The authors report candidate quasi-periodic oscillations at 2.5 to 3.5 Hz in four GRBs and identify them with a pre-merger neutron star's spin, though trial-corrected significances are low.
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X-ray and gamma-ray timing of GRB 180720B, GRB 181222B, GRB 211211A and GRB 220910A observed with Fermi and ASIM
The authors report candidate quasi-periodic oscillations at 2.5 to 3.5 Hz in four GRBs and identify them with a pre-merger neutron star's spin, though trial-corrected significances are low.