XMM Observations of the misaligned Blazar PKS0521-365

We propose to observe the blazar PKS 0521365 for 70 ks with EPIC imaging andspectroscopy. We intend to establish the presence of the Fe Kalpha line,or lackthereof, which will enable a direct measurement or to put strict limits on theparameters of the accretion disk. At the same time we would be able to imagethe halo detected by ROSAT in much better detail : we intend to study its spatial and spectral parameters and to determine the physical parameters of the cooling flow, like the pressure surrounding the optical jet: this sourceis unique showing inflow and outflow on comparable scales Usage of the OM with the UV grism will allow measurement of the Ly alpha intensity and of the UV spectrum at the same time of the Xray observation. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]