A DEEP SPECTRAL-TIMING STUDY OF THE X-RAY BRIGHT AGN 1H 1934-963

NuSTAR can make a transformational advance in our understanding ofhow luminous accreting black holes work through long observations ofrapidlyvariable, Xraybright AGN. This enables Xray reverberationstudies, already a commonplace feature of AGN, to proceed to the nextlevel and follow the behavior of the powerful dynamic corona and map theaccretion flow immediately next to the black hole, measuring both spinand mass of the black hole. We propose a 500ks NuSTAR observation of theXray brightest high variability NLS1 AGN 1H1934063, with 260ks of XMM, tomeasure relativistic reflection and reverberation in 3 flux states. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]