A more probable explanation for a continuum flash towards a redshift ≈ 11 galaxy-Reference-Cited by-同舟云学术

A more probable explanation for a continuum flash towards a redshift ≈ 11 galaxy

Published:2021-10 Issue:10 Volume:5 Page:993-994
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Steinhardt Charles Louis^ORCID,Andersen Michael I.^ORCID,Brammer Gabriel B.^ORCID,Christensen Lise^ORCID,Fynbo Johan P. U.^ORCID,Laursen Peter^ORCID,Milvang-Jensen Bo^ORCID,Oesch Pascal A.^ORCID,Toft Sune^ORCID

Funder

Danmarks Grundforskningsfond

EC | Horizon 2020 Framework Programme

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

https://www.nature.com/articles/s41550-021-01473-2.pdf

Reference21 articles.

1. Jiang, L. et al. A possible bright ultraviolet flash from a galaxy at redshift z ≈ 11. Nat. Astron. 5, 262–267 (2021).

2. Oesch, P. A. et al. A remarkably luminous galaxy at z=11.1 measured with Hubble Space Telescope grism spectroscopy. Astrophys. J. 819, 129–139 (2016).

3. Jakobsson, P. J. et al. Swift identification of dark gamma-ray bursts. Astrophys. J. 617, L21–L24 (2004).

4. Japelj, J. S. et al. Spectrophotometric analysis of gamma-ray burst afterglow extinction curves with X-Shooter. Astron. Astrophys. 579, A74–A90 (2015).

5. Li, L. et al. A correlated study of optical and X-Ray afterglows of GRBs. Astrophys. J. 805, 13–44 (2015).

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