A 10-year NuSTAR campaign characterizes the 20-300 mHz QPO of M82 X-1, associates it with the source via Chandra, finds no 3-5 Hz twin QPOs, and argues the QPO is not a reliable black-hole mass indicator.
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A NuSTAR study of quasi-periodic oscillations from the ultraluminous X-ray sources in M82
A 10-year NuSTAR campaign characterizes the 20-300 mHz QPO of M82 X-1, associates it with the source via Chandra, finds no 3-5 Hz twin QPOs, and argues the QPO is not a reliable black-hole mass indicator.