Four shapes of SEDs sorted according to the criteria in Table 2. The SEDs are normalized to 1 μm to emphasize the emission of the AGN. Note the break between 10⁻³ μm and 0.5 × 10⁻² μm where there is no data. For each shape, the bold black line shows the median SED. Almost half the AGN (94/194) are in Shape 3, as in C. Auge et al. (2023) (note: C. Auge et al. 2023 breaks the SEDs into five panels; our Shape 1–2 is a combination of their Shape 1 and Shape 2 due to the dearth of unobscured AGN in our sample). 51% of Shape 3 galaxies have FIR (100 μm detections) higher than both Shape 4 (45%) and Shape 5 (12%).