Image Details
Caption: Figure 14.
Nonthermal X-ray “prompt emission” at Eobs = 1 keV in the observer’s frame, based on the extrapolated Band function. The jet duration is tobs = 10 s for on-axis (θv = 0°) observers. In the on-axis lightcurves, the power-law decay at tobs > 10 s arises from the high-latitude emission. The blue (θv = 0°), orange (θv = 6°), and green (θv = 8°) lightcurves correspond to different viewing angles. Solid and dashed lines are for different jet Lorentz factors of Γj = 300 and 100, respectively.
© 2026. The Author(s). Published by the American Astronomical Society.