NGC 3516: Disk Diagnostics from a Windy BLSy1 in a High-State

Recent advances have shown Xray flux to be simply correlated withreflectionsignatures from the disk and an associated wind. It appears twothings are essential to observe the disk/wind: 1) catch the Seyfert in ahighstate where disk/wind features show up strongly and 2) separate outreprocessing from distant gas to allow isolation of disk/wind features. NGC 3516provides the ideal source for further study in this regard. The source iscurrently in a very high state, which we predict will lead to observablefeatures from the disk and its wind. We request 210 ks XMM exposure on NGC 3156with supporting Chandra time to test our prediction of fluxlinked diskreflection and wind. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]