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Cosmological Evolution of Gamma-Ray Bursts

  • Authors: Sujay Champati, Vahé Petrosian, Maria G. Dainotti

Sujay Champati et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 9.

Robustness of the reconstructed luminosity function and cumulative formation-rate evolution for the non-ML GRB catalog to the uncertainty in the luminosity evolution parameter k. Curves are shown for the best-fit value of k and for the two values corresponding to the 1σ EP range, defined by τ = ±1. The luminosity functions and cumulative formation rates retain nearly the same shape across the allowed range of k, differing primarily in normalization.

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