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A [gamma]-ray burst at a redshift of z [asymptotically =] 8.2
Long-duration γ-ray bursts (GRBs) are thought to result from the explosions of certain massive stars^sub 1^, and some are bright enough that they should be observable out to redshifts of z>20 using current technology^sup 2-4^. Hitherto, the highest redshift measured for any object was z=6.96, for...
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Published in: | Nature (London) 2009-10, Vol.461 (7268), p.1254 |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Article |
Language: | English |
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Online Access: | Get full text |
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Summary: | Long-duration γ-ray bursts (GRBs) are thought to result from the explosions of certain massive stars^sub 1^, and some are bright enough that they should be observable out to redshifts of z>20 using current technology^sup 2-4^. Hitherto, the highest redshift measured for any object was z=6.96, for a Lyman-α emitting galaxy^sup 5^. Here we report that GRB 090423 lies at a redshift of z[asymptotically =]8.2, implying that massive stars were being produced and dying as GRBs~630 Myr after the Big Bang. The burst also pinpoints the location of its host galaxy. [PUBLICATION ABSTRACT] |
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ISSN: | 0028-0836 1476-4687 |
DOI: | 10.1038/nature08459 |