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.
Credit: Paul, Debdutta
Site: https://github.com/DebduttaPaul/luminos ... n_of_lGRBs
Preferred citation method: http://adsabs.harvard.edu/abs/2018MNRAS.473.3385P