Extended Data Fig. 1: Burst durations and spectral parameters.
From: Broadband X-ray burst spectroscopy of the fast-radio-burst-emitting Galactic magnetar
Time is from 2020 April 28, 00 h. The burst with an asterisk is the one burst where a BB+CPL model is required to provide a statistically good fit to the data. A 2BB model cannot provide a good fit as is evident from the last column. The burst highlighted in bold face is the one presented in Fig. 1 of the main text. Numbers in parentheses represent the 1s uncertainty on the corresponding last digit.
