediate-mass [I], low-mass [L]), the vertical scale height (vertical hydrostatic equilibrium [V] for models with well-mixed gas and dust, normal flaring with q = 1 / 7 [F], settled/flat disks with q = 0 [S], very flared disks with q = 1/4 [XF], together with the value of (H/R)_out if no vertical iteration is performed), indication of inner holes/gaps (inner hole in transitional disk [TD] with innermost disk temperature, radial temperature at which radial properties change in pre-transitional disk [PTD]), followed by the grain distribution (with p = 2.5 or p = 3.5) and a label in case we consider grains up to 100 μm only (sm).