Differential Source Count for Gamma-Ray Bursts

Shreya Banerjee

doi:10.3847/1538-4357/ac1a6f

Differential Source Count for Gamma-Ray Bursts

2021-11-02

2

OA

AI

DOI：10.3847/1538-4357/ac1a6f

Original

Original request for help

Save

Abstract

En 中文

Different forms of long gamma-ray burst (GRB) luminosity functions are considered on the basis of an explicit physical model. The inferred flux distributions are compared with the observed ones from two samples of GRBs, Swift and Fermi GBM. The best-fit parameters of the luminosity functions are found, and the physical interpretations are discussed. The results are consistent with the observation of a comparable number of flat-phase afterglows and monotonically decreasing ones.

Keywords:

LUMINOSITY FUNCTION

3RD CLASS

REDSHIFT

JETS

DISTRIBUTIONS

EVOLUTION

CATALOG

Differential Source Count for Gamma-Ray Bursts

Abstract

Journal

Organization