X-ray Reprocessing Features in the z=1.265 Quasar 4C 06.41

XMM may prove to be the premier instrument for studying Fe K lines in quasars. We propose a 60 ksec XMM observation of the z1.265 quasar 4C 06.41 to study the Fe Kalpha emission line detected with ASCA as well as other features of reflection and intrinsic absorption. 4C 06.41 is an Xray bright radio loud quasar and is one of the few highz quasars to possess a significant Fe Kalpha line. Since Fe K lines in highz quasars are so rare, this makes 4C 06.41 an excellent target to help expand our knowledge of quasars in the highz regime. XMM is needed to improve upon the signaltonoise available from the archival ASCA spectrum in order to make useful measurements of the line and continuum. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]