Image Details
Caption: Figure 7.
Differential fluence distributions of bursts from all sample (black), SGR J1935+2154 (orange), SGR J1550−5418 (green), SGR 1806−20 (blue dashed line ), and 1E 1841−045 (red dashed line). The best-fitting PL model is overlaid on each distribution. The fluence values were calculated over the 8−200 keV energy range.
© 2026. The Author(s). Published by the American Astronomical Society.