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Gamma-Ray Bursts Reveal the History and Faint Contributors of Cosmic Reionization

  • Authors: Jing-Meng Hao, Paolo Cassata, Zhen-Ya Zheng, Andrea Grazian, Giulia Rodighiero, Alvio Renzini, Jun-Hui Fan, Andrea Ferrara

Jing-Meng Hao et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 5.

Evolution of the observable fraction of star formation, ﹩{f}_{{\rm{obs}}}(z)={\dot{\rho }}_{\star }^{{\rm{obs}}}(z)/{\dot{\rho }}_{\star }^{{\rm{tot}}}(z)﹩, where ﹩{\dot{\rho }}_{\star }^{{\rm{obs}}}(z)﹩ and ﹩{\dot{\rho }}_{\star }^{{\rm{tot}}}(z)﹩ represent the SFRDs in observable galaxies with MUV ≤ −17 and all galaxies, respectively. Shown are the results integrated from the two LF models (Schechter as the orange line, and DPL as the purple line).

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