no code implementations • 8 Aug 2020 • M. Cruces, L. G. Spitler, P. Scholz, R. Lynch, A. Seymour, J. W. T. Hessels, C. Gouiffès, G. H. Hilmarsson, M. Kramer, S. Munjal
We model the bursts cumulative energy distribution, with energies from ${\sim}10^{38}$-$10^{39}$ erg, and find that it is well described by a power-law with slope of $\gamma=-1. 1\pm 0. 2$.
High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
no code implementations • 6 Mar 2019 • K. Gourdji, D. Michilli, L. G. Spitler, J. W. T. Hessels, A. Seymour, J. M. Cordes, S. Chatterjee
The bursts are generally detected in less than a third of the 580-MHz observing bandwidth, demonstrating that narrow-band FRB signals may be more common than previously thought.
High Energy Astrophysical Phenomena
no code implementations • 5 Feb 2019 • L. J. M. Houben, L. G. Spitler, S. ter Veen, J. P. Rachen, H. Falcke, M. Kramer
A significant variation was observed in the burst repeat rate R at L-band.
High Energy Astrophysical Phenomena
