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A gamma-ray burst at a redshift of z approximately 8.2.

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posted on 2020-05-12, 14:00 authored by NR Tanvir, DB Fox, AJ Levan, E Berger, K Wiersema, JP Fynbo, A Cucchiara, T Krühler, N Gehrels, JS Bloom, J Greiner, PA Evans, E Rol, F Olivares, J Hjorth, P Jakobsson, J Farihi, R Willingale, RL Starling, SB Cenko, D Perley, JR Maund, J Duke, RA Wijers, AJ Adamson, A Allan, MN Bremer, DN Burrows, AJ Castro-Tirado, B Cavanagh, A de Ugarte Postigo, MA Dopita, TA Fatkhullin, AS Fruchter, RJ Foley, J Gorosabel, J Kennea, T Kerr, S Klose, HA Krimm, VN Komarova, SR Kulkarni, AS Moskvitin, CG Mundell, T Naylor, K Page, BE Penprase, M Perri, P Podsiadlowski, K Roth, RE Rutledge, T Sakamoto, P Schady, BP Schmidt, AM Soderberg, J Sollerman, AW Stephens, G Stratta, TN Ukwatta, D Watson, E Westra, T Wold, C Wolf
Long-duration gamma-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 any object was z = 6.96, for a Lyman-alpha emitting galaxy. Here we report that GRB 090423 lies at a redshift of z approximately 8.2, implying that massive stars were being produced and dying as GRBs approximately 630 Myr after the Big Bang. The burst also pinpoints the location of its host galaxy.

Funding

We thank Ph. Yock, B. Allen, P. Kubanek, M. Jelinek and S. Guziy for their assistance with the BOOTES-3 YA telescope observations (Supplementary Information). This work was partly based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the US National Science Foundation on behalf of the Gemini partnership: the National Science Foundation (United States), the Science and Technology Facilities Council (United Kingdom), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), the Ministério da Ciência e Tecnologia (Brazil) and SECYT (Argentina). This work was also partly based on observations made using ESO telescopes at the La Silla or Paranal observatories by G. Carraro, L. Schmidtobreick, G. Marconi, J. Smoker, V. Ivanov, E. Mason and M. Huertas-Company. The UKIRT is operated by the Joint Astronomy Centre on behalf of the UK Science and Technology Facilities Council. R.J.F. acknowledges a Clay Fellowship.

History

Citation

Nature, 2009, 461 (7268), pp. 1254-1257

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

  • AM (Accepted Manuscript)

Published in

Nature

Volume

461

Issue

7268

Pagination

1254-1257

Publisher

Nature Research (part of Springer Nature)

eissn

1476-4687

Acceptance date

2009-08-19

Copyright date

2009

Available date

2009-10-29

Publisher version

https://www.nature.com/articles/nature08459

Language

eng

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