Mining the Sky for Blazars

Details Mining the Sky for Blazars Mining the Sky for Blazars

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..311..365p&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

We use a large sample of blazars to provide new constraints on the spectral energy distributions and energetics of AGN jets. We have discovered a new population of X-ray loud flat-spectrum quasars, missed by previous radio surveys. The new class are the strong-lined counterparts to high-energy peaked BL Lacs, with UV/X-ray synchrotron peaks. Once these sources are included, we do not find agreement with the blazar sequence scenario. A more complete account of this work has recently appeared (Padovani et al. 2003).

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