Very high energy afterglow of structured jets: GW 170817 and prospects for future detections

Open Access

Fig. 12.

Evolution of $γ_{c} / {\hat{γ}}_{c}$ $\gamma_{\mathrm{c}} / \widehat{\gamma}_{\mathrm{c}}$ (top) and of the Compton parameter at γ_c, Y(γ_c) (bottom) in the core jet. These quantities are plotted as a function of the observer time for the moderate (solid line) and optimistic (dashed line) reference cases (see Table 6) in the “SSC (Thomson)” case (green) and in the “SSC (with KN)” case (orange).

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