SED disk models for GM Aur (left) and J1615 (right). The total model (blue) consists of the photosphere (dotted gray line), outer disk (dashed gray line), and the optically thin inner dust component (solid gray line). Best-fit parameters can be found in Section 3.2 and Table 5. Photometry is de-reddened using the J. S. Mathis (1990) extinction law with A_V = 0.0 for J1615 and A_V = 0.6 for GM Aur (both from C. F. Manara et al. 2014). Labels refer to the observing mission/instrument and their references are included in Table 8 in Appendix B.