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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 7.

Left: formation rates derived from the C method for both the full (blue) and non-ML (red) GRB catalogs. The solid curves indicate the best-fit double-break power-law models. Cumulative luminosity functions for the GRB catalogs. Blue points with a solid fit line represent the full catalog, while red squares with a dashed fit line represent the non-ML subset. Both are fitted with a smooth double power-law model. Right: formation rates derived from the C method for both the full (blue) and non-ML (red) GRB catalogs. The solid curves indicate the best-fit double-break power-law models.

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