Gamma-Ray and X-Ray Observations of the Periodic-Repeater FRB 180916 During Active Phases
arXiv:2004.03676 · doi:10.3847/2041-8213/ab86b1
Abstract
FRB 180916 is a most intriguing source at 150 Mpc distance capable of producing repeating fast radio bursts with a periodic 16.35 day temporal pattern. We report on the X-ray and -ray observations of FRB 180916 obtained by AGILE and Swift. We focused on the recurrent 5-day time intervals of active radio bursting and present results obtained on Feb. 3 - 8; Feb. 25; Mar. 5 - 10; Mar. 22 - 28, 2020 during a multiwavelength campaign involving high-energy and radio observations. We also searched for temporal coincidences at millisecond timescales between all known radio bursts of FRB 180916 and X-ray and MeV events detectable by AGILE. We do not detect any simultaneous event or any extended X-ray and -ray emission on timescales of hours/days/weeks. Our cumulative X-ray (0.3-10 keV) flux upper limit of (obtained during 5-day active intervals) translates into an isotropic luminosity upper limit of . Observations above 100 MeV over a many-year timescale provide an average luminosity upper limit one order of magnitude larger. These results provide the so-far most stringent limits on high-energy emission from FRB 180916 and constrain the dissipation of magnetic energy from a magnetar-like source of radius , internal magnetic field and dissipation timescale to satisfy the relation , where is in units of cm, is in units of G, and in units of s.
arXiv commentAccepted for publication by the Astrophysical Journal Letters on April 5, 2020
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