arXiv · astro-ph/0210436
Determining the GRB (Redshift, Luminosity)-Distribution Using Burst Variability
Abstract
We use the possible Cepheid-like luminosity estimator for the long-duration gamma-ray bursts (GRBs) developed by Reichart et al. (2000) to estimate the intrinsic luminosity, and thus the redshift, of 907 long-duration GRBs from the BATSE 4B catalog. We describe a method based on Bayesian inference which allows us to infer the intrinsic GRB burst rate as a function of redshift for bursts with estimated intrinsic luminosities and redshifts. We apply this method to the above sample of long-duration GRBs, and present some preliminary results.
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Timothy Donaghy, Donald Q. Lamb, Daniel E. Reichart, Carlo Graziani. 2002-10-18. Determining the GRB (Redshift, Luminosity)-Distribution Using Burst Variability. https://doi.org/10.1063/1.1579399
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