What can we learn on the BLR from the smallest AGN? Or, how do the BLR properties change with luminosity, and what is it telling us? Specifically The BLR.
July 4, 2006 P. Padovani, Unidentified -ray Sources 1 The Blazar Sequence: Validity and Predictions Paolo Padovani (ESO) Blazar properties The Blazar.
Introduction Active Galactic Nuclei Reprocessed Radiation: IR, NLR/BLR, X-rays.
AGN and Surveys with the new X-ray observatories
Muliti-frequency observations of Blazars
