A γ-ray burst at a redshift of ≈ 8.2

N. R. Tanvir; D. B. Fox; A. J. Levan; E. Berger; K. Wiersema; J. P.U. Fynbo; A. Cucchiara; T. Krühler; N. Gehrels; J. S. Bloom; J. Greiner; P. A. Evans; E. Rol; F. Olivares; J. Hjorth; P. Jakobsson; J. Farihi; R. Willingale; R. L.C. Starling; S. B. Cenko; D. Perley; J. R. Maund; J. Duke; R. A.M.J. Wijers; A. J. Adamson; A. Allan; M. N. Bremer; D. N. Burrows; A. J. Castro-Tirado; B. Cavanagh; A. De Ugarte Postigo; M. A. Dopita; T. A. Fatkhullin; A. S. Fruchter; R. J. Foley; J. Gorosabel; J. Kennea; T. Kerr; S. Klose; H. A. Krimm; V. N. Komarova; S. R. Kulkarni; A. S. Moskvitin; C. G. Mundell; T. Naylor; K. Page; B. E. Penprase; M. Perri; P. Podsiadlowski; K. Roth; R. E. Rutledge; T. Sakamoto; P. Schady; B. P. Schmidt; A. M. Soderberg; J. Sollerman; A. W. Stephens; G. Stratta; T. N. Ukwatta; D. Watson; E. Westra; T. Wold; C. Wolf

doi:10.1038/nature08459

A γ-ray burst at a redshift of ≈ 8.2

N. R. Tanvir, D. B. Fox, A. J. Levan, E. Berger, K. Wiersema, J. P.U. Fynbo, A. Cucchiara, T. Krühler, N. Gehrels, J. S. Bloom, J. Greiner, P. A. Evans, E. Rol, F. Olivares, J. Hjorth, P. Jakobsson, J. Farihi, R. Willingale, R. L.C. Starling, S. B. CenkoD. Perley, J. R. Maund, J. Duke, R. A.M.J. Wijers, A. J. Adamson, A. Allan, M. N. Bremer, D. N. Burrows, A. J. Castro-Tirado, B. Cavanagh, A. De Ugarte Postigo, M. A. Dopita, T. A. Fatkhullin, A. S. Fruchter, R. J. Foley, J. Gorosabel, J. Kennea, T. Kerr, S. Klose, H. A. Krimm, V. N. Komarova, S. R. Kulkarni, A. S. Moskvitin, C. G. Mundell, T. Naylor, K. Page, B. E. Penprase, M. Perri, P. Podsiadlowski, K. Roth, R. E. Rutledge, T. Sakamoto, P. Schady, B. P. Schmidt, A. M. Soderberg, J. Sollerman, A. W. Stephens, G. Stratta, T. N. Ukwatta, D. Watson, E. Westra, T. Wold, C. Wolf

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Abstract

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 any object was z = 6.96, for a Lyman-α emitting galaxy. Here we report that GRB 090423 lies at a redshift of z 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.

Original language	English
Pages (from-to)	1254-1257
Number of pages	4
Journal	Nature
Volume	461
Issue number	7268
DOIs	https://doi.org/10.1038/nature08459
Publication status	Published - 29 Oct 2009

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Tanvir, N. R., Fox, D. B., Levan, A. J., Berger, E., Wiersema, K., Fynbo, J. P. U., Cucchiara, A., Krühler, T., Gehrels, N., Bloom, J. S., Greiner, J., Evans, P. A., Rol, E., Olivares, F., Hjorth, J., Jakobsson, P., Farihi, J., Willingale, R., Starling, R. L. C., ... Wolf, C. (2009). A γ-ray burst at a redshift of ≈ 8.2. Nature, 461(7268), 1254-1257. https://doi.org/10.1038/nature08459

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title = "A γ-ray burst at a redshift of ≈ 8.2",

abstract = "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 any object was z = 6.96, for a Lyman-α emitting galaxy. Here we report that GRB 090423 lies at a redshift of z 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.",

author = "Tanvir, {N. R.} and Fox, {D. B.} and Levan, {A. J.} and E. Berger and K. Wiersema and Fynbo, {J. P.U.} and A. Cucchiara and T. Kr{\"u}hler and N. Gehrels and Bloom, {J. S.} and J. Greiner and Evans, {P. A.} and E. Rol and F. Olivares and J. Hjorth and P. Jakobsson and J. Farihi and R. Willingale and Starling, {R. L.C.} and Cenko, {S. B.} and D. Perley and Maund, {J. R.} and J. Duke and Wijers, {R. A.M.J.} and Adamson, {A. J.} and A. Allan and Bremer, {M. N.} and Burrows, {D. N.} and Castro-Tirado, {A. J.} and B. Cavanagh and {De Ugarte Postigo}, A. and Dopita, {M. A.} and Fatkhullin, {T. A.} and Fruchter, {A. S.} and Foley, {R. J.} and J. Gorosabel and J. Kennea and T. Kerr and S. Klose and Krimm, {H. A.} and Komarova, {V. N.} and Kulkarni, {S. R.} and Moskvitin, {A. S.} and Mundell, {C. G.} and T. Naylor and K. Page and Penprase, {B. E.} and M. Perri and P. Podsiadlowski and K. Roth and Rutledge, {R. E.} and T. Sakamoto and P. Schady and Schmidt, {B. P.} and Soderberg, {A. M.} and J. Sollerman and Stephens, {A. W.} and G. Stratta and Ukwatta, {T. N.} and D. Watson and E. Westra and T. Wold and C. Wolf",

year = "2009",

month = oct,

day = "29",

doi = "10.1038/nature08459",

language = "English",

volume = "461",

pages = "1254--1257",

journal = "Nature",

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Tanvir, NR, Fox, DB, Levan, AJ, Berger, E, Wiersema, K, Fynbo, JPU, Cucchiara, A, Krühler, T, Gehrels, N, Bloom, JS, Greiner, J, Evans, PA, Rol, E, Olivares, F, Hjorth, J, Jakobsson, P, Farihi, J, Willingale, R, Starling, RLC, Cenko, SB, Perley, D, Maund, JR, Duke, J, Wijers, RAMJ, Adamson, AJ, Allan, A, Bremer, MN, Burrows, DN, Castro-Tirado, AJ, Cavanagh, B, De Ugarte Postigo, A, Dopita, MA, Fatkhullin, TA, Fruchter, AS, Foley, RJ, Gorosabel, J, Kennea, J, Kerr, T, Klose, S, Krimm, HA, Komarova, VN, Kulkarni, SR, Moskvitin, AS, Mundell, CG, Naylor, T, Page, K, Penprase, BE, Perri, M, Podsiadlowski, P, Roth, K, Rutledge, RE, Sakamoto, T, Schady, P, Schmidt, BP, Soderberg, AM, Sollerman, J, Stephens, AW, Stratta, G, Ukwatta, TN, Watson, D, Westra, E, Wold, T & Wolf, C 2009, 'A γ-ray burst at a redshift of ≈ 8.2', Nature, vol. 461, no. 7268, pp. 1254-1257. https://doi.org/10.1038/nature08459

TY - JOUR

T1 - A γ-ray burst at a redshift of ≈ 8.2

AU - Tanvir, N. R.

AU - Fox, D. B.

AU - Levan, A. J.

AU - Berger, E.

AU - Wiersema, K.

AU - Fynbo, J. P.U.

AU - Cucchiara, A.

AU - Krühler, T.

AU - Gehrels, N.

AU - Bloom, J. S.

AU - Greiner, J.

AU - Evans, P. A.

AU - Rol, E.

AU - Olivares, F.

AU - Hjorth, J.

AU - Jakobsson, P.

AU - Farihi, J.

AU - Willingale, R.

AU - Starling, R. L.C.

AU - Cenko, S. B.

AU - Perley, D.

AU - Maund, J. R.

AU - Duke, J.

AU - Wijers, R. A.M.J.

AU - Adamson, A. J.

AU - Allan, A.

AU - Bremer, M. N.

AU - Burrows, D. N.

AU - Castro-Tirado, A. J.

AU - Cavanagh, B.

AU - De Ugarte Postigo, A.

AU - Dopita, M. A.

AU - Fatkhullin, T. A.

AU - Fruchter, A. S.

AU - Foley, R. J.

AU - Gorosabel, J.

AU - Kennea, J.

AU - Kerr, T.

AU - Klose, S.

AU - Krimm, H. A.

AU - Komarova, V. N.

AU - Kulkarni, S. R.

AU - Moskvitin, A. S.

AU - Mundell, C. G.

AU - Naylor, T.

AU - Page, K.

AU - Penprase, B. E.

AU - Perri, M.

AU - Podsiadlowski, P.

AU - Roth, K.

AU - Rutledge, R. E.

AU - Sakamoto, T.

AU - Schady, P.

AU - Schmidt, B. P.

AU - Soderberg, A. M.

AU - Sollerman, J.

AU - Stephens, A. W.

AU - Stratta, G.

AU - Ukwatta, T. N.

AU - Watson, D.

AU - Westra, E.

AU - Wold, T.

AU - Wolf, C.

PY - 2009/10/29

Y1 - 2009/10/29

N2 - 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 any object was z = 6.96, for a Lyman-α emitting galaxy. Here we report that GRB 090423 lies at a redshift of z 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.

AB - 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 any object was z = 6.96, for a Lyman-α emitting galaxy. Here we report that GRB 090423 lies at a redshift of z 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.

UR - http://www.scopus.com/inward/record.url?scp=70350686721&partnerID=8YFLogxK

U2 - 10.1038/nature08459

DO - 10.1038/nature08459

M3 - Article

SN - 0028-0836

VL - 461

SP - 1254

EP - 1257

JO - Nature

JF - Nature

IS - 7268

ER -

A γ-ray burst at a redshift of ≈ 8.2

Abstract

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