Image Details
Caption: Figure 2.
Afterglow light curves in the X-ray (5 keV; orange), near-infrared (2 × 1014 Hz; blue), and radio (1.3 GHz; red) bands, compared with the observed data of GRB 250702B (X-ray: orange circles; near-infrared: blue diamonds; radio: red squares). The thick solid and thin dashed lines denote the predicted emission for the maximum (40 jets) and minimum (four jets) cases, respectively. Black arrows indicate the times of the observed gamma-ray flares.
© 2026. The Author(s). Published by the American Astronomical Society.