With the 0.5-10.0 keV background nearly resolved (e.g., Giacconi et al. 2000; Cowie et al. 2002), the emphasis has shifted towards understanding the nature of the faint X-ray population — a clear necessity if we wish to understand the formation and evolution of active galactic nuclei (AGN). Here we report on preliminary spectral and temporal Xray studies of AGN in the 2 Ms Chandra Deep Field-No...