The jet-disk connection in luminous radio-loud quasars

We propose to perform EPIC spectroscopy and OM photometry of 4 powerfulradioloud quasars with known large scale radio/X properties, and where an Feline was detected at 67 keV in our short Chandra observations. The proposedobservations will enable us to: 1) Quantify the Fe line profile and determineits origin; 2) Determine the shape of the underlying Xray continuum; and 3)Constrain the broadband SEDs, in particular search for thermal UV emissionwhich is asignature of standard disks. Ultimately, this will allow us to discernthe relative roles of beamed and isotropic radiation from the cores of RL AGN,yielding information on the jetdisk connection and on the origin of the RL/RQAGN division. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]