Reflection spectra from thick (Polish donut) accretion disks, when analyzed with thin-disk models, bias black hole spin upward and can create or mask apparent deviations from the Kerr metric.
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Reflection spectra of thick accretion disks
Reflection spectra from thick (Polish donut) accretion disks, when analyzed with thin-disk models, bias black hole spin upward and can create or mask apparent deviations from the Kerr metric.