  The high spectral resolution and sensitivity of FUSE have enabled
far-ultraviolet studies of AGN and QSOs that are a natural complement to
observations using HST, Chandra, and XMM-Newton. Through synergistic use of the
large sample of nearby AGN that serve as background probes of gas in the
Galactic halo and the ISM, the FUSE PI team has observed a large number
(approaching 100) of the nearest and brightest AGN. In addition to emission
from O VI, we identify emission lines due to C III, N III, S IV, and He II in
many of the Type-1 AGN. More than half of the Type 1 objects also show
intrinsic absorption by the O VI doublet as well as C IV absorption and
evidence of a soft X-ray warm absorber. Guest investigators have successfully
coordinated FUSE observations of bright AGN with simultaneous HST and X-ray
observations. These have contributed greatly to our understanding of the UV and
X-ray absoring gas in AGN as either a wind from the accretion disk, or a
thermally driven wind from the obscuring torus.
