Image Details
Caption: Figure 8.
Corner plots of the posterior distributions for the jet+cocoon model using VegasAfterglow code. As seen from these plots, the collimated corrected energy of the jet is reaching the highest value we impose as an upper limit for our prior, 3 × 1052 erg, the initial Lorentz factor of the jet is unconstrained and therefore serves as a lower limit. In addition, the observing angle is also reaching the highest value of the prior, θobs = 90°. In Figure 5, we present the radio SEDs with lines drawn from these posterior distributions.
© 2026. The Author(s). Published by the American Astronomical Society.