The Spectral Energy Distributions of AGN with Double-Peaked Balmer Lines
  We summarize the optical, UV, and X-ray properties of double-peaked emitters -- AGN with double-peaked Balmer emission lines believed to originate in the AGN accretion disk. We focus on the X-ray spectroscopic results obtained from a new sample of the 16 broadest Balmer line AGN observed with Chandra and Swift. 
I. Strateva (1), W. N. Brandt (2), M. Eracleous (2), G. Garmire (2),   S. Komossa (1) ((1) MPE, (2) Penn State)