Image Details
Caption: Figure 3.
Power spectral density of GRB 250706B/C with the light curve from T0−10 s to T0+60 s. The black dashed line and red line are the fitting of a simple power law plus the white-noise constant and bent power law (C. Guidorzi et al. 2016). No narrow feature is detected significantly.
© 2026. The Author(s). Published by the American Astronomical Society.