Fig. 12.
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Limits on the energy of X-ray and gamma-ray bursts at the time of radio bursts from FRB 20121102A (in blue; from Scholz et al. (2017) and in green; this work). The 0.5–10 keV data are from Chandra, 10–100 keV from Fermi/GBM and 25–400 keV from INTEGRAL. The dashed lines indicate 5σ upper limits for a single radio burst, whereas the solid lines indicate stacking multiple detected radio bursts. We do not include our optical limit in this plot as that was not obtained concurrently with radio bursts.
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