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Cited by 497

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GRB 090423 at a redshift of z ≈ 8.1

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Salvaterra, R., Valle, M. Della, Campana, S., Chincarini, G., Covino, S., D’Avanzo, P., Fernández-Soto, A., Guidorzi, C., Mannucci, F., Margutti, R., Thöne, C. C., Antonelli, L. A., Barthelmy, S. D., De Pasquale, M., D’Elia, V., Fiore, F., Fugazza, D., Hunt, L. K., Maiorano, E., Marinoni, S., Marshall, F. E., Molinari, E., Nousek, J., Pian, E., Racusin, J. L., Stella, L., Amati, L., Andreuzzi, G., Cusumano, G., Fenimore, E. E., Ferrero, P., Giommi, P., Guetta, D., Holland, S. T., Hurley, K., Israel, G. L., Mao, J., Markwardt, C. B., Masetti, N., Pagani, C., Palazzi, E., Palmer, D. M., Piranomonte, S., Tagliaferri, G., Testa, V.·2009·Nature

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.

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Authors
Salvaterra, R., Valle, M. D., Campana, S., Chincarini, G., Covino, S., D’Avanzo, P., Fernández-Soto, A., Guidorzi, C., Mannucci, F., Margutti, R., Thöne, C. C., Antonelli, L. A., Barthelmy, S. D., De Pasquale, M., D’Elia, V., Fiore, F., Fugazza, D., Hunt, L. K., Maiorano, E., Marinoni, S., Marshall, F. E., Molinari, E., Nousek, J., Pian, E., Racusin, J. L., Stella, L., Amati, L., Andreuzzi, G., Cusumano, G., Fenimore, E. E., Ferrero, P., Giommi, P., Guetta, D., Holland, S. T., Hurley, K., Israel, G. L., Mao, J., Markwardt, C. B., Masetti, N., Pagani, C., Palazzi, E., Palmer, D. M., Piranomonte, S., Tagliaferri, G., & Testa, V.
Venue
Nature
Published
2009-10
Volume
461
Issue
7268
Pages
1258-1260
ISSN
  • 0028-0836 (ISSN-L)
  • 1476-4687
OpenAlex
W1969939835
Cited by
497
References
0
FWCI
35.64
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: GRB 090423 at a redshift of z ≈ 8.1. https://app.cochat.ai/papers/10.1038/nature08445
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Salvaterra, R., Valle, M. D., Campana, S., Chincarini, G., Covino, S., D’Avanzo, P., Fernández-Soto, A., Guidorzi, C., Mannucci, F., Margutti, R., Thöne, 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 ≈ 8.1. Nature. https://doi.org/10.1038/nature08445

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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