TESTING FOR RELATIVISTIC REFLECTION IN NGC 1052

We propose a 60 ks NuSTAR observation of NGC 1052 with simultaneous XMMNewtoncoverage in order to accurately model the reflection features in this source.NGC 1052 is a LINER with a low Eddington rate that has shown hints of a broad FeKa line but no Compton reflection hump in the past. A short NuSTAR observationof the source, indicated that there may indeed be Compton reflection in thissource and a harder continuum than previously thought. Unfortunately, lack ofstatistics and low resolution in the Fe K bandpass of the current data negatethe possibility of a robust measurement. A longer broadband observation willallow us to robustly measure the reflection signatures and simultaneous XMMcoverage will allow us to carefully and consistently test for relativistic reflection. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]