Figure 1 from Analysis and Modeling of the Multi-wavelength Observations of the Luminous GRB 190114C

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Analysis and Modeling of the Multi-wavelength Observations of the Luminous GRB 190114C

Authors: N. Fraija, S. Dichiara, A.C. Caligula do E. S. Pedreira, A. Galvan-Gamez, R.L. Becerra, R. Barniol Duran, and B.B. Zhang

2019 The Astrophysical Journal Letters 879 L26.

Provider: AAS Journals

Caption: Figure 1.

Upper panel: Fermi-LAT energy flux (blue) and photon flux (red) light curves obtained between 0.1 and 300 GeV. The solid black line represents the best-fit curve found using our model. Lower panel: all the photons with energies >100 MeV and probabilities >90% of being associated with GRB 190114C. Fermi-LAT data were reduced using the public database at the Fermi website.

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