  We describe a new sample of Seyfert nuclei discovered during the course of an
optical spectroscopic survey of nearby galaxies. The majority of the objects,
many recognized for the first time, have luminosities much lower than those of
classical Seyferts and populate the faint end of the AGN luminosity function. A
significant fraction of the nuclei emit broad H-alpha emission qualitatively
similar to the broad lines seen in classical Seyfert 1 nuclei and QSOs.
