A Lyman-α protocluster at redshift 6.9-Reference-Cited by-同舟云学术

A Lyman-α protocluster at redshift 6.9

Published:2021-01-25 Issue:5 Volume:5 Page:485-490
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Hu Weida^ORCID,Wang Junxian^ORCID,Infante Leopoldo,Rhoads James E.^ORCID,Zheng Zhen-Ya,Yang Huan,Malhotra Sangeeta,Barrientos L. Felipe^ORCID,Jiang Chunyan,González-López Jorge,Prieto Gonzalo,Perez Lucia A.,Hibon Pascale,Galaz Gaspar^ORCID,Coughlin Alicia,Harish Santosh,Kong Xu,Kang Wenyong,Khostovan Ali Ahmad,Pharo John,Valdes Francisco,Wold Isak^ORCID,Walker Alistair R.,Zheng XianZhong^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://www.nature.com/articles/s41550-020-01291-y.pdf

Reference60 articles.

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2. Wang, J. X., Malhotra, S. & Rhoads, J. E. An overdensity of Lyα emitters at redshift z ~ 5.7 near the Hubble Ultra Deep Field. Astrophys. J. 622, L77–L80 (2005).

3. Malhotra, S. et al. An overdensity of galaxies at z = 5.9 ± 0.2 in the Hubble Ultra Deep Field confirmed using the ACS grism. Astrophys. J. 626, 666–679 (2005).

4. Jiang, L. et al. A giant protocluster of galaxies at redshift 5.7. Nat. Astron. 2, 962–966 (2018).

5. Harikane, Y. et al. SILVERRUSH. VIII. Spectroscopic identifications of early large-scale structures with protoclusters over 200 Mpc at z ~ 6−7: strong associations of dusty star-forming galaxies. Astrophys. J. 883, 142 (2019).

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