GRB 090423 at a redshift of z approximate to 8.1

R. Salvaterra; M. Della Valle; S. Campana; G. Chincarini; S. Covino; P. D'Avanzo; A. Fernandez-Soto; C. Guidorzi; F. Mannucci; R. Margutti; C. C. Thoene; L. A. Antonelli; S. D. Barthelmy; M. De Pasquale; V. D'Elia; F. Fiore; D. Fugazza; L. K. Hunt; E. Maiorano; S. Marinoni; F. E. Marshall; E. Molinari; J. Nousek; E. Pian; J. L. Racusin; L. Stella; L. Amati; G. Andreuzzi; G. Cusumano; E. E. Fenimore; P. Ferrero; P. Giommi; D. Guetta; S. T. Holland; K. Hurley; G. L. Israel; J. Mao; C. B. Markwardt; N. Masetti; C. Pagani; E. Palazzi; D. M. Palmer; S. Piranomonte; G. Tagliaferri; V. Testa

doi:10.1038/nature08445

GRB 090423 at a redshift of z approximate to 8.1

R. Salvaterra
, M. Della Valle
, S. Campana
, G. Chincarini
, S. Covino
, P. D'Avanzo
, A. Fernandez-Soto
, C. Guidorzi
, F. Mannucci
, R. Margutti
, C. C. Thoene
, L. A. Antonelli
, S. D. Barthelmy
, M. De Pasquale
, V. D'Elia
, F. Fiore
, D. Fugazza
, L. K. Hunt
, E. Maiorano
, S. Marinoni

F. E. Marshall, E. Molinari, J. Nousek, E. Pian, J. L. Racusin, L. Stella, L. Amati, G. Andreuzzi, G. Cusumano, E. E. Fenimore, P. Ferrero, P. Giommi, D. Guetta, S. T. Holland, K. Hurley, G. L. Israel, J. Mao, C. B. Markwardt, N. Masetti, C. Pagani, E. Palazzi, D. M. Palmer, S. Piranomonte, G. Tagliaferri, V. Testa

نتاج البحث: نشر في مجلة › مقالة › مراجعة النظراء

491 اقتباسات (Scopus)

ملخص

Gamma-ray bursts (GRBs) are produced by rare types of massive stellar explosion. Their rapidly fading afterglows are often bright enough at optical wavelengths that they are detectable at cosmological distances. Hitherto, the highest known redshift for a GRB was z = 6.7 (ref. 1), for GRB 080913, and for a galaxy was z = 6.96 (ref. 2). Here we report observations of GRB 090423 and the near-infrared spectroscopic measurement of its redshift, z =. This burst happened when the Universe was only about 4 per cent of its current age. Its properties are similar to those of GRBs observed at low/intermediate redshifts, suggesting that the mechanisms and progenitors that gave rise to this burst about 600,000,000 years after the Big Bang are not markedly different from those producing GRBs about 10,000,000,000 years later.

اللغة الأصلية	الإنجليزيّة
الصفحات (من إلى)	1258-1260
عدد الصفحات	3
دورية	Nature
مستوى الصوت	461
رقم الإصدار	7268
المعرِّفات الرقمية للأشياء	https://doi.org/10.1038/nature08445
حالة النشر	نُشِر - 29 أكتوبر 2009
منشور خارجيًا	نعم

الوصول إلى المستند

10.1038/nature08445

الملفات والروابط الأخرى

Link to publication in Scopus

قم بذكر هذا

Salvaterra, R., Della Valle, M., Campana, S., Chincarini, G., Covino, S., D'Avanzo, P., Fernandez-Soto, A., Guidorzi, C., Mannucci, F., Margutti, R., Thoene, C. C., Antonelli, L. A., Barthelmy, S. D., De Pasquale, M., D'Elia, V., Fiore, F., Fugazza, D., Hunt, L. K., Maiorano, E., ... Testa, V. (2009). GRB 090423 at a redshift of z approximate to 8.1. Nature, 461(7268), 1258-1260. https://doi.org/10.1038/nature08445

@article{646212a684d74c468f2f52e06f6ac22c,

title = "GRB 090423 at a redshift of z approximate to 8.1",

abstract = "Gamma-ray bursts (GRBs) are produced by rare types of massive stellar explosion. Their rapidly fading afterglows are often bright enough at optical wavelengths that they are detectable at cosmological distances. Hitherto, the highest known redshift for a GRB was z = 6.7 (ref. 1), for GRB 080913, and for a galaxy was z = 6.96 (ref. 2). Here we report observations of GRB 090423 and the near-infrared spectroscopic measurement of its redshift, z =. This burst happened when the Universe was only about 4 per cent of its current age. Its properties are similar to those of GRBs observed at low/intermediate redshifts, suggesting that the mechanisms and progenitors that gave rise to this burst about 600,000,000 years after the Big Bang are not markedly different from those producing GRBs about 10,000,000,000 years later.",

author = "R. Salvaterra and \{Della Valle\}, M. and S. Campana and G. Chincarini and S. Covino and P. D'Avanzo and A. Fernandez-Soto and C. Guidorzi and F. Mannucci and R. Margutti and Thoene, \{C. C.\} and Antonelli, \{L. A.\} and Barthelmy, \{S. D.\} and \{De Pasquale\}, M. and V. D'Elia and F. Fiore and D. Fugazza and Hunt, \{L. K.\} and E. Maiorano and S. Marinoni and Marshall, \{F. E.\} and E. Molinari and J. Nousek and E. Pian and Racusin, \{J. L.\} and L. Stella and L. Amati and G. Andreuzzi and G. Cusumano and Fenimore, \{E. E.\} and P. Ferrero and P. Giommi and D. Guetta and Holland, \{S. T.\} and K. Hurley and Israel, \{G. L.\} and J. Mao and Markwardt, \{C. B.\} and N. Masetti and C. Pagani and E. Palazzi and Palmer, \{D. M.\} and S. Piranomonte and G. Tagliaferri and V. Testa",

year = "2009",

month = oct,

day = "29",

doi = "10.1038/nature08445",

language = "אנגלית",

volume = "461",

pages = "1258--1260",

journal = "Nature",

issn = "0028-0836",

publisher = "Nature Research",

number = "7268",

}

Salvaterra, R, Della Valle, M, Campana, S, Chincarini, G, Covino, S, D'Avanzo, P, Fernandez-Soto, A, Guidorzi, C, Mannucci, F, Margutti, R, Thoene, CC, Antonelli, LA, Barthelmy, SD, De Pasquale, M, D'Elia, V, Fiore, F, Fugazza, D, Hunt, LK, Maiorano, E, Marinoni, S, Marshall, FE, Molinari, E, Nousek, J, Pian, E, Racusin, JL, Stella, L, Amati, L, Andreuzzi, G, Cusumano, G, Fenimore, EE, Ferrero, P, Giommi, P, Guetta, D, Holland, ST, Hurley, K, Israel, GL, Mao, J, Markwardt, CB, Masetti, N, Pagani, C, Palazzi, E, Palmer, DM, Piranomonte, S, Tagliaferri, G & Testa, V 2009, 'GRB 090423 at a redshift of z approximate to 8.1', Nature, المجلد 461, رقم 7268, الصفحات 1258-1260. https://doi.org/10.1038/nature08445

TY - JOUR

T1 - GRB 090423 at a redshift of z approximate to 8.1

AU - Salvaterra, R.

AU - Della Valle, M.

AU - Campana, S.

AU - Chincarini, G.

AU - Covino, S.

AU - D'Avanzo, P.

AU - Fernandez-Soto, A.

AU - Guidorzi, C.

AU - Mannucci, F.

AU - Margutti, R.

AU - Thoene, C. C.

AU - Antonelli, L. A.

AU - Barthelmy, S. D.

AU - De Pasquale, M.

AU - D'Elia, V.

AU - Fiore, F.

AU - Fugazza, D.

AU - Hunt, L. K.

AU - Maiorano, E.

AU - Marinoni, S.

AU - Marshall, F. E.

AU - Molinari, E.

AU - Nousek, J.

AU - Pian, E.

AU - Racusin, J. L.

AU - Stella, L.

AU - Amati, L.

AU - Andreuzzi, G.

AU - Cusumano, G.

AU - Fenimore, E. E.

AU - Ferrero, P.

AU - Giommi, P.

AU - Guetta, D.

AU - Holland, S. T.

AU - Hurley, K.

AU - Israel, G. L.

AU - Mao, J.

AU - Markwardt, C. B.

AU - Masetti, N.

AU - Pagani, C.

AU - Palazzi, E.

AU - Palmer, D. M.

AU - Piranomonte, S.

AU - Tagliaferri, G.

AU - Testa, V.

PY - 2009/10/29

Y1 - 2009/10/29

N2 - Gamma-ray bursts (GRBs) are produced by rare types of massive stellar explosion. Their rapidly fading afterglows are often bright enough at optical wavelengths that they are detectable at cosmological distances. Hitherto, the highest known redshift for a GRB was z = 6.7 (ref. 1), for GRB 080913, and for a galaxy was z = 6.96 (ref. 2). Here we report observations of GRB 090423 and the near-infrared spectroscopic measurement of its redshift, z =. This burst happened when the Universe was only about 4 per cent of its current age. Its properties are similar to those of GRBs observed at low/intermediate redshifts, suggesting that the mechanisms and progenitors that gave rise to this burst about 600,000,000 years after the Big Bang are not markedly different from those producing GRBs about 10,000,000,000 years later.

AB - Gamma-ray bursts (GRBs) are produced by rare types of massive stellar explosion. Their rapidly fading afterglows are often bright enough at optical wavelengths that they are detectable at cosmological distances. Hitherto, the highest known redshift for a GRB was z = 6.7 (ref. 1), for GRB 080913, and for a galaxy was z = 6.96 (ref. 2). Here we report observations of GRB 090423 and the near-infrared spectroscopic measurement of its redshift, z =. This burst happened when the Universe was only about 4 per cent of its current age. Its properties are similar to those of GRBs observed at low/intermediate redshifts, suggesting that the mechanisms and progenitors that gave rise to this burst about 600,000,000 years after the Big Bang are not markedly different from those producing GRBs about 10,000,000,000 years later.

UR - https://www.scopus.com/pages/publications/70350678973

U2 - 10.1038/nature08445

DO - 10.1038/nature08445

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SN - 0028-0836

VL - 461

SP - 1258

EP - 1260

JO - Nature

JF - Nature

IS - 7268

ER -

GRB 090423 at a redshift of z approximate to 8.1

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