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What can a uniform reflection pipeline establish about supermassive black hole spin? An audit and a corrected analysis of 57 AGN with XMM and NuSTAR
We audit an automated relativistic-reflection pipeline that fitted one XMM-Newton EPIC-pn and NuSTAR epoch for each of 57 AGN with relxillCp+xillverCp, and repeat the analysis with its failures corrected. The pipeline's apparent constraints were not controlled: Small Window pn backgrounds were never
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