Representative examples of the three model families used to fit the AGN spectra in this work. Each panel shows an observed AGN spectrum (gray), together with the corresponding best-fit model (black dashed line). The contribution from the elliptical accretion disk is shown in gold, while all nondisk line-emission components (narrow lines and the broad Gaussian) are shown in cyan. These examples illustrate the qualitative behavior of the disk+BLR, no BLR, and no disk model families (see Section 4) and highlight the different ways in which disk and nondisk components combine to reproduce the observed Hα line profiles.