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Probing Evolution of Long Gamma-Ray Burst Properties through Their Cosmic Formation History

  • Authors: Nikita S. Khatiya, Maria Giovanna Dainotti, Aditya Narendra, Dhruv S. Bal, Aleksander Ł. Lenart, Dieter H. Hartmann

Nikita S. Khatiya et al 2025 The Astrophysical Journal 990 .

  • Provider: AAS Journals

Caption: Figure 3.

Left panels: cumulative LGRB density distribution for the raw (blue) and corrected (orange) cases. The black solid line corresponds to the piecewise functional fit used to calculate the LGRB-RD later. Right panels: log–log distribution of Φ(L) and L (erg s−1). The blue and orange open stars show the raw and corrected Φ ( > L) points, respectively. The black dashed lines correspond to the best-fit functions described in Equation (11). Residuals for raw and corrected σ (z), and raw and corrected Φ (>L) cases are shown in the bottom panel.

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