Fig. 13.
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Period posteriors for all three instruments for the full light curves (left) and for the light curves without the Fermi/GBM BTIs of 2.5–7.5 s after trigger (right). The posteriors show a remarkable degree of agreement between the three instruments, at frequencies corresponding to ∼1.2 Hz (0.83 s period) for the full light curves and at ∼2.9 Hz (0.34 s) without BTI.
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