Near-IR diagnostic diagrams including Fe2S3-β, Fe2S3-α, P2S3, and C1S3. This figure is the analog of Fig. 8, but the emission line predictions for the NLR of AGNs are obtained using the AGN models described in Thomas et al. (2016, 2018). The markers, sizes, and colors of AGN models are the same as described in Fig. B.1. The star-forming models are the same as in Fig. 8. The maximum starburst and AGN lines are defined in Section 4.1 and in Table 6.