The Broad Line Radio Galaxy 3C 382

It is proposed to obtain the first XMMNewton observation of the Broad LineRadio Galaxies 3C382. This object is characterised by warm absorption in thesoft Xray spectrum and a controversial Fe line the origin of which is stilllargely unknown. In earlier data it appears to be extremely broad (ASCA),possibly relativistically broadened, while it is reported unresolved andconsistent with an origin in distant reflection in BeppoSAX data. Thecapabilities of XMMNewton will be fully exploited. It will be possible to studyin detail the FevirgulK line profile and the jet contribution to the soft Xrayspectrum using a high S/N pn spectrum and it will be possible to elucidate thepresence of Xray absorption thanks to the RGS high resolution data. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]