Fig. 3.
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Spectral fits to the afterglow observations of GRB 190114C at 90 s (black data points taken from MAGIC Collaboration 2019b). Each colour represents the best-fit spectrum for each of the possible radiative regimes (see text and Fig. 4). The spectral cases are detailed in Appendix B. This figure can be compared to Fig. 6 in Yamasaki & Piran (2022), which shows very similar fits.
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