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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 2.

Nonevolving luminosity L ₀ = L/(1 + z)^6.66 of 439 FRBs. The blue dots represent FRBs, and the blue solid line represents the observational limit considering the impact of k.

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