A photometric redshift of z = 6.39 0.12 for GRB 050904
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Altmetric Citations
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
Collections | ANU Research Publications |
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Date published: | 2006 |
Type: | Journal article |
URI: | http://hdl.handle.net/1885/30227 |
Source: | Nature |
DOI: | 10.1038/nature04552 |
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