Long gamma-ray burst rate at very high redshift

20 May 2019 Kinugawa Tomoya Harikane Yuichi Asano Katsuaki

Future missions for long gammma-ray burst (GRB) observations at high redshift such as HiZ-GUNDAM and THESEUS will provide clue to the star formation history in our universe. In this paper focusing on high redshift (z>8) GRBs, we calculate the detection rate of long GRBs by future observations, considering both Population (Pop) I&II stars and Pop III stars as GRB progenitors... (read more)

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  • HIGH ENERGY ASTROPHYSICAL PHENOMENA