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A photometric redshift of z = 6.39 0.12 for GRB 050904

Haislip, J B; Nysewander, M C; Reichart, D E; Levan, A; Cenko, Stephen B; Fox, Derek B; Price, Paul Antony; Castro-Tirado, A J; Figueredo, E; Cypriano, E S; Graham, J; Rhoads, J; Lamb, D Q; Kouveliotou, C; Wijers, R A M J; Schmidt, Brian; Harrison, F A; Hudec, R; Vitek, S; Kubanek, P; Canterna, R; Hartmann, D H; Henden, A A; Klose, S; Park, H-S; Williams, G G; Rol, E; Bersier, D; Jarvis, M J; Gehrels, N

Description

Gamma-ray bursts (GRBs) and their afterglows are the most brilliant transient events in the Universe. Both the bursts themselves and their afterglows have been predicted to be visible out to redshifts of z ≈ 20, and therefore to be powerful probes of th

CollectionsANU Research Publications
Date published: 2006
Type: Journal article
URI: http://hdl.handle.net/1885/30227
Source: Nature
DOI: 10.1038/nature04552

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