Fig. B.1.

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Parameter space exploration between the initial Lorentz factor, kinetic energy, and deceleration time (color coded) under the early afterglow scenario for three distinct uniform-density ISM regimes (from top to bottom: 10−2, 1 and 10 cm−3. As explained in §A, to explore this possibility, we assume a plausible range of parameters for GRBs using Eq. A.1. The red markers represent the condition tdec ≈ tX, peak = 110 ± 50 s.
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