Spectral energy distributions corresponding to our models of RY Lup: M50 for an inclination of 50° with r_in = 0.12 au (black solid line) and r_in = 0.17 au (red dashed line), and M70 for an inclination of 70° (black dotted-line) compared with the photometric measurements (orange circles; Table 2), the X-shooter spectrum (blue crosses), and the Spitzer/IRS spectrum (red plus). The green lines display the SEDs calculated with the disk parameters of M50 (dashed line) and of M70 (dotted line) models but using the stellar parameters (T_eff, L_*), and the inclination of 75° used by Langlois et al. (2018). See text for details.