We report on a non-detection of radio bursts from the soft gamma-ray repeater SGR 1935+2154 with LOFAR. These LOFAR observations had the goals of i. studying the detailed morphology of the radio bursts in order to potentially compare with the characteristic time-frequency structure seen in repeating FRBs (Hessels et al. 2019) and ii. studying interstellar scattering along this line of sight.
Bassa, C., Hessels, J. W. T., Kondratiev, V., et al. 2020, The Astronomer's Telegram, No. 13707.