LFlGRB: Luminosity function of long gamma-ray bursts
Abstract
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.
- Publication:
-
Astrophysics Source Code Library
- Pub Date:
- April 2018
- Bibcode:
- 2018ascl.soft04024P
- Keywords:
-
- Software