Extended Data Table 1 Energy flux between 0.3 and 1 TeV in selected time bins for GRB 190114C

From: Teraelectronvolt emission from the γ-ray burst GRB 190114C

  1. Values listed correspond to the light curve in Fig. 1. For each time bin, columns represent the start and end time of the bin, the EBL-corrected energy flux in the 0.3–1 TeV range, and the best-fit spectral photon indices. The last row reports the value of the intrinsic spectral index for the time-integrated spectrum (Fig. 2). The reported statistical errors (stat) correspond to one standard deviation, whereas systematic errors (sys) are derived from the variation of the light scale by ±15% (see Methods).