REFLECTION SPECTROSCOPY OF THE SEYFERT 1.5 AGN ESO 362-G18

We propose simultaneous 100 ks XMMNewton and NuSTAR observations of the Seyfert1.5 galaxy ESO 362G18 for the purpose of making a detailed study of thespectrum of radiation reflected from the inner accretion disk. Our chief aim isto constrain both the spin of the black hole and the properties of the coronathat illuminates the disk. The combination of NuSTARa??s highsensitivity in thehard Xray band, the softband coverage of XMMNewton, and our stateoftheartrelativistic reflection models will allow us to break degeneracies betweendifferent possible scenarios, and impose tight constraints on the accretiongeometry and black hole spin of this bright AGN. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]