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[ascl:1804.024] LFlGRB: Luminosity function of long gamma-ray bursts

LFlGRB models the luminosity function (LF) of long Gamma Ray Bursts (lGRBs) by using a sample of Swift and Fermi lGRBs to re-derive the parameters of the Yonetoku correlation and self-consistently estimate pseudo-redshifts of all the bursts with unknown redshifts. The GRB formation rate is modeled as the product of the cosmic star formation rate and a GRB formation efficiency for a given stellar mass.

Code site:
https://github.com/DebduttaPaul/luminosity_function_of_LGRBs_using_Swift_and_Fermi
Appears in:
http://adsabs.harvard.edu/abs/2018MNRAS.473.3385P
Bibcode:
2018ascl.soft04024P

ascl:1804.024
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