Extended Data Fig. 1: Prompt-emission light curves for different detectors.
From: Observation of inverse Compton emission from a long γ-ray burst
a–f, Light curves for Super-AGILE (a; 20–60 keV), Swift-BAT (b; 15–150 keV), Fermi-GBM (c; 10–1,000 keV), AGILE-MCAL (d; 0.4–1.4 MeV), AGILE-MCAL (e; 1.4–100 MeV) and Fermi-LAT (f; 0.1–10 GeV). The light curve of AGILE-MCAL is split into two bands to show the energy dependence of the first peak. Error bars show 1σ statistical errors.
