QSO polarization in the era of deep surveys and large telescopes

New, deep surveys axe uncovering populations of AGN with substantially different spectral energy distributions and polarization properties than have been traditionally cataloged. These differences likely indicate different viewing perspectives and/or nuclear geometries. At the same time, large-aperture telescopes axe providing the means for studying in detail the origin of the polarization. Among the new results axe several strongly polarized, obscured, broad-line QSOs where spectropolarimetry may reveal structural details on scales smaller than the broad-line region.