A cumulative search for hard X/-Ray emission associated with fast radio bursts in Fermi/GBM data
arXiv:1909.07165 · doi:10.1051/0004-6361/201936284
Abstract
Context. Fast Radio Bursts (FRBs) are millisecond-long bursts uniquely detected at radio frequencies. FRB 131104 is the only case for which a -ray transient positionally and temporally consistent was claimed. This high-energy transient had a duration of ~s and a 15-150~keV fluence erg . However, the association with the FRB is still debated. Aims. We aim at testing the systematic presence of an associated transient high-energy counterpart throughout a sample of the FRB population. Methods. We used an approach like that used in machine learning methodologies to accurately model the highly-variable Fermi/GBM instrumental background on a time interval comparable to the duration of the proposed -ray counterpart of FRB 131104. A possible -ray signal is then constrained considering sample average lightcurves. Results. We constrain the fluence of the possible -ray signal in the 8-1000 keV band down to () erg cm for a 200-s (1-s) integration time. Furthermore, we found the radio-to-gamma fluence ratio to be Jy ms erg cm. Conclusions. Our fluence limits exclude of Fermi/GBM detected long gamma-ray bursts and of Fermi/GBM detected short gamma-ray bursts. In addition, our limits on the radio-to-gamma fluence ratio point to a different emission mechanism from that of magnetar giant flares. Finally, we exclude a -ray counterpart as fluent as the one possibly associated with FRB 131104 to be a common feature of FRBs.
arXiv comment8 pages, 6 figures, Accepted on A&A
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