Bolometric luminosities versus redshift of the sample of NLAGN selected in this work (red squares) compared to the bolometric luminosities of other AGN samples selected using JWST spectroscopic observations or pre-JWST, as labeled. The darker red squares represent the baseline bolometric luminosities, derived using Netzer (2009) calibration, while the fainter red squares show the values of the bolometric luminosities obtained using the same calibration adopted in Scholtz et al. (2025). The compilation of JWST selected BLAGN includes the sources taken from Maiolino et al. (2024b), Harikane et al. (2023), Matthee et al. (2024), Übler et al. (2023), Kocevski et al. (2023). SDSS BLAGN at z > 3 (light blue crosses) are taken from Wu & Shen (2022). AGN from the KASHz and SUPER surveys at Cosmic Noon (gray and red gold crosses) are taken from Harrison et al. (2016) and Kakkad et al. (2020), respectively. QSOs samples at Epoch of Reionization are taken from Zappacosta et al. (2023) (green crosses, HYPERION sample), and Mazzucchelli et al. (2023) (dark-blue crosses, XQR-30).