Skip navigation
Skip navigation

A γ-ray burst at a redshift of z ≈ 8.2

Tanvir, Nial R; Fox, Derek B; Levan, A. J.; Berger, E; Wiersema, K; Fynbo, J. P. U; Cucchiara, A; Kruhler, T; Gehrels, N; Bloom, J S; Greiner, J; Dopita, Michael; Schmidt, Brian; Wolf, Christian


Long-duration γ-ray bursts (GRBs) are thought to result from the explosions of certain massive stars, and some are bright enough that they should be observable out to redshifts of z 20 using current technology. Hitherto, the highest redshift measured for

CollectionsANU Research Publications
Date published: 2009
Type: Journal article
Source: Nature
DOI: 10.1038/nature08459


File Description SizeFormat Image
01_Tanvir_A_γ-ray_burst_at_a_redshift_of_2009.pdf379.45 kBAdobe PDF    Request a copy

Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.

Updated:  20 July 2017/ Responsible Officer:  University Librarian/ Page Contact:  Library Systems & Web Coordinator