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Second Repeating FRB 180814.J0422+73: Ten-year Fermi-LAT Upper Limits and Implications

  • Authors: Yu-Han Yang, Bin-Bin Zhang, and Bing Zhang

2019 The Astrophysical Journal Letters 875 L19.

  • Provider: AAS Journals

Caption: Figure 3.

Constraints on the isotropic kinetic energy of the blastwave and the luminosity distance of the source for the on-axis GRB external shock model. The solid and dotted lines represent for the upper limits of Eiso with the ISM number density n0 = 1 cm−3 and 0.1 cm−3, respectively. The dashed lines are upper limits for the wind model with ﹩{A}_{\star }=0.1﹩. Besides, we set microphysics shock parameters to be εe = 0.1, εB = 0.01, and electron index p = 2.3.

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