FWHM_Hα,broad versus Log L_Hα,broad for our sample of BLAGNs. The points are colored by redshift. Along with our BLAGNs, we overlay other BLAGNs found by X. Lin et al. (2024) (•), J. E. Greene et al. (2024) (▴), R. Maiolino et al. (2024) (♦), Y. Harikane et al. (2023) (⬠), B. Trakhtenbrot et al. (2011) (◂) , and C. J. Willott et al. (2010) (▸). BLAGNs identified in this study are shown as ⋆. Similarly as Figure 3, contours show low-z AGNs from redshifts 1–2 (Q. Wu & Y. Shen 2022). Outlined points are known LRDs; see Section 5.3.