REVEALING THE HIGH-VELOCITY ABSORPTION IN IRAS 13349+2438

We propose a 200 ks NuSTAR observation of the z0.1085 quasar IRAS13349+2438, simultaneous with 100 ks of XMMNewton exposure. With this,we will be able to reveal the ultrafast outflow component of the complexabsorption found in this intriguing source. With the unique high energycoverage of NuSTAR, combined with high resolution low energy spectroscopyfrom XMMNewton, we will be able to map out the high energy absorptionlines, completing our knowledge of the ionized absorption. We will explorethe link between the low and high velocity absorbers, and determine theorigin of the relativistic Fe emission at 7 keV, revealing the geometry ofthe AGN system. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]