Evidence Against an Association Between Gamma-Ray Bursts and Type I Supernovae

dc.creatorGraziani, C.
dc.creatorLamb, D. Q.
dc.creatorMarion, G. H.
dc.date1999-09-01
dc.date.accessioned2026-07-07T02:33:00Z
dc.date.available2026-07-07T02:33:00Z
dc.descriptionWe use a rigorous method, based on Bayesian inference, for calculating the odds favoring the hypothesis that any particular class of astronomical transients produce gamma-ray bursts over the hypothesis that they do not. We then apply this method to a sample of 83 Type Ia supernovae and a sample of 20 Type Ib-Ic supernovae. We find overwhelming odds against the hypothesis that all Type Ia supernovae produce gamma-ray bursts, whether at low redshift ($10^{9}:1$) or high-redshift ($10^{12}:1$), and very large odds ($6000:1$) against the hypothesis that all Type Ib, Ib/c, and Ic supernovae produce observable gamma-ray bursts. We find large odds ($34:1$) against the hypothesis that a fraction of Type Ia supernovae produce observable gamma-ray bursts, and moderate odds ($6:1$) against the hypothesis that a fraction of Type Ib-Ic supernovae produce observable bursts.
dc.descriptionproc. of Gamma-Ray Bursts in the Afterglow Era, Nov. 1998, Rome, F. Frontera & L. Piro eds., A&A Suppl. Ser., in press
dc.identifierhttps://arxiv.org/abs/astro-ph/9909025
dc.identifierhttp://arxiv.org/abs/astro-ph/9909025
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14674
dc.subjectAstrophysics
dc.titleEvidence Against an Association Between Gamma-Ray Bursts and Type I Supernovae
dc.typetext

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