Using a population model, the authors constrain typical newborn magnetar magnetic fields to about 4e14 to 2e15 Gauss and predict that future MeV detectors will be dominated by extragalactic magnetar giant flares.
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Extragalactic Magnetar Giant Flares: Population Implications, Rates and Prospects for Gamma-Rays, Gravitational Waves and Neutrinos
Using a population model, the authors constrain typical newborn magnetar magnetic fields to about 4e14 to 2e15 Gauss and predict that future MeV detectors will be dominated by extragalactic magnetar giant flares.