Fig. 3
Top: 3−79 keV background-subtracted images of the NuSTAR observation of PG1247 (FPMA left and FPMB right). Contamination from the Coma cluster is visible in the upper left corner of FPMA. Bottom: 15−30 keV NuSTAR images, not background subtracted. In both panels the 1′ scale is shown, and the source and background extraction regions are shown with continuous and dashed lines, respectively. North is up and east is left.
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