Best-fit photometric vs. spectroscopic redshift for RUBIES sources with robust z_spec > 3.1 (gray histogram) and the LRD sample (red hexagons; triangle indicates out of plot). Photometric redshifts were measured using eazy Brammer et al. 2008 with two different template sets: the blue_sfhz_13 set optimized for high-redshift galaxies (left) and the agn_blue_sfhz_13 set which includes an AGN template constructed from the LRD of Killi et al. 2024 and a torus model (right). The dashed lines show |Δz|/(1 + z_spec) = 0.1. Although including this AGN template reduces the number of outliers and photometric redshift scatter for the LRD sample, a small bias toward higher photometric redshifts remains.