Histogram of intrinsic 0.5–7 keV X-ray luminosities in units of log [erg s⁻¹]. GOODS is unique in that its deep Chandra observations allow us to reliably detect faint, obscured AGN that are selected against when studying fields such as Stripe 82X or COSMOS. In studies such as C. Auge et al. (2023), these low-luminosity (10^42.5 < L_X < 10⁴³ erg s⁻¹) are removed due to potential contamination from luminous starburst galaxies present in larger area surveys. However, our sample constitutes entirely AGN, as verified through the construction of SEDs later in this paper.