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The Formation Rate and Luminosity Function of Fast Radio Bursts

  • Authors: J. H. Chen, X. D. Jia, X. F. Dong, F. Y. Wang

J. H. Chen et al 2024 The Astrophysical Journal Letters 973 .

  • Provider: AAS Journals

Caption: Figure 7.

Comparison between the formation rate of FRBs and other events. The red line represents the formation rate of FRBs. The green and blue lines represent the rates of short GRBs (G. Q. Zhang & F. Y. Wang 2018) and long GRBs (H. Yu et al. 2015), respectively. The gray dots and blue dashed line correspond to the observed SFR and the best fit (A. M. Hopkins & J. F. Beacom 2006), respectively.

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