QSO Polarization in the Era of Deep Surveys and Large Telescopes

Details QSO Polarization in the Era of Deep Surveys and Large Telescopes QSO Polarization in the Era of Deep Surveys and Large Telescopes

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..311..371s&link_type=abstract

AGN Physics with the Sloan Digital Sky Survey, Proceedings of a conference held in Princeton, NJ, USA, 27-31 July 2003, Edited b

Physics

Scientific paper

New, deep surveys are 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 are providing the means for studying in detail the origin of the polarization. Among the new results are several strongly polarized, obscured, broad-line QSOs where spectropolarimetry may reveal structural details on scales smaller than the broad-line region.

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