What is the redshift of gamma-ray burst 970508?
Astrophysics
2007-05-23 v1
Abstract
A Bayesian likelihood analysis is used to constrain the redshift of the optical transient associated with gamma-ray burst 970508, under the assumption that the absorption at redshift 0.835 is not physically associated with the transient. The maximum-likelihood, expectation value and 95-percent upper limit on the OT redshift are 0.835, 1.3 and 1.9 respectively.
Cite
@article{arxiv.astro-ph/9706068,
title = {What is the redshift of gamma-ray burst 970508?},
author = {Nahum Arav and David W. Hogg},
journal= {arXiv preprint arXiv:astro-ph/9706068},
year = {2007}
}
Comments
6 pages, including 2 figures, submitted to ApJ Letters